Dynamic science on the Stardust mission -: art. no. 8117

被引：6

作者：

Anderson, JD

Lau, EL

Bird, MK

Clark, BC

Giampieri, G

Pätzold, M

机构：

[1] CALTECH, Jet Prop Lab, Pasadena, CA 91109 USA

[2] Univ Bonn, Inst Radioastron, D-53121 Bonn, Germany

[3] Lockheed Martin Astronaut Co, Denver, CO 80201 USA

[4] Univ London Imperial Coll Sci Technol & Med, Dept Math, London SW7 2BW, England

[5] Univ Cologne, Inst Geophys & Meteorol, D-50923 Cologne, Germany

来源：

JOURNAL OF GEOPHYSICAL RESEARCH-PLANETS | 2003年 / 108卷 / E10期

关键词：

Wild; 2; Stardust; radio science;

D O I：

10.1029/2003JE002092

中图分类号：

P3 [地球物理学]; P59 [地球化学];

学科分类号：

0708 ; 070902 ;

摘要：

[1] Radio Doppler and ranging data at X band (similar to8.4 GHz), optical navigation data, and spacecraft attitude control data can be used to characterize the dust environment surrounding comet 81P/Wild 2 and possibly the mass and bulk density of its nucleus. As a secondary objective, a favorable solar conjunction prior to the cometary encounter on 2 January 2004 can be used to sound the Sun's corona at X band.

引用

页数：7

共 18 条

[1] Theoretical description of spacecraft flybys by variation of parameters [J].