Astronomy - binary magnitude conceptual question

In summary, in order to determine a star's trigonometric parallax, at least three measurements of its position relative to distant objects are needed. This is because all objects involved are constantly moving, and by taking measurements from multiple reference points, the position of the star can be accurately determined. Factors such as light obscuration from dust can also affect the star's position in the sky.
  • #1
accountkiller
121
0
astronomy - conceptual, trigonometric parallax

Homework Statement


To determine a star's trigonometric parallax, we need at least 3 measurements of its position relative to much more distanct objects. Explain why this is true. (What else could change its position on the sky?)

Homework Equations


Note - this is for galactic astronomy.

The Attempt at a Solution


Well, I understand what triangulation is.. take a measurement of the angle Earth at one end of its elliptical orbit and then six months alter at the other end, so you have the distance between, and with angles can figure out the distance to the star. But this question is asking relative to other distant objects, not Earth... so I'm not sure how to proceed thinking about it. What could change its position in the sky... light obscuration from dust, perhaps?

I'd appreciate any guidance, thanks!
 
Last edited:
Physics news on Phys.org
  • #2
Try drawing a picture for each situation. Draw one where you take measurements relative to just one star, just two stars and then just three stars. If you already know the position of these stars, then you only need to do this once to get the position of the fourth.

What could change it's position in the sky?
Remember that everything in this problem is moving, and each object may be moving in different ways relative to each other.
 
  • #3
Got it. Thank you :)
 

Related to Astronomy - binary magnitude conceptual question

1. What is binary magnitude in astronomy?

In astronomy, binary magnitude refers to the brightness of a binary star system as seen from Earth. It is a measure of the combined magnitude of both stars in the system.

2. How is binary magnitude calculated?

Binary magnitude is calculated by adding together the individual magnitudes of each star in the system. The magnitude scale is logarithmic, meaning that a difference of 5 magnitudes represents a difference of 100 times in brightness.

3. What is the difference between visual and absolute binary magnitude?

Visual binary magnitude is the apparent magnitude of the system as seen from Earth, while absolute binary magnitude is the true magnitude of the system, taking into account the distance from Earth. Absolute magnitude is often used to compare the brightness of different binary star systems.

4. How does the distance between binary stars affect their binary magnitude?

The distance between binary stars does not directly affect their binary magnitude, but it can impact their apparent magnitude if they have a wide separation. In a close binary system, the combined brightness of the two stars will appear brighter, while in a wide binary system, the combined brightness will appear dimmer.

5. Can binary magnitude change over time?

Yes, binary magnitude can change over time due to various factors such as changes in the stars' brightness, orbital changes, and other phenomena. These changes can be observed and studied by astronomers to better understand the behavior and evolution of binary star systems.

Similar threads

  • Introductory Physics Homework Help
Replies
10
Views
2K
  • Introductory Physics Homework Help
Replies
6
Views
2K
  • Introductory Physics Homework Help
Replies
1
Views
1K
  • Astronomy and Astrophysics
Replies
7
Views
1K
Replies
21
Views
1K
Replies
5
Views
1K
  • Astronomy and Astrophysics
Replies
10
Views
4K
  • Introductory Physics Homework Help
Replies
1
Views
2K
  • Astronomy and Astrophysics
Replies
1
Views
1K
  • Astronomy and Astrophysics
Replies
22
Views
3K
Back
Top