Autonomous navigation for the deep impact mission encounter with comet Tempel 1

被引:53
作者
Mastrodemos, N [1 ]
Kubitschek, DG [1 ]
Synnott, SP [1 ]
机构
[1] CALTECH, Jet Prop Lab, Opt Navigat Grp, Navigat & Mission Design Sect, Pasadena, CA 91109 USA
基金
美国国家航空航天局;
关键词
autonomous navigation; Tempel; 1; simulations;
D O I
10.1007/s11214-005-3394-4
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The engineering goal of the Deep Impact mission is to impact comet Tempel 1 on July 4, 2005, with a 370 kg active Impactor spacecraft (s/c). The impact velocity will be just over 10 km/s and is expected to excavate a crater approximately 20m deep and 100m wide. The Impactor s/c will be delivered to the vicinity of Tempel 1 by the Flyby s/c, which is also the key observing platform for the event. Following Impactor release, the Flyby will change course to pass the nucleus at an altitude of 500 km and at the same time slow down in order to allow approximately 800s of observation of the impact event, ejecta plume expansion, and crater formation. Deep Impact will use the autonomous optical navigation (AutoNav) software system to guide the Impactor s/c to intercept the nucleus of Tempel 1 at a location that is illuminated and viewable from the Flyby. The Flyby s/c uses identical software to determine its comet-relative trajectory and provide the attitude determination and control system (ADCS) with the relative position information necessary to point the High Resolution Imager (HRI) and Medium Resolution Imager (MRI) instruments at the impact site during the encounter. This paper describes the Impactor s/c autonomous targeting design and the Flyby s/c autonomous tracking design, including image processing and navigation ( trajectory estimation and maneuver computation). We also discuss the analysis that led to the current design, the expected system performance as compared to the key mission requirements and the sensitivity to various s/c subsystems and Tempel 1 environmental factors.
引用
收藏
页码:95 / 121
页数:27
相关论文
共 10 条
[1]   Autonomous optical navigation for interplanetary missions [J].
Bhaskaran, S ;
Riedel, JE ;
Synnott, SP .
SPACE SCIENCECRAFT CONTROL AND TRACKING IN THE NEW MILLENNIUM, 1996, 2810 :32-43
[2]  
BHASKARAN S, 1998, AAS AIAA SPAC FLIGHT
[3]   Comparison of USGS and DLR topographic models of Comet Borrelly and photometric applications [J].
Kirk, RL ;
Howington-Kraus, E ;
Soderblom, LA ;
Giese, B ;
Oberst, J .
ICARUS, 2004, 167 (01) :54-69
[4]  
RIEDEL JE, 2000, DEEP SPAC 1 TECHN VA
[5]  
Russ J.C., 1999, IMAGE PROCESSING HDB, V3rd
[6]  
STOOKE P, 2000, HALLEY NUCL SHAPE MO
[7]  
TROCHMAN W, 2001, DIIMPACS010 BATC
[8]   The origin of comets in the solar nebula: A unified model [J].
Weidenschilling, SJ .
ICARUS, 1997, 127 (02) :290-306
[9]  
ZARCHAN P, 1997, TACTICAL STRATEGIC M, V176
[10]  
ZIMPFER D, 2003, 26 ANN GUID CONTR C