Ring formation around giant planets by tidal disruption of a single passing large Kuiper belt object
Origin of rings still remains elusive. We investigate the possibility to make rings through tidal disruption of massive KBOs. * This could happen several times during the Late Heavy Bombardment. * SPH simulations show that about 1% of the mass of the KBOs can be trapped. Thus, rings around giant pla...
Ausführliche Beschreibung
Autor*in: |
Hyodo, Ryuki [verfasserIn] |
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Format: |
Artikel |
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Sprache: |
Englisch |
Erschienen: |
2016 |
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Rechteinformationen: |
Nutzungsrecht: © COPYRIGHT 2017 Elsevier B.V. |
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Schlagwörter: |
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Übergeordnetes Werk: |
Enthalten in: Icarus - Amsterdam [u.a.] : Elsevier, 1962, 282(2016), Seite 195 |
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Übergeordnetes Werk: |
volume:282 ; year:2016 ; pages:195 |
Links: |
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DOI / URN: |
10.1016/j.icarus.2016.09.012 |
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OLC1986945472 |
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10.1016/j.icarus.2016.09.012 doi PQ20170206 (DE-627)OLC1986945472 (DE-599)GBVOLC1986945472 (PRQ)a1957-ed1b1e8d1189fbe2a05aa1b91b6e62e48a4b9b5371561f065457894a97c9bdac0 (KEY)0009293220160000282000000195ringformationaroundgiantplanetsbytidaldisruptionof DE-627 ger DE-627 rakwb eng 520 530 DNB Hyodo, Ryuki verfasserin aut Ring formation around giant planets by tidal disruption of a single passing large Kuiper belt object 2016 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier Origin of rings still remains elusive. We investigate the possibility to make rings through tidal disruption of massive KBOs. * This could happen several times during the Late Heavy Bombardment. * SPH simulations show that about 1% of the mass of the KBOs can be trapped. Thus, rings around giant planets could be initially massive enough to produce their regular satellites. * Tidal disruption can explain the observed diversity of ring-systems. Nutzungsrecht: © COPYRIGHT 2017 Elsevier B.V. Planets Earth and Planetary Astrophysics Astrophysics Charnoz, Sébastien oth Ohtsuki, Keiji oth Genda, Hidenori oth Enthalten in Icarus Amsterdam [u.a.] : Elsevier, 1962 282(2016), Seite 195 (DE-627)129321966 (DE-600)131023-9 (DE-576)014554259 0019-1035 nnns volume:282 year:2016 pages:195 http://dx.doi.org/10.1016/j.icarus.2016.09.012 Volltext http://arxiv.org/abs/1609.02396 GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_47 GBV_ILN_70 GBV_ILN_2012 GBV_ILN_2279 GBV_ILN_2286 AR 282 2016 195 |
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Ring formation around giant planets by tidal disruption of a single passing large Kuiper belt object |
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Origin of rings still remains elusive. We investigate the possibility to make rings through tidal disruption of massive KBOs. * This could happen several times during the Late Heavy Bombardment. * SPH simulations show that about 1% of the mass of the KBOs can be trapped. Thus, rings around giant planets could be initially massive enough to produce their regular satellites. * Tidal disruption can explain the observed diversity of ring-systems. |
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Origin of rings still remains elusive. We investigate the possibility to make rings through tidal disruption of massive KBOs. * This could happen several times during the Late Heavy Bombardment. * SPH simulations show that about 1% of the mass of the KBOs can be trapped. Thus, rings around giant planets could be initially massive enough to produce their regular satellites. * Tidal disruption can explain the observed diversity of ring-systems. |
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Origin of rings still remains elusive. We investigate the possibility to make rings through tidal disruption of massive KBOs. * This could happen several times during the Late Heavy Bombardment. * SPH simulations show that about 1% of the mass of the KBOs can be trapped. Thus, rings around giant planets could be initially massive enough to produce their regular satellites. * Tidal disruption can explain the observed diversity of ring-systems. |
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Ring formation around giant planets by tidal disruption of a single passing large Kuiper belt object |
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