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
Gespeichert in:
| Autor*in: |
Hyodo, Ryuki [verfasserIn] |
|---|
| Format: |
Artikel |
|---|---|
| Sprache: |
Englisch |
| Erschienen: |
2016 |
|---|
| Rechteinformationen: |
Nutzungsrecht: © COPYRIGHT 2017 Elsevier B.V. |
|---|
| Schlagwörter: |
|---|
| Übergeordnetes Werk: |
Enthalten in: Icarus - Amsterdam [u.a.] : Elsevier, 1962, 282(2016), Seite 195 |
|---|---|
| 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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| 520 | |a 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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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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