《NASA邀请艺术家参观访问詹姆斯·韦伯空间望远镜》

  • 来源专题:天文仪器与技术信息
  • 编译者: zwg@niaot.ac.cn
  • 发布时间:2016-10-21
  • 见证历史:巨型的詹姆斯·韦伯空间望远镜的十八块镀金子镜已装配完成。

    Witness History: Be inspired by giant, golden, fully-assembled James Webb Space Telescope mirror on display at NASA Goddard.

    Are you an artist? If so, we have a unique opportunity to view the amazing and aesthetic scientific marvel that is the James Webb Space Telescope.

    Webb has a mirror that is nearly 22 feet high and (to optimize it for infrared observations) is covered in a microscopic layer of actual gold.

    Because of Webb’s visually striking appearance, we are hosting a special viewing event on Wednesday, Nov. 2, 2016, at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. Artists are invited to apply to attend.

    Participants will have the opportunity to:

    1:Hear an introduction to the telescope and what it will help us to learn about the universe

    Talk with experts about the engineering challenges with building such a cutting-edge mission:

    2:Get a behind-the-scenes tour of the center’s satellite integration and testing facilities.

    3:See the James Webb Space Telescope in person, and be given block of time to actively create.

    4:Share what they see and hear and create on their own social media platforms.

    5:The goal of this Artist Event is to allow artist attendees to set up their supplies for their artistic medium of choice right in front of the telescope itself, and be given time to create. This can include things like sketching, drawing, painting, photography, and digital art.

    Artists who work in non-visual artistic media are also invited to apply. While creative works do not have to be finished in the time allotted, we intend to display the finished products at minimum in an online gallery. We are investigating the possibility of a live event to showcase the works created as well.

    The applications for the James Webb Space Telescope Artist Event opens on this page on Oct. 20, and the deadline to apply is noon EDT on Oct. 25. All applications will be considered on a case-by-case basis.

  • 原文来源:http://www.nasa.gov/feature/goddard/2016/nasa-invites-artists-to-visit-james-webb-space-telescope
相关报告
  • 《NASA完成詹姆斯·韦伯空间望远镜主镜曲率中心测试》

    • 来源专题:天文仪器与技术信息
    • 编译者:zwg@niaot.ac.cn
    • 发布时间:2016-11-03
    • Engineers and technicians working on the James Webb Space Telescope successfully completed the first important optical measurement of Webb’s fully assembled primary mirror, called a Center of Curvature test. Taking a “before” optical measurement of the telescope’s deployed mirror is crucial before the telescope goes into several stages of rigorous mechanical testing. These tests will simulate the violent sound and vibration environments the telescope will experience inside its rocket on its way out into space. This environment is one of the most stressful structurally and could alter the shape and alignment of Webb’s primary mirror, which could degrade or, in the worst case, ruin its performance. Webb has been designed and constructed to withstand its launch environment, but it must be tested to verify that it will indeed survive and not change in any unexpected way. Making the same optical measurements both before and after simulated launch environment testing and comparing the results is fundamental to Webb’s development, assuring that it will work in space. “This is the only test of the entire mirror where we can use the same equipment during a before and after test,” said Ritva Keski-Kuha, the test lead and NASA’s Deputy Telescope Manager for Webb at NASA's Goddard Space Flight Center in Greenbelt, Maryland. “This test will show if there are any changes or damages to the optical system.” In order to conduct the test, optical engineers set up an interferometer, the main device used to measure the shape of Webb’s mirror. Waves of visible light are less than a thousandth of a millimeter long, and optics like Webb’s need to be shaped and aligned even more accurately than this to work correctly. Making measurements of the mirror shape and position by lasers prevents physical contact and damage (scratches to the mirror). So scientists use wavelengths of light to make tiny measurements. By measuring light reflected off the optics using an interferometer, they are able to measure extremely small changes in shape or position. An interferometer gets its name from the process of recording and measuring the ripple patterns that result when different beams of light mix and their waves combine or ‘interfere.’ During the test conducted by a team from NASA Goddard, Ball Aerospace of Boulder, Colorado, and the Space Telescope Science Institute in Baltimore Maryland, temperature and humidity conditions in the cleanroom were kept incredibly stable to minimize drift in the sensitive optical measurements over time. Even so, tiny vibrations are ever-present in the cleanroom that cause jitter during measurements, so the interferometer is a ‘high-speed’ one, taking 5,000 ‘frames’ every second, which is a faster rate than the background vibrations themselves. This allows engineers to subtract out jitter and get good, clean results. The Center of Curvature test measures the shape of Webb’s main mirror by comparing light reflected off of it with light from a computer-generated hologram that represents what Webb’s mirror ideally should be. By interfering the beam of light from Webb with the beam from the hologram reference, the interferometer accurately compares the two by measuring the difference to incredible precision. “Interferometry using a computer-generated hologram is a classic modern optical test used to measure mirrors,” said Keski-Kuha. With the largest mirror of any space telescope, taking this measurement is a challenge. “We have spent the last four years preparing for this test,” said David Chaney, Webb’s primary mirror metrology lead at Goddard. “The challenges of this test include the large size of the primary mirror, the long radius of curvature, and the background noise. Our test is so sensitive we can measure the vibrations of the mirrors due to people talking in the room.” After the measurements come back from the interferometer the team will analyze the data to make sure the mirrors are aligned perfectly before the launch environment tests. The Center of Curvature test will be repeated after the launch environment testing and the results compared to confirm that Webb’s optics will work after their launch into space. The most powerful space telescope ever built, the Webb telescope will provide images of the first galaxies ever formed, and explore planets around distant stars. It is a joint project of NASA, the European Space Agency and the Canadian Space Agency.
  • 《詹姆斯·韦伯空间望远镜技术验证结构热测试》

    • 来源专题:天文仪器与技术信息
    • 编译者:zwg@niaot.ac.cn
    • 发布时间:2016-10-19
    • In this photograph taken on Sept. 1, 2016, the James Webb Space Telescope Pathfinder structure has been configured for the Thermal Pathfinder Test at NASA Johnson Space Center's giant thermal vacuum chamber, called Chamber A. The Pathfinder is a test version of the structure that supports the telescope. This is where end-to-end testing of the actual telescope will occur in 2017. The dummy Aft Optical System (AOS) is visible in the center of the primary mirror segments. The AOS is the upright piece at the center of the primary mirror - it contains the telescope's tertiary and fine steering mirrors. Among the mirror segments can be seen are one gold-coated flight-spare beryllium segment (just in front of the AOS), one uncoated beryllium engineering unit segment, and ten gold-coated aluminum thermal simulator segments. The James Webb Space Telescope is the scientific successor to NASA's Hubble Space Telescope. It will be the most powerful space telescope ever built. Webb is an international project led by NASA with its partners, the European Space Agency and the Canadian Space Agency.