The DOI matches its Crossref record; 28 of the 28 references it cites were found in a registry or an index.
Geophysical evolution of the Themis family parent body
Open accessAbstract
We model the geophysical evolution of the Themis family parent body. This study is motivated by the recent detection of water ice at the surface of 24 Themis, the first detection of free water on the surface of an asteroid. The Themis family members display a variety of spectral properties and densities, a possible indication that their parent was differentiated at the time of break‐up. Differentiation of the parent body is better explained if it accreted as a mixture of ice within a few My after the production of CAIs. From these models we highlight a number of issues that provide a strong rationale for further ground‐based and future space exploration of that family.
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“Depending on the extent of hydrothermal activity, water on an asteroid may be consumed by water-rock reactions, or some of it may remain in a thin outer layer enriched in water, hydrates, and organics (Castillo-Rogez and Schmidt, 2010).”
From The Astrobiology Primer v2.0 (2016) · cites this paper as Castillo-Rogez and Schmidt, 2010
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Cites
Morbidelli, A., Bottke, W. F., Nesvorný, D., & Levison, H. F. (2009) · Icarus · doi:10.1016/j.icarus.2009.07.011 · Cited by 528
Asteroid Density, Porosity, and Structure
Britt, D. T., Yeomans, D., Housen, K., & Consolmagno, G. (2002) · Asteroids III · doi:10.2307/j.ctv1v7zdn4.37 · Cited by 471
Detection of ice and organics on an asteroidal surface
Rivkin, A. S., & Emery, J. P. (2010) · Nature · doi:10.1038/nature09028 · Cited by 364
Water ice and organics on the surface of the asteroid 24 Themis
Campins, H., Hargrove, K., Pinilla-Alonso, N., Howell, E. S., Kelley, M. S., Licandro, J., Mothé-Diniz, T., Fernández, Y., & Ziffer, J. (2010) · Nature · doi:10.1038/nature09029 · Cited by 356
Water and the thermal evolution of carbonaceous chondrite parent bodies
Grimm, R. E., & Mcsween, H. Y. (1989) · Icarus · doi:10.1016/0019-1035(89)90038-9 · Cited by 335
Ceres’ evolution and present state constrained by shape data
Castillo-Rogez, J. C., & McCord, T. B. (2010) · Icarus · doi:10.1016/j.icarus.2009.04.008 · Cited by 210
Self-citationThe Lifetime of Ice on Main Belt Asteroids
Schörghofer, N. (2008) · The Astrophysical Journal · doi:10.1086/588633 · Cited by 210
Models of Twenty Asteroids from Photometric Data
Kaasalainen, M., Torppa, J., & Piironen, J. (2002) · Icarus · doi:10.1006/icar.2002.6907 · Cited by 157
Collisional Evolution of Asteroid Families
Marzari, F. (1995) · Icarus · doi:10.1006/icar.1995.1014 · Cited by 140
The water regime of asteroid (1) Ceres
Fanale, F. P., & Salvail, J. R. (1989) · Icarus · doi:10.1016/0019-1035(89)90026-2 · Cited by 127
Research works printed but not linked: 2
- Lopez Garcia A., 1997, Proceedings of IAU Colloquium
- Zappala V., 1996, Completing the Inventory of the Solar System, 29
Cited by
Domagal-Goldman, S. D., Wright, K. E., Domagal-Goldman, S. D., Wright, K. E., Adamala, K., Arina de la Rubia, L., Bond, J., Dartnell, L. R., Goldman, A. D., Lynch, K., et al. (2016) · Astrobiology · doi:10.1089/ast.2015.1460 · Cited by 136
“Depending on the extent of hydrothermal activity, water on an asteroid may be consumed by water-rock reactions, or some of it may remain in a thin outer layer enriched in water, hydrates, and organics (Castillo-Rogez and Schmidt, 2010).”
Metadata
- Authors
- Castillo‐Rogez, J. C., & Schmidt, B. E.
- Affiliations
- Jet Propulsion Laboratory California Institute of Technology Pasadena California USA
- University of California, Los Angeles (US)
- ORCID
- Schmidt, B. E.
- Venue
- Geophysical Research Letters
- Publisher
- American Geophysical Union (AGU)
- Published
- 2010-05
- Volume
- 37
- Issue
- 10
- ISSN
- 0094-8276 (ISSN-L)
- 1944-8007
- OpenAlex
- W1667043941
- Cited by
- 47
- References
- 28
- Citations by year
- 2025: 1 · 2024: 1 · 2022: 4 · 2021: 4 · 2019: 2 · 2018: 1 · 2017: 4 · 2016: 4 · 2015: 6 · 2014: 3 · 2013: 1 · 2012: 3
- FWCI
- 2.68
- Type
- journal article
- Language
- en
- Open access
- bronze
- doi.org
- Locations
- Geophysical Research Letters (publishedVersion)
- Funders
- National Aeronautics and Space Administration
- California Institute of Technology
- Jet Propulsion Laboratory
- Topics
- Physical Sciences › Earth and Planetary Sciences › Space and Planetary Science › Astro and Planetary Science
- Physical Sciences › Earth and Planetary Sciences › Space and Planetary Science › Planetary Science and Exploration
- Physical Sciences › Earth and Planetary Sciences › Geophysics › High-pressure geophysics and materials
- Keywords
- Themis family, asteroid parent body, asteroid differentiation, asteroid accretion, calcium-aluminum-rich inclusions, asteroid spectral properties, asteroid density
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- Castillo‐Rogez, J. C., & Schmidt, B. E. (2010). Geophysical evolution of the Themis family parent body. Geophysical Research Letters. https://doi.org/10.1029/2009gl042353
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Bibliographic data: Semantic Scholar, OpenAlex, Crossref.
Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).
Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.
