Archivo de imágenes de Hubble

Atmósferas nubladas versus despejadas en los exoplanetas WASP-67 b y HAT-P-38 b

This diagram compares Hubble Space Telescope observations of two "hot Jupiter"-class planets orbiting very closely to different sunlike stars. Astronomers measured how light from each parent star is filtered through each planet's atmosphere. Hubble near-infrared observations were...

Fecha
Jan 1, 2017
Misión
Hubble Space Telescope
ID de archivo
hubblesite-images-2017-22-4050-image
Por

This diagram compares Hubble Space Telescope observations of two "hot Jupiter"-class planets orbiting very closely to different sunlike stars. Astronomers measured how light from each parent star is filtered through each planet's atmosphere. Hubble near-infrared observations were used to measure the spectral fingerprint caused by the presence of water vapor in the atmosphere. HAT-P-38 b did have a water signature indicated by the absorption-feature peak in the spectrum. This is interpreted as indicating the upper atmosphere is free of clouds or hazes. By contrast, a very similar hot Jupiter, WASP-67 b, has a flat spectrum that lacks any water-absorption feature. This suggests that most of the planet's atmosphere is masked by high-altitude clouds.

Credits

Artwork

NASA, ESA, Zena Levy (STScI)

Science

NASA, ESA, Giovanni Bruno (STScI)

Detalles de la imagen

About The Object
Object NameHAT-P-38 b WASP-67 b
Object DescriptionExtrasolar planet
R.A. PositionHAT-P-38 b: 02h 21m 31.9s; WASP-67b: 19h 42m 59.0s
Dec. PositionHAT-P-38 b: +32° 14' 46"; WASP-67 b: -19° 56' 58"
DistanceHAT-P-38 b: 812 light-years (249 parsecs); WASP-67 b: 734 light-years (225 parsecs)
DimensionsHAT-P-38 b is is 0.825 times Jupiter's diameter. WASP-67 b is 2.8 times Jupiter's diameter
About The Data
Data DescriptionThe data used in the HAT-P-38 b and WASP-67 b studies were from proposal , P.I. Drake Deming (University of Maryland).
InstrumentHST>WFC3/IR
Exposure DatesHAT-P-38 b: Mar. 2, 2016 - Aug. 26, 2016; WASP-67 b: Oct. 22, 2016
FiltersHAT-P-38 b: WFC3/IR G141 (red grism), 282 minutes WASP-67 b: WFC3/IR G141 (red grism), 108 minutes

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