Heck Yeah Galaxies
M74 seen in infrared
lori-rocks:
Teton Lights  by James Neeley
itsfullofstars:

APOD: Peculiar Galaxies of Arp 273
Credit: NASA, ESA, and the Hubble Heritage Team (STScI / AURA)
Explanation: The spiky stars in the foreground of this sharp cosmic portrait are well within our own Milky Way Galaxy. The two eye-catching galaxies lie far beyond the Milky Way, at a distance of over 300 million light-years. Their distorted appearance is due to gravitational tides as the pair engage in close encounters. Cataloged as Arp 273 (also as UGC 1810), the galaxies do look peculiar, but interacting galaxies are now understood to be common in the universe. In fact, the nearby large spiral Andromeda Galaxy is known to be some 2 million light-years away and approaching the Milky Way. Arp 273 may offer an analog of their far future encounter. Repeated galaxy encounters on a cosmic timescale can ultimately result in a merger into a single galaxy of stars. From our perspective, the bright cores of the Arp 273 galaxies are separated by only a little over 100,000 light-years. The release of this stunning vista celebrates the 21st anniversary of the Hubble Space Telescope in orbit.
cwnl:

Stargazing over The Geyser
Starry night above the World Heritage Site, Yellow Stone National Park, Wyoming, USA. The yellow patch in the foreground is an eruption of Old Faithful Geyser, a strong cone geyser that can shoot 14000–32000 liters of boiling water to a height of 30–55 meters.
Copyright: Wally Pacholka
NGC 891, an edge on spiral galaxy.
undefinedgrace:

The outlying regions around the Southern Pinwheel galaxy, or M83, are highlighted in this composite image from NASA’s Galaxy Evolution Explorer and the National Science Foundation’s Very Large Array in New Mexico. The blue and pink pinwheel in the center is the galaxy’s main stellar disk, while the flapping, ribbon-like structures are its extended arms.
mohandasgandhi:

The Universe is expanding at 73.8 +/- 2.4 km/sec/megaparsec! So there.

In 1998, two teams of astronomers independently reported amazing and  bizarre news: the Universal expansion known for decades was not slowing  down as expected, but was speeding up. Something was accelerating the  Universe.
Since then, the existence of this something was fiercely  debated, but time after time it fought with and overcame objections.  Almost all professional astronomers now accept it’s real, but we still  don’t know what the heck is causing it. So scientists keep going back to  the telescopes and try to figure it out.
This gorgeous image is of the nearby spiral galaxy NGC 5584, where of  course “nearby” to an astronomer means 72 million light years. This  galaxy is loaded with a specific type of variable star — called Cepheids  — which are very important: the way they change their brightness  depends on how luminous they are. Measure the change, and you measure  the luminosity, and if you measure how bright they appear in the sky you  get their distance. It’s a bit like judging how far away a car is by  gauging how bright its headlights are. Except in this case astronomers  use Hubble instead of their eyes. It’s a tad more accurate.
It so happens that in 2007, NGC 5584 was the host of a Type Ia  supernova, the Golden Standard of distance indicators. These are so  bright they can be seen clear across the Universe! By knowing the  distance to the one in NGC 5584, we can then use that to get the  distances to supernovae much, much farther away.
It’s a bootstrappy way of measuring the cosmic distance scale.
But it appears to work.  By measuring the  Cepheids in eight galaxies that also hosted Type 1a supernovae,  astronomers (led by my old pal Adam Riess; we were grad students  together when he cracked the Type 1a code that led to the discovery of  the universal acceleration — which will win him the Nobel one day, I’d  wager) were able to hone the distance bootstrap even better.
And now, by measuring first the Cepheids and then using them to  determine the distance to far-flung supernovae, they have nailed down  just how fast the Universe is expanding: 73.8 (plus or minus 2.4)  km/sec/megaparsec.
OK, so what does that mean?
We see galaxies rushing away from us. Moreover, the farther away they  are, the faster they appear to be moving. The rate of that expansion is  what was measured. If you find a galaxy 1 megaparsec away (about 3.26  million light years), the expansion of space would carry it along at  73.8 km/sec (fast enough to cross the United States in about one  minute!). A galaxy 2 megaparsecs away would be traveling away at 147.6  km/sec, and so on*.
The last time this was measured accurately,  the speed was seen to be 74.2 +/- 3.6 km/sec/mpc. Note the uncertainty;  both the old and new measurements overlap to within their uncertainty  (which is good!), but the new one has a smaller uncertainty. In other  words it’s most likely more accurate.
By knowing this number so well, it allows better understanding of how  the Universe is behaving. It also means astronomers can study just how  much the Universe deviates from this constant rate at large distances  due to the acceleration. And that in turn allows us to throw out some  ideas for what dark energy is, and entertain notions of what it might  be. For example, one idea was that instead of dark energy accelerating  the Universe, it was an illusion due to our region in the local Universe  being unusually underdense — that would make it look like distant  galaxies are receding faster than expected. However, the precision of  the new measurement rules this out; the value needed by the void model  would have to be much lower. So right away we know that this explanation  doesn’t work, and the idea of dark energy survives another battle.
So that number of 73.8 +/- 2.4 km/sec/mpc may sound arcane and weird  to you, but it is in fact the key to understanding the Universe itself.  It’s amazing that so much can ride on one number… but that’s the  Universe for you.
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