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Evolution of the Edgeworth-Kuiper Belt
| Content Provider | Scilit |
|---|---|
| Author | Ipatov, S. I. |
| Copyright Year | 2002 |
| Description | Due to gravitational interactions with large trans-neptunian objects (TNOs) several percent of TNOs can change their semimajor axes by more that 1 AU during last 4 Gyr. Now about 30000 1-km former TNOs can be Jupiter crossers and about 20% of Earth-crossing objects can be former TNOs which now move in Jupiter-crossing orbits. |
| Related Links | https://www.cambridge.org/core/services/aop-cambridge-core/content/view/1588AB52442DCC86C4084C1C9EB5F1EC/S153929960001340Xa.pdf/div-class-title-evolution-of-the-edgeworth-kuiper-belt-div.pdf |
| Ending Page | 248 |
| Page Count | 2 |
| Starting Page | 247 |
| ISSN | 15392996 |
| DOI | 10.1017/s153929960001340x |
| Journal | Highlights of Astronomy |
| Volume Number | 12 |
| Language | English |
| Publisher | Cambridge University Press (CUP) |
| Publisher Date | 2002-01-01 |
| Access Restriction | Open |
| Subject Keyword | Highlights of Astronomy Particles and Fields Physics Former Tnos Crossing Objects Edgeworth Kuiper Belt Due Jupiter Crossing Gravitational Interactions Trans Neptunian Neptunian Objects Crossing Orbits |
| Content Type | Text |
| Resource Type | Article |