FREE BOOKS

Author's List




PREV.   NEXT  
|<   147   148   149   150   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   180   181   182   183   184   185   186   187   188   189   190   191   192   193   194   195   196   >>   >|  
very peculiar. Deimos, being only 10 miles in diameter and about 12,500 miles from the surface of the planet, does not give rise to so many phenomena as the nearer satellite: still they are very numerous. It revolves round the planet in 30-1/4 hours, but appears to take 131-1/2 hours to do so, being above the horizon about 60 hours, and below it nearly 72 hours. These are the times as seen from the equator; but, as in the case of Phobos, the farther the place is from the equator the shorter is the period that Deimos is seen above the horizon, until, when latitude 82 deg. is reached in either hemisphere, it ceases to become visible at all. Our moon, being so very much more distant from our earth, could be seen from both the poles. Deimos also passes nearly twice through all its phases whilst it is above the horizon, viz. during about 60 hours, and may be seen twice full and twice new in that time. Eclipses of Deimos by the planet and occultations of it by the other satellite are very frequent. Being so small, it can never cause an eclipse of the sun, but it transits the sun as a dark spot about one hundred and twenty times during the Martian year. This is really a very inadequate list of the phenomena connected with the satellites, but it will be seen that the number is enormous compared with the few eclipses of the sun or moon seen on the earth during the course of one year. Certainly Mars is an astronomer's world! Merna heard my statements respecting these movements and phenomena as I explained them to my two friends; and when I had finished, he remarked, "You seem to be fairly well posted in these matters, sir?" "Yes," I said; "thanks to our astronomers, both professional and amateur, all these things have been very carefully calculated; and, with the exception of a few doubtful points, we probably know nearly as much about them as the Martians themselves do." M'Allister then turned to me and said, "Professor, you told us that the two satellites of Mars revolved round the planet in a certain time, but in each case you afterwards said they appeared to take a much longer time to do so. I'm rather puzzled to understand how that can be." "It's really a simple matter, M'Allister," I answered, "and I think I can make it clear to you. While the satellite is making one revolution round the planet the latter is turning on its axis in the same direction as the satellite is moving, following it up in fact;
PREV.   NEXT  
|<   147   148   149   150   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   180   181   182   183   184   185   186   187   188   189   190   191   192   193   194   195   196   >>   >|  



Top keywords:

planet

 

Deimos

 
satellite
 

horizon

 

phenomena

 
Allister
 

satellites

 
equator
 
friends
 

astronomers


explained
 

amateur

 

professional

 

statements

 

fairly

 

respecting

 

movements

 

remarked

 

matters

 
posted

finished
 

things

 

Professor

 
answered
 
matter
 

simple

 

puzzled

 
understand
 

making

 

moving


direction
 

revolution

 

turning

 
longer
 

Martians

 

points

 

doubtful

 

carefully

 

calculated

 
exception

appeared

 
revolved
 

turned

 
shorter
 
period
 

farther

 
Phobos
 

latitude

 

visible

 
ceases