he transmission spectrum obtained by Webb observations of rocky exoplanet GJ 486 b (IMAGE)
Caption
This graphic shows the transmission spectrum obtained by Webb observations of rocky exoplanet GJ 486 b. The science team’s analysis shows hints of water vapor; however, computer models show that the signal could be from a water-rich planetary atmosphere (indicated by the blue line) or from starspots from the red dwarf host star (indicated by the yellow line). The two models diverge noticeably at shorter infrared wavelengths, indicating that additional observations with other Webb instruments will be needed to constrain the source of the water signal.
Credit
Credits: NASA, ESA, CSA, Joseph Olmsted (STScI)
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License
Public Domain