
WASP-67 b - Science@NASA
2024年10月24日 · WASP-67 b is a gas giant exoplanet that orbits a K-type star. Its mass is 0.43 Jupiters, it takes 4.6 days to complete one orbit of its star, and is 0.05179 AU from its star. Its discovery was announced in 2012.
WASP-67 - Wikipedia
WASP-67 is a K-type main-sequence star about 620 light-years away. The stars age is poorly constrained, but is likely older than the Sun`s at approximately 8.7+5.5
WASP-67b: Exoplanet with iron rainfall is even more extreme than ... - CNN
2021年10月5日 · Droplets of iron rain fall from the sky at night on WASP-67b, a sizzling exoplanet about the size of Jupiter. Now, researchers have also detected calcium in the planet’s atmosphere.
WASP-67 b - exoplanetkyoto.org
WASP-67 b is an exoplanet orbiting the star WASP-67, located about 628.4 light-years (192.7 pc) away from Solar System. Its discovery was publicly announced on 2011. The host star WASP-67 has apparent magnitude of 12.5, with absolute magnitude of 6.1. It is 0.9 times more massive and 0.9 times bigger compared with our Sun.
The grazing transit of WASP-67b - WASP Planets
2014年7月1日 · The hot-Jupiter exoplanet WASP-67b is a curiosity, being the only known exoplanet with a grazing transit, such that not all of the planet transits the host-star's disc. This means that the characteristic "second contact" and "third contact" points are missing from the transit lightcurves.
Seven transiting hot Jupiters from WASP-South, Euler and TRAPPIST: WASP ...
2012年10月11日 · We present seven new transiting hot Jupiters from the WASP-South survey. The planets are all typical hot Jupiters orbiting stars from F4 to K0 with magnitudes of V = 10.3–12.5. The orbital periods are all in the range of 3.9–4.6 d, the planetary masses range from 0.4 to 2.3 MJup and the radii from 1.1 to 1.4 RJup.
WASP-67b – WASP Planets
The hot-Jupiter exoplanet WASP-67b is a curiosity, being the only known exoplanet with a grazing transit, such that not all of the planet transits the host-star’s disc.
A comparative study of WASP-67b and HAT-P-38b from WFC3 data
2017年12月9日 · WASP-67 b, with mass 0.27 M and radius 0.83 , shows a more muted water absorption feature than that of HAT-P-38 b, indicating either a higher cloud deck in the atmosphere or a more metal-rich composition. The difference in the spectra supports the hypothesis that giant exoplanet atmospheres carry traces of their formation history.
WASP-67b - astro.vaporia.com
WASP -67b is a transiting hot Jupiter orbiting a K-type star (0.91 solar masses) in a 4-day orbit. Characteristics: Host star: WASP 67. Discovery: by the transit method in 2011. 190 pc - distance. 0.05 AU - orbital radius. 4.6 days - orbital period. 1.15 - radius in Jupiter radii. 0.43 - Jupiter masses. 1050 K - equilibrium temperature.
Planet WASP-67 b
High-resolution Imaging of Transiting Extrasolar Planetary systems (HITEP). I. Lucky imaging observations of 101 systems in the southern hemisphere. Detailed information about planet …
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