Literature DB >> 17801529

First images of asteroid 243 ida.

M J Belton, C R Chapman, J Veverka, K P Klaasen, A Harch, R Greeley, R Greenberg, J W Head, A McEwen, D Morrison, P C Thomas, M E Davies, M H Carr, G Neukum, F P Fanale, D R Davis, C Anger, P J Gierasch, A P Ingersoll, C B Pilcher.   

Abstract

The first images of the asteroid 243 Ida from Galileo show an irregular object measuring 56-kilometers by 24 kilometers by 21 kilometers. Its surface is rich in geologic features, including systems of grooves, blocks, chutes, albedo features, crater chains, and a full range of crater morphologies. The largest blocks may be distributed nonuniformly across the surface; lineaments and dark-floored craters also have preferential locations. Ida is interpreted to have a substantial regolith. The high crater density and size-frequency distribution (-3 differential power-law index) indicate a surface in equilibrium with saturated cratering. A minimum model crater age for Ida-and therefore for the Koronis family to which Ida belongs-is estimated at 1 billion years, older than expected.

Entities:  

Year:  1994        PMID: 17801529     DOI: 10.1126/science.265.5178.1543

Source DB:  PubMed          Journal:  Science        ISSN: 0036-8075            Impact factor:   47.728


  1 in total

1.  Shape, size and multiplicity of main-belt asteroids I. Keck Adaptive Optics survey.

Authors:  F Marchis; M Kaasalainen; E F Y Hom; J Berthier; J Enriquez; D Hestroffer; D Le Mignant; I de Pater
Journal:  Icarus       Date:  2006-11       Impact factor: 3.508

  1 in total

北京卡尤迪生物科技股份有限公司 © 2022-2023.