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Glossary term: 超新星遺跡

Description: 超新星遺跡是超新星爆炸後殘留的結構。它由超新星沖擊產生的熾熱氣體和等離子體組成。在許多超新星遺跡中,恆星超新星爆炸所產生的黑洞或中子星也存在,不過在某些超新星遺跡中,黑洞或中子星已被爆炸的力量拋出。

超新星的爆炸能量會產生沖擊波,沖擊周圍的星際氣體。這種沖擊波將周圍的氣體加熱並電離到極高的溫度(超過一百萬開爾文)。這種高溫氣體會發出各種波長的光,包括 X 射線的重要來源。沖擊還能將粒子加速到很高的速度,使超新星殘骸成為宇宙射線的重要來源。

通過觀察超新星殘骸的膨脹速度,天文學家可以估算出它需要多長時間才能達到目前的大小。這樣,天文學家就能確定超新星爆炸的大致時間。銀河系中的幾顆大型超新星遺跡都是通過這種方法測定的時間,並與天文學家數百年前觀測到的超新星聯繫在一起。

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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

The OAE Multilingual Glossary is a project of the IAU Office of Astronomy for Education (OAE) in collaboration with the IAU Office of Astronomy Outreach (OAO). The terms and definitions were chosen, written and reviewed by a collective effort from the OAE, the OAE Centers and Nodes, the OAE National Astronomy Education Coordinators (NAECs) and other volunteers. You can find a full list of credits here. All glossary terms and their definitions are released under a Creative Commons CC BY-4.0 license and should be credited to "IAU OAE".

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Related Diagrams


金牛座呈現為開口指向東北的Y字形。黃道從西南偏西(WSW)方向延伸至東北偏東(ENE)方向,貫穿了金牛座的北半部。

金牛座星圖

Caption: 金牛座及其明亮恆星與周邊星座示意圖。從頂部開始沿順時針方向,金牛座周邊的星座依次為:英仙座、白羊座、鯨魚座、波江座、獵戶座、雙子座和御夫座。金牛座最亮的恆星是畢宿五,位於整個星座的中央。金牛座位於黃道上。從地球看來,太陽以一年為週期在天球上移動,所經過的路徑稱為黃道,在圖中以藍色實線標注。太陽在每年五月中旬到六月下旬位於金牛座。太陽系中的其他行星也經常出現在金牛座。 金牛座大部分位於天赤道以北,小部分位於天赤道以南。在地球上,除了南極地區和北極點周圍的一小部分地區以外,一年中的某些時候都能看到整個金牛座。金牛座在北半球的冬季和南半球的夏季夜晚最適宜觀測。 在金牛座的東部,可以看到超新星遺跡M1,通常稱為蟹狀星雲,在圖中以綠色方塊標注。在金牛座的東北部,可以看到全天最著名的疏散星團之一M45,即昴星團,在圖中以黃色圓圈標注。畢宿五附近(但不包括畢宿五本身)的許多恆星都是另一個星團——畢星團的成員。不過畢星團離太陽系比較近,因此在天球上顯得過於分散,不像昴星團那樣擁有梅西葉天體編號。 該圖的縱軸為赤緯,橫軸為赤經,方向為上北下南左東右西。圖中標注的恆星大小對應其視星等——衡量天體視亮度的標準,較大的圓點代表著較亮的恆星。圖中的希臘字母標注著星座中最亮的恆星。這些恆星按亮度排序,最亮的一般被標記為α星,第二亮的一般為β星,等等,不過這種字母排序並不總是和實際亮度排序完全一致。圖中虛線標注的是國際天文學聯合會劃定的星座邊界,綠色實線則是一種常見的星座形象連線。需要注意的是,在實際觀測時,這些邊界與連線都不會出現在天空中。
Credit: 國際天文學聯合會天文教育辦公室(IAU OAE)根據國際天文學聯合會和《天空與望遠鏡》的原文改編

License: CC-BY-4.0 Creative Commons 姓名標示 4.0 國際 (CC BY 4.0) icons


Cygnus looks like a swan in flight with the neck pointing to the lower right (south-west). Deneb is the tail

Cygnus Constellation Map

Caption: The constellation Cygnus with its bright stars and surrounding constellations. Cygnus is surrounded by (going clockwise from the top): Cepheus, Draco, Lyra, Vulpecula, Pegasus and Lacerta. Cygnus is notable for its brightest star Deneb. This forms one vertex of the prominent Summer Triangle asterism that is visible in northern hemisphere summer evenings. Cygnus is a northern constellation and thus the whole of the constellation is visible at some point in the year in the whole northern hemisphere. The whole constellation is also visible from equatorial regions of the southern hemisphere with parts of the constellation visible from temperate southern regions. The plane of the Milky Way runs through Cygnus and thus the constellation is rich in nebulae and star clusters. These include the North America Nebula (NGC 7000) and the Crescent Nebula (NGC 6888). The Veil Nebula is a huge supernova remnant, parts of which are marked here as NGC 6960 and NGC 6992/5. All of the previously-mentioned nebulae are marked with green squares. The planetary nebula NGC 6826 is marked here with a green circle superimposed on a plus sign. The open star clusters M29 and M39 are marked here with yellow circles. The y-axis of this diagram is in degrees of declination with north as up and the x-axis is in hours of right ascension with east to the left. The sizes of the stars marked here relate to the star's apparent magnitude, a measure of its apparent brightness. The larger dots represent brighter stars. The Greek letters mark the brightest stars in the constellation. These are ranked by brightness with the brightest star being labeled alpha, the second brightest beta, etc., although this ordering is not always followed exactly. The dotted boundary lines mark the IAU's boundaries of the constellations and the solid green lines mark one of the common forms used to represent the figures of the constellations. Neither the constellation boundaries, nor the lines joining the stars appear on the sky.
Credit: Adapted by the IAU Office of Astronomy for Education from the original by the IAU and Sky & Telescope

License: CC-BY-4.0 Creative Commons 姓名標示 4.0 國際 (CC BY 4.0) icons