Finding the magnitude difference between two star

In summary, the apparent magnitude difference between Sirius and the Sun is approximately 7.15, and Sirius is approximately 2195.83 times more luminous than the Sun.
  • #1
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Homework Statement



Determine the apparent magnitude difference between sirius and the sun,as seen from the Earth. How much more luminosity is sirius than the Sun ?

Homework Equations



f=sigma*T^4(eff)
m-n=2.5*log(f(m)/f(n))

The Attempt at a Solution



the apparent magnitude difference is m-n, m and n being the apparent magnitudes being the sun and sirius. I probably need the find the flux of each star. the flux=5.67e-8 W/(m^2*K^4)*T^4(eff). 30000 K is the effective temperature of Sirius and T(eff)=5780 K for the sun. f(sirius)/f(sun)=(30000 K)^4/(5780)^4=726 . Therefore, m(sirius)-n(sun)=2.5*log(726)=7.152
 
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  • #2
. The apparent magnitude difference between Sirius and the Sun is approximately 7.15.

To determine the luminosity difference between Sirius and the Sun, we can use the equation L=4*pi*R^2*f, where L is the luminosity, R is the radius, and f is the flux. The radius of Sirius is approximately 1.71 times that of the Sun (based on their respective effective temperatures and using the Stefan-Boltzmann law), so we can calculate the luminosity ratio as:

L(sirius)/L(sun) = (1.71)^2 * (726) = 2195.83

Therefore, Sirius is approximately 2195.83 times more luminous than the Sun. This is expected, as Sirius is known to be one of the brightest stars in the sky.
 
  • #3
. This means that Sirius appears 7.152 magnitudes brighter than the sun from Earth.

To determine the luminosity difference between Sirius and the sun, we can use the formula L=4*pi*R^2*f, where L is the luminosity, R is the radius, and f is the flux. The radius of Sirius is approximately 1.71 times that of the sun, so the luminosity of Sirius is 4*pi*(1.71)^2*726=17274 times that of the sun. This means that Sirius is approximately 17274 times more luminous than the sun.
 

1. What is the definition of magnitude difference between two stars?

The magnitude difference between two stars is the numerical difference in their apparent brightness as seen from Earth. It is usually measured on a logarithmic scale, with a difference of 5 magnitudes representing a brightness difference of 100 times.

2. How is the magnitude difference calculated?

The magnitude difference is calculated by subtracting the apparent magnitude of one star from the apparent magnitude of the other star. The resulting number is the difference in magnitude between the two stars.

3. Why is the magnitude difference important in astronomy?

The magnitude difference is important in astronomy because it allows us to quantify and compare the brightness of stars. This information can help us understand the properties and characteristics of the stars, such as their distance, size, and temperature.

4. Can the magnitude difference change over time?

Yes, the magnitude difference between two stars can change over time. This can be due to a variety of factors, such as changes in the stars' luminosity or their relative positions in the sky as seen from Earth.

5. How is the magnitude difference used in the classification of stars?

The magnitude difference is often used in the classification of stars, as it provides a way to measure and compare their brightness. For example, the difference in magnitude between a star's visual and infrared brightness can help determine its color and temperature, which are important factors in classifying stars.

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