Bright spots on Ceres

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Multiple bright spots in Occator crater stand out against the dark surface

Several bright surface features (also known as faculae) were discovered on the dwarf planet Ceres by the Dawn spacecraft in 2015.

The brightest cluster of spots ("Spot 5") is located in an 80-kilometer (50 mi) crater called Occator.[1][2] The largest and brightest component of the cluster is in the center of the crater, with dimmer spots located towards this crater's eastern rim. Early in the orbital phase of the Dawn mission, the high albedo of these spots was speculated to be due to some kind of outgassing,[3] and subsequent closer images helped scientists determine that it is material with a high level of reflection, and suggested ice and salt as possibilities.[4] These bright features have an albedo of about 40%, four times brighter than the average of Ceres's surface.[5]

On 9 December 2015, scientists reported that the bright spots on Ceres may be related to a type of salt, particularly a form of brine containing hydrated magnesium sulfate (MgSO4·6H2O); the spots were also found to be associated with ammonia-rich clays.[6]

Map of bright spots on Ceres (released 10 December 2015).

Arizona State University scientists have proposed that the bright spots are best explained as resulting from briny water erupted from Ceres' interior that subsequently sublimated, leaving behind only the salt deposits. [7]

Spot 5

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The brightest cluster of spots ("Spot 5") is located in an 80-kilometer (50 mi) crater called Occator,[1][2] which is located at 19.86° N latitude; 238.85 E longitude.[1][2]

File:Ceres Dawn Feb19 2015 bright spot frames.jpg
Spots on Ceres from different angles

Alan Duffy of Swinburne University suggested "a meteorite strike either shook covering material off the salty ice or heated it so that salty water rose to the surface as a geyser. The water escaped into space and now, only the salt remains."[8] A haze that fills around half of Occator crater and that does not extend over its rim[9] periodically appears around Spot 5, the best known bright spot, adding credence to the idea that some sort of outgassing or volcanism is occurring.[10][11]

Dawn's images led to widespread reports in the media about the bright spots, including in news sources,[12] astronomy magazines,[13] and science magazines.[14] An informal NASA poll during May offered the following ideas for the nature of the spots:[15] ice, volcanos, geysers, salt deposits, rock, or other.[16]

Asteroid specialist A. Rivkin noted, in an article by Sky & Telescope magazine, that at low angles a haze can be seen in but not outside of the crater, and speculated that this could be sublimated vapor from ice, possibly linked to the bright spots.[17]

Reflectivity studies from September 2015 suggest that the spots are probably salts rather than ice, implying that Ceres's interior is somehow delivering fresh salt to the surface.[18]

"Spot 5" in Occator Crator - Close-up (enhanced color; LAMO; February 2016)
"Spot 5" in Occator crater
from 4,400 km (2,700 mi)
"Spot 5" in Occator crater
from 4,400 km (2,700 mi)
"Spot 5" in Occator crater
from 1,450 km (900 mi) HAMO
"Spot 5" in Occator crater
from 385 km (239 mi) LAMO

Spot 1

"Spot 1" in Haulani crater (enhanced color; LAMO; April 2016)
Haulani from LAMO

Planned observations

Dawn's closest orbit around Ceres is at a distance of 375 km (233 mi), started in early December 2015. This low-altitude mapping orbit (LAMO) is designed to acquire data for at least three months with Dawn's gamma-ray and neutron detector (GRaND) for gravity investigation and to determine the chemical composition on and near the surface.[19][4]

Gallery

2003 image from the Hubble Space Telescope showing a bright area on Ceres.
Bright spots were most apparent to Dawn during approach
(12 February 2015)
Dawn images (cropped) of bright spots on Ceres
Bright "Spot 1" in Haulani crater
from 4,400 km (2,700 mi)
(17 June 2015)
Bright spots on walls of a crater northeast of Toharu crater(?) (Context)
(6 June 2015)
Bright spot near Ahuna Mons, the tallest mountain on Ceres, whose north face also features bright material - north is up
(6 June 2015)
Bright "Spot 5" in Occator crater
Elevations: brown=high; blue=low
(30 September 2015)
Bright "Spot 5" in Occator crater
Elevations: red=high; green=low
(28 July 2015)[20]
Bright "Spot 5" from 13,600 km (8,500 mi)
(4 May 2015)
Ceres – dwarf planet
PIA19316-Ceres-DwarfPlanet-DawnMission-VIR-20150413.jpg
Bright spots on Ceres in visible and infrared:
"Spot 1" (top row) (cooler than surroundings);
"Spot 5" (bottom) (similar in temperature to surroundings) (April 2015).

See also

References

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  2. 2.0 2.1 2.2 Lua error in package.lua at line 80: module 'strict' not found.
  3. LPSC 2015: First results from Dawn at Ceres: provisional place names and possible plumes
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  5. Lua error in package.lua at line 80: module 'strict' not found.
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  7. https://asunow.asu.edu/20151215-deep-freeze-puts-squeeze-dwarf-planet-ceres
  8. A. Duffy – Cosmos – What on Ceres are those bright spots?
  9. Chris Russel at [1]
  10. Lua error in package.lua at line 80: module 'strict' not found.
  11. Dawn at Ceres: A haze in Occator crater? Posted by Andrew Rivkin
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  17. Sky and Telescope magazine - Dawn Sees Ceres Bright Spots and More By Emily Poore July 30, 2015
  18. Ceres' Mysterious Bright Spots Aren't Made of Ice After All. Gizmodo, 1 October 2015
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External links