《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.

  • 原文来源:http://www.nasa.gov/image-feature/testing-the-james-webb-space-telescope-pathfinder
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.
  • 《人工智能恢复詹姆斯·韦伯望远镜的清晰视觉》

    • 来源专题:人工智能
    • 编译者:高楠
    • 发布时间:2025-10-28
    • 两名来自悉尼的博士生在不离开地面的情况下,帮助恢复了世界上最强大的空间天文台的清晰视觉。现在是荷兰莱顿大学博士后研究员的路易斯·德斯多伊茨和他的同事麦克斯·查尔斯用他们修复的仪器的纹身来庆祝他们的成就——这是他们对空间科学贡献的永久纪念。 突破性的软件修复 悉尼大学的研究人员开发了一种创新的软件解决方案,可以纠正美国国家航空航天局耗资数十亿美元的詹姆斯·韦伯太空望远镜(JWST)拍摄的图像中的模糊现象。他们的突破恢复了望远镜关键仪器之一的完全精度,实现了曾经需要昂贵的宇航员维修任务。 这一成功建立在JWST唯一由澳大利亚设计的部件——孔径掩蔽干涉仪(AMI)的基础上。由悉尼大学物理学院和悉尼天文研究所的Peter Tuthill教授创建的AMI允许天文学家捕捉恒星和系外行星的超高分辨率图像。它的工作原理是将来自望远镜主镜不同部分的光结合起来,这个过程被称为干涉测量法。当JWST号开始它的科学操作时,研究人员注意到AMI的性能受到其红外摄像探测器中微弱电子失真的影响。这些扭曲造成了微妙的图像模糊,让人想起哈勃太空望远镜著名的早期光学缺陷,必须通过宇航员太空行走来纠正。 从地球上解决一个太空问题 博士生路易斯·德斯多伊茨和麦克斯·查尔斯没有尝试物理修复,而是与图希尔教授和本·波普副教授(在麦考瑞大学)合作,设计了一种纯粹基于软件的校准技术来修复来自地球的失真。 他们的系统名为AMIGO(孔径掩模干涉测量生成观测),使用先进的模拟和神经网络来复制望远镜的光学和电子设备在太空中的功能。通过查明电荷轻微扩散到邻近像素的问题——这种现象被称为更亮更胖效应——该团队设计了数字校正图像的算法,完全恢复了AMI的性能。“他们没有派宇航员去安装新零件,而是设法用代码来修复东西,”塔希尔教授说。“这是澳大利亚创新如何在太空科学领域产生全球影响的一个出色例子。” 对宇宙更清晰的看法 结果是惊人的。随着AMIGO的投入使用,詹姆斯·韦伯太空望远镜已经提供了迄今为止最清晰的图像,以前所未有的细节捕捉到了微弱的天体。这包括一颗暗淡的系外行星和一颗红棕色矮星的直接图像,它们围绕附近的恒星HD 206893旋转,距离地球约133光年。 麦克斯·查尔斯领导的一项相关研究进一步证明了AMI的新精确度。使用改进的校准,望远镜产生了黑洞射流、木星卫星木卫一炽热表面和WR 137充满尘埃的星风的清晰图像——表明JWST现在可以比以前探测得更深更清晰。 “这项工作使JWST的视野更加清晰,”德斯多伊茨博士说。“看到一个软件解决方案扩展了望远镜的科学研究范围,并且知道不需要离开实验室就可以实现这一点,这是令人难以置信的回报。” 德斯多伊茨博士现在已经在荷兰莱顿大学获得了一个享有盛誉的博士后研究职位。 这两项研究都发表在印前服务器arXiv上。Desdoigts博士的论文已经通过了同行评审,不久将发表在澳大利亚天文学会出版物。我们已经发布了这个新闻稿,以配合最新一轮的詹姆斯韦伯太空望远镜一般观察员,调查和档案研究计划。 副教授Benjamin Pope在悉尼SXSW会议上介绍了这些发现,他说研究小组渴望尽快把新代码送到研究JWST的研究人员手中。