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Cited by 96

The DOI matches its Crossref record; 3 of the 3 references it cites were found in a registry or an index.

Formation of Phobos and Deimos via a giant impact

Citron, Robert I., Genda, Hidenori, Ida, Shigeru·2015·Icarus
DOI 10.1016/j.icarus.2015.02.011
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Research works printed but not linked: 32

  1. Agnor, 2004, Accretion efficiency during planetary collisions, Astrophys. J., 613, L157, 10.1086/425158 · DOI · Paper page
  2. Andert, 2010, Precise mass determination and the nature of Phobos, Geophys. Res. Lett., 37, L09202, 10.1029/2009GL041829 · doi:10.1029/2009gl041829
  3. Andrews-Hanna, 2008, The Borealis basin and the origin of the martian crustal dichotomy, Nature, 453, 1212, 10.1038/nature07011 · DOI · Paper page
  4. Benz, 1986, The origin of the Moon and the single-impact hypothesis. I, Icarus, 66, 515, 10.1016/0019-1035(86)90088-6 · DOI · Paper page
  5. Benz, 1987, The origin of the Moon and the single-impact hypothesis. II, Icarus, 71, 30, 10.1016/0019-1035(87)90160-6 · DOI · Paper page
  6. Benz, 1989, The origin of the Moon and the single impact hypothesis. III, Icarus, 81, 113, 10.1016/0019-1035(89)90129-2 · DOI · Paper page
  7. Bottke, 2000, Interpreting the elliptical crater populations on Mars, Venus, and the Moon, Icarus, 145, 108, 10.1006/icar.1999.6323 · DOI
  8. Burns, 1978, On the orbital evolution and origin of the martian moons, Vistas Astron., 22, 193, 10.1016/0083-6656(78)90015-6 · DOI
  9. Cameron, 1997, The origin of the Moon and the single impact hypothesis. V, Icarus, 126, 126, 10.1006/icar.1996.5642 · DOI
  10. Cameron, 1991, The origin of the Moon and the single impact hypothesis. IV, Icarus, 92, 204, 10.1016/0019-1035(91)90046-V · DOI · Paper page
  11. Canup, R.M., Salmon, J., 2014. On an impact origin of Phobos-Deimos. In: AAS/Division for Planetary Sciences Meeting Abstracts, vol. 46 (abstract).
  12. Canup, 2001, A scaling relationship for satellite-forming impacts, Icarus, 150, 288, 10.1006/icar.2000.6581 · DOI
  13. Craddock, 2011, Are Phobos and Deimos the result of a giant impact?, Icarus, 211, 1150, 10.1016/j.icarus.2010.10.023 · DOI · Paper page
  14. Cuk, 2012, Making the Moon from a fast-spinning Earth: A giant impact followed by resonant despinning, Science, 338, 1047, 10.1126/science.1225542 · DOI · Paper page
  15. Gault, 1974, Impact cratering, Primer Lunar Geol., 137
  16. Gault, D.E., Wedekind, J.A., 1977. Experimental hypervelocity impact into quartz sand – II: Effects of gravitational acceleration. In: Impact and Explosion Cratering: Planetary and Terrestrial Implications; Proceedings of the Symposium on Planetary Cratering Mechanics, pp. 1231–1244.
  17. Genda, 2012, Merging criteria for giant impacts of protoplanets, Astrophys. J., 744, 137, 10.1088/0004-637X/744/2/137 · DOI
  18. Giuranna, 2011, Compositional interpretation of PFS/MEx and TES/MGS thermal infrared spectra of Phobos, Planet. Space Sci., 59, 1308, 10.1016/j.pss.2011.01.019 · DOI
  19. Ida, 1997, Lunar accretion from an impact-generated disk, Nature, 389, 353, 10.1038/38669 · DOI · Paper page
  20. Marinova, 2008, Mega-impact formation of the Mars hemispheric dichotomy, Nature, 453, 1216, 10.1038/nature07070 · DOI · Paper page
  21. Monaghan, 1992, Smoothed Particle Hydrodynamics, Annu. Rev. Astron. Astrophys., vol. 30 (A93-25826 09-90), 30, 543, 10.1146/annurev.aa.30.090192.002551 · DOI · Paper page
  22. Murchie, 1991, Color heterogeneity of the surface of PHOBOS – Relationships to geologic features and comparison to meteorite analogs, J. Geophys. Res., 96, 5925, 10.1029/90JB02354 · doi:10.1029/90jb02354
  23. Nimmo, 2008, Implications of an impact origin for the martian hemispheric dichotomy, Nature, 453, 1220, 10.1038/nature07025 · DOI · Paper page
  24. Pätzold, 2014, Phobos: Observed bulk properties, Planet. Space Sci., 102, 86, 10.1016/j.pss.2014.01.004 · doi:10.1016/j.pss.2014.01.004
  25. Reese, 2011, Impact megadomes and the origin of the martian crustal dichotomy, Icarus, 213, 433, 10.1016/j.icarus.2011.03.028 · DOI
  26. Richardson, 2002, Gravitational aggregates: Evidence and evolution, Asteroids III, 501, 10.2307/j.ctv1v7zdn4.38 · DOI
  27. Rosenblatt, 2011, The origin of the martian moons revisited, Astron. Astrophys. Rev., 19, 1, 10.1007/s00159-011-0044-6 · DOI
  28. Rosenblatt, 2012, On the formation of the martian moons from a circum-martian accretion disk, Icarus, 221, 806, 10.1016/j.icarus.2012.09.009 · DOI
  29. Schultz, 1982, The structure and evolution of ancient impact basins on Mars, Int. Colloq. Mars, 87, 9803
  30. Strom, 1992, The martian impact cratering record, Mars, 383
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Metadata

Authors
Citron, R. I., Genda, H., & Ida, S.
Venue
Icarus
Publisher
Elsevier BV
Published
2015-05
Volume
252
Pages
334-338
ISSN
0019-1035
DOI
10.1016/j.icarus.2015.02.011
Cited by
96
References
3
Language
en
Licence
www.elsevier.com/tdm/userlicense/1.0/ (tdm)
Funders
  • NSF’s East Asia and Pacific Summer Institute
  • Japan Society for the Promotion of Science’s Summer Science Program

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CoChat. (2026). Citation check: Formation of Phobos and Deimos via a giant impact. https://app.cochat.ai/papers/10.1016/j.icarus.2015.02.011
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Citron, R. I., Genda, H., & Ida, S. (2015). Formation of Phobos and Deimos via a giant impact. Icarus. https://doi.org/10.1016/j.icarus.2015.02.011

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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.