银河系

由此你可以算出银河系的总质量。

From this you can calculate the total mass in the Galaxy

银河系由1,000亿颗恒星组成。

The Galaxy consists of 100 billion stars .

此项研究的核心是早期宇宙和银河系的形成。

The main thrust of the research will be the study of the early Universe and galaxy formation

对银河系的研究表明，遥远星系在太空中的分布并不像理论所预言的那样均匀。

Galactic surveys show that distant galaxies are not as evenly distributed in space as theory predicts .

地球是银河系中的星球之一。

The earth is one of the planets in the galaxy .

首先,我们会在银河系中发现其他生命形式。

First , we 'll find other life forms in our galaxy .

它将帮助我们寻找银河系以外的智慧生命,探索宇宙的起源。

It will help us to search for intelligent life outside of the Galaxy and explore the origins of the universe .

说明：我们宏伟的银河系蜿蜒穿过这幅高企图心之全天影像

Explanation : Our magnificent Milky Way Galaxy sprawls across this ambitious all-sky panorama .

中国科学家近日宣布，中国高海拔宇宙线观测站（LHAASO拉索）在银河系内发现大量超高能宇宙加速器，这一发现可能颠覆人类对银河系的认识，并有助于揭示宇宙线起源这个困扰了科学家一个世纪的问题。

Chinese scientists have detected a dozen ultra-high-energy ( UHE ) cosmic accelerators within the Milky ( LHAASO ) .

解决G矮星问题的银河系化学演化三成分模型

Solving the G-dwarf Problem with a Three-Component Model of the Chemical Evolution of the Galaxy

银河系恒星形成区的OH、H2O脉泽

The OH and H2O Masers in the Star Forming Regions of the Galaxy

选用银河系中29个累积光谱型为F型的球状星团样本。

The 29 F globular clusters in the galaxy are selected as samples .

它们主要位于银河系（MilkyWay）等星系的旋臂和年轻星团中。

They mostly inhabit the spiral arms and younger parts of galaxies like the Milky Way .

银河系球状星团轨道参数分布的MonteCarlo模拟

Monte Carlo Simulation of Distribution of Orbital Parameters for Globular Clusters in the Galaxy

银河系中球状星团的空间分布、运动轨道及MonteCarlo模拟

Space Distribution , Motional Orbits and Monte Carlo Simulation of Globular Clusters in the Galaxy

关于太阳在银河系中所受引力与到银心距离r的关系的讨论

A discussion on the relation between the gravitation affecting the Sun in the Galaxy and the distance r to the center of the Galaxy

光学仪器是看不见这种日冕的，通过FUSE可看到，这种日冕围绕在银河系周围，象一个蓝色足球形状的外壳。

Invisible to optical devices , the halo can be seen by FUSE as a blue , football-shaped envelope around the galaxy .

本文利用HEAO-1A2的2-60keV弥漫X射线资料，扣除了银河系起源的X弥漫背景影响，得到有关宇宙X背景的资料。

Using the new data of the 2-60 keV diffuse X-ray background from HEAO-1 A2 and subtracting the model galactic X-ray component , the cosmic X-ray background data have been obtained .

对银河系中心超大质量黑洞候选体SgrA~的VLBI观测研究

VLBI observations of SGR a ~ : a supermassive black hole candidate at the Galactic Centre

令人怀念的《银河系漫游指南》作者道格拉斯·亚当斯（DOUGLASADAMS）幻想出过很多漫画创作。

DOUGLAS ADAMS , the late lamented author of " The Hitchhiker 's Guide to the Galaxy ", dreamed up many comic creations .

本文给出了银河系12颗碳星的J、H、K波段的测光结果，并讨论了星际红化的影响。

The infrared photometry in J , H and K bands for 12 carbon stars in Our Galaxy are given in this paper , while the effect of interstellar reddening are discussed .

中国很快将发射其第一颗X射线太空望远镜--硬X射线调制望远镜，以观察银河系从而监测天体的X射线源。

China will soon launch its first X-ray space telescope , the Hard X-ray Modulation Telescope ( HXMT ) , with the aim of surveying the Milky Way to observe celestial sources of X-rays .

此次公布的银河系新图像是基于美国NASA斯皮策空间望远镜以红外线对银河系的观察。

The new survey of an extensive swath of the Milky Way was done with NASA 's Spitzer Space Telescope , which detects infrared light .

富氧AGB星在银河系中的分布

The Galactic distribution of O-rich AGB Stars

许多黑洞和中子星被认为隐藏在银河系中，由于它们不能发出可见光，或是隐藏在尘埃后面，只有通过X射线太空望远镜才能观测到。

Many black holes and neutron stars are thought to be hidden in the Milky Way . Since they don 't emit visible light , or are covered by dust , only X-ray telescopes can find them .

他在告诉我们ori为什么要来到这个银河系。

He just told you why the ori are on their way to this galaxy .

据美国国家航空航天局（Nasa）和其他宇航机构最新收集的数据表明，在银河系，有多达400亿个潜在的可居住星球。

The latest data collected by Nasa and other space agencies suggests there could be as many as 40 billion potentially habitable planets in our galaxy , the Milky Way .

HIPPARCOS后的银河系距离尺度

Post-Hipparcos Galactic Distance Scales

Segue2是围绕着银河系运转的数十个卫星星系的其中之一。

Segue 2 is one of dozens of " companion " galaxies that orbit the Milky Way .

明亮的OH脉泽是探测银河系中各类天体甚至河外星系的极好工具，但是对OH脉泽的抽运机制的鉴别和模拟上的困难使得这个极好工具一直没有得到极好的发挥。

The bright OH masers are excellent probes of different kinds of astronomical objects in the Galaxy and even of distant galaxies , but the difficulties in identifying the pumping mechanisms of these OH masers and modeling them have hindered the application of this excellent probe .