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Catalogue POP – Notice individuelle de publication

Küppers Michael, O'Rourke Laurence, Bockelée-Morvan Dominique, Zakharov Vladimir, Lee Seungwon, Allmen Paul von, Carry Benoît, Teyssier David, Marston Anthony, Müller Thomas G., Crovisier Jacques, Barucci Maria Antonella, Moreno Raphaël

Localized sources of water vapour on the dwarf planet (1)Ceres

Nature, 2014, vol. 505, pp. 525-527

Référence DOI : 10.1038/nature12918
Référence ADS : 2014Natur.505..525K

Résumé :

The `snowline' conventionally divides Solar System objects into dry bodies, ranging out to the main asteroid belt, and icy bodies beyond the belt. Models suggest that some of the icy bodies may have migrated into the asteroid belt. Recent observations indicate the presence of water ice on the surface of some asteroids, with sublimation a potential reason for the dust activity observed on others. Hydrated minerals have been found on the surface of the largest object in the asteroid belt, the dwarf planet (1)Ceres, which is thought to be differentiated into a silicate core with an icy mantle. The presence of water vapour around Ceres was suggested by a marginal detection of the photodissociation product of water, hydroxyl (ref. 12), but could not be confirmed by later, more sensitive observations. Here we report the detection of water vapour around Ceres, with at least 10<SUP>26</SUP> molecules being produced per second, originating from localized sources that seem to be linked to mid-latitude regions on the surface. The water evaporation could be due to comet-like sublimation or to cryo-volcanism, in which volcanoes erupt volatiles such as water instead of molten rocks.

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