Consequences of large impacts on Enceladus’ core shape
We investigated the deep consequences of large collisions on Enceladus. * We used the code iSALE2D considering large differentiated impactors. * The post-impact core deflections are governed by the impactor radius and velocity. * Multiple low velocity collisions may explain the irregular shape of En...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Choblet, G [verfasserIn] |
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Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2016 |
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| Rechteinformationen: |
Nutzungsrecht: © COPYRIGHT 2016 Elsevier B.V. |
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| Übergeordnetes Werk: |
Enthalten in: Icarus - Amsterdam [u.a.] : Elsevier, 1962, 264(2016), Seite 300-310 |
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| Übergeordnetes Werk: |
volume:264 ; year:2016 ; pages:300-310 |
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| DOI / URN: |
10.1016/j.icarus.2015.09.034 |
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| 520 | |a We investigated the deep consequences of large collisions on Enceladus. * We used the code iSALE2D considering large differentiated impactors. * The post-impact core deflections are governed by the impactor radius and velocity. * Multiple low velocity collisions may explain the irregular shape of Enceladus' core. | ||
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We investigated the deep consequences of large collisions on Enceladus. * We used the code iSALE2D considering large differentiated impactors. * The post-impact core deflections are governed by the impactor radius and velocity. * Multiple low velocity collisions may explain the irregular shape of Enceladus' core. |
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We investigated the deep consequences of large collisions on Enceladus. * We used the code iSALE2D considering large differentiated impactors. * The post-impact core deflections are governed by the impactor radius and velocity. * Multiple low velocity collisions may explain the irregular shape of Enceladus' core. |
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We investigated the deep consequences of large collisions on Enceladus. * We used the code iSALE2D considering large differentiated impactors. * The post-impact core deflections are governed by the impactor radius and velocity. * Multiple low velocity collisions may explain the irregular shape of Enceladus' core. |
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Consequences of large impacts on Enceladus’ core shape |
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shape</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">2016</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="a">Text</subfield><subfield code="b">txt</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="a">ohne Hilfsmittel zu benutzen</subfield><subfield code="b">n</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="a">Band</subfield><subfield code="b">nc</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">We investigated the deep consequences of large collisions on Enceladus. * We used the code iSALE2D considering large differentiated impactors. * The post-impact core deflections are governed by the impactor radius and velocity. * Multiple low velocity collisions may explain the irregular shape of Enceladus' core.</subfield></datafield><datafield tag="540" ind1=" " ind2=" "><subfield code="a">Nutzungsrecht: © COPYRIGHT 2016 Elsevier B.V.</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Collins, G.S</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Tobie, G</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Monteux, J</subfield><subfield code="4">oth</subfield></datafield><datafield tag="773" ind1="0" ind2="8"><subfield code="i">Enthalten in</subfield><subfield code="t">Icarus</subfield><subfield code="d">Amsterdam [u.a.] : Elsevier, 1962</subfield><subfield code="g">264(2016), Seite 300-310</subfield><subfield code="w">(DE-627)129321966</subfield><subfield code="w">(DE-600)131023-9</subfield><subfield code="w">(DE-576)014554259</subfield><subfield code="x">0019-1035</subfield><subfield code="7">nnns</subfield></datafield><datafield 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