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tris_d
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Drakkith said:Look at my explanation of the Sun. As long as the Sun is larger than 1 square arcminute in apparent size, you will see the same amount of light coming from that square arcminute of sky. When the Sun is smaller than 1 square arcminute we can switch to a smaller unit, such as square arcseconds, and the process is still the same. No matter how close or far the Sun is, the amount of light from each square arcminute is exactly the same. The only difference is the total apparent size of the Sun as a whole. A few stars further away than the Sun could be positioned to take up the same apparent area of sky as the Sun did, and the result would be the same.
Now extrapolate from that to other stars. If every star was the same as the Sun, then every single section of sky that falls on a star would be exactly the same brightness. Closer stars would be larger in apparent size, but that is irrelevant as I just explained. Stars further away would add together and fill up the view between the gaps of closer stars.
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\ -- -- -- -- / |- 2r
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\ ---- ---- / |- 1r
\ / |
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Four further stars not only leave less bright imprints, but there is also more "black" between and around them, so I conclude: while the total emitted intensity is the same, perceived overall brightness of the second shell is much less.
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