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The Haus der Astronomie building. This is a white, modernist building shaped like an simplified depiction of a spiral galaxy

Haus der Astronomie

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图注: Haus der Astronomie in early 2019
来源: HdA


文件 ( 图像 247.43 kB)


Infrared all-sky survey map with bright Milky Way band and scattered sources across the sky.

WISE Survey Capturing the Whole Sky in Infrared Light

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图注: This image presents the entire sky mapped in infrared light from space by the WISE satellite. While dust in the plane of the Milky Way blocks visible light, obscuring the heart of our Galaxy, infrared light passes through the dust. The most prominent feature is the broad, bright band running horizontally through the centre — this is the plane of our Milky Way galaxy. Numerous brighter knots and patches appear above and below the band, marking regions of active star formation and nearby galaxies. Such a dataset is a classic example of an astronomical survey, in which large portions of the sky is scanned to build a comprehensive catalogue of cosmic sources. The WISE satellite operated in space, allowing it to study parts of the infrared spectrum blocked by Earth's atmosphere.
来源: NASA/JPL-Caltech
来源链接

词汇表: 红外天文学 , 天文巡天

授权许可: 公共领域 公共领域 图标

文件 ( 图像 64.59 MB)


The SOFIA Telescope sits inside the body of a modified Boeing 747 aircraft and observes the universe.

SOFIA: Unveiling the Infrared Universe from the Skies

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图注: This image shows the Stratospheric Observatory for Infrared Astronomy (SOFIA) telescope. This telescope which operated from 2010 to 2022 was mounted in a modified Boeing 747 aircraft with a section of the rear fuselage removed to allow the telescope to observe the sky and with other modifications that allow it to fly at a higher altitude than a standard 747. Many molecules which are common in the Earth's atmosphere (such as water, carbon dioxide and methane) absorb radiation at infrared wavelengths. This interferes with infrared observations made from the ground. SOFIA flew at an altitude that puts it above most of the water vapour in the Earth's atmosphere, greatly reducing the impact of absorption by water molecules on its observations.
来源: NASA photo / Jim Ross
来源链接

词汇表: 红外天文学 , 红外望远镜

授权许可: 公共领域 公共领域 图标

文件 ( 图像 1.76 MB)


The space shuttle is shaped like a stubby airplane with a grayscale image on the left and blue-red colorscale on the right

Infrared Reentry Analysis: Shuttle Orbiter Columbia

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图注: A composite image of the Space Shuttle Columbia's reentry, captured by NASA's Kuiper Airborne Observatory. The right hand side of the image was taken in infrared light with the left hand side taken in visible light. The image reveals the intense heating patterns encountered during descent. The temperature scale for the infrared image goes from violet at the coolest end to red at the hottest. We can see here that the wing and tail of the space shuttle are glowing the brightest, indicating that they are the hottest.
来源: NASA with minor adjustments by wikicommons user Ke4roh
来源链接

词汇表: 红外线(IR)
分类: 观测天文学 , 太空探索

授权许可: 公共领域 公共领域 图标

文件 ( 图像 3.07 MB)


The left image has finger-shaped clouds with bright edges. In the right image we see stars shining through those clouds

The Pillars of Creation in comparison

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图注: The 'Pillars of Creation' are a renowned astronomical feature situated within the Eagle Nebula in the Serpens constellation. The illustration provides a direct comparison between images captured by the Hubble Space Telescope (HST) and the James Webb Space Telescope (JWST), showcasing the pillars, which span several light years in diameter, in both visible light (also known as optical light) and infrared light. On the left are the pillars as seen by Hubble in visual light, taken in 2014. It displays dark pillars against an opaque background, with only a handful of visible stars. Conversely, the counterpart on the right is Webb’s near-infrared view published in 2022, penetrating the dust and revealing numerous stars of varying sizes. Their distance from Earth is approximately 6,500 to 7,000 light years. Within these pillars, new stars are constantly forming, making them a subject of extensive study by astronomers. Composed mostly of cool molecular hydrogen and small amounts of interstellar dust, they are subject to erosion by the intense ultraviolet radiation emitted by nearby massive and newborn stars, a process known as photoevaporation.
来源: NASA, ESA, CSA, STScI
来源链接

词汇表: 红外天文学 , 红外望远镜 , 光学天文学 , 恒星形成 , 可见光谱 , 尘埃云
分类: 银河系与星际介质 , 恒星

授权许可: 知识共享许可协议 Attribution 2.0 Generic 知识共享许可协议 Attribution 2.0 Generic 图标

文件 ( 图像 12.03 MB)


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