Titan possesses a thick N2-CH4 atmosphere that makes it difficult to study its surface spectroscopically. The chemical composition of the solid surface of Titan thus remains very uncertain. By leveraging JWST’s high sensitivity and large spectral coverage, we searched for any signature from Titan’s surface in the broad and less explored 5-μm atmospheric window. We […] The post An Unidentified Absorption Feature At 5.11 μm On The Surface Of Titan…
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