TY - GEN

T1 - The autonomous asteroid mapping mission "bering"

AU - Andersen, A. C.

AU - Michelsen, R.

AU - Haack, H.

AU - Jørgensen, J. L.

AU - Betto, M.

AU - Jørgensen, P. S.

PY - 2003/11/1

Y1 - 2003/11/1

N2 - 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. High-speed collisions between asteroids are gradually resulting in their break-up. The size distribution of kilometer-sized asteroids implies that the presently un-detected 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.

AB - 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. High-speed collisions between asteroids are gradually resulting in their break-up. The size distribution of kilometer-sized asteroids implies that the presently un-detected 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.

KW - Ephermerides

KW - Instrumentation: detectors, spectrographs

KW - Instruments

KW - Methods: observational

KW - Minor planets, asteroids

KW - Space vehicles

UR - http://www.scopus.com/inward/record.url?scp=0842332802&partnerID=8YFLogxK

M3 - Conference article

AN - SCOPUS:0842332802

SP - 307

EP - 312

JO - European Space Agency, (Special Publication) ESA SP

JF - European Space Agency, (Special Publication) ESA SP

SN - 0379-6566

IS - 542

T2 - Proceedings of the 5th IAA International Conference on Low-Cost Planetary Missions

Y2 - 24 September 2003 through 26 September 2003

ER -