James Webb Telescope Reveals Sand Clouds a...

Spectroscopic observations from JWST unveil the atmospheric composition of WASP-107b, revealing silicate rain ! Swipe to see →

A SPECTACULAR DISCOVERY IN THE ATMOSP...

Astronomers operating the James Webb Space Telescope have released unprecedented spectroscopic data on the atmosphere of exoplanet WASP-1...

THE UNIQUE DYNAMICS OF THE SAND RAIN ...

Unlike the gas planets in our solar system, WASP-107b has an average atmospheric temperature of five hundred degrees Celsius. In this ext...

THE CHEMISTRY OF SULFUR DIOXIDE AND T...

One of the most surprising findings from the spectral analysis was the unambiguous identification of sulfur dioxide in the atmosphere of ...

TRANSMISSION SPECTROSCOPY WITH THE JA...

The technique employed to characterize the atmosphere of WASP-107b is known as transit transmission spectroscopy. As the exoplanet crosse...

THE RELATIONSHIP BETWEEN HOST STAR AN...

The host star, known as WASP-107, is a K-type orange dwarf slightly cooler and less massive than our Sun. Despite its moderate luminosity...

INTERNAL STRUCTURE AND THE NATURE OF ...

With a mass equivalent to just thirty times that of Earth spread over a volume nearly equal to Jupiter, WASP-107b has a mean density of o...

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