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Max Planck Institute for Extraterrestrial Physics

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effects of the Earth's atmosphere, but also instruments on ground-based observatories are used whenever possible. Scientific work is done in four major research areas that are supervised by one of the directors, respectively: optical and interpretative astronomy (Bender), infrared and sub-millimeter/millimeter astronomy (Genzel), high-energy astrophysics (Nandra), and in the Centre for Astrochemical Studies (Caselli). Within these areas scientists lead individual experiments and research projects organised in about 25 project teams. The research topics pursued at MPE range from the physics of cosmic plasmas and of stars to the physics and chemistry of interstellar matter, from star formation and nucleosynthesis to extragalactic astrophysics and cosmology.
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this department into a sub-institute of the Max Planck Institute for Physics and Astrophysics on May 15, 1963. Professor Lüst was appointed director of the institute. Another Senate resolution on March 8, 1991, finally established MPE as an autonomous institute within the Max Planck Society. It is dedicated to the experimental and theoretical exploration of the space outside of Earth as well as astrophysical phenomena. A continuous reorientation to new, promising fields of research and the appointment of new members ensures steady advancement.
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1980, because of a burning instability in the first stage of the launch rocket. The same fate was to overtake the four satellites of the CLUSTER-Mission on June 4, 1996, when the first Ariane 5 was launched. This time the disaster was attributed to an error in the rocket's software. The most recent loss was "ABRIXAS", an X-ray satellite built by industry under the leadership of MPE. After few hours in orbit, a malfunction of the power system caused the total loss of the satellite.
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this department into a sub-institute of the Max-Planck-Institute for Physics and Astrophysics on May 15, 1963. Professor Lüst was appointed director of the institute. Another Senate resolution on March 8, 1991, finally established MPE as an autonomous institute within the Max-Planck-Gesellschaft. It is dedicated to the experimental and theoretical exploration of the space outside of Earth as well as astrophysical phenomena.
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students). It is noteworthy that permanent positions at the institute have not increased since 1973 - despite its celebrated scientific achievements. The increasingly complex tasks and international obligations have been mainly maintained by staff members with positions having limited duration and funded by external organizations.
58:. The Max Planck Institute for Extraterrestrial Physics was founded as sub-institute in 1963. The scientific activities of the institute are mostly devoted to astrophysics with telescopes orbiting in space. A large amount of the resources are spent for studying black holes in the Milky Way Galaxy and in the remote universe. 203:
Another field of research also became important: astrophysical observations of electromagnetic radiation which could not be observed from the surface of the Earth because the wavelengths are such that the radiation is absorbed by the Earth's atmosphere. These observations and inferences therefrom are
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New observation techniques using satellites has necessitated the recording, processing and accessible storage of high data fluxes over long periods of time. This demanding task is performed by a data processing group, which has grown quickly in the last decade. Special data centers were established
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During the early years, the scientific work at the Institute concentrated on the investigation of extraterrestrial plasmas and the magnetosphere of the Earth. This work was performed with measurements of particles and electromagnetic fields as well as a specially developed ion-cloud technique using
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Because the institute has assumed a leading position in astronomy internationally, it has attracted guest scientists throughout the world. The number of long-term guests increased from 12 in 1974 to a maximum of 72 in 2000. In recent years MPE has hosted an average of about 50 guest scientists each
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Besides the many successes, there have also been disappointments. The malfunctioning of the Ariane carrier rockets on test launches in 1980 and 1996 were particularly bitter setbacks. The satellite "Firewheel", in which many members of the Institute had invested years of work, was lost on May 23,
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The Max Planck Institute for Extraterrestrial Physics (MPE) was preceded by the department for extraterrestrial Physics in the Max Planck Institute for Physics and Astrophysics. This department was established by Professor Reimar Lüst on October 23, 1961. A Max-Planck Senate resolution transformed
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The Max-Planck-Institute for extraterrestrial physics (MPE) was preceded by the department for extraterrestrial physics in the Max-Planck-Institute for physics and astrophysics. This department was established by Professor Reimar Lüst on October 23, 1961. A Max-Planck Senate resolution transformed
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The institute was founded in 1963 as a sub-institute of the Max-Planck-Institut für Physik und Astrophysik and established as an independent institute in 1991. Its main research topics are astronomical observations in spectral regions which are only accessible from space because of the absorbing
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Many experiments of the Max Planck Institute for Extraterrestrial Physics (MPE) have to be carried out above the dense Earth's atmosphere using aircraft, rockets, satellites and space probes. In the early days experiments were also flown on balloons. To run advanced extraterrestrial physics and
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Scientific projects at the MPE are often the efforts of the different research departments to build, maintain, and use experiments and facilities which are needed by the many different scientific research interest at the institute. Apart from hardware projects, there are also projects that use
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Since the 1990s, satellites have become the preferred observation platforms because of their favorable observation-time/cost ratio. Nevertheless, high-flying observation airplanes and ground-based telescopes are also used to obtain data, especially for optical and near-infrared observations.
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Among the 29 employees of the Institute when it was founded in 1963 were 9 scientists and 1 Ph.D. student. Twelve years later in 1975 the number of employees had grown to 180 with 55 scientists and 13 Ph.D. students, and today (status 2015) there are some 400 staff (130 scientists and 75 PhD
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the subject matter of infra-red astronomy as well as X-ray- and gamma-ray-astronomy. In addition to more than 100 rockets, an increasing number of high-altitude balloons (up to now more than 50; e.g. HEXE) have been used to carry experiments to high altitudes.
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Observers and experimenters perform their research work at the institute in close contact with each other. Their interaction while interpreting observations and propounding new hypotheses underlies the successful progress of the institute's research projects.
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state-of-the-art experimental astrophysics, the institute continues to develop high-tech instrumentation in-house. This includes detectors, spectrometers, and cameras as well as telescopes and complete payloads (e.g.
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At the end of the year 2022 a total of 508 employees were working at the institute, numbering among them about 100 scientists, 60 junior scientists, 10 apprentices and 140 visiting researchers.
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1990 Joachim Trümper together with the MPI for Physics (MPP) founds the semiconductor laboratory as a joint project between the MPE and the MPP (since 2012 operated by the MPG)
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Deep observations of the extragalactic X-ray sky with ROSAT, XMM-Newton and Chandra and resolving the background radiation into individual sources (since 1998)
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Desert and is planned to be finished by 2027, MPE is developing the first-light instrument MICADO (Multi-AO Imaging Camera for Deep Observations).
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The first detection of water-molecule lines in an expanding shell of a star using the Fabry-Perot spectrometer on board the ISO satellite (1996)
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2001 The "International Max-Planck- Research School on Astrophysics" (IMPRS) is opened by MPE, MPA, ESO, MPP and the universities of Munich
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The measurement of the element- and isotope-composition of the solar wind by the CELIAS experiment on board the SOHO satellite (1996)
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First gamma-ray sky map in the energy range 3 to 10 MeV as measured with the imaging Compton telescope COMPTEL on board CGRO (1994)
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The ERIS (Enhanced Resolution Imager and Spectrograph) infrared camera will replace the NACO and SINFONI instruments at the VLT.
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Measurement of the magnetic field of the neutron star Her-X1 using the cyclotron line emission (balloon experiments 1978)
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archival data and are not necessarily connected to a new instrument. A brief overview of the most recent projects.
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2000 G. Morfill together with the IPP founds the "Center for Interdisciplinary Plasma Science" (CIPS) (until 2004)
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The first map of the X-ray sky as measured with the imaging X-ray telescope on board the ROSAT satellite (1993)
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2002 Ralf Bender becomes scientific member and director at the institute (optical and interpretative astronomy)
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The first map of the galactic gamma-ray emission ( > 70 MeV) as measured with the satellite COS-B (1978)
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Confirmation that a supermassive black hole resides at the centre of the Milky Way Galaxy (2002)
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Determining the energy source for ultraluminous infrared galaxies with the satellite ISO (1998)
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The plasma-crystal experiment and its successors on the International Space Station (1996–2013)
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2001 Günther Hasinger becomes scientific member and director at the institute (X-ray astronomy)
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1975 Joachim Trümper becomes director and scientific member at the institute (X-ray astronomy)
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becomes scientific member and director at the institute (infrared-/submillimeter astronomy)
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Over the years, however, the history of MPE is primarily a story of scientific successes.
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becomes scientific member and director at the institute (Center for Astrochemical Studies)
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founds the "UCB-MPG Center for International Exchange in Astrophysics and Space Science"
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1963 Foundation as a sub-institute within the MPI für Physik und Astrophysik; director
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Max Planck Harvard Research Center for the Archaeoscience of the Ancient Mediterranean
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Resolving the cosmic infrared background into individual galaxies with Herschel (2011)
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Exploration of the Ionosphere and Magnetosphere by means of ion clouds (1963–1985)
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becomes scientific member and director at the institute (high-energy astrophysics)
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1969 Klaus Pinkau becomes director at the institute (cosmic rays, gamma-astronomy)
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Determining the gas content of normal galaxies in the early universe (since 2010)
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https://web.archive.org/web/20120609132517/http://www.mpia.de/Public/menu-e.php
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Reconstruction of the evolution history of stars in elliptical galaxies (2005)
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1981 The MPE X-ray test facility "Panter" located in Neuried starts operation
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in July 2019, the first complete sky survey in the X-ray range was achieved.
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becomes director and scientific member at the institute (infrared astronomy)
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Stellar disks rotating around the black hole in the Andromeda galaxy (2005)
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split up into the Max Planck Institute for Extraterrestrial Physics, the
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Detection of gamma-ray line emission (Ti) from supernova remnants (1998)
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First detection of X-ray emission from comets and planets (1996, 2001)
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The GRAVITY instrument enables the four 8-metre telescopes at the
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becomes director and scientific member at the institute (theory)
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Detection of a binary active galactic nucleus in X-rays (2003)
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Numerical simulation of a collision-free shock wave (1990)
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Major events in the history of the institute include:
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Experimental proof of the reconnection process (1979)
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Genzel together with the 715:Study of Crime, Security and Law 52:Max Planck Institute for Physics 1059:Molecular and Cellular Biology 735:Dynamics and Self-Organization 492: 474:"History of the MPE: Overview" 373:and an extended field of view. 1: 805:Immunobiology and Epigenetics 765:Friedrich Miescher Laboratory 429: 850:Social Law and Social Policy 705:Research on Collective Goods 7: 1437:Physics research institutes 1310:Christiane Nüsslein-Volhard 865:Mathematics in the Sciences 336: 70: 10: 1458: 1386:Max Planck Digital Library 1115:Experimental Endocrinology 1026:Ernst Strüngmann Institute 950:Molecular Plant Physiology 920:Physics of Complex Systems 915:Chemical Physics of Solids 895:Multidisciplinary Sciences 835:Tax Law and Public Finance 820:Innovation and Competition 750:Chemical Energy Conversion 61: 1373: 1218: 1153: 1092: 1039: 1018: 625:Evolutionary Anthropology 613: 16:German research institute 1135:Physics and Astrophysics 930:Extraterrestrial Physics 900:Neurobiology of Behavior 885:Terrestrial Microbiology 800:Science of Human History 159:for his research on the 1054:Heart and Lung Research 945:Plant Breeding Research 785:Heart and Lung Research 710:Colloids and Interfaces 665:Biological Intelligence 1379:Kaiser Wilhelm Society 1334:Emmanuelle Charpentier 1140:Psychological Research 890:Microstructure Physics 855:European Legal History 760:Neuroscience (Florida) 720:Biological Cybernetics 650:Art History (Florence) 348:EUCLID space telescope 310: 153:Nobel Prize in Physics 23: 1422:Max Planck Institutes 1100:Behavioral Physiology 1019:Associated institutes 1010:Sustainable Materials 1000:Solar System Research 780:Gravitational Physics 770:Fritz Haber Institute 675:Molecular Biomedicine 560:48.26167°N 11.67167°E 409:http://www.mpe.mpg.de 301:Agreement Signed for 300: 223:Selected achievements 163:at the centre of the 22: 1442:Garching bei München 1256:Georges J. F. Köhler 1049:Evolutionary Biology 1005:Solid State Research 985:Security and Privacy 940:Molecular Physiology 755:Evolutionary Biology 725:Demographic Research 480:on 16 September 2011 454:on 16 September 2011 448:"History of the MPE" 419:http://www.nasa.gov/ 363:Very Large Telescope 1427:Education in Munich 880:Marine Microbiology 825:Intelligent Systems 630:Social Anthropology 556: /  1274:Johann Deisenhofer 1262:Klaus von Klitzing 1079:Organismal Biology 990:Study of Societies 790:History of Science 775:Molecular Genetics 645:Art History (Rome) 606:Max Planck Society 565:48.26167; 11.67167 311: 200:sounding rockets. 32:Max Planck Society 24: 1409: 1408: 1316:Theodor W. Hänsch 1093:Former institutes 1069:Molecular Biology 970:Psycholinguistics 810:Infection Biology 795:Human Development 670:Biology of Ageing 376:For the 39-metre 371:laser guide stars 90:Gerhard Haerendel 1449: 1401: 1400:Schloss Ringberg 1394: 1387: 1380: 1352:Klaus Hasselmann 1203:Martin Stratmann 1042:research schools 995:Software Systems 960:Polymer Research 910:Science of Light 870:Medical Research 745:Chemical Ecology 617: 607: 598: 591: 584: 575: 574: 571: 570: 568: 567: 566: 561: 557: 554: 553: 552: 549: 537: 536: 534: 532: 523:. Archived from 517: 511: 510: 508: 506: 496: 490: 489: 487: 485: 476:. Archived from 470: 464: 463: 461: 459: 450:. Archived from 444: 183:Detailed history 176:Frank Eisenhauer 1457: 1456: 1452: 1451: 1450: 1448: 1447: 1446: 1412: 1411: 1410: 1405: 1399: 1392: 1385: 1378: 1369: 1340:Reinhard Genzel 1304:Paul J. Crutzen 1219:Nobel laureates 1214: 1167:Adolf Butenandt 1149: 1088: 1041: 1035: 1014: 980:Radio Astronomy 935:Nuclear Physics 660:Biogeochemistry 615: 609: 605: 602: 564: 562: 558: 555: 550: 547: 545: 543: 542: 540: 530: 528: 519: 518: 514: 504: 502: 498: 497: 493: 483: 481: 472: 471: 467: 457: 455: 446: 445: 436: 432: 405: 367:adaptive optics 339: 295: 293:Scientific work 225: 185: 157:Reinhard Genzel 110:Reinhard Genzel 73: 64: 30:is part of the 17: 12: 11: 5: 1455: 1445: 1444: 1439: 1434: 1429: 1424: 1407: 1406: 1404: 1403: 1396: 1389: 1382: 1374: 1371: 1370: 1368: 1367: 1361: 1355: 1349: 1343: 1337: 1331: 1328:Stefan W. Hell 1325: 1319: 1313: 1307: 1301: 1295: 1289: 1286:Hartmut Michel 1283: 1277: 1271: 1265: 1259: 1253: 1247: 1241: 1235: 1229: 1222: 1220: 1216: 1215: 1213: 1212: 1209:Patrick Cramer 1206: 1200: 1194: 1188: 1185:Hans F. 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Index


Max Planck Society
Garching
Munich
Germany
Max Planck Institute for Physics
Max Planck Institute for Astrophysics
Reimar Lüst
Gerhard Haerendel
Gregor Morfill
Reinhard Genzel
University of California Berkeley
Kirpal Nandra
Paola Caselli
Nobel Prize in Physics
Reinhard Genzel
black hole
Milky Way
Sagittarius A*
Frank Eisenhauer

MICADO
E-ELT
ROSAT
eROSITA
EUCLID space telescope
dark matter
dark energy
Very Large Telescope
adaptive optics

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