Phobos and Mars orbit as a base for asteroid exploration and mining

The number and total mass of high value near-Earth asteroids (NEOs) are limited. If space exploration and mining becomes profitable then at some point it will benefit from moving on to the far greater resources of the Main Belt Asteroids (MBAs). Most MBAs are energetically too hard to reach with pre...

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Veröffentlicht in:Planetary and space science 2022-05, Vol.214, p.105450, Article 105450
Hauptverfasser: Taylor, Anthony J., McDowell, Jonathan C., Elvis, Martin
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Sprache:eng
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Zusammenfassung:The number and total mass of high value near-Earth asteroids (NEOs) are limited. If space exploration and mining becomes profitable then at some point it will benefit from moving on to the far greater resources of the Main Belt Asteroids (MBAs). Most MBAs are energetically too hard to reach with present technology from low Earth orbit. An alternative is to use Mars orbit as a base from which to conduct MBA research, prospecting, and mining. We have developed PARC: Python Asteroid Rendezvous Code which uses a fast Lambert's problem solver and straightforward maneuver schemes to survey the delta-v necessary to rendezvous with any known asteroid from either Earth or Mars orbit given a specified launch date and time of flight. We used PARC to investigate whether Phobos-like orbits around Mars at altitudes of ∼9000 ​km, are more energetically favorable and useful locations from which to dispatch missions to MBAs. We find that they are. From a Phobos-like orbit, around 100,000 known MBAs have delta-v
ISSN:0032-0633
1873-5088
DOI:10.1016/j.pss.2022.105450