Newton, Isaac
,
Philosophia naturalis principia mathematica
,
1713
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lis (1/(4 7/8))
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AE,
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ſeu (1/39)
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AE
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quamproxime. </
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<
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>A perpendiculo autem a
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ſtella
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A
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ad rectam
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PE
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demiſſo, diſtantia Cometæ erat 4/5
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PE.
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LIBER
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TERTIUS.</
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<
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is
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,
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Feb.
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27. hor. </
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<
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>8 1/4 P.M. </
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<
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>Cometæ in
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Q
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exiſtentis di
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ſtantia a ſtella
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O
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æquabat diſtantiam ſtellarum
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O
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&
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H,
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& recta
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<
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QO
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producta tranſibat inter ſtellas
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K
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&
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B.
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Poſitionem hujus
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rectæ ob nubes intervenientes, magis accurate definire non potui. </
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<
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>Die
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tis
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,
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Mart
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1, hor. </
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<
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>11. P.M. </
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<
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>Cometa in
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R
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exiſtens, ſtellis
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<
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K
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&
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C
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accurate interjacebat, & rectæ
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CRK
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pars
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CR
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paulo
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major erat quam 1/3
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CK,
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& paulo minor quam 1/3
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CK
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+1/8
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CR,
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adeoque æqualis 1/3
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CK
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+(1/16)
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CR
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ſeu (16/45)
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CK.
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<
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ii
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,
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Mart.
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2. hor. </
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<
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>8. P.M. </
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<
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>Cometæ exiſtentis in
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S,
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di
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ſtantia a ſtella
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C
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erat 4/9
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FC
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quamproxime. </
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<
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>Diſtantia ſtellæ
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F
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a
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recta
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CS
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producta erat (1/24)
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FC
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; & diſtantia ſtellæ
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B
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ab eadem recta,
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erat quintuplo major quam diſtantia ſtellæ
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F.
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Item recta
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NS
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producta tranſibat inter ſtellas
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H
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&
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I,
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quintuplo vel ſextuplo pro
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pior exiſtens ſtellæ
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H
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quam ſtellæ
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I.
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<
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>Die
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ni
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,
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Mart.
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5. hor. </
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>11 1/2. P. M. </
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<
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>Cometa exiſtente in
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T,
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recta
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MT
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æqualis erat 1/2
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ML,
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& recta
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LT
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producta tranſibat
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inter
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B
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&
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F,
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quadruplo vel quintuplo propior
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F
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quam
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B,
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au
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ferens a
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BF
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quintam vel ſextam ejus partem verſus
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F.
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Et
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MT
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<
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producta tranſibat extra ſpatium
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BF
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ad partes ſtellæ
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B,
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quadru
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plo propior exiſtens ſtellæ
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B
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quam ſtellæ
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F.
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Erat
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M
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ſtella pere
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xigua quæ per Teleſcopium videri vix potuit, &
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L
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ſtella major
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quaſi magnitudinis octavæ. </
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<
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>Ex hujuſmodi obſervationibus per conſtructiones figurarum &
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computationes (poſito quod ſtellarum
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A
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&
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B
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diſtantia eſſet
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2
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gr.
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6′. </
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<
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>46″, & ſtellæ
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A
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longitudo 26
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gr.
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41′. </
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<
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>50″ & latitudo
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borealis 12
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gr.
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8′ 1/2, ſtellæque
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B
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longitudo 28
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gr.
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40′. </
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>
<
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>24″ & lati
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tudo borealis 11
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gr.
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(17′ 9/10);) derivabam longitudines & latitudines
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Cometæ. </
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<
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>Micrometro parum affabre conſtructo uſus ſum, ſed
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longitudinum tamen & latitudinum errores (quatenus ab ob
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ſervationibus noſtris oriantur) dimidium minuti unius primi vix
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ſuperant, præterquam in obſervatione ultima
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Mart.
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9. ubi poſi
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tiones ſtellarum minus accurate determinare potui.
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Caſſinus
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qui
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aſcenſionem rectam Cometæ eodem tempore obſervavit, decli
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nationem ejus tanquam invariatam manentem parum diligenter
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definivit. </
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<
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>Nam Cometa (juxta obſervationes noſtras) in fine </
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