
K2-18b
2015 CE
Reading a Planet's Air from Far Away
K2-18b was first detected because it passes in front of its host star, causing tiny, regular dips in brightness. When the planet transits, some starlight filters through its atmosphere, imprinting spectral fingerprints that telescopes can measure. Interpreting those spectra requires careful modelling, and small differences in assumptions can change whether a signal looks like water vapour, methane, or something else.
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K2-18b was first detected because it passes in front of its host star, causing tiny, regular dips in brightness. When the planet transits, some starlight filters through its atmosphere, imprinting spectral fingerprints that telescopes can measure. Interpreting those spectra requires careful modelling, and small differences in assumptions can change whether a signal looks like water vapour, methane, or something else.






























































