FREE BOOKS

Author's List




PREV.   NEXT  
|<   167   168   169   170   171   172   173   174   175   176   177   178   179   180   181   182   183   184   185   186   187   188   189   190   191  
192   193   194   195   196   197   198   199   200   201   202   203   204   205   206   207   208   209   210   211   212   213   214   215   216   >>   >|  
geographer; while its rocks and their contents, its volcanoes and its earthquakes, are to be studied by the geologists and the physicists. CHAPTER X. MARS. Our nearer Neighbours in the Heavens--Surface of Mars can be Examined in the Telescope--Remarkable Orbit of Mars--Resemblance of Mars to a Star--Meaning of Opposition--The Eccentricity of the Orbit of Mars--Different Oppositions of Mars--Apparent Movements of the Planet--Effect of the Earth's Movement--Measurement of the Distance of Mars--Theoretical Investigation of the Sun's Distance--Drawings of the Planet--Is there Snow on Mars?--The Rotation of the Planet--Gravitation on Mars--Has Mars any Satellites?--Prof. Asaph Hall's great Discovery--The Revolutions of the Satellites--Deimos and Phobos--"Gulliver's Travels." The special relation in which we stand to one planet of our system has necessitated a somewhat different treatment of that globe from the treatment appropriate to the others. We discussed Mercury and Venus as distant objects known chiefly by telescopic research, and by calculations of which astronomical observations were the foundation. Our knowledge of the earth is of a different character, and attained in a different way. Yet it was necessary for symmetry that we should discuss the earth after the planet Venus, in order to give to the earth its true position in the solar system. But now that the earth has been passed in our outward progress from the sun, we come to the planet Mars; and here again we resume, though in a somewhat modified form, the methods that were appropriate to Venus and to Mercury. Venus and Mars have, from one point of view, quite peculiar claims on our attention. They are our nearest planetary neighbours, on either side. We may naturally expect to learn more of them than of the other planets farther off. In the case of Venus, however, this anticipation can hardly be realised, for, as we have already pointed out, its dense atmosphere prevents us from making a satisfactory telescopic examination. When we turn to our other planetary neighbour, Mars, we are enabled to learn a good deal with regard to his appearance. Indeed, with the exception of the moon, we are better acquainted with the details of the surface of Mars than with those of any other celestial body. This beautiful planet offers many features for consideration besides those presented by its physical str
PREV.   NEXT  
|<   167   168   169   170   171   172   173   174   175   176   177   178   179   180   181   182   183   184   185   186   187   188   189   190   191  
192   193   194   195   196   197   198   199   200   201   202   203   204   205   206   207   208   209   210   211   212   213   214   215   216   >>   >|  



Top keywords:

planet

 

Planet

 

Distance

 

Satellites

 

treatment

 

planetary

 

telescopic

 

Mercury

 
system
 
nearest

features

 

attention

 
peculiar
 

claims

 

neighbours

 

consideration

 

offers

 
celestial
 

beautiful

 
progress

outward

 
passed
 

physical

 

presented

 

methods

 

resume

 

modified

 

details

 

pointed

 

realised


anticipation
 

atmosphere

 
neighbour
 

examination

 

satisfactory

 

making

 

prevents

 

enabled

 

exception

 

expect


Indeed

 

naturally

 

acquainted

 

appearance

 

farther

 

planets

 
regard
 

surface

 

observations

 

Apparent