Mars Science Laboratory entry, descent, and landing system

被引:0
作者
Steltzner, Adam [1 ]
Kipp, Devin [1 ]
Chen, Allen [1 ]
Burkhart, Dan [1 ]
Guernsey, Carl [1 ]
Mendeck, Gavin [2 ]
Mitcheltree, Robert [1 ]
Powell, Richard [3 ]
Rivellini, Tommaso [1 ]
San Martin, Miguel [1 ]
Way, David [3 ]
机构
[1] CALTECH, Jet Prop Lab, 4800 Oak Grove Dr, Pasadena, CA 91109 USA
[2] NASA, Johnson Space Flight Ctr, Houston, TX USA
[3] NASA, Langley Res Ctr, Hampton, VA USA
来源
2006 IEEE AEROSPACE CONFERENCE, VOLS 1-9 | 2006年
关键词
D O I
暂无
中图分类号
V [航空、航天];
学科分类号
08 ; 0825 ;
摘要
In 2010, the Mars Science Laboratory (MSL) mission will pioneer the next generation of robotic Entry, Descent, and Landing (EDL) systems by delivering the largest and most capable rover to date to the surface of Mars. In addition to landing more mass than prior missions to Mars, MSL will offer access to regions of Mars that have been previously unreachable. By providing an EDL system capable of landing at altitudes as high as 2 km above the reference areoid, as defined by the Mars Orbiting Laser Altimeter (MOLA) program, MSL will demonstrate sufficient performance to land on a large fraction of the Martian surface. By contrast, the highest altitude landing to date on Mars has been the Mars Exploration Rover (MER) MER-B at 1.44 kin below the areoid. The coupling of this improved altitude performance with latitude limits as large as 60 degrees off of the equator and a precise delivery to within 10 km of a surface target will allow the science community to select the MSL landing site from thousands of scientifically interesting possibilities. In meeting these requirements, MSL is extending the limits of the EDL technologies qualified by the Mars Viking, Mars Pathfinder, and MER missions. This paper discusses the MSL EDL architecture, system, and subsystem design and discusses some of the challenges faced in delivering such an unprecedented rover payload to the surface of Mars.(1,2).
引用
收藏
页码:857 / +
页数:2
相关论文
共 4 条
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Carman GL, 1998, AIAA ATM FLIGHT MECH
[2]  
Justus C.G., 2001, TM2001210961 NASA
[3]  
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[4]  
WAY DW, 2006, IEEE AER C MARCH 4 1