2011A&A...532A..58V


C.D.S. - SIMBAD4 rel 1.7 - 2020.07.14CEST19:39:53

2011A&A...532A..58V - Astronomy and Astrophysics, volume 532A, 58-58 (2011/8-1)

Atmospheric studies of habitability in the Gliese 581 system.

VON PARIS P., GEBAUER S., GODOLT M., RAUER H. and STRACKE B.

Abstract (from CDS):

The M-type star object Gliese 581 is orbited by at least one terrestrial planet candidate in the habitable zone, i.e. GL 581d. Orbital simulations have shown that additional planets inside the habitable zone of GL 581 would be dynamically stable. Recently, two other planet candidates have been claimed, one of them in the habitable zone. In view of the ongoing search for planets around M stars that is expected to result in numerous detections of potentially habitable super-Earths, we take the GL 581 system as an example for investigating such planets. In contrast to previous studies of habitability in the GL 581 system, we use a consistent atmospheric model to assess surface conditions and habitability. Furthermore, we performed detailed atmospheric simulations for a much larger subset of potential planetary and atmospheric scenarios than previously considered. A 1D radiative-convective atmosphere model was used to calculate temperature and pressure profiles of model atmospheres, which we assumed to be composed of molecular nitrogen, water, and carbon dioxide. In these calculations, key parameters such as surface pressure and CO2 concentration, as well as orbital distance and planetary mass are varied.
Result. imply that surface temperatures above freezing could be obtained, independent of the atmospheric scenarios considered here, at an orbital distance of 0.117AU. For an orbital distance of 0.146AU, CO2 concentrations as low as 10 times the present Earth's value are sufficient to warm the surface above the freezing point of water. At 0.175AU, only scenarios with CO2 concentrations of 5% and 95% were found to be habitable, so an additional super-Earth planet in the GL 581 system in the previously determined dynamical stability range would be considered a potentially habitable planet.

Abstract Copyright:

Journal keyword(s): astrobiology - planets and satellites: atmospheres - planetary systems - stars: individual object: Gliese 581

Simbad objects: 5

goto Full paper

goto View the reference in ADS

Number of rows : 5

N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2020
#notes
1 CoRoT-7b Pl 06 43 49.4690410679 -01 03 46.825797768           ~ 346 1
2 BD-07 4003c Pl 15 19 26.8271336166 -07 43 20.190958776           ~ 96 1
3 BD-07 4003d Pl 15 19 26.8271336166 -07 43 20.190958776           ~ 136 1
4 BD-07 4003 BY* 15 19 26.8271336166 -07 43 20.190958776 13.403 11.76 10.560 9.461 8.911 M3V 534 2
5 NAME G 139-21b Pl 17 15 18.9337265994 +04 57 50.064695682           ~ 533 1

    Equat.    Gal    SGal    Ecl

To bookmark this query, right click on this link: simbad:objects in 2011A&A...532A..58V and select 'bookmark this link' or equivalent in the popup menu


2020.07.14-19:39:53

© Université de Strasbourg/CNRS

    • Contact