the solar system.
To determine a star's luminosity is from size and temperature.
the size of a star
Its size and temperature.
an increase in temperature or radius causes an increase in luminosity, assuming the other variable doesn't change. luminosity is the total energy output, rather than a measure of energy output against size.
It has to be of sufficient size and luminosity to be visible through a telescope.
I said SIZE! Look in the dicussion for your answers. Choose one!
To determine a star's luminosity is from size and temperature.
Several ways.By its size, orientation, colour, luminosity are some possible criteria.Several ways.By its size, orientation, colour, luminosity are some possible criteria.Several ways.By its size, orientation, colour, luminosity are some possible criteria.Several ways.By its size, orientation, colour, luminosity are some possible criteria.
the size of a star
Its size and temperature.
luminosity and temperature depend on their size but also on their mass
The size of a quasar can be inferred from the timescale of variations in its light output. Assuming that no signal can travel across the source faster than the speed of light, the time scale of the fastest variations sets an upper limit on the size of the quasar (i.e., size quals approximately the variation timescale times speed of light). An alternative method called 'reverberation mapping' monitors changes in the quasar's light output, then looks for these same changes in the light output from specific spectral lines. The delay times the speed of light gives the size of the quasar.
Yes, a average quasar is the size of our solar system
They do not necessarily have greater luminosity, it depends on their size. Betelgeuse is cooler and brighter; a red dwarf is cooler and less bright.
an increase in temperature or radius causes an increase in luminosity, assuming the other variable doesn't change. luminosity is the total energy output, rather than a measure of energy output against size.
A star's real luminosity is proportional to the the square of its diameter, and more or less proportional to the fourth power of its absolute temperature. The star's apparent luminosity is proportional to its real luminosity. It is also inversely proportional to the square of the distance.
It has to be of sufficient size and luminosity to be visible through a telescope.