FREE BOOKS

Author's List




PREV.   NEXT  
|<   106   107   108   109   110   111   112   113   114   115   116   117   118   119   120   121   122   123   124   125   126   127   128   129   130  
131   132   133   134   135   136   137   138   139   140   141   142   143   144   145   146   147   148   149   150   151   152   153   154   155   >>   >|  
_, t. i., p. 107. He interposed, but tentatively only, another similar body between Mercury and Venus.] [Footnote 196: _Allgemeine Naturgeschichte_ (ed. 1798), pp. 118, 119.] [Footnote 197: _Cosmologische Briefe_, No. 1 (quoted by Von Zach, _Monat. Corr._, vol. iii., p. 592).] [Footnote 198: Second ed., p. 7. See Bode, _Von dem neuen Hauptplaneten_, p. 43, _note_.] [Footnote 199: The representative numbers are obtained by adding 1 to the following series (irregular, it will be observed, in its first member, which should be 1/2 instead of 0); 0, 3, 6, 12, 24, 48, etc. The formula is a purely empirical one, and is, moreover, completely at fault as regards the distance of Neptune.] [Footnote 200: _Monat. Corr._, vol. iii., p. 596.] [Footnote 201: Wolf, _Geschichte der Astronomie_, p. 648.] [Footnote 202: Such reversals of direction in the apparent movements of the planets are a consequence of the earth's revolution in its orbit.] [Footnote 203: _Dissertatio Philosophica de Orbitis Planetarum_, 1801. See Wolf, _Gesch. d. Astr._, p. 685.] [Footnote 204: Observations on Uranus, as a supposed fixed star, went back to 1690.] [Footnote 205: He had caught a glimpse of it on December 7, but was prevented by bad weather from verifying his suspicion. _Monat. Corr._, vol. v., p. 171.] [Footnote 206: Planetary fragments, hurled _in any direction_, and _with any velocity_ short of that which would for ever release them from the solar sway, would continue to describe elliptic orbits round the sun, all passing through the scene of the explosion, and thus possessing a common line of intersection.] [Footnote 207: _Phil. Trans._, vol. xcii., part ii., p. 228.] [Footnote 208: _Ibid._, p. 218. In a letter to Von Zach of June 24, 1802, he speaks of Pallas as "almost incredibly small," and makes it only seventy English miles in diameter. _Monat. Corr._, vol. vi., pp. 89, 90.] [Footnote 209: Olbers, _Monat. Corr._, vol. vi., p. 88.] [Footnote 210: _Conn. d. Tems_ for 1814, p. 218.] [Footnote 211: _Popular Astronomy_, p. 327.] [Footnote 212: _Month. Not._, vol. vii., p. 299; vol. viii., p. 1.] [Footnote 213: _Ibid._, p. 146.] [Footnote 214: Airy, _Mem. R. A. S._, vol. xvi., p. 386.] [Footnote 215: See Newcomb's _Pop. Astr._, p. 359. The error of Uranus amounted, in 1844, to 2'; but even the tailor of Breslau, whose extraordinary powers of vision Humboldt commemorates (_Kosmos_, Bd. ii., p. 112), could
PREV.   NEXT  
|<   106   107   108   109   110   111   112   113   114   115   116   117   118   119   120   121   122   123   124   125   126   127   128   129   130  
131   132   133   134   135   136   137   138   139   140   141   142   143   144   145   146   147   148   149   150   151   152   153   154   155   >>   >|  



Top keywords:
Footnote
 

direction

 

Uranus

 

Pallas

 

speaks

 
letter
 
release
 

velocity

 

Planetary

 
fragments

hurled

 

continue

 
describe
 

explosion

 

possessing

 
common
 

orbits

 
elliptic
 

passing

 
intersection

Olbers

 

Newcomb

 

amounted

 
Humboldt
 
vision
 

commemorates

 

Kosmos

 
powers
 
extraordinary
 

tailor


Breslau

 
diameter
 

incredibly

 

seventy

 
English
 

Popular

 

Astronomy

 

Observations

 

adding

 
obtained

series

 
irregular
 

numbers

 

representative

 

Hauptplaneten

 

observed

 

formula

 

purely

 

empirical

 
member