《美国光干涉仪MROI初光》

  • 来源专题:天文仪器与技术信息
  • 编译者: zwg@niaot.ac.cn
  • 发布时间:2016-12-14
  • The first of ten telescopes that will make up the Magdalena Ridge Observatory Interferometer (MROI) will experience first light on the evening of Tuesday, November 29th. The MROI First Light event will be streamed live on the Magdalena Ridge Observatory website, www.mrop.nmt.edu, starting at 7:30 Mountain Time on Tuesday, November 29th.

    The MROI is an optical interferometer with an array of ten 1.4-meter diameter telescopes spread out across the mountaintop in a Y configuration, and the light from all ten telescopes can be combined to observe objects in the sky with incredible resolution.

    “Our telescopes are unique,” said Dr. Ifan Payne, the Program Director for Magdalena Ridge Observatory, “they were specially designed for interferometry and together they will create the most powerful optical array on earth.” The degree of detail is strong enough that you could almost make out the face of a person standing on the moon, or, looking from Los Angeles, you could see a dime being held by someone in New York.

    The Magdalena Ridge Observatory Interferometer (MROI) is currently under development in the Magdalena Mountains, 28 miles west of Socorro, New Mexico. The array of 10 telescopes is located on a ridge at an altitude of 10,460 above sea level and is being designed and installed in a collaboration between New Mexico Tech and the University of Cambridge under federal funding administered by the Air Force Research Lab (AFRL) which is based in Albuquerque, NM.

    “We are thrilled that we have been able to come this far with the project,” said Dr. Payne, “It has been a long journey for a complex undertaking to which so many have contributed over the years. All of us, weather permitting of course, will be celebrate First Light as being the most significant mile stone to date on that journey.”

    Work on developing the Interferometer began when scientists from the University of Cambridge in the UK joined the team at New Mexico Tech to design the ground breaking, world-class astronomical facility. There are currently three operating optical interferometers in the world, in Arizona, California and Chile, and the MROI will be up to a thousand times more powerful than any of them. In fact, depending on the wavelength, the MROI will be 100 to 200 times more powerful than the Hubble Telescope.

    The Magdalena Ridge Observatory Interferometer is funded by a Cooperative Agreement (number FA9453-15-2-0086) with the Air Force Research Laboratory (AFRL).

  • 原文来源:http://www.mro.nmt.edu/news/mro-news
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  • 《欧洲南方天文台甚大望远镜干涉仪上中红外仪器初光》

    • 来源专题:天文仪器与技术信息
    • 编译者:zwg@niaot.ac.cn
    • 发布时间:2018-03-07
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Thomas Henning, director at the Max Planck Institute for Astronomy (MPIA) in Heidelberg, Germany, and MATISSE co-principal investigator, comments: "By looking at the inner regions of protoplanetary discs with MATISSE, we hope to learn the origin of the various minerals contained in these discs — minerals that will later go on to form the solid cores of planets like the Earth.” Walter Jaffe, the project scientist and co-principal investigator from University of Leiden in the Netherlands, and Gerd Weigelt, co-principal investigator from the Max Planck Institute for Radio Astronomy (MPIfR), Bonn, Germany, add: “MATISSE will give us dramatic images of planet-forming regions, multiple stars, and, when working with the VLT Unit Telescopes, also the dusty discs feeding supermassive black holes. 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We are looking forward to the exciting science to come!” Notes [1] MATISSE was designed, funded and built in close collaboration with ESO, by a consortium composed of institutes in France (INSU-CNRS in Paris and OCA in Nice hosting the PI team), Germany (MPIA, MPIfR and University of Kiel), the Netherlands (NOVA and University of Leiden), and Austria (University of Vienna). The Konkoly Observatory and Cologne University have also provided some support in the manufacture of the instrument. [2] With MATISSE, the last of the suite of second generation VLT/VLTI instruments has now arrived at Paranal. For the VLTI this means that 17 years — almost exactly to the day — after obtaining first fringes with VINCI and two siderostats, the first generation of instruments has now been replaced by PIONIER, GRAVITY and MATISSE, all of them combining four telescopes (UTs or ATs) and together covering a wide range of infrared wavelengths (from 1.6–13 µm). 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  • 《新原子干涉仪可以测量并记录精度的惯性力》

    • 来源专题:集成电路
    • 编译者:Lightfeng
    • 发布时间:2017-01-03
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