How to Calculate Angular Diameter of a Galaxy with a Given Diameter?

In summary, the angular diameter of a galaxy is a measure of its size as seen from Earth, calculated using the small angle formula and providing important information about its size, distance, and appearance. This diameter can change over time due to various factors, but these changes are often small and require long-term measurements.
  • #1
P-Jay1
32
0
If I know the diameter of a galaxy in the sky is 150 arcseconds,

how do I find the angular diameter?
 
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  • #2
150 arcseconds is the angular diameter.
 
  • #3
phyzguy said:
150 arcseconds is the angular diameter.

I just realized damn
 

1. What is the angular diameter of a galaxy?

The angular diameter of a galaxy is a measure of the size of the galaxy as seen from Earth, expressed in degrees. It is the angle between two imaginary lines drawn from the observer to opposite points on the galaxy's edge.

2. How is the angular diameter of a galaxy calculated?

The angular diameter of a galaxy is typically calculated using the small angle formula, which takes into account the distance to the galaxy and its physical diameter. This formula is θ = d/D, where θ is the angular diameter, d is the physical diameter of the galaxy, and D is the distance to the galaxy.

3. Why is the angular diameter of a galaxy important?

The angular diameter of a galaxy is important because it provides information about the size and scale of the galaxy. It can also help astronomers determine the distance to the galaxy and its place in the universe.

4. How does the angular diameter of a galaxy affect its appearance?

The angular diameter of a galaxy can greatly affect its appearance. A larger angular diameter means the galaxy will appear larger and more spread out in the sky, while a smaller angular diameter will make the galaxy appear smaller and more compact.

5. Can the angular diameter of a galaxy change?

Yes, the angular diameter of a galaxy can change over time. This can be due to a variety of factors, such as the expansion of the universe or the movement of the galaxy itself. However, these changes are often very small and can only be measured over long periods of time.

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