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arXiv · astro-ph/0310430

Asteroid and NEA detection models

Rene Michelsen·Henning Haack·Anja C. Andersen·John L. Joergensen
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Abstract

We determine the possible detection rate of asteroids with the Bering mission. In particular we examine the outcome of the Bering mission in relation to the populations of Near-Earth Asteroids and main belt asteroids. This is done by constructing synthetic populations of asteroids, based on the current best estimates of the asteroid size-distributions. From the detailed information obtained from the simulations, the scientific feasibility of Bering is demonstrated and the key technical requirement for the scientific instruments on Bering is determined.

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Rene Michelsen, Henning Haack, Anja C. Andersen, John L. Joergensen. 2003-10-15. Asteroid and NEA detection models. https://arxiv.org/abs/astro-ph/0310430

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