返回
朗读
暂停
+书签

视觉:
关灯
护眼
字体:
声音:
男声
女声
金风
玉露
学生
大叔
司仪
学者
素人
女主播
评书
语速:
1x
2x
3x
4x
5x

上一页 书架管理 下一页
3 THE REVEREND EVANS’S UNIVERSE
an enormous amount of ne provided t reference to supernovaeand to neutron stars; convincingly explained tion; correctly calculatedted supernovaexplosions to tion of a mysterious neionary to say t. Neutron stars  be confirmed for ty-four years. tion,t been verified yet. Altogetract ecrop Kip S. t prescient documents in tory of pronomy.”

    Interestingly, Zanding of whis would happen.

    According to t understand to be able tosubstantiate alent ly—to do tical sweeping up.

    Z to recognize t t nearly enougo oget t be some otational influence—ter. One to see  if a neutron star s  even lig escape its immense gravitationalpull. You ely, Zracted almost no notice. er, tRobert Oppenurned tention to neutron stars in a landmark paper,  asingle reference to any of Z doions concerning dark matter attract serious attention for nearly four decades. e can only assume t  of pushis period.

    Surprisingly little of to us  6,000 stars are visible to t 2,000 can be seenfrom any one spot. itars you can see from a single locationrises to about 50,000, and  leaps to 300,000. iteen-incelescope, suco count not in stars but in galaxies. From ensof billions of stars. table numbers, but even o take in,supernovae are extremely rare. A star can burn for billions of years, but it dies just once andquickly, and only a fears explode. Most expire quietly, like a campfire at daypical galaxy, consisting of a ars, a supernova tle bit like standingon tion platform of tate Building elescope and se
上一页 书架管理 下一页

首页 >A Short History of Nearly Everything简介 >A Short History of Nearly Everything目录 > 3 THE REVEREND EVANS’S UNIVERSE