Exoplanets & Exomoons

Chasing Nomadic Worlds: A New Class of Deep Space Missions

By Keith Cowing
Status Report
July 25, 2023
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Chasing Nomadic Worlds: A New Class of Deep Space Missions
The typical flight time expected to reach a nomadic world (y-axis) with radius > 𝑅 (x-axis) by utilizing a laser sail traveling at 1% the speed of light (3000 km/s); the plot is generated from (22). — astro-ph.EP

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 100km≲R≲104km. The cumulative number density n>(>R) appears to follow a heuristic power law given by n>∝R−3. 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 thus comprise closer interstellar targets than any planets bound to stars.

For the first time, we systematically analyze the feasibility of exploring these unbounded objects via deep space missions. We investigate what near-future propulsion systems could allow us to reach nomadic worlds of radius >R in a 50-year flight timescale. Objects with R∼100 km are within the purview of multiple propulsion methods such as electric sails, laser electric propulsion, and solar sails. In contrast, nomadic worlds with R≳1000 km are accessible by laser sails (and perhaps nuclear fusion), thereby underscoring their vast potential for deep space exploration.

Manasvi Lingam, Andreas M. Hein, T. Marshall Eubanks

Comments: 22 pages including “Highlights” page; accepted by Acta Astronautica
Subjects: Earth and Planetary Astrophysics (astro-ph.EP); Astrophysics of Galaxies (astro-ph.GA)
Cite as: arXiv:2307.12411 [astro-ph.EP] (or arXiv:2307.12411v1 [astro-ph.EP] for this version)
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Submission history
From: T. Marshall Eubanks Mr
[v1] Sun, 23 Jul 2023 19:30:33 UTC (225 KB)

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