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Resolution dependence of disruptive collisions between planetesimals in the gravity regime

Genda, Hidenori, Fujita, Tomoaki, Kobayashi, Hiroshi, Tanaka, Hidekazu, Abe, Yutaka·2015·Icarus

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Research works printed but not linked: 53

  1. Agnor, 1999, On the character and consequences of large impacts in the late stage of terrestrial planet formation, Icarus, 142, 219, 10.1006/icar.1999.6201 · DOI · Paper page
  2. Barnes, 1986, A hierarchical O (N logN) force-calculation algorithm, Nature, 324, 446, 10.1038/324446a0 · DOI · Paper page
  3. Benz, 1999, Catastrophic disruptions revisited, Icarus, 142, 5, 10.1006/icar.1999.6204 · DOI · Paper page
  4. Bottke, 2005, Linking the collisional history of the main asteroid belt to its dynamical excitation and depletion, Icarus, 179, 63, 10.1016/j.icarus.2005.05.017 · DOI · Paper page
  5. Citron, 2015, Formation of Phobos and Deimos via a giant impact, Icarus, 252, 334, 10.1016/j.icarus.2015.02.011 · DOI · Paper page
  6. Durda, 1998, Collisional models and scaling laws: A new interpretation of the shape of the main-belt asteroid size distribution, Icarus, 135, 431, 10.1006/icar.1998.5960 · DOI · Paper page
  7. Fukushige, 2005, GRAPE-6A: A single-card GRAPE-6 for parallel PC-GRAPE cluster systems, Publ. Astron. Soc. Jpn., 57, 1009, 10.1093/pasj/57.6.1009 · DOI
  8. Genda, 2003, Modification of a proto-lunar disk by hydrodynamic escape of silicate vapor, Earth Planets Space, 55, 53, 10.1186/BF03352462 · DOI
  9. Genda, 2015, Warm debris disks produced by giant impacts during terrestrial planet formation, Atrophies. J., 10.1088/0004-637X/810/2/136 · DOI
  10. Genda, 2012, Merging criteria for giant impacts of protoplanets, Astrophys. J., 744, 137, 10.1088/0004-637X/744/2/137 · DOI
  11. Goldreich, 1973, The formation of planetesimals, Astrophys. J., 183, 1051, 10.1086/152291 · DOI · Paper page
  12. Greenberg, 1978, Planetesimals to planets: Numerical simulation of collisional evolution, Icarus, 35, 1, 10.1016/0019-1035(78)90057-X · DOI · Paper page
  13. Hernquist, 1989, TREESPH: A unification of SPH with hierarchical tree method, Astrophys. J. Suppl. Ser., 70, 419, 10.1086/191344 · DOI · Paper page
  14. Hosono, 2013, Density-independent smoothed particle hydrodynamics for a non-ideal equation of state, Publ. Astron. Soc. Jpn., 65, 108(1), 10.1093/pasj/65.5.108 · DOI · Paper page
  15. Housen, 1990, On the fragmentation of asteroids and planetary satellites, Icarus, 84, 226, 10.1016/0019-1035(90)90168-9 · DOI · Paper page
  16. Housen, 1999, Scale effects in strength-dominated collisions of rocky asteroids, Icarus, 142, 21, 10.1006/icar.1999.6206 · DOI · Paper page
  17. Ida, 2004, Toward a deterministic model of planetary formation. I. A desert in the mass and semimajor axis distributions of extrasolar planets, Astrophys. J., 604, 388, 10.1086/381724 · DOI · Paper page
  18. Inaba, 2003, Formation of gas giant planets: Core accretion models with fragmentation and planetary envelope, Icarus, 166, 46, 10.1016/j.icarus.2003.08.001 · DOI
  19. Jutzi, 2015, SPH calculations of asteroid disruptions: The role of pressure dependent failure model, Planet. Space Sci., 107, 3, 10.1016/j.pss.2014.09.012 · DOI
  20. Jutzi, 2010, Fragment properties at the catastrophic disruption threshold: The effect of the parent body’s internal structure, Icarus, 207, 54, 10.1016/j.icarus.2009.11.016 · doi:10.1016/j.icarus.2009.11.016
  21. Kataoka, 2013, Static compression of porous dust aggregates, Astron. Astrophys., 554, 1, 10.1051/0004-6361/201321325 · doi:10.1051/0004-6361/201321325
  22. Kenyon, 2008, Variations on debris disks: Icy planet formation at 30–150AU for 1–3 Msun main-sequence stars, Astrophys. J. Suppl. Ser., 179, 451, 10.1086/591794 · DOI · Paper page
  23. Kenyon, 2012, Coagulation calculations of icy planet formation at 15–150AU: A correlation between the maximum radius and the slope of the size distribution for trans-neptunian objects, Astrophys. J., 143, 63
  24. Kitsionas, 2002, Smoothed Particle Hydrodynamics with particle splitting, applied to self-gravitating collapse, Mon. Not. R. Astron. Soc., 330, 129, 10.1046/j.1365-8711.2002.05115.x · doi:10.1046/j.1365-8711.2002.05115.x
  25. Kobayashi, 2013, Small planetesimals formed Mars, Icarus, 225, 122, 10.1016/j.icarus.2013.03.006 · DOI
  26. Kobayashi, 2014, Debris disc formation induced by planetary growth, Mon. Not. R. Astron. Soc., 442, 3266, 10.1093/mnras/stu1073 · doi:10.1093/mnras/stu1073
  27. Kobayashi, 2010, Fragmentation model dependence of collision cascades, Icarus, 206, 735, 10.1016/j.icarus.2009.10.004 · DOI
  28. Kobayashi, 2010, Planetary growth with collisional fragmentation and gas drag, Icarus, 209, 836, 10.1016/j.icarus.2010.04.021 · DOI
  29. Kobayashi, 2011, Planetary core formation with collisional fragmentation and atmosphere to form gas giant planets, Astrophys. J., 738, 35, 10.1088/0004-637X/738/1/35 · DOI
  30. Kobayashi, 2012, Rapid formation of Saturn after Jupiter completion, Astrophys. J., 756, 70, 10.1088/0004-637X/756/1/70 · DOI
  31. Kokubo, 2010, Formation of terrestrial planets from protoplanets under a realistic accretion condition, Astrophys. J., 714, 21, 10.1088/2041-8205/714/1/L21 · DOI
  32. Kokubo, 1996, On runaway growth of planetesimals, Icarus, 123, 180, 10.1006/icar.1996.0148 · DOI · Paper page
  33. Leinhardt, 2002, N-body simulations of planetsimal evolution: Effect of varying impactor mass ratio, Icarus, 159, 303, 10.1006/icar.2002.6909 · DOI
  34. Leinhardt, 2009, Full numerical simulations of catastrophic small body collisions, Icarus, 199, 542, 10.1016/j.icarus.2008.09.013 · DOI · Paper page
  35. Leinhardt, 2012, Collisions between gravity-dominated bodies. I. Outcome regimes and scaling laws, Astrophys. J., 745, 79, 10.1088/0004-637X/745/1/79 · DOI · Paper page
  36. Leinhardt, 2012, Tidal disruption of satellites and formation of narrow rings, Mon. Not. R. Astron. Soc., 424, 1419, 10.1111/j.1365-2966.2012.21328.x · DOI
  37. Love, 1996, Catastrophic impacts on gravity dominated asteroids, Icarus, 124, 141, 10.1006/icar.1996.0195 · DOI · Paper page
  38. Melosh, 1997, Asteroids: Shattered but not dispersed, Icarus, 129, 562, 10.1006/icar.1997.5797 · doi:10.1006/icar.1997.5797
  39. Mizutani, 1990, New scaling laws on impact fragmentation, Icarus, 87, 307, 10.1016/0019-1035(90)90136-W · doi:10.1016/0019-1035(90)90136-w
  40. Monaghan, 1992, Smoothed particle hydrodynamics, Annu. Rev. Astron. Astrophys., 30, 543, 10.1146/annurev.aa.30.090192.002551 · DOI · Paper page
  41. Nakamura, 2009, Collisional disruption experiments of porous targets, Planet. Space Sci., 57, 111, 10.1016/j.pss.2008.07.027 · doi:10.1016/j.pss.2008.07.027
  42. Price, 2007, An energy-conserving formalism for adaptive gravitational force softening in smoothed particle hydrodynamics and N-body codes, Mon. Not. R. Astron. Soc., 374, 1347, 10.1111/j.1365-2966.2006.11241.x · DOI · Paper page
  43. Sekine, 2012, Giant impacts in the saturnian system: A possible origin of diversity in the inner mid-sized satellites, Planet. Space Sci., 63, 133, 10.1016/j.pss.2011.05.015 · DOI
  44. Springel, 2010, Smoothed particle hydrodynamics in astrophysics, Annu. Rev. Astron. Astrophys., 48, 391, 10.1146/annurev-astro-081309-130914 · DOI · Paper page
  45. Tillotson, J.H., 1962. Metallic Equations of State for Hypervelocity Impact. General Atomic Rept. GA-3216, pp. 1–142.
  46. Wada, 2007, Numerical simulation of dust aggregate collisions. I. Compression and disruption of two-dimensional aggregates, Astrophys. J., 661, 320, 10.1086/514332 · doi:10.1086/514332
  47. Wada, 2008, Numerical simulation of dust aggregate collisions. II. Compression and disruption of three-dimensional aggregates in head-on collisions, Astrophys. J., 677, 1296, 10.1086/529511 · DOI · Paper page
  48. Wada, 2009, Collisional growth conditions for dust aggregates, Astrophys. J., 702, 1490, 10.1088/0004-637X/702/2/1490 · doi:10.1088/0004-637x/702/2/1490
  49. Weidenschilling, 1980, Dust to planetesimals: Settling and coagulation in the solar nebula, Icarus, 44, 172, 10.1016/0019-1035(80)90064-0 · DOI
  50. Weidenschilling, 1984, Evolution of grains in a turbulent solar nebula, Icarus, 60, 553, 10.1016/0019-1035(84)90164-7 · DOI
  51. Wetherill, 1980, Formation of the terrestrial planets, Annu. Rev. Astron. Astrophys., 18, 77, 10.1146/annurev.aa.18.090180.000453 · DOI · Paper page
  52. Wetherill, 1989, Accumulation of a swarm of small planetesimals, Icarus, 77, 330, 10.1016/0019-1035(89)90093-6 · DOI · Paper page
  53. Wyatt, 2007, Transience of hot dust around Sun-like stars, Astrophys. J., 658, 569, 10.1086/510999 · DOI · Paper page

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Metadata

Authors
Genda, H., Fujita, T., Kobayashi, H., Tanaka, H., & Abe, Y.
Venue
Icarus
Publisher
Elsevier BV
Published
2015-12
Volume
262
Pages
58-66
ISSN
0019-1035
Cited by
49
References
2
Language
en
Licence
www.elsevier.com/tdm/userlicense/1.0/ (tdm)
Funders
JSPS KAKENHI (26287101, 15K13562)

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CoChat. (2026). Citation check: Resolution dependence of disruptive collisions between planetesimals in the gravity regime. https://app.cochat.ai/papers/10.1016/j.icarus.2015.08.029
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Genda, H., Fujita, T., Kobayashi, H., Tanaka, H., & Abe, Y. (2015). Resolution dependence of disruptive collisions between planetesimals in the gravity regime. Icarus. https://doi.org/10.1016/j.icarus.2015.08.029

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