Dr. Hannelore Hämmerle
Dr. Hannelore Hämmerle
Press Officer
Phone:+49 89 30000-3980Fax:+49 89 30000-3569

All News (2011 - ....)

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One-Percent Measure of the Universe Constrains Dark Energy

January 08, 2014
At the January AAS meeting, researchers from the Baryon Oscillation Spectroscopic Survey (BOSS) announced that they have measured the distance to galaxies more than six billion light years away to an accuracy of one percent. Together with information on the rate at which the Universe was expanding, these measurements allow the scientists at the Max Planck Institute for Extraterrestrial Physics to place powerful constraints on the properties of the mysterious Dark Energy. This component is thought to be responsible for the current accelerated expansion of the Universe. [more]
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Parents’ Office at MPE

December 19, 2013
For more than half a year, since May 2013, parents with young children benefit from a new service at MPE: the Institute now offers a parents office which provides a laptop workplace for parents, and toys as well as a bed and a changing table for children. The parents office is open to all MPE employees and IMPRS students with children, who need the room once in a while, e.g. on a day when their usual childcare is unavailable. It is located next to the print shop, in room 2C7. [more]
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Universe PhD Awards for Oliver Pfuhl

December 12, 2013
This year’s “Universe Award” in the category “experiment” goes to Oliver Pfuhl from the IR group at MPE. In his dissertation he developed innovative components for the GRAVITY interferometer. The prize for the best theoretical work was awarded to Martin Winkler (TUM). During the Science Week 2013 of the excellence clusters both junior scientists were presented with their awards, which are endowed with 2000 Euros each.   [more]
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Meeting of MPG mechanical engineers

December 02, 2013
In mid-November, some 50 MPG workshop managers and staff members came together to share their experiences about mechanics. Topics included new developments and processes in industry as well as at the other institutes. The two-day event was organized jointly by MPE and MPP, which also provided the venues. [more]
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A New View into the Hot and Energetic Universe

November 28, 2013
ESA selects science theme for its next large mission [more]
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First Laser Beacons with ARGOS

November 19, 2013
On 5 November 2013 the ARGOS laser system has been successfully tested on the sky for the first time. From behind the secondary mirrors of the Large Binocular Telescope (LBT), a bundle of laser beams was propagated into the night skies above Arizona. [more]

eROSITA mirrors are done!

November 13, 2013
After more than seven years of development and construction, the last of the eight mirror modules for the eROSITA X-ray telescope was completed on Friday, 8 November 2013. The Max Planck Institute for Extraterrestrial Physics leads the development and construction of the entire telescope, including its various components, in an international cooperation. [more]
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Dramatic end of plasma crystal experiment

November 04, 2013
For seven years it delivered outstanding results for science and technology on the International Space Station, now the successful plasma crystal laboratory PK-3 Plus operated one last time. After undocking from the International Space Station the ESA Einstein transporter with the laboratory on board entered the Earth's atmosphere beginning of November and burned up - and PK-3 Plus produced its last plasma, a hot one. In June the operational phase of PK-3 Plus ended with a last series of experiments and with a spectacular finish; the scientists will still need some time to analyse these data. [more]
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Long arms reach out of giant cluster

September 20, 2013
Unusual structures have been found in the central region of the Coma cluster, a large collection of thousands of galaxies located about 300 million light years from Earth. Observations with the X-ray satellites Chandra and XMM-Newton led by Jeremy Sanders from Max Planck Institute for Extraterrestrial Physics revealed remarkably long arms that tell astronomers about the collisions between Coma and other galaxy clusters over the last billion years. [more]
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The inside of our Milky Way in 3D

September 12, 2013
Scientists at the Max Planck Institute for Extraterrestrial Physics have produced the first detailed three-dimensional map of the stars that form the inner regions of our Milky Way, using publicly available VVV survey data from the science archive facility at ESO. They find a box/peanut shaped bulge with an elongated bar and a prominent X-structure, which had been hinted at in previous studies. This indicates that the Milky Way was originally a pure disk of stars, which then formed a thin bar, before buckling into the box/peanut shape seen today. The new map can be used for more detailed studies of the dynamics and evolution of our Milky Way. [more]
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Primary mission for Fermi complete, much more to come

August 23, 2013
During its five-year primary mission, NASA's Fermi Gamma-ray Space Telescope has given astronomers an increasingly detailed portrait of the universe's most extraordinary phenomena, from giant black holes in the hearts of distant galaxies to thunderstorms on Earth. But its job is not done yet. On Aug. 11, Fermi entered an extended phase of its mission -- a deeper study of the high-energy cosmos. This is a significant step toward the science team's planned goal of a decade of observations, ending in 2018. MPE scientists use data from both instruments on-board Fermi, one of which was built jointly by MPE and colleagues abroad. [more]
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Close encounter: gas cloud swings around galactic centre black hole

July 16, 2013
Recent observations from April this year of the galactic centre have revealed that parts of the in-falling gas cloud, which was detected in 2011, have already swung past the black hole at the heart of our Milky Way. Due to the tidal force of the gravity monster, the gas cloud has become further stretched, with its front moving now already 500 km/s faster than its tail. This confirms earlier predictions that its orbital motion brings it is close to the black hole, that it will not survive the encounter. With the new, detailed observations, the astronomers from the Max Planck Institute for Extraterrestrial Physics can now also place new constraints the origins of the gas cloud, making it increasingly unlikely that it contains a faint star inside, from which the cloud might have formed. [more]
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