FREE BOOKS

Author's List




PREV.   NEXT  
|<   43   44   45   46   47   48   49   50   51   52   53   54   55   56   57   58   59   60   61   62   63   64   65   66   67  
68   69   70   71   >>  
ame of the constellation is given; for example, Vega is known as [a] Lyrae, meaning alpha of Lyra, Aldebaran as [a] Tauri, alpha of Taurus, etc. The twilight hour affords an excellent opportunity of fixing the relative positions of the first-magnitude stars in the mind, for at that time they alone, save the planets, are visible. METEORS, OR SHOOTING-STARS. As this work is designed primarily to cover what is observable in the starlit heavens with the naked eye, the subject of meteors, or shooting-stars, comes properly within its scope. There are few persons, if any, who have not witnessed the sight of a splendid meteor speeding across the sky, and such a sight always calls forth exclamations of wonder and delight. Apparently these evanescent wanderers in space are without distinctive features, and baffle classification; but, like all that nature reveals to us, they have been found, for the most part, to conform to certain laws, and to bear certain marks of resemblance that permit of their identification and classification. By careful observation for over fifty years the meteors, generally speaking, have been so arranged that they come under the head of one of the nearly three hundred distinct showers which are now recognized by astronomers. Many of these showers are too feeble and faint to be worthy of the attention of one not especially interested in the subject, but certain ones are well worth observing. There is always a pleasure in being able to recognize at a glance a certain definite manifestation of nature, be it a rare flower or a flashing meteor. The generally accepted theory respecting the meteors is that they were all originally parts of comets now disintegrated, and the four well-known showers of April 20th, August 10th and 14th, and November 27th, bear testimony to this theory. The apparent velocity of the meteors is between ten and forty-five miles a second, and their average height is about seventy-six miles at first appearance, and fifty-one miles at disappearance. Occasionally a meteor is so large and compact as to escape total destruction, and falls to the earth. Specimens of these meteorites are to be found in our best museums. I have seen fit to divide the principal meteor showers into four groups, according to the seasons in which they appear, and have placed them respectively at the conclusion of each season's work on the constellations. By radiant point is meant th
PREV.   NEXT  
|<   43   44   45   46   47   48   49   50   51   52   53   54   55   56   57   58   59   60   61   62   63   64   65   66   67  
68   69   70   71   >>  



Top keywords:

meteor

 

showers

 

meteors

 

classification

 

nature

 
subject
 

theory

 

generally

 

originally

 

comets


attention
 

respecting

 

disintegrated

 

recognized

 

feeble

 

worthy

 

observing

 
interested
 

recognize

 

manifestation


glance

 

definite

 

flower

 

accepted

 

astronomers

 

flashing

 
pleasure
 
principal
 

divide

 
groups

seasons

 

meteorites

 

museums

 
radiant
 

constellations

 

conclusion

 

season

 

Specimens

 
velocity
 

apparent


testimony

 

August

 

November

 

average

 

height

 

escape

 
compact
 
destruction
 

Occasionally

 

seventy