Water and carbon dioxide distribution in the 67P/Churyumov-Gerasimenko coma from VIRTIS-M infrared observations

Persistent Link:
http://hdl.handle.net/10150/614953
Title:
Water and carbon dioxide distribution in the 67P/Churyumov-Gerasimenko coma from VIRTIS-M infrared observations
Author:
Migliorini, A.; Piccioni, G.; Capaccioni, F.; Filacchione, G.; Bockelée-Morvan, D.; Erard, S.; Leyrat, C.; Combi, M. R.; Fougere, N.; Crovisier, J.; Taylor, F. W.; De Sanctis, M. C.; Capria, M. T.; Grassi, D.; Rinaldi, G.; Tozzi, G. P.; Fink, U.
Affiliation:
Univ Arizona, Lunar & Planetary Lab
Issue Date:
2016-04-12
Publisher:
EDP SCIENCES S A
Citation:
Water and carbon dioxide distribution in the 67P/Churyumov-Gerasimenko coma from VIRTIS-M infrared observations 2016, 589:A45 Astronomy & Astrophysics
Journal:
Astronomy & Astrophysics
Rights:
© ESO 2016
Collection Information:
This item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at repository@u.library.arizona.edu.
Abstract:
Context. Studying the coma environment of comet 67P/Churyumov-Gerasimenko (67P) is one of the primary scientific goals of the VIRTIS experiment on the ESA Rosetta mission. Aims. The distribution and variability of water vapour and carbon dioxide in the comet's coma are needed to estimate their production rate, abundances in the nucleus, and the spatial distribution of the active regions. Methods. Infrared emission lines from vibrational bands of water and carbon dioxide at 2.67 and 4.27 mu m, respectively, were observed by the VIRTIS-M imaging channel and mapped from close to the nucleus up to similar to 10 km altitude with a resolution of similar to 40 m/px. A dataset consisting of 74 observations in the 1 5 mu m spectral range acquired from 8 to 14 April 2015 when 67P was at a heliocentric distance of 1.9 AU is analysed in this work. A statistical correlation between the gas distribution and the surface's active regions was performed. Results. The maximum H2O emission is observed within 3 km from the nucleus and is mainly concentrated above two active regions, Aten-Babi and Seth-Hapi, while the CO2 distribution appears more uniform with significant emissions coming from both the "head" and southern latitude regions. In the equatorial region, the column densities of both species decrease with altitude, although CO2 decreases more rapidly than H2O. The calculated CO2/H2O column density ratios above Aten-Babi and Seth-Hapi are 2.4 +/- 0.6% and 3.0 +/- 0.7%, respectively. A value equal to 3.9 +/- 1.0% is observed at equatorial latitudes in the region encompassing Imothep. Conclusions. VIRTIS-M has mapped the distribution of water vapour and carbon dioxide around the nucleus of 67P with unprecedented spatial resolution. The different water and carbon dioxide outgassing above the surface, seen in the VIRTIS-M data, might be indicative of a different thermal history of the northern and southern hemispheres of 67P.
ISSN:
0004-6361; 1432-0746
DOI:
10.1051/0004-6361/201527661
Keywords:
comets: individual: 67P/CG; techniques: imaging spectroscopy
Version:
Final published version
Sponsors:
Italian Space Agency (ASI - Italy); Centre National d'Etudes Spatiales (CNES - France); Deutsches Zentrum fur Luftund Raumfahrt (DLR-Germany); National Aeronautic and Space Administration (NASA-USA); ASI; Observatoire de Meudon; CNES; DLR
Additional Links:
http://www.aanda.org/10.1051/0004-6361/201527661

Full metadata record

DC FieldValue Language
dc.contributor.authorMigliorini, A.en
dc.contributor.authorPiccioni, G.en
dc.contributor.authorCapaccioni, F.en
dc.contributor.authorFilacchione, G.en
dc.contributor.authorBockelée-Morvan, D.en
dc.contributor.authorErard, S.en
dc.contributor.authorLeyrat, C.en
dc.contributor.authorCombi, M. R.en
dc.contributor.authorFougere, N.en
dc.contributor.authorCrovisier, J.en
dc.contributor.authorTaylor, F. W.en
dc.contributor.authorDe Sanctis, M. C.en
dc.contributor.authorCapria, M. T.en
dc.contributor.authorGrassi, D.en
dc.contributor.authorRinaldi, G.en
dc.contributor.authorTozzi, G. P.en
dc.contributor.authorFink, U.en
dc.date.accessioned2016-06-29T01:00:42Z-
dc.date.available2016-06-29T01:00:42Z-
dc.date.issued2016-04-12-
dc.identifier.citationWater and carbon dioxide distribution in the 67P/Churyumov-Gerasimenko coma from VIRTIS-M infrared observations 2016, 589:A45 Astronomy & Astrophysicsen
dc.identifier.issn0004-6361-
dc.identifier.issn1432-0746-
dc.identifier.doi10.1051/0004-6361/201527661-
dc.identifier.urihttp://hdl.handle.net/10150/614953-
dc.description.abstractContext. Studying the coma environment of comet 67P/Churyumov-Gerasimenko (67P) is one of the primary scientific goals of the VIRTIS experiment on the ESA Rosetta mission. Aims. The distribution and variability of water vapour and carbon dioxide in the comet's coma are needed to estimate their production rate, abundances in the nucleus, and the spatial distribution of the active regions. Methods. Infrared emission lines from vibrational bands of water and carbon dioxide at 2.67 and 4.27 mu m, respectively, were observed by the VIRTIS-M imaging channel and mapped from close to the nucleus up to similar to 10 km altitude with a resolution of similar to 40 m/px. A dataset consisting of 74 observations in the 1 5 mu m spectral range acquired from 8 to 14 April 2015 when 67P was at a heliocentric distance of 1.9 AU is analysed in this work. A statistical correlation between the gas distribution and the surface's active regions was performed. Results. The maximum H2O emission is observed within 3 km from the nucleus and is mainly concentrated above two active regions, Aten-Babi and Seth-Hapi, while the CO2 distribution appears more uniform with significant emissions coming from both the "head" and southern latitude regions. In the equatorial region, the column densities of both species decrease with altitude, although CO2 decreases more rapidly than H2O. The calculated CO2/H2O column density ratios above Aten-Babi and Seth-Hapi are 2.4 +/- 0.6% and 3.0 +/- 0.7%, respectively. A value equal to 3.9 +/- 1.0% is observed at equatorial latitudes in the region encompassing Imothep. Conclusions. VIRTIS-M has mapped the distribution of water vapour and carbon dioxide around the nucleus of 67P with unprecedented spatial resolution. The different water and carbon dioxide outgassing above the surface, seen in the VIRTIS-M data, might be indicative of a different thermal history of the northern and southern hemispheres of 67P.en
dc.description.sponsorshipItalian Space Agency (ASI - Italy); Centre National d'Etudes Spatiales (CNES - France); Deutsches Zentrum fur Luftund Raumfahrt (DLR-Germany); National Aeronautic and Space Administration (NASA-USA); ASI; Observatoire de Meudon; CNES; DLRen
dc.language.isoenen
dc.publisherEDP SCIENCES S Aen
dc.relation.urlhttp://www.aanda.org/10.1051/0004-6361/201527661en
dc.rights© ESO 2016en
dc.subjectcomets: individual: 67P/CGen
dc.subjecttechniques: imaging spectroscopyen
dc.titleWater and carbon dioxide distribution in the 67P/Churyumov-Gerasimenko coma from VIRTIS-M infrared observationsen
dc.typeArticleen
dc.contributor.departmentUniv Arizona, Lunar & Planetary Laben
dc.identifier.journalAstronomy & Astrophysicsen
dc.description.collectioninformationThis item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at repository@u.library.arizona.edu.en
dc.eprint.versionFinal published versionen
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