Discover the Correct Star Radius with These Key Answers | Choose Wisely!

In summary, the article provides essential insights for determining the correct radius of stars, highlighting key questions and answers that guide readers in making informed choices about stellar measurements. It emphasizes the importance of accurate data and methods in astrophysics, encouraging careful consideration of relevant factors when assessing star sizes.
  • #1
wanwa
1
0
Homework Statement
A star shows periodic brightness variations indicating a transiting pair of stars. If the minimum stellar flux is 98.2 percent of the uncapped flux, what is the radius of the other star in that pair, in terms of stellar radius, assuming the other star does not radiate?
Relevant Equations
I have no idea which equations should be used, star Flux is = L / (4πR^2).

Thank you in advance for anyone trying to solve this question. If something odd/wrong with the question let me know (because the original question is on another language).
I have the key answer for this (choosing 1 answer)

A. 0,018

B. 1,134

C. 0,278

D. 0,974

E. 0,982
 
Last edited:
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  • #2
Please show some sort of effort. If you don't know where to start, try explaining what you do understand about the problem and any thoughts you might have on how to solve it.
 
  • #3
wanwa said:
star Flux is = L / (4πR^2).
Are you sure? According to https://en.wikipedia.org/wiki/Radiant_flux, it is the total power, not power per unit area. (And what is L?)
 
  • #4
haruspex said:
Are you sure? According to https://en.wikipedia.org/wiki/Radiant_flux, it is the total power, not power per unit area. (And what is L?)
The equation is fine. However, it's not really relevant here. There's very little maths needed.

The poster is new to the site, so it bears explaining that the response in post #2 was not being cheeky. That's a moderator enforcing forum guidelines on homework help: We don't spell out answers, but we can guide you to them (this is the Way ;) ).

@wanwa just describe what you think an observer would see when looking at the occultation. Or which part of the larger star is giving out light during the event. Think in terms of areas.

Also, ar the risk of potentially giving out the answer, the answer key either contains a mistake or is mistyped in the OP.
 
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FAQ: Discover the Correct Star Radius with These Key Answers | Choose Wisely!

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What is the significance of determining the correct star radius?

Determining the correct star radius is crucial for understanding various stellar properties, such as luminosity, temperature, and evolutionary stage. It also helps in calculating other important parameters like the star's mass and its potential habitability zones for orbiting planets.

What methods are commonly used to measure the radius of a star?

Common methods to measure a star's radius include direct imaging using interferometry, analyzing the star's light curves during eclipsing binary events, and using the star's luminosity and temperature in conjunction with the Stefan-Boltzmann law.

How does the radius of a star affect its luminosity?

The radius of a star directly affects its luminosity. According to the Stefan-Boltzmann law, the luminosity of a star is proportional to the fourth power of its radius and the fourth power of its surface temperature. Thus, even small changes in radius can lead to significant changes in luminosity.

What challenges are faced in accurately determining a star's radius?

Challenges in determining a star's radius include the distance to the star, interstellar dust affecting observations, variability in the star's brightness, and limitations of current technology in resolving distant stars. These factors can introduce uncertainties in the measurements.

Why is it important to choose the correct method for determining a star's radius?

Choosing the correct method for determining a star's radius is important because different methods have varying degrees of accuracy and applicability depending on the star's characteristics and observational data available. Using the most appropriate method ensures more reliable and precise results, which are essential for further astrophysical research and modeling.

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