Astronomers use a special term to talk about the brightness of stars. The term is "magnitude". The magnitude scale was invented by the ancient Greeksaround 150 B.C. The Greeks put the stars they could see into six groups. They put the brightest stars into group 1, and called them magnitude 1 stars. Stars that they could barely see were put into group 6. So, in the magnitude scale, bright stars have lower numbers.
a stars brightness as seen from Earth
Brightness of stars (apparent and absolute magnitude) is measured by convention, taking an another star as a standard.
1) absolute brightness 2) distance 3) intervening dust
Theres `Absolute Magnitude` which is the brightness of a star at a set distance. Then there is `Apparent Magnitude` which is the apparent brightness from earth, regardless of distance.
An apparent brightness is the brightness of a star as measured by an observer.
The measure of a star's brightness is its magnitude. A star's brightness as it appears from Earth is called its Apparent Magnitude.Star's brightness is measured by there magnitude.
a stars brightness as seen from Earth
The measure of a star's brightness is its magnitude. A star's brightness as it appears from Earth is called its Apparent Magnitude.Star's brightness is measured by there magnitude.
Brightness of stars (apparent and absolute magnitude) is measured by convention, taking an another star as a standard.
Both relate to brightness; both are measured in the same units; both are used for astronomical objects such as stars or galaxies.
No - a star as seen from earth is it's apparentbrightness. It's absolute brightness is measured by astronomical instruments. The brightest visible star from earth is Sirius, in the constellation Canis Major. Spica, in Virgo, has a much higher absolute brightness than Sirius, but Sirius is much closer to earth, so it is apparently brighter than Spica.
midorz
false
Distance from Earth, size of star, and temperature of star.
Distance from Earth, size of star, and temperature of star.
1) absolute brightness 2) distance 3) intervening dust
For nearby stars, the parallax method is used. Briefly, the star's apparent position changes, due to Earth's movement around the Sun. For objects that are farther away, several "standard candle" methods are used, meaning that the brightness of objects is measured that are assumed to have a more or less constant brightness; for example, "the brightest stars of a certain type of star, in a galaxy".