Published July 20, 2020
| Version 1.0
Dataset
Open
Parent aggregates
Description
Rubble pile models of parent aggregates. The models are obtained through numerical N-body simulations, using the GRAINS software. Simulations are performed using non-spherical particles, mutually interacting under contact/collisions and self-gravity. See Ferrari & Tanga 2020 (doi: 10.1016/j.icarus.2020.113871), Ferrari et al 2020 (doi: 10.1093/mnras/stz3458), Ferrari et al 2016 (doi: 10.1007/s11044-016-9547-2) for further details on the numerical model.
Files
parent_m_13061.txt
Files
(29.8 MB)
| Name | Size | Download all |
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md5:cd510908d33ab6faabe8f0a0f04746e8
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6.3 MB | Preview Download |
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md5:76893a7c37c5cf60fa76c282f1ec5354
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1.9 MB | Preview Download |
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md5:ab7d8f2a99cfa3e751f6e84d0829fe26
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3.2 MB | Preview Download |
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md5:38e660ac912153bacfc2bb39e76cc90f
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4.9 MB | Preview Download |
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md5:96ded23e3a758ee4af3563ff172edc23
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6.4 MB | Preview Download |
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md5:0092db032c7a4a786608c634781eef86
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7.0 MB | Preview Download |
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md5:fb673b79c10295af24c76a249a91fe2f
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355 Bytes | Preview Download |
Additional details
Related works
- References
- Journal article: 10.1016/j.icarus.2020.113871 (DOI)
- Journal article: 10.1093/mnras/stz3458 (DOI)
- Journal article: 10.1007/s11044-016-9547-2 (DOI)
Funding
References
- Ferrari & Tanga (2020). Doi: 10.1016/j.icarus.2020.113871)
- Ferrari et al (2016). Doi: 10.1007/s11044-016-9547-2
- Ferrari et al (2020). Doi: 10.1093/mnras/stz3458