When we look through a Kepler telescope. The size is determined by looking at the amount of light that passes through the front of a planetary star.
It calculates the year by looking at the time differences that pass through it
Then the atmospheres can be understood by looking at the spectrum of a planet as it moves closer to a star
And when the planet rotates, the star will move slightly because of the gravitational pull. We can find the mass by looking at it.
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