Relative Stargazing: Adjusting Time Distortion for True Representation

In summary, the time it takes for a star's light to reach us can give us a slightly distorted view of the night sky, but the effect is minimal because the stars with the largest proper motions are typically closer to us. This may have some impact on modeling objects in space, but for the majority of stars that are farther away and have small proper motions, the distortion is insignificant.
  • #1
Jellymeat
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Does the time taken for a stars light to reach us, relative to it's true position as it moves through the galaxy give us a time distorted view of the night sky? I assume so, has there ever been an attempt to adjust this time distortion to give us a true representation of what we are really looking at?

Would this potentially affect how we model objects in space, given that our photography gives us misrepresentations?
 
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  • #2
The difference would be pretty insignificant. The stars with the largest proper motions tend to be the closer stars and light takes less time to reach us from them. For example 61 Cygni has one of the highest proper motions, but is only 11.35 light years distant. With its proper motion, in 11.35 years it will have shift position by about 1 arc min, or approximately 1/30 the width of the Moon.

The majority of the stars we see at night are very bright stars that are farther away. Consequently, they have small proper motions. Polaris, the north star is 430 light years away, but has a small proper motion. In the time it takes for its light to reach us, it will only have shifted 20 arc sec, or 1/90 of the width of the Moon.
 

1. What is relative stargazing?

Relative stargazing is a technique used in astronomy to adjust for time distortion caused by the speed of light. It allows us to see celestial objects as they truly are in the present moment, rather than how they appeared in the past due to the time it takes for their light to reach us.

2. How does relative stargazing work?

Relative stargazing works by taking into account the distance between Earth and a celestial object, as well as the speed of light. By calculating the time it takes for the light from the object to reach us, we can adjust our observations to account for the time it took for the light to travel.

3. Why is relative stargazing important?

Relative stargazing is important because it allows us to see celestial objects as they are in the present moment. This is especially useful when studying objects that are extremely far away, as their light may have taken millions or even billions of years to reach us, and without adjustment, we would only see them as they appeared in the past.

4. Can relative stargazing be used for all celestial objects?

Yes, relative stargazing can be used for all celestial objects. However, it is most commonly used for objects that are very far away, such as galaxies, quasars, and other deep space objects.

5. Are there any limitations to relative stargazing?

There are some limitations to relative stargazing. One limitation is that it requires precise measurements of distance and the speed of light, which can be challenging for objects that are extremely far away. Additionally, relative stargazing can only account for time distortion caused by the speed of light, and not other factors such as gravitational time dilation.

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