J/ApJ/742/L19   Physics of Kepler hot rocky planetary candidates (Miguel+, 2011)

Compositions of hot super-Earth atmospheres: exploring Kepler candidates. Miguel Y., Kaltenegger L., Fegley B., Schaefer L. <Astrophys. J., 742, L19 (2011)> =2011ApJ...742L..19M 2011ApJ...742L..19M
ADC_Keywords: Planets ; Stars, double and multiple ; Stars, diameters ; Effective temperatures ; Models Keywords: astrobiology - planets and satellites: composition - planets and satellites: atmospheres - atmospheric effects Abstract: This paper outlines a simple approach to evaluate the atmospheric composition of hot rocky planets by assuming different types of planetary composition and using corresponding model calculations. To explore hot atmospheres above 1000K, we model the vaporization of silicate magma and estimate the range of atmospheric compositions according to the planet's radius and semi-major axis for the Kepler 2011 February data release. Our results show five atmospheric types for hot, rocky super-Earth atmospheres, strongly dependent on the initial composition and the planet's distance to the star. We provide a simple set of parameters that can be used to evaluate atmospheric compositions for current and future candidates provided by the Kepler mission and other searches. Description: The Kepler mission recently announced 1235 planetary candidates (Borucki et al. 2011, Cat. J/ApJ/736/19), of which 615 are consistent with models of rocky interior (R<2±0.5R), accounting for the 25% error in radii in the Kepler data set). Of these Kepler objects of interest (KOI), 193 have potentially extremely high temperatures on their surfaces (Tp>1000K, when assuming a 0.01 albedo), due to the intense stellar irradiation to which they are exposed, because of their proximity to the central star. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table2.dat 32 191 Planetary and stellar parameters for Kepler candidates with radius less than 2.5 Earth radius and temperatures higher than 1000K -------------------------------------------------------------------------------- See also: V/133 : Kepler Input Catalog (Kepler Mission Team, 2009) J/ApJS/204/24 : Kepler planetary candidates. III. (Batalha+, 2013) J/ApJ/736/19 : Kepler planetary candidates. II. (Borucki+, 2011) J/ApJ/736/L25 : Habitability of Kepler planet candidates (Kaltenegger+, 2011) J/ApJ/707/1707 : Ks-band light curve of CoRoT-1b (Rogers+, 2009) J/A+A/469/L43 : Radial velocities of Gl 581 (Udry+, 2007) Byte-by-byte Description of file: table2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 7 F7.2 --- KOI [69.01/1608.01] Kepler-Object-of-Interest number 9- 13 F5.3 AU a Semi-major axis of planetary candidate 15- 17 F3.1 Rgeo Rp [0.6/2.5] Radius of planetary candidate 19- 22 I4 K Tp [1001/3074] Equilibrium temperature of planet 24- 27 I4 K Teff [3684/6869] Effective temperature of star 29- 32 F4.2 Rsun R* [0.53/1.88] Radius of parent star -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Greg Schwarz [AAS], Emmanuelle Perret [CDS] 26-Apr-2013
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line