Loading
  • 21 Aug, 2019

  • By, Wikipedia

Tirawa (crater)

Tirawa is the largest impact basin on Saturn's moon Rhea. It was glimpsed by Voyager 1 during its flyby of the moon and later photographed in greater detail by the Cassini orbiter. Tirawa is elongated in shape and overlaps Mamaldi, a larger and more degraded basin to its southwest.

Observation and naming

Tirawa was first observed by the Voyager 1 as it captured imagery of Rhea during its flyby of the Saturn system on 13 November 1980. Though poorly imaged from the Voyager 1 encounter, Tirawa was identified as an impact structure by 1983 and provisionally named Basin A. Tirawa was later named after the primary deity in Pawnee mythology, Tirawa; the name was officially approved by the International Astronomical Union (IAU) in 1987. Tirawa was later observed in greater detail by the Cassini orbiter in multiple flybys of Rhea throughout the late 2000's and the 2010's.

Geology

With a rough diameter of 350 kilometers, Tirawa is the largest identified impact structure on Rhea. Tirawa is a peak-ring impact basin, with a degraded inner ring of ridges and plateaus roughly 180 kilometers across. Individual ridges in the peak ring are typically ~50 kilometers across at their base and rise 1–3 kilometers above the basin floor. Tirawa is slightly elongated into an ellipsoid, with an a/b ratio of ~0.9, indicating that it was created in a low-angle oblique impact. Based on the crater counting method, Tirawa is about 4 billion years old.

The impact event that created Tirawa ejected massive amounts of material, with up to ~15-20% of the material ejected at speeds exceeding Rhea's escape velocity. Any such impact ejecta would've escaped Rhea's influence entirely, directly orbiting Saturn. Some of the ejecta later impacted Rhea, likely accounting for a large amount of Rhea's small craters.

See also

  • Odysseus – An impact basin on Tethys that is analogous to Tirawa in size and structure

References

  1. ^ "Tirawa". Gazetteer of Planetary Nomenclature. USGS Astrogeology Research Program. (Center Latitude: 34.20°, Center Longitude: 151.70°; Planetographic, +West)
  2. ^ Moore, Jeffrey M.; Schenk, Paul M.; Bruesch, Lindsey S.; Asphaug, Erik; McKinnon, William B. (October 2004). "Large impact features on middle-sized icy satellites". Icarus. 171 (2): 421–443. Bibcode:2004Icar..171..421M. doi:10.1016/j.icarus.2004.05.009.
  3. ^ Wagner, R. J.; Neukum, G.; Giese, B.; Roatsch, T.; Wolf, U. (March 2007). The Global Geology of Rhea: Preliminary Implications from the Cassini ISS Data (PDF). 38th Lunar and Planetary Science Conference. The Woodlands, Texas, United States. 1958. Archived (PDF) from the original on 3 March 2016. Retrieved 22 January 2008.
  4. ^ Moore, J. M.; Horner, V. M.; Greeley, R. (February 1985). "The geomorphology of RHEA - Implications for geologic history and surface processes". Journal of Geophysical Research. 90: C785–C795. Bibcode:1985LPSC...15..785M.
  5. ^ Leliwa-Kopystynski, Jacek; Banaszek, Marcin; Wlodarczyk, Ireneusz (January 2012). "Longitudinal asymmetry of craters' density distributions on the icy satellites". Planetary and Space Science. 60 (1): 181–192. Bibcode:2012P&SS...60..181L. doi:10.1016/j.pss.2011.08.002.