FREE BOOKS

Author's List




PREV.   NEXT  
|<   131   132   133   134   135   136   137   138   139   140   141   142   143   144   145   146   147   148   149   150   151   152   153   154   155  
156   157   158   159   160   161   162   163   164   165   166   167   168   169   170   171   172   173   174   175   176   177   178   179   180   >>   >|  
flights of meteoric masses enormous in size and many in number, which, falling on the sun's globe with the enormous velocity corresponding to their vast orbital range and their near approach to the sun--a velocity of some 360 miles per second--would, beyond all doubt, excite his whole frame, and especially his surface regions, to a degree of heat far exceeding what he now emits. We have had evidence of the tremendous heat to which the sun's surface would be excited by the downfall of a shower of large meteoric masses. Carrington and Hodgson, on September 1, 1859, observed (independently) the passage of two intensely bright bodies across a small part of the sun's surface--the bodies first increasing in brightness, then diminishing, then fading away. It is generally believed that these were meteoric masses raised to fierce heat by frictional resistance. Now so much brighter did they appear, or rather did that part of the sun's surface appear through which they had rushed, that Carrington supposed the dark glass screen used to protect the eye had broken, and Hodgson described the brightness of this part of the sun as such that the part shone like a brilliant star on the background of the glowing solar surface. Mark, also, the consequences of the downfall of those two bodies only. A magnetic disturbance affected the whole frame of the earth at the very time when the sun had been thus disturbed. Vivid auroras were seen not only in both hemispheres, but in latitudes where auroras are very seldom witnessed. 'By degrees,' says Sir J. Herschel, 'accounts began to pour in of great auroras seen not only in these latitudes, but at Rome, in the West Indies, in the tropics within eighteen degrees of the equator (where they hardly ever appear); nay, what is still more striking, in South America and in Australia--where, at Melbourne, on the night of September 2, the greatest aurora ever seen there made its appearance. These auroras were accompanied with unusually great electro-magnetic disturbances in every part of the world. In many places the telegraph wires struck work. They had too many private messages of their own to convey. At Washington and Philadelphia, in America, the electric signal-men received severe electric shocks. At a station in Norway the telegraphic apparatus was set fire to; and at Boston, in North America, a flame of fire followed the pen of Bain's electric telegraph, which writes down the message upon chemically
PREV.   NEXT  
|<   131   132   133   134   135   136   137   138   139   140   141   142   143   144   145   146   147   148   149   150   151   152   153   154   155  
156   157   158   159   160   161   162   163   164   165   166   167   168   169   170   171   172   173   174   175   176   177   178   179   180   >>   >|  



Top keywords:

surface

 

auroras

 

America

 

electric

 

bodies

 

masses

 

meteoric

 
brightness
 

Carrington

 

magnetic


velocity
 

enormous

 

downfall

 

Hodgson

 
degrees
 
September
 

latitudes

 

telegraph

 

Melbourne

 

Australia


striking

 

seldom

 

witnessed

 

hemispheres

 
disturbed
 

Herschel

 

Indies

 
tropics
 

eighteen

 

accounts


equator

 

Norway

 

station

 

telegraphic

 

apparatus

 

shocks

 

severe

 

Philadelphia

 
signal
 

received


Boston

 

message

 

chemically

 

writes

 

Washington

 

convey

 

accompanied

 

unusually

 
electro
 

disturbances