Oxo (crater)

{{Short description|Crater on Ceres}}

{{Use dmy dates|date=January 2025}}

{{Infobox feature on celestial object

|name = Oxo

|image = PIA20360 Oxo crater on Ceres (edited).jpg

|caption = Oxo imaged by Dawn from LAMO

|type = Impact crater

|location = Ceres

|coordinates= {{coord|42.21|N|359.6|E|globe:ceres_type:landmark|display=inline,title}}

|coordinates_footnotes = {{cite web|url=https://planetarynames.wr.usgs.gov/Feature/15383|website=planetarynames.wr.usgs.gov|title=Planetary Names: Crater, craters: Oxo on Ceres|access-date=2021-09-15}}

|length =

|width =

|diameter = {{convert|10|km|mi}}

|depth = {{convert|4802|m|ft}}

|area =

|dimensions =

|peak =

|discoverer = Dawn

|naming =

|eponym = After the Candomblé god of agriculture

}}

Oxo {{IPAc-en|ˈ|ɒ|ʃ|oʊ}} is a small impact crater on the dwarf planet Ceres. Located in Ceres's northern hemisphere, it is the second-brightest feature on Ceres, after Haulani Crater. The crater was named after the Candomblé (and Yoruba) god of agriculture.{{cite web|title=Planetary Names: Crater, craters: Oxo on Ceres|url=http://planetarynames.wr.usgs.gov/Feature/15383|website=Gazetteer of Planetary Nomenclature|date=21 September 2015}}

Formation

Oxo is a very young crater, having been formed only {{val|190|100|70}} ka (thousand years) ago,{{harvnb|Nathues|Platz|Hoffmann|Thangjam|2017|p=1}} and it is entirely located within the older, heavily degraded crater Duginavi.{{harvnb|Nathues|Platz|Hoffmann|Thangjam|2017|p=9}} 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.{{harvnb|Nathues|Platz|Hoffmann|Thangjam|2017|pp=3-4}}

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.{{harvnb|Nathues|Platz|Hoffmann|Thangjam|2017|p=3}}

Oxo is actively undergoing the sublimation of water ice, due to its young age. This ice is located along the crater's southern wall.{{harvnb|Formisano|Federico|Magni|Raponi|2018|p=2}}

See also

References

=Citations=

{{Reflist}}

=Bibliography=

{{refbegin}}

  • {{cite journal|title=Surface Temperatures and Water Ice Sublimation Rate of Oxo Crater: A Comparison With Juling Crater|journal=Journal of Geophysical Research: Planets|publisher=American Geophysical Union|last1=Formisano|first1=Michelangelo|last2=Federico|first2=Constanzo|last3=Magni|first3=Giacomo|last4=Raponi|first4=Andrea|date=10 December 2018|display-authors=et al|volume=124|issue=1|pages=2–13|doi=10.1029/2018JE005839|s2cid=133821860 |doi-access=free}}
  • {{cite journal|title=Oxo Crater on (1) Ceres: Geological History and the Role of Water-ice|journal=The Astronomical Journal|publisher=IOP Publishing|last1=Nathues|first1=Andreas|last2=Platz|first2=Thomas|last3=Hoffmann|first3=Susanne M.|last4=Thangjam|first4=Guneshwar|display-authors=et al|date=4 August 2017|volume=154|number=3|page=84 |doi=10.3847/1538-3881/aa7a04|hdl=10150/625818 |s2cid=55137098 |hdl-access=free |doi-access=free }}

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{{Ceres}}

{{Commons category-inline}}

Category:Impact craters on asteroids

Category:Surface features of Ceres

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