Calculating distance to a star using magnitudes

In summary, The conversation revolved around solving a problem involving the absolute magnitude of an object. The equation ##m = m_0 − 2.5 log_{10} f## was discussed, with the attempt to find the absolute V-band magnitude of Star A using Vega's value. However, the observed/apparent magnitude of Star A remains unknown and the R-band magnitude of Vega is needed to proceed with the problem.
  • #1
samjohnny
84
1

Homework Statement


Obs.JPG


Homework Equations


##m = m_0 − 2.5 log_{10} f## where ##m## is the absolute magnitude of an object, and ##m_0## is the zero point.

The Attempt at a Solution



I'm having difficulty with is part b, the answer to which I believe is required for the subsequent parts.

I obtain the following through treatment of the given equation: ##M_{abs}=m_{obs}-5log_5(\frac{d}{10})## where ##d## is the distance we're looking to compute. Using the fact that both Star A and Vega are A0 stars, I assumed that the absolute V-band magnitude of Star A would be the same as Vega's, which would be ##M_{abs}=+0.6##, however the observed/apparent magnitude ##m_{obs}## remains unknown, and so I'm unable to proceed to compute the distance.

It seems simple, but I can't quite put my finger on it..
 
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  • #2
You'll need the R-band magnitude of Vega I think. The question part about the colors indicates that you have to find some relation between R and V band.
Afterwards you can use the R band magnitude from (a).
 

1. How do you calculate the distance to a star using magnitudes?

The distance to a star can be calculated using the formula d = 10^(m-M+5)/5, where d is the distance in parsecs, m is the apparent magnitude of the star, and M is the absolute magnitude of the star.

2. What is the difference between apparent magnitude and absolute magnitude?

Apparent magnitude is the measure of a star's brightness as seen from Earth, while absolute magnitude is the measure of a star's intrinsic brightness. Absolute magnitude takes into account the distance of the star from Earth, while apparent magnitude does not.

3. How accurate is the distance calculated using magnitudes?

The accuracy of the distance calculated using magnitudes depends on the accuracy of the values used in the formula. Small errors in the values of m and M can lead to significant differences in the calculated distance. However, with precise measurements, the distance can be calculated with high accuracy.

4. Can the distance to a star be calculated using other methods besides magnitudes?

Yes, there are other methods for calculating the distance to a star, such as parallax, spectroscopic parallax, and the period-luminosity relationship for variable stars. Each method has its own strengths and limitations, and the most appropriate method may vary depending on the characteristics of the star being studied.

5. How are magnitudes used in astronomy?

Magnitudes are used to measure the brightness of celestial objects such as stars and galaxies. They are also used to classify objects based on their brightness, with lower magnitudes indicating brighter objects. Magnitudes are an important tool in studying the properties and distances of objects in the universe.

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