Long-wavelength lunar gravity field recovery from simulated orbit and inter-satellite tracking data

2013 ◽  
Vol 52 (11) ◽  
pp. 1919-1928 ◽  
Author(s):  
Jianguo Yan ◽  
Oliver Baur ◽  
Li Fei ◽  
Ping Jinsong
2020 ◽  
Vol 636 ◽  
pp. A45
Author(s):  
Jianguo Yan ◽  
Shanhong Liu ◽  
Chi Xiao ◽  
Mao Ye ◽  
Jianfeng Cao ◽  
...  

Context. Chinese lunar missions have grown in number over the last ten years, with an increasing focus on radio science investigations. In previous work, we estimated two lunar gravity field models, CEGM01 and CEGM02. The recently lunar mission, Chang’e 5T1, which had an orbital inclination between 18 and 68 degrees, and collected orbital tracking data continually for two years, made an improved gravity field model possible. Aims. Our aim was to estimate a new lunar gravity field model up to degree and order 100, CEGM03, and a new tidal Love number based on the Chang’e 5T1 tracking data combined with the historical tracking data used in the solution of CEGM02. The new model makes use of tracking data with this particular inclination, which has not been used in previous gravity field modeling. Methods. The solution for this new model was based on our in-house software, LUGREAS. The gravity spectrum power, post-fit residuals after precision orbit determination (POD), lunar surface gravity anomalies, correlations between parameters, admittance and coherence with topography model, and accuracy of POD were analyzed to validate the new CEGM03 model. Results. We analyzed the tracking data of the Chang’e 5T1 mission and estimated the CEGM03 lunar gravity field model. We found that the two-way Doppler measurement accuracy reached 0.2 mm s−1 with 10 s integration time. The error spectrum shows that the formal error for CEGM03 was at least reduced by about 2 times below the harmonic degree of 20, when compared to the CEGM02 model. The admittance and correlation of gravity and topography was also improved when compared to the correlations for the CEGM02 model. The lunar potential Love number k2 was estimated to be 0.02430±0.0001 (ten times the formal error). Conclusions. From the model analysis and comparison of the various models, we identified improvements in the CEGM03 model after introducing Chang’e 5T1 tracking data. Moreover, this study illustrates how the low and middle inclination orbits could contribute better accuracy for a low degree of lunar gravity field.


2010 ◽  
Vol 85 (4) ◽  
pp. 205-228 ◽  
Author(s):  
S. Goossens ◽  
K. Matsumoto ◽  
Q. Liu ◽  
F. Kikuchi ◽  
K. Sato ◽  
...  

2012 ◽  
Vol 117 (E2) ◽  
pp. n/a-n/a ◽  
Author(s):  
Sander Goossens ◽  
Yoshiaki Ishihara ◽  
Koji Matsumoto ◽  
Sho Sasaki

2007 ◽  
Vol 50 (2) ◽  
pp. 399-403
Author(s):  
Jian-Guo YAN ◽  
Jing-Song PING ◽  
Fei LI ◽  
K Matsumoto ◽  
Guang-Li WANG ◽  
...  

2008 ◽  
Vol 42 (2) ◽  
pp. 331-336 ◽  
Author(s):  
Koji Matsumoto ◽  
Hideo Hanada ◽  
Noriyuki Namiki ◽  
Takahiro Iwata ◽  
Sander Goossens ◽  
...  

2008 ◽  
Vol 42 (2) ◽  
pp. 337-340 ◽  
Author(s):  
Jianguo Yan ◽  
Jingsong Ping ◽  
K. Matsumoto ◽  
Fei Li

Knowledge of long-wavelength features of the geopotential is significantly improved by the use of precision satellite tracking with lasers. Tracking data on nine satellites are combined with terrestrial gravimetry to obtain a spherical-harmonics representation of the geopotential complete through degree and order 24. An improved gravity-field model provides better satellite ephemerides and a reference for analysing satellite-to-sea-surface altimetry.


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