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A simulation experiment on the GM estimation for Comet 133P/Elst-Pizarro
作者姓名:Wu-Tong Gao  Jian-Guo Yan  Wei-Tong Jin  Xuan Yang  Chen Yang  Mao Ye  Fei Li  Jean-Pierre Barriot
作者单位:l State Key Laboratory of Information Engineering in Surveying;China Academy of Space Technology;Geodesy Observatory of Tahiti
基金项目:the National Natural Science Foundation of China(U1831132 and 41874010);Innovation Group of Natural Fund of Hubei Province(2018CFA087);supported by a DAR fund in planetology from the French Space Agency(CNES)。
摘    要:In China’s asteroid mission to be launched around 2025,(7968)133 P/Elst-Pizarro(hereafter 133 P)will be the second target,after a visit to asteroid(469219)Kamo’oalewa.This paper describes a simulation of precise orbit determination for the spacecraft around comet 133 P,as well as estimation of its gravitational parameter(GM)value and the solar radiation pressure coefficient Cr for the spacecraft.Different cometocentric distances of 200,150 and 100 km orbits are considered,as well as two tracking modes:exclusive two-way range-rate mode(Earth station to spacecraft)and combinations of two-way range-rate and local spacecraft onboard ranging to the comet.Compared to exclusive two-way range-rate,the introduction of local ranging observables improves the final GM uncertainties by up to one order of magnitude.An ephemeris error in the orbit of 133 P is also considered,and we show that,to obtain a reliable estimate of the GM for 133 P,this error cannot exceed a one km range.

关 键 词:celestial  mechanics  space  vehicles  comets:individual(133P/Elst-Pizarro)  methods:statistical
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