Phase Light Curves for Extrasolar Jupiters and Saturns
نویسندگان
چکیده
منابع مشابه
Phase light curves for extrasolar Jupiters and Saturns
We predict how a remote observer would see the brightness variations of giant planets similar to those in our Solar System as they orbit their central stars. We model the geometry of Jupiter, Saturn and Saturn’s rings for varying orbital and viewing parameters. Scattering properties for the planets and rings at wavelenghts 0.6-0.7 microns are assumed to follow these observed by Pioneer and Voya...
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We present results from Spitzer Space Telescope observations of the mid-infrared phase variations of three short-period extrasolar planetary systems: HD 209458, HD 179949 and 51 Peg.We gathered Infrared Array Camera (IRAC) images in multiple wavebands (3.6 μm or 4.5 μm, and 8 μm) at eight phases of each planet’s orbit. We find the uncertainty in relative photometry from one epoch to the next to...
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We present results from Spitzer Space Telescope observations of the mid-infrared phase variations of three short-period extrasolar planetary systems: HD 209458, HD 179949 and 51 Peg.We gathered Infrared Array Camera (IRAC) images in multiple wavebands (3.6 μm or 4.5 μm, and 8 μm) at eight phases of each planet’s orbit. We find the uncertainty in relative photometry from one epoch to the next to...
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We have created a general methodology for calculating the wavelength-dependent light curves of close-in extrasolar giant planets (EGPs) as they traverse their orbits. Focussing on the transiting EGPs HD189733b, TrES-1, and HD209458b, we calculate planet/star flux ratios during secondary eclipse and compare them with the Spitzer data points obtained so far in the mid-infrared. We introduce a sim...
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We explore the infrared spectrum of a three-dimensional dynamical model of planet HD 209458b as a function of orbital phase. The dynamical model predicts dayside atmospheric pressure-temperature profiles that are much more isothermal at pressures less than 1 bar than one-dimensional radiative-convective models have found. The resulting dayside thermal spectra are very similar to a blackbody, an...
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ژورنال
عنوان ژورنال: The Astrophysical Journal
سال: 2005
ISSN: 0004-637X,1538-4357
DOI: 10.1086/426050