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The Universe

How big is it?   How do we find out?

 

Topics
  1. Cosmology
  2. Relativity

This picture:

 Click this Thumbnail to see a larger version of this picture. (Click for a larger view)

taken by the Hubble Space Telescope and known as the Hubble Deep Field, is of an area near the handle of the Big Dipper about the size, from our perspective, of the head of a straight pin held at arm's length!

You can see about every type of galaxy, (at least 1,500!)  at distances of tens of millions to billions of light-years from Earth.  There are only a handful of stars from our galaxy in the foreground of this picture.  Every thing else appears to be a galaxy!

Follow links on the Hubble pages to see other Deep Field-type pictures, and updates, like THIS ONE.

Its counterpart in the southern hemisphere, the Hubble Deep Field South, is equally stunning.


So where is our galaxy?  It's part of a cluster of a few galaxies called The Local Group
(look at a 3-D Local Group, see also this from SEDS) that looks something like this  Small Group of Galaxies.

...but only sort of.  Then, our little cluster is part of a bigger one that may look something like this image of a portion of the Virgo Cluster that consists of about 2,000 galaxies, or this of the Coma Cluster...
containing hundreds or thousands of galaxies, or millions in a grouping called a supercluster.
Look at Galaxy Clusters, The Nearest 15,000 Galaxies, The Local Supercluster and Galaxy Cluster Mug Shots to see even more great images.

More Information:

 

Dr. Strous' Universe Tree - a resource of much information

How do we find out the size of the universe?

Spectra

    • As mentioned elsewhere, we can use their spectra to find out a lot about stars.

    • We can also use their Spectra to find out about galaxies, in the same way:

The Doppler Effect

    Is one way to use spectra for distance

    • Like the changing sound of a horn, as a car approaches you, then recedes -

    So it is the same with light ...

à As a galaxy or star approaches us, the familiar absorption lines of particular elements show up, but are shifted toward the blue end of the spectrum.
• As a galaxy or star recedes from us, the shift is toward the red end of the spectrum.

This is known as:

    Red Shift
Red shift links HERE, HEREHERE, & HERE • Most galaxies are moving away from us.

• Those the farthest from us are moving the fastest!

So what is... the size and age of the universe?

Those are questions from Cosmology - the Origin and Fate of the Universe

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UPDATED: 03/03/08