Oxo (crater)
Formation
Oxo is a very young crater, having been formed only 190+100
−70 Ka (thousand years) ago, and it is entirely located within the older, heavily degraded crater Duginavi. Despite its relatively small size, the impact that created Oxo penetrated more deeply into Ceres than many larger craters, reaching a depth of 4,802 metres, and it excavated significant amounts of bright material that was distributed unevenly throughout the crater's ejecta blanket.
Physical features
As a result of Oxo's young age it has a very sharp crater rim and a well-defined ejecta blanket. It is also home to many large boulders; boulders produced by older craters have largely been destroyed by micrometeoroid impacts.
Oxo is actively undergoing the sublimation of water ice, due to its young age. This ice is located along the crater's southern wall.
See also
References
Citations
- ^ "Planetary Names: Crater, craters: Oxo on Ceres". planetarynames.wr.usgs.gov. Retrieved 2021-09-15.
- ^ "Planetary Names: Crater, craters: Oxo on Ceres". Gazetteer of Planetary Nomenclature. 21 September 2015.
- ^ Nathues et al. 2017, p. 1
- ^ Nathues et al. 2017, p. 9
- ^ Nathues et al. 2017, pp. 3–4
- ^ Nathues et al. 2017, p. 3
- ^ Formisano et al. 2018, p. 2
Bibliography
- Formisano, Michelangelo; Federico, Constanzo; Magni, Giacomo; Raponi, Andrea; et al. (10 December 2018). "Surface Temperatures and Water Ice Sublimation Rate of Oxo Crater: A Comparison With Juling Crater". Journal of Geophysical Research: Planets. 124 (1). American Geophysical Union: 2–13. doi:10.1029/2018JE005839. S2CID 133821860.
- Nathues, Andreas; Platz, Thomas; Hoffmann, Susanne M.; Thangjam, Guneshwar; et al. (4 August 2017). "Oxo Crater on (1) Ceres: Geological History and the Role of Water-ice". The Astronomical Journal. 154 (3). IOP Publishing: 84. doi:10.3847/1538-3881/aa7a04. hdl:10150/625818. S2CID 55137098.
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