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PLANCK steps closer to the cosmic blueprint

14/02/2012

RELEASE FROM THE EUROPEAN SPACE AGENCY - 13 February 2011

Image crédits: ESA/consortia HFI/LFI+ T. dame et al., 2001

ESA’s Planck mission has revealed that our galaxy contains previously undiscovered islands of cold gas and a mysterious haze of microwaves. These results give scientists new treasure to mine and take them closer to revealing the blueprint of cosmic structure.

The new results are being presented this week at an international conference in Bologna, Italy, where astronomers from around the world are discussing the mission’s intermediate results.

These results include the first map of carbon monoxide to cover the entire sky. Carbon monoxide is a constituent of the cold clouds that populate the Milky Way and other galaxies. Predominantly made of hydrogen molecules, these clouds provide the reservoirs from which  stars are born.

However, hydrogen molecules are difficult to detect because they do not readily emit radiation. Carbon monoxide forms under similar  conditions and, even though it is much rarer, it emits light more readily and therefore is more easily detectable. So, astronomers use  it to trace the clouds of hydrogen.

“Planck turns out to be an excellent detector of carbon monoxide across the entire sky,” says Planck collaborator Jonathan Aumont from  the Institut d’Astrophysique Spatiale, Universite Paris XI, Orsay, France.

Surveys of carbon monoxide undertaken with radio telescopes on the ground are extremely time consuming, hence they are limited to  portions of the sky where molecular clouds are already known or expected to exist.

“The great advantage of Planck is that it scans the whole sky, allowing us to detect concentrations of molecular gas where we didn’t  expect to find them,” says Dr. Aumont.

Planck has also detected a mysterious haze of microwaves that presently defies explanation.  It comes from the region surrounding the galactic center and looks like a form of energy called synchrotron emission. This is produced  when electrons pass through magnetic fields after having been accelerated by supernova explosions.

The curiosity is that the synchrotron emission associated with the galactic haze exhibits different characteristics from the synchrotron  emission seen elsewhere in the Milky Way.

The galactic haze shows what astronomers call a ‘harder’ spectrum: its emission does not decline as rapidly with increasing energies.

Several explanations have been proposed for this unusual behavior, including higher supernova rates, galactic winds and even the  annihilation of dark-matter particles.

So far, none of them has been confirmed and it remains puzzling.

“The results achieved thus far by Planck on the galactic haze and on the carbon monoxide distribution provide us with a fresh view on some  interesting processes taking place in our galaxy,” says Jan Tauber, ESA’s Project Scientist for Planck.

Planck’s primary goal is to observe the Cosmic Microwave Background (CMB), the relic radiation from the Big Bang, and to measure its  encoded information about the constituents of the Universe and the origin of cosmic structure.

But it can only be reached once all sources of foreground emission, such as the galactic haze and the carbon monoxide signals, have been  identified and removed.

“The lengthy and delicate task of foreground removal provides us with prime datasets that are shedding new light on hot topics in galactic  and extragalactic astronomy alike,” says Dr. Tauber. “We look forward to characterizing all foregrounds and then being able to reveal the CMB in unprecedented detail.”

Planck’s first cosmological dataset is expected to be released in 2013.
 

Media Contact:

 Markus Bauer
 ESA Science and Robotic Exploration Communication Officer
 +31 71 565 6799; cell: +31 61 594 3 954
markus.bauer@esa.int

Science Contacts:
 Jan Tauber
 ESA Planck Project Scientist
 +31 71 565 5342
 jan.tauber@esa.int
 Jean-Loup Puget
 Institut d’Astrophysique Spatiale
 CNRS-Université Paris Sud, France
 +33 1 69 85 86 65
jean-loup.puget@ias.u-psud.fr

Link:

Text&  Images:
http://www.esa.int/export/esaSC/SEM0FLYXHYG_index_0.html

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