epa03817047 (FILE) A National Aeronautics and Space Administration (NASA) handout photo made available 20 May 2009 and taken by an STS-125 crew member aboard the Space Shuttle Atlantis shows the Hubble Space Telescope as the two spacecraft continued their relative separation on 19 May 2009, after having been linked together for a time to complete a final servicing mission for the orbital observatory by sevral Shuttle crew spacewalks. NASA on 08 August 2013 reports that astronomers using NASA's Hubble Space Telescope have solved a 40-year mystery on the origin of the Magellanic Stream, a long ribbon of gas stretching nearly halfway around our Milky Way galaxy. A team of astronomers, led by Andrew J. Fox of the Space Telescope Science Institute in Baltimore, Md., USA, determined the source of the gas filament by using Hubble's Cosmic Origins Spectrograph to measure the amount of heavy elements, such as oxygen and sulfur, at six locations along the Magellanic Stream. They observed faraway quasars, the brilliant cores of active galaxies, that emit light that passes through the stream. They detected the heavy elements from the way the elements absorb ultraviolet light. EPA/NASA / HANDOUT HANDOUT EDITORIAL USE ONLY
epa03817047 (FILE) A National Aeronautics and Space Administration (NASA) handout photo made available 20 May 2009 and taken by an STS-125 crew member aboard the Space Shuttle Atlantis shows the Hubble Space Telescope as the two spacecraft continued their relative separation on 19 May 2009, after having been linked together for a time to complete a final servicing mission for the orbital observatory by sevral Shuttle crew spacewalks. NASA on 08 August 2013 reports that astronomers using NASA's Hubble Space Telescope have solved a 40-year mystery on the origin of the Magellanic Stream, a long ribbon of gas stretching nearly halfway around our Milky Way galaxy. A team of astronomers, led by Andrew J. Fox of the Space Telescope Science Institute in Baltimore, Md., USA, determined the source of the gas filament by using Hubble's Cosmic Origins Spectrograph to measure the amount of heavy elements, such as oxygen and sulfur, at six locations along the Magellanic Stream. They observed faraway quasars, the brilliant cores of active galaxies, that emit light that passes through the stream. They detected the heavy elements from the way the elements absorb ultraviolet light. EPA/NASA / HANDOUT HANDOUT EDITORIAL USE ONLY
© APA/NASA / HANDOUT

Astronomie

Spektrometer für Hubble-Nachfolger ist fertig

Es soll noch tiefer ins Weltall schauen und Bilder von weit entfernten Himmelskörpern liefern: das neue "Superauge" für den Nachfolger des Weltraumteleskops "Hubble". Das vom Raumfahrtunternehmen Astrium entwickelte, 230 Kilogramm schwere Spektrometer erkennt noch so schwache Infrarotstrahlung. Es macht nicht nur Aufnahmen, sondern analysiert auch die Zusammensetzung der Materie in den Tiefen des Alls. "NIRSpec" kann 100 Galaxien gleichzeitig beobachten. Am Freitag wurde das 160 Millionen Euro teure Superauge vor dem Transport zur NASA in Taufkirchen bei München übergeben.

Astrium-Chef Eric Beranger nannte es eine besondere Herausforderung, das Spektrometer unter Normalbedingungen für den Betrieb in der Schwerelosigkeit und bei minus 235 Grad Celsius zu bauen. "Heute sehen wir unser Baby", sagte Beranger zu NASA-Vertreter Eric Smith, der für das neue Weltraumteleskop "James Webb" zuständig ist. Es soll 2018 ins All gebracht werden.

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