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Chemistry
Chemistry
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Chemistry is the scientific study of the properties and behavior of matter.[1][2] It is a physical science within the natural sciences that studies the chemical elements that make up matter and compounds made of atoms, molecules and ions: their composition, structure, properties, behavior and the changes they undergo during reactions with other substances.[3][4][5][6] Chemistry also addresses the nature of chemical bonds in chemical compounds.

In the scope of its subject, chemistry occupies an intermediate position between physics and biology.[7] It is sometimes called the central science because it provides a foundation for understanding both basic and applied scientific disciplines at a fundamental level.[8] For example, chemistry explains aspects of plant growth (botany), the formation of igneous rocks (geology), how atmospheric ozone is formed and how environmental pollutants are degraded (ecology), the properties of the soil on the Moon (cosmochemistry), how medications work (pharmacology), and how to collect DNA evidence at a crime scene (forensics).

Chemistry has existed under various names since ancient times.[9] It has evolved, and now chemistry encompasses various areas of specialisation, or subdisciplines, that continue to increase in number and interrelate to create further interdisciplinary fields of study. The applications of various fields of chemistry are used frequently for economic purposes in the chemical industry.

Etymology

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The word chemistry comes from a modification during the Renaissance of the word alchemy, which referred to an earlier set of practices that encompassed elements of chemistry, metallurgy, philosophy, astrology, astronomy, mysticism, and medicine. Alchemy is often associated with the quest to turn lead or other base metals into gold, though alchemists were also interested in many of the questions of modern chemistry.[10][11]

The modern word alchemy in turn is derived from the Arabic word al-kīmīā (الكیمیاء). This may have Egyptian origins since al-kīmīā is derived from the Ancient Greek χημία, which is in turn derived from the word Kemet, which is the ancient name of Egypt in the Egyptian language.[12] Alternately, al-kīmīā may derive from χημεία 'cast together'.[13]

Modern principles

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Laboratory, Institute of Biochemistry, University of Cologne in Germany

The current model of atomic structure is the quantum mechanical model.[14] Traditional chemistry starts with the study of elementary particles, atoms, molecules,[15] substances, metals, crystals and other aggregates of matter. Matter can be studied in solid, liquid, gas and plasma states, in isolation or in combination. The interactions, reactions and transformations that are studied in chemistry are usually the result of interactions between atoms, leading to rearrangements of the chemical bonds which hold atoms together. Such behaviors are studied in a chemistry laboratory.

The chemistry laboratory stereotypically uses various forms of laboratory glassware. However glassware is not central to chemistry, and a great deal of experimental (as well as applied/industrial) chemistry is done without it.

Solutions of substances in reagent bottles, including ammonium hydroxide and nitric acid, illuminated in different colors

A chemical reaction is a transformation of some substances into one or more different substances.[16] The basis of such a chemical transformation is the rearrangement of electrons in the chemical bonds between atoms. It can be symbolically depicted through a chemical equation, which usually involves atoms as subjects. The number of atoms on the left and the right in the equation for a chemical transformation is equal. (When the number of atoms on either side is unequal, the transformation is referred to as a nuclear reaction or radioactive decay.) The type of chemical reactions a substance may undergo and the energy changes that may accompany it are constrained by certain basic rules, known as chemical laws.

Energy and entropy considerations are invariably important in almost all chemical studies. Chemical substances are classified in terms of their structure, phase, as well as their chemical compositions. They can be analyzed using the tools of chemical analysis, e.g. spectroscopy and chromatography. Scientists engaged in chemical research are known as chemists.[17] Most chemists specialize in one or more sub-disciplines. Several concepts are essential for the study of chemistry; some of them are:[18]

Matter

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In chemistry, matter is defined as anything that has rest mass and volume (it takes up space) and is made up of particles. The particles that make up matter have rest mass as well – not all particles have rest mass, such as the photon. Matter can be a pure chemical substance or a mixture of substances.[19]

Atom

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A diagram of an atom based on the Rutherford model

The atom is the basic unit of chemistry. It consists of a dense core called the atomic nucleus surrounded by a space occupied by an electron cloud. The nucleus is made up of positively charged protons and uncharged neutrons (together called nucleons), while the electron cloud consists of negatively charged electrons which orbit the nucleus. In a neutral atom, the negatively charged electrons balance out the positive charge of the protons. The nucleus is dense; the mass of a nucleon is approximately 1,836 times that of an electron, yet the radius of an atom is about 10,000 times that of its nucleus.[20][21]

The atom is also the smallest entity that can be envisaged to retain the chemical properties of the element, such as electronegativity, ionization potential, preferred oxidation state(s), coordination number, and preferred types of bonds to form (e.g., metallic, ionic, covalent).

Element

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Standard form of the periodic table of chemical elements. The colors represent different blocks of elements.

A chemical element is a pure substance which is composed of a single type of atom, characterized by its particular number of protons in the nuclei of its atoms, known as the atomic number and represented by the symbol Z. The mass number is the sum of the number of protons and neutrons in a nucleus. Although all the nuclei of all atoms belonging to one element will have the same atomic number, they may not necessarily have the same mass number; atoms of an element which have different mass numbers are known as isotopes. For example, all atoms with 6 protons in their nuclei are atoms of the chemical element carbon, but atoms of carbon may have mass numbers of 12 or 13.[21]

The standard presentation of the chemical elements is in the periodic table, which orders elements by atomic number. The periodic table is arranged in groups, or columns, and periods, or rows. The periodic table is useful in identifying periodic trends.[22]

Compound

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Carbon dioxide (CO2), an example of a chemical compound

A compound is a pure chemical substance composed of more than one element. The properties of a compound bear little similarity to those of its elements.[23] The standard nomenclature of compounds is set by the International Union of Pure and Applied Chemistry (IUPAC). Organic compounds are named according to the organic nomenclature system.[24] The names for inorganic compounds are created according to the inorganic nomenclature system. When a compound has more than one component, then they are divided into two classes, the electropositive and the electronegative components.[25] In addition the Chemical Abstracts Service (CAS) has devised a method to index chemical substances. In this scheme each chemical substance is identifiable by a number known as its CAS registry number.

Molecule

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A ball-and-stick representation of the caffeine molecule (C8H10N4O2)

A molecule is the smallest indivisible portion of a pure chemical substance that has its unique set of chemical properties, that is, its potential to undergo a certain set of chemical reactions with other substances. However, this definition only works well for substances that are composed of molecules, which is not true of many substances (see below). Molecules are typically a set of atoms bound together by covalent bonds, such that the structure is electrically neutral and all valence electrons are paired with other electrons either in bonds or in lone pairs.

Thus, molecules exist as electrically neutral units, unlike ions. When this rule is broken, giving the "molecule" a charge, the result is sometimes named a molecular ion or a polyatomic ion. However, the discrete and separate nature of the molecular concept usually requires that molecular ions be present only in well-separated form, such as a directed beam in a vacuum in a mass spectrometer. Charged polyatomic collections residing in solids (for example, common sulfate or nitrate ions) are generally not considered "molecules" in chemistry. Some molecules contain one or more unpaired electrons, creating radicals. Most radicals are comparatively reactive, but some, such as nitric oxide (NO) can be stable.

A 2-D structural formula of a benzene molecule (C6H6)

The "inert" or noble gas elements (helium, neon, argon, krypton, xenon and radon) are composed of lone atoms as their smallest discrete unit, but the other isolated chemical elements consist of either molecules or networks of atoms bonded to each other in some way. Identifiable molecules compose familiar substances such as water, air, and many organic compounds like alcohol, sugar, gasoline, and the various pharmaceuticals.

However, not all substances or chemical compounds consist of discrete molecules, and indeed most of the solid substances that make up the solid crust, mantle, and core of the Earth are chemical compounds without molecules. These other types of substances, such as ionic compounds and network solids, are organized in such a way as to lack the existence of identifiable molecules per se. Instead, these substances are discussed in terms of formula units or unit cells as the smallest repeating structure within the substance. Examples of such substances are mineral salts (such as table salt), solids like carbon and diamond, metals, and familiar silica and silicate minerals such as quartz and granite.

One of the main characteristics of a molecule is its geometry often called its structure. While the structure of diatomic, triatomic or tetra-atomic molecules may be trivial, (linear, angular pyramidal etc.) the structure of polyatomic molecules, that are constituted of more than six atoms (of several elements) can be crucial for its chemical nature.

Substance and mixture

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Examples of pure chemical substances. From left to right: the elements tin (Sn) and sulfur (S), diamond (an allotrope of carbon), sucrose (pure sugar), and sodium chloride (salt) and sodium bicarbonate (baking soda), which are both ionic compounds.

A chemical substance is a kind of matter with a definite composition and set of properties.[26] A collection of substances is called a mixture. Examples of mixtures are air and alloys.[27]

Mole and amount of substance

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The mole is a unit of measurement that denotes an amount of substance (also called chemical amount). One mole is defined to contain exactly 6.02214076×1023 particles (atoms, molecules, ions, or electrons), where the number of particles per mole is known as the Avogadro constant.[28] Molar concentration is the amount of a particular substance per volume of solution, and is commonly reported in mol/dm3.[29]

Phase

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Diagram showing relationships among the phases and the terms used to describe phase changes

In addition to the specific chemical properties that distinguish different chemical classifications, chemicals can exist in several phases. For the most part, the chemical classifications are independent of these bulk phase classifications; however, some more exotic phases are incompatible with certain chemical properties. A phase is a set of states of a chemical system that have similar bulk structural properties, over a range of conditions, such as pressure or temperature.

Physical properties, such as density and refractive index tend to fall within values characteristic of the phase. The phase of matter is defined by the phase transition, which is when energy put into or taken out of the system goes into rearranging the structure of the system, instead of changing the bulk conditions.

Sometimes the distinction between phases can be continuous instead of having a discrete boundary; in this case the matter is considered to be in a supercritical state. When three states meet based on the conditions, it is known as a triple point and since this is invariant, it is a convenient way to define a set of conditions.

The most familiar examples of phases are solids, liquids, and gases. Many substances exhibit multiple solid phases. For example, there are three phases of solid iron (alpha, gamma, and delta) that vary based on temperature and pressure. A principal difference between solid phases is the crystal structure, or arrangement, of the atoms. Another phase commonly encountered in the study of chemistry is the aqueous phase, which is the state of substances dissolved in aqueous solution (that is, in water).

Less familiar phases include plasmas, Bose–Einstein condensates and fermionic condensates and the paramagnetic and ferromagnetic phases of magnetic materials. While most familiar phases deal with three-dimensional systems, it is also possible to define analogs in two-dimensional systems, which has received attention for its relevance to systems in biology.

Bonding

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An animation of the process of ionic bonding between sodium (Na) and chlorine (Cl) to form sodium chloride, or common table salt. Ionic bonding involves one atom taking valence electrons from another (as opposed to sharing, which occurs in covalent bonding).

Atoms sticking together in molecules or crystals are said to be bonded with one another. A chemical bond may be visualized as the multipole balance between the positive charges in the nuclei and the negative charges oscillating about them.[30] More than simple attraction and repulsion, the energies and distributions characterize the availability of an electron to bond to another atom.

The chemical bond can be a covalent bond, an ionic bond, a hydrogen bond or just because of Van der Waals force. Each of these kinds of bonds is ascribed to some potential. These potentials create the interactions which hold atoms together in molecules or crystals. In many simple compounds, valence bond theory, the Valence Shell Electron Pair Repulsion model (VSEPR), and the concept of oxidation number can be used to explain molecular structure and composition.

An ionic bond is formed when a metal loses one or more of its electrons, becoming a positively charged cation, and the electrons are then gained by the non-metal atom, becoming a negatively charged anion. The two oppositely charged ions attract one another, and the ionic bond is the electrostatic force of attraction between them. For example, sodium (Na), a metal, loses one electron to become an Na+ cation while chlorine (Cl), a non-metal, gains this electron to become Cl. The ions are held together due to electrostatic attraction, and that compound sodium chloride (NaCl), or common table salt, is formed.

In the methane molecule (CH4), the carbon atom shares a pair of valence electrons with each of the four hydrogen atoms. Thus, the octet rule is satisfied for C-atom (it has eight electrons in its valence shell) and the duet rule is satisfied for the H-atoms (they have two electrons in their valence shells).

In a covalent bond, one or more pairs of valence electrons are shared by two atoms: the resulting electrically neutral group of bonded atoms is termed a molecule. Atoms will share valence electrons in such a way as to create a noble gas electron configuration (eight electrons in their outermost shell) for each atom. Atoms that tend to combine in such a way that they each have eight electrons in their valence shell are said to follow the octet rule. However, some elements like hydrogen and lithium need only two electrons in their outermost shell to attain this stable configuration; these atoms are said to follow the duet rule, and in this way they are reaching the electron configuration of the noble gas helium, which has two electrons in its outer shell.

Similarly, theories from classical physics can be used to predict many ionic structures. With more complicated compounds, such as metal complexes, valence bond theory is less applicable and alternative approaches, such as the molecular orbital theory, are generally used.

Energy

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In the context of chemistry, energy is an attribute of a substance as a consequence of its atomic, molecular or aggregate structure. Since a chemical transformation is accompanied by a change in one or more of these kinds of structures, it is invariably accompanied by an increase or decrease of energy of the substances involved. Some energy is transferred between the surroundings and the reactants of the reaction in the form of heat or light; thus the products of a reaction may have more or less energy than the reactants.

A reaction is said to be exergonic if the final state is lower on the energy scale than the initial state; in the case of endergonic reactions the situation is the reverse. A reaction is said to be exothermic if the reaction releases heat to the surroundings; in the case of endothermic reactions, the reaction absorbs heat from the surroundings.

Chemical reactions are invariably not possible unless the reactants surmount an energy barrier known as the activation energy. The speed of a chemical reaction (at given temperature T) is related to the activation energy E, by the Boltzmann's population factor – that is the probability of a molecule to have energy greater than or equal to E at the given temperature T. This exponential dependence of a reaction rate on temperature is known as the Arrhenius equation. The activation energy necessary for a chemical reaction to occur can be in the form of heat, light, electricity or mechanical force in the form of ultrasound.[31]

A related concept free energy, which also incorporates entropy considerations, is a very useful means for predicting the feasibility of a reaction and determining the state of equilibrium of a chemical reaction, in chemical thermodynamics. A reaction is feasible only if the total change in the Gibbs free energy is negative, ; if it is equal to zero the chemical reaction is said to be at equilibrium.

There exist only limited possible states of energy for electrons, atoms and molecules. These are determined by the rules of quantum mechanics, which require quantization of energy of a bound system. The atoms/molecules in a higher energy state are said to be excited. The molecules/atoms of substance in an excited energy state are often much more reactive; that is, more amenable to chemical reactions.

The phase of a substance is invariably determined by its energy and the energy of its surroundings. When the intermolecular forces of a substance are such that the energy of the surroundings is not sufficient to overcome them, it occurs in a more ordered phase like liquid or solid as is the case with water (H2O); a liquid at room temperature because its molecules are bound by hydrogen bonds.[32] Whereas hydrogen sulfide (H2S) is a gas at room temperature and standard pressure, as its molecules are bound by weaker dipole–dipole interactions.

The transfer of energy from one chemical substance to another depends on the size of energy quanta emitted from one substance. However, heat energy is often transferred more easily from almost any substance to another because the phonons responsible for vibrational and rotational energy levels in a substance have much less energy than photons invoked for the electronic energy transfer. Thus, because vibrational and rotational energy levels are more closely spaced than electronic energy levels, heat is more easily transferred between substances relative to light or other forms of electronic energy. For example, ultraviolet electromagnetic radiation is not transferred with as much efficacy from one substance to another as thermal or electrical energy.

The existence of characteristic energy levels for different chemical substances is useful for their identification by the analysis of spectral lines. Different kinds of spectra are often used in chemical spectroscopy, e.g. IR, microwave, NMR, ESR, etc. Spectroscopy is also used to identify the composition of remote objects – like stars and distant galaxies – by analyzing their radiation spectra.

Emission spectrum of iron

The term chemical energy is often used to indicate the potential of a chemical substance to undergo a transformation through a chemical reaction or to transform other chemical substances.

Reaction

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During chemical reactions, bonds between atoms break and form, resulting in different substances with different properties. In a blast furnace, iron oxide, a compound, reacts with carbon monoxide to form iron, one of the chemical elements, and carbon dioxide.

When a chemical substance is transformed as a result of its interaction with another substance or with energy, a chemical reaction is said to have occurred. A chemical reaction is therefore a concept related to the "reaction" of a substance when it comes in close contact with another, whether as a mixture or a solution; exposure to some form of energy, or both. It results in some energy exchange between the constituents of the reaction as well as with the system environment, which may be designed vessels—often laboratory glassware.

Chemical reactions can result in the formation or dissociation of molecules, that is, molecules breaking apart to form two or more molecules or rearrangement of atoms within or across molecules. Chemical reactions usually involve the making or breaking of chemical bonds. Oxidation, reduction, dissociation, acid–base neutralization and molecular rearrangement are some examples of common chemical reactions.

A chemical reaction can be symbolically depicted through a chemical equation. While in a non-nuclear chemical reaction the number and kind of atoms on both sides of the equation are equal, for a nuclear reaction this holds true only for the nuclear particles viz. protons and neutrons.[33]

The sequence of steps in which the reorganization of chemical bonds may be taking place in the course of a chemical reaction is called its mechanism. A chemical reaction can be envisioned to take place in a number of steps, each of which may have a different speed. Many reaction intermediates with variable stability can thus be envisaged during the course of a reaction. Reaction mechanisms are proposed to explain the kinetics and the relative product mix of a reaction. Many physical chemists specialize in exploring and proposing the mechanisms of various chemical reactions. Several empirical rules, like the Woodward–Hoffmann rules often come in handy while proposing a mechanism for a chemical reaction.

According to the IUPAC gold book, a chemical reaction is "a process that results in the interconversion of chemical species."[34] Accordingly, a chemical reaction may be an elementary reaction or a stepwise reaction. An additional caveat is made, in that this definition includes cases where the interconversion of conformers is experimentally observable. Such detectable chemical reactions normally involve sets of molecular entities as indicated by this definition, but it is often conceptually convenient to use the term also for changes involving single molecular entities (i.e. 'microscopic chemical events').

Ions and salts

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The crystal lattice structure of potassium chloride (KCl), a salt which is formed due to the attraction of K+ cations and Cl anions. The overall charge of the ionic compound is zero.

An ion is a charged species, an atom or a molecule, that has lost or gained one or more electrons. When an atom loses an electron and thus has more protons than electrons, the atom is a positively charged ion or cation. When an atom gains an electron and thus has more electrons than protons, the atom is a negatively charged ion or anion. Cations and anions can form a crystalline lattice of neutral salts, such as the Na+ and Cl ions forming sodium chloride, or NaCl. Examples of polyatomic ions that do not split up during acid–base reactions are hydroxide (OH) and phosphate (PO43−).

Plasma is composed of gaseous matter that has been completely ionized, usually through high temperature.

Acidity and basicity

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Hydrogen bromide exists in the gas phase as a diatomic molecule.

A substance can often be classified as an acid or a base. There are several different theories which explain acid–base behavior. The simplest is Arrhenius theory, which states that an acid is a substance that produces hydronium ions when it is dissolved in water, and a base is one that produces hydroxide ions when dissolved in water. According to Brønsted–Lowry acid–base theory, acids are substances that donate a positive hydrogen ion to another substance in a chemical reaction; by extension, a base is the substance which receives that hydrogen ion.

A third common theory is Lewis acid–base theory, which is based on the formation of new chemical bonds. Lewis theory explains that an acid is a substance which is capable of accepting a pair of electrons from another substance during the process of bond formation, while a base is a substance which can provide a pair of electrons to form a new bond. There are several other ways in which a substance may be classified as an acid or a base, as is evident in the history of this concept.[35]

Acid strength is commonly measured by two methods. One measurement, based on the Arrhenius definition of acidity, is pH, which is a measurement of the hydronium ion concentration in a solution, as expressed on a negative logarithmic scale. Thus, solutions that have a low pH have a high hydronium ion concentration and can be said to be more acidic. The other measurement, based on the Brønsted–Lowry definition, is the acid dissociation constant (Ka), which measures the relative ability of a substance to act as an acid under the Brønsted–Lowry definition of an acid. That is, substances with a higher Ka are more likely to donate hydrogen ions in chemical reactions than those with lower Ka values.

Redox

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Redox (reduction-oxidation) reactions include all chemical reactions in which atoms have their oxidation state changed by either gaining electrons (reduction) or losing electrons (oxidation). Substances that have the ability to oxidize other substances are said to be oxidative and are known as oxidizing agents, oxidants or oxidizers. An oxidant removes electrons from another substance. Similarly, substances that have the ability to reduce other substances are said to be reductive and are known as reducing agents, reductants, or reducers.

A reductant transfers electrons to another substance and is thus oxidized itself. And because it "donates" electrons it is also called an electron donor. Oxidation and reduction properly refer to a change in oxidation number—the actual transfer of electrons may never occur. Thus, oxidation is better defined as an increase in oxidation number, and reduction as a decrease in oxidation number.

Equilibrium

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Although the concept of equilibrium is widely used across sciences, in the context of chemistry, it arises whenever a number of different states of the chemical composition are possible, as for example, in a mixture of several chemical compounds that can react with one another, or when a substance can be present in more than one kind of phase.

A system of chemical substances at equilibrium, even though having an unchanging composition, is most often not static; molecules of the substances continue to react with one another thus giving rise to a dynamic equilibrium. Thus the concept describes the state in which the parameters such as chemical composition remain unchanged over time.

Chemical laws

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Chemical reactions are governed by certain laws, which have become fundamental concepts in chemistry. Some of them are:

History

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The history of chemistry spans a period from the ancient past to the present. Since several millennia BC, civilizations were using technologies that would eventually form the basis of the various branches of chemistry. Examples include extracting metals from ores, making pottery and glazes, fermenting beer and wine, extracting chemicals from plants for medicine and perfume, rendering fat into soap, making glass, and making alloys like bronze.

Chemistry was preceded by its protoscience, alchemy, which operated a non-scientific approach to understanding the constituents of matter and their interactions. Despite being unsuccessful in explaining the nature of matter and its transformations, alchemists set the stage for modern chemistry by performing experiments and recording the results. Robert Boyle, although skeptical of elements and convinced of alchemy, played a key part in elevating the "sacred art" as an independent, fundamental and philosophical discipline in his work The Sceptical Chymist (1661).[36]

While both alchemy and chemistry are concerned with matter and its transformations, the crucial difference was given by the scientific method that chemists employed in their work. Chemistry, as a body of knowledge distinct from alchemy, became an established science with the work of Antoine Lavoisier, who developed a law of conservation of mass that demanded careful measurement and quantitative observations of chemical phenomena. The history of chemistry afterwards is intertwined with the history of thermodynamics, especially through the work of Willard Gibbs.[37]

Definition

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The definition of chemistry has changed over time, as new discoveries and theories add to the functionality of the science. The term "chymistry", in the view of noted scientist Robert Boyle in 1661, meant the subject of the material principles of mixed bodies.[38] In 1663, the chemist Christopher Glaser described "chymistry" as a scientific art, by which one learns to dissolve bodies, and draw from them the different substances on their composition, and how to unite them again, and exalt them to a higher perfection.[39]

The 1730 definition of the word "chemistry", as used by Georg Ernst Stahl, meant the art of resolving mixed, compound, or aggregate bodies into their principles; and of composing such bodies from those principles.[40] In 1837, Jean-Baptiste Dumas considered the word "chemistry" to refer to the science concerned with the laws and effects of molecular forces.[41] This definition further evolved until, in 1947, it came to mean the science of substances: their structure, their properties, and the reactions that change them into other substances—a characterization accepted by Linus Pauling.[42] More recently, in 1998, Professor Raymond Chang broadened the definition of "chemistry" to mean the study of matter and the changes it undergoes.[43]

Background

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Democritus' atomist philosophy was later adopted by Epicurus (341–270 BCE).

Early civilizations, such as the Egyptians,[44] Babylonians, and Indians,[45] amassed practical knowledge concerning the arts of metallurgy, pottery and dyes, but did not develop a systematic theory.

A basic chemical hypothesis first emerged in Classical Greece with the theory of four elements as propounded definitively by Aristotle stating that fire, air, earth and water were the fundamental elements from which everything is formed as a combination. Greek atomism dates back to 440 BC, arising in works by philosophers such as Democritus and Epicurus. In 50 BCE, the Roman philosopher Lucretius expanded upon the theory in his poem De rerum natura (On The Nature of Things).[46][47] Unlike modern concepts of science, Greek atomism was purely philosophical in nature, with little concern for empirical observations and no concern for chemical experiments.[48]

An early form of the idea of conservation of mass is the notion that "Nothing comes from nothing" in Ancient Greek philosophy, which can be found in Empedocles (approx. 4th century BC): "For it is impossible for anything to come to be from what is not, and it cannot be brought about or heard of that what is should be utterly destroyed."[49] and Epicurus (3rd century BC), who, describing the nature of the Universe, wrote that "the totality of things was always such as it is now, and always will be".[50]

15th-century artistic impression of Jābir ibn Hayyān (Geber), a Perso-Arab alchemist and pioneer in organic chemistry

In the Hellenistic world the art of alchemy first proliferated, mingling magic and occultism into the study of natural substances with the ultimate goal of transmuting elements into gold and discovering the elixir of eternal life.[51] Work, particularly the development of distillation, continued in the early Byzantine period with the most famous practitioner being the 4th century Greek-Egyptian Zosimos of Panopolis.[52] Alchemy continued to be developed and practised throughout the Arab world after the Muslim conquests,[53] and from there, and from the Byzantine remnants,[54] diffused into medieval and Renaissance Europe through Latin translations.

The Arabic works attributed to Jabir ibn Hayyan introduced a systematic classification of chemical substances, and provided instructions for deriving an inorganic compound (sal ammoniac or ammonium chloride) from organic substances (such as plants, blood, and hair) by chemical means.[55] Some Arabic Jabirian works (e.g., the "Book of Mercy", and the "Book of Seventy") were later translated into Latin under the Latinized name "Geber",[56] and in 13th-century Europe an anonymous writer, usually referred to as pseudo-Geber, started to produce alchemical and metallurgical writings under this name.[57] Later influential Muslim philosophers, such as Abū al-Rayhān al-Bīrūnī[58] and Avicenna[59] disputed the theories of alchemy, particularly the theory of the transmutation of metals.

Georgius Agricola, author of De re metallica, was the first to drop the Arabic definite article al-, exclusively writing chymia and chymista, giving chemistry its modern name.[60][61][62]

Improvements of the refining of ores and their extractions to smelt metals was widely used source of information for early chemists in the 16th century, among them Georg Agricola (1494–1555), who published his major work De re metallica in 1556. His work, describing highly developed and complex processes of mining metal ores and metal extraction, were the pinnacle of metallurgy during that time. His approach removed all mysticism associated with the subject, creating the practical base upon which others could and would build. The work describes the many kinds of furnaces used to smelt ore, and stimulated interest in minerals and their composition. Agricola has been described as the "father of metallurgy" and the founder of geology as a scientific discipline.[63][61][62]

Under the influence of the Scientific Revolution and its new empirical methods propounded by Sir Francis Bacon and others, a group of chemists at Oxford, Robert Boyle, Robert Hooke and John Mayow began to reshape the old alchemical traditions into a scientific discipline. Boyle in particular questioned some commonly held chemical theories and argued for chemical practitioners to be more "philosophical" and less commercially focused in The Sceptical Chemyst.[36] He formulated Boyle's law, rejected the classical "four elements" and proposed a mechanistic alternative of atoms and chemical reactions that could be subject to rigorous experiment.[64]

Antoine-Laurent de Lavoisier is considered the "Father of Modern Chemistry".[65]

In the following decades, many important discoveries were made, such as the nature of 'air' which was discovered to be composed of many different gases. The Scottish chemist Joseph Black and the Flemish Jan Baptist van Helmont discovered carbon dioxide, or what Black called 'fixed air' in 1754; Henry Cavendish discovered hydrogen and elucidated its properties and Joseph Priestley and, independently, Carl Wilhelm Scheele isolated pure oxygen. The theory of phlogiston (a substance at the root of all combustion) was propounded by the German Georg Ernst Stahl in the early 18th century and was only overturned by the end of the century by the French chemist Antoine Lavoisier, the chemical analogue of Newton in physics. Lavoisier did more than any other to establish the new science on proper theoretical footing, by elucidating the principle of conservation of mass and developing a new system of chemical nomenclature used to this day.[66]

English scientist John Dalton proposed the modern theory of atoms; that all substances are composed of indivisible 'atoms' of matter and that different atoms have varying atomic weights.

The development of the electrochemical theory of chemical combinations occurred in the early 19th century as the result of the work of two scientists in particular, Jöns Jacob Berzelius and Humphry Davy, made possible by the prior invention of the voltaic pile by Alessandro Volta. Davy discovered nine new elements including the alkali metals by extracting them from their oxides with electric current.[67]

In his periodic table, Dmitri Mendeleev predicted the existence of 7 new elements,[68] and placed all 60 elements known at the time in their correct places.[69]

British William Prout first proposed ordering all the elements by their atomic weight as all atoms had a weight that was an exact multiple of the atomic weight of hydrogen. J.A.R. Newlands devised an early table of elements, which was then developed into the modern periodic table of elements[70] in the 1860s by Dmitri Mendeleev and independently by several other scientists including Julius Lothar Meyer.[71][72] The inert gases, later called the noble gases were discovered by William Ramsay in collaboration with Lord Rayleigh at the end of the century, thereby filling in the basic structure of the table.

Organic chemistry was developed by Justus von Liebig and others, following Friedrich Wöhler's synthesis of urea.[73] Other crucial 19th century advances were; an understanding of valence bonding (Edward Frankland in 1852) and the application of thermodynamics to chemistry (J. W. Gibbs and Svante Arrhenius in the 1870s).

Top: Expected results: alpha particles passing through the plum pudding model of the atom undisturbed.
Bottom: Observed results: a small portion of the particles were deflected, indicating a small, concentrated charge.

At the turn of the twentieth century the theoretical underpinnings of chemistry were finally understood due to a series of remarkable discoveries that succeeded in probing and discovering the very nature of the internal structure of atoms. In 1897, J.J. Thomson of the University of Cambridge discovered the electron and soon after the French scientist Becquerel as well as the couple Pierre and Marie Curie investigated the phenomenon of radioactivity. In a series of pioneering scattering experiments Ernest Rutherford at the University of Manchester discovered the internal structure of the atom and the existence of the proton, classified and explained the different types of radioactivity and successfully transmuted the first element by bombarding nitrogen with alpha particles.

His work on atomic structure was improved on by his students, the Danish physicist Niels Bohr, the Englishman Henry Moseley and the German Otto Hahn, who went on to father the emerging nuclear chemistry and discovered nuclear fission. The electronic theory of chemical bonds and molecular orbitals was developed by the American scientists Linus Pauling and Gilbert N. Lewis.

The year 2011 was declared by the United Nations as the International Year of Chemistry.[74] It was an initiative of the International Union of Pure and Applied Chemistry, and of the United Nations Educational, Scientific, and Cultural Organization and involves chemical societies, academics, and institutions worldwide and relied on individual initiatives to organize local and regional activities.

Practice

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In the practice of chemistry, pure chemistry is the study of the fundamental principles of chemistry, while applied chemistry applies that knowledge to develop technology and solve real-world problems.

Subdisciplines

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Chemistry is typically divided into several major sub-disciplines. There are also several main cross-disciplinary and more specialized fields of chemistry.[75]

  • Analytical chemistry is the analysis of material samples to gain an understanding of their chemical composition and structure. Analytical chemistry incorporates standardized experimental methods in chemistry. These methods may be used in all subdisciplines of chemistry, excluding purely theoretical chemistry.[76]
In analytical chemistry, spectroscopy studies interactions between electromagnetic radiation (light) and matter.[77] A spectrophotometer is a machine used to measure the effect light has on matter. The model pictured is the Beckman DU-640
The Kaminsky catalyst is an organometallic complex that features either zirconium or hafnium metal centers. Depending on the placement of the catalyst's cyclopentadiene ligands, it can produce polypropylenes with different tacticity.[80] 1 creates atactic polypropylene, which is soft and amorphous with a free-flowing composition. 2 creates isotactic polypropylene, which is hard and used in re-usable plastic containers. 3 creates syndiotactic polypropylene, which is rubbery and semi-crystalline.[81]
The Little Boy is an atomic bomb utilizing a uranium-235 fission reaction.[85] By firing sub-critical uranium into another mass of sub-critical uranium within the bomb, creating a supercritical mass, a self-sustaining nuclear reaction starts. It generated an explosive force of over 15,000 tons of equivalent TNT.
  • Organic chemistry is the study of the structure, properties, composition, mechanisms, and reactions of organic compounds. An organic compound is defined as any compound based on a carbon skeleton. Organic compounds can be classified, organized and understood in reactions by their functional groups, unit atoms or molecules that show characteristic chemical properties in a compound.[86]
4-Hydroxybutanal is an organic compound with an aldehyde (right) functional group and an alcohol (left) functional group.
The Solvay Conference of 1927 featured foundational scientists to the field of theoretical chemistry and physics. This conference discussed electrons and photons.

Other subdivisions include electrochemistry, femtochemistry, flavor chemistry, flow chemistry, immunohistochemistry, hydrogenation chemistry, mathematical chemistry, molecular mechanics, natural product chemistry, organometallic chemistry, petrochemistry, photochemistry, physical organic chemistry, polymer chemistry, radiochemistry, sonochemistry, supramolecular chemistry, synthetic chemistry, and many others.

Interdisciplinary

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Interdisciplinary fields include agrochemistry, astrochemistry (and cosmochemistry), atmospheric chemistry, chemical engineering, chemical biology, chemo-informatics, environmental chemistry, geochemistry, green chemistry, immunochemistry, marine chemistry, materials science, mechanochemistry, medicinal chemistry, molecular biology, nanotechnology, oenology, pharmacology, phytochemistry, solid-state chemistry, surface science, thermochemistry, and many others.

Industry

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The chemical industry represents an important economic activity worldwide. The global top 50 chemical producers in 2013 had sales of US$980.5 billion with a profit margin of 10.3%.[87]

Professional societies

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See also

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References

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Bibliography

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Further reading

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Revisions and contributorsEdit on WikipediaRead on Wikipedia
from Grokipedia
Chemistry is the scientific discipline that studies , its , composition, , and the changes it undergoes during interactions with other and . At its core, chemistry explores the behavior of atoms, molecules, and ions, encompassing everything from the simplest elements to complex compounds, and it forms the foundation for understanding natural phenomena and technological advancements. The field is broadly divided into several key branches that address different aspects of matter and its transformations. Analytical chemistry focuses on methods to separate, identify, and quantify components in samples, essential for fields like forensics and . Organic chemistry examines carbon-containing compounds, which are vital for pharmaceuticals, plastics, and biological molecules. Inorganic chemistry studies non-carbon compounds, including metals and minerals, contributing to and . Physical chemistry applies principles of physics to chemical systems, investigating reaction mechanisms, , and quantum behaviors. Biochemistry, overlapping with , explores chemical processes within living organisms, such as and . These branches interconnect, driving innovations in medicine, energy, and sustainability. Chemistry's importance permeates daily life, as it underpins the air we breathe, the food we consume, and the materials we use, from clothing to electronics. It enables the transformation of natural resources into life-improving products, such as cleaner fuels and effective drugs, while addressing global challenges like climate change through sustainable practices. Historically, chemistry evolved from ancient alchemical pursuits to a rigorous science in the 18th century, with Antoine Lavoisier establishing foundational principles like the conservation of mass through precise experimentation. This progression, including the development of the periodic table in the 19th century, has solidified chemistry as a central pillar of modern science.

Core Concepts

Matter and Its Properties

is defined as anything that has mass and occupies space, possessing both volume and the ability to exert gravitational attraction. This fundamental concept forms the foundation of chemistry, encompassing all tangible substances from everyday objects to natural phenomena. can exist in various forms and is characterized by observable attributes that distinguish one type from another. is classified into two broad categories: pure substances and mixtures. Pure substances consist of a single type of particle and cannot be separated into simpler components by physical means; they are further divided into elements, which are basic substances like oxygen or that cannot be broken down chemically, and compounds, such as or , formed by combining elements in fixed ratios. Mixtures, on the other hand, comprise two or more substances that retain their individual properties and can be separated physically; these are subdivided into homogeneous mixtures, which have uniform composition throughout (e.g., saltwater solutions), and heterogeneous mixtures, which exhibit non-uniform regions (e.g., sand in ). Physical properties of matter are characteristics that can be observed or measured without altering the substance's . Key examples include , defined as per unit and measured by dividing the (often via a balance) by the (displaced or geometric calculation); color, assessed visually or spectrophotometrically; , the at which a becomes a , determined using a melting point apparatus; and , the at which a turns to gas under standard , measured with a in a controlled heating setup. These properties aid in identifying and characterizing , providing insights into its behavior under different conditions. Matter exists in four primary states: , , , and plasma, each defined by the arrangement and movement of its particles. In , particles are tightly packed in a fixed, vibrating lattice, giving definite and ; feature particles close together but able to slide past one another, resulting in a definite but indefinite that conforms to the container; gases have particles far apart and moving rapidly in random directions, leading to neither fixed nor , expanding to fill available space; and plasma, an ionized gas, consists of charged particles (free electrons and ions) that conduct , commonly observed in and . Transitions between states occur with energy changes: converts to by overcoming particle attractions; (or ) shifts to gases by further increasing ; and sublimation directly transforms to gases, as seen in . Properties of matter are categorized as extensive or intensive based on their dependence on sample size. Extensive properties, such as (measured by weighing) and (calculated via displacement or dimensions), vary with the amount of matter present. In contrast, intensive properties like (gauged with thermometers) and (measured by barometers or manometers) remain constant regardless of sample quantity, making them useful for material identification. During physical changes, such as state transitions or dissolving, the total of matter is conserved, meaning no matter is created or destroyed—the before equals the after the process. This principle, rooted in classical observations, underscores that physical processes merely rearrange matter without altering its total quantity.

Atoms and Elements

Atoms are the fundamental building blocks of , as proposed by in his atomic theory published in 1808. Dalton's theory, based on the laws of and definite proportions, posited five key postulates: all is composed of tiny, indivisible particles called atoms; atoms of the same element are identical in mass and properties, while atoms of different elements differ in mass and properties; atoms cannot be created or destroyed in chemical reactions but can rearrange; compounds form when atoms of different elements combine in simple whole-number ratios; and the relative numbers and kinds of atoms in a compound are constant across samples. Although later discoveries revealed atoms are divisible and isotopes exist, Dalton's framework laid the foundation for modern chemistry by shifting from continuous to discrete views of . Subatomic particles constitute the structure of atoms. The , with a charge of -1 and mass approximately 1/1836 atomic mass units (u), was discovered by J.J. Thomson in 1897 via cathode ray tube experiments, revealing negatively charged particles within atoms. The proton, positively charged at +1 and mass about 1 u, was identified by in 1919 through scattering, confirming a dense positive nucleus. The , neutral with mass roughly 1 u, was discovered by in 1932 using beryllium bombardment, explaining isotopic mass variations. Protons and neutrons reside in the , while electrons occupy the surrounding electron cloud or orbitals. The (Z) equals the number of protons in the nucleus, defining the element's identity, as established by in 1913 through . The (A) is the sum of protons and neutrons. Isotopes are atoms of the same element (same Z) but different A, such as and , first recognized by in 1913. The , reported in the periodic table, is the weighted average of naturally occurring isotopes' masses, accounting for their relative abundances. The periodic table organizes the 118 known elements based on increasing , refining Dmitri Mendeleev's 1869 arrangement by that predicted undiscovered elements like and . It features seven periods (horizontal rows) corresponding to principal fillings and 18 groups (vertical columns) sharing similar configurations and properties. Key trends include , which decreases across a period due to increasing and increases down a group from added s; first , the energy to remove an , which increases across periods (stronger nuclear pull) and decreases down groups (s farther from nucleus); and , the ability to attract s in bonds, which rises across periods and falls down groups, quantified on the Pauling scale from 0.7 () to 4.0 (). A seminal discovery was , the lightest element (Z=1), isolated and described as "inflammable air" by in 1766 through reactions of metals with acids in his laboratory. Cavendish noted its low density and to form , though later named it in 1783. Elemental abundances vary by context, reflecting cosmic and geological processes. In the , dominates at about 73.5% by mass, followed by at 23.8%, with oxygen (1%) and carbon (0.46%) next from stellar fusion; heavier elements total ~2%.
Top Elements in Universe (by mass %)
: 73.5
: 23.8
Oxygen: 1.0
Carbon: 0.46
: 0.13
In Earth's crust, oxygen is most abundant at 46.6%, comprising silicates and oxides, followed by silicon (27.7%), aluminum (8.1%), and iron (5.0%).
Top Elements in Earth's Crust (by mass %)
Oxygen: 46.6
Silicon: 27.7
Aluminum: 8.1
Iron: 5.0
Calcium: 3.6
In the , oxygen constitutes 65% by mass (mostly in ), carbon 18%, 10%, 3%, calcium 1.5%, and 1%, with trace elements like iron (~0.006%) essential for functions such as oxygen transport.
Top Elements in Human Body (by mass %)
Oxygen: 65
Carbon: 18
Hydrogen: 10
Nitrogen: 3
Calcium: 1.5

Molecules, Compounds, and Mixtures

Molecules are electrically neutral entities consisting of more than one atom, where the atoms are bound together by chemical bonds, and the structure corresponds to a depression on the deep enough to confine at least one vibrational state. This definition encompasses discrete units that can exist independently, such as diatomic molecules like O₂ or polyatomic ones like CO₂. Molecules form the basis of molecular compounds, which are substances composed of covalently bonded atoms forming discrete units, in contrast to ionic compounds, where the basic structural unit is an extended lattice of ions held together by electrostatic attractions rather than individual molecules. For instance, (H₂O) is a molecular compound consisting of two hydrogen atoms covalently bonded to one oxygen atom, while (NaCl) is an ionic compound formed from sodium ions and chloride ions in a crystalline lattice. Compounds are chemical substances formed by the chemical combination of two or more elements in fixed proportions by mass, as established by the law of definite proportions, first proposed by Joseph Louis Proust in his 1794 publication on sugars. This law states that every chemical compound contains its constituent elements in a constant ratio by mass, regardless of the source or method of preparation, providing a foundational principle for understanding compound composition. Chemical formulas represent these compositions: the empirical formula gives the simplest whole-number ratio of atoms (e.g., CH₂O for formaldehyde), the molecular formula indicates the actual number of atoms (e.g., C₂H₄O₂ for acetic acid), and the structural formula depicts the arrangement of atoms and bonds. To determine an empirical formula from percentage composition, one assumes a 100 g sample, calculates the moles of each element by dividing the mass percentage by the atomic mass, divides by the smallest mole value to find the ratio, and multiplies to obtain whole numbers if necessary; for example, a compound with 40.0% carbon, 6.71% hydrogen, and 53.3% oxygen yields moles of 3.33, 6.67, and 3.33, respectively, giving a ratio of 1:2:1 and thus CH₂O. In contrast to compounds, mixtures consist of two or more substances physically combined without fixed proportions, retaining their individual properties. Homogeneous mixtures, or solutions, feature uniform distribution of solute particles (ions or molecules smaller than 1 nm) throughout the , allowing independent movement of components; is an example, with salt ions dispersed in . Colloids are heterogeneous mixtures with dispersed particles of 1–1000 nm, which do not settle and scatter light (), such as milk where fat globules are suspended in . Suspensions are heterogeneous mixtures with larger particles (>1000 nm) that settle upon standing, like sand in . Separation techniques exploit these differences: removes suspended solids from liquids by passing through a porous barrier, separates solutions based on differing points by and , and divides components by differential adsorption or partitioning on a stationary phase as they move with a mobile phase. Alloys, such as ( and ), exemplify homogeneous mixtures of metals that enhance properties like strength, while amalgams are specific alloys incorporating mercury, used historically in thermometers and for their fluidity.

Mole and Amount of Substance

The amount of substance, denoted by the symbol nn, is a measure of the number of specified elementary entities, such as atoms, molecules, ions, or other particles, in a sample. The mole is the International System of Units (SI) base unit for amount of substance, adopted to quantify substances on a macroscopic scale while linking to the microscopic realm of individual particles. In 2019, the mole was redefined to contain exactly 6.02214076×10236.02214076 \times 10^{23} elementary entities, establishing Avogadro's constant NAN_A as a fixed value rather than a measured quantity, which enhanced precision in chemical measurements. This redefinition aligns the mole with fundamental physical constants, improving consistency across metrology and chemistry. Avogadro's constant represents the number of entities in one mole, bridging the gap between countable particles and weighable masses in chemical analysis. The concept originated from Amedeo Avogadro's 1811 hypothesis, which posited that equal volumes of different gases, under the same and , contain an equal number of molecules, providing a foundation for understanding molecular quantities in gases. This idea, initially overlooked, was later championed by in 1858, leading to its widespread acceptance and the development of atomic weights. The hypothesis gained experimental support through methods like , where Michael Faraday's laws in the 1830s demonstrated that the mass of a substance deposited or liberated at an is proportional to the passed, allowing indirect determination of particle numbers when combined with the . For instance, electrolyzing solution deposits atoms proportional to electrons transferred, yielding Avogadro's constant as NA=F/eN_A = F / e, where FF is the (96485.332196485.3321 C/mol) and ee is the electron charge; modern values confirm NAN_A near 6.022×10236.022 \times 10^{23} mol1^{-1}. Molar mass MM, expressed in grams per mole (g/mol), is the mass of one mole of a substance, calculated by summing the es of its constituent elements as defined by IUPAC standard atomic weights. For elements, it equals the in atomic mass units (u) numerically; for compounds like (H2_2O), M=2×1.008+15.999=18.015M = 2 \times 1.008 + 15.999 = 18.015 g/mol. These values, derived from and other techniques, enable precise stoichiometric calculations. Conversions involving the mole facilitate practical measurements in chemistry. To find moles from , use n=mMn = \frac{m}{M}, where mm is in grams; for example, 36.03 g of yields 2 mol. The number of entities NN relates via N=n×NAN = n \times N_A, so 1 mol of contains exactly 6.02214076×10236.02214076 \times 10^{23} atoms. For gases at (STP: 0°C and 1 ), the is 22.414 L/mol for an , allowing volume-to-mole conversion as n=V22.414n = \frac{V}{22.414}; thus, 44.8 L of oxygen gas equals 2 mol. In , the mole quantifies reactant and product amounts in chemical equations, ensuring conservation of atoms. For the reaction 2H2+O22H2O2\text{H}_2 + \text{O}_2 \to 2\text{H}_2\text{O}, 2 mol of gas react with 1 mol of oxygen gas to produce 2 mol of , guiding predictions of yields from measured quantities. This approach underpins reaction scaling in laboratories and industry. composition by of an element in a compound is calculated as \left( \frac{\text{[atomic mass](/page/Atomic_mass)} \times \text{number of atoms}}{M} \right) \times 100\%; for in , it is (2×1.00818.015)×100%11.19%\left( \frac{2 \times 1.008}{18.015} \right) \times 100\% \approx 11.19\%. Empirical formulas derive from these percentages by converting to moles (e.g., divide by atomic masses), then simplifying ratios; for a compound with 40% carbon, 6.7% , and 53.3% oxygen by , mole ratios approximate C:H:O = 3.3:6.7:3.3 or CH2_2O after division by the smallest. These tools, rooted in molar concepts, enable determination of simplest formulas from analytical data like .

Chemical Bonding and Interactions

Types of Chemical Bonds

Chemical bonds are the attractive forces that hold atoms together to form molecules, ions, and extended structures, primarily arising from interactions between valence electrons of atoms. The main types of chemical bonds—ionic, covalent, and metallic—differ in how electrons are involved in the bonding process, leading to distinct properties in the resulting substances. These bonds form when atoms achieve more stable electron configurations, often approaching a filled outer shell. Ionic bonds occur through the complete transfer of one or more valence electrons from a metal atom to a atom, resulting in the formation of positively charged cations and negatively charged anions that are held together by electrostatic attractions. This typically happens between metals, which have low and tend to lose electrons, and nonmetals, which have high and gain electrons. A classic example is (NaCl), where sodium (Na) loses one electron to become Na⁺, and (Cl) gains it to become Cl⁻, forming a crystalline lattice stabilized by these oppositely charged ions. The strength of ionic bonds in such lattices is quantified by , which is the energy released when gaseous ions combine to form a solid ionic compound; higher lattice energies indicate stronger bonds, influenced by ion charges and distances. Covalent bonds form when two atoms, usually nonmetals, share one or more pairs of valence electrons to achieve configurations, allowing each atom partial access to the shared electrons. These bonds can be single (one shared pair), double (two shared pairs), or triple (three shared pairs), with multiple bonds being shorter and stronger than single bonds due to greater overlap. Covalent bonds are classified as nonpolar if the electronegativity difference between the atoms is small (typically less than 0.4), leading to equal sharing, as in H₂, or polar if the difference is moderate (0.4 to 1.7), resulting in unequal sharing and a dipole moment, as in HCl where pulls electrons more strongly. Metallic bonds characterize the bonding in pure metals and alloys, where valence electrons are delocalized and free to move throughout a lattice of positively charged metal ions, creating a "sea of electrons" that binds the structure together. This delocalization explains key metallic properties, such as high electrical and thermal conductivity, as the mobile electrons can carry charge and heat efficiently, and malleability and , since the ions can shift positions under stress without breaking the bond network. Unlike ionic or covalent bonds, metallic bonds are nondirectional, allowing metals to deform without fracturing. The strength and dimensions of chemical bonds are described by , the energy required to break one mole of bonds in the gas phase, and , the average distance between bonded nuclei; generally, stronger bonds have higher energies and shorter lengths. Factors influencing these include —the number of shared pairs—with higher orders (e.g., triple bonds) yielding shorter lengths and greater energies due to increased orbital overlap—and atomic size, where bonds between smaller atoms are stronger. For instance, the C≡C bond in has a bond energy of about 839 kJ/mol and length of 120 pm, compared to the C-C at 348 kJ/mol and 154 pm. Lewis dot structures provide a visual representation of valence electrons and bonds in molecules and ions, using dots for lone pairs and lines for shared pairs (bonds) around atomic symbols. To construct them, one counts total valence electrons from the atoms involved, arranges them to form bonds between the central atom and others, and distributes remaining electrons as lone pairs to satisfy the where possible. For example, in H₂O, oxygen's six valence electrons pair with two from atoms to form two single bonds, leaving two lone pairs on oxygen. These structures help predict patterns but are simplified models. The states that atoms tend to gain, lose, or share electrons to achieve eight valence electrons in their outer shell, mimicking stability, which guides much of bond formation in main-group elements. However, exceptions exist, particularly for incomplete octets in electron-deficient compounds like those of , which has only three valence electrons and often forms three bonds without a full octet; for instance, (BF₃) has boron with six electrons, making it a Lewis acid that can accept additional pairs. Other exceptions include expanded octets in elements beyond the second period, but compounds highlight the rule's limitations for lighter elements.

Molecular Structure and Geometry

Molecular structure refers to the arrangement of atoms within a , while describes the three-dimensional spatial configuration of those atoms, which profoundly influences chemical and physical properties such as reactivity, polarity, and intermolecular interactions. The shapes of molecules arise from the balance of repulsions and bonding forces, determining everything from boiling points to . Understanding these geometries is essential for predicting molecular behavior in various environments. The provides a foundational framework for predicting molecular geometries by considering the repulsion between pairs in the valence shell of the central atom. Developed by Ronald J. Gillespie and Ronald S. Nyholm, this model posits that pairs arrange themselves to minimize repulsion, leading to characteristic shapes such as linear for two electron domains (e.g., BeCl₂), trigonal planar for three (e.g., BF₃), and tetrahedral for four (e.g., CH₄). Lone pairs exert greater repulsion than bonding pairs, distorting geometries; for instance, five electron domains yield trigonal bipyramidal arrangements, while six produce octahedral. This simple yet effective approach applies to main-group compounds and explains deviations from ideal bond angles. Hybridization theory complements VSEPR by describing how atomic orbitals mix to form new hybrid orbitals suitable for the molecule's geometry. introduced this concept within , proposing that s and p orbitals combine to create hybrid orbitals with equivalent energy and directional properties. For example, in (CH₄), the carbon atom undergoes sp³ hybridization, forming four equivalent tetrahedral orbitals at 109.5° angles, as confirmed by experimental bond lengths of approximately 1.086 Å and angles of 109.47°. In ethene (C₂H₄), carbon uses sp² hybridization for trigonal planar geometry with 120° angles, while in ethyne (C₂H₂), sp hybridization results in linear arrangements at 180°. This orbital mixing accounts for the observed symmetries and strengths of covalent bonds in organic and inorganic molecules. Molecular polarity emerges from the asymmetric distribution of , quantified by the dipole moment, which measures the charge separation across the . In (H₂O), the bent geometry from sp³ hybridization on oxygen, with a bond angle of 104.5°, creates a net dipole moment of 1.855 D due to the difference between oxygen and , making it a polar . Conversely, (CO₂) exhibits a linear geometry from sp hybridization, with symmetric O=C=O bonds canceling individual bond , resulting in a zero net dipole moment and nonpolar character, as verified by spectroscopic data showing no permanent . This polarity dictates , bonding capability, and interactions in solutions. Isomerism arises when molecules share the same molecular formula but differ in atom connectivity or spatial arrangement, often due to geometric constraints. Structural isomers vary in bonding patterns, such as chain branching in alkanes (e.g., n-butane vs. ), while stereoisomers maintain connectivity but differ in 3D orientation. Geometric (cis-trans) isomers occur in compounds with restricted rotation, like square planar complexes or alkenes, where substituents on the same side (cis) or opposite (trans) affect stability and reactivity. Optical isomers, or enantiomers, feature non-superimposable mirror images due to chiral centers, as in with tetrahedral carbon atoms bearing four different groups, leading to distinct biological activities. These geometric variations underscore how subtle shape differences can yield vastly different properties. Illustrative examples highlight these principles. (CH₄) adopts a tetrahedral via sp³ hybridization, with all C-H bonds equivalent and a zero dipole moment, contributing to its nonpolar nature and gaseous state at . (NH₃), however, features trigonal pyramidal due to a on in an sp³ hybridized valence shell, resulting in a bond angle of 107° and a dipole moment of 1.47 D, which enables hydrogen bonding. In solid states, molecular geometry extends to extended structures like crystal lattices, where repeating units dictate material properties. Ionic crystals, such as (NaCl), form cubic rock salt lattices with octahedral coordination around each ion, determined by X-ray diffraction revealing Na-Cl distances of 2.81 . Molecular crystals, like (H₂O), consist of discrete molecules linked by hydrogen bonds in a , with tetrahedral arrangements around each oxygen, leading to open structures and lower than liquid . These architectures influence , melting points, and conductivity in solids.

Intermolecular Forces and Phases

Intermolecular forces are the attractive interactions between s that arise from electrostatic effects, influencing the physical properties of substances, particularly their phase behavior. These forces are weaker than intramolecular chemical bonds but play a crucial role in determining how molecules associate in liquids and solids, affecting properties such as and points. Unlike intramolecular bonds, which hold atoms within a molecule, intermolecular forces operate between separate molecules and include several types: London dispersion forces, dipole-dipole interactions, hydrogen bonding, and ion-dipole forces. London dispersion forces, present in all molecules, result from temporary fluctuations in distribution that induce momentary s, leading to weak attractions; their strength increases with molecular size and . Dipole-dipole interactions occur between polar molecules, where the positive end of one dipole attracts the negative end of another, providing stronger attractions than dispersion forces in polar substances. Hydrogen bonding is a particularly strong dipole-dipole interaction involving hydrogen atoms bonded to highly electronegative atoms like , oxygen, or , forming with the lone pairs on adjacent electronegative atoms. Ion-dipole forces, the strongest among these, arise between ions and polar molecules, as seen in solutions where cations or anions align with the dipole of molecules like . These intermolecular forces directly govern phase transitions by determining the energy required to separate molecules during or . Stronger forces lead to higher and points, as more is needed to overcome the attractions holding molecules in the solid or phase. For instance, —the pressure exerted by a substance's vapor in equilibrium with its —increases with but decreases with stronger intermolecular forces, since molecules are less likely to escape into the gas phase. occurs when equals , so substances with robust intermolecular forces, like those exhibiting bonding, require higher temperatures to boil. A classic example is , whose of 100°C is anomalously high compared to similar-sized molecules like H₂S (boiling point -60°C), due to extensive bonding networks that enhance cohesion. points follow a similar trend, with stronger forces resulting in more stable solid lattices that resist transition to the phase. The , expressed as PV=nRTPV = nRT, where PP is , VV is , nn is the , RR is the , and TT is , assumes no intermolecular forces or molecular volume, treating gases as point particles with only elastic collisions. Real gases deviate from this behavior at high s or low s, where intermolecular attractions reduce the pressure exerted on container walls (causing PV/nRT<1PV/nRT < 1) or repulsive forces at close distances increase effective (causing PV/nRT>1PV/nRT > 1). These deviations highlight how intermolecular forces become significant when molecules are closer together, transitioning gases toward liquid-like behavior. Phase diagrams map the conditions under which different phases of a substance coexist or predominate, illustrating the effects of and on phase stability influenced by intermolecular forces. The marks the unique and where , , and gas phases are in equilibrium, such as 0.01°C and 611 Pa for . The critical point represents the end of the liquid-gas coexistence curve, beyond which the distinction between liquid and gas vanishes in a ; for , this occurs at 374°C and 22.1 MPa, where intermolecular forces are overcome by . In high-energy conditions, such as those in stars or plasma torches, can enter the plasma phase, the fourth state where atoms are ionized into a of positively charged nuclei and free electrons, behaving collectively under electromagnetic fields due to the dominance of over intermolecular attractions.

Energy and Reactions

Thermochemistry and Energy Changes

Thermochemistry is the branch of chemistry that studies the energy changes associated with chemical reactions and physical transformations, focusing primarily on transfers under constant or conditions. It provides essential insights into the feasibility and energetics of processes, distinguishing between absorbed or released during bond breaking and formation. The first law of thermodynamics, a fundamental principle in , states that the change in of a system, denoted as ΔU\Delta U, equals the added to the system ([q](/page/Q)[q](/page/Q)) plus the work done on the system ([w](/page/W)[w](/page/W)), expressed as ΔU=[q](/page/Q)+[w](/page/W)\Delta U = [q](/page/Q) + [w](/page/W). UU represents the total kinetic and of the system's particles, while [q](/page/Q)[q](/page/Q) is energy transferred due to differences, and work [w](/page/W)[w](/page/W) typically involves pressure-volume changes, such as w=PΔVw = -P\Delta V for expansion against constant pressure. This underscores the , ensuring that cannot be created or destroyed in chemical processes. To address limitations of in constant-pressure scenarios, chemists use HH, defined as H=U+PVH = U + PV, where PP is and VV is . The change in ΔH\Delta H approximates the heat transferred at constant (qp=ΔHq_p = \Delta H), making it particularly useful for reactions in open systems like laboratories. Standard changes, denoted ΔH\Delta H^\circ, are measured under standard conditions of 298 K and 1 bar , often referenced to standard states of pure substances. Hess's law enables the calculation of ΔH\Delta H^\circ for a reaction by summing the standard enthalpies of formation (ΔHf\Delta H_f^\circ) of products minus those of reactants, without directly performing the reaction. Formally, ΔH=ΔHf(products)ΔHf(reactants)\Delta H^\circ = \sum \Delta H_f^\circ (\text{products}) - \sum \Delta H_f^\circ (\text{reactants}), as is a independent of pathway. This approach is invaluable for complex reactions, such as or synthesis, where direct measurement is impractical. Bond dissociation energies (BDEs) quantify the required to break a specific bond homolytically into radicals, contributing to the net change in reactions. For instance, the BDE for the C-H bond in is approximately 439 kJ/mol, indicating the input needed to cleave it. In , the overall ΔH\Delta H for a reaction approximates the sum of BDEs of bonds broken minus those formed, providing a method to estimate changes from molecular . Chemical reactions are classified as exothermic if they release (ΔH<0\Delta H < 0), warming the surroundings, or endothermic if they absorb (ΔH>0\Delta H > 0), cooling the surroundings. Combustion of fuels, like , is a classic , while exemplifies an endothermic one. Calorimetry measures these heat changes experimentally. In a bomb calorimeter, reactions occur at constant volume, yielding ΔU\Delta U from temperature rise in surrounding , where qv=CΔTq_v = C \Delta T and CC is the . For constant-pressure measurements, a coffee-cup calorimeter uses cups to approximate adiabatic conditions, directly providing ΔH=qp=CΔT\Delta H = -q_p = -C \Delta T. These devices, often calibrated with known reactions like of , allow precise determination of enthalpies for solids, liquids, or gases. While enthalpy indicates energy changes, spontaneity of processes depends on G=HTSG = H - TS, where TT is and SS is ; a negative ΔG\Delta G suggests a spontaneous reaction under constant and . This criterion integrates enthalpic and entropic contributions, though full analysis of equilibrium constants lies beyond basic .

Chemical Kinetics

Chemical kinetics examines the speeds at which chemical reactions occur and the mechanisms by which they proceed, focusing on how factors like concentration, , and catalysts influence reaction rates. Unlike , which addresses the energy changes in reactions, chemical kinetics explores the temporal aspects, revealing pathways from reactants to products. This field is essential for understanding reaction dynamics in both and industrial contexts, enabling predictions of reaction behavior under varying conditions. The rate of a is quantitatively described by a rate law, typically expressed as rate = k [A]^m [B]^n, where k is the rate constant, [A] and [B] are reactant concentrations, and m and n are the partial reaction orders with respect to each reactant. These orders are not necessarily equal to the stoichiometric coefficients and must be determined experimentally through methods such as initial rate analysis or integrated rate plots, as the rate law reflects the rather than the balanced equation. The overall reaction order is the sum of the partial orders (m + n), which indicates the sensitivity of the rate to concentration changes; for instance, a zero-order reaction shows rate independence from concentration, while first- and second-order reactions exhibit linear and inverse dependencies, respectively. For first-order reactions, where the rate depends on a single reactant's concentration (rate = k [A]), the half-life—the time required for the reactant concentration to halve—is constant and independent of initial concentration, given by t_{1/2} = \frac{\ln 2}{k} \approx \frac{0.693}{k}. This derivation arises from integrating the rate law, yielding [A] = [A]_0 e^{-kt}, and setting [A] = [A]_0 / 2 to solve for t, highlighting the characteristic of processes like or certain decompositions./Kinetics/02%3A_Reaction_Rates/2.04%3A_Half-lives) Temperature profoundly affects reaction rates through (E_a), the minimum energy barrier that reactants must overcome to form products, often visualized as the energy difference to a high-energy . The quantifies this relationship: k = A e^{-E_a / RT}, where A is the representing collision frequency and orientation, R is the , and T is . Proposed by in 1889, this empirical model explains the exponential increase in rate with temperature, as higher temperatures provide more molecules with sufficient to surmount E_a, typically determined by plotting \ln k versus 1/T to yield a straight line with slope -E_a / R. (Note: Direct link to original paper; use DOI if available: 10.1515/zpch-1889-0406) Collision theory, independently developed by Max Trautz in 1916 and William Lewis in 1918, posits that reactions occur only when reactant molecules collide with sufficient energy (at least E_a) and proper orientation, with the rate proportional to the adjusted by a . This model successfully predicts the dependence via the Maxwell-Boltzmann distribution of molecular speeds but underestimates rates for complex molecules due to orientation requirements. , advanced by Henry Eyring in 1935, refines this by describing an or at the energy maximum, where the rate constant relates to the free energy of : k = \frac{k_B T}{h} e^{-\Delta G^\ddagger / RT}, with k_B as Boltzmann's constant and h as Planck's constant. This quasi-equilibrium approach between reactants and the provides a more accurate framework for bimolecular reactions, emphasizing effects alongside . Catalysts accelerate reactions by offering an alternative pathway with lower , without being consumed, thus increasing the rate constant while leaving the overall unchanged. Homogeneous catalysts operate in the same phase as reactants, such as or base catalysts in solution that stabilize transition states; heterogeneous catalysts, like metal surfaces in (e.g., in catalytic converters), adsorb reactants to weaken bonds and facilitate reaction at interfaces; enzymes, biological catalysts, exhibit high specificity and efficiency, often reducing E_a by 10-20 kcal/mol through precise active-site geometries that orient substrates optimally. Most reactions proceed via multi-step mechanisms consisting of elementary steps—single molecular events that are unimolecular (rate = k [A]), bimolecular (rate = k [A][B]), or rarely termolecular—whose sum yields the overall reaction. The rate-determining step, the slowest elementary step, governs the overall rate, as subsequent faster steps cannot compensate for the bottleneck; for example, if an initial fast equilibrium precedes a slow step, the rate law incorporates the equilibrium constant. In nucleophilic substitution reactions, the SN2 mechanism is a concerted bimolecular elementary step where the nucleophile attacks the carbon as the leaving group departs, with rate = k [alkyl halide][nucleophile] and inversion of configuration, favored for primary substrates. Conversely, the SN1 mechanism involves two elementary steps: a slow unimolecular dissociation to form a carbocation intermediate (rate-determining, rate = k [alkyl halide]), followed by rapid nucleophile attack, leading to racemization and suitability for tertiary substrates, as elucidated in Christopher Ingold's electronic theory of organic reactions./Kinetics/03%3A_Rate_Laws/3.02%3A_Reaction_Mechanisms/3.2.03%3A_Rate_Determining_Step)

Chemical Equilibrium

Chemical equilibrium refers to the state in a reversible where the concentrations of reactants and products remain constant over time, as the forward and reverse reaction rates become equal. This dynamic condition arises because both reactions continue to occur, but at balanced speeds, preventing net changes in composition. The concept underpins many natural and , distinguishing equilibrium from complete reaction by emphasizing reversibility and balance rather than exhaustion of reactants. The , denoted as K, quantifies this balance for a given reaction at a specific . For a general aA+bBcC+dDa\mathrm{A} + b\mathrm{B} \rightleftharpoons c\mathrm{C} + d\mathrm{D}, where A and B are reactants and C and D are products, K is expressed as K=[C]c[D]d[A]a[B]bK = \frac{[\mathrm{C}]^c [\mathrm{D}]^d}{[\mathrm{A}]^a [\mathrm{B}]^b} at equilibrium, with concentrations in molarity (or partial pressures for gases). This formulation, known as the law of mass action, was first proposed by Cato Maximilian Guldberg and Peter Waage in 1864, establishing that the extent of reaction depends on the product of reactant concentrations raised to stoichiometric powers. The value of K indicates the reaction's tendency: K > 1 favors products, while K < 1 favors reactants. K varies with temperature but is independent of initial concentrations or total pressure. Thermodynamically, K connects to the standard Gibbs free energy change (ΔG\Delta G^\circ) via ΔG=RTlnK\Delta G^\circ = -RT \ln K where R is the gas constant (8.314 J/mol·K) and T is the absolute temperature. This equation, derived from the principles of chemical potential equality at equilibrium, shows that spontaneous reactions (negative ΔG\Delta G^\circ) have K > 1, linking equilibrium position to energetic favorability as outlined in ' foundational work on heterogeneous equilibria. A reference to free energy changes highlights how ΔG\Delta G^\circ determines overall feasibility, though actual ΔG\Delta G depends on conditions. To predict the direction of approach to equilibrium, the Q is used, calculated identically to K but with concentrations at any instant: Q=[C]c[D]d[A]a[B]bQ = \frac{[\mathrm{C}]^c [\mathrm{D}]^d}{[\mathrm{A}]^a [\mathrm{B}]^b} If Q < K, the forward reaction predominates to increase products; if Q > K, the reverse reaction occurs to consume excess products; and Q = K signals equilibrium. This comparison allows assessment of whether a system will shift left or right without waiting for balance./Equilibria/Chemical_Equilibria/Difference_Between_K_And_Q) Le Chatelier's principle describes how equilibrium responds to perturbations, stating that the system shifts to minimize the imposed change. Increasing reactant concentration drives the reaction forward to consume the added species, while adding products shifts it reverse. For gaseous reactions, raising pressure favors the side with fewer moles of gas; for example, in N2(g)+3H2(g)2NH3(g)\mathrm{N_2(g)} + 3\mathrm{H_2(g)} \rightleftharpoons 2\mathrm{NH_3(g)}, higher pressure promotes formation. Temperature changes affect based on reaction exothermicity: heating an exothermic equilibrium decreases , shifting toward reactants, whereas endothermic reactions increase with heat. Catalysts accelerate both forward and reverse rates equally, hastening equilibrium attainment without altering or position. These effects, first articulated by Henri Louis Le Chatelier in 1884, guide optimization in processes like synthesis. In acid-base equilibria, the principle applies briefly to dissociation, such as HAH++A\mathrm{HA} \rightleftharpoons \mathrm{H^+} + \mathrm{A^-}, where the acid dissociation constant Ka=[H+][A][HA]K_a = \frac{[\mathrm{H^+}][\mathrm{A^-}]}{[\mathrm{HA}]} governs the balance, with shifts responding to pH or added base per Le Chatelier's predictions. Similarly, solubility equilibria for precipitates use the solubility product constant Ksp, the equilibrium constant for dissolution: for MX(s)M+(aq)+X(aq)\mathrm{MX}(s) \rightleftharpoons \mathrm{M^+}(aq) + \mathrm{X^-}(aq), Ksp=[M+][X]K_{sp} = [\mathrm{M^+}][\mathrm{X^-}]. Low Ksp values indicate poor solubility, and common ions reduce dissolution by shifting equilibrium left. For silver chloride, Ksp=[Ag+][Cl]=1.8×1010K_{sp} = [\mathrm{Ag^+}][\mathrm{Cl^-}] = 1.8 \times 10^{-10} at 25°C, exemplifying precipitation control./Equilibria/Solubilty/Solubility_Product_Constant_Ksp) A key industrial example is the Haber-Bosch process for ammonia synthesis: N2(g)+3H2(g)2NH3(g)\mathrm{N_2(g)} + 3\mathrm{H_2(g)} \rightleftharpoons 2\mathrm{NH_3(g)}, an with Kp4.5×105K_p \approx 4.5 \times 10^{-5} at 450°C. Low K limits yield, but high pressure shifts equilibrium right (fewer gas moles on product side), moderate balances kinetics, and iron catalysts speed approach without changing K. This application of enables large-scale fertilizer production, though unreacted gases are recycled to maintain Q < K./Equilibria/Le_Chateliers_Principle/The_Haber_Process)

Key Processes and Laws

Acids, Bases, and pH

Acids and bases are fundamental classes of chemical compounds that play crucial roles in numerous reactions and processes. According to the Arrhenius definition, proposed by in his 1887 dissertation on electrolytic dissociation, an acid is a substance that increases the concentration of hydrogen ions (H⁺) in aqueous solution, while a base increases the concentration of hydroxide ions (OH⁻). This model explains the behavior of many common substances, such as (HCl), which dissociates completely to produce H⁺ and Cl⁻ ions, and (NaOH), which produces Na⁺ and OH⁻ ions. However, the Arrhenius theory is limited to aqueous solutions and does not account for reactions without water or proton transfer. To address these limitations, Johannes Nicolaus Brønsted and Thomas Martin Lowry independently developed a broader definition in 1923. In the Brønsted-Lowry theory, an acid is a proton (H⁺) donor, and a base is a proton acceptor; this framework emphasizes acid-base reactions as proton transfer processes, forming conjugate acid-base pairs. For instance, in the reaction HCl + NH₃ → NH₄⁺ + Cl⁻, HCl acts as the acid (donating H⁺) and NH₃ as the base (accepting H⁺), with NH₄⁺ and Cl⁻ as the conjugate acid and base, respectively. This definition applies beyond aqueous media and highlights reversible equilibria. Complementing this, Gilbert N. Lewis proposed in 1923 that an acid is an electron-pair acceptor and a base is an electron-pair donor, focusing on coordinate covalent bond formation; for example, BF₃ accepts an electron pair from NH₃ to form F₃B–NH₃. The Lewis theory encompasses a wider range of reactions, including those without protons, such as metal-ligand complexes. The strength of an acid or base refers to its degree of dissociation in solution, quantified by s. Strong acids, like HCl, completely dissociate in water (e.g., HCl → H⁺ + Cl⁻), yielding high concentrations of H⁺ and having very large acid s (K_a > 1). Weak acids, such as acetic acid (CH₃COOH), partially dissociate according to the equilibrium CH₃COOH ⇌ H⁺ + CH₃COO⁻, with K_a = 1.8 × 10⁻⁵ at 25°C, indicating limited . Similarly, strong bases like NaOH fully dissociate to OH⁻, while weak bases like (NH₃) partially ionize via NH₃ + H₂O ⇌ NH₄⁺ + OH⁻, with base K_b = 1.8 × 10⁻⁵. The K_a for an acid HA is defined as Ka=[H+][A][HA]K_a = \frac{[H^+][A^-]}{[HA]} where concentrations are at equilibrium; pK_a = -log K_a measures acidity, with lower pK_a indicating stronger acids. For bases, K_b follows an analogous form. These constants derive from the applied to dissociation equilibria. The scale provides a quantitative measure of acidity in aqueous solutions, defined by Søren P.L. Sørensen in as = -log₁₀[H⁺], where [H⁺] is the concentration in moles per liter. This logarithmic scale ranges from 0 to 14 under standard conditions at 25°C, with < 7 indicating acidity, > 7 basicity, and = 7 neutrality (pure water, where [H⁺] = [OH⁻] = 10⁻⁷ M). The complementary pOH = -log₁₀[OH⁻] relates via the ion product of water, K_w = [H⁺][OH⁻] = 10⁻¹⁴, so + pOH = 14. For example, 0.1 M HCl has ≈ 1 (highly acidic), while 0.1 M NH₃ has ≈ 11 (basic). This scale facilitates precise comparisons without handling extreme concentration values. Buffers are solutions that maintain stable pH against added acid or base, typically consisting of a weak acid and its conjugate base (or weak base and conjugate acid). They operate via the , where the presence of a common ion (e.g., A⁻ from the salt) suppresses the dissociation of HA, shifting the equilibrium per Le Châtelier's principle. The pH of such a buffer is approximated by the Henderson-Hasselbalch equation, derived by Lawrence J. Henderson in 1908 and reformulated in logarithmic form by Karl A. Hasselbalch in 1916: pH=pKa+log10([A][HA])\text{pH} = \text{p}K_a + \log_{10}\left(\frac{[A^-]}{[HA]}\right) For an acetate buffer (acetic acid and sodium acetate), pH ≈ 4.76 when [CH₃COO⁻] = [CH₃COOH], near pK_a = 4.76. This equation assumes dilute solutions and negligible H⁺/OH⁻ from water. Buffers are essential in biological systems, like blood (pH ≈ 7.4 via H₂CO₃/HCO₃⁻). Acid-base titrations determine the concentration of an unknown acid or base by adding a titrant of known concentration until neutralization. The equivalence point occurs when the moles of acid equal moles of base added, marked by a sharp pH change; for strong acid-strong base titrations (e.g., HCl with NaOH), pH jumps from ≈3 to ≈11 around pH 7. Weak acid-strong base titrations (e.g., CH₃COOH with NaOH) have equivalence at pH > 7 due to hydrolysis of the conjugate base. Acid-base indicators, weak organic acids or bases, change color near their pK_a (e.g., phenolphthalein, colorless to pink at pH 8–10, suitable for strong base titrations). The endpoint is visually approximated to the equivalence point for accurate molarity calculations.

Redox Reactions

Redox reactions, also known as oxidation-reduction reactions, are chemical processes involving the transfer of electrons between species, where one substance is oxidized and another is reduced simultaneously. These reactions are fundamental to many natural and industrial processes, powering everything from biological respiration to devices. In a reaction, oxidation refers to the loss of electrons by a , resulting in an increase in its , while reduction involves the gain of electrons, leading to a decrease in . The substance undergoing oxidation acts as the , donating electrons to another , whereas the substance undergoing reduction serves as the , accepting those electrons. For instance, in the reaction between and copper(II) ions, is oxidized to Zn²⁺ and acts as the , while Cu²⁺ is reduced to metal and functions as the . Balancing equations is typically achieved by separating the reaction into oxidation and reduction half-reactions, then ensuring and charge. In acidic media, the steps include: writing the unbalanced half-reactions, balancing all elements except and oxygen, adding H₂O to balance oxygen, adding H⁺ to balance , and finally adding electrons to balance charge; the half-reactions are then multiplied to equalize electrons and combined. For basic media, the acidic method is followed first, then OH⁻ ions are added to both sides to neutralize H⁺, producing H₂O on the appropriate side. Consider the reaction of (MnO₄⁻) with iron(II) in acidic solution: Oxidation: \ceFe2+>Fe3++eReduction: \ceMnO4+8H++5e>Mn2++4H2O\begin{align*} &\text{Oxidation: } \ce{Fe^2+ -> Fe^3+ + e^-} \\ &\text{Reduction: } \ce{MnO4^- + 8H^+ + 5e^- -> Mn^2+ + 4H2O} \end{align*} Multiplying the oxidation by 5 and combining yields the balanced equation: \ce5Fe2++MnO4+8H+>5Fe3++Mn2++4H2O\ce{5Fe^2+ + MnO4^- + 8H^+ -> 5Fe^3+ + Mn^2+ + 4H2O}. The tendency of a species to undergo reduction is quantified by its standard , EE^\circ, measured in volts relative to the (SHE) under standard conditions (1 M concentrations, 1 atm pressure, 25°C). A more positive EE^\circ indicates a stronger . The potential for a redox reaction, EcellE^\circ_\text{cell}, determines spontaneity: Ecell=EcathodeEanodeE^\circ_\text{cell} = E^\circ_\text{cathode} - E^\circ_\text{anode}, where a positive value signifies a spontaneous reaction. For the zinc-copper reaction, E(\ceCu2+/Cu)=+0.34E^\circ(\ce{Cu^2+/Cu}) = +0.34 V and E(\ceZn2+/Zn)=0.76E^\circ(\ce{Zn^2+/Zn}) = -0.76 V, so Ecell=0.34(0.76)=1.10E^\circ_\text{cell} = 0.34 - (-0.76) = 1.10 V, confirming spontaneity. Electrochemistry harnesses reactions in electrochemical cells. In voltaic (galvanic) cells, spontaneous processes generate , with oxidation at the and reduction at the , separated by a to maintain charge balance. Conversely, electrolytic cells use external to drive non-spontaneous reactions, such as in . Faraday's laws govern : the mass mm of a substance altered is proportional to the charge QQ passed (m=QnFMm = \frac{Q}{nF} \cdot M), where nn is electrons per mole, FF is Faraday's constant (96,485 C/mol), and MM is ; a second law states the masses of substances produced by the same charge are proportional to their equivalent weights. Corrosion exemplifies undesirable redox processes, particularly the rusting of iron, where iron acts as the anode (\ceFe>Fe2++2e\ce{Fe -> Fe^2+ + 2e^-}) and oxygen reduction occurs at the cathode (\ceO2+2H2O+4e>4OH\ce{O2 + 2H2O + 4e^- -> 4OH^-}), forming Fe(OH)₃ (rust) in the presence of water and oxygen. This electrochemical deterioration can be mitigated by protective coatings or cathodic protection. Redox reactions power practical applications like batteries and fuel cells. The , a classic voltaic cell, uses and electrodes in their respective solutions, producing 1.10 V via \ceZn+Cu2+>Zn2++Cu\ce{Zn + Cu^2+ -> Zn^2+ + Cu}, serving as an early model for rechargeable batteries. Fuel cells, such as hydrogen-oxygen types, continuously supply reactants for sustained reactions (\ce2H2+O2>2H2O\ce{2H2 + O2 -> 2H2O}), achieving efficiencies over 50% and enabling clean energy conversion without combustion byproducts.

Fundamental Chemical Laws

The law of , formulated by in 1789, states that in a , the total of reactants in a equals the total of products, implying that matter is neither created nor destroyed during chemical processes. This principle, articulated in Lavoisier's seminal work Traité Élémentaire de Chimie, provided a quantitative foundation for chemistry by emphasizing precise measurements and overturning earlier phlogiston theories. Lavoisier's experiments, such as those involving and , demonstrated this law through careful weighing, establishing as a core tenet of quantitative analysis. Building on this, Joseph Louis Proust proposed the in 1794, asserting that a always contains its constituent elements in fixed mass ratios, regardless of the source or preparation method. Proust's investigations into metal oxides and sulfides, published in the Annales de Chimie, showed, for instance, that cupric oxide (CuO) consistently comprised copper and oxygen in an approximately 4:1 mass ratio. This law highlighted the constancy of composition in compounds, supporting the idea of discrete chemical entities. Complementing Proust's work, introduced the in 1803, which states that when two elements form more than one compound, the mass ratios of one element that combine with a fixed mass of the other are small whole numbers. Dalton's analysis of oxides of carbon illustrated this principle: 12 g of carbon combines with 16 g of oxygen in and 32 g of oxygen in , so the masses of oxygen are in the ratio 1:2. The , also known as the , was enunciated by Jeremias Benjamin Richter in , positing that if two elements each combine separately with a third element, the mass ratios in which they combine with the third are the same as, or simple multiples of, the ratio in which they combine with each other. Richter's work on salts and acids, detailed in his Anfangsgründe der Stöchiometrie, enabled the construction of tables, where, for example, the equivalents of and oxygen relative to mirrored their direct combination ratio. This law laid groundwork for understanding chemical equivalence and was later refined through concepts like Avogadro's hypothesis. Joseph Louis Gay-Lussac's law of combining volumes, published in 1808, observed that gases reacting at constant and combine in volumes that are simple ratios, such as two volumes of with one volume of oxygen forming . In response, proposed his hypothesis in 1811, suggesting that equal volumes of different gases at the same and contain equal numbers of molecules, distinguishing between atoms and molecules to reconcile Gay-Lussac's findings with atomic theory. Avogadro's essay in the Journal de Physique explained volume ratios through molecular counts, for instance, attributing the 2:1 hydrogen-oxygen ratio in to diatomic molecules. Dmitri Mendeleev formulated the periodic law in 1869, stating that the properties of elements vary periodically with their atomic weights, leading to the arrangement of elements in a table that predicted undiscovered species. Presented to the Russian Chemical Society, Mendeleev's table grouped elements by similar properties, such as , sodium, and , and forecasted properties for elements like , confirmed shortly after. This law encapsulated recurring chemical behaviors, reinforcing the atomic nature of elements. Collectively, these laws provided empirical evidence for John Dalton's atomic theory, proposed in 1808, by demonstrating consistent and volume relationships that implied indivisible atoms combining in fixed ratios. Lavoisier's conservation and Proust's definite proportions suggested atoms as the stable units preserving composition, while Dalton's multiple proportions and Richter's reciprocity indicated discrete atomic combinations. Gay-Lussac's volumes and Avogadro's resolved gaseous discrepancies by introducing molecular aggregates, and Mendeleev's periodicity extended atomic theory to systematic elemental organization. These principles collectively shifted chemistry toward a quantitative, atomistic framework, enabling modern and structural understanding.

Historical Development

Ancient and Pre-Modern Chemistry

Ancient civilizations laid the foundational practices that would evolve into chemistry, with early emerging prominently in around 3000 BCE, where artisans smelted and later for tools, weapons, and decorative items using basic furnaces and crucibles. Egyptian metalworkers also employed leafing and alloying techniques, such as combining with silver to create , demonstrating an empirical understanding of material properties without theoretical frameworks. In parallel, Greek philosophers in the 5th century BCE proposed conceptual models for matter; of Acragas introduced the theory of four elements—earth, air, fire, and water—as the indivisible (rhizomata) from which all substances arise through mixing and separation, influenced by cycles of Love and Strife. This elemental scheme, later refined by , shifted focus from practical crafts to philosophical speculation on the nature of change and composition. Alchemy, emerging around the CE in Hellenistic and spreading across cultures, pursued the transmutation of base metals into , the creation of elixirs for , and the purification of the through material operations, blending proto-scientific experimentation with mystical and philosophical goals. In the , (c. 721–815 CE), often called the father of chemistry, advanced alchemical methodology by systematizing processes using the , which separated volatile substances like alcohol and acids, and documented over 500 treatises on chemical reactions and apparatus. His emphasis on precise measurements and classification of substances marked a shift toward empirical rigor, though still tied to transmutational aims. By the , European alchemist (1493–1541) pioneered iatrochemistry, integrating alchemy with medicine to treat diseases using chemical remedies like mercury compounds and , rejecting Galenic humoral theory in favor of mineral-based therapeutics derived from observation. Non-Western traditions contributed significantly to alchemical knowledge; in , , a branch of dating back to ancient texts like the (circa 300 BCE), focused on elixirs () for longevity and later incorporated metallic preparations (dhatu vidya) in medieval alchemical works like the Rasaratnakara (12th–13th century CE) describing mercurial processes and herbal distillations for rejuvenation. In , Taoist alchemists during the (618–907 CE) experimented with elixirs of immortality, inadvertently inventing around the 9th century through mixing saltpeter, , and in pursuit of incendiary or medicinal compounds, which evolved into military applications by the . These practices refined early techniques, including for purifying essences and for isolating salts, as alchemists heated, filtered, and evaporated solutions to obtain pure forms, laying groundwork for reproducible chemical operations. By the , alchemical thought culminated in the , proposed by Johann Joachim Becher (1635–1682) and elaborated by (1659–1734), positing phlogiston as a fire-like principle released during and —a process thought to involve the loss of this substance, though it required adjustments like negative weight to explain weight gains in metal calcination. However, flaws emerged: the theory failed to account for weight increases in without invoking for phlogiston, and experiments showed calxes (metal oxides) heavier than original metals, undermining its explanatory power. This period marked the transition to modern chemistry, as growing skepticism toward mystical transmutation and reliance on quantitative experiments—championed by figures like —rejected alchemical esotericism in favor of mechanistic and observational paradigms, paving the way for systematic science.

Birth of Modern Chemistry

The birth of modern chemistry in the marked a pivotal shift from speculative and the dominant to an empirical, quantitative science grounded in experimentation and precise measurement. The , which posited an inflammable released during , began to crumble under rigorous testing, particularly through the work of , who demonstrated that involved the addition of a substance rather than its removal. Lavoisier's experiments in the 1770s showed that metals gained weight when burned, contradicting phlogiston's predictions and paving the way for oxygen-based explanations of chemical reactions. A cornerstone of this revolution was the discovery of oxygen, isolated independently by in 1772 and in 1774, though Lavoisier was the first to recognize its role in and respiration, naming it "oxygen" in 1777 for its acid-forming properties. Building on these findings, Lavoisier established the law of in 1789, proving through sealed-vessel experiments that the total mass of reactants equals that of products in chemical reactions, thus rejecting notions of matter creation or destruction. In 1787, Lavoisier collaborated with Guyton de Morveau, Claude-Louis Berthollet, and Antoine-François de Fourcroy to introduce a systematic in Méthode de Nomenclature Chimique, replacing vague alchemical terms with names reflecting composition, such as "" for metallic compounds with oxygen. These reforms emphasized clarity and empirical basis, transforming chemistry into a standardized . Marie-Anne Pierrette Paulze, Lavoisier's wife, played a crucial role by translating foreign scientific texts, illustrating experimental apparatus in their publications, and assisting in laboratory work, including precise engravings for Traité Élémentaire de Chimie (1789). Extending these foundations, revived and quantified ancient atomic ideas in his 1808 publication A New System of Chemical Philosophy, proposing that all matter consists of indivisible atoms of fixed mass unique to each element, which combine in simple whole-number ratios to form compounds, providing a mechanistic explanation for chemical laws like definite proportions. In 1811, advanced this framework with his hypothesis that equal volumes of gases at the same and contain equal numbers of molecules, distinguishing between atoms of elements and molecules of compounds or diatomic gases like . further solidified atomic theory in the 1810s through experiments, developing the electrochemical theory that classified elements as electropositive or electronegative based on their behavior in electrolytic cells, and introducing the modern system of chemical symbols—abbreviated Latin or element names, such as "O" for oxygen—facilitating stoichiometric calculations. This era also saw the rise of , the quantitative study of reactant-product proportions, pioneered by Jeremias Benjamin Richter in the late and refined through Lavoisier and Dalton's work, enabling chemists to predict reaction outcomes based on atomic weights and ratios rather than empirical trial-and-error. By the early , these developments had firmly established chemistry as a modern discipline, emphasizing verifiable experimentation, atomic realism, and mathematical precision over mystical or qualitative interpretations.

Major Milestones and Figures

In the late 19th century, played a pivotal role in establishing accurate atomic weights by reviving Avogadro's hypothesis in his 1858 pamphlet "Sunto di un corso di filosofia chimica," which clarified the distinction between atomic and molecular weights and influenced the 1860 Karlsruhe Congress. This foundation enabled to formulate the periodic table in 1869, arranging elements by increasing atomic weight and predicting properties of undiscovered elements like , , and , which were later confirmed. Mendeleev's table, published in the Russian Journal of Chemistry, revealed periodicity in chemical properties and left gaps for missing elements, revolutionizing element classification. The discovery of radioactivity marked another breakthrough, with identifying spontaneous emissions from salts in 1896 through experiments, initially mistaken for but proven as a new atomic phenomenon. Building on this, Pierre and Marie Curie isolated and from pitchblende in 1898, demonstrating their intense radioactivity and introducing the term "radioactive" to describe elements that emit rays spontaneously. Their work, detailed in Comptes Rendus reports, laid the groundwork for and earned the 1903 shared with Becquerel. The early 20th century saw quantum theory transform chemical understanding, starting with Niels Bohr's 1913 model of the , which incorporated quantized energy levels to explain spectral lines, bridging classical and . This was advanced by Erwin Schrödinger's 1926 , which described electrons as probability waves and enabled quantum mechanical calculations of molecular structures, fundamentally altering chemical bonding theories. extended these ideas in the 1930s, applying to valence bonds in his seminal 1939 book The Nature of the Chemical Bond, introducing concepts like hybridization and that explained molecular geometries and reactivity. Polymer chemistry emerged as a major field with Hermann Staudinger's proposition of macromolecules, challenging the association theory by demonstrating that polymers like rubber consist of long chains of repeating units, a view vindicated by his . built on this at , synthesizing in 1935 through polycondensation of and , creating the first fully with high tensile strength and versatility for industrial applications. In biochemistry, and proposed the double-helix structure of in their Nature paper, integrating X-ray data from to reveal base-pairing and hydrogen bonding that underpin genetic replication. Recent advancements highlight chemistry's role in biotechnology, as seen in the 2010s development of CRISPR-Cas9, where chemical engineering of guide RNAs and nucleases enabled precise , earning and the 2020 for this molecular tool. Complementing this, —pioneered by K. Barry Sharpless and Morten Meldal in the early for efficient copper-catalyzed azide-alkyne cycloadditions, and expanded by Carolyn Bertozzi's bioorthogonal variants—facilitated targeted reactions in living cells, recognized by the 2022 . Continuing into the 21st century, the 2023 was awarded to Moungi G. Bawendi, , and Alexei Ekimov for the discovery and synthesis of quantum dots. In 2024, David Baker, , and John Jumper received the prize for computational and using AI. The 2025 went to Susumu Kitagawa, Richard Robson, and for the development of metal-organic frameworks (MOFs), enabling new materials for storage and catalysis.

Applications and Fields

Subdisciplines of Chemistry

Chemistry encompasses several major subdisciplines, each specializing in distinct aspects of and its transformations, ranging from molecular structures to nuclear processes. These branches employ unique methodologies to investigate chemical systems, contributing to foundational in the field. centers on the scientific study of carbon-containing compounds, encompassing their structure, properties, composition, reactions, and synthesis. This subdiscipline emphasizes the preparation of complex molecules through controlled reactions, often involving the manipulation of functional groups—specific arrangements of atoms within molecules that determine chemical reactivity, such as alcohols (-OH), aldehydes (-CHO), and carboxylic acids (-COOH). Functional groups serve as key molecular descriptors, enabling chemists to predict and design reaction pathways for applications in pharmaceuticals and materials. Seminal work in , like the total synthesis of complex natural products, highlights the field's reliance on stereoselective methods and catalytic processes to achieve high yields and selectivity. Inorganic chemistry investigates the properties, synthesis, and behavior of compounds involving non-carbon elements, including metals, minerals, and organometallic . It focuses on main-group elements, transition metals, and coordination compounds, where central metal atoms or ions are surrounded by ligands to form stable complexes with defined geometries, such as octahedral or tetrahedral structures. Coordination chemistry explores bonding theories like and to explain electronic properties and reactivity, with high-impact contributions including the development of catalysts for industrial processes. This branch also examines solid-state materials and bioinorganic systems, drawing on experimental techniques like for structural analysis. Physical chemistry applies principles from physics to understand chemical systems at the molecular and atomic levels, integrating , kinetics, and . Thermodynamics provides frameworks for predicting equilibrium and changes in reactions, as described by laws governing , , and . Quantum chemistry employs computational methods, such as , to model electronic structures and molecular orbitals, enabling predictions of properties and reaction mechanisms. This subdiscipline bridges theory and experiment through techniques like and , with influential works including the application of quantum principles to explain bond formation and molecular vibrations. Analytical chemistry is dedicated to the qualitative and quantitative determination of the composition and structure of matter, utilizing precise measurement techniques to obtain reliable chemical information. Core methods include , which identifies substances based on their interaction with —such as for functional group detection or for molecular connectivity—and , which separates mixtures by differential partitioning between mobile and stationary phases, as in for volatile compounds. These tools enable trace-level analysis with high sensitivity, exemplified by coupled with chromatography for identifying complex mixtures. The field's emphasis on validation and accuracy stems from standards set by organizations like the International Union of Pure and Applied Chemistry, ensuring reproducible results in diverse samples. Biochemistry examines the chemical processes within and relating to living organisms, integrating principles of chemistry and to elucidate molecular mechanisms in cells. It focuses on biomolecules like proteins, nucleic acids, and carbohydrates, with enzymes—biological catalysts typically proteins—playing a central role in accelerating reactions through active sites that lower activation energies. Metabolic pathways, such as and the , represent interconnected sequences of enzyme-mediated reactions that convert nutrients into energy and building blocks, regulated by factors like allosteric effectors. High-impact research includes the elucidation of via Michaelis-Menten models, which quantify substrate affinity and maximum reaction rates, informing studies on metabolic disorders. Nuclear chemistry, a specialized subdiscipline, studies the chemical aspects of atomic nuclei, including , nuclear reactions, and the behavior of radionuclides. It investigates radioactivity through processes like , and gamma emission, where unstable nuclei transform to achieve stability, as quantified by measurements. Key phenomena include , the splitting of heavy nuclei like to release energy and neutrons, and fusion, the merging of light nuclei such as isotopes to form , powering stars and experimental reactors. This field applies chemical separation techniques to isolate isotopes and employs for , with foundational contributions from the discovery of artificial radioactivity by Irène and Frédéric Joliot-Curie in 1934.

Industrial and Applied Chemistry

Industrial and applied chemistry encompasses the large-scale production of chemicals and materials using chemical principles, driving advancements in , , and consumer products. This field transforms fundamental reactions into practical processes, enabling the synthesis of everyday items from fuels to medicines while addressing efficiency, cost, and environmental impacts. Key innovations have revolutionized global industries, from the derivation of polymers from to the development of life-saving drugs. In the petrochemical sector, thermal and catalytic cracking processes break down long-chain hydrocarbons in crude oil or into shorter, more versatile molecules such as and , which serve as building blocks for numerous products. These feedstocks undergo reactions to produce plastics like , first achieved through Ziegler-Natta in the , enabling the of durable, lightweight materials used in , , and containers. This process has scaled to produce billions of tons annually, underscoring chemistry's role in modern economies. Pharmaceutical chemistry applies synthetic to design and manufacture drugs, with aspirin (acetylsalicylic acid) marking a milestone when synthesized by at in 1899, providing a safer alternative to natural salicylates for pain relief and fever reduction. The discovery and industrial-scale production of antibiotics, beginning with penicillin isolated by in 1928 and scaled up by and in the 1940s, revolutionized by combating bacterial infections on a global scale. These developments rely on precise control of reaction conditions to ensure purity and efficacy in therapeutic applications. Fertilizer production exemplifies applied chemistry's impact on , with the Haber-Bosch process—developed by and in the 1910s—enabling the fixation of atmospheric into via high-pressure synthesis with iron catalysts, supporting food production for billions. This method, operational since 1913, accounts for over 80% of global output, though it consumes significant energy. Emerging alternatives, such as electrochemical reduction using renewable electricity and catalysts like those based on , aim to reduce carbon emissions and dependence on fossil fuels. Materials chemistry drives innovations in electronics and nanotechnology, where silicon doping—introducing impurities like phosphorus or boron into pure silicon lattices—creates semiconductors with controlled electrical properties, foundational to technology since the 1950s. The discovery of fullerenes, (C60) isolated by Harold Kroto, , and in 1985 using laser vaporization of , opened avenues for carbon-based in and superconductors. Environmental chemistry applies catalytic processes to mitigate pollution, such as three-way catalytic converters in vehicles, which use and to convert exhaust gases like and nitrogen oxides into less harmful substances, reducing urban since their widespread adoption in the 1970s. These systems achieve over 90% efficiency in emissions control under optimal conditions. Safety and regulations in industrial chemistry ensure worker protection and public health, with the (OSHA) establishing standards like the Hazard Communication Standard in 1983, requiring labeling and safety data sheets for chemicals. Globally, the Globally Harmonized System (GHS) of classification and labeling, adopted by the in 2003, standardizes hazard symbols like flames for flammability and skulls for toxicity, facilitating and .

Interdisciplinary Connections

Chemistry's interdisciplinary connections span multiple scientific domains, integrating chemical principles with biological, physical, and environmental processes to address complex challenges in health, energy, and . These interfaces leverage molecular-level understanding to drive innovations, such as designing therapeutics through or modeling atmospheric reactions in . By combining experimental synthesis with computational tools, chemistry facilitates breakthroughs in fields like and , where atomic-scale manipulations yield novel properties. This collaborative nature has accelerated discoveries, from interstellar detection in to AI-enhanced reaction predictions in . In chemical biology, chemistry intersects with life sciences to study biomolecules and develop drugs, focusing on how small molecules interact with biological targets to modulate cellular functions. This field employs to probe protein structures and pathways, enabling the identification of drug candidates that bind specifically to enzymes or receptors. For instance, chemical biology techniques have revealed mechanisms for targeting disease-related proteins, such as kinases in cancer pathways, by using synthetic probes to map binding sites and allosteric effects. Seminal work in this area includes the development of covalent inhibitors that irreversibly bind therapeutic targets, advancing precision medicine. in chemical biology often integrates structure-activity relationships, where chemists optimize lead compounds for potency and selectivity, as demonstrated in of biomolecule libraries to combat antimicrobial resistance. Chemistry's role in materials science emphasizes the design of polymers and superconductors, where molecular architecture dictates macroscopic properties like conductivity and mechanical strength. Polymers, such as conjugated polyacetylenes and polythiophenes, are synthesized to form and sensors, with their electronic delocalization enabling applications in . These materials bridge and , allowing tunable bandgaps through side-chain modifications. In superconductors, chemical doping of cuprates or achieves zero-resistance states at higher temperatures, with recent discoveries under highlighting chemistry's contribution to . For example, systems have demonstrated at approximately 250 K (−23 °C), informed by computational screening of elemental compositions. This integration has led to durable, lightweight materials for and transmission. Environmental science draws on chemistry to analyze dynamics, particularly CO2 cycles and , elucidating how chemical reactions influence global systems. In chemistry, the involves photochemical and biogeochemical processes that sequester or release CO2, with overwhelming natural sinks like oceanic absorption and . Anthropogenic emissions have increased atmospheric CO2 concentrations by 52% since pre-industrial levels (from ~280 ppm to 425.7 ppm as of 2025), driving and through carbonate equilibrium shifts. within this context examines how stressors exacerbate contaminant mobility; elevated temperatures enhance the volatility and bioavailability of pollutants like and persistent organics, amplifying in ecosystems. For instance, warming waters increase formation in aquatic food chains, posing risks to and human health. These insights guide mitigation strategies, such as carbon capture via chemical sorbents. Computational chemistry provides tools for molecular modeling and (DFT), revolutionizing predictions of chemical behavior across scales. Molecular modeling simulates atomic interactions using and , allowing visualization of reaction pathways and without physical experiments. DFT, formalized in the through the Hohenberg-Kohn theorems, posits that the ground-state uniquely determines all molecular properties, enabling efficient calculations of energies and geometries for large systems. The Kohn-Sham formulation reformulates the into single-particle equations, making DFT practical for studying and material defects. Widely adopted since the 1990s, DFT has predicted properties of thousands of compounds, underpinning drug screening and nanomaterial design with accuracies rivaling experiments for many systems. Astrochemistry merges chemistry with to explore interstellar molecules, revealing the origins of cosmic complexity in diffuse clouds and star-forming regions. As of September 2025, 338 molecules, including hydrocarbons, alcohols, and precursors, have been detected via radio , with H3+ ions initiating ion-molecule reactions that build complexity from atomic and CO. Key discoveries, such as in hot cores, suggest prebiotic chemistry in space, where UV radiation and cosmic rays drive radical formations. These findings, from facilities like the Atacama Large Millimeter/submillimeter Array, inform models of by tracing from to protoplanetary disks. In nanotechnology, chemistry enables the synthesis of quantum dots and self-assembled structures, harnessing size-dependent quantum effects for optoelectronics and sensing. Quantum dots, semiconductor nanocrystals like CdSe or InP, exhibit tunable fluorescence due to confinement, with emission wavelengths shifting from UV to near-IR based on 2-10 nm diameters. Chemical routes, such as colloidal synthesis, control monodispersity for applications in LEDs and bioimaging. Self-assembly directs nanoparticles into ordered arrays via ligand interactions or electrostatic forces, forming photonic crystals or metamaterials with emergent properties. For example, evaporative-driven assembly of quantum dots yields dense films for high-efficiency displays, while DNA-templated methods create programmable nanostructures. These advances stem from surface chemistry principles, optimizing stability and functionality. Emerging connections in and AI-driven reaction prediction are transforming chemical innovation in the . applies chemical synthesis to engineer biological systems, redesigning metabolic pathways for production or novel therapeutics using standardized DNA parts. This field integrates with genetic circuits, enabling cell-free platforms for scalable cascades. Concurrently, AI models predict reaction outcomes by learning from vast datasets, outperforming traditional methods in retrosynthesis planning. Generative AI, such as flow-based networks, simulates reaction flows with physical realism, forecasting yields for unseen substrates and accelerating . These tools, trained on millions of reactions, reduce experimental iterations by 50-70% in some cases, fostering sustainable synthesis.

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