超新星 的英文怎麼說

中文拼音 [chāoxīnxīng]
超新星 英文
supernova; supernova star超新星爆發 supernova outburst; 超新星爆發（殘余）[遺跡] remnant of supernova explosion; supernova remnant; relic of supernova; 超新星源 supernova source
  • 超 : Ⅰ動詞1 （越過; 高出） exceed; surpass; overtake 2 （在某個范圍以外; 不受限制） transcend; go beyo...
  • 新 : Ⅰ形容詞1 （剛出現的或剛經驗到的） new; fresh; novel; up to date 2 （沒有用過的） unused; new 3 （...
  • 星 : 名詞1 （夜晚天空中閃爍發光的天體） star 2 [天文學] （宇宙間能發射光或反射光的天體） heavenly body...
  1. A supernova is observed by the chinese and amerindians near the star tauri

    1054年的今天，一顆位於金牛座附近的超新星被中國及印第安人發現並記載。
  2. The astrocalendar incorporates twelve fine quality photographs on the themes of astronomy and space science, such as southern sky trails, the vela supernova remnant, rho ophiuchus and the region of antares, night view of ancient beijing observatory, the tarantulas nebula ( 30 doradus ), sunset on mauna kea, dunhuang star charts, etc. the calendar also includes the 1987 hong kong almanac, special astronomical phenomena and important historical events of astronomy

    精選的十二幅精彩天文和太空圖片包括：南天極星流跡、船帆座超新星爆發遺跡、蛇夫座與心宿二天區、北京古觀象臺夜景、劍魚座毒蛛星雲、英法美莫納克亞天文臺、敦煌星圖等。此月歷並附有1987年香港天象圖、特別天象資料、重要天文歷史大事等。
  3. The astrocalendar incorporates twelve fine quality photographs on the themes of astronomy and space science, such as southern sky trails, the vela supernova remnant, rho ophiuchus and the region of antares, night view of ancient beijing observatory, the tarantulas nebula 30 doradus, sunset on mauna kea, dunhuang star charts, etc. the calendar also includes the 1987 hong kong almanac, special astronomical phenomena and important historical events of astronomy

    精選的十二幅精彩天文和太空圖片包括：南天極星流跡船帆座超新星爆發遺跡蛇夫座與心宿二天區北京古觀象臺夜景劍魚座毒蛛星雲英法美莫納克亞天文臺敦煌星圖等。此月歷並附有1987年香港天象圖特別天象資料重要天文歷史大事等。
  4. There is a good chance that this outward diffusion of neutrinos and antineutrinos plays a crucial role in the supernova explosion.

    中微子和反中微子的這種向外的散射很可能在超新星爆發中起著關鍵的作用。
  5. The supernova explosion disrupts the binary.

    超新星爆發會瓦解雙星系統。
  6. There is a positive observational and theoretical basis for believing that neutron stars and black holes follow as a result of supernovae.

    中子星和黑洞則是超新星的產物，觀測上和理論上的依據使我們相信這一點。
  7. Cepheid variables are dimmer than the type i supernova. as a result, the supernova allows us to measure the distances of galaxies further away, but it happens much less often

    I型超新星比造父變星光亮，所以能夠量度更遙遠星系的距離，唯一缺點是不經常有i型超新星爆發。
  8. In the first seconds after a supernova, a region rich in protons emerges around the dead star ' s core, which has most likely collapsed into a neutron star

    在發生超新星爆炸后的最初幾秒內，這個死亡恆星的核心（最可能塌縮形成中子星的地方）周圍，會產生一個富含質子的區域。
  9. Dark red dots mark the locations of supernova remnants * *

    屏保中暗紅的點表示已知的超新星遺跡* * 。
  10. Data from the chandra observation show that the central ten - million - degree celsius cloud is the remains of a supernova explosion that destroyed a white dwarf star

    來自錢德拉的觀測數據表明，中心溫度達上千萬攝氏度的雲湍團是超新星爆發的殘余，爆發摧毀了一顆白矮星。
  11. In the case of n132d, the horseshoe shape of the remnant is thought to be due to shock waves from the collision of the supernova ejecta with cool giant gas clouds

    在n132d中，遺跡的馬蹄鐵狀外觀據信是因超新星拋出物與巨大的冷分子云相撞所致的。
  12. In the only other supernova remnant ( the vela supernova remnant ) where such features have been observed, the crescent shapes are clearly produced by ejecta fragments

    其他超新星遺跡中，只有一個（船帆座超新星遺跡）觀測到了這樣的特徵，可以確信，該遺跡的新月形外觀是拋出的碎片造就的。
  13. Pulsating variables vary periodically, but for some stars, there may be sudden changes in their brightness. such kinds of stars are called eruptive variables. they include

    ：脈動變星的光度會周期性地改變，但有一些恆星的光度會在毫無先兆下變得光芒萬丈，這種恆星包括新星和超新星皆統稱為爆發變星。
  14. After the supernova sn1987a exploded for more than a decade, the surrounding gas ring gradually brightened up

    超新星sn1987a爆發后十多年，周圍的氣體環反而逐漸變亮。
  15. When a giant star, for example, exhausts its fuel, it can detonate in a flash as luminous as 10 billion suns ? a supernova

    舉例來說，當一個巨星耗盡了燃料以後，它就會爆炸開來，亮度高達太陽的百億倍，此即超新星。
  16. For decades, scientists have known that supernovae, the explosive deaths of giant stars, trigger reactions to forge most of the heavy elements in the universe

    巨大的恆星在死亡時會產生超新星爆炸，所引發的反應，製造了宇宙中大多數的重元素，這是科學家幾十年前就已經知道的。
  17. Systems as diverse as the early universe, the interstellar medium, red giant stars, and supernova explosions are currently the focus of intense studies utilizing sophisticated computer models - models which require large quantities of nuclear data as input

    如早期的宇宙，星際介質，紅巨星，超新星爆， x -射線爆和-射線爆等多樣的系統，這些核天體過程是利用復雜的計算機模型，進行重點研究的焦點。
  18. Composed of micro diamonds, aluminum oxide, and silicon carbide, the isotopic distribution of these grains bore the telltale marks of their birth : ancient supernovas and red giant stars, that shone brightly and then flickered out, billions of years ago, before the birth of the solar system

    由微金剛石、鋁氧化物、碳化硅組成的這些微粒的同位素分佈透露出它們的誕生：那些數十億年前，在太陽系尚未誕生時，曾經閃耀並最終熄滅的古老超新星和紅巨星。
  19. On the bases of the galaxy evolution theory, we use the therotical chemical evolution model of three zone ( such as halo, thick disk and thin isk ) and multi - phase ( diffuse gas, molecular clouds, stars of both low and high mass, the remnants ). by comparing with the observational constraints, such assurface densities, age - metallicity relation, g - dwarf metallicity distribution in the solar neighbourhood and the correlation between [ a / fe ] and [ fe / h ], supernovae rates, infall rates. the rationality of the model is verified. based on the theory model, we calculate the abundance of neutron capture element

    本文正是在銀河系化學演化的基礎上，利用銀河系的三成分（ threezone ） （即暈、厚盤和薄盤）多相（ multi - phase ） （氣體，分子云，大、小質量恆星以及剩餘物質）的化學演化的理論模型，通過與觀測約束（質量面密度、場星的年齡-金屬豐度關系、太陽附近g矮星金屬含量分佈函數、三成份的特徵量、元素的星系化學演化、超新星的爆炸率、內落速率等）的比較，來檢驗模型的合理性。
  20. In 1987, the brightest supernova in recent history occurred in the large magellanic clouds

    1987年，近代歷史上最明亮的超新星出現在大麥哲倫星系。
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