2024年10月24日 · WASP-31 b is a gas giant exoplanet that orbits a F-type star. Its mass is 0.478 Jupiters, it takes 3.4 days to complete one orbit of its star, and is 0.04659 AU from its star. Its …

WASP-31b is a low-density (puffy) "hot Jupiter" extrasolar planet orbiting the metal-poor (63% of solar metallicity) dwarf star WASP-31. [1] The exoplanet was discovered in 2010 by the WASP …

Detailed information about planet WASP-31 b and its parameters. How do wavelength correlations affect transmission spectra? Application of a new fast and flexible 2D Gaussian …

2010年11月25日 · We report the discovery of the low-density, transiting giant planet WASP-31b. The planet is 0.48 Jupiter masses and 1.55 Jupiter radii. It is in a 3.4-day orbit around a metal …

WASP-31b is a planet of 0.5 Jupiter masses that is bloated up to 1.5 Jupiter radii. This gives it a large atmospheric scale height that makes it a good target for transmission spectroscopy, …

2023年8月28日 · First discovered in 2011, WASP-31b is a so-called hot Jupiter exoplanet. It has a mass of 0.5 times that of Jupiter and a radius of 1.5 Jupiter radii, making it one of the lowest …

Investigating giant planet migration history via improved eccentricity and mass determination for 231 transiting planets. New and updated stellar parameters for 90 transit hosts. The effect of …

2023年8月28日 · Now, Flagg and a Cornell-led team of researchers have confirmed, using high-resolution spectral observations, the presence of chromium hydride in an exoplanet …

2023年8月28日 · Now, Flagg and a Cornell-led team of researchers have confirmed, using high-resolution spectral observations, the presence of chromium hydride in an exoplanet …

2023年8月29日 · Now, Flagg and a Cornell-led team of scientists have confirmed, using high-resolution spectral observations, the presence of chromium hydride in an exoplanet …