On the shapes and spins of “rubble pile” asteroids
✍ Scribed by Alan W. Harris; Eugene G. Fahnestock; Petr Pravec
- Publisher
- Elsevier Science
- Year
- 2009
- Tongue
- English
- Weight
- 811 KB
- Volume
- 199
- Category
- Article
- ISSN
- 0019-1035
No coin nor oath required. For personal study only.
✦ Synopsis
pioneered the field of radar astronomy, particularly in exploring near-Earth asteroids and the methods of inversion of both radar and optical data to obtain shape models of irregular bodies. Without such tools we would not have detailed "images" of asteroids and binary systems that provide the essential input for the modeling in Sections 2 and 4 of this paper. Anyone who has co-authored a paper with Steve is aware, sometimes painfully so, of his insistence on rigorous analysis, and that it is at least as important to explore and define what one cannot say from the data, as it is to present what one can say. It is in this spirit that we present Section 3 of this paper.
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A relation between the radii arid rotation ratcs of S-type asteroids is discussed. According to this relation these objects do not rotate with the same spin rate. Ausgehend voii radionietrisch bestimmten Durchmesserii wird eine der Aimahme glcicher Rotationsgeschwipdigkeitcn widersprechende Beziehu