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Trajectory design and operational challenges for the exploration of phobos

Trajectory design and operational challenges for the exploration of phobos
Trajectory design and operational challenges for the exploration of phobos

Designing trajectories to allow for long observation campaigns of planetary moons is not an easy task. Quasi-Satellite Orbits are a type of distant retrograde orbits suitable for Phobos exploration missions, as they offer a convenient means to orbit this moon in the sense of relative motion. MMX (Martian Moons eXploration mission) is a chemical-propulsion sample return mission currently under development at the Japanese exploration agency (JAXA) which plans to make extensive use of QSO (Quasi Satellite Orbits) trajectories during its three-year stay in the vicinity of Phobos. Moreover, the French Space Agency (CNES) contributes to the mission analysis studies of MMX for the Phobos proximity phase in the frame of a larger collaboration between the Japanese and the French agencies, which also includes the delivery of a major payload (MIRS), as well as a rover built in collaboration with the German agency (DLR). Several of the major challenges that MMX teams have to face when building orbital scenarios exhibiting the best trade-off in terms of scientific return, maneuver cost and operational risk will be outlined in this paper. In particular, this work focuses on the contribution of the flight dynamics team at CNES to the design of three dimensional QSO trajectories and their operational use. An overview of the methods implemented to support the choice of suitable spatial trajectories around Phobos, in addition to the design of transfer trajectories, station-keeping and eclipse analyses for 3D-QSO will be presented.

0065-3438
1493-1507
Univelt, Inc.
Canalias, Elisabet
900c6845-45ee-4422-b21b-810d5f27f21d
Lorda, Laurence
a292b8d8-d65b-4733-b74f-0a620c308dcd
Chen, Hongru
8286469d-afe1-46e5-b107-694017de4d97
Ikeda, Hitoshi
d4216f54-eeb2-4120-ae94-6a6485ea567f
Wilson, Roby S.
Shan, Jinjun
Howell, Kathleen C.
Hoots, Felix R.
Canalias, Elisabet
900c6845-45ee-4422-b21b-810d5f27f21d
Lorda, Laurence
a292b8d8-d65b-4733-b74f-0a620c308dcd
Chen, Hongru
8286469d-afe1-46e5-b107-694017de4d97
Ikeda, Hitoshi
d4216f54-eeb2-4120-ae94-6a6485ea567f
Wilson, Roby S.
Shan, Jinjun
Howell, Kathleen C.
Hoots, Felix R.

Canalias, Elisabet, Lorda, Laurence, Chen, Hongru and Ikeda, Hitoshi (2021) Trajectory design and operational challenges for the exploration of phobos. Wilson, Roby S., Shan, Jinjun, Howell, Kathleen C. and Hoots, Felix R. (eds.) In ASTRODYNAMICS 2020. vol. 175, Univelt, Inc. pp. 1493-1507 .

Record type: Conference or Workshop Item (Paper)

Abstract

Designing trajectories to allow for long observation campaigns of planetary moons is not an easy task. Quasi-Satellite Orbits are a type of distant retrograde orbits suitable for Phobos exploration missions, as they offer a convenient means to orbit this moon in the sense of relative motion. MMX (Martian Moons eXploration mission) is a chemical-propulsion sample return mission currently under development at the Japanese exploration agency (JAXA) which plans to make extensive use of QSO (Quasi Satellite Orbits) trajectories during its three-year stay in the vicinity of Phobos. Moreover, the French Space Agency (CNES) contributes to the mission analysis studies of MMX for the Phobos proximity phase in the frame of a larger collaboration between the Japanese and the French agencies, which also includes the delivery of a major payload (MIRS), as well as a rover built in collaboration with the German agency (DLR). Several of the major challenges that MMX teams have to face when building orbital scenarios exhibiting the best trade-off in terms of scientific return, maneuver cost and operational risk will be outlined in this paper. In particular, this work focuses on the contribution of the flight dynamics team at CNES to the design of three dimensional QSO trajectories and their operational use. An overview of the methods implemented to support the choice of suitable spatial trajectories around Phobos, in addition to the design of transfer trajectories, station-keeping and eclipse analyses for 3D-QSO will be presented.

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More information

Published date: 2021
Additional Information: Publisher Copyright: © 2021, Univelt Inc. All rights reserved.
Venue - Dates: AAS/AIAA Astrodynamics Specialist Conference, 2020, , Virtual, Online, 2020-08-09 - 2020-08-12

Identifiers

Local EPrints ID: 499248
URI: http://eprints.soton.ac.uk/id/eprint/499248
ISSN: 0065-3438
PURE UUID: 2f8963a2-0594-4d1a-aeb8-2a033783b6c1
ORCID for Hongru Chen: ORCID iD orcid.org/0000-0001-9453-6962

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Date deposited: 12 Mar 2025 17:56
Last modified: 12 Mar 2025 17:56

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Contributors

Author: Elisabet Canalias
Author: Laurence Lorda
Author: Hongru Chen ORCID iD
Author: Hitoshi Ikeda
Editor: Roby S. Wilson
Editor: Jinjun Shan
Editor: Kathleen C. Howell
Editor: Felix R. Hoots

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