恆星時 的英文怎麼說

中文拼音 [héngxīngshí]
恆星時 英文
sidereal time恆星時記時器 siderograph
  • : 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...
  • : 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...
  • : shí]Ⅰ名1 (比較長的一段時間)time; times; days:當時at that time; in those days; 古時 ancient tim...
  • 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之亮度一直包括到七等以等級標志的諸之大小諸的位置御夫座沃爾辛厄姆路172大衛的戰車173土光環螺旋雲凝固后形成有衛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之起源年紀較輕的天體觀測者誕生的那個期火上所出現的「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辰一等出現了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,出現在七花冠座里而後又消失了的一顆同一起源亮度卻稍遜的宿二等182還有約於斯蒂芬迪達勒斯出生,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斗183 。
  2. In some binary star systems, gas escapes from one star and is captured by the gravity of the other to form a disk

    某些雙系統中,當從一個逃出的氣體被另一個體的重力捕獲,也會形成盤狀結構。
  3. As not as calamitous as a cataclysmic annihilation of the planet in consequence of collision with a dark sun

    這一災難還不像行與隱蔽的相撞所發生的毀滅性劇變那樣大。
  4. Carbon stars with c / o > 1 are a kind of stars that form at the agb stage and evolved from oxygen - rich agb stars with mid - mass

    是中等質量演化到agb階段可能形成的一種,它由氧演化而來, [ c o ] 1 。
  5. We have to use some other methods to measure the luminosity or equivalently the absolute magnitude of the cepheid variable. since we can readily measure the apparent magnitude of a cepheid variable, to measure the luminosity means measuring the distance. we use some distance measurement methods, for example, parallax, to determine the relation

    要弄清這個關系,我們要知道不同造父變的光度和光變周期數據,量度光變周期當然不是問題,但要得知一顆的光度,我們首先要得知它的距離,這便須藉助好像視差法等其他量度天體距離的方法。
  6. Caption : : astronomers were surprised to discover a 25 - million - year - old protoplanetary disk around a pair of red dwarf stars 350 light - years away

    天文學家一直認為形成的同一定會形成行,但最近一項發現推翻了這定律。
  7. If the ascendant be one of those signs called “ mute ”, and mercury in one that is not humane, with any fixed star of the nature of saturn, the native will never speak well, but bring forth his words with difficulty

    當上升點位於啞座,水落入非人形座且位於土屬性的附近,盤主談吐不暢,且伴有語言障礙。
  8. 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

    巨大的在死亡會產生超新爆炸,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。
  9. A quantitative analysis of this idea led to the prediction that a star remaining about three times the mass of the sun at the end of its evolution ( usually as a neutron star ), will almost inevitably shrink to the critical size needed to undergo a gravitational collapse

    該想法的定量分析導致預言一顆在終止它演化候保持大約三倍太陽的質量(通常看做一顆中子) ,將會幾乎不可避免收縮到臨界體積必須遭受引力坍塌。
  10. Evolution of stars of all masses takes place on a hydrodynamic time scale.

    各種質量的的演化,均以流體力學的間尺度進行。
  11. From long ago, by an established tradition that can be traced to the hypothesis of immanuel kant and the marquis de laplace, astronomers have assumed that stars develop out of a scattered, diffuse medium of gas and dust.

    很長間以來,天文學家承襲了可以追溯至康德和拉普拉斯假說所建立的概念,認為由散布在空中的彌漫氣塵物質演變而來。
  12. When the star becomes hot enough, it ionizes its surrounding gas from which the dust has been expelled.

    變得足夠熱的候,它將四周的氣體電離,氣體中的塵埃被趕走。
  13. But during an eclipse, stars whose line of sight lies near the sun can be photographed.

    但在日蝕的候,那些在我們的視線看來處在太陽附近的,卻可以用照相方法攝下來。
  14. 5 a star begins to form when nuclear fusion takes place

    核聚變(核子融合)發生,一顆就開始了形成過程。
  15. This is the apparent magnitude of an object at some standard distance from us. this standard distance is chosen to be about 32 light years 10 parsecs, see below

    絕對等是距離為約32光年或10秒差距請參閱下一節等。
  16. Usually, proper motion of a star is very small and can only be detected if we observe the star for decades. there is one important exception however

    ,但的移動非常非常緩慢,非要經過數十年的間,再加上精確的量度,才能夠偵測出來。
  17. Local sidereal time

    地方恆星時
  18. Local apparent sideral time

    地方視恆星時
  19. As they move into their near - star orbits, hot jupiters could be playing violent games of planetary billiards that produce earthlike planets, he says

    在它們靠近恆星時,它們可能會發生可怕的碰撞並產生類似地球的行
  20. This telescope has just recently found what many astronomers believe to be a black hole, after being focused on a star orbiting empty space

    這架天文望遠鏡在對準一顆環繞空蕩蕩的空間運轉的恆星時,發現了被許多天文學家認為是黑洞的東西。
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