Astronomy - Measure distance to other galaxies

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Discussion Overview

The discussion revolves around methods for measuring distances to celestial objects, particularly stars and galaxies, including those that are very far away, such as superclusters. Participants explore various techniques and their implications, touching on both theoretical and observational aspects.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested
  • Mathematical reasoning

Main Points Raised

  • Some participants note that the parallax method is effective for nearby stars but becomes less accurate for distant objects.
  • Others describe the use of Cepheid variables, which have brightness cycles related to their distance, as a method for measuring distances to nearby galaxies like Andromeda.
  • Type Ia supernovae are mentioned as another distance measurement method, with their consistent characteristics allowing for distance estimation based on their light output.
  • One participant emphasizes that no single method is used to calculate distances; instead, multiple methods provide bounds and margins of error that can be combined for more reliable results.
  • There is mention of cosmological effects, such as Hubble's law, being relevant for estimating distances at larger scales, particularly beyond millions of light-years.
  • Some participants express skepticism about the concept of dark energy, suggesting it may be a response to observations of the universe's accelerating expansion, while others defend the scientific reasoning behind it.
  • Several participants highlight the ongoing search for new methods to measure extragalactic distances, indicating that the field is still evolving.

Areas of Agreement / Disagreement

Participants generally agree on the existence of multiple methods for measuring astronomical distances, but there is no consensus on the implications of these methods or the validity of dark energy as an explanation for cosmic observations. The discussion remains unresolved regarding the best approaches and interpretations of the data.

Contextual Notes

Limitations include the dependence on various assumptions and definitions related to distance measurement methods, as well as the unresolved nature of certain observational errors and their impact on the conclusions drawn from different techniques.

tosv
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I have understand that the Parallax method can be used to measure the distance to stars, but what happens when the parallax angle gets to small to be measures accurate?

What kind of methods are used to measure distance to star that are like 5000 light years away, or to Superclusters that are maybe 1 000 000 000 light years away?
 
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For close by objects, such as the Andromeda Galaxy, we can see a type of star called a Cepheid variable. These have variations in brightness that occur in cycles. These cycles vary themselves, however it was found that the brightness of the star was directly related to the time between cycles. Meaning that the dimmer stars are on a different cycle than the brighter stars. By measuring how bright these stars are and their cycles, we know about how far away they are.

Supernova are another way we can judge distance. A type 1a supernova is the result of a White Dwarf star accumulating matter on it's surface until the extra mass results in the collapse of the star in a supernova. Type 1a supernovas are all very similar, as they all result from an almost identical set of circumstances, so again we can judge distance based on the light emitted from the supernova.
 
Drakkith said:
For close by objects, such as the Andromeda Galaxy, we can see a type of star called a Cepheid variable. These have variations in brightness that occur in cycles. These cycles vary themselves, however it was found that the brightness of the star was directly related to the time between cycles. Meaning that the dimmer stars are on a different cycle than the brighter stars. By measuring how bright these stars are and their cycles, we know about how far away they are.

Supernova are another way we can judge distance. A type 1a supernova is the result of a White Dwarf star accumulating matter on it's surface until the extra mass results in the collapse of the star in a supernova. Type 1a supernovas are all very similar, as they all result from an almost identical set of circumstances, so again we can judge distance based on the light emitted from the supernova.

...and using this presumedly accurate method to gauge extremely distant galaxies comes back with measurements showing that the expansion of the universe is accelerating. Uh oh, better come up with something to sell this to people with. Let's call it...[cue ominous music] "Dark Energy!"
Lol
 
tosv said:
What kind of methods are used to measure distance to star that are like 5000 light years away, or to Superclusters that are maybe 1 000 000 000 light years away?

Drakkith gave an excellent answer for moderate distances.

At larger distances (i.e. larger than millions of light-years) cosmological effects (e.g.http://en.wikipedia.org/wiki/Hubble%27s_law" ) you can estimate how far away it is.
 
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twistedspark said:
...and using this presumedly accurate method to gauge extremely distant galaxies comes back with measurements showing that the expansion of the universe is accelerating. Uh oh, better come up with something to sell this to people with. Let's call it...[cue ominous music] "Dark Energy!"
Lol
If you're bemused by such lofty concepts, feel free to ask questions to clarify your understanding.
 
twistedspark said:
...and using this presumedly accurate method

What laypeople often fail to realize is that no one method is used to calculate distances. Many methods, built on many decades of research cause us to arrive at these numbers. One method (say, parallax) will provide an upper and lower bound to distances and/or a margin for error. Another independent method (say, Cepheids) provide another set of bounds. The two methods combine, resulting in an intersection of limits and of margins of error, the outcome being much smaller than anyone method alone.

Do this with multiple methods, with a large data set, and do it with objects very close, where the margins of error are small, and you can generate some pretty reliable techniques.Do not judge unless you know what you're talking about.
 
twistedspark said:
...and using this presumedly accurate method to gauge extremely distant galaxies comes back with measurements showing that the expansion of the universe is accelerating. Uh oh, better come up with something to sell this to people with. Let's call it...[cue ominous music] "Dark Energy!"
Lol

Here are the two major papers on the topic

http://adsabs.harvard.edu/abs/1998AJ...116.1009R

http://adsabs.harvard.edu/abs/2004ApJ...607..665R

They are pretty good examples of scientific reasoning. They do a pretty good job of going through all of the possible observational errors and then explaining why none of them will work. At this point dark energy is weirder, but any of the other explanations are even weirder.

Also people are looking for other ways of measuring extragalactic distances. The wikipedia article lists seven.
 
DaveC426913 said:
One method (say, parallax) will provide an upper and lower bound to distances and/or a margin for error. Another independent method (say, Cepheids) provide another set of bounds.

The other thing is that people use different methods with different physics to calculate the same number. If you end up with roughly the same number, you get a nice warm feeling that you may have something close to the real number.

It's also the situation that people are always trying to think of new things.
 
  • #10
Doreen said:
Continue learning. The astronomy is still have more thing need we think and "dig".

Doreen do you speak english as a first language? It is very difficult to understand you.
 

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