Goldstone Solar System Radar

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Goldstone Solar System Radar
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The Goldstone Solar System Radar (GSSR) is a large radar system used for investigating objects in the Solar System, a field called radar astronomy. 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 DSS 14 antenna at the Goldstone Deep Space Communications Complex.[1] It has been used to investigate Mercury, Venus, Mars, the asteroids, and moons of Jupiter and Saturn.

The solar system radar is only active a small percentage of the time, as the 70 meter antenna is primarily used for tracking and communicating with spacecraft as part of the NASA Deep Space Network.

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. Since the GSSR takes about 5 seconds to switch from transmit to receive,[2] 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[3]
  • 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.[4][5]
  • Moons of Jupiter
  • Rings and moons of Saturn

Upcoming asteroid observations can be found online at the Goldstone Asteroid Schedule.[6]

Other scientific uses

Similar facilities

The GSSR is the only planetary radar in current regular operation.[8] Others are or were:

There are proposals and prototypes for possible additional radars:

  • The Green Bank Observatory is investigating a Ku-band radar for its 100 meter radio telescope.[11] Its low power prototype has imaged the moon.
  • China is developing a planetary radar.[12] Their initial phase has imaged the moon.

References

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  1. ^ Page Module:Citation/CS1/styles.css has no content.Latifiyan, Pouya (April 2021). "Space Telecommunications, how?". Take off (in Persian). 1. Tehran: Civil Aviation Technology College: 15.{{cite journal}}: CS1 maint: unrecognized language (link)
  2. ^ Page Module:Citation/CS1/styles.css has no content."Goldstone Solar System Radar (GSSR) Learning Manual" (PDF).
  3. ^ Page Module:Citation/CS1/styles.css has no content.Williams, Matt (4 May 2021). "How Long is a Day on Venus? We Finally Know the Exact Answer". Universe Today.
  4. ^ Page Module:Citation/CS1/styles.css has no content.Brozović, Marina; Benner, Lance A. M.; Giorgini, Jon D.; Naidu, Shantanu P.; Busch, Michael W.; Lawrence, Kenneth J.; Jao, Joseph S.; Lee, Clement G.; Snedeker, Lawrence G.; Silva, Marc A.; Slade, Martin A.; Chodas, Paul W. (27 December 2018). "Goldstone Radar Observations of Horseshoe-orbiting Near-Earth Asteroid 2013 BS45, a Potential Mission Target". The Astronomical Journal. 157 (1): 24. doi:10.3847/1538-3881/aaf04f. S2CID 126514636.
  5. ^ Page Module:Citation/CS1/styles.css has no content.Lawrence, Kenneth J.; Benner, Lance A.M.; Brozovic, Marina; Ostro, Steven J.; Jao, Joseph S.; Giorgini, Jon D.; Slade, Martin A.; Jurgens, Raymond F.; Nolan, Michael C.; Howell, Ellen S.; Taylor, Patrick A. (January 2018). "Arecibo and Goldstone radar images of near-Earth Asteroid (469896) 2005 WC1". Icarus. 300: 12–20. Bibcode:2018Icar..300...12L. doi:10.1016/j.icarus.2017.08.028.
  6. ^ Page Module:Citation/CS1/styles.css has no content."Goldstone Asteroid Schedule".
  7. ^ Page Module:Citation/CS1/styles.css has no content.David, Leonard (May 1999). "Saving SOHO" (PDF). Aerospace America. p. 66.
  8. ^ Page Module:Citation/CS1/styles.css has no content.Virkki, Anne K.; Neish, Catherine D.; Rivera-Valentín, Edgard G.; Bhiravarasu, Sriram S.; Hickson, Dylan C.; Nolan, Michael C.; Orosei, Roberto (2023). "Planetary radar—State-of-the-art review". Remote Sensing. 15 (23). MDPI: 5605. Bibcode:2023RemS...15.5605V. doi:10.3390/rs15235605.
  9. ^ Page Module:Citation/CS1/styles.css has no content.Evans, JV; Ingalls, RP; Pettengill, GH (1970). "The Haystack Planetary Ranging Radar". Technical Report-Jet Propulsion Laboratory, California Institute of Technology (32). Jet Propulsion Laboratory, California Institute of Technology: 27. Bibcode:1970sarr.conf...27E.
  10. ^ Page Module:Citation/CS1/styles.css has no content."BISTATIC RADAR TEST ACTIVITIES AT THE ITALIAN MEDICINA RADIOTELESCOPES" (PDF).
  11. ^ Page Module:Citation/CS1/styles.css has no content."The next generation planetary radar system on the Green Bank Telescope" (PDF).
  12. ^ Page Module:Citation/CS1/styles.css has no content."China begins construction on world's most far-reaching radar system, to boost defense against near-Earth asteroid impact".

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