interstellar medium 中文意思是什麼
interstellar medium
解釋
星際介質- interstellar : adj. 【天文學】星際的。 interstellar aeronautics 星際航行。 interstellar space 星際空間。
- medium : n (pl dia )1 媒介物;傳導體;媒質,基質,介質,介體;中間物;環境、生活情形。2 手段,方法;媒介...
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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。 -
What new information have we gleaned about the comparatively dense gas-dust complexes of the interstellar medium over the past dozen years ?
過去的十幾年裡,有關星際介質的較密氣塵復合體我們探明了哪些新東西呢? -
Stars are born from a kind of primal soup known as the interstellar medium.
恆星是由一種稱為星際介質的「原湯」形成的。 -
Topics include : planets, planet formation ; stars, the sun, " normal " stars, star formation ; stellar evolution, supernovae, compact objects ( white dwarfs, neutron stars, and black holes ), plusars, binary x - ray sources ; star clusters, globular and open clusters ; interstellar medium, gas, dust, magnetic fields, cosmic rays ; distance ladder ; galaxies, normal and active galaxies, jets ; gravitational lensing ; large scaling structure ; newtonian cosmology, dynamical expansion and thermal history of the universe ; cosmic microwave background radiation ; big - bang nucleosynthesis
課程的主題包含了:行星、行星形成;恆星、太陽、正常的恆星、恆星形成;恆星演化、超新星、緻密天體(白矮星、中子星及黑洞) 、波霎、雙x -射線源;星團、球狀及疏散星團;星際介質、氣體、塵埃、磁場、宇宙射線;距離階梯;星系、正常及活躍星系、噴流;重力透鏡;大尺度結構;牛頓宇宙學、宇宙的動力膨脹及溫度發展歷史;宇宙背景微波輻射;大霹靂核合成。 -
Simple laws of physics suggest, that gas-dust complexes in the interstellar medium may evolve, first into protostars and subsequently into stars.
簡單的物理學定律揭示出,星際介質中的氣塵復合體可以進化,先是演化為原恆星,接下去再演化為恆星。 -
In a relatively short time ( about 1000 years ) the entire shells will be ejected into space, joining the gas and dust in the interstellar medium
在相對較短的一段時間里(大約1000年)整個殼層將被拋入太空,加入到星際介質的氣體和塵埃中。 -
As gas flies away from the detonated star, it decays and reacts with the interstellar medium, producing light in many different colors and energy bands
當氣體從爆炸的中心遠離時,它的亮度會減弱,並和附近的星際介質發生交互作用,產生各種顏色和波段的光。 -
Introduction to astronomy provides a quantitative introduction to physics of the solar system, stars, interstellar medium, the galaxy, and universe, as determined from a variety of astronomical observations and models
天文學導論這門課提供了對太陽系、恆星、星際介質、星系及宇宙等的物理入門。這些都建立在各種的天文觀測及模型的基礎下。 -
A star is formed when a cloud of gas collapses from the interstellar medium toward high density.
一個氣體雲自星際物質中坍縮,密度達到很高時,即形成了一個恆星。 -
The outer layers of the star crashed into the interstellar medium, driving a shock wave that is still visible today
這顆星的外層撞到星際物質,由其產生的沖擊波至今仍然可見。 -
It says that the stars indeed rotate at different speed, but the density of the interstellar medium form a wave. at the wave front, where the density is higher, star formation is enhanced. that is why we find young stars along the spiral arms and old stars elsewhere
這個理論認為雖然恆星會以不同速度移動,但星際物質的密度會產生波動,在密度最高的波陣面會催生出新的恆星,這解釋了為何通常在旋臂會找到新生恆星,而在其他地方只有古老恆星的原因。
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