2007MNRAS.375.1495S


C.D.S. - SIMBAD4 rel 1.7 - 2021.01.22CET21:45:54

2007MNRAS.375.1495S - Mon. Not. R. Astron. Soc., 375, 1495-1502 (2007/March-2)

A stability catalogue of the habitable zones in extrasolar planetary systems.

SANDOR Z., SULI A., ERDI B., PILAT-LOHINGER E. and DVORAK R.

Abstract (from CDS):

In the near future, space missions will be launched (e.g. COROT, KEPLER) to detect Earth-like extrasolar planets. The orbital elements of these (still hypothetic) planets will contain some uncertainties that can only be eliminated by careful dynamical investigations of the hosting planetary systems. The proportion of extrasolar planetary systems with one known giant planet is high (∼90 per cent). Therefore, as a first step we have investigated the possible existence of terrestrial planets in these systems. In this paper, the development of a stability catalogue of the habitable zones of exoplanetary systems is reported. This catalogue is formed by a series of stability maps, which can help to establish where Earth-like planets could exist in extrasolar planetary systems having one giant planet. After a description of the dynamical model and the numerical methods, details of the stability maps are discussed. An application of the stability catalogue to 15 known exoplanetary systems is also shown, and a characterization of the stability properties of their habitable zones is given.

Abstract Copyright: 2007 The Authors. Journal compilation © 2007 RAS

Journal keyword(s): astrobiology - methods: numerical - celestial mechanics - planetary systems

Simbad objects: 17

goto Full paper

goto View the reference in ADS

Number of rows : 17

N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2021
#notes
1 HD 8574 PM* 01 25 12.5155869426 +28 34 00.101503796       6.8   F8 135 1
2 * 109 Psc PM* 01 44 55.8251018821 +20 04 59.336256238   6.984 6.279     G3Va 255 2
3 * eps Eri BY* 03 32 55.8449634 -09 27 29.731165 5.19 4.61 3.73 3.00 2.54 K2V 1728 1
4 HD 30177 PM* 04 41 54.3739541801 -58 01 14.724686984   9.18 8.37     G8V 118 1
5 HD 50554 PM* 06 54 42.8262327211 +24 14 44.008992953   7.41 6.84     F8V 171 1
6 HD 52265 PM* 07 00 18.0357152121 -05 22 01.778490073   6.845 6.282     G0V 295 1
7 HD 70642 PM* 08 21 28.1371964750 -39 42 19.480026866   7.89 7.18     G6VCN+0.5 141 1
8 HD 72659 PM* 08 34 03.1900792374 -01 34 05.579345170   8.08 7.47     G2V 132 1
9 * 47 UMa PM* 10 59 27.9738644892 +40 25 48.922388918   5.66   4.7   G1-VFe-0.5 722 1
10 * 47 UMa b Pl 10 59 27.9738644892 +40 25 48.922388918           ~ 146 1
11 HD 114729 PM* 13 12 44.2594905817 -31 52 24.057468040   7.31 6.69     G0V 164 1
12 * 70 Vir PM* 13 28 25.8081883620 +13 46 43.642951116 5.930 5.680 4.970 4.37 3.98 G4Va 677 1
13 HD 121504 PM* 13 57 17.2384093173 -56 02 24.156313081   8.12 7.52     G2V 149 1
14 * 14 Her PM* 16 10 24.3152754550 +43 49 03.498734567   7.57   6.1   K0V 412 1
15 HD 178911B PM* 19 09 03.0984180671 +34 35 59.473294546   8.71   7.3   G5 116 1
16 HD 190360 PM* 20 03 37.4049065078 +29 53 48.495330996   6.44   5.2   G7IV-V 396 1
17 * 51 Peg Ro* 22 57 27.9804167474 +20 46 07.782240714 6.39 6.16 5.46 4.97 4.61 G2IV 1085 1

    Equat.    Gal    SGal    Ecl

To bookmark this query, right click on this link: simbad:objects in 2007MNRAS.375.1495S and select 'bookmark this link' or equivalent in the popup menu


2021.01.22-21:45:54

© Université de Strasbourg/CNRS

    • Contact