Based on the tracking observations of radio ranges and VLBI delays of Chang’E-1 (CE-1) satellite during the controlled landing on the Moon on March 1, 2009, the landing trajectory and the coordinates of the landing point are determined by positioning analysis. It is shown that the landing epoch (the emission epoch of the last signal) of CE-1 satellite on the Moon was at UTC8h13m6.51s. The lunar longitude, latitude and surface height of the landing point in the lunar primary axes frame are respectively 52.2732°, 1.6440° and −3.56 km (the reference lunar radius is 1738 km). The uncertainties are 0.0040°, 0.0168° and 0.18 km. The corresponding uncertainty in the tangential direction of the lunar surface is 0.52 km and the three-dimensional (3D) positioning uncertainty is 0.55 km. It is accordingly deduced that even with the present technical specifications of the radio ranges and VLBI delays, the 1 km 3D positioning precision could be guaranteed for the lander in the second stage of China’s Lunar Exploration Project. Concerning the trace determination of the rover on the lunar surface, because only telemetry signal will be emitted, VLBI would be the sole tracking technique from the Earth. The application of the constraint of geocentric distance is shown to be helpful to improving the positioning precision. It is worthy to pay close attention to the applications of the same beam VLBI technique, the lunar topographic model and the on-board observations of the lander and rover to the position/trace determination of the rover.
[1]
I. Miles.
Measuring the future: Statistics and the information age
,
1991
.
[2]
Christopher S. Jacobs,et al.
Astrometry and geodesy with radio interferometry: experiments, models, results
,
1998
.
[3]
J. L. Li,et al.
Monitoring the lunar capture of Chang'E-1 satellite by real-time reduction of the instantaneous state vectors
,
2007,
Proceedings of the International Astronomical Union.
[4]
Jinling Li,et al.
The Chinese VLBI network and its astrometric role
,
2007
.
[5]
ZongYu Yue,et al.
Automated detection of lunar craters based on object-oriented approach
,
2008
.
[6]
李金岭.
The Contribution of CVN to the CE-1 Mission
,
2008
.
[7]
Jianfeng Cao,et al.
Lunar topographic model CLTM-s01 from Chang’E-1 laser altimeter
,
2009
.