| タイトル | Radar studies of the planets |
| 本文（外部サイト） | http://hdl.handle.net/2060/19740024146 |
| 著者（英） | Sebring, P. B.; Ingalls, R. P.; Rogers, A. E. E.; Pettengill, G. H.; Shapiro, I. I. |
| 著者所属（英） | Northeast Radio Observatory Corp. |
| 発行日 | 1974-08-29 |
| 言語 | eng |
| 内容記述 | The radar measurements phase of the lunar studies involving reflectivity and topographic mapping of the visible lunar surface was ended in December 1972, but studies of the data and production of maps have continued. This work was supported by Manned Spacecraft Center, Houston. Topographic mapping of the equatorial regions of Mars has been carried out during the period of each opposition since that of 1967. The method comprised extended precise traveling time measurements to a small area centered on the subradar point. As measurements continued, planetary motions caused this point to sweep out extensive areas in both latitude and longitude permitting the development of a fairly extensive topographical map in the equatorial region. Radar observations of Mercury and Venus have also been made over the past few years. Refinements of planetary motions, reflectivity maps and determinations of rotation rates have resulted. |
| NASA分類 | SPACE SCIENCES |
| レポートNO | 74N32259
NASA-CR-139580 |
| 権利 | No Copyright |
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