Press Release

Our Galaxy’s Geysers are Towers of Power

By SpaceRef Editor
January 2, 2013
Filed under , , ,

“Monster” outflows of charged particles from the center of our galaxy, stretching more than halfway across the sky, have been detected and mapped with CSIRO’s 64-m (210-ft) Parkes radio telescope in eastern Australia.

The outflows were detected by astronomers from Australia, the USA, Italy and The Netherlands. They report their finding in today’s issue of Nature.

“These outflows contain an extraordinary amount of energy — about a million times the energy of an exploding star,” said the research team’s leader, CSIRO’s Dr. Ettore Carretti.

But the outflows pose no danger to Earth or the solar system.

The speed of the outflow is supersonic, about 1000 kilometers a second. “That’s fast, even for astronomers,” Dr. Carretti said.

“They are not coming in our direction, but go up and down from the galactic plane. We are 30,000 light-years away from the galactic center, in the plane. They are no danger to us.”

From top to bottom the outflows extend 50,000 light-years [five hundred thousand million million kilometers] out of the galactic plane.

That’s equal to half the diameter of our galaxy (which is 100,000 light-years — a million million million kilometers — across).

Seen from Earth, the outflows stretch about two-thirds across the sky from horizon to horizon.

The outflows correspond to a “haze” of microwave emission previously spotted by the WMAP and Planck space telescopes and regions of gamma-ray emission detected with NASA’s Fermi space telescope in 2010, which were dubbed the “Fermi Bubbles”.

The WMAP, Planck and Fermi observations did not provide enough evidence to indicate definitively the source of the radiation they detected, but the new Parkes observations do.

“The options were a quasar-like outburst from the black hole at the galactic center, or star-power — the hot winds from young stars, and exploding stars,” said team member Dr. Gianni Bernardi of the Harvard-Smithsonian Center for Astrophysics, in Cambridge, Massachusetts.

“Our observations tell us it’s star-power.”

In fact, the outflows appear to have been driven by many generations of stars forming and exploding in the galactic center over the last hundred million years.

The key to determining this was to measure the outflows’ magnetic fields.

“We did this by measuring a key property of the radio waves from the outflows — their polarization,” said team member Dr. Roland Crocker of the Max-Planck-Institut fuer Kernphysik in Heidelberg, Germany, and the Australian National University.

The new observations also help to answer one of astronomers’ big questions about our galaxy: how it generates and maintains its magnetic field.

“The outflow from the galactic center is carrying off not just gas and high-energy electrons, but also strong magnetic fields,” said team member Dr. Marijke Haverkorn of Radboud University Nijmegen in The Netherlands.

“We suspect this must play a big part in generating the galaxy’s overall magnetic field.”

PIO Contact:
Helen Sim
CSIRO Astronomy and Space Science
+61 419 635 905

Science Contacts:
Dr. Ettore Carretti
Senior Systems Scientist, CSIRO Astronomy and Space Science
+61 424 104 542 (currently in the UK)

Dr. Gianni Bernardi
Harvard-Smithsonian Center for Astrophysics
+39 339 895 9270 (Currently in Italy)

Dr. Roland Crocker
Max-Planck-Institut fuer Kernphysik and the Australian National University
+61 438 499 129

Dr. Marijke Haverkorn
Radboud University Nijmegen, The Netherlands
+31 (0)24 365 2809

Reference: Ettore Carretti, Roland M. Crocker, Lister Staveley-Smith, Marijke Haverkorn, Cormac Purcell, B. M. Gaensler, Gianni Bernardi, Michael J. Kesteven & Sergio Poppi. “Giant magnetized outflows from the center of the Milky Way.” Nature, volume 493, issue 7430, pp 66-69. DOI: 10.1038/nature11734


Caption: The new-found outflows of particles (pale blue) from the galactic Center. The background image is the whole Milky Way at the same scale. The curvature of the outflows is real, not a distortion caused by the imaging process.

Credit: radio image — E. Carretti (CSIRO); radio data — S-PASS team; optical image — A. Mellinger (Central Michigan University); scientific imager, E. Bressert (CSIRO)

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SpaceRef staff editor.