FREE BOOKS

Author's List




PREV.   NEXT  
|<   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   >>  
out 64 miles in diameter, with an internal depth of 14,000 to 18,000 feet, and a beautiful central group of mountains, one-third of that height, on its floor. This proves that the last eruptive efforts in this part of the moon fully equalled in intensity those that had preceded them. Although Theophilus is on the whole the deepest crater we can see in the moon, it has received little or no deformation by secondary eruptions." But perhaps the most remarkable object on the whole hemisphere of the moon is "the majestic Tycho," which rises from the surface near the south pole, and at a distance of about 1/6th of the diameter of the sphere from its margin. Its depth is stated by Ball to be 17,000 feet, and its diameter 50 miles. But its special distinction amongst the other volcanic craters lies in the streaks of light which radiate from it in all directions for hundreds and even thousands of miles, stretching with superb indifference across vast plains, into the deepest craters, and over the highest opposing ridges. When the sun rises on Tycho these streaks are invisible, but as soon as it has reached a height of 25 deg. to 30 deg. above the horizon, the rays emerge from their obscurity, and gradually increase in brightness until full moon, when they become the most conspicuous objects on her surface. As yet no satisfactory explanation has been given of the origin of these illuminated rays,[10] but I may be permitted to add that their form and mode of occurrence are eminently suggestive of gaseous exhalations from the volcano illumined by the sun's rays; and owing to the absence of an atmosphere, spreading themselves out in all directions and becoming more and more attenuated until they cease to be visible. The above account will probably suffice to give the reader a general idea of the features and inferential structure of the moon's surface. That she was once a molten mass is inferred from her globular form; but, according to G. F. Chambers, the most delicate measurements indicate no compression at the poles.[11] That her surface has cooled and become rigid is also a necessary inference; though Sir J. Herschel considered that the surface still retains a temperature _possibly_ exceeding that of boiling water.[12] However this may be, it is pretty certain that whatever changes may occur upon her surface are not due to present volcanic action, all evidence of such action being admittedly absent. If, when the earth and moo
PREV.   NEXT  
|<   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   >>  



Top keywords:

surface

 

diameter

 

height

 

streaks

 

craters

 

volcanic

 
directions
 
deepest
 

action

 

account


visible

 

permitted

 

reader

 

general

 

suffice

 

occurrence

 

gaseous

 

suggestive

 

exhalations

 
volcano

illumined

 

illuminated

 

absence

 

attenuated

 

origin

 

atmosphere

 

eminently

 

spreading

 
boiling
 

However


pretty

 

exceeding

 

possibly

 

considered

 

retains

 
temperature
 

admittedly

 

absent

 

evidence

 

present


Herschel

 
globular
 

inferred

 

Chambers

 

molten

 

structure

 
inferential
 

delicate

 

measurements

 
inference