How do we know galaxies are exactly where we see them?

Click For Summary

Discussion Overview

The discussion revolves around the question of how we can be certain that distant galaxies and planets are located where we observe them, considering the time it takes for light to travel from these objects to Earth. Participants explore implications of light travel time, the effects of gravitational lensing, and the challenges of estimating distances to celestial objects.

Discussion Character

  • Exploratory
  • Debate/contested
  • Technical explanation

Main Points Raised

  • Some participants express doubt about the accuracy of locating distant galaxies and planets due to the finite speed of light, suggesting that we are seeing the past and questioning whether these objects are still in the same position.
  • Others introduce gravitational lensing as a phenomenon that complicates our perception of the location of galaxies, proposing that light can be bent by massive objects, leading to potential misinterpretations of their positions.
  • One participant discusses the limitations of distance estimation for celestial objects, noting that while parallax can provide accurate measurements for nearby stars, it becomes less reliable for more distant objects, which rely on other methods with greater uncertainty.
  • Another participant suggests that when considering travel to a distant exoplanet, it is necessary to calculate its future position rather than its past location, due to the time delay in light travel.
  • One contribution details how the proper and radial motion of stars can be measured, providing a method to adjust for their movement over time when aiming for a target star.
  • Some participants note that while galaxies move slowly compared to the speed of light, the uncertainty in their current positions increases with distance, particularly for objects observed billions of years ago.
  • A later reply challenges the idea that proper motion is trivial compared to recession velocity, suggesting that there is a known amount of distance based on the expansion of the universe.

Areas of Agreement / Disagreement

Participants express a range of views, with some agreeing on the challenges of determining current positions of distant objects while others contest specific aspects of motion and distance estimation. The discussion remains unresolved with multiple competing perspectives on the implications of light travel time and motion of celestial objects.

Contextual Notes

Limitations include the dependence on various methods for distance estimation, the effects of gravitational lensing, and the assumptions made regarding the motion of celestial objects over time. There are unresolved mathematical steps related to the calculations of proper and radial motions.

Armando Valle
Messages
28
Reaction score
0
i have a doubt, how do we know far away (light years) galaxies and planets are on the right spot we see them? if light takes a lot of time to reach the Earth it means we are seeing the past of the galaxy/planet. Example: If Earth is becoming extinct and we need to find an exoplanet 30,000 light years away, when we are going to the direction we saw it on the telescope it would be there because we saw the past of the galaxy from Earth and wouldn't be able to find it. can someone give me a solution? thanks
 
Astronomy news on Phys.org
Another example can be gravitational lensing, a massive object of something that have a lot of gravitational pulse can bend light of where we see it, so we can see galaxies from another place in front of us, the universe is a very mysterious thing... it could be that everything we see far away could be scrambled away from all places of the universe and is nerve-racking.
 
The further away from Earth a celestial object, the less accurate is our estimate of how far away it is.

For objects whose distances can be estimated by parallax, the estimates are pretty good. For objects much further away, parallax cannot be used to estimate distances, and other means, like measuring the magnitudes of certain stars or observing supernova explosions in distant galaxies, can provide rough estimates of distance, but the uncertainty is rather large.

https://en.wikipedia.org/wiki/Cosmic_distance_ladder

I wouldn't worry too much about navigating between stars and galaxies just yet. We have not returned to the Moon in almost half a century, and that body is only a quarter million miles away.
 
  • Like
Likes   Reactions: |Glitch|
Armando Valle said:
Example: If Earth is becoming extinct and we need to find an exoplanet 30,000 light years away, when we are going to the direction we saw it on the telescope it would be there because we saw the past of the galaxy from Earth and wouldn't be able to find it. can someone give me a solution? thanks

It's not that we would need to know where that planet is 'now', it's that we would have to calculate where it will be in the future in order to get the right trajectory to get to this planet. It's an unavoidable effect of the finite speed of light and spaceships.
 
Armando Valle said:
i have a doubt, how do we know far away (light years) galaxies and planets are on the right spot we see them? if light takes a lot of time to reach the Earth it means we are seeing the past of the galaxy/planet. Example: If Earth is becoming extinct and we need to find an exoplanet 30,000 light years away, when we are going to the direction we saw it on the telescope it would be there because we saw the past of the galaxy from Earth and wouldn't be able to find it. can someone give me a solution? thanks

When we look at a star we can also tell how fast it is moving with respect to us. This is divided into two types of motion, its proper motion ( at right angles to the viewing line) and its radial motion ( along the viewing line). So let's take a star Mu Cephei which is 6000 light years away. it has a proper motion of ~ 6 mas/yr ( a mas is a milli-arcsecond or 1/3600000 of a degree) and a radial motion of - 20.63 km/sec. So in the 6000 yrs since the light left it has moved 3.9e12 km closer to the Earth, or about 1/2424 of a light year. In that same 6000 years it also will have moved 1/100 of a degree in terms of proper motion.( where we see it now is 1/100 of degree from the direction it actually is in.)

So if we were to head to that star at 0.5 light speed for example, we would aim for for a point 3/100 of a degree from where the star is. Of course, that would just be our initial aiming point. We would likely have to adjust our course slightly as we traveled to make up for inaccuracies in our initial measurements or course heading. But the main point is that the star is not going to have moved that much that we can't just point ourselves pretty much in the direction we see it in and then make minor course corrections along the way
 
Last edited:
ohh, nice Drakkith i liked the "now" from where will it be in the future, however thanks!
 
Galaxies move slowly compared to the speed of light. If we look deep deep into space, yeah, we have no idea where things might be now. There are Hubble pictures of galaxies 12 billion years ago, we couldn't hope to guess where that galaxy actually is now. Things closer to us, however, are much easier. Part of the reason it took humans so long to realize that the stars actually moved is because they do it so so slowly. If you went 10,000 years into the future, the night sky would look more or less the same. Some of the closest stars may have move a little, but they move at tens of thousands miles an hour, not a hundred of thousand a second like light does.
 
newjerseyrunner said:
Galaxies move slowly compared to the speed of light. If we look deep deep into space, yeah, we have no idea where things might be now. There are Hubble pictures of galaxies 12 billion years ago, we couldn't hope to guess where that galaxy actually is now. Things closer to us, however, are much easier. Part of the reason it took humans so long to realize that the stars actually moved is because they do it so so slowly. If you went 10,000 years into the future, the night sky would look more or less the same. Some of the closest stars may have move a little, but they move at tens of thousands miles an hour, not a hundred of thousand a second like light does.
The part I've bolded in your post, I disagree with. Their proper motion relative to us is likely to be trivial compared to their recession velocity relative to us so we have quite a good idea where they are ... they are along the same line of sight (more or less) but a known amount farther away based on their farther recession due to to 12 billion more years of expansion.
 

Similar threads

  • · Replies 7 ·
Replies
7
Views
2K
  • · Replies 12 ·
Replies
12
Views
2K
  • · Replies 13 ·
Replies
13
Views
3K
  • · Replies 148 ·
5
Replies
148
Views
13K
  • · Replies 3 ·
Replies
3
Views
2K
  • · Replies 7 ·
Replies
7
Views
2K
  • · Replies 2 ·
Replies
2
Views
2K
  • · Replies 4 ·
Replies
4
Views
2K
  • · Replies 25 ·
Replies
25
Views
3K
  • · Replies 2 ·
Replies
2
Views
1K