Abstract
We examine possible locations for the primordial disk of the Edgeworth-Kuiper Belt (EKB), using several subsets of the known objects as markers of the total mass distribution. Using a secular perturbation theory, we find that the primordial plane of the EKB could have remained thin enough to escape detection only if it is clustered very closely about the invariable plane of the Solar System.
Original language | English |
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Pages (from-to) | 22-26 |
Number of pages | 5 |
Journal | Icarus |
Volume | 162 |
Issue number | 1 |
DOIs | |
Publication status | Published - 01 Mar 2003 |
Externally published | Yes |
Keywords
- Orbits
- Origin, solar system
- Planetary dynamics
- Transneptunian objects
ASJC Scopus subject areas
- Astronomy and Astrophysics
- Space and Planetary Science