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<blockquote style="position: relative; padding-left: 55px;"><section><a href="https://fosstodon.org/users/AkaSci/statuses/114350616757462526">AkaSci 🛰️ (akasci@fosstodon.org)'s status on Thursday, 17-Apr-2025 21:34:41 JST</a><a href="https://fosstodon.org/@AkaSci" title="akasci@fosstodon.org"><img src="https://gnusocial.jp/avatar/20805-48-20221219024513.webp" width="48" height="48" alt="AkaSci 🛰️" style="position: absolute; left: 0; top: 0;">AkaSci 🛰️</a><div><a href="https://fosstodon.org/@AkaSci/114350562719494367" rel="in-reply-to">in reply to</a></div></section><article><p>The team led Dr. Madhusudhan had published data on planet K2-18 b in 2023, with detection of Methane, CO2 and even dimethyl sulfide using the JWST.</p><p>There were exciting discussions at the time about the possibility of life on K2-18 b, but the data was weak and further study was warranted.</p><p>The new announcement is apparently based on additional observations by JWST made in 2024.</p><p>As we know, extraordinary claims require extraordinary evidence. Time will tell.</p><p><a href="https://www.nasa.gov/universe/exoplanets/webb-discovers-methane-carbon-dioxide-in-atmosphere-of-k2-18-b/" rel="nofollow noreferrer">https://www.nasa.gov/universe/exoplanets/webb-discovers-methane-carbon-dioxide-in-atmosphere-of-k2-18-b/</a><br>2/</p></article><footer><a rel="bookmark" href="https://gnusocial.jp/conversation/4906763#notice-9616799">In conversation</a><time datetime="2025-04-17T21:34:41+09:00" title="Thursday, 17-Apr-2025 21:34:41 JST">about 10 days ago</time> <span>from <span><a href="https://fosstodon.org/@AkaSci/114350616757462526" rel="external" title="Sent from fosstodon.org via ActivityPub">fosstodon.org</a></span></span><a href="https://fosstodon.org/@AkaSci/114350616757462526">permalink</a><h4>Attachments</h4><ol><li><label><a rel="external" href="https://gnusocial.jp/attachment/4480860">
Spectra of K2-18 b, obtained with Webb’s NIRISS (Near-Infrared Imager and Slitless Spectrograph) and NIRSpec (Near-Infrared Spectrograph), display an abundance of methane and carbon dioxide in the exoplanet’s atmosphere, as well as a possible detection of a molecule called dimethyl sulfide (DMS). The detection of methane and carbon dioxide, and shortage of ammonia, support the hypothesis that there may be a water ocean underneath a hydrogen-rich atmosphere in K2-18 b. K2-18 b, 8.6 times as massive as Earth, orbits the cool dwarf star K2-18 in the habitable zone and lies 120 light-years from Earth.
Illustration: NASA, CSA, ESA, R. Crawford (STScI), J. Olmsted (STScI), Science: N. Madhusudhan (Cambridge University)</a></label><br><a href="https://cdn.fosstodon.org/media_attachments/files/114/350/570/803/515/777/original/20548d7461c8fa82.jpeg" rel="external">https://cdn.fosstodon.org/media_attachments/files/114/350/570/803/515/777/original/20548d7461c8fa82.jpeg</a></li><li><label><a rel="external" href="https://gnusocial.jp/attachment/4480861">Untitled attachment</a></label><br></li></ol></footer></blockquote>

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AkaSci 🛰️ (akasci@fosstodon.org)'s status on Thursday, 17-Apr-2025 21:34:41 JST AkaSci 🛰️
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The team led Dr. Madhusudhan had published data on planet K2-18 b in 2023, with detection of Methane, CO2 and even dimethyl sulfide using the JWST.
There were exciting discussions at the time about the possibility of life on K2-18 b, but the data was weak and further study was warranted.
The new announcement is apparently based on additional observations by JWST made in 2024.
As we know, extraordinary claims require extraordinary evidence. Time will tell.
https://www.nasa.gov/universe/exoplanets/webb-discovers-methane-carbon-dioxide-in-atmosphere-of-k2-18-b/
2/
In conversationabout 10 days ago from fosstodon.orgpermalink
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1. Spectra of K2-18 b, obtained with Webb’s NIRISS (Near-Infrared Imager and Slitless Spectrograph) and NIRSpec (Near-Infrared Spectrograph), display an abundance of methane and carbon dioxide in the exoplanet’s atmosphere, as well as a possible detection of a molecule called dimethyl sulfide (DMS). The detection of methane and carbon dioxide, and shortage of ammonia, support the hypothesis that there may be a water ocean underneath a hydrogen-rich atmosphere in K2-18 b. K2-18 b, 8.6 times as massive as Earth, orbits the cool dwarf star K2-18 in the habitable zone and lies 120 light-years from Earth. Illustration: NASA, CSA, ESA, R. Crawford (STScI), J. Olmsted (STScI), Science: N. Madhusudhan (Cambridge University)
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