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. Since the GSSR takes about 5 seconds to switch from transmit to receive, nearby targets must necessarily use bistatic mode. 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: Small asteroids appear only as unresolved points of light in ground-based optical telescopes. Radar, however, can image near-Earth asteroids and comets 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, most existing images of binary asteroids were obtained through radar astronomy. • Moons of Jupiter • Rings and moons of Saturn Toutatis.jpg|
4179 Toutatis in 1996 Asteroid 1999 JM8.gif|
(53319) 1999 JM8 in 1999 2005YU55-20111107.jpg|
(308635) 2005 YU55 in 2011 Upcoming asteroid observations can be found online at the Goldstone Asteroid Schedule. ==Other scientific uses==