A small galaxy, called Sextans A, is shown here in a multi-wavelength
mosaic captured by the European Space Agency's Herschel mission, in
which NASA is a partner, along with NASA's Galaxy Evolution Explorer
(GALEX) and the National Radio Astronomy Observatory's Jansky Very Large
Array observatory near Socorro, New Mexico. Image credit:
ESA/NASA/JPL-Caltech/NRAO. Full image and caption
What makes one rose bush blossom with flowers, while another remains
barren? Astronomers ask a similar question of galaxies, wondering how
some flourish with star formation and others barely bloom.
A new study published in the Oct. 16 issue of the journal Nature
addresses this question by making some of the most accurate measurements
yet of the meager rates at which small, sluggish galaxies create stars.
The report uses data from the European Space Agency's Herschel mission,
in which NASA is a partner, and NASA's Spitzer Space Telescope and
Galaxy Evolution Explorer (GALEX).
The findings are helping researchers figure out how the very first
stars in our universe sprouted. Like the stars examined in the new
study, the first-ever stars from billions of years ago took root in poor
conditions. Growing stars in the early cosmos is like trying to
germinate flower seeds in a bed of dry, poor soil. Back then, the
universe hadn't had time yet to make "heavy metals," elements heavier
than hydrogen and helium.
"The metals in space help act in some ways like a fertilizer to help
stars grow," said George Helou, an author of the new study and director
of NASA's Infrared Processing and Analysis Center (IPAC) at the
California Institute of Technology, Pasadena. The lead author of the
study is Yong Shi, who performed some of the research at IPAC before
moving to Nanjing University in China.
The two slow-going galaxies in the study, called Sextans A and ESO
146-G14, lack in heavy metals, just like our young and remote cosmos,
only they are a lot closer to us and easier to see. Sextans A is
located about 4,500 light-years from Earth, and ESO 146-G14 is more than
70,000 light-years away.
These smaller galaxies are late bloomers. They managed to travel
through history while remaining pristine, and never bulked up in heavy
metals (heavy metals not only help stars to form, but are also created
themselves by stars).
"The metal-poor galaxies are like islands left over from the early
universe," said Helou. "Because they are relatively close to us, they
are especially valuable windows to the past."
Studying star formation in poor growing environments such as these is
tricky. The galaxies, though nearby, are still faint and hard to see.
Shi and his international team wrangled the problem with a
multi-wavelength approach. The Herschel data, captured at the longest
infrared wavelengths of light, let the researchers see the cool dust in
which stars are buried. The dust serves as a proxy for the total amount
of gas in the region -- the basic ingredient of stars. To other
telescopes, this dust is cold and invisible. Herschel, on the other
hand, can pick up its feeble glow.
Supporting radio-wavelength measurements of some of the gas in the
galaxies came from the National Radio Astronomy Observatory's Jansky
Very Large Array observatory near Socorro, New Mexico, and the Australia
Telescope Compact Array observatory, near Narrabri.
Meanwhile, archived data from Spitzer and GALEX were used to look at
the rate of star formation. Spitzer sees shorter-wavelength infrared
light, which comes from dust that is warmed by new stars. GALEX images
capture ultraviolet light from the shining stars themselves.
Putting all these pieces together enabled the astronomers to
determine that the galaxies are plodding along, creating stars at rates
10 times lower than their normal counterparts.
"Star formation is very inefficient in these environments," said Shi.
"Extremely metal-poor nearby galaxies are the best way to know what
went on billions of years ago."
The heavy metals in present-day galaxies help star formation to
flourish through cooling effects. For a star to form, a ball of gas
needs to fall in on itself with the help of its own gravity. Ultimately,
the material has to become dense enough for atoms to fuse and ignite,
creating starlight. But as this cloud collapses, it heats up and puffs
back out again, counteracting the process. Heavy metals cool everything
down by radiating away the heat, enabling the cloud to condense into a
star.
How stars in the early universe were able to do this without the cooling benefits of heavy metals remains unknown.
Studies like this shine light on the very first stellar buds, giving us a glimpse into the roots of our cosmic history.
NASA's Jet Propulsion Laboratory, Pasadena, California, manages the
Spitzer Space Telescope mission for NASA's Science Mission Directorate,
Washington. The GALEX mission, which ended in 2013, was also managed by
JPL for NASA and led by Caltech. JPL served as the NASA Herschel Project
Office for the European Space Agency's Herschel mission, which also
ended in 2013.
Data from Spitzer and Herschel are accessible through the Infrared
Science Archive housed at the Infrared Processing and Analysis Center at
Caltech. Caltech manages JPL for NASA.
Media Contact
Whitney Clavin
818-354-4673
Jet Propulsion Laboratory, Pasadena, Calif.
whitney.clavin@jpl.nasa.gov
