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Fig. 1:
Artist's impression of the Planck spacecraft
Credits: ESA - C. Carreau
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Fig. 2:
The anisotropies of the cosmic microwave background (CMB) as observed by Planck.
Credit: ESA and the Planck Collaboration
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Mission controllers at ESA’s operations centre in Darmstadt, Germany
sent the final command to the Planck satellite on 23 October. Launched
in 2009, Planck was designed to tease out the faintest relic radiation
from the Big Bang – the Cosmic Microwave Background (CMB). The CMB
preserves a picture of the Universe as it was about 380 000 years
after the Big Bang, and provides details of the initial conditions
that led to the Universe we live in today.
The mission began drawing to a close in August, when the satellite was
nudged away from its operational orbit around the Sun–Earth "L2" point
towards a more distant long-term stable parking orbit around the
Sun. In the last weeks, the spacecraft has been prepared for permanent
hibernation, with the closing activities using up all of the remaining
fuel and finally switching off the transmitter.
The mission’s instrumentation needed to be maintained at just
one-tenth of a degree above the coldest temperature reachable in the
Universe, –273.15°C, so that the spacecraft’s own heat did not swamp
the signal from the sky. This enabled temperature variations of just a
few millionths of a degree to be distinguished in the CMB. But cooling
instruments to these extreme temperatures cannot be maintained forever
and, indeed, the
High Frequency Instrument (HFI) exhausted its liquid
helium coolant in January 2012, just as expected.
The Low Frequency Instrument (LFI) meanwhile was able to operate at
somewhat higher temperatures using the remaining two coolers and
continued making observations until 3 October. After conducting
post-science activities, it was manually switched off on 19 October.
The mission’s original target was to complete two whole surveys of the
sky but, in the end, Planck completed five full-sky surveys with both
instruments. Moreover, by mid-August, LFI had completed its eighth
survey of the entire sky. The first detailed image of the faint signal
from the CMB from Planck
was released earlier this year,
after foreground emission from our own Milky Way Galaxy as well as all
other galaxies had been removed. These latter data resulted in a new
catalogue of objects, including many never-before-seen galaxy clusters
in the distant Universe.
The 2013 data release provided revised values for the relative
proportions of the ingredients of the Universe, namely normal matter
that makes up stars and galaxies, dark matter, which has thus far only
been detected indirectly by its gravitational influence, and dark
energy, a mysterious force thought to be responsible for accelerating
the expansion of the Universe.
Link:
Full ESA Press Release: Planck on course for safe retirement
Contact:
Dr. Torsten Enßlin
Max-Planck-Institut für Astrophysik
Tel. 089 30000-2243
E-mail: tensslinmpa-garching.mpg.de
Dr. Hannelore Hämmerle
Pressesprecherin
Max-Planck-Institut für Astrophysik
und Max-Planck-Institut für extraterrestrische Physik
Tel. 089 30000-3980
E-mail: prmpa-garching.mpg.de
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