Several methods exist.
A fairly obvious one is the parallax method - while Earth moves around the Sun, it changes its position by about 300 million km.; this will change the apparent position of nearby stars.
For star clusters or galaxies that are further away, several "standard candle" methods exist, which basically consist of comparing the real luminosity of objects that have a known brightness (like certain types of stars) with their apparent luminosity.
what is the type of star used by the Hubble to measure the distance to other galaxies.
It means that the distance is greater than a certain amount - depending on how precisely you can measure the parallax.
Distance. Absolute magnitude is a measure of the intrinsic brightness of a star, independent of its distance from Earth.
It means that the distance is greater than a certain amount - depending on how precisely you can measure the parallax.
The distance to a star can be determined using the measure of parallax by observing the star from two different points in Earth's orbit around the Sun. By measuring the apparent shift in the star's position against more distant background stars, astronomers can calculate the star's distance based on the angle of the parallax.
The apparent movement of a star used to measure its distance from Earth is called parallax. Astronomers observe how a star's position changes relative to more distant stars as Earth orbits the Sun, allowing them to calculate the star's distance based on the angle of this shift.
The most basic way to measure the distance to a star is through parallax. This involves observing the shift in the star's position as seen from different points in Earth's orbit, allowing astronomers to calculate the star's distance based on its apparent movement.
parallax
No, a star's absolute magnitude is a measure of its intrinsic brightness regardless of its distance from the observer. It is a standardized measure that allows for comparison of the brightness of stars at a set distance.
Astronomers use a method called parallax to measure the distance to nearby stars. By observing how a star's position changes when viewed from different points in Earth's orbit around the Sun, astronomers can calculate the star's distance based on the angle of this apparent shift.
Most of the time we use light years, but their are other units to measure distance such as parsecs and arcminutes.
At farther distances, the parallax becomes too small to measure accurately. At a distance of 1 parsec, a star would have a parallax of 1 second (1/3600 of a degree). (The closest star, Toliman, is a little farther than that.) At a distance of 100 parsecs, the parallax is only 1/100 of a second.