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Query : 2011ApJ...743...41K |
2011ApJ...743...41K - Astrophys. J., 743, 41 (2011/December-2)
Climate instability on tidally locked exoplanets.
KITE E.S., GAIDOS E. and MANGA M.
Abstract (from CDS):
Both instabilities are suppressed if the atmosphere has a high radiative efficiency. Our results are most relevant for atmospheres that are thin, have low greenhouse-gas radiative efficiency, and have a principal greenhouse gas that is also the main constituent of the atmosphere. ESWI also requires land near the substellar point, and tectonic resurfacing (volcanism, mountain-building) is needed for large jumps in pressure. These results identify a new pathway by which habitable-zone planets can undergo rapid climate shifts and become uninhabitable.
Abstract Copyright: ∼
Journal keyword(s): planets and satellites: atmospheres - planets and satellites: general - planets and satellites: surfaces - stars: individual (Kepler-10, CoRoT-7, GJ1214, 55 Cnc, Kepler-9, Kepler-11)
Simbad objects: 7
Number of rows : 7 |
N | Identifier | Otype |
ICRS (J2000) RA |
ICRS (J2000) DEC |
Mag U | Mag B | Mag V | Mag R | Mag I | Sp type |
#ref
1850 - 2024 |
#notes |
---|---|---|---|---|---|---|---|---|---|---|---|---|
1 | CoRoT-7 | * | 06 43 49.4690164104 | -01 03 46.826642700 | 12.78 | 11.73 | 11.36 | 10.87 | K0V | 211 | 1 | |
2 | * rho01 Cnc | EB* | 08 52 35.8111044043 | +28 19 50.954994470 | 7.45 | 6.82 | 5.4 | K0IV-V | 1121 | 1 | ||
3 | BD-07 4003 | BY* | 15 19 26.8269387505 | -07 43 20.189497466 | 13.403 | 11.76 | 10.560 | 9.461 | 8.911 | M3V | 641 | 2 |
4 | G 139-21 | PM* | 17 15 18.9339850845 | +04 57 50.066612336 | 14.394 | M4.5V | 325 | 1 | ||||
5 | Kepler-9 | Er* | 19 02 17.7544327200 | +38 24 03.176851896 | 13.9 | 13.791 | G2 | 190 | 1 | |||
6 | Kepler-10 | Ro* | 19 02 43.0613892904 | +50 14 28.701617339 | 11.00 | G2V | 202 | 1 | ||||
7 | Kepler-11 | Er* | 19 48 27.6226218768 | +41 54 32.903163504 | 14.635 | 13.838 | 13.742 | G2V | 351 | 1 |
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