k TRAPPIST1Image provided TRAPPIST1 exoplanet system. Illustration of two of the Earthsized exoplanets in the TRAPPIST1 system transiting their parent star. The planets TRAPPIST1b and TRAPPIST1c are the black dots passing across the face of the star as seen from Earth. The atmospheres of the planets were studied using NASAs Hubble Space Telescope. The results indicate an increased chance of these worlds being habitable. Spectroscopic analysis revealed a low concentration of hydrogen and helium in the planetary atmospheres. The planets orbit a red dwarf star that is at least 500 million years old, located 39 light years away in the constellation of Aquarius. This rare double transit occurred on 4 May 2016. The planets were studied as part of the SPECULOOS survey. Editorial Stock Photo - Afloimages
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TRAPPIST 1  Image provided  TRAPPIST 1 exoplanet system. Illustration of two of the Earth sized exoplanets in the TRAPPIST 1 system transiting their parent star. The planets  TRAPPIST 1b and TRAPPIST 1c  are the black dots passing across the face of the star as seen from Earth. The atmospheres of the planets were studied using NASA s Hubble Space Telescope. The results indicate an increased chance of these worlds being habitable. Spectroscopic analysis revealed a low concentration of hydrogen and helium in the planetary atmospheres. The planets orbit a red dwarf star that is at least 500 million years old, located 39 light years away in the constellation of Aquarius. This rare double transit occurred on 4 May 2016. The planets were studied as part of the SPECULOOS survey.
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TRAPPIST-1 (Image provided)

TRAPPIST-1 exoplanet system. Illustration of two of the Earth-sized exoplanets in the TRAPPIST-1 system transiting their parent star. The planets (TRAPPIST-1b and TRAPPIST-1c) are the black dots passing across the face of the star as seen from Earth. The atmospheres of the planets were studied using NASA's Hubble Space Telescope. The results indicate an increased chance of these worlds being habitable. Spectroscopic analysis revealed a low concentration of hydrogen and helium in the planetary atmospheres. The planets orbit a red dwarf star that is at least 500 million years old, located 39 light years away in the constellation of Aquarius. This rare double transit occurred on 4 May 2016. The planets were studied as part of the SPECULOOS survey.

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38151235

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License type
Editorial

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Creation date
23-02-2017

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