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 p...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Hyodo, Ryuki [verfasserIn] |
|---|
| Format: |
E-Artikel |
|---|---|
| Sprache: |
Englisch |
| Erschienen: |
2017 |
|---|
| Umfang: |
19 |
|---|
| Übergeordnetes Werk: |
Enthalten in: Development of electrophysiological and behavioural measures of electrode discrimination in adult cochlear implant users - Mathew, Rajeev ELSEVIER, 2018, international journal of solar system studies, Orlando, Fla |
|---|---|
| Übergeordnetes Werk: |
volume:282 ; year:2017 ; day:15 ; month:01 ; pages:195-213 ; extent:19 |
| Links: |
|---|
| DOI / URN: |
10.1016/j.icarus.2016.09.012 |
|---|
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ELV025606824 |
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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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Ring formation around giant planets by tidal disruption of a single passing large Kuiper belt object |
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