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Project Longshot
Project Longshot
from Wikipedia
  1. Initial configuration
  2. Configuration at 33 years
  3. Configuration at 67 years
  4. Configuration at 100 years

Project Longshot was a conceptual interstellar spacecraft design. It would have been an uncrewed starship (about 400 tonnes), intended to fly to and enter orbit around Alpha Centauri B powered by nuclear pulse propulsion.[1]

History

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Developed by the US Naval Academy and NASA, from 1987 to 1988, Longshot was designed to be built at Space Station Freedom, the precursor to the existing International Space Station. Similar to Project Daedalus, Longshot was designed with existing technology in mind, although some development would have been required; for example, the Project Longshot concept assumes "a three-order-of-magnitude leap over current propulsion technology".[1]

Mission

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Unlike Daedalus, which used an open-cycle fusion engine, Longshot would use a long-lived nuclear fission reactor for power. Initially generating 300 kilowatts, the reactor would power a number of lasers in the engine that would be used to ignite inertial confinement fusion similar to that in Daedalus. The main design difference is that Daedalus also relied on the fusion reaction to power the ship, whereas in the Longshot design the internal reactor would provide this power.[1]

The reactor would also be used to power a laser for communications back to Earth, with a maximum power of 250 kW. For most of the journey, this would be used at a much lower power for sending data about the interstellar medium; but during the flyby, the main engine section would be discarded and the entire power capacity dedicated to communications at about 1 kilobit per second.

Longshot would have a mass of 396 tonnes (873,000 lb) at the start of the mission including 264 tonnes of helium-3/deuterium pellet fuel/propellant. The active mission payload, which includes the fission reactor but not the discarded main propulsion section, would have a mass of around 30 tonnes.

A difference in the mission architecture between Longshot and the Daedalus study is that Longshot would go into orbit about the target star, while the higher-speed Daedalus would do a one shot fly-by lasting a comparatively short time.

A travel to Alpha Centauri with a Longshot spacecraft would take about one century.

See also

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References

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Bibliography

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Revisions and contributorsEdit on WikipediaRead on Wikipedia
from Grokipedia
Project Longshot was a conceptual design study for an unmanned developed by midshipmen at the U.S. Naval Academy under the /USRA University Advanced Design Program in 1987-1988, aimed at sending a to the star system—the nearest to the Sun—using a pulsed system to enable a roughly 100-year transit time. The primary objectives of the mission included gathering data on the properties of the , characterizing the three-star Alpha Centauri system (Alpha Centauri A, B, and ), and performing high-precision to refine measurements of stellar distances. The spacecraft design featured a total mass of approximately 396 metric tons, powered by a 300-kilowatt fission reactor to support onboard systems, including a 250-kilowatt communication array operating at a 0.532-micron for data transmission rates up to 1,000 bits per second over interstellar distances. At the heart of the propulsion system was an innovative pulsed fusion microexplosion drive, utilizing and as fuel to achieve a of 1,000,000 seconds—far exceeding conventional chemical or even nuclear thermal rockets—by detonating tiny fusion pellets to generate . The mission profile envisioned assembly of the in using infrastructure, followed by an initial boost from chemical upper stages to escape the Solar System, after which the fusion drive would accelerate the craft to a cruise velocity of about 14,700 km/s (5% of lightspeed) for the long-duration flight. Upon arrival, the would enter around Alpha Centauri B to conduct extended observations. Key challenges highlighted in the study included the need for fuel sourcing (potentially from Jupiter's atmosphere or lunar ), ensuring 100-year operational reliability through advanced and radiation-hardened components, and the substantial investment required for a launch in the early . Although never funded or built, Project Longshot represented an early exploration of fusion-based concepts, influencing subsequent discussions on deep-space propulsion technologies.

Background

Development History

Project Longshot originated from recommendations in the 1986 report by the National Commission on Space, Pioneering the Space Frontier, which advocated for to initiate a program aimed at sending a series of unmanned probes to nearby stars as part of long-term interstellar exploration efforts beyond initial operations. The commission's vision emphasized advancing through innovative missions to the nearest stellar systems, positioning such endeavors as a natural progression from near-Earth activities. The project was developed collaboratively between the (USNA), , and the during 1987–1988 as part of 's University Advanced Design Program sponsored by the Universities Space Research Association (USRA). This initiative involved USNA students and faculty working under oversight to conceptualize interstellar mission architectures, marking it as a student-led effort with institutional support to explore feasible technologies for deep-space travel. The study concluded on June 30, 1988, producing a comprehensive preliminary design that highlighted the project's role in advancing 's long-range planning. The core output of the development was the report A Study of an Unmanned Mission to Alpha Centauri, published as NASA Technical Paper 3163 in 1988 and authored by Keith A. Beals, Martin Beaulieu, Frank J. Dembia, Joseph Kerstiens, Daniel L. Kramer, Jeffrey R. West, and James A. Zito from the USNA. This document proposed Project Longshot as a preliminary design study for an unmanned probe launch in the early , with the intended for assembly at —the planned predecessor to the —before embarking on a century-long journey to Alpha Centauri. The system was identified as the core innovation to enable this ambitious timeline.

Scientific Rationale

Project Longshot targeted the Alpha Centauri system, the nearest stellar system to the Sun at approximately 4.3 light-years away, comprising three stars: Alpha Centauri A (a G2V sun-like star), Alpha Centauri B (a K1V orange dwarf), and (an M5.5V ). This proximity made it the logical first destination for an interstellar probe, enabling the collection of data on a nearby stellar environment that could not be obtained through remote observations alone. By sending a probe to this system, scientists aimed to gather in-situ measurements that would reveal details about the , including its magnetic fields and particle densities, during the long transit. The mission's scientific foundation rested on the need to advance fundamental astrophysical knowledge through direct exploration of Alpha Centauri's and potential . Studying the interactions within this trinary star setup would provide insights into processes, gravitational influences on orbiting bodies, and the stability of planetary environments in multi-star configurations. Furthermore, investigations into possible exoplanets around these stars were expected to enhance understanding of formation and factors, such as atmospheric compositions and exposure to stellar , which are critical for assessing the prevalence of life-supporting worlds beyond the Solar System. In the broader context, Project Longshot aligned with NASA's visionary objectives for human expansion into , as articulated in 1980s reports like the National Commission on Space's "Pioneering the Space Frontier," which advocated for unmanned precursor missions to lay the groundwork for eventual crewed interstellar endeavors. These reports emphasized developing high-velocity for trajectories to nearby , supporting a century-scale commitment to exploration that would yield data returns on cosmic timescales, such as the probe's anticipated 100-year journey.

Mission Objectives

Primary Goals

The primary goals of Project Longshot centered on achieving a pioneering interstellar mission to the Alpha Centauri , with a targeted transit duration of approximately 100 years to enable detailed in-situ observations. This ambitious timeline allowed the probe to conduct comprehensive studies of the star 's composition, including the stellar atmospheres of Alpha Centauri A and B, as well as any potential planet-sized bodies, using onboard spectrophotometers and imagers. Additionally, the mission aimed to investigate the 's dynamics, such as magnetic fields, solar winds, and orbital interactions within the trinary configuration involving , providing unprecedented data on extrasolar stellar environments. A key operational objective was to collect high-resolution scientific data throughout the mission phases, encompassing the approach to the system and subsequent orbital insertion around Alpha Centauri B as the mission endpoint. During these close operations, the probe was designed to transmit data at rates of up to 1 kbit/s via communications, facilitating the relay of imagery, analyses, and astrometric measurements back to over the century-long journey. This data collection prioritized resolving questions about the en route and the potential presence of planets in the system. Beyond scientific exploration, Project Longshot sought to demonstrate the feasibility of —specifically a pulsed fusion microexplosion drive—for traversing interstellar distances, achieving velocities around 14,700 km/s. This technology validation was intended to serve as a proof-of-concept for future unmanned and potentially crewed missions, highlighting the viability of long-duration autonomous operations powered by a 300 kW fission reactor. By successfully executing these goals, the project aimed to expand humanity's technological horizon for deep-space exploration.

Target System

The Alpha Centauri system, located approximately 4.3 light-years from , served as the primary target for Project Longshot due to its status as the nearest stellar system to the Sun, offering unique opportunities for in-depth astronomical study. This trinary system consists of Alpha Centauri A and B forming a close binary pair, with the more distant as a loosely bound companion. The binary components orbit each other with a period of approximately 80 years and an eccentricity that causes their separation to vary between 11.2 and 35.6 astronomical units (AU). Alpha Centauri A, a G2V star similar to the Sun, and Alpha Centauri B, a cooler K1V dwarf with an of 5,260 K, together enable comparative analysis of solar-type and lower-mass stellar environments. Project Longshot specifically targeted Alpha Centauri B for orbital insertion, selected for its relatively understudied nature as a K-type star and its potential to host stable planetary zones less perturbed by the brighter Alpha Centauri A. The cooler temperature of Alpha Centauri B supports the possibility of temperate conditions for hypothetical planets, contrasting with the more intense from Alpha Centauri A, and allowing for focused observations of potential indicators of planetary systems such as dynamical stability in its circumstellar disk. , a flare-active M5.5Ve orbiting the binary pair at about 12,500 AU (roughly 0.21 light-years), was noted but not prioritized as the main target due to its extreme variability and lower scientific yield for the mission's objectives. The proximity of the Alpha Centauri system facilitates unprecedented detailed examination of stellar phenomena that are challenging to resolve in more distant targets, such as the interactions of stellar winds with circumstellar material and the structure of dust disks potentially indicative of planetary formation. Unlike later missions aimed at systems tens or hundreds of light-years away, Longshot's design leveraged this nearness to probe the environment around Alpha Centauri B with higher resolution, using instruments to map , ultraviolet emissions, and signatures of debris. This approach promised insights into K-dwarf stellar environments, which constitute a significant fraction of stars in the galaxy.

Spacecraft Design

Overall Configuration

Project Longshot's featured a optimized for assembly in low-Earth orbit (LEO), consisting of several distinct components integrated via a central structure. The overall configuration included a probe head for instruments and communications, six cylindrical fuel tanks, a collapsible , a fission module, and a fusion drive assembly. This architecture allowed for phased construction using multiple launches from , minimizing the mass penalties associated with trajectories. The total mass of the assembled spacecraft was 396.4 metric tons, comprising 264.3 metric tons of / pellet , 30 metric tons of (including the head, post-propulsion system discard), and the remaining structural elements such as tanks, , and components. The tanks were constructed from 2 mm thick aluminum sheets, each with a radius of 2.5 meters and a length of 31.68 meters, designed to be jettisoned sequentially as was expended to reduce mass during the mission. The central served as the primary structural backbone, a collapsible that connected the forward head to the aft and power modules, enabling efficient packaging for launch and deployment. When fully assembled, the spacecraft reflected the elongated profile dominated by the fuel tank array and extended truss. The fission reactor module, weighing 6.4 metric tons including shielding and support systems, was integrated into the truss for stability, while the fusion drive assembly occupied the rear section. This LEO-based modular approach facilitated the use of heavy-lift vehicles like the Advanced Launch System (ALS) or Space Shuttle derivatives for component delivery to an orbital assembly platform.

Propulsion System

The propulsion system of Project Longshot was designed as a pulsed fusion microexplosion drive, employing to generate thrust for the interstellar journey. Small pellets composed of (He³) and (D) served as the fusion fuel, injected into a reaction chamber where they were imploded and ignited to produce high-velocity plasma exhaust directed rearward through a magnetic . This approach drew inspiration from earlier concepts like but adapted for unmanned operation with onboard power constraints. Ignition of the pellets relied on high-energy particle beams to compress and the , triggering the D-He³ fusion reaction that primarily yields and protons as exhaust products, with minimal production to reduce irradiation. The pellets were launched in liquid form from and processed into solid form in for storage and injection. During the main phase, the fusion reactions became self-sustaining after initial startup, with the plasma exhaust magnetically channeled to provide continuous . A fission reactor briefly powered the igniters and banks for the first pulses. The system's performance was characterized by a of 1,020,000 seconds, enabling efficient use over the long mission duration despite the low profile. Pellet injection frequency was not fixed but scaled to mission requirements, influencing the mass of ignition coils and beams; engineering trade studies indicated rates sufficient for gradual acceleration to about 14,000 km/s over several years. For in-system operations, the assumed orbital assembly, obviating the need for dedicated chemical boosters post-launch. The exhaust velocity vev_e, fundamental to the drive's , was derived from the energy released per fusion pulse. Assuming the pulse energy EE is fully converted to the of the mass mpm_p (primarily the fusion products), 12mpve2=E\frac{1}{2} m_p v_e^2 = E Rearranging yields ve=2Emp.v_e = \sqrt{\frac{2E}{m_p}}.
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