Television pictures of Phobos: first results

Creators: Avanesov, G. A.; Bonev, B. I.; Kempe, F.; Bazilevskii, A. T.; Boicheva, V.; Wiede, G. -G.; Gromatikov, P.; Duxbury, T.; Danz, M.; Dimitrov, D.; Zhukov, B. S.; Ziman, Ya. L.; Kolev, V.; Kostenko, V. I.; Kottsov, V. A.; Krasavtsev, V. M.; Krasikov, V. A.; Krumov, A.; Kuz'min, A. A.; Losev, K. D.; Lumme, K.; Mohlmmann, D.; Murchie, S.; Mishev, D. N.; Muinonen, K.; Murav'ev, V. M.; Murray, B.; Neumann, W.; Paul, L.; Possel, W.; Petkov, D.; Petukhova, P.; Rebel, B.; Simeonov, S.; Smith, B.; Totev, A.; Uzunov, Yu.; Fedotov, V. P.; Halman, D.; Head, J.; Heifets, V. N.; Zapfe, H.; Chikov, K. N.; Shkuratov, Yu. G.

Abstract

In February-March 1989, 37 television images of the Martian satellite Phobos were obtained by the Phobos 2 spacecraft from distances of 200-1100 km. These images provide an important supplement to the TV data from the American Mariner 9 and Viking spacecraft in coverage of t4e surface of Phobos and in resolution in certain regions, in spectral range, and in range of phase angles. They make it possible to refine the figure and topographic and geological maps of the surface of Phobos, its spectral and angular reflective characteristics, the surface composition and texture, and characteristics of the orbital and librational motion.

Additional Information

© 1990 American Institute of Physics. Submitted September 4, 1989. In conclusion, we express our gratitude to all the specialists who took part in the preparation and execution of the television experiment.

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