star stars 中文意思是什麼

star stars 解釋
星中星
  • star : n 1 星;【天文學】恆星 (opp planet)。2 星狀物,星(形勛)章。3 【印刷】星形號〈 〉。4 【占星術...
  • stars : storage]短期聽力恢復及存儲
  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. There has been many papers to discuss the in - medium quark and gluon condensates in nuclear matter which use the models with su ( 2 ) l su ( 2 ) r sym - metry. now, we make use of the chiral model su ( 3 ) l su ( 3 ) n including the baryon octet to discuss the quark condensate < qq > in strange matter, where q is an up or down quark field. on the one hand, from the experimetal data, it is found that < qq > vac = - ( 225 25mev ) 3, on the other hand, with the hellmann - feynman theorem, quark condensate can be evaluated on the hadronic level. in this paper, we will investigate the quark condensate in strange matter with the chiral symmetry su ( 3 ) l x su ( 3 ) rspontaneous breaking lagrangian to obtain the variation of the quark condensate in the strange matter when the baryon number change. it can be applied to understand the neutron stars when the neutron star are considered to be constructed by the strange matter. because nertron stars are homogeneous and at very low temperature, we will use the mean - field approximation and zero temperature throughout this paper

    鑒于已有大量文獻討論了核物質中的夸克凝聚,本文將討論在奇異物質中的夸克凝聚。而在介質中的夸克凝聚的基本公式可由hellmann - feynman理論導出,所以運用手征對稱自發破缺拉氏量以及平均場近似,我們就可以討論在奇異物質中的夸克凝聚,由所計算的結果表明: ( 1 )奇異物質中的夸克凝聚隨奇異物質密度的增大而單調減小。 ( 2 ) -凝聚的出現對衰減率有影響。
  3. A binary star is a double star, consisting of two stars turning round each other

    雙星是兩顆星,是由相互圍繞旋轉的兩顆星組成。
  4. Many stars orbit around other stars under the mutual gravitational attractions. if two stars orbit around one another, they form a binary star system

    在天空中,不少恆星會在相互的引力下互相繞著對方運行,假若系統只有兩顆星,我們會稱之為
  5. One of the stars shall be bigger than the others, with its circumcircle s diameter being 310ths of the height of the flag, and shall be placed in the left ; the four other stars shall be smaller, with their circumcircle s diameter being 110th of the height of the flag, encircling the big star on its right in the shape of an arc

    旗面為紅色,長方形,其長與高為三與二之比,旗面左上方綴黃色五角星五顆。一星較大,其外接圓直徑為旗高十分之三,居左;四星較小,其外接圓直徑為旗高十分之一,環拱于大星之右。
  6. The brighter of two stars that make up a double star

    雙星中較亮的一顆組成兩顆雙星中的較亮的一顆
  7. We arbitrarily choose one fixed star as the reference and define its magnitude as zero. then, the magnitude one stars are about 2. 51 times dimmer for 2. 51

    我們隨意找了一顆恆星,把它的亮度定義為0等,那麼,因為2 . 51
  8. The star to be moving rapidly, perhaps in an orbit around the densely concentrated stars of the galactic nucleus.

    這顆星看來正在以高速運動著,其運動軌道大概就圍繞著由高度密集的恆星所構成的銀河系核心。
  9. A few stars are known which are hardly bigger than the earth, but the majority are so large that hundreds of thousands of earths could be packed inside each and leave room to spare ; here and there we come upon a giant star large enough to contain millions of millions of earths

    人們所知道的幾個星球並不比地球大多少,但絕大多數的星球卻大得足以容納成千上萬個地球還綽綽有餘;我們到處都能遇見大得足以包容千千萬萬個地球的巨星。
  10. We consider the macroscopic thermal properties of the gas throughout the interstellas region ionized by an exciting star or group of stars.

    我們將考察被一顆或一群激發星電離的星際區域中各種氣體的宏觀熱力學性質。
  11. If three or more stars interact with each other, they form a multiple star system

    ,若有三顆或更多的星互相影響,我們則稱之為多重星或聚星。
  12. When compared with the multiple star systems, they consist of many more stars, from tens to millions

    相對于多重星,星團內恆星的數目多很多,由數十以至數百萬顆不等。
  13. Nature of the universe - chapter thirteen our sun is a single star with approximately constant brightness. in fact, in the universe, many stars are not alone, they interact with each other to form binary or multiple star systems

    我們的太陽在太空中孤獨地發放穩定的光芒,但在宇宙中,很多星星並不會單獨地存在,而是和其它恆星組成雙星或甚至多重星系統。
  14. These stars appear to move around the north star

    這些星星似乎環繞著北極星轉。
  15. Try to shoot star trails of the northern sky, all stars appear to revolve around the polaris

    如朝向北方拍攝,可以見到所有星體都好像圍繞著北極星旋轉,十分有趣。
  16. Regarding matthew ' s statements that the star " went before " and " stood over ", molnar and others have maintained that the greek words used there refer to jupiter ' s retrogradation ( i. e. apparent but not actual retrograde motion ) and stationing, respectively, as the movement of jupiter against the background of the stars appears to reverse course for a time and then stops before resuming the normal progression

    關于馬太對「居先」和「站立」的恆星的陳述,蒙爾耐和其他人聲稱這里是使用了希臘單詞來分別地代表木星的倒行和停留(例如,外觀上並不是真正的逆行運動) ,當木星逆著恆星背景而行,在一段時間內呈現出相反路線,然後在重新開始正常行進之前停止。
  17. Returning to a theme he has voiced many times before, the cambridge university cosmologist said that space - rockets propelled by the kind of matter / antimatter annihilation technology popularised in star trek would be needed to help homo sapiens colonise hospitable planets orbiting alien stars

    這位劍橋大學宇宙論者重提他過去曾多次探討的主題說,星艦奇航記中那種廣為人知的物質?反物質的互相抵消科技推動的太空火箭,可以用來幫助人類移民到環繞外星球運行的友善行星。
  18. The bulk of the mass is spread out, forcing stars to trace a spirograph - like rosette : an ellipse that does not close on itself but gets offset each time the star completes one revolution [ see box at right ]

    整體質量分散開來,迫使恆星運行方式如旋轉繪圖盤所畫出的花瓣狀螺線:那不是每圈都會封閉起來的橢圓,恆星繞行一周后,軌道並不接合便又重新開始下一周的運動(見右方整理軌道秩序) 。
  19. A galaxy or a star cluster consists mainly of the stars

    星系和星團主要由恆星組成。
  20. One way to see more massive stars have shorter lives is to study the star clusters

    大質量恆星壽命較短的直接證據可以在星團中找到。
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