Statistical investigation of the amount of main belt asteroids larger than 1 km

Details Statistical investigation of the amount of main belt asteroids larger than 1 km Statistical investigation of the amount of main belt asteroids larger than 1 km

Nov 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002esasp.500..533e&link_type=abstract

In: Proceedings of Asteroids, Comets, Meteors - ACM 2002. International Conference, 29 July - 2 August 2002, Berlin, Germany. Ed

Statistics

Asteroids, Statistics

Scientific paper

A statistical investigation is made for estimating the total amount of main belt asteroids larger than 1 km. Starting from the well known investigation by van Houten et al. (1970), a comparison is made with the results recently obtained by ESA's Infrared Space Observatory, ISO (1996-1997). From this it seems that the asteroids in our Solar System (between Mars and Jupiter = main belt asteroids) may be more numerous than previously thought.

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