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Galaxies

Universe Galaxies-1 Milky Way

Artist's Conception - The Milky Way
Where are we?
We live in a somewhat remote arm of the Milky Way. This video shows you the way from our home to a vantage point outside the Local Group.
Animation (Quicktime, 3MB)

Universe Galaxies-3 Deep Field
Hubble Ultra Deep Field galaxies:
Credit: NASA, ESA, S. Beckwith (STScI) and the HUDF Team

Our galaxy, the Milky Way, is typical: it has hundreds of billions of stars, enough gas and dust to make billions more stars, and at least ten times as much dark matter as all the stars and gas put together. And it’s all held together by gravity.

Like more than two-thirds of the known galaxies, the Milky Way has a spiral shape. At the center of the spiral, a lot of energy and, occasionally, vivid flares. are being generated. Based on the immense gravity that would be required explain the movement of stars and the energy expelled, the astronomers conclude that the center of the Milky Way is a supermassive black hole.

Other galaxies have elliptical shapes, and a few have unusual shapes like toothpicks or rings. The Hubble Ultra Deep Field (HUDF) shows this diversity. Hubble observed a tiny patch of sky (one-tenth the diameter of the moon) for one million seconds (11.6 days) and found approximately 10,000 galaxies, of all sizes, shapes, and colors. From the ground, we see very little in this spot, which is in the constellation Fornax.

Formation

After the Big Bang, the Universe was composed of radiation and subatomic particles. What happened next is up for debate - did small particles slowly team up and gradually form stars, star clusters, and eventually galaxies? Or did the Universe first organize as immense clumps of matter that later subdivided into galaxies?

Collisions

The shapes of galaxies are influenced by their neighbors, and, often, galaxies collide. The Milky Way is itself on a collision course with our nearest neighbor, the Andromeda galaxy. Even though it is the same age as the Milky Way, Hubble observations reveal that the stars in Andromeda's halo are much younger than those in the Milky Way. From this and other evidence, astronomers infer that Andromeda has already smashed into at least one and maybe several other galaxies.

Recent Discoveries

April 23, 2013 Galaxy Goes Green in Burning Stellar Fuel
April 4, 2013 Taken Under the "Wing" of the Small Magellanic Cloud
April 1, 2013 Light and Dust in a Nearby Starburst Galaxy
February 21, 2013 Stellar Motions in Outer Halo (Milky Way)
January 28, 2013 The Moment the Lights Went Out
January 10, 2013 Largest-Known Spiral Galaxy (NGC 6872)
December 17, 2012 The Needle Galaxy (IC 2233)
November 29, 2012 A Multi-Wavelength View of Radio Galaxy Hercules A
November 26, 2012 A Peculiar Compact Blue Dwarf Galaxy (NGC 5253)
November 20, 2012 Colossal Intergalactic Bridge
November 19, 2012 A Loose Spiral Galaxy (ESO 499-G37)
November 15, 2012 Cluster MACS J0647 Provides Three Magnified Views of Distant Galaxy
October 19, 2012 Surprising Trend in Galaxy Evolution
September 24, 2012 Galactic Halo Around Milky Way
September 19, 2012 Ultra-Distant Galaxy Amidst Cosmic 'Dark Ages' (most distant galaxy yet?)
September 17, 2012 Glowing Gas and Dark Dust in a Side-on Spiral (NGC 4634)
September 10, 2012 An Actively Star-forming Galaxy (NGC 7090)
September 6, 2012 Odd Galaxy Couple on Space Voyage (M60)
August 30, 2012 A Surprisingly Bright Superbubble (NGC 1929 in N44)
July 10, 2012 Ghost Galaxies
June 26, 2012 Galaxy Cluster IDCS J1426.5+3508 and Giant Arc