A dataset provided by the European Space Agency

Name DDT_mkuepper_1
Title Confirming an following up on the detection of water vapour from Ceres
URL

http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342254428&instrument_name=HIFI&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342266018&instrument_name=HIFI&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342266019&instrument_name=HIFI&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342266020&instrument_name=HIFI&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342266021&instrument_name=HIFI&product_level=LEVEL0&compress=true

DOI 10.5270/esa-1hdtt7i
Author kuppers, m.
Description The question of dwarf planet Ceres potentially being water rich is highly important for solar system science. A Herschel observation on 11 Oct. showed a clear detection of water absorption in Ceres spectrum, but only in H polarisation. An immediate reobservation is here requested.
Publication Herschel celestial calibration sources. Four large main-belt asteroids as prime flux calibrators for the far-IR-sub-mm range . Müller Thomas et al. . Experimental Astronomy, Volume 37, Issue 2, pp.253-330 . 37 . 10.1007\/s10686-013-9357-y . 2014ExA....37..253M ,
Localized sources of water vapour on the dwarf planet (1)Ceres . Küppers Michael et al. . Nature, Volume 505, Issue 7484, pp. 525-527 (2014). . 505 . 10.1038\/nature12918 . 2014Natur.505..525K ,
Thermal Stability of Water Ice in Ceres. Craters: The Case of Juling Crater . Formisano M. et al. . Journal of Geophysical Research: Planets, Volume 123, Issue 9, pp. 2445-2463 . 123 . 10.1029\/2017JE005417 . 2018JGRE..123.2445F ,
Surface Temperatures and Water Ice Sublimation Rate of Oxo Crater: A Comparison With Juling Crater . Formisano M. et al. . Journal of Geophysical Research: Planets, Volume 124, Issue 1, pp. 2-13 . 124 . 10.1029\/2018JE005839 . 2019JGRE..124....2F ,
Instrument HIFI_HifiPoint_dbs
Temporal Coverage 2012-10-24T19:54:52Z/2013-03-06T13:07:56Z
Version SPG v14.1.0
Mission Description Herschel was launched on 14 May 2009! It is the fourth 'cornerstone' mission in the ESA science programme. With a 3.5 m Cassegrain telescope it is the largest space telescope ever launched. It is performing photometry and spectroscopy in approximately the 55-671 µm range, bridging the gap between earlier infrared space missions and groundbased facilities.
Creator Contact https://support.cosmos.esa.int/herschel/
Date Published 2013-09-06T10:35:13Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2013-09-06T10:35:13Z, DDT_mkuepper_1, SPG v14.1.0. https://doi.org/10.5270/esa-1hdtt7i