Arecibo S-band radar program

Astronomy and Astrophysics – Astronomy

Scientific paper

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Mars (Planet), Moon, Radar Maps, Radar Reflectors, Superhigh Frequencies, Temporal Resolution, Venus (Planet), Deimos, Equatorial Regions, Galilean Satellites, Jupiter Satellites, Mercury (Planet), Phobos, Rangefinding, Solar System

Scientific paper

The high powered 12.6 cm wavelength radar on the 1000 ft Arecibo reflector is used for a variety of studies of solar system bodies. These include: (1) the radar mapping of the surfaces of Mercury, Venus, the moon and Mars in both senses (usually the two circulars) of received polarization; (2) high time resolution ranging measurements to Mercury and Mars to obtain height profiles and scattering parameters in the equatorial region and to test relativistic and gravitational theories; (3) measurements of the orbital parameters, scattering properties, figure and spin vectors of asteroids and comets; and (4) observations of the satellites of Mars, Phobos and Deimos, and the Galilean satellites of Jupiter.

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