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Physics and Star Wars
The interstellar space opera epic Star Wars uses science and technology in its settings and storylines. The series has showcased many technological concepts, both in the movies and in the expanded universe of novels, comics and other forms of media. The Star Wars movies' primary objective is to build upon drama, philosophy, political science and less on scientific knowledge. Many of the on-screen technologies created or borrowed for the Star Wars universe were used mainly as plot devices.
The iconic status that Star Wars has gained in popular culture and science fiction allows it to be used as an accessible introduction to real scientific concepts. Many of the features or technologies used in the Star Wars universe are not yet considered possible. Despite this, their concepts are still probable.
In the past, scientists thought that planets would be unlikely to form around binary stars. However, recent simulations indicate that planets are just as likely to form around binary star systems as single-star systems. Of the 3457 exoplanets currently known, 146 actually orbit binary star systems (and 39 orbit multiple star systems with three or more stars). Specifically, they orbit what are known as "wide" binary star systems where the two stars are fairly far apart (several AU). Tatooine appears to be of the other type — a "close" binary, where the stars are very close, and the planets orbit their common center of mass.
The first observationally confirmed binary — Kepler-16b — is a close binary. Exoplanet researchers' simulations indicate that planets form frequently around close binaries, though gravitational effects from the dual star system tend to make them very difficult to find with current Doppler and transit methods of planetary searches. In studies looking for dusty disks—where planet formation is likely—around binary stars, such disks were found in wide or narrow binaries, or those whose stars are more than 50 or less than 3 AU apart, respectively. Intermediate binaries, or those with between 3 and 50 AU between them, had no dusty disks. In 2011 it was reported by The Guardian that NASA space telescope Kepler had discovered a planet, named Kepler-16b, with twin suns as seen in the Star Wars films.
Certified astrophysicist and Star Wars fan Jeanne Cavelos explains that scientists have been skeptical about the likelihood of binary star systems such as Tatooine since the gravity of one star may prevent planets from developing around the other. Two stars of different masses orbiting one another would cause gravity fields to shift, causing potential instabilities in the orbits of any planets in their system.
According to her, even planets in more stable orbits of a binary star system would suffer other kinds of problems such as climatic problems. As an example, a planet in a binary star system orbiting the larger star would be drawn closer to its gravitational field, causing the planet to endure heat of great temperatures during this period. As the planet passes its larger star and reaches the orbit of its smaller star, the gravitational field of that star would give the planet more distance from it. The distance (perhaps along with the smaller solar projection of the star) would send the planet into extreme frigid temperatures.
According to Cavelos, astronomers hypothesize at least two possible solutions to these problems exist and that even life supporting binary star systems could exist. One scenario could be two stars billions of kilometres apart. A planet or planets would be able to orbit one star while at minimum influence of the other. A star known as Proxima Centauri, or Alpha Centauri C, is about one trillion kilometres away from its sister stars, Alpha Centauri A and B. Also according to Cavelos, astronomers believe that Proxima Centauri could have planets of its own. If so, they would be minimally influenced by Proxima Centauri's sister stars due to the vast distance between them and these sister stars. Assuming the existence of planets around Proxima Centauri, from these planets the sister suns would appear as bright stars in the sky.
Another scenario would be two stars that would be closer to one another at a distance of only a few million kilometres. A planet orbiting far enough away would be affected by their gravitational fields almost as if there were one. If the distance between the two stars was a small fraction of the distance between them and the planet, it would be stable for the planet. Dawn and dusk would occur on such a planet as they would on Tatooine.
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Physics and Star Wars
The interstellar space opera epic Star Wars uses science and technology in its settings and storylines. The series has showcased many technological concepts, both in the movies and in the expanded universe of novels, comics and other forms of media. The Star Wars movies' primary objective is to build upon drama, philosophy, political science and less on scientific knowledge. Many of the on-screen technologies created or borrowed for the Star Wars universe were used mainly as plot devices.
The iconic status that Star Wars has gained in popular culture and science fiction allows it to be used as an accessible introduction to real scientific concepts. Many of the features or technologies used in the Star Wars universe are not yet considered possible. Despite this, their concepts are still probable.
In the past, scientists thought that planets would be unlikely to form around binary stars. However, recent simulations indicate that planets are just as likely to form around binary star systems as single-star systems. Of the 3457 exoplanets currently known, 146 actually orbit binary star systems (and 39 orbit multiple star systems with three or more stars). Specifically, they orbit what are known as "wide" binary star systems where the two stars are fairly far apart (several AU). Tatooine appears to be of the other type — a "close" binary, where the stars are very close, and the planets orbit their common center of mass.
The first observationally confirmed binary — Kepler-16b — is a close binary. Exoplanet researchers' simulations indicate that planets form frequently around close binaries, though gravitational effects from the dual star system tend to make them very difficult to find with current Doppler and transit methods of planetary searches. In studies looking for dusty disks—where planet formation is likely—around binary stars, such disks were found in wide or narrow binaries, or those whose stars are more than 50 or less than 3 AU apart, respectively. Intermediate binaries, or those with between 3 and 50 AU between them, had no dusty disks. In 2011 it was reported by The Guardian that NASA space telescope Kepler had discovered a planet, named Kepler-16b, with twin suns as seen in the Star Wars films.
Certified astrophysicist and Star Wars fan Jeanne Cavelos explains that scientists have been skeptical about the likelihood of binary star systems such as Tatooine since the gravity of one star may prevent planets from developing around the other. Two stars of different masses orbiting one another would cause gravity fields to shift, causing potential instabilities in the orbits of any planets in their system.
According to her, even planets in more stable orbits of a binary star system would suffer other kinds of problems such as climatic problems. As an example, a planet in a binary star system orbiting the larger star would be drawn closer to its gravitational field, causing the planet to endure heat of great temperatures during this period. As the planet passes its larger star and reaches the orbit of its smaller star, the gravitational field of that star would give the planet more distance from it. The distance (perhaps along with the smaller solar projection of the star) would send the planet into extreme frigid temperatures.
According to Cavelos, astronomers hypothesize at least two possible solutions to these problems exist and that even life supporting binary star systems could exist. One scenario could be two stars billions of kilometres apart. A planet or planets would be able to orbit one star while at minimum influence of the other. A star known as Proxima Centauri, or Alpha Centauri C, is about one trillion kilometres away from its sister stars, Alpha Centauri A and B. Also according to Cavelos, astronomers believe that Proxima Centauri could have planets of its own. If so, they would be minimally influenced by Proxima Centauri's sister stars due to the vast distance between them and these sister stars. Assuming the existence of planets around Proxima Centauri, from these planets the sister suns would appear as bright stars in the sky.
Another scenario would be two stars that would be closer to one another at a distance of only a few million kilometres. A planet orbiting far enough away would be affected by their gravitational fields almost as if there were one. If the distance between the two stars was a small fraction of the distance between them and the planet, it would be stable for the planet. Dawn and dusk would occur on such a planet as they would on Tatooine.