FREE BOOKS

Author's List




PREV.   NEXT  
|<   338   339   340   341   342   343   344   345   346   347   348   349   350   351   352   353   354   355   356   357   358   359   360   361   362  
363   364   365   366   367   368   369   370   371   372   373   374   375   376   377   378   379   380   381   382   383   384   385   386   387   >>   >|  
f two stars which revolve around each other in regular orbits, and are among some of the most interesting objects in the heavens. About 1000 Binary stars are known altogether. Their motions, however, are very slow, and only in a comparatively few cases have the dimensions of their orbits been ascertained. Some of the Binary stars are Zeta Hercules, which has a period of about 36 years; Eta Coronae Borealis, which has a period of 43 years; while the brightest star, Sirius, is also a Binary star, with a period of about 50 years. _The Milky Way._--The Milky Way is the name given to that band of light which stretches across the sky at night-time, and forms a zone or belt that completely circles the celestial sphere. This belt of light has maintained from the earliest ages the same relative position among the stars, and, when resolved by powerful telescopes, is found to consist entirely of stars scattered by millions across the expanse of the heavens. The whole zone or belt is composed of nothing but stars, whose average magnitude, according to Herschel, is about the tenth. Stars of all magnitudes are, however, found in this zone. Of the brightest stars, about twelve are found in this region, while the majority of stars of the second, third, and fourth magnitudes are also found in or near it. The great majority of star clusters are also found along the course of the Milky Way, while many of the irresolvable nebulae seem to congregate near the poles of this starry region. The Milky Way is divided in one part of its course by a stream of stars, which seems to branch off as a separate stream, thus dividing it into two parts. All these facts seem to point to the conclusion that the stars of the universe, instead of being scattered about haphazard in the space, form a ring or layer, of which the thickness is very small compared with its length and breadth. Our own solar system, according to Herschel, occupies a place somewhere about the middle of the thickness of the zone, and near the point where it divides into two parts. Recent observations go to show that there is a tendency of the sun's apex to drift along the edge of the Milky Way, and this drift seems to point to a plane of motion of the sun, nearly coinciding with the plane of the Milky Way. ART. 118. _Stars and Kepler's Laws._--We have learned in a previous chapter that the sun is the centre of a system which comprises a retinue of planets, wi
PREV.   NEXT  
|<   338   339   340   341   342   343   344   345   346   347   348   349   350   351   352   353   354   355   356   357   358   359   360   361   362  
363   364   365   366   367   368   369   370   371   372   373   374   375   376   377   378   379   380   381   382   383   384   385   386   387   >>   >|  



Top keywords:

period

 

Binary

 
brightest
 

system

 

thickness

 
orbits
 
magnitudes
 
region
 

majority

 

Herschel


scattered
 

stream

 

heavens

 
comprises
 
motion
 
dividing
 
branch
 

separate

 

starry

 
irresolvable

learned

 

centre

 

previous

 

chapter

 

nebulae

 
coinciding
 

Kepler

 

congregate

 

divided

 

observations


breadth

 

Recent

 
clusters
 

planets

 

occupies

 

middle

 

retinue

 
divides
 

length

 

universe


conclusion

 

haphazard

 

compared

 

tendency

 

expanse

 
Hercules
 
ascertained
 

dimensions

 

Sirius

 

Coronae