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The Goldstone Solar System Radar, or GSSR, is a large radar system used for investigating objects in the Solar system. Located in the desert near Barstow, California, it comprises a 500-kW X-band (8500 MHz) transmitter and a low-noise receiver on the 70-m antenna at the Goldstone Deep Space Communications Complex. It has been used to investigate Mercury, Venus, (), the asteroids, and moons of Jupiter and Saturn. The most comparable facility is the radar at Arecibo Observatory. ==Planetary observations== GSSR can work in two different modes. In the monostatic radar mode, GSSR both transmits and receives. In bistatic mode, GSSR transmits and other radio astronomy facilities receive. Although more difficult to schedule, this offers two advantages - the transmitter does not need to turn off to allow the receiver to listen, and it allows the use of interferometry to extract more information from the reflected signal. Bodies that have been investigated using GSSR include: *Mercury: In particular, by watching specific reflected features of Mercury sweep across the Earth's surface (using spatially separated receivers), GSSR enables the pole position to be computed quite accurately. The measured librations show Mercury has a liquid core. *Venus *Mars: GSSR was used extensively to characterize sites for Mars landers. *Asteroids: Asteroids appear only as unresolved points of light in ground-based optical telescopes. Radar, however, can image near-Earth asteroids with a resolution of several meters. For example, the asteroid 4179 Toutatis was imaged in 1992, 1996, 2000, 2004, 2008, and 2012. Although spacecraft such as Dawn can image particular asteroids in much finer detail, radar astronomy can investigate many more asteroids of different characteristics. For example, all existing images of binary asteroids were obtained through radar astronomy. *Moons of Jupiter *Rings and moons of Saturn 抄文引用元・出典: フリー百科事典『 ウィキペディア（Wikipedia）』 ■ウィキペディアで「Goldstone Solar System Radar」の詳細全文を読む スポンサード リンク
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