Author
Listed:
- M. C. De Sanctis
(Istituto di Astrofisica e Planetologia Spaziali, INAF)
- E. Ammannito
(Istituto di Astrofisica e Planetologia Spaziali, INAF
Institute of Geophysics and Planetary Physics, University of California)
- A. Raponi
(Istituto di Astrofisica e Planetologia Spaziali, INAF)
- S. Marchi
(Istituto di Astrofisica e Planetologia Spaziali, INAF
Southwest Research Institute)
- T. B. McCord
(Bear Fight Institute)
- H. Y. McSween
(University of Tennessee)
- F. Capaccioni
(Istituto di Astrofisica e Planetologia Spaziali, INAF)
- M. T. Capria
(Istituto di Astrofisica e Planetologia Spaziali, INAF)
- F. G. Carrozzo
(Istituto di Astrofisica e Planetologia Spaziali, INAF)
- M. Ciarniello
(Istituto di Astrofisica e Planetologia Spaziali, INAF)
- A. Longobardo
(Istituto di Astrofisica e Planetologia Spaziali, INAF)
- F. Tosi
(Istituto di Astrofisica e Planetologia Spaziali, INAF)
- S. Fonte
(Istituto di Astrofisica e Planetologia Spaziali, INAF)
- M. Formisano
(Istituto di Astrofisica e Planetologia Spaziali, INAF)
- A. Frigeri
(Istituto di Astrofisica e Planetologia Spaziali, INAF)
- M. Giardino
(Istituto di Astrofisica e Planetologia Spaziali, INAF)
- G. Magni
(Istituto di Astrofisica e Planetologia Spaziali, INAF)
- E. Palomba
(Istituto di Astrofisica e Planetologia Spaziali, INAF)
- D. Turrini
(Istituto di Astrofisica e Planetologia Spaziali, INAF)
- F. Zambon
(Istituto di Astrofisica e Planetologia Spaziali, INAF)
- J.-P. Combe
(Bear Fight Institute)
- W. Feldman
(Planetary Science Institute)
- R. Jaumann
(Institute of Planetary Research, German Aerospace Center (DLR))
- L. A. McFadden
(NASA Goddard Space Flight Center)
- C. M. Pieters
(Environmental, and Planetary Sciences, Brown University)
- T. Prettyman
(Planetary Science Institute)
- M. Toplis
(Institut de Recherche d’Astrophysique et Planétologie, Observatoire Midi Pyrénées, Université)
- C. A. Raymond
(Jet Propulsion Laboratory, California Institute of Technology)
- C. T. Russell
(Institute of Geophysics and Planetary Physics, University of California)
Abstract
Infrared spectra of (1) Ceres acquired at distances of 82,000 to 4,300 kilometres from the surface indicate widespread ammoniated phyllosilicates; the presence of ammonia suggests that material from the outer Solar System was incorporated into Ceres.
Suggested Citation
M. C. De Sanctis & E. Ammannito & A. Raponi & S. Marchi & T. B. McCord & H. Y. McSween & F. Capaccioni & M. T. Capria & F. G. Carrozzo & M. Ciarniello & A. Longobardo & F. Tosi & S. Fonte & M. Formisa, 2015.
"Ammoniated phyllosilicates with a likely outer Solar System origin on (1) Ceres,"
Nature, Nature, vol. 528(7581), pages 241-244, December.
Handle:
RePEc:nat:nature:v:528:y:2015:i:7581:d:10.1038_nature16172
DOI: 10.1038/nature16172
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Citations
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Cited by:
- Yamei Li & Norio Kitadai & Yasuhito Sekine & Hiroyuki Kurokawa & Yuko Nakano & Kristin Johnson-Finn, 2022.
"Geoelectrochemistry-driven alteration of amino acids to derivative organics in carbonaceous chondrite parent bodies,"
Nature Communications, Nature, vol. 13(1), pages 1-14, December.
- A. Nathues & M. Hoffmann & N. Schmedemann & R. Sarkar & G. Thangjam & K. Mengel & J. Hernandez & H. Hiesinger & J. H. Pasckert, 2022.
"Brine residues and organics in the Urvara basin on Ceres,"
Nature Communications, Nature, vol. 13(1), pages 1-13, December.
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