218 



INDEX. 



/^i-nerical rcctilta exceeding the grasp 

 of the comprehension, funiiahcd alike 

 by the minutest oi-ganisms and the so- 

 called fixed stars, 30 ; encouraging views 

 on the subject, 31. 



<)ptical and physical double stars, 200; 

 often confounded, 200. 



Oi bits of double stars, calculation of the, 

 211; theix great eccentricity, 211; hy- 

 pothesis, that the brighter of the two 

 stars is at rest, and its companion re- 

 volves about it, probably correct, and a 

 great epoch in cosmical knowledge, 212. 



Orion, the sis stars of the trapezium of 

 tlie nebula of, probably subject to pe- 

 culiar physical attraction, 210, 211. 



PantschatS or Pantschatra, the Indian the- 

 ory of the five elements, 31. 



Parallax, means of discovering the, point- 

 ed out by Galileo, 188 ; number of par- 

 allaxes hitherto discovered, 190 ; detail 

 of nine of the best ascertained, 190. 



Penetrating power of the telescope, 145, 

 146. 



Periodically changeable stars, 164. 



Periods within periods of variable stars, 

 168 ; Argelander on, 168. 



Peru, climate of, unfavorable to astronom- 

 ical observations, 10.'3. 



Peters on parallax, 192. 



Photometric relations of selflurainous 

 bodies, 89 ; scale, 99. 



Photometry yet in its infancy, 94 ; first 

 numerical scale of, 94 ; Arago's meth- 

 od, 96. 



Plato on ultimate principles, 12, 13. 



Pleiades, one of the, invisible to the naked 

 eye of ordinary visual power, 48 ; de- 

 scribed, 141, 



Pliny estimates the number of stars vis- 

 ible in Italy at only 1600, 108. 



Poisson, his view of the consolidation of 

 the earth's strata, 36, 37. 



Polarization of light, 45, 47. 



Poles of greatest cold, 36. 



Pouillet's estimate of the temperature of 

 space, 36. 



Prismatic spectra, 44 ; difference of the 

 dark lines of, 45. 



Ptolemy, his classification of the stairs, 

 90; southern constellationB known to, 

 137. 



Pulkowa, number of multiple stars dis- 

 covered at, 205, 20f). 



Pythacroreans, mathematical symbolism 

 of the, 12. 



Quaternary systems of stars, 210. 



vj Radiating heat, 35. 



Ratio of various colors among the mul- 

 tiple and double stars, 209. 



Rays of stars, 52, 126-128 ; number of, in- 

 dicate distances, 128 ; disappear when 

 the star id viewed through a very small 

 aperture, »28, 129. 



Red stjirs, 131 ; variable stars mostly red, 

 165 



Reflecting ><extants applied to the det€STT> 

 ination of the inten.sity of stellar ligh^ 



Reflecting and refracting telescopes. Si. 

 Regal stars of the ancients, 136. 

 Resisting medium, proved by obsenri- 



tions on Encke's and other comets, 'i% 

 Right ascension, distribution of stars »?• 



cording to, by Schwinck, 140. 

 Pdngs, colored, measurement of the in* 



tensity of light by, 96. 

 Rings, concentric, of stars, the hypothppJa 



of, favored by the most recent obaen'v 



tions, 149. 

 Rosse's, Lord, his great telescope, 65 ; iU 



serrices to astronomy, 66. 

 Ruby-colored stars, 135. 



Saint Gall, the monk of, observed a ncrr 

 star distant from the MiUsy Way, 162. 



Saussure asserts that stars may be seen 

 in daylight on the Alps, 57 ; the asser- 

 tion not supported by other travelers' 

 experience, 58. 



Savary, on the application of the aberra- 

 tion of light to the determination of the 

 parallaxes, 194 ; an early calculator of 

 the orbits of double stars, 211. 



Schlegel, A. W. von, probably mistaken 

 as to the high antiquity of the Indiaa 

 zodiacs, 121. 



Schwinck, distribution of the fixed stara 

 in his " Mappa coelestis," 140. 



Scintillation of the stars, 73 ; variations 

 in its intensity, 76 ; mentioned in the 

 Chinese records, 77 ; httle observed in 

 tropical regions, 77, 78 ; always accom- 

 panied by a change of color, 202. 



Seidel, his attempt to determine the quan- 

 tities of light of certain stars of the firat 

 ma^^itude, 93. 



Selfluminous cosmical bodies, or suns, 

 199. 



Seneca, on discovering new planets, 23 



Simplidus, the Eclectic, contrasts the cen- 

 tripetal and centrifugal forces, 12 ; hia 

 vague view of gravitation, 18. 



Sirius, its absolute intensity of light, 95, 

 historically proved to have changed ita 

 color, 131 ; its association with the ear- 

 liest development of civilization in the 

 valley of the Nile, 133 ; etymological re- 

 searches concerning, 133, 134. 



Smyth, Capt. W. H., calculations of tho 

 orbits of double stars by, 211. 



Smyth, Piazzi, on the Milky Way, 146, 

 147 ; on a Centauri, 185. 



Sotliis, the Egyptian name of Sirius, 133, 

 134. 



South, Sir James, observation of 380 dou- 

 ble stars by, in conjunction with Sir 

 John Herschel, 205. 



Southern constellations known to Ptol« 

 emy, 137. 



Southern Cross, formerly visible on the 

 shores of the Baltic, 138. 



Southern hemisphere, in parts remark- 

 ably deficient in constellations, 112; dis- 

 tances of its stars, first measured about 

 the end of the sixteenth century, 138 



