Mariner 9 television observations of Phobos and Deimos
Icarus
By: James B. Pollack, J. Veverka, M. Noland, C. Sagan, W.K. Hartmann, T. C. Duxbury, G.H. Born, D. J. Milton, and B.A. Smith
Links
- More information: Publisher Index Page (via DOI)
- Download citation as: RIS | Dublin Core
Abstract
Mariner 9 photographs of Phobos and Deimos have yielded new information about the orbits, rotation periods, sizes, shapes, and surface characteristics of the satellites. Both satellites appear to be in synchronous rotation. They are irregular, heavily cratered bodies whose shapes appear to have been determined largely by impact fragmentation and spalling. The surfaces of both satellites have crater densities close to saturation and nearly identical, very low albedos. Lower limits on the tensile and yield strengths are estimated, and it is concluded that both satellites may consist of well-consolidated, though possibly highly fractured material.
| Publication type | Article |
|---|---|
| Publication Subtype | Journal Article |
| Title | Mariner 9 television observations of Phobos and Deimos |
| Series title | Icarus |
| DOI | 10.1016/0019-1035(72)90007-3 |
| Volume | 17 |
| Issue | 2 |
| Year Published | 1972 |
| Language | English |
| Publisher | Elsevier |
| Description | 14 p. |
| First page | 394 |
| Last page | 407 |
| Google Analytic Metrics | Metrics page |