Chasing Nomadic Worlds: A New Class of Deep Space Missions
Manasvi Lingam, Andreas M. Hein, T. Marshall Eubanks

TL;DR
This paper estimates the abundance of nomadic worlds not bound to stars, analyzes their potential for exploration, and evaluates feasible deep space mission strategies to reach them within 50 years.
Contribution
It introduces a systematic analysis of the feasibility of exploring nomadic worlds using near-future propulsion systems within a 50-year timeframe.
Findings
Nomadic worlds are likely numerous, especially smaller ones, and could be close to the Solar System.
Multiple propulsion methods could reach 100 km radius objects within 50 years.
Larger nomadic worlds (>1000 km) are accessible via laser sails or nuclear fusion propulsion.
Abstract
Nomadic worlds, i.e., objects not gravitationally bound to any star(s), are of great interest to planetary science and astrobiology. They have garnered attention recently due to constraints derived from microlensing surveys and the recent discovery of interstellar planetesimals. In this paper, we roughly estimate the prevalence of nomadic worlds with radii of . The cumulative number density appears to follow a heuristic power law given by . Therefore, smaller objects are probably much more numerous than larger rocky nomadic planets, and statistically more likely to have members relatively close to the inner Solar system. Our results suggest that tens to hundreds of planet-sized nomadic worlds might populate the spherical volume centered on Earth and circumscribed by Proxima Centauri, and may…
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Taxonomy
TopicsAstro and Planetary Science · Space Satellite Systems and Control · Spacecraft Dynamics and Control
