Goldstone solar system radar

Details Goldstone solar system radar Goldstone solar system radar

Sep 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986plas.rept....5j&link_type=abstract

In NASA, Washington Reports of Planetary Astronomy, 1985 p 5-7 (SEE N87-12407 03-89)

Computer Science

Performance

Planetary Orbits, Planetary Rotation, Planetary Surfaces, Radar Astronomy, Terrestrial Planets, Computer Systems Performance, Data Processing, Remote Sensing, Space Exploration, Topography, Very Large Array (Vla)

Scientific paper

Information is provided about physical nature planetary surfaces and their topography as well as dynamical properties such as orbits and spin states using ground based radar as a remote sensing tool. Accessible targets are the terrestrial planets: the Earth's Moon, Mercury, Venus and Mars, the outer planets rings and major moons, and many transient objects such as asteroids and comets. Data acquisition utilizes the unique facilities of the Goldstone Deep Space Network, occasionally the Arecibo radar, and proposed use of the VLA (very large array).

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