What does the Universe look like beyond our Galaxy? [Starts With A Bang]

“Who are we? We find that we live on an insignificant planet of a humdrum star lost in a galaxy tucked away in some forgotten corner of a universe in which there are far more galaxies than people.” -Carl Sagan

Our night sky, quite literally, is our window to the Universe.

Image credit: Miloslav Druckmuller, Brno University of Technology.

Well, it’s kind of a window to the Universe. I say only “kind of” because, with the exception of those two faint, fuzzy clouds in the lower right, everything else visible in the image above is part of our own Milky Way galaxy. In fact, practically everything we’ve ever seen or heard of in the Universe we learned from observations of our own Milky Way. It is vast, beautiful, and full of hundreds of billions of stars, trillions of planets, and much, much more.

Image credit: Richard Powell, Atlas of the Universe.

But this is only one of hundreds of billions of galaxies in the Universe! We know this most convincingly through deep-sky observations of regions of the Universe where there happen to be no (or very few) galactic stars, gas, or dust in the way of our telescopes.

Image credit: NASA, ESA, S. Beckwith (STScI) and the HUDF Team.

What we find, by treating these regions as representatively typical of the rest of the Universe, is that there are at minimum over 100 billion galaxies in the Universe. But there’s more to learn than just a number; among other things, we want to know:

how these galaxies cluster and clump together,
how far away they are from us,
how quickly they’re moving either towards or away from both us and one another,
how massive they are,
what type of galaxy are they, and
when was the last time they underwent intense star formation?

In other words, we want to know what the Universe looks like — in detail – beyond our own galaxy!

Image credit: Thomas Jarrett (IPAC/Caltech), 2MASS (2-Micron All-Sky Survey).

And what we’ve known, for many decades now, is that galaxies are neither distributed uniformly throughout the Universe nor are they distributed randomly. Instead, they are clumped and clustered together in a very particular and intricate way. Looking in detail at our own corner of the Universe, we’ve constructed detailed maps of hundreds of thousands of nearby galaxies.

The most recent, and also the most powerful (and still ongoing) survey of galaxies in the Universe is the Sloan Digital Sky Survey, which has just publicly released data for over 500,000 galaxies and 100,000 quasars.

Image credit: 2010-2012 SDSS-III.

The wide-field camera and imaging system aboard this 2.5-meter diameter telescope is the most advanced in the world, and has allowed us to construct the most detailed map of the cosmic web of all time.

Image credit: Sloan Digital Sky Survey team.

What we’ve learned from looking at the Universe and the way galaxies cluster together in it includes information about how galaxies form, merge and evolve, but also about what makes up the Universe we’re in.

How much of the Universe is made up of normal (protons, neutrons, and electrons) matter? How much is dark matter? Is the dark matter hot, warm or cold? By plotting how a large sample of these galaxies cluster on different distance scales, we can learn about the ratio of normal-to-dark matter by looking at the size of the “wiggles” in the graph (known as a Power Spectrum), below, and by looking at the scale of when there’s a vertical plummet towards zero, we can learn about dark matter’s temperature.

Image credit: Shaun Cole et al., 2005, for the 2-degree Field Galaxy Redshift Survey.

A Universe with no normal matter would have no wiggles and would have a totally smooth power spectrum; a Universe with no dark matter would have wiggles that extended down to the bottom of the graph. A Universe that had dark matter of a certain temperature would have a “cutoff” in the spectrum where it simply dived down towards zero on small scales. What we see tells us that the Universe has about a 1:5 ratio of normal-to-dark matter, a total amount of matter that’s equal to about 25% of the Universe’s total energy density, and that dark matter is cold enough that if it has any temperature at all, it’s well below what we’ve been able to observe. (See here for more on Dark Matter.)

Combined with information about the flatness and expansion of the Universe (from, say, the cosmic microwave background and observations of distant supernovae), we’ve arrived at the model of the Universe we have today, complete with dark matter, dark energy, and the tiny bit of normal matter we actually understand.

Image credit: Suzuki et al., 2011 (The Supernova Cosmology Project).

The “BAO” label stands for baryon acoustic oscillations, which are the pressure waves in the normal matter that cause the wiggles in the graph of the power spectrum (and the specific clustering features of the galaxies themselves), above.

But you might enjoy a much more visual approach to knowing what the Universe looks like, beyond our galaxy. Well, the SDSS team has outdone themselves, with Miguel Aragon, Mark Subbarao and Alex Szalay teaming up to create the following video of a fly-through of approximately 400,000 galaxies in our Universe, of a journey spanning 1.3 billion light years.

This, for reference, is less than 2% of the diameter of the known, observable Universe, but is a large enough sample to give a fair representation of where we live. This is what your Universe looks like; enjoy!