Simulation of Phobos gravity field estimation from Tianwen-1 flybys and implications for the modelling of Phobos’ internal structure

Author:

Guo X1,Yan J G1,Yang X2,Liu L1,Chen Y H1,Ye M1,Barriot J P13

Affiliation:

1. State Key Laboratory of Engineering in Surveying, Mapping and Remote Sensing, Wuhan University , 129 Luoyu Road, Wuhan 430070, China

2. State Key Laboratory of Satellite Navigation System and Equipment Technology , 589 Zhongshan Road, Shijiazhuang 050081, China

3. Geodesy Observatory of Tahiti, University of French Polynesia , BP 6570, Faa’a 98702, Tahiti, French Polynesia

Abstract

ABSTRACT Doppler radio tracking data from Tianwen-1, China’s first Mars mission, could contribute to a better estimate of the gravity field of Phobos. In this study, we show that a determination up to degree and order 3 is feasible by considering five additional flybys of Phobos by the Tianwen-1 spacecraft, in addition to the previous flybys already done by the Mars Express spacecraft, and probably degree and order 5 is within reach. Three cases of mass repartition are considered: (i) a homogeneous case, (ii) a core-dominated Phobos, and (iii) a mantle-dominated Phobos. The case of a mantle-dominated Phobos is the easiest to detect, followed by a homogeneous Phobos, and finally by a core-dominated Phobos. We also discuss implications about the modelling of the internal structure of Phobos.

Funder

National Natural Science Foundation of China

China Scholarship Council

CNES

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

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