How Does the Size of an Eclipsing Planet Affect Star Brightness?

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The size of a planet eclipsing a star affects the star's brightness by comparing the area of the planet's disk to that of the star's disk, using the formula area = pi r^2. During an eclipse, the brightness changes due to the subtraction of the planet's area from the star's, leading to a rise, a peak, and a decline in brightness. Limb darkening introduces complexity, but the brightness is generally proportional to the visible fraction of the star's surface area obscured by the planet. Unlike the Moon-Sun eclipse, the star-planet scenario can be treated as if viewed from an infinite distance, simplifying calculations. Understanding these dynamics is crucial for accurate modeling of stellar brightness during eclipses.
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how does the size of planet eclipsing a star effect the brightness of the star?
thanks.
 
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think about when the moon gets in the way of the sun.
 
Picture the star as a disk of light. And the planet, as a disk of darkness.

Subtract the area of the planet's disk from the area of the star's disk to compare eclipse / non-eclipse brightness. Limb darkening complicates it a bit, so you'll see a rise, a sharp peak and a decline. (Area = pi r^2)

This is a bit different than an eclipse of the Sun by the Moon. Both Sun and Moon are close enough to affect the ratio of their actual sizes and their appearant sizes. But at their distances, the ratio of their actual sizes and their appearant sizes is very, very close to 1. A star and its planet can be treated as if at an infinate perspective.
 
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right, but is brightness directly proportional to the apparent area we see? probably a stupid question, but thanks
 
skiboka33 said:
right, but is brightness directly proportional to the apparent area we see?
Roughly proportional to the visible fraction of the surface area, yes. There are effects like limb darkening that complicate the picture a bit, but for the most part, eclipses can be modeled as simply as this.
 
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