Different methods are used for different stars. For stars that are relatively near to us, the parallax method is used. This means that - as Earth moves around the Sun, and changes its position by about 300 million kilometers (2 AU) within half a year (and then back again) - the apparent position of the observed star will change. The larger this angle, the nearer the star is to us. For more details, do some reading (e.g., in the Wikipedia) about the parallax method. For other methods (for stars or galaxies that are further away), check the Wikipedia article on "cosmic distance ladder".
Distance from Earth, size of star, and temperature of star.
Distance from Earth, size of star, and temperature of star.
Your place on the earth, The brightness of the star, Its distance.
use a piggy bank and measure the distance from the piggy bank and a star
1) absolute brightness 2) distance 3) intervening dust
parallax
Each star has a different distance.
They use trigonometry to determine the distance to nearby stars. They measure the star's positions at one point in time, and again six months later, calibrating against the backdrop of the far distant stars. The nearby stars will show a parallax shift in position, so they calculate a triangle, with the Earth at two points, and the base 186 million miles long. The star is the third point on the triangle, and it is simple trigonometry from there to figure out the distance.
Passive voice: It has always been hard to determine distance to the stars. Present voice. As always, it is difficult to determine the distance to the stars. Future participle: According to Einstein, it will always be difficult to determine if relativity is correct. Object; What is a sentence of always?
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Each star in Scorpius is a different distance from the other stars.
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