Glossary term: X 射線天文學
Description: X 射線天文學是一個收集和分析來自宇宙的高能電磁輻射(能量高於紫外線輻射,但低於伽馬射線輻射)信息的研究領域。X 射線的頻率介於 30 拍赫茲和 30 艾赫茲之間,相當於 10 皮米和 10 納米之間的波長。在許多天文學領域(包括X射線天文學)仍然使用的舊單位制中,這對應於0.1到100埃(Å)。鑑於在該頻譜部分光的粒子性更顯著,X射線天文學家通常使用光子能量而非波長來表徵光子的特徵。用電子伏特(eV),即粒子物理學中常用的能量單位,上述頻率和波長範圍對應的光子能量在100 eV到100 keV之間。由於大氣層吸收了大部分X射線,因此X射線天文學通常通過空間望遠鏡進行。來自天文源的X射線來自於極其高溫的區域。這些區域包括黑洞或中子星等緊湊天體周圍的盤和恆星的高溫日冕。
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Term and definition status: The original definition of this term in English have been approved by a research astronomer and a teacher The translation of this term and its definition is still awaiting approval
This is an automated transliteration of the simplified Chinese translation of this term
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In Other Languages
- 阿拉伯語: علم الفلك بالأشعة السينية
- 德語: Röntgenastronomie
- 英語: X-ray Astronomy
- 法語: Astronomie des rayons X
- 印地語: एक्स-रे खगोल विज्ञान
- 義大利語: Astronomia a raggi X
- 日語: X線天文学 (external link)
- 簡體中文: X 射线天文学
Related Media
Remnant of SN 1006
Caption: This image shows the remnant of the supernova SN 1006. This was probably the result of a white dwarf that accreted so much material from a binary companion star that the white dwarf exploded (this is called a Type 1a supernova by astronomers). This explosion happened several thousand years ago, however it took time for the light from this event to reach Earth, only arriving in the year 1006. This bright explosion was noticed by observers across the Earth and its appearance was noted in the records of many different societies.
Here we see the effect that supernova has had on its surroundings in the galaxy. The force of the explosion has blown a huge bubble in the surrounding interstellar gas with a hot shockwave at its edge. The image appears to be a simple color picture but it actually represents light far beyond what our eye can see. The blue is X-ray data from NASA's Chandra X-ray Observatory, the yellow and orange are data from optical telescopes and the red is detections in radio waves from the Very Large Array and the Green Bank Telescope. The bright blue of the outer shell shows the gas there is very hot and that the explosion produced energetic shock waves.
Credit: X-ray: NASA/CXC/Rutgers/G.Cassam-Chenai, Hughes et al.; Radio: NRAO/AUI/NSF/GBT/VLA/Dyer, Maddalena & Cornwell; Optical: Middlebury College/F.Winkler, NOAO/AURA/NSF/CTIO Schmidt & DSS
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