| 1. | " for their discovery of cosmic microwave background radiation
发现宇宙微波背景辐射 |
| 2. | They had found the cool afterglow of the big bang : the cosmic microwave background radiation
他们发现的是大霹雳冷却后的馀晖：宇宙微波背景辐射。 |
| 3. | The cosmic microwave background radiation we see today is from the era just before the temperature was low enough to allow neutral hydrogen to form
简单来说，科学家所探测到的宇宙微波背景辐射，是来自刚转为透明前的宇宙。 |
| 4. | Other astronomers also reached the same conclusion when they were studying the fluctuations of the microwave background radiation
无独有偶，另一些天文学家通过测量宇宙的微波背景辐射在宇宙空间中的起伏变化，也获得同样的结论！ |
| 5. | Energy from the microwave background radiation and from collisions among the atoms would have sufficed to flip electrons and induce the hydrogen to glow feebly
从微波背景辐射以及原子碰撞而来的能量，已足够翻转电子，使得氢气微微发光。 |
| 6. | For examples , observation of the gravitational lens phenomenon and the scattering phenomenon produced by microwave background radiation and hot plasmas from galaxies clusters
，例如利用引力透镜现象及微波背景辐射与星系团的热等离子体造成的散射现象等等。 |
| 7. | We have a snapshot of the universe as it was 400 , 000 years after the big bang ? the cosmic microwave background radiation ? as well as pictures of individual galaxies a billion years later
我们已拥有宇宙在大霹雳40万年后光景的快照：宇宙微波背景辐射，与大霹雳10亿年后星系个体的影像。 |
| 8. | The nobel prize in physics goes to john mather and george smoot " for their discovery of the blackbody form and anisotropy of the cosmic microwave background radiation
2006年的诺贝尔物理学奖授予了美国科学家约翰?马瑟和乔治?斯穆特，以表彰他们发现了宇宙微波背景辐射的黑体形式和各向异性。 |
| 9. | Scientists used wilkinson microwave anisotropy probe wmap to capture the cosmic portrait that reveals the afterglow of the big bang , i . e . the cosmic microwave background radiation
科学家利用威尔金森微波各向异性探测器wilkinson microwave anisotropy probe , wmap ，测量来自不同方向的宇宙微波背景辐射，展示了大爆炸后的馀辉。 |
| 10. | 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
课程的主题包含了：行星、行星形成；恒星、太阳、正常的恒星、恒星形成；恒星演化、超新星、致密天体(白矮星、中子星及黑洞) 、波霎、双x -射线源；星团、球状及疏散星团；星际介质、气体、尘埃、磁场、宇宙射线；距离阶梯；星系、正常及活跃星系、喷流；重力透镜；大尺度结构；牛顿宇宙学、宇宙的动力膨胀及温度发展历史；宇宙背景微波辐射；大霹雳核合成。 |
