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Cited by 476Astro and Planetary ScienceAstrophysics and Star Formation StudiesStellar, planetary, and galactic studies

The DOI matches its Crossref record.

Planetesimals to planets: Numerical simulation of collisional evolution

Greenberg, Richard, Wacker, John F., Hartmann, William K., Chapman, Clark R.·1978·Icarus
DOI 10.1016/0019-1035(78)90057-x
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Crossref · 10.1016/0019-1035(78)90057-x

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  • Large-scale complex phenomena, such as the weather, planet accretion/collision and galaxy formation, are studied almost exclusively by computer simulations.

    “Such an attitude seems oblivious to the fact that large-scale complex phenomena, such as the weather, planet accretion/collision and galaxy formation are studied almost exclusively by computer simulations [252].”

    From Systems protobiology: origin of life in lipid catalytic networks (2018) · cites this paper as [252]

Citations

Cites

No references could be resolved yet.

Research works printed but not linked: 23

  1. Chapman, 1975, Asteroid collisional evolution: Evidence for a much larger early population, Science, 190, 553, 10.1126/science.190.4214.553 · DOI
  2. Franklin, 1970, A dynamical model for the radial structure of Saturn's rings, Icarus, 12, 338, 10.1016/0019-1035(70)90003-5 · DOI
  3. Fujiwara, 1977, Destruction of basaltic bodies by high velocity impact, Icarus, 31, 277, 10.1016/0019-1035(77)90038-0 · DOI
  4. Gault, 1963, Spray ejected from the lunar surface by meteoroid impact, NASA Tech. Note D-1767
  5. Goldreich, 1965, An explanation of the frequent occurrence of commensurable mean motions in the solar system, Mon. Not. Roy. Astron. Soc., 130, 159, 10.1093/mnras/130.3.159 · DOI
  6. Goldreich, 1973, The formation of planetesimals, Astrophys. J., 183, 1051, 10.1086/152291 · DOI
  7. Greenberg, 1977, Orbit-orbit resonances in the solar system: Varieties and similarities, Vistas in Astronomy, 21, 209, 10.1016/0083-6656(77)90031-9 · DOI
  8. Greenberg, 1978, Orbital resonance in a dissipative medium, Icarus, 33, 62, 10.1016/0019-1035(78)90024-6 · DOI
  9. Greenberg, 1977, Size distribution of particles in a planetary ring, Icarus, 30, 769, 10.1016/0019-1035(77)90094-X · DOI
  10. Harris, 1975, Collisional breakup in a planetary ring, Icarus, 24, 190, 10.1016/0019-1035(75)90097-4 · DOI
  11. Hartmann, 1969, Terrestrial, lunar and interplanetary rock fragmentation, Icarus, 10, 201, 10.1016/0019-1035(69)90022-0 · DOI
  12. Hartmann, 1978, Planet formation: Mechanism of early growth, Icarus, 33, 50, 10.1016/0019-1035(78)90023-4 · DOI
  13. Hartmann, 1975, Satellite-sized planetesimals and lunar origin, Icarus, 24, 504, 10.1016/0019-1035(75)90070-6 · DOI
  14. Hayashi, 1977, Long term behaviors of planetesimals and the formation of the planets, Kyoto University preprint KUNS 379
  15. Isaacman, 1977, Computer simulations of planetary accretion dynamics: Sensitivity to initial conditions, Icarus, 31, 510, 10.1016/0019-1035(77)90153-1 · DOI
  16. Kaula, 1975, Early scattering by Jupiter and its collision effects in the terrestrial zone, Icarus, 25, 18, 10.1016/0019-1035(75)90186-4 · DOI
  17. Kuiper, 1974, On the origin of the solar system, Celestial Mechanics, 9, 321, 10.1007/BF01228575 · DOI
  18. Lecar, 1973, On the original distribution of the asteroids, Icarus, 20, 422, 10.1016/0019-1035(73)90015-8 · DOI
  19. Marcus, 1969, Speculations on mass loss by meteoroid impact and formation of planets, Icarus, 11, 76, 10.1016/0019-1035(69)90117-1 · DOI
  20. Safronov, 1972, Evolution of protoplanetary clouds and formation of the earth and planets, NASA TT F-677
  21. Stöffler, 1975, Experimental hypervelocity impact into quartz sand: Distribution and shock metamorphism of ejecta, JGR, 80, 4062, 10.1029/JB080i029p04062 · DOI
  22. Weidenschilling, 1974, A model for accretion of the terrestrial planets, Icarus, 22, 426, 10.1016/0019-1035(74)90075-X · DOI
  23. Weidenschilling, 1975, Mass loss from the region of Mars and the asteroid belt, Icarus, 26, 361, 10.1016/0019-1035(75)90180-3 · DOI

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Metadata

Authors
Greenberg, R., Wacker, J. F., Hartmann, W. K., & Chapman, C. R.
Affiliations
  • University of Arizona (US)
  • Planetary Science Institute (US)
ORCID
Venue
Icarus
Publisher
Elsevier BV
Published
1978-07
Volume
35
Issue
1
Pages
1-26
ISSN
0019-1035 (ISSN-L)
DOI
10.1016/0019-1035(78)90057-x
OpenAlex
W1990763154
Cited by
476
References
0
Citations by year
2026: 4 · 2025: 8 · 2024: 5 · 2023: 8 · 2022: 8 · 2021: 5 · 2020: 11 · 2019: 7 · 2018: 35 · 2017: 1 · 2016: 16 · 2015: 12 · 2014: 15 · 2013: 14 · 2012: 11
FWCI
13.89
Type
journal article
Language
en
Open access
closed
Licence
www.elsevier.com/tdm/userlicense/1.0/ (tdm)
Locations
Icarus (publishedVersion)
Topics
  • Physical Sciences › Earth and Planetary Sciences › Space and Planetary Science › 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 › Stellar, planetary, and galactic studies
Keywords
planetesimal formation, planet formation, collisional evolution, early solar system, gravitational instability, solar nebula, impact dynamics, rebound, crater formation, random velocity, collision cross sections, planetesimals

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