67P/Churyumov-Gerasimenko, a Jupiter family comet with a high D/H ratio
dc.contributor.author | Altwegg, K. | |
dc.contributor.author | Balsiger, H. | |
dc.contributor.author | Bar-Nun, A. | |
dc.contributor.author | Berthelier, J.J. | |
dc.contributor.author | Bieler, A. | |
dc.contributor.author | Bochsler, P. | |
dc.contributor.author | Briois, C. | |
dc.contributor.author | Calmonte, U. | |
dc.contributor.author | Combi, M. | |
dc.contributor.author | De Keyser, J. | |
dc.contributor.author | Eberhardt, P. | |
dc.contributor.author | Fiethe, B. | |
dc.contributor.author | Fuselier, S. | |
dc.contributor.author | Gasc, S. | |
dc.contributor.author | Gombosi, T.I. | |
dc.contributor.author | Hansen, K.C. | |
dc.contributor.author | Hassig, M. | |
dc.contributor.author | Jackel, A. | |
dc.contributor.author | Kopp, E. | |
dc.contributor.author | Korth, A. | |
dc.contributor.author | LeRoy, L. | |
dc.contributor.author | Mall, U. | |
dc.contributor.author | Marty, B. | |
dc.contributor.author | Mousis, O. | |
dc.contributor.author | Neefs, E. | |
dc.contributor.author | Owen, T. | |
dc.contributor.author | Reme, H. | |
dc.contributor.author | Rubin, M. | |
dc.contributor.author | Semon, T. | |
dc.contributor.author | Tzou, C.-T. | |
dc.contributor.author | Wait, H. | |
dc.contributor.author | Wurz, P. | |
dc.date | 2015 | |
dc.date.accessioned | 2016-03-24T12:08:14Z | |
dc.date.available | 2016-03-24T12:08:14Z | |
dc.identifier.uri | https://orfeo.belnet.be/handle/internal/2790 | |
dc.description | The provenance of water and organic compounds on Earth and other terrestrial planets has been discussed for a long time without reaching a consensus. One of the best means to distinguish between different scenarios is by determining the deuterium-to-hydrogen (D/H) ratios in the reservoirs for comets and Earth’s oceans. Here, we report the direct in situ measurement of the D/H ratio in the Jupiter family comet 67P/Churyumov-Gerasimenko by the ROSINA mass spectrometer aboard the European Space Agency’s Rosetta spacecraft, which is found to be (5.3 ± 0.7) × 10−4—that is, approximately three times the terrestrial value. Previous cometary measurements and our new finding suggest a wide range of D/H ratios in the water within Jupiter family objects and preclude the idea that this reservoir is solely composed of Earth ocean–like water. | |
dc.language | eng | |
dc.title | 67P/Churyumov-Gerasimenko, a Jupiter family comet with a high D/H ratio | |
dc.type | Article | |
dc.subject.frascati | Natural sciences | |
dc.audience | Scientific | |
dc.source.title | Science | |
dc.source.volume | 347 | |
dc.source.issue | 6220 | |
dc.source.page | 1261952 | |
Orfeo.peerreviewed | Yes | |
dc.identifier.doi | 10.1126/science.1257377 |