Consider a star of mass M=10 solar masses, composed entirely of fully ionized 12C. Its core temperature is Tc=6E8 kelvin(compared to Tc=1.5E7 kelvin for the Sun). If the luminosity of the star is L=107 LSun, what is the effective surface temperature?
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Consider a star of mass M=10 solar masses, composed entirely of fully ionized 12C. Its core temperature is Tc=6E8 kelvin(compared to Tc=1.5E7 kelvin for the Sun). If the luminosity of the star is L=107 LSun, what is the effective surface temperature?
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- Given the distance to a star is 276394.84AU, and its apparent magnitude is 4.74. What is the luminosity of the star?Imagine a planet orbiting a star. Observations show a Doppler shift in the star's spectrum of 58 m/s over the 3.3 day orbit of the planet. What is the mass of the planet in kg? Assume the star has the same mass as the Sun (2.0 x1030 kg), there are 365.25 days in a year, and 1AU = 1.5 x 1011 m.When the Sun becomes a red giant, it's luminosity will be 2000 times its current value. The solar flux at Earth will also increase by a factor of 2000. Neglecting the greenhouse effect, the surface temperature of the earth is determined by thermal equilibrium: the flux of radiation absorbed equals the flux of radiation emitted. This means the Earth's surface flux must also increase by a factor of 2000. If the current average surface temperature is 58 degrees F, what will the average surface temperature be when the Sun is a red giant. Express your answer in units of degrees Fahrenheit. [Hint: Recall that the Stefan-Boltzmann law says that the flux F emitted by a blackbody is related to its surface temperature T (measured in Kelvins) is F=σT4 . Use this law in the form of a ratio, expressing T in Kelvins. Then convert back to Fahrenheit.]