Fraction of incident flux that escapes from a star

In summary, the formula for the fraction of incident flux that escapes from a star is F=F0*e^k(R^-2-r0^-2) and the percentage of flux that escapes is found by dividing F(R)/F(r) or F(2R)/F(r).
  • #1
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If the flux entering such an atmosphere from the core of the star at a radius is r0 is F0,
the flux that reaches radius r is given by

F(r)=F0*e^k(r^-2-r0^-2)

where k is a constant

a) Write down a formula for the fraction of the incident flux that escapes from the star
entirely. {3}
b) If 50% of the flux escapes from a star where the base of this stellar atmosphere lies at a
radius r0, what percentage of the flux escapes if this atmosphere only starts at twice as
large a radius? {3}



Is the answer to (a) just F=F0*e^k(R^-2-r0^-2) where R=radius of star and then to find the fraction you just do F(R)/F(r)?

Thanks :)
 
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  • #2
Yes, that is correct. To answer part (b), you can use the same formula and plug in twice the radius for R. Then, the fraction of the flux that escapes is F(2R)/F(r).
 

1. What is the fraction of incident flux that escapes from a star?

The fraction of incident flux that escapes from a star is known as the albedo. It is the amount of light that is reflected away from the star compared to the total amount of light that is incident upon it.

2. How is the fraction of incident flux that escapes from a star calculated?

The fraction of incident flux that escapes from a star is calculated by dividing the amount of light that is reflected (albedo) by the total amount of light that is incident upon the star. This can be expressed as a percentage or a decimal value.

3. What factors affect the fraction of incident flux that escapes from a star?

The fraction of incident flux that escapes from a star is affected by several factors including the composition of the star's atmosphere, the star's surface temperature, and the wavelength of light being considered. These factors can impact the amount of light that is absorbed, reflected, and transmitted by the star's atmosphere.

4. How does the fraction of incident flux that escapes from a star relate to its overall brightness?

The fraction of incident flux that escapes from a star is directly related to its overall brightness. A higher albedo means that more light is being reflected away from the star, resulting in a lower overall brightness. On the other hand, a lower albedo means that more light is being absorbed and/or transmitted, resulting in a higher overall brightness.

5. Why is the fraction of incident flux that escapes from a star important to study?

Studying the fraction of incident flux that escapes from a star can provide valuable insights into the composition and characteristics of the star's atmosphere. It can also help scientists understand the star's energy balance and its impact on its surrounding environment. Additionally, understanding the albedo of a star can aid in the search for habitable planets and the potential for life in other solar systems.

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