I First atmospheric spectroscopy of Earth-sized exoplanets

AI Thread Summary
The Hubble telescope has successfully conducted the first atmospheric spectroscopy of Earth-sized exoplanets TRAPPIST-1b and TRAPPIST-1c, confirming that a large hydrogen/helium atmosphere is unlikely. TRAPPIST-1, located 40 light years away, is smaller and cooler than the sun, providing ideal conditions for studying atmospheric interactions with sunlight. While Hubble cannot detect specific gases like ozone or methane, it identifies promising candidates for further investigation with advanced telescopes such as JWST, E-ELT, GMT, and TMT. The E-ELT will have a mirror surface area equivalent to the 20 largest existing telescopes combined, enhancing future research capabilities. The ongoing development of sunshade missions remains uncertain, with no recent significant funding reported.
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The Hubble telescope lead to the first spectroscopy of the atmospheres of two Earth-sized exoplanets, TRAPPIST-1b and TRAPPIST-1c. A large hydrogen/helium atmosphere could be ruled out - not that surprising, but still nice to have this confirmed.

The main star, TRAPPIST-1, is just 40 light years away and significantly smaller and cooler than our sun, and the two planets transit it as seen from Earth. Ideal viewing conditions to study how the sunlight gets absorbed or scattered by the atmosphere.

Hubble is not sensitive enough to search for gases like ozone, water vapor, or methane, but it can help to find candidates that can be investigated further with the upcoming better telescopes - JWST in space, and E-ELT*, GMT and TMT on the ground.

*the E-ELT will have as much mirror surface as the 20 largest existing telescopes combined.

Further details:
University website
http://www.nature.com/nature/journal/vaop/ncurrent/full/nature18641.html
 
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It has been around as idea for a while, but I don't think there is any sunshade mission that got significant funding.
 
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