Planetary accretion in the inner Solar System
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Once a planet forms, further changes can differentiate elements between layers, with dense components such as iron, nickel, or metallic hydrogen sinking to form the core and less dense materials becoming incorporated into the mantle and crust.
“Once a planet forms (under any model) there can be further changes that result in the differentiation of elements between layers (Chambers, 2004).”
From The Astrobiology Primer v2.0 (2016) · cites this paper as Chambers, 2004
Cites
Origin of the Moon in a giant impact near the end of the Earth's formation
Canup, R. M., & Asphaug, E. (2001) · Nature · doi:10.1038/35089010 · Cited by 1,094 · see citing works
Source regions and timescales for the delivery of water to the Earth
Morbidelli, A., Chambers, J., Lunine, J. I., Petit, J. M., Robert, F., Valsecchi, G. B., & Cyr, K. E. (2000) · Meteoritics & Planetary Science · doi:10.1111/j.1945-5100.2000.tb01518.x · Cited by 881 · cited 3× · see citing works
“It is hard to explain the abundances of the other noble gases in the atmosphere today unless some volatiles came to Earth from another source, such as impacts by comets or asteroids [36,37].”
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Magma oceans in the inner solar system
Elkins-Tanton, L. T. (2012) · Annual Review of Earth and Planetary Sciences · doi:10.1146/annurev-earth-042711-105503 · Cited by 601 · see citing works
Emergence of a Habitable Planet
Zahnle, K., Arndt, N., Cockell, C., Halliday, A., Nisbet, E., Selsis, F., & Sleep, N. H. (2007) · Space Science Reviews · doi:10.1007/s11214-007-9225-z · Cited by 380 · see citing works
Equilibration in the aftermath of the lunar-forming giant impact
Pahlevan, K., & Stevenson, D. J. (2007) · Earth and Planetary Science Letters · doi:10.1016/j.epsl.2007.07.055 · Cited by 381 · see citing works
Widespread mixing and burial of Earth’s Hadean crust by asteroid impacts
Marchi, S., Bottke, W. F., Elkins-Tanton, L. T., Bierhaus, M., Wuennemann, K., Morbidelli, A., & Kring, D. A. (2014) · Nature · doi:10.1038/nature13539 · Cited by 277 · see citing works
A Decreased Probability of Habitable Planet Formation around Low‐Mass Stars
Raymond, S. N., Scalo, J., & Meadows, V. S. (2007) · The Astrophysical Journal · doi:10.1086/521587 · Cited by 210 · see citing works
“We assume that the disk evolved following the standard model of terrestrial planet growth (e.g. Chambers 2004): grains coalesced to form kmsized planetesimals; and embryos formed from planetes- imals via runaway and oligarchic growth (e.g., Kokubo & Ida 1998), spaced by 5-10 mutual Hill radii (RH,m…”
BackgroundIllusory Late Heavy Bombardments
Boehnke, P., & Harrison, T. M. (2016) · Proceedings of the National Academy of Sciences · doi:10.1073/pnas.1611535113 · Cited by 138 · see citing works
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 · see citing works
“Once a planet forms (under any model) there can be further changes that result in the differentiation of elements between layers (Chambers, 2004).”
Tides and the Evolution of Planetary Habitability
Barnes, R., Raymond, S. N., Jackson, B., & Greenberg, R. (2008) · Astrobiology · doi:10.1089/ast.2007.0204 · Cited by 122 · see citing works
Mottl, M. J., Glazer, B. T., Kaiser, R. I., & Meech, K. J. (2007) · Geochemistry · doi:10.1016/j.chemer.2007.09.002 · Cited by 117 · see citing works
Harrison, T. M. (2020) · doi:10.1007/978-3-030-46687-9 · Cited by 53 · see citing works
- Authors
- Chambers, J. E.
- Affiliations
- Carnegie Institution for Science (US)
- Corresponding author
- Chambers, John E.
- ORCID
- Chambers, John E.
- Venue
- Earth and Planetary Science Letters
- Publisher
- Elsevier BV
- Published
- 2004-07
- Volume
- 223
- Issue
- 3-4
- Pages
- 241-252
- ISSN
- 0012-821X (ISSN-L)
- OpenAlex
- W2136705981
- Cited by
- 341
- References
- 2
- Citations by year
- 2026: 5 · 2025: 11 · 2024: 14 · 2023: 12 · 2022: 13 · 2021: 9 · 2020: 20 · 2019: 12 · 2018: 18 · 2017: 14 · 2016: 21 · 2015: 19 · 2014: 20 · 2013: 9 · 2012: 16
- FWCI
- 9.63
- Type
- journal article
- Language
- en
- Open access
- closed
- Locations
- Earth and Planetary Science Letters (publishedVersion)
- Topics
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Astro and Planetary Science
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Astrophysics and Star Formation Studies
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Planetary Science and Exploration
- Keywords
- terrestrial planet formation, planetesimal formation, inner solar system, planetesimals, planetary embryos, giant impacts, Moon formation, asteroid belt, meteorites, protoplanetary disks, young Sun-like stars
About these checks
Registry, retraction, Cites and statistics results are computed, not judged, with one exception: a printed reference that no index lists is read once by a model before it counts as a citation error. Claims are extracted by a model and kept only when their quote appears verbatim in the text; each cited source is then checked, with a model’s help, for whether it says what the claim relies on. Those verdicts can be wrong — read the claim’s quote and the cited source before relying on one.
Statistics and arithmetic are recomputed, not judged.
Confidence bands are shown only for fields calibrated on our annotated test set. None is calibrated yet, so no band is shown.
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