Subscribe free to our newsletters via your
. GPS News .




STELLAR CHEMISTRY
Astronomers Uncover A Surprising Trend in Galaxy Evolution
by Francis Reddy for Goddard Space Flight Center
Greenbelt MD (SPX) Oct 22, 2012


This plot shows the fractions of settled disk galaxies in four time spans, each about 3 billion years long. (full size chart) There is a steady shift toward higher percentages of settled galaxies closer to the present time. At any given time, the most massive galaxies are the most settled. More distant and less massive galaxies on average exhibit more disorganized internal motions, with gas moving in multiple directions, and slower rotation speeds. Credit: NASA's Goddard Space Flight Center.

A comprehensive study of hundreds of galaxies observed by the Keck telescopes in Hawaii and NASA's Hubble Space Telescope has revealed an unexpected pattern of change that extends back 8 billion years, or more than half the age of the universe.

"Astronomers thought disk galaxies in the nearby universe had settled into their present form by about 8 billion years ago, with little additional development since," said Susan Kassin, an astronomer at NASA's Goddard Space Flight Center in Greenbelt, Md., and the study's lead researcher. "The trend we've observed instead shows the opposite, that galaxies were steadily changing over this time period."

Today, star-forming galaxies take the form of orderly disk-shaped systems, such as the Andromeda Galaxy or the Milky Way, where rotation dominates over other internal motions. The most distant blue galaxies in the study tend to be very different, exhibiting disorganized motions in multiple directions. There is a steady shift toward greater organization to the present time as the disorganized motions dissipate and rotation speeds increase. These galaxies are gradually settling into well-behaved disks.

Blue galaxies - their color indicates stars are forming within them - show less disorganized motions and ever-faster rotation speeds the closer they are observed to the present. This trend holds true for galaxies of all masses, but the most massive systems always show the highest level of organization.

Researchers say the distant blue galaxies they studied are gradually transforming into rotating disk galaxies like our own Milky Way.

"Previous studies removed galaxies that did not look like the well-ordered rotating disks now common in the universe today," said co-author Benjamin Weiner, an astronomer at the University of Arizona in Tucson. "By neglecting them, these studies examined only those rare galaxies in the distant universe that are well-behaved and concluded that galaxies didn't change."

Rather than limit their sample to certain galaxy types, the researchers instead looked at all galaxies with emission lines bright enough to be used for determining internal motions. Emission lines are the discrete wavelengths of radiation characteristically emitted by the gas within a galaxy. They are revealed when a galaxy's light is separated into its component colors. These emission lines also carry information about the galaxy's internal motions and distance.

The team studied a sample of 544 blue galaxies from the Deep Extragalactic Evolutionary Probe 2 (DEEP2) Redshift Survey, a project that employs Hubble and the twin 10-meter telescopes at the W. M. Keck Observatory in Hawaii. Located between 2 billion and 8 billion light-years away, the galaxies have stellar masses ranging from about 0.3 percent to 100 percent of the mass of our home galaxy.

A paper describing these findings will be published Oct. 20 in The Astrophysical Journal.

The Milky Way galaxy must have gone through the same rough-and-tumble evolution as the galaxies in the DEEP2 sample, and gradually settled into its present state as the sun and solar system were being formed.

In the past 8 billion years, the number of mergers between galaxies large and small has decreased sharply. So has the overall rate of star formation and disruptions of supernova explosions associated with star formation. Scientists speculate these factors may play a role in creating the evolutionary trend they observe.

Now that astronomers see this pattern, they can adjust computer simulations of galaxy evolution until these models are able to replicate the observed trend. This will guide scientists to the physical processes most responsible for it.

The DEEP2 survey is led by Lick Observatory at the University of California at Santa Cruz in collaboration with the University of California at Berkeley, the University of Hawaii at Manoa, Johns Hopkins University in Baltimore, Md., the University of Chicago and the California Institute of Technology in Pasadena.

The Hubble Space Telescope is a project of international cooperation between NASA and the European Space Agency. NASA's Goddard Space Flight Center in Greenbelt, Md., manages the telescope. The Space Telescope Science Institute (STScI) in Baltimore, Md., conducts Hubble science operations. STScI is operated by the Association of Universities for Research in Astronomy, Inc. in Washington.

.


Related Links
NASA's Hubble website
Stellar Chemistry, The Universe And All Within It






Comment on this article via your Facebook, Yahoo, AOL, Hotmail login.

Share this article via these popular social media networks
del.icio.usdel.icio.us DiggDigg RedditReddit GoogleGoogle








STELLAR CHEMISTRY
Hubble Sees Galaxy in a spin
Washington DC (SPX) Oct 22, 2012
NGC 3344 is a glorious spiral galaxy around half the size of the Milky Way, which lies 25 million light-years distant. We are fortunate enough to see NGC 3344 face-on, allowing us to study its structure in detail. The galaxy features an outer ring swirling around an inner ring with a subtle bar structure in the center. A bar is an elongated distribution of stars and gas in the center of a ... read more


STELLAR CHEMISTRY
Panels reject study on GM corn but urge wider probes

Indian farmers cotton on to sustainable farming

Pesticides have knock-on effect for bees: study

Some 500 scientists have created a Top 10 list of plant-damaging fungi

STELLAR CHEMISTRY
Breakthrough offers new route to large-scale quantum computing

Bus service for qubits

Developing the next generation of microsensors

ORNL study confirms magnetic properties of silicon nano-ribbons

STELLAR CHEMISTRY
Boeing EMARSS Risk Reduction Prototype Makes First Flight

NASA Seeks Student Experiments For 2013 High-Altitude Scientific Balloon Flight

Raytheon-led team graduates first Afghan Air Force pilots on Warfighter FOCUS program contract

Second UK F-35 And Marine Corps F-35B Delivered To Eglin

STELLAR CHEMISTRY
Nissan to build 'steer-by-wire' cars

Australian race crew in faster-than-a-bullet bid

China to test driverless cars for 75 miles

Cadillac to introduce electric gas hybrid

STELLAR CHEMISTRY
Japan trade tumbles amid global slowdown, China spat

French minister lambasts WTO over eurozone trade deficit with China

Huawei row shines light on East-West culture clash

eBay pays 1.2m pounds in British taxes on sales of 800m pounds

STELLAR CHEMISTRY
Sting forces venue switch in Philippines tree row

Ozone Affects Forest Watersheds

Study: Windblown forests best left alone

Brazil president makes final changes to forestry law

STELLAR CHEMISTRY
Landsat Science Team to Help Guide Next Landsat Mission

TerraSAR-X images Bonneville salt flats

Earth Observation Commercial Data Market Remains Strong Despite Slowdown in 2011

Antarctic Rift Subject of International Attention

STELLAR CHEMISTRY
Manufacturing complex 3D metallic structures at nanoscale made possible

A novel scheme to enhance local electric fields around metal nanostructures

University of Florida chemists pioneer new technique for nanostructure assembly

New Techniques Stretch Carbon Nanotubes, Make Stronger Composites




The content herein, unless otherwise known to be public domain, are Copyright 1995-2014 - Space Media Network. AFP, UPI and IANS news wire stories are copyright Agence France-Presse, United Press International and Indo-Asia News Service. ESA Portal Reports are copyright European Space Agency. All NASA sourced material is public domain. Additional copyrights may apply in whole or part to other bona fide parties. Advertising does not imply endorsement,agreement or approval of any opinions, statements or information provided by Space Media Network on any Web page published or hosted by Space Media Network. Privacy Statement