File:Atmospheric Methane of Brown Dwarfs W1935 and W2220 (NIRSpec) (2024-103).tiff

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Astronomers used NASA’s James Webb Space Telescope to study 12 cold brown dwarfs. Two of them – W1935 and W2220 – appeared to be near twins of each other in composition, brightness, and temperature.

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English: Astronomers used NASA’s James Webb Space Telescope to study 12 cold brown dwarfs. Two of them – W1935 and W2220 – appeared to be near twins of each other in composition, brightness, and temperature. However, W1935 showed emission from methane, as opposed to the anticipated absorption feature that was observed toward W2220. The team speculates that the methane emission may be due to processes generating aurorae. NASA, ESA, CSA, Leah Hustak (STScI)
Date 9 January 2024, 16:15:00 (upload date)
Source Atmospheric Methane of Brown Dwarfs W1935 and W2220 (NIRSpec)
Author Illustration NASA, ESA, CSA, Leah Hustak (STScI)
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Public domain This file is in the public domain because it was created by NASA, ESA and CSA. NASA Webb material is copyright-free and may be freely used as in the public domain without fee, on the condition that only NASA, STScI, and/or ESA/CSA is credited as the source of the material. This license does not apply if source material from other organizations is in use.
The material was created for NASA by Space Telescope Science Institute under Contract NAS5-03127. Copyright statement at webbtelescope.org.
For material created by the European Space Agency on the esawebb.org site, use the {{ESA-Webb}} tag.

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current10:37, 10 January 2024Thumbnail for version as of 10:37, 10 January 202416,000 × 10,226 (135.44 MB)OptimusPrimeBot (talk | contribs)#Spacemedia - Upload of https://stsci-opo.org/STScI-01HKMVR7FMANXRNTKFC5W00CYB.tif via Commons:Spacemedia

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