Abstract
We consider the survivability of planetary systems in the globular cluster 47 Tucanae. We compute the cross-sections for the breakup of planetary systems via encounters with single stars and binaries. We also compute the cross-sections to leave planets on eccentric orbits. We find that wider planetary systems (d ≳ 0.3 au) are likely to be broken up in the central regions of 47 Tucanae (within the half-mass radius of the cluster). However, tighter systems and those in less-dense regions may survive. Tight systems will certainly survive in less-dense clusters where subsequent surveys should be conducted.
Original language | English (US) |
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Pages (from-to) | 612-616 |
Number of pages | 5 |
Journal | Monthly Notices of the Royal Astronomical Society |
Volume | 324 |
Issue number | 3 |
DOIs | |
State | Published - Jul 1 2001 |
All Science Journal Classification (ASJC) codes
- Astronomy and Astrophysics
- Space and Planetary Science