FREE BOOKS

Author's List




PREV.   NEXT  
|<   28   29   30   31   32   33   34   35   36   37   38   39   40   41   42   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   72   73   74   75   76   77   >>   >|  
of all. If we look at her even with the naked eye, we can see that she is elongated or drawn out, but her brilliance prevents us from seeing her shape exactly; to do this we must use a telescope. [Illustration: DIFFERENT PHASES OF VENUS.] It is a curious fact that some planets shine much more brightly than others, without regard to their size--that is to say, the surface on which the sun's rays strike is of greater reflecting power in some than in others. One of the brightest things in Nature that we can imagine is a bank of snow in sunlight; it is so dazzling that we have to look away or wink hard at the sight; and the reflective power of the surface of Venus is as dazzling as if she were made of snow. This is probably because the light strikes on the upper surface of the clouds which surround her. In great contrast to this is the surface of Mercury, which reflects as dully as a mass of lead. Our own moon has not a high reflecting power, as will be easily understood if we imagine what the world would be if condemned to perpetual moonlight only. It would, indeed, be a sad deprivation if the mournful cold light of the moon, welcome enough as a change from sunlight, were to take the place of sunlight in the daytime. For a very long time astronomers could not discover what time Venus took in rotating on her own axis--that is to say, what the length of her day was. She is difficult to observe, and in order to find out the rotation it is necessary to note some fixed object on the surface which turns round with the planet and comes back to the same place again, so that the time it takes in its journey can be measured. But the surface of Venus is always changing, so that it is impossible to judge at all certainly. Opinions differ greatly, some astronomers holding that Venus's day is not much longer than an earthly day, while others believe that the planet's day is equal to her year, just as in the case of Mercury. Venus's year is 225 days, or about seven and a half of our months, and if, indeed, her day and year are the same length, very peculiar effects would follow. For instance, terrible heat would be absorbed by the side of the planet facing the sun in the perpetual summer; and the cold which would be felt in the dreary winter's night would far exceed our bitterest Arctic climate. We cannot but fancy that any beings who might live on a planet of this kind must be different altogether from ourselves. Then, there is ano
PREV.   NEXT  
|<   28   29   30   31   32   33   34   35   36   37   38   39   40   41   42   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   72   73   74   75   76   77   >>   >|  



Top keywords:

surface

 
planet
 
sunlight
 

imagine

 

reflecting

 

dazzling

 

Mercury

 

perpetual

 
astronomers
 

length


changing
 
observe
 

Opinions

 

differ

 

greatly

 

impossible

 

difficult

 
measured
 

holding

 

object


rotation

 
journey
 
facing
 

beings

 

summer

 

absorbed

 
dreary
 

winter

 

climate

 

Arctic


bitterest

 

exceed

 

terrible

 

earthly

 

follow

 

instance

 

effects

 

peculiar

 
altogether
 

months


longer

 

condemned

 

regard

 
brightly
 
planets
 
strike
 

greater

 

Nature

 

brightest

 

things