Eclipsing binary stars question

In summary, the conversation discusses a figure showing the light curve for an eclipsing binary system with 2 stars, one with a surface temperature of 5000 K and the other with a surface temperature of 10000 K. The ratio of their radii is 4 and the fluxes when one star passes in front of the other are labeled as fa and fb. The question asks to compute the ratios of fa/fnormal and fb/fnormal, but the concept of brightness is also brought up.
  • #1
warfreak131
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Homework Statement



Figure 1 showed the light curve for an exlipsing binary system. This system consists of 2 stars. Star is is the larrger of the stars, and has a surface temp of T1=5000 K. Star 2 has a surface temp of T2=10000K. The ratio of their radii is R1/R2=4. Fnormal is the flux from the system when neither star is blocked. and fa and fb are the fluxes when star 2 passes in front of, or behind star 1, as seen from Earth.

(A)Compute fa/fnormal
(B)Compute fb/fnormal

The light curve looks like this:

http://www.ifa.hawaii.edu/users/mendez/ASTRO110LAB07/modeleb.gif

where the top line is fnormal, the drop at x=.5 is fa, and the drop at x=1 is fb.

Homework Equations



Flux = [tex]{\sigma}T^{4}[/tex]
Brightness = [tex]{\pi}R^{2}{\sigma}T^{4}[/tex]

The Attempt at a Solution



I am being thrown off because the question says compare the fluxes, but just computing the flux doesn't take into account the fact that you are blocking out some light from each star when one passes in front of another. For that I would use brightness, but he makes no mention of using brightness in the question.
 
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  • #2
sorry, i didnt post this in the astronomy section
 

Related to Eclipsing binary stars question

1. What are eclipsing binary stars?

Eclipsing binary stars are a type of binary star system in which two stars orbit around a common center of mass. These stars are close enough together that they appear to pass in front of each other, causing periodic dips in their combined brightness as seen from Earth.

2. How are eclipsing binary stars different from other types of binary stars?

Eclipsing binary stars are unique because they orbit in such a way that their orbital planes are aligned with our line of sight from Earth. This allows us to observe the periodic eclipses and gather information about the stars' properties and orbital dynamics.

3. What can we learn from studying eclipsing binary stars?

Studying eclipsing binary stars allows us to determine the stars' masses, sizes, and distances from each other. By analyzing the light curve during eclipses, we can also gather information about their temperatures, luminosities, and surface compositions.

4. How do astronomers detect eclipsing binary stars?

Eclipsing binary stars are typically detected through their periodic changes in brightness, which can be observed using telescopes or satellites. These changes in brightness are known as eclipses and can help astronomers identify potential binary star systems.

5. Can eclipsing binary stars be used to measure the age of a star system?

Yes, eclipsing binary stars can provide valuable information about the age of a star system. By measuring the stars' properties, such as their masses and luminosities, and using models of stellar evolution, astronomers can estimate the age of the system. This can help us better understand the formation and evolution of stars and their surrounding environments.

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