4.6 Article

A HERSCHEL STUDY OF D/H IN WATER IN THE JUPITER-FAMILY COMET 45P/HONDA-MRKOS-PAJDUSAKOVA AND PROSPECTS FOR D/H MEASUREMENTS WITH CCAT

期刊

ASTROPHYSICAL JOURNAL LETTERS
卷 774, 期 1, 页码 -

出版社

IOP PUBLISHING LTD
DOI: 10.1088/2041-8205/774/1/L3

关键词

comets: general; comets: individual (45P/Honda-Mrkos-Pajdusakova); molecular processes; submillimeter: planetary systems

资金

  1. NASA through JPL/Caltech
  2. NSF [AST-1108686]
  3. NASA [NNX12AH91H]
  4. Polish MNiSW [181/N-HSO/2008/0]
  5. Direct For Mathematical & Physical Scien
  6. Division Of Astronomical Sciences [1118243] Funding Source: National Science Foundation

向作者/读者索取更多资源

We present Herschel observations of water isotopologues in the atmosphere of the Jupiter-family comet 45P/Honda-Mrkos-Pajdusakova. No HDO emission is detected, with a 3 sigma upper limit of 2.0 x 10(-4) for the D/H ratio. This value is consistent with the earlier Herschel measurement in the Jupiter-family comet 103P/Hartley 2. The canonical value of 3 x 10(-4) measured pre-Herschel in a sample of Oort-cloud comets can be excluded at a 4.5 sigma level. The observations presented here further confirm that a diversity of D/H ratios exists in the comet population and emphasize the need for additional measurements with future ground-based facilities, such as CCAT, in the post-Herschel era.

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