RESISTING MEDIUM. 39 



etars,* and from his ingenious experiments on the space-pen- 

 etrating power of his great telescopes, seem to show, that if 

 the light of Sirius in its passage to us through a gaseous or 

 ethereal fluid loses only 7 £ 7 tb of its intensity, this assump- 

 tion, which gives the amount of the density of a fluid capa- 

 ble of diminishing light, would suffice to explain the phe- 

 nomena as they manifest themselves. Among the doubts 

 advanced by the celebrated author of " The New Outlines 

 of Astronomy' * against the views of Olbers and Struve, one 

 of the most important is that his twenty-feet telescope shows, 

 throughout the greater portion of the Milky "Way in both hem- 

 ispheres, the smallest stars projected on a black ground. f 



A better proof, and one based, as we have already stated, 

 upon direct observation of the existence of a resisting fluid, :j 

 is afforded by Encke's comet, and by the ingenious and im> 

 portant conclusion to which my friend was led in his observ- 

 ations on this body. This resisting medium must, however, 

 be regarded as different from the all-penetrating light-ether, 

 because the former is only capable of offering resistance in- 

 asmuch as it can not penetrate through solid matter. These 

 observations require the assumption of a tangential force to 

 explain the diminished period of revolution (the diminished 

 major axis of the ellipse), and this is most directly afforded 

 by the hypothesis of a resisting fluid. § The greatest action 



* Cosmos, vol. i., p. 86, 87. 



t " Throughout by far the larger portion of the extent of the Milky 

 Way in both hemisphei'es, the general blackness of the ground of the 

 heavens, on which its stars are projected .... In those regions where 

 the zone is clearly resolved into stars, well separated, and seen projected 

 on a black ground, and where we look out beyond them into space. . . ." 

 — Sir John Herschel, Outlines of Astr., p. 537, 539. 



\ Cosmos, vol. i., p. 85, 86, 107 ; compare also Laplace, Essai Philos- 

 ophique sur les Probability, 1825, p. 133 ; Arago, in the Annuaire du 

 Bureau des Long, pour 1832, p. 188, pour 1836, p. 216; and Sir John 

 Herschel, Outlines of Astr., § 577. 



§ The oscillatory movement of the emanations from the head of some 

 comets, as jn that of 1744, and in Halley's, as observed by Bessel, be- 

 tween the 12th and 22d of October, 1835 (Schumacher, Astron. Nachr., 

 Nos. 300, 302, $ 185, 232), "may indeed, in the case of some individ- 

 uals of this class of cosmical bodies, exert an influence on the transla- 

 tory and rotatory motion, and lead us to infer the action of polar force3 

 (§ 201, 229), which differ from the ordinary attracting force of the sun ;" 

 but the regular acceleration observable for sixty -three years in Encke's 

 comet (whose period of revolution is 3^ years), can not be regarded as 

 the result of incidental emanations. Compare, on this cosmically im- 

 portant subject, Bessel, in Schum., Astron. Nachr., No. 289, s. 6, and 

 No. 310, s. 345-350, with Encke's Treatise on the hypothesis of the re« 

 sisting medium, in Schum., No. 305, s. 265-274 



