《欧洲39米望远镜主镜第一块子镜坯制作完成》

  • 来源专题:天文仪器与技术信息
  • 编译者: zwg@niaot.ac.cn
  • 发布时间:2018-01-11
  • The first six hexagonal segments for the main mirror of ESO’s Extremely Large Telescope (ELT) have been successfully cast by the German company SCHOTT at their facility in Mainz. These segments will form parts of the ELT’s 39-metre main mirror, which will have 798 segments in total when completed. The ELT will be the largest optical telescope in the world when it sees first light in 2024.

    The 39-metre-diameter primary mirror of ESO’s Extremely Large Telescope will be by far the largest ever made for an optical-infrared telescope. Such a giant is much too large to be made from a single piece of glass, so it will consist of 798 individual hexagonal segments, each measuring 1.4 metres across and about 5 centimetres thick. The segments will work together as a single huge mirror to collect tens of millions of times as much light as the human eye.

    Marc Cayrel, head of ELT optomechanics at ESO, was present at the first castings: “It was a wonderful feeling to see the first segments being successfully cast. This is a major milestone for the ELT!”

    As with the telescope’s secondary mirror blank, the ELT main mirror segments are made from the low-expansion ceramic material Zerodur© [1] from SCHOTT. ESO has awarded this German company with contracts to manufacture the blanks of the first four ELT mirrors (known as M1 to M4, with M1 being the primary mirror) (eso1704).

    The first segment castings are important as they allow the engineers at SCHOTT to validate and optimise the manufacturing process and the associated tools and procedures.

    The casting of the first six segments is a major milestone, but the road ahead is long — in total more than 900 segments will need to be cast and polished (798 for the main mirror itself, plus a spare set of 133). When fully up to speed, the production rate will be about one segment per day.

    After casting, the mirror segment blanks will go through a slow cooling and heat treatment sequence and will then be ground to the right shape and polished to a precision of 15 nanometres across the entire optical surface. The shaping and polishing will be performed by the French company Safran Reosc, which will also be responsible for additional testing (eso1717).

    Notes

    [1] Zerodur© was originally developed for astronomical telescopes in the late 1960s. It has an extremely low coefficient of thermal expansion, meaning that even in the case of large temperature fluctuations, the material does not expand. Chemically, Zerodur© is very resistant and can be polished to a high standard of finish. The actual reflective layer, made of aluminium or silver, is usually vaporised onto the extremely smooth surface shortly before a telescope is put into operation and at regular intervals afterwards. Many well-known telescopes with Zerodur© mirrors have been operating reliably for decades, including ESO's Very Large Telescope in Chile.

    More information

    ESO is the foremost intergovernmental astronomy organisation in Europe and the world’s most productive ground-based astronomical observatory by far. It is supported by 16 countries: Austria, Belgium, Brazil, the Czech Republic, Denmark, France, Finland, Germany, Italy, the Netherlands, Poland, Portugal, Spain, Sweden, Switzerland and the United Kingdom, along with the host state of Chile and by Australia as a strategic partner. ESO carries out an ambitious programme focused on the design, construction and operation of powerful ground-based observing facilities enabling astronomers to make important scientific discoveries. ESO also plays a leading role in promoting and organising cooperation in astronomical research. ESO operates three unique world-class observing sites in Chile: La Silla, Paranal and Chajnantor. At Paranal, ESO operates the Very Large Telescope and its world-leading Very Large Telescope Interferometer as well as two survey telescopes, VISTA working in the infrared and the visible-light VLT Survey Telescope. ESO is also a major partner in two facilities on Chajnantor, APEX and ALMA, the largest astronomical project in existence. And on Cerro Armazones, close to Paranal, ESO is building the 39-metre Extremely Large Telescope, the ELT, which will become “the world’s biggest eye on the sky”.

  • 原文来源:http://www.eso.org/public/news/eso1801/
相关报告
  • 《欧洲39米望远镜第一批18块主镜子镜镜坯运到法国》

    • 来源专题:天文仪器与技术信息
    • 编译者:zwg@niaot.ac.cn
    • 发布时间:2019-08-07
    • The first set of 18 blanks for the primary mirror of ESO’s Extremely Large Telescope have arrived safely at Safran Reosc in Poitiers, France. The contracts for casting the blanks of the mirror segments, as well as polishing, mounting and testing them, were signed in 2017 with respectively the German company SCHOTT and the French company Safran Reosc, a subsidiary of Safran Electronics & Defense. Mirror blanks are packed by six into a special wooden transport crate and six of these crates can fit inside a regular shipping container. Sophisticated shock sensors travel with the blanks to measure any sudden acceleration or shock that could affect the blanks. The shipping container with the first 18 blanks was sent from SCHOTT in Mainz, Germany, on 23 July and arrived at Safran Reosc the following day. The ELT mirror blanks are made of the low-expansion glass-ceramic Zerodur© [1] and are circular, measuring 1.5 metres across and about 5 centimetres thick. The back of each blank is flat and the front surface is concave. The blanks come in three types with slightly differently shaped front surfaces, depending on the planned location of the segment in the primary mirror. The first primary mirror segments were cast by SCHOTT in 2018. SCHOTT manufactures the blanks to approximate shape so that Safran Reosc does not need to remove too much material during the polishing process. Safran Reosc will polish the blanks before they are cut into hexagons and receive a final precise polishing using Ion Beam Figuring. When it is completed, the primary mirror will comprise 798 hexagonal segments and will have a total light-collecting area of 978 m2. In total, more than 900 segments will need to be cast and polished (including a spare set of 133 segments). Once built the ELT will be the largest ground-based telescope in operation. The telescope is being built at Cerro Armazones in the Atacama Desert of northern Chile. With a primary mirror almost 40 metres in diameter, the ELT will gather almost 100 million times more light than the human eye, which will allow scientists to tackle some of the biggest challenges in current astrophysics, such as the formation of the first stars, the assembly of the first galaxies, the characterisation of the atmospheres of Earth-like exoplanets, or the nature of dark matter and dark energy, among many other questions. Notes [1] Zerodur© was originally developed for astronomical telescopes in the late 1960s. It has an extremely low coefficient of thermal expansion, meaning that even in the case of large temperature fluctuations, the material does not expand. Chemically, Zerodur© is very resistant and can be polished to a high standard of finish. The actual reflective layer, made of aluminium or silver, is usually vaporised onto the extremely smooth surface shortly before a telescope is put into operation and is renewed at regular intervals afterwards. Many well-known telescopes with Zerodur© mirrors have been operating reliably for decades, including ESO's Very Large Telescope in Chile.
  • 《欧洲39米望远镜自适应变形镜的第一块壳完成(共6块)》

    • 来源专题:天文仪器与技术信息
    • 编译者:zwg@niaot.ac.cn
    • 发布时间:2018-03-25
    • The French optics company Safran Reosc has completed the first of six shells that will comprise the M4 deformable mirror system, which forms a fundamental part of ESO’s Extremely Large Telescope (ELT). When complete, the adaptive M4 mirror will be 2.4 metres in diameter but only 1.95 millimetres thick. This very thin mirror is one of the five main mirrors of the ELT’s optical system, with the main segmented mirror being 39 metres in diameter. Safran Reosc are manufacturing all six of the deformable shell mirrors that comprise the M4 mirror. Together, these 60-degree petal sections form the circular segmented M4 mirror. They will be mounted and supported in the adaptive mirror unit. Meanwhile, the Italian consortium AdOptica is manufacturing the complex adaptive support system needed for the M4. Deformable mirrors, such as the M4 mirror of the ELT, are key components of adaptive optics systems, which help reduce the effects of atmospheric distortions. Adaptive optics systems work by measuring atmospheric turbulence — often with the help of laser guide stars — and compensating for this turbulence by adjusting the shape of a deformable mirror. The actuators and controls in the adaptive support system will allow the ELT to make these corrections in real time. The system will also be able to correct for effects caused by the wind, which can sometimes deform the structure of the main telescope. The combination of the M4 mirror shells and their adaptive support systems will form part of the largest adaptive mirror unit ever made and means that images obtained by the ELT will be almost as sharp as those taken in space.