Huygens, Christiaan
,
Christiani Hugenii opera varia; Bd. 2: Opera geometrica. Opera astronomica. Varia de optica
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SYSTEMA SATURNIUM.
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ris ipſius Saturni ante vel pone comitem objectu. </
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que obſervationes anni 1655 & </
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quam maximè compreſſa brachia erant, oſtendunt comitem
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etiam in ea recta tunc perpetuo apparuiſſe quæ per utrum-
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que illorum extendebatur.</
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<
s
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xml:space
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">Et hac quidem in re diſſidet Saturniæ Lunæ curſus ab eo
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qui in noſtrate Luna animadvertitur; </
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<
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quatoris noſtri ſed magis eclipticæ plano obnoxia eſt, à quo
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quinque tantummodo partibus exorbitat.</
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<
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anſarum @@-
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titudo ſenſim
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contrah@uc.
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TAB. L.
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fig. 2.</
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vel I, vel ex adverſo ad O vel P, paulo anguſtiorem jam
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annuli ellipſin, eadem tamen qua prius longitudine nobis
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aſpici oportet, quum ſupra planum annuli minus altè hoc
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ſitu viſus noſter efferatur. </
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in tabellæ LII. </
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perſpicere valentibus, ea quæ ſexta eſt efficietur.</
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loca hiſce oppoſita N & </
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minorem ellipſis diametrum, quippe magis ex obliquo in-
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ſpectam. </
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anno 1658 obſervavimus (T. </
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nis teleſcopiis excepta degeneravit in illam quæ quinta in ta-
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bella LII. </
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patulæ vide-
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ri anſæ de-
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ſinant.</
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loco Saturnus remotus invenitur, velut in Q & </
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& </
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<
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rima ſuperſit viſui pervia, ea tamen propter exilitatem & </
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liqui corporis ſplendorem conſpici nequeat; </
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turni forma ejuſmodi appareat qualem anno 1655 & </
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nos ſpectaſſe ſupra meminimus (T. </
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quæ quomodo aliis omnibus hactenus teleſcopiorum culpâ
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triſphærica exiſtimata ſit, antea quoque oſtenſum eſt.</
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<
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priuſquam tranſeam, de inclinatione magnæ Saturni diame-
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tri, ſive anſarum lineæ, ut ſupra eam vocavi, pauca adno-
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tanda ſunt.</
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