We present a radiative equilibrium model for extrasolar giant planets applied to 51 Peg b. The atmospheric model extends from 10 -5 to ∼10 bar and is limited at the bottom by an optically thick cloud of silicate (Mg 2 SiO 4 or MgSiO 3 ) or iron (Fe) particles. Rayleigh scattering at short wavelength
✦ LIBER ✦
Radiative Equilibrium Model of 51 Peg B
✍ Scribed by C. Goukenleuque; B. Bézard; E. Lellouch
- Book ID
- 110234289
- Publisher
- Springer Netherlands
- Year
- 1998
- Tongue
- English
- Weight
- 57 KB
- Volume
- 81
- Category
- Article
- ISSN
- 1573-0794
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