Due to the inverse square law, stars that are far away from Earth are generally dimmer than stars that are close to Earth. However, there are many exceptions, since stars can also appear brighter or dimmer depending on their luminosity.
If the same star (or a star of the same absolute (real) brightness) is farther away, it will look less bright to us. Specifically there is an inverse-square law; for example, at ten times the distance, it would appear 100 times dimmer - assuming we can ignore other effects, such as light extinction through interstellar gas or dust.
If the same star (or a star of the same absolute (real) brightness) is farther away, it will look less bright to us. Specifically there is an inverse-square law; for example, at ten times the distance, it would appear 100 times dimmer - assuming we can ignore other effects, such as light extinction through interstellar gas or dust.
If the same star (or a star of the same absolute (real) brightness) is farther away, it will look less bright to us. Specifically there is an inverse-square law; for example, at ten times the distance, it would appear 100 times dimmer - assuming we can ignore other effects, such as light extinction through interstellar gas or dust.
If the same star (or a star of the same absolute (real) brightness) is farther away, it will look less bright to us. Specifically there is an inverse-square law; for example, at ten times the distance, it would appear 100 times dimmer - assuming we can ignore other effects, such as light extinction through interstellar gas or dust.
The brighter and bigger a star is than the shorter it's life span will be because the star uses up all of it's hydrogen fuel on being so bright and big the the star will then collapse in on itself and turn into a white dwarf star.
If the same star (or a star of the same absolute (real) brightness) is farther away, it will look less bright to us. Specifically there is an inverse-square law; for example, at ten times the distance, it would appear 100 times dimmer - assuming we can ignore other effects, such as light extinction through interstellar gas or dust.
Its called the inverse square law.
Stars twice as far away are one quarter as bright. (3 times as far, one 9th as bright, etc).
Their distance away from you and their intrinsic luminosity.
The relationship between the planet's SPEED and its distance from the Sun is given by Kepler's Third Law.From there, it is fairly easy to derive a relationship between the period of revolution, and the distance.
To find the number of light years between two celestial objects, we first find the distance from each object to earth. If we connect the dots between Earth and the two objects, we have a triangle. We to sides lengths of that triangle (the distances between Earth and the objects), and we can measure one angle (the angle at the vertex where Earth is. This is enough information to find the distance between the objects using trigonometry (in this case, the law of cosines). Finding the distance from Earth to an object can be a bit complex. One commonly used method is to look for a pulsating star. We can figure out the absolute brightness (how bright it is without factoring in distance away) of these stars by how often they pulse. Then we can measure the apparent brightness (how bright it looks to us). We can then use both these values to find the distance to the star. (This also works for some supernovae.) Another method is to use objects that are considered to be 'standard candles'. These objects do not pulse, but we know the relationship between their absolute brightness, apparent brightness, and distance away.
True!
the planets
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With maths and light brightness.... Distance between two points...
Time = (distance) divided by (speed) Distance = (speed) multiplied by (time) Speed = (distance) divided by (time)
Absolute Brightness: How bright a star appears at a certain distance. Apparent Brightness: The brightness of a star as seen from Earth.
Describe the relationship between mass and weight.
As temperature increases the absolute brightness increases
Brightness tells you the temperature and mostly temperature would tell the brightness of the star that we are talking about.
Hertzsprung and Russell.
Hertzsprung and Russell.
um Long-distance relationship?
edwin hubble
scale