Project Lyra: Sending a Spacecraft to 1I/'Oumuamua (former A/2017 U1), the Interstellar Asteroid
Andreas M. Hein, Nikolaos Perakis, T. Marshall Eubanks, Adam Hibberd,, Adam Crowl, Kieran Hayward, Robert G. Kennedy III, Richard Osborne

TL;DR
This paper analyzes feasible near-term mission designs to intercept the interstellar object 1I/'Oumuamua, considering high-velocity trajectories, propulsion options, and technological constraints to enable direct study of material from other star systems.
Contribution
It presents a high-level analysis of potential mission architectures and propulsion technologies capable of reaching 1I/'Oumuamua within 5-10 years using current or near-term technology.
Findings
A Falcon Heavy-class launcher could send a spacecraft to 1I/'Oumuamua if launched in 2021.
A Saturn flyby could enable a spacecraft comparable to New Horizons to reach the object.
Deceleration at 'Oumuamua is highly desirable for maximizing scientific return.
Abstract
The first definitely interstellar object 1I/'Oumuamua (previously A/2017 U1) observed in our solar system provides the opportunity to directly study material from other star systems. Can such objects be intercepted? The challenge of reaching the object within a reasonable timeframe is formidable due to its high heliocentric hyperbolic excess velocity of about 26 km/s; much faster than any vehicle yet launched. This paper presents a high-level analysis of potential near-term options for a mission to 1I/'Oumuamua and potential similar objects. Launching a spacecraft to 1I/'Oumuamua in a reasonable timeframe of 5-10 years requires a hyperbolic solar system excess velocity between 33 to 76 km/s for mission durations between 30 to 5 years. Different mission durations and their velocity requirements are explored with respect to the launch date, assuming direct impulsive transfer to the…
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