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Q: What is the relationship between Luminosity and Temp for main sequence stars?
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What correctly describes the relationship between the luminosity of two stars that have the same radius?

The star that is hotter will have a higher luminosity.


Relationship between stars distance to earth and luminosity?

Generally speaking, the apparent luminosity would be an inverse square relationship, which is to say, if the same star was at twice the distance, a quarter of the light would be reaching the observer. But absolute luminosity can of course vary without regard to distance from Earth - dim stars can be close, or bright stars distant, or vice-versa.


Do the stars on the main sequence illustrate the mass-luminosity relationship?

Luminosity depends directly on mass because more massive main-sequence stars do not need to graviationally contract as far to reach fusion temperatures, and so they have a larger volume and contain a much larger amount of light energy, which diffuses out and generates a higher luminosity, very roughly in proportion to the higher volume.


Which type of star best obey mass-luminosity relation?

Main sequence stars


How do you measure the distance to a cepheid?

Cepheids have a certain relationship between their period, and their absolute luminosity. Thus, their absolute luminosity can be determined. Comparing this with their apparent luminosity allows us to calculate their distance.Cepheids have a certain relationship between their period, and their absolute luminosity. Thus, their absolute luminosity can be determined. Comparing this with their apparent luminosity allows us to calculate their distance.Cepheids have a certain relationship between their period, and their absolute luminosity. Thus, their absolute luminosity can be determined. Comparing this with their apparent luminosity allows us to calculate their distance.Cepheids have a certain relationship between their period, and their absolute luminosity. Thus, their absolute luminosity can be determined. Comparing this with their apparent luminosity allows us to calculate their distance.

Related questions

What is the rleationship between luminosity and tempeature for stars on the main sequence?

On a logarithmic scale for luminosity, it is quite close to a negative linear relationship.


Which statement describes the general relationship between temperature and luminosity of main sequence stars?

as surface temperature increases, luminosity increases


Are main sequence stars called medium sized stars?

No. Main sequence stars are simply stars that are fusing hydrogen into helium and have a specific relationship between color and luminosity. They range from red dwarfs to large O-type main sequence stars.


What describes the relationship between the luminosity of two stars that have the same radius?

The star that is hotter will have a higher luminosity.


What correctly describes the relationship between the luminosity of two stars that have the same radius?

The star that is hotter will have a higher luminosity.


Which of the following luminosity classes refers to stars on the main sequence?

The basic luminosity classes are: I for supergiants, III for giants, and V for main-sequence stars.


What is the relationship between luminosity and temperature for main sequence stars?

On such a diagram, those stars lie on a curve called the "main sequence". It is not a simple relationship - for example, it isn't a straight line on the diagram. Therefore, it isn't easy to describe in words. It's best if you look up "Main sequence", for example on the Wikipedia, and look at the corresponding diagram.


What is the general relationship between the temperature and the luminosity of main sequence stars?

The scatter plot of the relationship between a star's temperature and luminosity is represented by the Hertzsprung-Russell diagram. In a standard H-R diagram the horizontal axis shows the [surface] temperature, increasing from right to left, while the vertical axis shows luminosity increasing from bottom to top. When both axis are on a logarithmic scale, the main sequence stars from a diagonal belt stretching from top right (very hot and very luminous) to bottom left (not so hot and not so luminous).


What is the use of Hertzsprung Russell diagram?

It shows the relationship between stars luminosity versus their classifications and effective temperatures


How does star color relate to mass?

There is no simple relation. The color does not depend only on the mass. The same star can change color, without a significant change in mass. For example, our Sun is currently yellow; in a few billion years, it is expected to get much larger, becoming a red giant. However, if we limit the sample of stars to those on the "main sequence" of the "HR diagram", there is something of a relation between mass and color. The most massive stars are blue or white. They are also hottest and most luminous. The least massive are the red dwarf stars, which are relatively cool and dim. Our Sun, which is a "main sequence" star at present, is somewhere in between those extremes. (There is a strong relationship between mass and luminosity for main sequence stars. The HR diagram, of course, shows there is a relationship between luminosity and color for the main sequence stars.)


Relationship between stars distance to earth and luminosity?

Generally speaking, the apparent luminosity would be an inverse square relationship, which is to say, if the same star was at twice the distance, a quarter of the light would be reaching the observer. But absolute luminosity can of course vary without regard to distance from Earth - dim stars can be close, or bright stars distant, or vice-versa.


Do the stars on the main sequence illustrate the mass-luminosity relationship?

Luminosity depends directly on mass because more massive main-sequence stars do not need to graviationally contract as far to reach fusion temperatures, and so they have a larger volume and contain a much larger amount of light energy, which diffuses out and generates a higher luminosity, very roughly in proportion to the higher volume.