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TalonD
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rough estimate, how many galaxies in the visible portion of the universe? Just curious.
russ_watters said:You can also reach a similar estimate by taking the Hubble Ultra Deep Field (which contains around 10,000 galaxies) and extrapolating it across the whole sky.
Wallace said:...all you really get is a hazy blob seen in a few different filters (e.g. in different colours) from which you make an informed guess about the redshift, based on what colours you expect galaxies to be in their rest frame.
negitron said:Huh? I do not think you understand the process here. Redshift measurement doesn't involve guesswork except to the extent that it's difficult to get readable spectra from such distant, faint objects. Once a clean spectrum has been obtained, however, redshift can be measured precisely because it doesn't involve guessing about colors, it looks for specific signature spectral emission and/or absorption lines, such as the ones for hydrogen and measures exactly how far it has been shifted towards the red (or blue, as the case may be). The color of the galaxy is irrelevant.
I was under the impression there was a different type of telescope (a radio telescope maybe?) that could see galaxies further away, but can't remember where I heard that. In any case, yeah, Hubble probably gets us on the right order of magnitude.Wallace said:Hubble, being the best telescope we have ever had for this sort of thing, has seen the most distant galaxies ever observed (measured by their redshift).
Wallace said:Hubble has a spectrograph, it did get broken, but has been replaced in a recent servicing mission. Hubble spectra are pretty crappy though, because the Hubble mirror is so small (only ~2m).
Wallace said:Ground based telescopes are actually better than Hubble for spectra because the distortion effects of the atmosphere are not a problem, so it is a case of bigger is better. The highest redshift spectra have been obtained from the ground, not from space.
Wallace said:Ah okay. I was comparing Hubble spectra to Keck spectra that I worked on years ago, the Keck ones were waaaay better than Hubble. So seeing is still a problem for getting spectra (which makes sense) but not so bad such that a 10m ground based telescope still beats (by a fair way) a 2m space telescope, which is not the case for imaging?
nicksauce said:From Wikipedia: 'There are probably more than 100 billion galaxies in the observable universe", with the reference: http://astronomy.swin.edu.au/~gmackie/billions.html
But we can do an order of magnitude calculation to estimate this.
Assumptions:
1) All the baryonic matter in the universe is in galaxies, in the form of stars
2) The universe is flat with [itex]\Omega_Bh^2 = 0.02[/itex]
3) Each galaxy has 100 billion stars, averaging 1 solar mass
4) The size of the observable universe is about 4 * 10^32 ly^3 (http://en.wikipedia.org/wiki/Observable_universe)
This gives about 6 * 10^11 galaxies, close to the 100 billion quoted by Wikipedia.
TalonD said:6*10^11 is 600 trillion, that's not quite the same as 100 billion
negitron said:Eh? 6E11 = 600,000,000,000 = 600 billion.
TalonD said:Correct me if I'm wrong, and I very well may be considering I'm just a layperson. But wouldn't the most distant galaxies we can see be limited by the surface of last scattering, that is, the microwave background radiation. so the radius of the visible universe is around 45 billion light years? So is hubble's resolution high enough to image galaxies or protogalaxies that far away?
TalonD said:600b is still five hundred billion more than 100 billion. I wouldn't say that was close.
ideasrule said:The microwave background radiation was emitted when the universe was only 400 000 years old. At that time, the baryonic matter of the universe had just begun to cool down into a gas from a plasma. There were no stars, let alone galaxies. The first galaxies formed a few hundred million years after the Big Bang, so none of them are "behind" the surface of last scattering.
As for Hubble's imaging capabilities, it certainly can't see every galaxy there is to see. That's part of the reason Herschel (see http://www.space.com/scienceastronomy/090512-herschel-sidebar.html) was launched: to see some of the earliest galaxies.
Chronos said:I believe the 100 billion galaxies estimate came from the HDF [hubble deep field] survey [which covered a miniscule slice of the sky]. As Wallace noted, any such estimate accurate to the nearest zero is usually considered very good in cosmology.
Scientists use telescopes to observe and count the number of galaxies in a given area of the sky. They can also use mathematical models and simulations to estimate the total number of galaxies in the observable universe.
Estimates vary, but it is currently believed that there are around 2 trillion galaxies in the observable universe. However, this number is constantly changing and may increase as technology advances and we are able to observe more of the universe.
There are estimated to be around 100 billion stars in our own galaxy, the Milky Way. Based on current estimates, there are significantly more galaxies than stars in the universe. This means that there are trillions of trillions of stars in the universe.
No, we can only observe a small portion of the universe due to the limitations of our technology and the speed of light. The observable universe is estimated to be around 93 billion light-years in diameter, but the entire universe is much larger and may contain an infinite number of galaxies.
It is believed that the number of galaxies in the universe has remained relatively constant over time. However, galaxies are constantly merging and evolving, so the individual galaxies we see today may not have existed in the same form in the past. Additionally, the expansion of the universe may create new galaxies in the future.