Using data from NASA telescopes and other observatories, astronomers reveal the secrets of UGC 1382, revealing that the galaxy is 10 times bigger than previously thought and, unlike most galaxies, its insides are younger than its outsides, almost as if it had been built using spare parts.
About 250 million light-years away, there’s a neighborhood of our universe that astronomers had considered quiet and unremarkable. But now, scientists have uncovered an enormous, bizarre galaxy possibly formed from the parts of other galaxies.
“This rare, ‘Frankenstein’ galaxy formed and is able to survive because it lies in a quiet little suburban neighborhood of the universe, where none of the hubbub of the more crowded parts can bother it,” said study co-author Mark Seibert of the Observatories of the Carnegie Institution for Science, Pasadena, California. “It is so delicate that a slight nudge from a neighbor would cause it to disintegrate.”
Seibert and Lea Hagen, a graduate student at Pennsylvania State University, University Park, came upon this galaxy by accident. They had been looking for stars forming in run-of-the-mill elliptical galaxies, which do not spin and are more three-dimensional and football-shaped than flat disks. Astronomers originally thought that UGC 1382 was one of those.
But while looking at images of galaxies in ultraviolet light through data from NASA’s Galaxy Evolution Explorer (GALEX), a behemoth began to emerge from the darkness.
“We saw spiral arms extending far outside this galaxy, which no one had noticed before, and which elliptical galaxies should not have,” said Hagen, who led the study. “That put us on an expedition to find out what this galaxy is and how it formed.”
Researchers then looked at data of the galaxy from other telescopes: the Sloan Digital Sky Survey, the Two Micron All-Sky Survey (2MASS), NASA’s Wide-field Infrared Survey Explorer (WISE), the National Radio Astronomy Observatory’s Very Large Array and Carnegie’s du Pont Telescope at Las Campanas Observatory. After GALEX revealed previously unseen structures to the astronomers, optical and infrared light observations from the other telescopes allowed the researchers to build a new model of this mysterious galaxy.
As it turns out, UGC 1382, at about 718,000 light-years across, is more than seven times wider than the Milky Way. It is also one of the three largest isolated disk galaxies ever discovered, according to the study. This galaxy is a rotating disk of low-density gas. Stars don’t form here very quickly because the gas is so spread out.
But the biggest surprise was how the relative ages of the galaxy’s components appear backward. In most galaxies, the innermost portion forms first and contains the oldest stars. As the galaxy grows, its outer, newer regions have the youngest stars. Not so with UGC 1382. By combining observations from many different telescopes, astronomers were able to piece together the historical record of when stars formed in this galaxy — and the result was bizarre.
“The center of UGC 1382 is actually younger than the spiral disk surrounding it,” Seibert said. “It’s old on the outside and young on the inside. This is like finding a tree whose inner growth rings are younger than the outer rings.”
The unique galactic structure may have resulted from separate entities coming together, rather than a single entity that grew outward. In other words, two parts of the galaxy seem to have evolved independently before merging — each with its own history.
At first, there was likely a group of small galaxies dominated by gas and dark matter, which is an invisible substance that makes up about 27 percent of all matter and energy in the universe (our own matter is only 5 percent). Later, a lenticular galaxy, a rotating disk without spiral arms, would have formed nearby. At least 3 billion years ago, the smaller galaxies may have fallen into orbit around the lenticular galaxy, eventually settling into the wide disk seen today.
More galaxies like this may exist, but more research is needed to look for them.
“By understanding this galaxy, we can get clues to how galaxies form on a larger scale, and uncover more galactic neighborhood surprises,” Hagen said.
Reference: “On the Classification of UGC1382 as a Giant Low Surface Brightness Galaxy” by Lea M. Z. Hagen, Mark Seibert, Alex Hagen, Kristina Nyland, James D. Neill, Marie Treyer, Lisa M. Young, Jeffrey A. Rich and Barry F. Madore, 1 August 2016, The Astrophysical Journal.
DOI: 10.3847/0004-637X/826/2/210
arXiv:1607.02147
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How the cosmic structures are forming? By cosmic structures we mean not only a large scale network but all the objects populating the cosmos: the stars, star associations and clusters, gas bubbles and shells, galaxies and quasars, star- and galactic- jets, groups
and clusters of galaxies, and finally the large scale structures of the cosmos. Do we have a unique cosmological picture of creation and evolution of this diverse zoo? This question needs elucidation. The answer depends on what we mean by cosmology. Where is the boundary between cosmology and the rest of astrophysics? For example, are the
proto-galactic gas clouds in the province of the cosmology or astrophysics? From the point of cosmology these clouds obviously exist, however an observational astrophysics has never seen them. In some sense the difference is as follows: what we really see is
astrophysics, however what we believe we could see is a cosmology.