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Ahuna Mons[2] /əˈhnə ˈmɒnz/ is the largest mountain on the dwarf planet and asteroid Ceres. It protrudes above otherwise smooth terrain, it is not an impact feature, and it appears to be the only mountain of its kind on Ceres. Bright streaks run top to bottom on its slopes; these streaks are thought to be salt, similar to the better known Cererian bright spots,[3] and likely resulted from cryovolcanic activity from Ceres's interior.[4] It is named after the traditional post-harvest festival Ahuna of the Sumi Naga people of India.

Ahuna Mons
Lone conical mountain on Ceres from HAMO.jpg
The mountain imaged by the Dawn spacecraft. North is down.
Pronunciation /əˈhnə ˈmɒnz/
Location Ceres
Coordinates 10°28′S 315°48′E / 10.46°S 315.8°E / -10.46; 315.8Coordinates: 10°28′S 315°48′E / 10.46°S 315.8°E / -10.46; 315.8
Peak about 4 km (2 mi or 13,000 ft) high[1]
Discoverer Dawn spacecraft team
2015
Eponym Ahuna, harvest festival of the Sumi Naga from India.

Contents

DiscoveryEdit

The mountain was discovered on images taken by the Dawn spacecraft in orbit around Ceres in 2015.[5] It is estimated to have an average height of about 4 km (2.5 mi; 13,000 ft) and a maximum height of about 5 km (3.1 mi; 16,000 ft) on its steepest side; it is about 20 km (12 mi; 66,000 ft) wide at the base.[1]

OriginEdit

It has been proposed that Ahuna Mons formed as a cryovolcanic dome.[6][7] It is the closest cryovolcano to the Sun yet discovered in the Solar System.[8] It is roughly antipodal to the largest impact basin on Ceres, 280 km (170 mi) diameter Kerwan. Seismic energy from the Kerwan-forming impact may have been focused on the opposite side of Ceres, fracturing the outer layers of the area and facilitating the movement of high viscosity cryovolcanic magma (consisting of muddy water ice softened by its content of salts) that was then extruded onto the surface. Crater counts suggest that formation of the mountain continued into the last several hundred million years, making this a relatively young geological feature.[7]

GalleryEdit

 
Computer-generated image of Ahuna Mons
Elevation exaggerated by two (1 September 2016).
Overhead view
Side view
Overhead view
Side view
3D view

AnimationsEdit

Ceres flyover animations
Surface features exaggerated
(simulated; 01:15; 8 June 2015)[9]
Flight over dwarf planet Ceres
(color; 03:43; 29 January 2016)

See alsoEdit

ReferencesEdit

  1. ^ a b "PIA20348: Ahuna Mons Seen from LAMO". Jet Propulsion Lab. 7 March 2016. Retrieved 2016-04-14. 
  2. ^ Gazetteer of Planetary Nomenclature – Ahuna Mons
  3. ^ Stone, Maddie (October 1, 2015). "Ceres' Mysterious Bright Spots Aren't Made of Ice After All". Gizmodo. Retrieved 2016-03-25. 
  4. ^ Burnham, Robert (December 15, 2015). "Deep freeze puts the squeeze on dwarf planet Ceres". Arizona State University. Retrieved 2016-03-25. 
  5. ^ "NASA spies 3-mile-tall 'pyramid,' more bright spots on Ceres". Cnet. 17 June 2015. Retrieved 2015-06-19. 
  6. ^ Skibba, R. (2016-09-01). "Giant ice volcano spotted on dwarf planet Ceres". Nature. doi:10.1038/nature.2016.20526. 
  7. ^ a b Ruesch, O.; Platz, T.; Schenk, P.; McFadden, L. A.; Castillo-Rogez, J. C.; Quick, L. C.; Byrne, S.; Preusker, F.; OBrien, D. P.; Schmedemann, N.; Williams, D. A.; Li, J.- Y.; Bland, M. T.; Hiesinger, H.; Kneissl, T.; Neesemann, A.; Schaefer, M.; Pasckert, J. H.; Schmidt, B. E.; Buczkowski, D. L.; Sykes, M. V.; Nathues, A.; Roatsch, T.; Hoffmann, M.; Raymond, C. A.; Russell, C. T. (2016-09-02). "Cryovolcanism on Ceres". Science. 353 (6303): aaf4286–aaf4286. Bibcode:2016Sci...353.4286R. doi:10.1126/science.aaf4286. 
  8. ^ "THE MYSTERY OF AHUNA MONS, THE LONELY ICE VOLCANO". States News Service. 23 January 2017. Retrieved 12 February 2017 – via Gale. 
  9. ^ Landau, Elizabeth; Dyches, Preston (8 June 2015). "Fly Over Ceres in New Video". NASA. Retrieved 9 June 2015. 

External linksEdit