When you look at a normal galaxy, most of the light comes from the stars in visible wavelengths and is evenly distributed throughout the galaxy. However, if you observe some galaxies, you'll see intense light coming from their nuclei. And if you look at these same galaxies in the X-ray, ultraviolet, infrared and radio wavelengths, they appear to be giving off enormous amounts of energy, apparently from the nucleus. These are active galaxies, which represent a very small percentage of all galaxies. There are four classifications of active galaxy, but the type we observe may depend more upon our viewing angle than structural differences.
- Seyfert galaxies
- Radio galaxies
To explain active galaxies, scientists must be able to explain how they emit such large amounts of energy from such small areas of the galactic nuclei. The most accepted hypothesis is that at the center of each of these galaxies is a massive or supermassive black hole. Around the black hole is an accretion disk of rapidly spinning gas that's surrounded by a torus (a donut-shaped disk of gas and dust). As the material from the accretion disk falls into the area around the black hole (the event horizon), it heats to millions of degrees Kelvin and is accelerated outward in the jets.
Discovered by Carl Seyfert in 1943, these galaxies (2 percent of all spiral galaxies) have broad spectra indicating cores of hot, low-density ionized gas. The nuclei of these galaxies change brightness every few weeks, so we know that the objects in the center must be relatively small (about the size of a solar system). Using Doppler shifts, astronomers have noticed that velocities at the center of Seyfert galaxies are about 30 times greater than those of normal galaxies.
Radio galaxies are elliptical (0.01 percent of all galaxies are radio galaxies). Their nuclei emit jets of high-velocity gas (near the speed of light) above and below the galaxy -- the jets interact with magnetic fields and emit radio signals.
Quasars (quasi-stellar objects)
Quasars were discovered in the early 1960s. About 13,000 have been discovered, but there could be as many as 100,000 out there [source: A Review of the Universe]. They're billions of light years away from the Milky Way and are the most energetic objects in the universe. The extreme brightness of quasars can fluctuate over daylong periods, which indicates that the energy is coming from a very small area. Thousands of quasars have been found, and they're believed to be emanating from the cores of distant galaxies.
Blazars are a type of active galaxy -- about 1,000 have been cataloged [source: A Review of the Universe]. From our viewpoint, we are looking "head-on" at the jet emanating from the galaxy. Like quasars, their brightness can fluctuate rapidly -- sometimes in less than one day.
Take a look at the links below for more information about galaxies.
- Is there a hole in the universe?
- How Stars Work
- How the Sun Works
- How the Earth Works
- How Dark Matter Works
- How Black Holes Work
- How Light Works
- How Telescopes Work
- How the Hubble Space Telescope Works
- How Lunar Liquid Mirror Telescopes Work
- If you were to move all the matter in the universe into one corner, how much space would it take up?
More Great Links
- A Map of the Milky Way. http://www.atlasoftheuniverse.com/milkyway.html
- A Review of the Universe - Structures, Evolutions, Observations, and Theories. http://universe-review.ca/F05-galaxy.htm
- A Teacher's Guide to the Universe. http://www.astro.princeton.edu/~clark/teachersguide.html.
- Bennett, J et al. "The Cosmic Perspective (third edition)." Pearson, 2004.
- Chandra X-ray Observatory - X-ray Astronomy Field Guide, Starburst Galaxies. http://chandra.harvard.edu/xray_sources/starburst.html
- Galaxy Classification and Evolution Lab. http://cosmos.phy.tufts.edu/~zirbel/laboratories/Galaxies.pdf
- Henry, J. Patrick et al. "The Evolution of Galaxy Clusters." Scientific American, December 1998. http://atropos.as.arizona.edu/aiz/teaching/a204/darkmat/SciAm98b.pdf
- NASA Imagine the Universe, "The Hidden Lives of Galaxies" book. http://imagine.gsfc.nasa.gov/docs/teachers/galaxies/imagine/titlepage.html
- NASA Imagine the Universe, Active Galaxies and Quasars. http://imagine.gsfc.nasa.gov/docs/science/know_l1/active_galaxies.html
- NASA Imagine the Universe, The Hidden Lives of Galaxies poster. http://imagine.gsfc.nasa.gov/docs/teachers/galaxies/imagine/poster.jpg
- NASA/JPL Galaxy Evolution Explorer (GALEX). http://www.galex.caltech.edu/
- NASA/JPL GALEX. Galaxies and UV. http://www.galex.caltech.edu/SCIENCE/science.html
- Science @NASA. What are Galaxies? How Do They Form and Evolve? http://science.hq.nasa.gov/universe/science/galaxies.html
- SEDS.org, Galaxies. http://www.seds.org/messier/galaxy.html
- Seeds, MA. "Stars & Galaxies (second edition)." Brooks/Cole, 2001.
- Stephens, S. "Galaxy Sorting Handout." http://www-tc.pbs.org/seeinginthedark/pdfs/galaxy_sorting_handout.pdf
- University of Washington Astronomy Department. Lecture" "Galaxies: Classification, Formation, and Evolution." http://www.astro.washington.edu/larson/Astro101/LecturesBennett/Galaxies/galaxies.html
- Windows to the Universe, Galaxies.http://www.windows.ucar.edu/cgi-bin/tour.cgi-link=/the_universe/Galaxy.html&sw=false&sn=1&d=/the_universe&edu=high&br=graphic&back=/pluto/pluto.html&cd=false&fr=f&tour=
- WMAP Cosmology 101: What is the Universe Made of? http://map.gsfc.nasa.gov/m_uni/uni_101matter.html