Elliptical galaxies are, usually, quite simple: massive spheres of old stars. But the giant galaxy Centaurus A (Cen A) hides a complex environment deep in its core. Recent observations reveal gaseous spiral arms, several thousand light-years across, swirling about the heart of the galaxy. The arms, never before seen in an elliptical galaxy, most likely formed after Cen A swallowed another galaxy sometime in the last few hundred million years. The discovery is another step towards understanding the formation and evolution of some of the most massive galaxies in the universe.
Cen A is known for being unusual. The most striking feature is a dark dust lane bisecting our view of its halo of stars. The dark band, filled with hydrogen gas and interstellar dust grains, are the remains of another galaxy torn apart by a close encounter with Cen A. The new observations use radio telescopes to peer through the thick dust clouds into the galaxy’s center. The images reveal a disk of carbon monoxide gas that formed spiral arms much like the grand spirals of our own Milky Way galaxy.
Computer simulations indicate that the recent collision most likely delivered the gas to the galaxy’s core. Gas stripped off the cannibalized galaxy was funneled into the center while gravitational perturbations triggered the formation of spiral arms. As the arms sweep through the galaxy, they compress gas along their leading edges and spark new waves of star formation. While most elliptical galaxies have stopped making new stars, these spiral arms may be giving Cen A a new lease on life!
The results were published September 1, 2012 in The Astrophysical Journal Letters.
Cen A is an ideal laboratory for understanding galaxy evolution. Sitting 12 million light-years away in the southern constellation Centaurus, the Centaur, Cen A is the closest giant elliptical galaxy to Earth. Both its proximity and size make Cen A the fifth brightest galaxy in the sky and therefore a popular target for amateur telescopes. In addition to its unusual dust bands, Cen A also hosts a supermassive black hole at its center. This massive beast contains the mass of 55 million suns and drives million light-year long jets that eject gas into intergalactic space at half the speed of light!
The spiral arms were observed at the Submillimeter Array (SMA), a network of radio telescopes located 4080 meters (13,386 feet) above sea level at the summit of Mauna Kea, Hawai’i. The high elevation places the SMA above most of the water vapor in Earth’s atmosphere that would otherwise interfere with observations like these. The SMA is a joint project between the Smithsonian Astrophysical Observatory and the Academia Sinica Institute of Astronomy and Astrophysics.
Bottom line: Astronomers using the Submillimeter Array radio telescopes have discovered young spiral arms in the center of the giant elliptical galaxy Centaurus A. The spiral arms formed shortly after a collision with another galaxy several hundred million years ago. The discovery helps astronomers piece together the history of giant galaxies and understand how they form and evolve.
Chris Crockett got his Ph.D. in astronomy from UCLA in 2011 and worked at Lowell Observatory and the U.S. Naval Observatory. He then realized he enjoyed talking about astronomy a lot more than actually doing it. After being awarded a Mass Media Fellowship in 2013 by the American Association for the Advancement of Science, he spent a summer writing for Scientific American, then went on to become the staff astronomy writer at Science News from 2014 - 2017. These days, he freelances, focusing on stories about astronomy, planetary science, and physics. His work has appeared in Science News, Scientific American, Smithsonian Magazine, Knowable, Sky & Telescope, and the American Physical Society's online magazine Physics.