Bulk composition of the transiting hot Neptune around GJ 436
نویسندگان
چکیده
منابع مشابه
Transit Infrared Spectroscopy of the Hot Neptune Around GJ 436 with the Hubble Space
The nearby transiting system GJ 436b offers a unique opportunity to probe the structure and atmosphere of an extra-solar “hot Neptune”. In this Letter, we present the main results of observations covering two transit events with the NICMOS camera on the Hubble Space Telescope. The data consist of high-cadence time series of grism spectra covering the 1.1-1.9 μm spectral range. We find Rpl = 4.0...
متن کاملTransit infrared spectroscopy of the hot Neptune around GJ 436 with the Hubble Space Telescope★
The nearby transiting system GJ 436b offers a unique opportunity to probe the structure and atmosphere of an extra-solar “hot Neptune”. In this Letter, we present the main results of observations covering two transit events with the NICMOS camera on the Hubble Space Telescope. The data consist in high-cadence time series of grism spectra covering the 1.1-1.9 μm spectral range. We find Rpl = 4.0...
متن کاملThe M Dwarf GJ 436 and its Neptune - Mass Planet
We determine stellar parameters for the M dwarf GJ 436 that hosts a Neptunemass planet. We employ primarily spectral modeling at low and high resolution, examining the agreement between model and observed optical spectra of five comparison stars of type, M0-M3. Modeling high resolution optical spectra suffers from uncertainties in TiO transitions, affecting the predicted strengths of both atomi...
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We present a detailed analysis of the dayside atmosphere of the hot-Neptune GJ 436b, based on recent Spitzer observations. We report statistical constraints on the thermal and chemical properties of the planetary atmosphere, study correlations between the various molecular species, and discuss scenarios of equilibrium and non-equilibrium chemistry in GJ 436b. We model the atmosphere with a one-...
متن کامل0 v 2 4 D ec 2 00 6 The M Dwarf GJ 436 and its Neptune - Mass Planet
We determine stellar parameters for the M dwarf GJ 436 that hosts a Neptunemass planet. We employ primarily spectral modeling at low and high resolution, examining the agreement between model and observed optical spectra of five comparison stars of type, M0-M3. Modeling high resolution optical spectra suffers from uncertainties in TiO transitions, affecting the predicted strengths of both atomi...
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ژورنال
عنوان ژورنال: Astronomy & Astrophysics
سال: 2008
ISSN: 0004-6361,1432-0746
DOI: 10.1051/0004-6361:20078951