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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nus in gr. </
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<
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">18. </
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<
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xml:space
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">♓, hoc eſt 2{1/2} gr. </
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<
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xml:space
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">à loco æquinoctii, quæ di-
<
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ſtantia dat declinationem gr. </
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<
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xml:space
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">unius.</
s
>
<
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xml:id
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xml:space
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</
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<
s
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xml:space
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">Ut igitur ſecundum hæc de rotunda phaſi judicium ſera-
<
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xml:space
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">Saturnus
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brachiorum
<
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expers futu-
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rus quo mo-
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do cognoſca-
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tur.</
note
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tur, illud in primis reſpicere oportet, quod gradibus ab æ-
<
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quinoctio ſuo, hoc eſt, à gr. </
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<
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xml:space
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">20{1/2}. </
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<
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xml:space
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">♍ vel ♓, Saturni locus ec-
<
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centricus abſit. </
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<
s
xml:id
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xml:space
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">Ac mihi quidem phænomena antecedentia
<
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expendenti, videtur ita ſtatuendum, ut quoties non amplius
<
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/>
quam 6 gr. </
s
>
<
s
xml:id
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echoid-s6776
"
xml:space
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">circiter in alterutram partem, à dictis locis Sa-
<
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turni locus ex Sole diſtabit, nunquam brachia ejus conſpici
<
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queant, quicunque demum oculi noſtri ſitus fuerit; </
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<
s
xml:id
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xml:space
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">hoc eſt,
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nulla ducta ratione Saturni loci apparentis. </
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<
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xml:space
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">Quod tamen
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ita accipiendum eſt, ſi perſpicillis non melioribus quam qui-
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bus Galilæus & </
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>
<
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xml:space
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">Gaſſendus uſi ſunt Saturnus inſpiciatur. </
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>
<
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xml:id
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xml:space
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">Nam
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ſi noſtris ſimilia adhibeantur, forſitan jam in illa 6 graduum
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diſtantia tenue quoddam brachiorum exordium percipi poſ-
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ſit. </
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>
<
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xml:space
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">Certè anno 1656, 13. </
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<
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">Oct. </
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<
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xml:space
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">renata illa vidimus, cum
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Saturni locus ex Sole tantum gradibus 6. </
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<
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xml:space
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">æquinoctii ſui
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punctum prætergreſſus eſſet. </
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<
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xml:space
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">Erant autem æquè conſpicua
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ferè atque ante phaſin rotundam, anno 1655. </
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<
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xml:space
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noribus teleſcopiis eum tunc obſervitabant, ut Joh. </
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<
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xml:space
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">Hodier-
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na, penè adhuc rotundum repererunt: </
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>
<
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xml:id
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xml:space
="
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">ait enim is, tantum
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tenuiſſimos quoſdam veluti radios utrinque è lateribus Sa-
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turnum vibrare viſum. </
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>
<
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xml:space
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">Quamobrem noſtris teleſcopiis for-
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taſſe arctiores paulò prædicti limites ſumendi ſint; </
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<
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xml:space
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">quod ta-
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men minimum quid erit, ſequentiumque annorum expe-
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rientiâ definiendum.</
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<
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</
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<
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<
s
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xml:space
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">Rurſus cum amplius 9. </
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<
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">gr. </
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<
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xml:space
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lum, ab æquinoctiis ſuis ſive 20{1/2} gr. </
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<
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xml:space
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">♍ aut ♓ locus Saturni
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eccentricus diſtare invenietur, jam inde brachiis anſiſve præ-
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ditum dicemus: </
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>
<
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">nullâ ne hic quidem apparentis loci conſi-
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deratione, quoniam hinc jam apparens locus & </
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<
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">eccentricus
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ab eadem parte loci æquinoctialis habentur; </
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xml:space
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">ac propterea ea-
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dem annuli ſuperficies, per ea quæ ſupra demonſtrata ſunt,
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Soli & </
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>
<
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xml:space
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">viſui noſtro obverſa eſt, idque ita ut Sol plus tribus
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gr. </
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>
<
s
xml:id
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xml:space
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">ſupra ipſam elevatus ſit, viſus vero noſter ut minimum
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gr. </
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<
s
xml:id
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xml:space
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">uno: </
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>
<
s
xml:id
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xml:space
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">quo fit ut brachia ſaltem tenuia animadverti de-
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beant.</
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