1-24 (24 pages) This tutorial is an introduction to techniques used to characterize the atmospheres of transiting exoplanets. We intend it to ... phase curves, transit spectroscopy, and convolution ...

As planets pass in front of their parent stars as viewed from Earth, they cause a tiny dip in the amount of starlight we ...

Astronomers measured how light from each parent star is filtered through each planet's atmosphere. HAT-P-38 b did have a water signature indicated by the absorption-feature peak in the spectrum.

Astronomers largely circumvent this problem by instead observing the side of an exoplanet ... and atmosphere. However, such observations are more time-consuming than transit spectroscopy.

An alien world with a seemingly sulphur-filled atmosphere may be the most volcanic ... aren’t powerful enough to take images of exoplanets’ surfaces. We might be able to spot alien volcanoes ...

WASP-17 b is one of the largest and puffiest known exoplanets. This, along with its short orbital period of just 3.7 Earth-days, makes the planet ideal for transmission spectroscopy: a technique ...

"The rate at which the planet is evaporating is utterly cataclysmic, and we are incredibly lucky to be witnessing the final hours of this dying planet." ...

One of the big highlights of the release of the first science data from the James Webb Space Telescope was the spectrum of an exoplanet atmosphere ... Object Slitless Spectroscopy (SOSS) mode.

If you buy through a BGR link, we may earn an affiliate commission, helping support our expert product labs. New data found by researching one of the most extreme exoplanets we know of could help ...

The transmission spectrum of the exoplanet WASP-39b is obtained using observations from the Single-Object Slitless Spectroscopy ... absorption feature at 4.05 μm arising from SO 2 in the ...