NASA's Spitzer Finds Distant Galaxies Grazed on Gas

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News release: 2011-200 June 30, 2011

NASA's Spitzer Finds Distant Galaxies Grazed on Gas

The full version of this story with accompanying images is at:
http://www.jpl.nasa.gov/news/news.cfm?release=2011-200&cid=release_2011-200

PASADENA, Calif. -- Galaxies once thought of as voracious tigers are more like grazing cows,
according to a new study using NASA's Spitzer Space Telescope.

Astronomers have discovered that galaxies in the distant, early universe continuously ingested their
star-making fuel over long periods of time. This goes against previous theories that the galaxies
devoured their fuel in quick bursts after run-ins with other galaxies.

"Our study shows the merging of massive galaxies was not the dominant method of galaxy growth
in the distant universe," said Ranga-Ram Chary of NASA's Spitzer Science Center at the California
Institute of Technology in Pasadena, Calif. "We're finding this type of galactic cannibalism was rare.
Instead, we are seeing evidence for a mechanism of galaxy growth in which a typical galaxy fed
itself through a steady stream of gas, making stars at a much faster rate than previously thought."

Chary is the principal investigator of the research, appearing in the Aug. 1 issue of the Astrophysical
Journal. According to his findings, these grazing galaxies fed steadily over periods of hundreds of
millions of years and created an unusual amount of plump stars, up to 100 times the mass of our sun.

"This is the first time that we have identified galaxies that supersized themselves by grazing," said
Hyunjin Shim, also of the Spitzer Science Center and lead author of the paper. "They have many
more massive stars than our Milky Way galaxy."

Galaxies like our Milky Way are giant collections of stars, gas and dust. They grow in size by
feeding off gas and converting it to new stars. A long-standing question in astronomy is: Where did
distant galaxies that formed billions of years ago acquire this stellar fuel? The most favored theory
was that galaxies grew by merging with other galaxies, feeding off gas stirred up in the collisions.

Chary and his team addressed this question by using Spitzer to survey more than 70 remote galaxies
that existed 1 to 2 billion years after the Big Bang (our universe is approximately 13.7 billion years
old). To their surprise, these galaxies were blazing with what is called H alpha, which is radiation
from hydrogen gas that has been hit with ultraviolet light from stars. High levels of H alpha indicate
stars are forming vigorously. Seventy percent of the surveyed galaxies show strong signs of H alpha.
By contrast, only 0.1 percent of galaxies in our local universe possess this signature.

Previous studies using ultraviolet-light telescopes found about six times less star formation than
Spitzer, which sees infrared light. Scientists think this may be due to large amounts of obscuring
dust, through which infrared light can sneak. Spitzer opened a new window onto the galaxies by
taking very long-exposure infrared images of a patch of sky called the GOODS fields, for Great
Observatories Origins Deep Survey.

Further analyses showed that these galaxies furiously formed stars up to 100 times faster than the
current star-formation rate of our Milky Way. What's more, the star formation took place over a long
period of time, hundreds of millions of years. This tells astronomers that the galaxies did not grow
due to mergers, or collisions, which happen on shorter timescales. While such smash-ups are
common in the universe -- for example, our Milky Way will merge with the Andromeda galaxy in
about 5 billion years -- the new study shows that large mergers were not the main cause of galaxy
growth. Instead, the results show that distant, giant galaxies bulked up by feeding off a steady supply
of gas that probably streamed in from filaments of dark matter.

Chary said, "If you could visit a planet in one of these galaxies, the sky would be a crazy place, with
tons of bright stars, and fairly frequent supernova explosions."

NASA's Jet Propulsion Laboratory in Pasadena, Calif., manages the Spitzer Space Telescope
mission for the agency's Science Mission Directorate in Washington. Science operations are
conducted at the Spitzer Science Center at Caltech. Caltech manages JPL for NASA.

For more information about Spitzer, visit http://www.nasa.gov/spitzer and
http://spitzer.caltech.edu/ .

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