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Hydroxyl molecule signature detected in an ultra-hot Jupiter exoplanet

Astronomers obtain the first direct evidence of hydroxyl molecules in the atmosphere of a planet beyond the Solar System. Artist’s impression of an ultra-hot Jupiter exoplanet, WASP-33b. Image credit Astrobiology Center An international collaboration of astronomers led by a researcher from the Astrobiology Center and Queen’s University Belfast, and including researchers from Trinity College Dublin, has detected a new chemical signature in the atmosphere of an extrasolar planet (a planet that orbits a star other than our Sun). The hydroxyl radical (OH) was found on the dayside of the exoplanet WASP-33b. This planet is an “ultra-hot Jupiter”, a gas-giant planet orbiting its host star much closer than Mercury orbits the Sun and therefore reaching atmospheric temperatures of more than 2,500°C (hot enough to melt most metals).

Astronomers detect first ever hydroxyl molecule signature in an exoplanet atmosphere

Astronomers detect first ever hydroxyl molecule signature in an exoplanet atmosphere
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Astronomers Detect New Chemical Signature in an Exoplanet s Atmosphere

Astronomers Detect New Chemical Signature in an Exoplanet’s Atmosphere April 27th 2021, 1:08 pm This planet is a so-called ultra-hot Jupiter, a gas-giant planet orbiting its host star much closer than Mercury orbits the sun Image Credit: Share Email An international collaboration of astronomers led by a researcher from the Astrobiology Center and Queen’s University Belfast has detected a new chemical signature in the atmosphere of an extrasolar planet i.e., a planet that orbits a star other than our sun. The hydroxyl radical (OH) was found on the dayside of the exoplanet WASP-33b. This planet is a so-called ‘ultra-hot Jupiter,” a gas-giant planet orbiting its host star much closer than Mercury orbits the sun (Figure 1) and therefore reaching atmospheric temperatures of more than 2500 degrees C (hot enough to melt most metals).

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