2017A&A...603A.108A


Query : 2017A&A...603A.108A

2017A&A...603A.108A - Astronomy and Astrophysics, volume 603A108-108 (2017/7-1)

The rotation of planets hosting atmospheric tides: from Venus to habitable super-Earths.

AUCLAIR-DESROTOUR P., LASKAR J., MATHIS S. and CORREIA A.C.M.

Abstract (from CDS):

The competition between the torques induced by solid and thermal tides drives the rotational dynamics of Venus-like planets and super-Earths orbiting in the habitable zone of low-mass stars. The resulting torque determines the possible equilibrium states of the planet's spin. Here we have computed an analytic expression for the total tidal torque exerted on a Venus-like planet. This expression is used to characterize the equilibrium rotation of the body. Close to the star, the solid tide dominates. Far from it, the thermal tide drives the rotational dynamics of the planet. The transition regime corresponds to the habitable zone, where prograde and retrograde equilibrium states appear. We demonstrate the strong impact of the atmospheric properties and of the rheology of the solid part on the rotational dynamics of Venus-like planets, highlighting the key role played by dissipative mechanisms in the stability of equilibrium configurations.

Abstract Copyright: © ESO, 2017

Journal keyword(s): planet-star interactions - planets and satellites: dynamical evolution and stability - planets and satellites: atmospheres - celestial mechanics - celestial mechanics

Simbad objects: 1

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Number of rows : 1
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 * rho01 Cnc e Pl 08 52 35.8111044043 +28 19 50.954994470           ~ 682 1

Query : 2017A&A...603A.108A

Basic data :
* rho01 Cnc e -- Extra-solar Planet
Other object types:
otypes_help
* (*,HD), Pl (2004ApJ), Pl? (TOI)
ICRS coord. (ep=J2000) :
08 52 35.8111044043 +28 19 50.954994470 (Optical) [ 0.0299 0.0198 90 ] A 2020yCat.1350....0G
FK4 coord. (ep=B1950 eq=1950) :
08 49 37.3653494907 +28 31 23.237903251 [ 0.0299 0.0198 90 ]
Gal coord. (ep=J2000) :
196.7946531107533 +37.6988974333162 [ 0.0299 0.0198 90 ]
Proper motions mas/yr :
-485.681 -233.517 [0.040 0.037 90] A 2020yCat.1350....0G
Parallaxes (mas):
79.4482 [0.0429] A 2020yCat.1350....0G
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Hierarchy : number of linked objects
whatever the membership probability is (see description here ) :

: 1 : 4 Display criteria :

Identifiers (6) :
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* rho01 Cnc e HD 75732e TOI-1773e
* 55 Cnc e NAME Janssen TOI-1773.01

References (682 between 1850 and 2026) (Total 682)
Simbad bibliographic survey began in 1850 for stars (at least bright stars) and in 1983 for all other objects (outside the solar system).
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