Not exact matches
This involves determining the composition of a planetary atmosphere by measuring its spectra, the distinctive radiation that gases
absorb at their own
particular wavelengths.
Since different elements and compounds
absorb light
at characteristic
wavelengths, astronomers can determine what chemicals make up a planet's atmosphere by measuring the relative amounts of light that come in
at particular wavelengths.
Planets with atmospheres are able to warp starlight in another way: while the body of the planet blocks a big chunk of starlight as it crosses in front of its host star, the planet's thin, enveloping atmosphere
absorbs starlight
at particular colors, or
wavelengths.
If there is a greater density of CO2 molecules, then the probability of a
particular photon,
at one of these
wavelengths that CO2
absorbs, coming across a CO2 molecule, is clearly increased.