《美国25米望远镜GMT2028年安装镜面》

  • 来源专题:天文仪器与技术信息
  • 编译者: zwg@niaot.ac.cn
  • 发布时间:2019-11-06
  • GMTO Corp., the organization managing the development of the Giant Magellan Telescope on behalf of its U.S. and international founders, has signed a contract with MT Mechatronics and Ingersoll Machine Tools, to design, build and install the telescope’s precision steel structure.

    The GMTO telescope’s primary mirror is specified to combine seven 8.4m-diameter circular segments to form an effective aperture 24.5m in diameter. To be located at Las Campanas Observatory in Chile’s Atacama Desert, the planned optical-infrared observatory is designed to explore the frontiers of astronomy, including seeking to answer one of humanity’s most pressing questions: “Are we alone?”

    MT Mechatronics and Ingersoll Machine Tools, part of the Italian Camozzi Group, will design and manufacture the 1,800-ton precision mechanism, known as the telescope structure, which will hold the GMT’s optics and smoothly track celestial targets. The structure will be designed by MT Mechatronics and manufactured by Ingersoll before being installed at the observatory site in the Chilean Andes.

    Mirrors installed in 2028

    The total value of the telescope structure contract is $135 million. The agreement between GMTO, MT Mechatronics and Ingersoll Machine Tools will involve nine years of work and 1,300 tons of structural steel, and the structure is expected to be delivered to Chile at the end of 2025 and be ready to accept mirrors in 2028.

    “Manufacturing the telescope structure is one of the biggest steps we will take on our journey to building the Giant Magellan Telescope,” said Dr. Shelton, GMTO President.

    “We selected MT Mechatronics and Ingersoll Machine Tools for their commitment to quality, extensive experience with astronomical telescopes and abilities to manufacture complex precision structures, following a two-year global competition,” added Dr. James Fanson, GMTO Project Manager.

    The telescope structure will hold the GMT’s seven giant mirrors in place as they bring light from distant stars and galaxies to a focus so it can be analyzed by scientific instruments mounted deep inside the telescope. The mirrors, the largest in the world, are to be made at the University of Arizona’s Richard F. Caris Mirror Lab.

    When in operation, the telescope structure, complete with mirrors and instruments, will weigh 2,100 tons but will float on a film of oil just 50µm thick – allowing it to move essentially without friction as it compensates for Earth’s rotation, tracking celestial bodies in their arc across the sky. The GMT will produce images that are 10 times sharper than those from the Hubble Space Telescope in the infrared region of the spectrum.

    “Being a part of an endeavor with objectives as distinguished as the Giant Magellan Telescope’s is compelling for MT Mechatronics and we’re eager to support the GMT on its quest to answer the deepest questions in astronomy,” said Thomas Zimmerer, Senior VP, Business Development Sales & Marketing, Product Development, MT Mechatronics.

    “We are happy to work with GMTO and MTM to create this unique tool for the study of new worlds. The project honors and motivates all of us at Ingersoll,” said Lodovico Camozzi, CEO of Camozzi Group. “It will be a special day when the GMT’s telescope structure is completed and placed in service in Chile,” said Chip Storie, CEO of Ingersoll Machine Tools.

    MT Mechatronics has over 50 years’ experience with telescopes, beginning with the Parkes Radio Telescope in Australia. It was part of a European consortium constructing the European Atacama Large Millimeter/submillimeter Array (ALMA) telescope antennas and was the mount designer for the Daniel K. Inouye Solar Telescope (DKIST) in Hawaii.

    Since its inception in 1891, Ingersoll Machine Tools Inc. has been an iconic name in the milling machines sector, successfully serving the defense sector and then the newborn aeronautics and aerospace industry. Ingersoll has many decades of experience with manufacturing precision steel structures, including recently partnering with MT Mechatronics on the construction of the DKIST telescope mount.

    The mount contract completes another significant milestone for GMTO in 2019. In March, the excavations for the foundations of the telescope’s pier and enclosure were finished, and in July the second of GMT’s seven primary mirror segments was completed and shipped to temporary storage. Casting of the sixth primary mirror segment at the University of Arizona is expected to begin in mid-2020.

  • 原文来源:https://optics.org/news/10/10/51
相关报告
  • 《美国25米光学望远镜~2016年11月通讯》

    • 来源专题:天文仪器与技术信息
    • 编译者:zwg@niaot.ac.cn
    • 发布时间:2016-11-18
    • Contents 1:Telescope Mount Industry Briefing 2:Site Update 3:Board Member Profile: Dr. James Wyant 4:GMT Community Science Meeting 5:Community Outreach in Chile
  • 《美国25米望远镜(GMT)开始磨制第5块子镜》

    • 来源专题:天文仪器与技术信息
    • 编译者:zwg@niaot.ac.cn
    • 发布时间:2017-11-08
    • The Giant Magellan Telescope Organization (GMTO) today announced that it has initiated the casting of the fifth of seven mirrors that will form the heart of the Giant Magellan Telescope (GMT). The mirror is being cast at the University of Arizona’s Richard F. Caris Mirror Laboratory, the facility known for creating the world’s largest mirrors for astronomy. The 25-meter diameter GMT will be sited in the Chilean Andes and will be used to study planets around other stars and to look back to the time when the first galaxies formed. The process of “casting” the giant mirror involves melting nearly 20 tons of glass in a spinning furnace. Once cooled, the glass disk will be polished to its final shape using state-of-the-art technology developed by the University of Arizona. The GMT will combine the light from seven of these 8.4 meter mirrors to create a telescope with an effective aperture 24.5 meters in diameter (80 feet). With its unique design, the GMT will produce images that are 10 times sharper than those from the Hubble Space telescope in the infrared region of the spectrum. “We are thrilled to be casting the Giant Magellan Telescope’s fifth mirror,” said Dr. Robert N. Shelton, President of GMTO. “The Giant Magellan Telescope project will enable breakthrough discoveries in astronomy, and perhaps entirely new fields of study. With the talents of the team at the University of Arizona and across our entire community, we are taking the next step towards completing the seven-mirror GMT.” Each of GMT’s light-weighted mirrors is a marvel of engineering. The mirrors begin as pristine blocks of custom manufactured low-expansion E6 glass from the Ohara Corporation of Japan. Precisely 17,481 kg of these glass blocks have been placed by hand into a custom-built furnace pre-loaded with a hexagonal mold. At the peak of the lengthy casting process, in which the giant furnace spins at up to five revolutions per minute, the glass is heated to 1165°C (2129°F) for about four hours until it liquefies and flows into the mold. The casting process continues as the glass is carefully cooled for three months while the furnace spins at a slower rate. The glass then undergoes an extended period of shaping and polishing. The result of this high-precision process is a mirror that is polished to an accuracy of one twentieth of a wavelength of light, or less than one thousandth of the width of a human hair. “Casting the mirrors for the Giant Magellan Telescope is a huge undertaking, and we are very proud of the UA’s leading role creating this new resource for scientific discovery. The GMT partnership and Caris Mirror Lab are outstanding examples of how we can tackle complex challenges with innovative solutions,” said UA President Robert C. Robbins. “The University of Arizona has such an amazing tradition of excellence in space exploration, and I have been constantly impressed by the things our faculty, staff, and students in astronomy and space sciences can accomplish.” With its casting this weekend, the fifth GMT mirror joins three additional GMT mirrors at various stages of production in the Mirror Lab. Polishing of mirror 2’s front surface is well underway; coarse grinding will begin on the front of the third mirror shortly and mirror number 4, the central mirror, will soon be ready for coarse grinding following mirror 3. The first GMT mirror was completed several years ago and was moved to a storage location in Tucson this September, awaiting the next stage of its journey to Chile. The glass for mirror 6 has been delivered to Tucson and mirror seven’s glass is on order from the Ohara factory in Japan. In time, the giant mirrors will be transported to GMT’s future home in the Chilean Andes at the Carnegie Institution for Science’s Las Campanas Observatory. This site is known for being one of the best astronomical sites on the planet with its clear, dark skies and stable airflow producing exceptionally sharp images. GMTO has broken ground in Chile and has developed the infrastructure on the site needed to support construction activities. “Creating the largest telescope in history is a monumental endeavor, and the GMT will be among the largest privately-funded scientific initiatives to date,” said Taft Armandroff, Professor of Astronomy and Director of the McDonald Observatory at The University of Texas at Austin, and Vice-Chair of the GMTO Corporation Board of Directors. “With this next milestone, and with the leadership, technical, financial and scientific prowess of the members of the GMTO partnership, we continue on the path to the completion of this great observatory.”