The autonomous asteroid mapping mission "Bering"

被引:1
|
作者
Andersen, A. C.
Michelsen, R.
Haack, H.
Jorgensen, J. L.
Betto, M.
Jorgensen, P. S.
机构
[1] NORDITA, DK-2100 Copenhagen, Denmark
[2] Univ Copenhagen, Astron Observ, NBIfAFG, DK-2100 Copenhagen, Denmark
[3] Univ Copenhagen, Geol Museum, DK-1350 Copenhagen, Denmark
[4] Tech Univ Denmark, Orsted DTU, MIS, DK-2800 Lyngby, Denmark
关键词
space vehicles; instruments; minor planets; asteroids; ephermerides; instrumentation; detectors; spectrographs; methods; observational;
D O I
10.1016/j.actaastro.2005.07.025
中图分类号
V [航空、航天];
学科分类号
08 ; 0825 ;
摘要
Asteroids are believed to be the remnants of the material from which the Solar System formed. This view is supported by the way the predominating asteroid type changes with increasing distance from the Sun within the asteroid belt. Highspeed collisions between asteroids are gradually resulting in their break-up. The size distribution of kilometer-sized asteroids implies that the presently undetected population of sub-kilometer asteroids far outnumber the known larger objects. Sub-kilometer asteroids are expected to provide unique insight into the evolution of the asteroid belt and to the meteorite-asteroid connection. We propose a space mission to detect and characterize sub-kilometer asteroids between Jupiter and Venus. The mission is named "Bering" after the famous navigator and explorer Vitus Bering. A key feature of the mission is an advanced payload package, providing full on board autonomy of both object detection and tracking, which is required in order to study fast moving objects in deep space. The autonomy has the added advantage of reducing the cost of running the mission to a minimum, thus enabling science to focus on the main objectives. (c) 2005 Elsevier Ltd. All rights reserved.
引用
收藏
页码:966 / 973
页数:8
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