Astronomy - Parallax error calculation.

In summary, to find the distance to two stars in the same cluster with measured parallax angles, you can use the formula D = 1/p where D is the distance in pc and p is the parallax in arcseconds. To calculate the combined distance, you will need to use the formula for error propagation, taking into account the errors in both measurements. It is always a good idea to double check your calculations for accuracy.
  • #1
knowlewj01
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Homework Statement



Two stars belong to the same cluster, the parallax measured to one star is
(2±1)x10^-3 arcseconds, towards the other the parallax is
(4±2)x10^-3 arcseconds.

Find the distance to both objects seperatly and also compute the distance when both measurements are combined.


Homework Equations



D = [tex]\frac{1}{p}[/tex]

where D is the distance in pc
and p is the parallax in arcseconds

The Attempt at a Solution



If it weren't for the error in the parallax angle this would be easy but I'm not sure how to go about it. here is my attempt at it:

Star 1: D = 1/p = 500pc

calculating error in D: ([tex]\Delta[/tex]D)^2 = ([tex]\frac{dD}{dp}[/tex][tex]\Delta[/tex]p)^2

([tex]\Delta[/tex]D)^2 = ([tex]\frac{1}{p^2}[/tex][tex]\Delta[/tex]p)^2

([tex]\Delta[/tex]D)^2 = (250000 x 0.001)^2

([tex]\Delta[/tex]D) = ± 15.8 pc

does this seem reasonable?
I'm not too great with error calculation, does this seem right?

I have done exactly the same for the second star, have no idea what the last bit of the question means at all 'when both measurements are combined'. anyone have any ideas?
 
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  • #2




Thank you for your question. Your approach to calculating the distance to each star is correct. However, to find the combined distance, you will need to use the formula for error propagation. This formula takes into account the errors in both measurements to give a more accurate estimate of the combined distance.

The formula for error propagation is as follows:

(\DeltaD)^2 = (\frac{dD}{dp_1}\Deltap_1)^2 + (\frac{dD}{dp_2}\Deltap_2)^2

where D is the combined distance, p1 and p2 are the parallax angles for the first and second star respectively, and Delta p1 and Delta p2 are their corresponding errors.

Using this formula, you can calculate the combined distance for the two stars. This will give you a more accurate estimate of the distance to the cluster.

In addition, it is always a good idea to double check your calculations and make sure they seem reasonable. In this case, your calculated error for the distance to each star seems reasonable, but it is always a good idea to check your calculations with a calculator or by hand to make sure you are not making any mistakes.

I hope this helps and good luck with your calculations!
 

1. What is parallax error in astronomy?

Parallax error in astronomy is the apparent shift in the position of an object due to the change in the observer's viewing angle. This error occurs when measuring the distance of a celestial object using the parallax method.

2. How is parallax error calculated?

Parallax error is calculated by taking the difference between the observed position and the true position of an object, and dividing it by the distance between the observer and the object. This gives the angle of parallax, which can then be used to correct for the error.

3. Why is parallax error important in astronomy?

Parallax error is important in astronomy because it can affect the accuracy of measurements, especially when determining the distances of celestial objects. It is crucial to account for and correct this error to obtain precise and reliable data.

4. How does parallax error impact the measurement of distances in astronomy?

Parallax error can impact the measurement of distances in astronomy by introducing a margin of error in the results. The larger the parallax angle, the larger the error in the distance measurement. This is why it is important to minimize and correct for parallax error when making astronomical observations.

5. Can parallax error be eliminated completely?

No, parallax error cannot be eliminated completely. However, it can be minimized by using more precise instruments and techniques, such as reducing the distance between the observer and the object, taking multiple measurements, and calculating the average. Additionally, advanced methods, such as interferometry, can be used to further reduce parallax error in astronomical measurements.

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