How can scientists point a telescope at a distant star or planet and confidently say “this one is ice with a methane atmosphere” or whatever? How do they know if that’s true?

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How can scientists point a telescope at a distant star or planet and confidently say “this one is ice with a methane atmosphere” or whatever? How do they know if that’s true?

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Spectroscopy! My favorite scientific advancement of all time: trying to figure out why substances make those patterns in a prism was what led to quantum physics, trying to explain why the patterns change frequencies in distant galaxies led to discovering the big bang, and in the meantime it’s just a very practical tool for measuring substances remotely based on light.

So yeah, if you pass the light from a star or planet through a prism (or diffraction grating these days) you get [a pattern that might look like this](https://www.cloudynights.com/uploads/monthly_04_2008/post-11401-14072472558332_thumb.jpg) and the particular dark bands form a “fingerprint” identifying the various substances.

A distant planet outside our solar system, I don’t think we can separate its light directly like that. But we can watch how the spectrum of the parent star changes as its planet moves behind/alongside/in front of the star, reflecting or absorbing light according to its atmosphere.

There’s other clues, other methods, but that’s a big one.