Ceres: Sulfur deposits and graphitized carbon

Abstract We report new results from observations of the dwarf planet Ceres using the Hubble Space Telescope in the spectral range 1160–5700 Å. Comparisons between Ceres' UV‐visible spectra and laboratory measurements indicate that both sulfur species and graphitized carbon are important on Cere...

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Main Authors: Amanda R. Hendrix, Faith Vilas, Jian‐Yang Li
Format: Article
Language:English
Published: Wiley 2016-09-01
Series:Geophysical Research Letters
Subjects:
Online Access:https://doi.org/10.1002/2016GL070240
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author Amanda R. Hendrix
Faith Vilas
Jian‐Yang Li
author_facet Amanda R. Hendrix
Faith Vilas
Jian‐Yang Li
author_sort Amanda R. Hendrix
collection DOAJ
description Abstract We report new results from observations of the dwarf planet Ceres using the Hubble Space Telescope in the spectral range 1160–5700 Å. Comparisons between Ceres' UV‐visible spectra and laboratory measurements indicate that both sulfur species and graphitized carbon are important on Ceres' surface. We find a latitudinal gradient in UV absorption, with northern latitudes being more UV absorbing than southern latitudes, a trend that can be explained by increasing abundances of sulfur and SO2 toward northern latitudes. The presence of graphitized carbon is consistent with the surface of this airless body being carbonized in response to processes such as charged particle bombardment. The presence of volatile sulfur species is consistent with the idea that Ceres exhibits geothermal activity. Spectral differences with previous UV observations are likely due to the changing sulfurous and carbonaceous surface of Ceres.
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publishDate 2016-09-01
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series Geophysical Research Letters
spelling doaj-art-b58142b028194e5d82b47f60acf8f0b72025-08-20T01:52:04ZengWileyGeophysical Research Letters0094-82761944-80072016-09-0143178920892710.1002/2016GL070240Ceres: Sulfur deposits and graphitized carbonAmanda R. Hendrix0Faith Vilas1Jian‐Yang Li2Planetary Science Institute Tucson Arizona USAPlanetary Science Institute Tucson Arizona USAPlanetary Science Institute Tucson Arizona USAAbstract We report new results from observations of the dwarf planet Ceres using the Hubble Space Telescope in the spectral range 1160–5700 Å. Comparisons between Ceres' UV‐visible spectra and laboratory measurements indicate that both sulfur species and graphitized carbon are important on Ceres' surface. We find a latitudinal gradient in UV absorption, with northern latitudes being more UV absorbing than southern latitudes, a trend that can be explained by increasing abundances of sulfur and SO2 toward northern latitudes. The presence of graphitized carbon is consistent with the surface of this airless body being carbonized in response to processes such as charged particle bombardment. The presence of volatile sulfur species is consistent with the idea that Ceres exhibits geothermal activity. Spectral differences with previous UV observations are likely due to the changing sulfurous and carbonaceous surface of Ceres.https://doi.org/10.1002/2016GL070240dwarf planetCeres
spellingShingle Amanda R. Hendrix
Faith Vilas
Jian‐Yang Li
Ceres: Sulfur deposits and graphitized carbon
Geophysical Research Letters
dwarf planet
Ceres
title Ceres: Sulfur deposits and graphitized carbon
title_full Ceres: Sulfur deposits and graphitized carbon
title_fullStr Ceres: Sulfur deposits and graphitized carbon
title_full_unstemmed Ceres: Sulfur deposits and graphitized carbon
title_short Ceres: Sulfur deposits and graphitized carbon
title_sort ceres sulfur deposits and graphitized carbon
topic dwarf planet
Ceres
url https://doi.org/10.1002/2016GL070240
work_keys_str_mv AT amandarhendrix ceressulfurdepositsandgraphitizedcarbon
AT faithvilas ceressulfurdepositsandgraphitizedcarbon
AT jianyangli ceressulfurdepositsandgraphitizedcarbon