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| Content Provider | Springer Nature Link |
|---|---|
| Author | Paulech, Tomáš Jakubík, Marián Neslušan, Luboš Dybczyński, Piotr A. Leto, Giuseppe |
| Copyright Year | 2009 |
| Abstract | A fraction of small bodies from the once existing proto-planetary disc was ejected, by the giant planets, to large heliocentric distances and start to build the comet Oort cloud. Considering four models of initial proto-planetary disc, we attempt to roughly map a dependence between the initial disc’s structure and some properties of the Oort cloud. We find that it is difficult to construct the proto-planetary disc if (i) the amount of heavy chemical elements in Jupiter and Saturn is as high as currently accepted and (ii) the total mass of the minimum-mass solar nebula is assumed to be lower than $$\approx0.05\,\hbox{M}_{\odot}.$$ The behaviour of the Oort cloud formation does not crucially depend on the initial disc model. Some differences in its structure are obvious: since the cloud is known to be filled mainly by Uranus and Neptune, the efficiency of its formation is higher when the initial amount of particles in the Uranus-Neptune region is relatively higher. A significantly large number of Jupiter Trojans in our simulation appears, however, only in the case of the initially non-gapped disc, with the particles situated also close to the Jupiter’s orbit. |
| Starting Page | 367 |
| Ending Page | 371 |
| Page Count | 5 |
| File Format | |
| ISSN | 01679295 |
| Journal | Earth, Moon, and Planets |
| Volume Number | 105 |
| Issue Number | 2-4 |
| e-ISSN | 15730794 |
| Language | English |
| Publisher | Springer Netherlands |
| Publisher Date | 2009-03-17 |
| Publisher Place | Dordrecht |
| Access Restriction | Subscribed |
| Subject Keyword | Comets: general Oort cloud Solar system: formation Astrophysics Extraterrestrial Physics, Space Sciences Planetology Astronomy |
| Content Type | Text |
| Resource Type | Article |
| Subject | Astronomy and Astrophysics Space and Planetary Science |
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