Far-infrared astronomy
Far-infrared astronomy is the branch of astronomy and astrophysics that deals with objects visible in far-infrared radiation (extending from 30 µm towards submillimeter wavelengths around 450 µm). In the far-infrared, stars are not especially bright, but we can see emission from very cold matter (140 Kelvins or less) that is not seen at shorter wavelengths.
Far-infrared astronomy
Far-infrared astronomy is the branch of astronomy and astrophysics that deals with objects visible in far-infrared radiation (extending from 30 µm towards submillimeter wavelengths around 450 µm). In the far-infrared, stars are not especially bright, but we can see emission from very cold matter (140 Kelvins or less) that is not seen at shorter wavelengths.
has abstract
Far-infrared astronomy is the ...... between comets and asteroids."
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遠紅外線天文學是天文學和天文物理的分支，主要的觀測對象是以遠 ...... TRO-F和赫歇爾太空天文台，還有同溫層紅外線天文台望遠鏡。
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736,527,325
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Far-infrared astronomy is the ...... t seen at shorter wavelengths.
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遠紅外線天文學是天文學和天文物理的分支，主要的觀測對象是以遠 ...... 熱了星際塵雲，使這些星系在遠紅外線下遠比一般的星系更為明亮。
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label
Far-infrared astronomy
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遠紅外線天文學
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