- 更多网络例句与天体望远镜相关的网络例句 [注：此内容来源于网络，仅供参考]
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One of the main works of astrometry is to observe celestial bodies, reduceobservational data and obtain the information of objects.
天体测量学的主要工作之一是利用天文望远镜观测天体，并对所得资料进行分析处理，获取目标天体的有用信息。
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One of the main works of astrometry is to observe celestial bodies, reduce observational data and obtain the information of objects.
天体测量学的主要工作之一是利用天文望远镜观测天体，并对所得资料进行分析处理，获取目标天体的有用信息。
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They mounted an astronomical telescope on the roof.
他们把天体望远镜装在屋顶上。
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Also have Sirius B, centering at around Sirius A, but due to small size, can not be seen by the naked eye until 1862, American astronomer Alvin Clark with the largest at that time, the latest celestial telescope, they discovered its existence.
另外还有天狼星 B ，围绕在天狼星 A 的周围，但因体积小，无法以肉眼看到，一直到 1862 年，美国天文学家艾尔文·克拉克用当时最大、最新的天体望远镜，才发现了它的存在。
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As a coelostat, MA tracks the motion of celestial objects observed at their meridian passages.
MA 作为定天镜跟踪天体的运动，望远镜在天体中天前后进行观测。
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Astrometry with new technologies created and is dedicated to the Space Telescope astrometric space orbit around the Earth observation and research on the scientific .1989 8 8, the European Space Agency launch astrometric Satellite Iba Valley satellite, which contains a 29 cm diameter reflecting telescope, four ground stations for data reception and analysis with the aim of space-based observations compiled by 120,000 to contain space for satellite measurement of star form, the location accuracy of ± 0002, parallax measurement accuracy ± 0002, on their own a year 0002, CDCDCD preliminary estimate of the above three data are now actual for the 0004,0003 and 0005; CDCDCD190 year in April the U.S. launch of the Hubble Space Telescope, containing 24 m diameter Wang C far mirror can work 15-20 years, 17-18 so you can measure the parallax of stars, are hundreds of thousands of stars of the measurement results.
伴随天体测量新技术而产生，是专门用于天体测量的空间望远镜在围绕地球的空间轨道上进行观测研究的科学。1989年8月8日，欧洲空间局发射天体测量卫星伊巴谷号卫星，它载有口径29厘米反射望远镜，4个地面观测站进行资料接收与分析，目的是要通过空间观测编出含星12万颗的空间测量星表，位置精度为±0002，测量视差的精度为±0002，自行为每年0002，CDCDCD现在初步估计上述三个数据实际为0004、0003和0005；CDCDCD190年4月美国发射哈勃空间望远镜，载有口径24米的望C远镜，可工作15—20年，可以测量出17—18等星的视差，得到几十万颗星的测量结果。
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Other authors include Daniel Apai of the Space Telescope Science Institute, Baltimore, Md.; Kevin Luhman of Pennsylvania State University, University Park; Thomas Henning and Jeroen Bouwman of the Max Planck Institute for Astronomy, Germany; Michael Meyer of the University of Arizona, Tucson; Fred Lahuis of the SRON Netherlands Institute for Space Research, the Netherlands; and Antonella Natta of the Arcetri Astrophysical Observatory, Italy.
其他论文作者：马里兰州巴尔的摩市太空望远镜科学研究所的丹尼尔·Apai；宾西法尼亚州立大学的凯文·Luhman；德国马克士普朗克天体物理研究所托马斯·亨宁和Jeroen·Bouwman；图森市亚利桑那大学的迈克尔·梅耶尔；荷兰尼德兰空间研究协会的弗雷德·拉豪斯；意大利佛罗伦斯市雅赛墔天体物理观测站的Antonella·纳塔等。
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Other authors include Daniel Apai of the Space Telescope ScienceInstitute, Baltimore, Md.; Kevin Luhman of Pennsylvania StateUniversity, University Park; Thomas Henning and Jeroen Bouwman of theMax Planck Institute for Astronomy, Germany; Michael Meyer of theUniversity of Arizona, Tucson; Fred Lahuis of the SRON NetherlandsInstitute for Space Research, the Netherlands; and Antonella Natta ofthe Arcetri Astrophysical Observatory, Italy.
其他论文作者：马里兰州巴尔的摩市太空望远镜科学研究所的丹尼尔·Apai；宾西法尼亚州立大学的凯文·Luhman；德国马克士普朗克天体物理研究所托马斯·亨宁和Jeroen·Bouwman；图森市亚利桑那大学的迈克尔·梅耶尔；荷兰尼德兰空间研究协会的弗雷德·拉豪斯；意大利佛罗伦斯市雅赛墔天体物理观测站的Antonella·纳塔等。
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The controller calculates the position of heavenly bodies based on time, date, and location, and the telescope swivels to lock on for you.
控制器会根据时间、日期及方位计算出天体的位置，然后望远镜自动旋转，跟踪锁定天体。
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Accordingly, as the major targets weighing the quality of the telescope,its luminous energy concentration degree directly influence the quality of the image of the celestial body. So many kinds of technique about the optical quality testing of telescope have came forth. Hartmann screen test is one of the most classical among them and it has become one of the main testing method on several large-scale telescopes in the world because of some strongpoints suchas briefness, visuality and easy handlment.The image through the350mm telescope of the Yunnan observatory has aberration in general, subsequently,the relative position of the primary mirrior has err when blooming and reinstalling .
因此，天文望远镜光能集中度作为衡量天文望远镜质量的重要指标，直接影响到所成天体像的质量好坏，所以就出现了多种天文望远镜光学质量检测方法，其中最经典的是哈特曼光栏法，它因简单、直观、操作方便等优点而成为世界上多台大型天文望远镜的重要质量检测方法之一。
- 更多网络解释与天体望远镜相关的网络解释 [注：此内容来源于网络，仅供参考]
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astrometry：天体测量
当然是理科 现在天文的研究方法,一部分是观测,就是用各种望远镜观测,包括光学的和射电望远镜,除了需要对星图熟悉之外,还...天文学属于一级学科,一般下分三个二级学科: 天体物理(astrophysics),天体力学(Celestial Mechanics)和天体测量(astrometry),...
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astronautics：宇宙航行学
astern turbine 倒车轮机 | astronautics 宇宙航行学 | astronomical telescope 天体望远镜
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astronomical telescope：天体望远镜
astronautics 宇宙航行学 | astronomical telescope 天体望远镜 | asymmetry 不对称
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astronomical telescope：天体望远镜, 天文望远镜
astronomical telegram 天文电报 | astronomical telescope 天体望远镜, 天文望远镜 | astronomical test 天文检验
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astronomical optics telescope：天文光学望远镜
astronomical ECD spectrometer 电子耦合器件天文光谱仪 | astronomical optics telescope 天文光学望远镜 | astronomical spectrograph 天体摄谱仪
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celestial telescope：天体望远镜
cavity resonator 空腔共振器 | celestial telescope 天体望远镜 | cell 电池,细胞
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radio telescope：射电望远镜
射电望远镜(radio telescope)是指观测和研究来自天体的射电波的基本设备,可以测量天体射电的强度、频谱及偏振等量. 包括收集射电波的定向天线,放大射电信号的高灵敏度接收机,信息记录、处理和显示系统等.
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star cluster：星团
在"前望远镜时代"(pre-telescopic times)它被用于将天空点状的星体和不像星星的天体区分开. 在那时许多被称作"nebulae(星云)"的天体都被现代科学证明为星团(star cluster). 因此当时的术语"Nebula"所指是我们现在所说的"深空天体"(Deepsky Object).
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Radio telescopes：射电望远镜
这一范围从10兆赫延伸至100千兆赫,这使得地球表面能用射电望远镜(radio telescopes)拾取这一范围内天体射频源辐射的电磁波. 100兆赫以下的无线电波被电离层反射;100千兆赫以上时,则随着频率增高,受分子吸收的影响越大. 热力发动机的工作周期.
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astronomic radio source：天体射电源
astronomic longitude 天文经度;黄经 | astronomic radio source 天体射电源 | astronomic telescope 天文望远镜