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Distant Retrograde Orbits for space-based Near Earth Objects detection

Distant Retrograde Orbits for space-based Near Earth Objects detection
Distant Retrograde Orbits for space-based Near Earth Objects detection
We analyse a concept for the detection of Potentially Hazardous Asteroids (PHAs) from a space-based network of telescopes on retrograde Distant Periodic Orbits. Planar periodic orbits are designed in the Sun–Earth circular restricted three-body problem, starting from initial conditions in the Hill’s problem available from the literature. A family of retrograde orbits centred at the Earth is selected as baseline, based on their maximum distance from Earth, larger than the Earth–L2 distance. Indeed, spacecraft on such orbits can detect PHAs incoming from the Sun direction, which could not otherwise be monitored from current Earth-based systems. A trade-off on the orbit amplitude, asteroid diameter to be detected, and the constellation size is performed considering current visible sensor telescope technology. The Chelyabinsk meteor scenario is studied and the potential warning time that could be gained with a space-based survey system with respect to an Earth based-survey system is shown.
0273-1177
967-988
Stramacchia, Michele
a82506fd-6885-4567-a510-17e3fbb46ef2
Colombo, Camilla
595ced96-9494-40f2-9763-ad4a0f96bc86
Bernelli-Zazzera, Franco
4b3eb3b1-d06e-47cd-9676-f465dba2b1e7
Stramacchia, Michele
a82506fd-6885-4567-a510-17e3fbb46ef2
Colombo, Camilla
595ced96-9494-40f2-9763-ad4a0f96bc86
Bernelli-Zazzera, Franco
4b3eb3b1-d06e-47cd-9676-f465dba2b1e7

Stramacchia, Michele, Colombo, Camilla and Bernelli-Zazzera, Franco (2016) Distant Retrograde Orbits for space-based Near Earth Objects detection. Advances in Space Research, 58 (6), 967-988. (doi:10.1016/j.asr.2016.05.053).

Record type: Article

Abstract

We analyse a concept for the detection of Potentially Hazardous Asteroids (PHAs) from a space-based network of telescopes on retrograde Distant Periodic Orbits. Planar periodic orbits are designed in the Sun–Earth circular restricted three-body problem, starting from initial conditions in the Hill’s problem available from the literature. A family of retrograde orbits centred at the Earth is selected as baseline, based on their maximum distance from Earth, larger than the Earth–L2 distance. Indeed, spacecraft on such orbits can detect PHAs incoming from the Sun direction, which could not otherwise be monitored from current Earth-based systems. A trade-off on the orbit amplitude, asteroid diameter to be detected, and the constellation size is performed considering current visible sensor telescope technology. The Chelyabinsk meteor scenario is studied and the potential warning time that could be gained with a space-based survey system with respect to an Earth based-survey system is shown.

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Accepted/In Press date: 30 May 2016
e-pub ahead of print date: 4 June 2016
Published date: 15 September 2016
Organisations: Astronautics Group

Identifiers

Local EPrints ID: 402548
URI: http://eprints.soton.ac.uk/id/eprint/402548
ISSN: 0273-1177
PURE UUID: 58c4b0ca-9bcd-4a83-9359-a12ec2577948
ORCID for Camilla Colombo: ORCID iD orcid.org/0000-0001-9636-9360

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Date deposited: 10 Nov 2016 14:53
Last modified: 15 Mar 2024 06:03

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Contributors

Author: Michele Stramacchia
Author: Camilla Colombo ORCID iD
Author: Franco Bernelli-Zazzera

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