Explain the difference between the absolute and apparent magnitudes of stars using the Sun as an example.
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Apparent magnitude is how bright the star looks from _here_ (on earth).
A star's apparent magnitude depends not only on how bright the star "really" is (up close); but also how far away it is. Star "A" may be putting out 100 times as much light as Star "B"; yet B may look brighter to _us_ just becase B is so much closer. In that case we say the _apparent_ magnitude of B is brighter than the _apparent_ magnitude of A.
But suppose you could take a space ship so you were exactly 10 parsecs away from Star "A"; and then take another trip to 10 parsecs away from Star "B". In that case, you would definitely be able to tell that "A" was the brighter star, because you compared the two from the same distance. So we say the _absolute_ magnitude of A is brighter than the _absolute_ magnitude of B.
The absolute magnitude is one way of describing how much light a star actually puts out, rather than just how bright it happens to look from earth.
As relates to the sun: The _apparent_ magnitude of the sun is extremely bright (because we're so close to it). Its _absolute_ magnitude (how it would look from 10 parsecs away) would be much, much dimmer.
Apparent magnitude describes the brightness of a particular object, or star, AS WE SEE IT, with all of the interfering gas and dust in the light path to our eyes.
Apparent magnitudinal values are always lower than absolute magnitudinal values, with the exception of near Earth objects (the Sun, the Moon, solar system planets, asteroids, etc.)
I'm pretty sure that's it.
Yeah, that's it.
Think of absolute and apparent size - If you hold a quarter out at arms length, it's apparent size is the same as the sun or the moon. The Sun and the moon are obviously A LOT bigger, but the quarter is alot closer.
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