Bodily Tides
The equilibrium tide model in the weak friction approximation is used by the binary star and exoplanet communities to study the tidal evolution of short-period systems. However, each uses a slightly different approach which potentially leads to different conclusions about the timescales on which va...
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| Format: | Article |
| Language: | English |
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EDP Sciences
2011-02-01
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| Series: | EPJ Web of Conferences |
| Online Access: | http://dx.doi.org/10.1051/epjconf/20101103002 |
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doaj-f6b45a5bdd204da08c699b8dda4c8dad2021-08-02T08:12:26ZengEDP SciencesEPJ Web of Conferences2100-014X2011-02-01110300210.1051/epjconf/20101103002Bodily TidesMardling Rosemary.A.The equilibrium tide model in the weak friction approximation is used by the binary star and exoplanet communities to study the tidal evolution of short-period systems. However, each uses a slightly different approach which potentially leads to different conclusions about the timescales on which various processes occur. Here we present an overview of these two approaches, and show that for short-period planets the circularization timescales they predict differ by at most a factor of a few. A discussion of the timescales for orbital decay, spin-orbit synchronization and spin-oribt alignment is also presented. http://dx.doi.org/10.1051/epjconf/20101103002 |
| collection |
DOAJ |
| language |
English |
| format |
Article |
| sources |
DOAJ |
| author |
Mardling Rosemary.A. |
| spellingShingle |
Mardling Rosemary.A. Bodily Tides EPJ Web of Conferences |
| author_facet |
Mardling Rosemary.A. |
| author_sort |
Mardling Rosemary.A. |
| title |
Bodily Tides |
| title_short |
Bodily Tides |
| title_full |
Bodily Tides |
| title_fullStr |
Bodily Tides |
| title_full_unstemmed |
Bodily Tides |
| title_sort |
bodily tides |
| publisher |
EDP Sciences |
| series |
EPJ Web of Conferences |
| issn |
2100-014X |
| publishDate |
2011-02-01 |
| description |
The equilibrium tide model in the weak friction approximation is used by the binary star and exoplanet communities to study the tidal evolution of short-period systems. However, each uses a slightly different approach which potentially leads to different conclusions about the timescales on which various processes occur. Here we present an overview of these two approaches, and show that for short-period planets the circularization timescales they predict differ by at most a factor of a few. A discussion of the timescales for orbital decay, spin-orbit synchronization and spin-oribt alignment is also presented. |
| url |
http://dx.doi.org/10.1051/epjconf/20101103002 |
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