Astronomy - Measure distance to other galaxies

In summary, different methods are used to measure distances to stars and galaxies, such as parallax and Cepheid variables. These methods provide upper and lower bounds with margins of error, and when combined, can provide a more accurate measurement. The concept of dark energy has arisen from these measurements, and further research is being done to find new ways of measuring distances.
  • #1
tosv
13
0
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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  • #2
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.
 
  • #3
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
 
  • #4
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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  • #5
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.
 
  • #6
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.
 
  • #8
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.
 
  • #9
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.
 

What is the study of measuring distance to other galaxies?

The study of measuring distance to other galaxies is known as astrometry. It involves using various techniques and tools to determine the distance between objects in space.

Why is it important to measure the distance to other galaxies?

Measuring the distance to other galaxies is important for several reasons. It helps us understand the scale of the universe and its structure. It also allows us to study the evolution of galaxies and the expansion of the universe. Additionally, measuring distances allows us to accurately calculate the brightness and energy output of objects in space.

How do scientists measure the distance to other galaxies?

There are several methods that scientists use to measure the distance to other galaxies. One common method is called parallax, which involves measuring the apparent shift in position of a nearby object when viewed from different locations. Other methods include using standard candles, such as supernovae, and using the redshift of light from galaxies to determine their distance.

What are some challenges in measuring the distance to other galaxies?

One of the main challenges in measuring the distance to other galaxies is the vastness of space. This makes it difficult to accurately measure distances using traditional methods. Additionally, the expansion of the universe and the presence of dark matter can also affect distance measurements.

How accurate are the distance measurements to other galaxies?

The accuracy of distance measurements to other galaxies depends on the method used and the technology available. Generally, measurements using parallax or standard candles have a margin of error of around 5-10%. However, as technology and measurement techniques improve, the accuracy of these measurements is also increasing.

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