恆星測光 的英文怎麼說

中文拼音 [héngxīngcèguāng]
恆星測光 英文
stellar photometry
  • 恆 : Ⅰ形容詞1 （永久; 持久） permanent; lasting 2 （平常; 經常） usual; common; constant Ⅱ名詞1 （恆心...
  • 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...
  • 測 : 動詞1. （測量） survey; fathom; measure 2. （測度; 推測） conjecture; infer
  • 光 : Ⅰ名詞1 （照耀在物體上、使人能看見物體的一種物質） light; ray 2 （景物） scenery 3 （光彩; 榮譽） ...
  • 恆星 : [天文學] fixed star; star恆星大氣 stellar atmosphere; 恆星導航 star navigation; stellar guidance;...
  1. The various colours significant of various degrees of vitality white, yellow, crimson, vermilion, cinnabar : their degrees of brilliancy : their magnitudes revealed up to and including the 7th : their positions : the waggoner s star : walsingham way : the chariot of david : the annular cinctures of saturn : the condensation of spiral nebulae into suns : the interdependent gyrations of double suns : the independent synchronous discoveries of galileo, simon marius, piazzi, le verrier, herschel, galle : the systematisations attempted by bode and kepler of cubes of distances and squares of times of revolution : the almost infinite compressibility of hirsute comets and their vast elliptical egressive and reentrant orbits from perihelion to aphelion : the sidereal origin of meteoric stones : the libyan floods on mars about the period of the birth of the younger astroscopist : the annual recurrence of meteoric showers about the period of the feast of s. lawrence martyr, 10 august : the monthly recurrence known as the new moon with the old moon in her arms : the posited influence of celestial on human bodies : the appearance of a star 1st magnitude of exceeding brilliancy dominating by night and day a new luminous sun generated by the collision and amalgamation in incandescence of two nonluminous exsuns about the period of the birth of william shakespeare over delta in the recumbent neversetting constellation of cassiopeia and of a star 2nd magnitude of similar origin but lesser brilliancy which had appeared in and disappeared from the constellation of the corona septentrionalis about the period of the birth of leopold bloom and of other stars of presumably similar origin which had effectively or presumably appeared in and disappeared from the constellation of andromeda about the period of the birth of stephen dedalus, and in and from the constellation of auriga some years after the birth and death of rudolph bloom, junior, and in and from other constellations some years before or after the birth or death of other persons : the attendant phenomena of eclipses, solar and lunar, from immersion to emersion, abatement of wind, transit of shadow, taciturnity of winged creatures, emergence of nocturnal or crepuscular animals, persistence of infernal light, obscurity of terrestrial waters, pallor of human beings

    顯示出不同程度之生命力的繽紛色彩白淺黃深紅朱紅銀朱諸星之亮度一直包括到七等星以等級標志的諸星之大小諸星的位置御夫座沃爾辛厄姆路172大衛的戰車173土星光環螺旋星雲凝固后形成有衛星的恆星群兩重大陽相互依存的旋轉運動伽利略西蒙馬里烏斯174皮亞175勒威耶赫歇耳加勒176等人各自獨立地同時所做的發現波得和開普勒所嘗試的距離的立方與回轉次數的平方的體系化177多毛的眾彗星178那幾殆無限的被壓縮性，以及自近日點至遠日點那廣漠的遠心的重返大氣層的橢圓軌道隕石的恆星之起源年紀較輕的天體觀測者誕生的那個時期火星上所出現的「暗波」現象179每年在聖勞倫斯節殉教者，八月十日前後降落的隕石雨每月都發生的所謂「新月抱舊月」現象180關于天體對人體的影響的假定威廉莎士比亞出生的時期，在斜倚卻永不沒落的仙后座那三角形上端，一顆不分晝夜散發著極亮光彩的星辰一等星出現了181這是兩個無光死滅了的太陽因相撞並汞合為白熱體而形成的燦爛的新太陽大約在利奧波德布盧姆出生時，出現在七星花冠星座里而後又消失了的一顆同一起源亮度卻稍遜的星宿二等星182還有約於斯蒂芬迪達勒斯出生時，出現在仙女座中之後又消失，小魯道爾夫布盧姆出生與夭折數年後出現于御夫座后又消失，以及另外一些人出生或去世前前後後出現在許許多多其他星座中而又消失了的假定是同一起源的實際存在或假定存在的星斗183 。
  2. The parallactic refraction between the stars and the satellite is small and well determinate, except for the irregular stellar movements known as erratics.

    除了通稱為游動的不規律星體運動之外，恆星和衛星之間的視差折光差微小，而且是容易測定的。
  3. In photographic photometry we use photographic plates of a certain region of the sky to determine the coordinates of the stars.

    在照相測光中，我們利用所拍攝的天空某一區域的照相底片來測定恆星的坐標。
  4. During the total solar eclipse in 1919, scientists verified that light from remote stars could be bent by the gravity of the sun - just as einstein predicted. einstein became world famous overnight

    1919年，當日食觀測隊藉日全食時證實來自遙遠恆星的光線被太陽的重力所偏折恰如愛因斯坦的預測一樣，一夜之間，愛因斯坦成為全世界的知名人物。
  5. We either use a real star or a light source on distant buildings for star test

    我們採用真正恆星或者利用遠處建築物的光源來進行星點測試。
  6. As supernova is the explosive death of a star in an event so violent that for a brief period that a single star shines as brightly as a whole galaxy of more than 100 billion ordinary stars, it can be easily seen even it is a few billion light - years away

    由於超新星是恆星垂死前的一次極猛烈爆炸，剎那間閃耀的光芒甚至蓋過整個星系中上千億顆恆星，因此遠至數十億光年外也能清楚測量得到。
  7. A convenient classification of stars is based upon the observed sequence of spectral types.

    一種實用的恆星分類法是基於測得的光譜類型序列。
  8. Because optical observations are impossible, speculation on the stellar content in dark clouds long received little attention.

    由於不可能進行光學觀測，所以關于暗雲中恆星數目的推算長期以來不受重視。
  9. If the distance between the star and the observer is double, we will see only 1 4 of the original intensity. this is the inverse square law

    若恆星和觀測者的距離倍增，那麼看到的恆星光度便只及原來的四分之一，這就是平方反比定律。
  10. Unlike looking at visible light, the spatial resolution of x - ray optics is not that high in the last two decades. hence, astronomers often do not know the correct identification of those x - ray sources in a crowded region when comparing to optical images

    然而在過去二十年來， x射線探測器的空間解析度始終及不上可見光波段的望遠鏡，因此天文學家往往很難在恆星密布的區域內，證認出究竟是那個天體發射出x射線。
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