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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<
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xml:space
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præcederet omnes obſervationes noſtras, conſtitui diem
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1 Jan. </
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<
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xml:space
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">meridie, anno 1653. </
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<
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xml:space
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Martii, 1659, hora 8 pom. </
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<
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xml:space
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">in perigæo Saturni Luna
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verſaretur, collegi retrorſum numerando, ad prædictam
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diem 1 Jan. </
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<
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">1653, abfuiſſe illam ab apogæi loco gr.
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xml:space
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">Locus Lun@
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Saturniæ
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quomod@
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ſupputetur@.</
note
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274, 21′. </
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pocha poſterius, inveniatur ejus ab apogæo diſtantia,
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(namque hinc facile deinde perſpicere eſt quam pro-
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pinqua Saturno apparitura ſit) addendus eſt ad mo-
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tum Epochæ, motus comitis uſque ad tempus datum,
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ex tabulis collectus; </
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<
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">hinc auferendus Saturni motus
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apparens per idem temporis intervallum, qui ex Ephe-
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meridibus cognoſcitur; </
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<
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ab apogæo quæſita. </
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<
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25 Martii, anno 1655, hora 8 pom. </
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ſtra fuit obſervatio: </
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næ Saturniæ ab apogæo tempore Epochæ, quæ eſt
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gr. </
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">274, 21′, addita ad motum ejuſdem Lunæ inde ab
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Epocha ad tempus datum, colligit gr. </
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ablato Saturni motu apparente per idem tempus, qui
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invenitur gr. </
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tia Lunæ Saturni ab apogæo, quæ invenienda erat.
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locum referebat, fere ad numerum 12 illam conſtitiſſe,
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eoque in maxima propemodum diſtantia viſam, uti re-
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vera contigit. </
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dinatur.</
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