New Hubble Discovery --Spiral Galaxies Like Milky Way Much Bigger Than Thought
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June 27, 2013

New Hubble Discovery --Spiral Galaxies Like Milky Way Much Bigger Than Thought


          M101_fuv_hi_24

 

New observations with Hubble's Cosmic Origins Spectrograph, or COS, show that normal spiral galaxies are surrounded by halos of gas that can extend to over 1 million light-years in diameter. The current estimated diameter of the Milky Way, for example, is about 100,000 light-years. One light-year is roughly 6 trillion miles.

The material for galaxy halos detected by a University of Colorado-Boulder team originally was ejected from galaxies by exploding stars known as supernovae, a product of the star formation process, said John Stocke of CU-Boulder's astrophysical and planetary sciences department. "This gas is stored and then recycled through an extended galaxy halo, falling back onto the galaxies to reinvigorate a new generation of star formation," he said. "In many ways this is the 'missing link' in galaxy evolution that we need to understand in detail in order to have a complete picture of the process."

Stocke gave a presentation on the research June 27 at the University of Edinburgh's Higgs Centre for Theoretical Physics in Scotland at a conference titled "Intergalactic Interactions." The CU-Boulder research team also included professors Michael Shull and James Green and research associates Brian Keeney, Charles Danforth, David Syphers and Cynthia Froning, as well as University of Wisconsin-Madison Professor Blair Savage.

Building on earlier studies identifying oxygen-rich gas clouds around spiral galaxies by scientists at the Space Telescope Science Institute in Baltimore, the University of Massachusetts, Amherst College and the University of California, Santa Cruz, Stocke and his colleagues determined that such clouds contain almost as much mass as all the stars in their respective galaxies. "This was a big surprise," said Stocke. "The new findings have significant consequences for how spiral galaxies change over time."

In addition, the CU-Boulder team discovered giant reservoirs of gas estimated to be millions of degrees Fahrenheit that were enshrouding the spiral galaxies and halos under study. The halos of the spiral galaxies were relatively cool by comparison -- just tens of thousands of degrees -- said Stocke, also a member of CU-Boulder's Center for Astrophysics and Space Astronomy, or CASA.

Shull, a professor in CU-Boulder's astrophysical and planetary sciences department and a member of CASA, emphasized that the study of such "circumgalactic" gas is in its infancy. "But given the expected lifetime of COS on Hubble, perhaps another five years, it should be possible to confirm these early detections, elaborate on the results and scan other spiral galaxies in the universe," he said.

Prior to the installation of COS on Hubble during NASA's final servicing mission in May 2009, theoretical studies showed that spiral galaxies should possess about five times more gas than was being detected by astronomers. The new observations with the extremely sensitive COS are now much more in line with the theories, said Stocke.

The CU-Boulder team used distant quasars -- the swirling centers of supermassive black holes -- as "flashlights" to track ultraviolet light as it passed through the extended gas haloes of foreground galaxies, said Stocke. The light absorbed by the gas was broken down by the spectrograph, much like a prism does, into characteristic color "fingerprints" that revealed temperatures, densities, velocities, distances and chemical compositions of the gas clouds.

"This gas is way too diffuse to allow its detection by direct imaging, so spectroscopy is the way to go," said Stocke. CU-Boulder's Green led the design team for COS, which was built by Ball Aerospace & Technologies Corp. of Boulder for NASA.

While astronomers hope the Hubble Space Telescope keeps on chugging for years to come, there will be no more servicing missions. And the James Webb Space Telescope, touted to be Hubble's successor beginning in late 2018, has no UV light-gathering capabilities, which will prevent astronomers from undertaking studies like those done with COS, said Green.

"Once Hubble ceases to function, we will lose the capability to study galaxy halos for perhaps a full generation of astronomers," said Stocke. "But for now, we are fortunate to have both Hubble and its Cosmic Origins Spectrograph to help us answer some of the most pressing issues in cosmology."

The image at the top of the page shows beautiful spiral galaxy M101 is one of the last entries in Charles Messier's famous catalog. About 170,000 light-years across, this galaxy is enormous, almost twice the size of our own Milky Way galaxy.This mosaic of M101 was assembled from Hubble Legacy Archive data. Additional ground-based data was included to further define the telltale reddish emission from atomic hydrogen gas in this gorgeous galaxy's star forming regions. The sharp image shows features in the galaxy's face-on disk of stars and dust along with background galaxies, some visible right through M101 itself. Also known as the Pinwheel Galaxy, M101 lies within the boundaries of the northern constellation Ursa Major, about 25 million light-years away.

The study was supported by a NASA/Hubble Space Telescope contract to the Cosmic Origins Spectrograph science team, general NASA/Hubble Space Telescope observing grants to Stocke and a National Science Foundation grant to Keeney.

The Daily Galaxy via  University of Colorado

Comments

It's cool to be living at a time when we have the tools to see and learn about so many fantastic things in our awesome universe.

I can hardly wait to see what is found with the James Webb Space Telescope.

A Cosmic Origins Spectrograph should be added to the James Webb telescope like what the Hubble telescope has.


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