Simulation of the Chang’E-5 mission contribution in lunar long wavelength gravity field improvement
Autor: | Mao Ye, Jianguo Yan, Shanhong Liu, Fei Li, Jinsong Ping, Xuan Yang, Jean-Pierre Barriot, Jin Weitong |
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Rok vydání: | 2018 |
Předmět: |
Physics
010504 meteorology & atmospheric sciences Field (physics) business.industry Astrophysics::Instrumentation and Methods for Astrophysics Mode (statistics) Astronomy and Astrophysics Tracking (particle physics) 01 natural sciences Gravitational field Orders of magnitude (time) Space and Planetary Science Physics::Space Physics 0103 physical sciences Polar Astrophysics::Earth and Planetary Astrophysics Love number Aerospace engineering Space research business 010303 astronomy & astrophysics 0105 earth and related environmental sciences |
Zdroj: | Astrophysics and Space Science. 363 |
ISSN: | 1572-946X 0004-640X |
DOI: | 10.1007/s10509-018-3350-x |
Popis: | The precision of lunar gravity field estimation has improved by means of three to five orders of magnitude since the successful GRAIL lunar mission. There are still discrepancies however, in the low degree coefficients and long wavelength components of the solutions developed by two space research centers (JPL and GSFC). These discrepancies hint at the possibilities for improving the accuracy in the long wavelength part of the lunar gravity field. In the near future, China will launch the Chang’E-5 lunar mission. In this sample-return mission, there will be a chance to do KBRR measurements between an ascending module and an orbiting module. These two modules will fly around lunar at an inclination of ∼49 degrees, with an orbital height of 100 km and an inter-satellite distance of 200 km. In our research, we simulated the contribution of the KBRR tracking mode for different GRAIL orbital geometries. This analysis indicated possible deficiencies in the low degree coefficient solutions for the polar satellite-to-satellite tracking mode at various orbital heights. We also investigated the potential contributions of the KBRR to the Chang’E-5 mission goal of lunar gravity field recovery, especially in the long wavelength component. Potential improvements were assessed using various power spectrums of the lunar gravity field models. In addition, we also investigated possible improvements in solving lunar tidal Love number K2. These results may assist the implementation of the Chang’E-5 mission. |
Databáze: | OpenAIRE |
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