Lexicon Technicum: Or, An Universal English Dictionary Of Arts And Sciences, fol. -
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- tiis Equinoctial Pares, and makes his Meridians
- much Llliprical, (0 25 ro be discernable by ine Tc.
- descope.
- The SunsHeac in Fupirer, is ac most noc abore
- one tvenes htch pare oF Wrhac ic is wich us; and
- consequenly vould bererr uncomtorrable lirin
- chere (iF ac all Portible) for _sen ot our Consticuri
- on: And ver some are very Cond of chinkins fupi
- ter an excellentplale tolire in.
- The Distance ot Fupiter rom the Sun, is abor
- sive rimes a5 greac a5 thar of the Farch From chc
- Sun, sec GrezoryS Astron. and consequenely che Dia
- meter oF che Sun co any Pyc in Fupiter, will bC
- noc a fitch part oE wrhac ic appears ro us, and chere.
- fore his Disse will BC abore 25 rimes lels, and in
- che Pame Proporrion ill his Listr and Lleat
- Be
- The Artificial Dar and Nighe (each OF S FTOurs,
- is oF che lame lenech in Fupiter, all over his Sur-
- tace; because the Axis ot his Diurnal Rerolurion
- is nearty at Righr Angles to che Plane oF his Annual
- Orbic Found etic Sun
- Alctio Fupicer hach a Primary Planers below him
- vet an Fye placed chere, and oF no Marper Sigh
- than one oF ours, could never behold any oneo
- ehem, untels 25 Spors transirins over the Suns Dist
- Wwhen They happeni ro he berveen che Torial Ry
- and che Sun: For Mars which soes Furthest oF aII
- Trom the Sun, will noc in Fupiter be seen above 18
- Degrees trom him; and since that Planer is BuE
- Emall, and reftects bur a weak Lishe, (0 near the
- Sun ic cannoc be visible: So chac Saturn IS FHC ON
- IV Planee chat can be seen in Fupiter, excepe tis
- Duon Four Noons or Sacellices.
- TheSuns Latanaa c super, willscarce
- be sensible any more than Sacurns; neither bein
- nuch abore 20 Seconds. So thatthe Suns appa.
- rent Diamerer in Fupiter, will noc be abore 6 MIi
- nutes. Bucche outermost ot his Sacallices will ap.
- pear almost as greac as the Moon doch to uS, viz
- OE sive rimes che Diamerer, and 25 cimes che Dist
- oF the Sun, seen From the lame Planet: And il chc
- orher Satellires are nor lels than che outermost, che.
- will vec appear much preater: (And che L earnec
- NII. Fruzens conceires them nor much tels than ou
- Farth) and sire che Planet a 800d Listie in che
- Nixtis, which allo can neret Me de ret
- 10n5.
- Indeed, it he can discover chac fapres morc
- round che sun, he inay be able (a5 CHC Voctor
- Aance oF Fuxiter and Satum from che Sun, octier-
- Wise nOL.
- Our Zovial Astronomer Theretore, By the helo ot
- his Senles onid distinguistr ew.s kinds oF Planees:
- Tour nearer ro him, Wvtich are che Sarellires, arit
- civo (25 che Sun and Saturn) IOrC RemOTe; aM
- chele lacrex vould appear irti a lesser Diamerer
- the Former wwich a preater. OF chie Remorest, the
- Sun vould appear in Diamerer abont siX Minures
- burche Diamieter oF Sacun voulel scarce be ; ot 2
- Minure.
- Fourth Woula appCat IO AN LSC IH FUPItCr, OL CHIC
- Bignels che MOOH aoh EO US: LHaL IS, WIIH a LI
- ameter sire rimes grCater, and a Disk RVenEy fIrC
- times preater chan che sun dorh chere. Besules
- ThC FOUT RCATeF, and ApparCHEIY SFCaTeK OBCS, WII
- be distinguia LIOMI CHC MOTC FCMIOLC AME SCMCI
- ones, in chis, chac in chenearer Planers che. Sguares
- oF che Periodick Pimes, are as the Cubes of cheir
- Distances From the Center oF Fupiter, Wvhich voue
- by no means be rrue, it any one oF che Greatet
- vere compared vich ans ese et Ie seller. Anc
- brighethen cher; For From cheir Faces, Wtrich de
- Pend upon hest Situacton, Wn Tespeet TotHe SuB
- ther wiis appeaL AIKC 1O MIaM MOOnS: FTOn
- OF Monchs, accordins 1o che NumbeF OF MOOIS.
- There will be contained abore 2407 oF che lent
- Monchs in a TCat, atu aWDuE hals the Number
- OF MOnHS HeNL 1O MesC; IC NUIDeE OL thC
- druple ot lhe tric, altet ene nees et lie fleale
- WilI be abouc 254. So thac altho che Noration ot
- Fime, bemuch more intricare in Tupiter, by Fez
- Con OF thC OrCaE NuHIDEL Ot DasS Wtich cheir
- YCar COntainS, vet IEIS much tacMCated DY There
- pere arc onty 4 DayS and a quarter, buc in elle
- TBCWS, Prop. 2.) co determine che Rario ot etie Di
- OF ThC FOUT ReATeF PIaNCIS, OF SALCHHLES, THC
- altho chenearer chele Planers are, ce) afeas eHe
- Breatet; VCL LHC SUN WII DC MCMCI MOC
- wohence a Speclaror in Fupiter will hareTOL RIHaS
- Monchs ot te chird SatelMe CONCaM a MH a LCaI
- vill be nearty subduple ot che second, or subqua
- tour Rinds oF Monts; tor eC sCal MOeh
- DE. Crecory, (Erom Whence ehis compatative
- AAtronomy is collected) Caith also, Thac an AArO.
- nomer placed in Fupiter, vould easily compare
- the Diltances of the four Inferior Planers vich che
- Drameters oF Fupiter, a5 we do ihe Distances oF
- us tom the Planers, br comparine chem wich che
- Diameter oF the Farth: And ehis vould be donc
- do lo che four nearest ones, calier chan we compure
- Jhe Distance oF the Moon by che Farths Diame.
- Ter: For che FTorizontal Parallax of the remores
- oF the Planers seen From Fupiter, is above twice 25
- Great a5 che Florizontal Parallax of the Moon Peer
- Trom the Farch; and cheretore must be very sensi-
- ble and considerable. And cho the Globe ot Fu-
- piter be raslr large, in comparison ot our Parch:
- vec the Suns Parallax, when hesbeheld trom Fu.
- piter, will noc be quire 20 Seconds, and conse-
- quently scarce sensible: Nor will che Parallax oE
- Saturn, (cho Wrhen in Oppolicion co che Sun, aud
- neXETO Fupicer) be much greater; and cheretore
- cwill be very disticule For che Zovial Astronomer 10
- Srealete lomechins more chen 40.
- Besides, chese Moons sutter an Eclixse when ches
- bestis in Opposition co che Sun, happen ro Fall inco
- ihe Strador ot Fupiter; and asan Wontent enes
- acede e secona Which deriares a liccle; upor
- thes decoune Llay cheir Pelipses are Ceneral, anc
- consequenr most lastins, wten the Sun is in one
- OF eHC Lodes ot thole MOOnS. Bur when the SMM
- is our ofchis Polirion, che Lcliples may be lotal,
- tho BOc C entral, because the BreadeM OF Zupiter
- Stradon, is nearts decuple che Breadrh of any ot
- the Sacellites, ard the apparene Diameter oF als
- OE chose MOOnS, is nearly quincuple the apparen
- Diamerer of theSun. Andchisremarkeable inequa
- lier of the Diameters, and che (malI Inclination che
- Plain oF the Orbits oF che Sacellires has co rhe Plaim
- estimare che Distance ot Saturn, or oF rhe Sun Erom os fuxiterS Orbirroundche Sun, is rherealon uhy
- in eaet te todnto 2 q e
- (beins in Conjunction wich che sun, project thei
- Wwhere ne Saco Tats fisen LLeston IS d ret
- Or makes an Anse seh fuptiets Orbir aboutche
- Stadous lo fupiter, etes tane a LCPIC OI enC
- Sun eo an Fye Placed in chac Region OE Zupiter.
- (maII ParE OE FupiterS Surtace) just as our HOOn
- does; bur because the Orbies oF thole MOOnS 2
- Bour Zupiter, are in a Plain which is enclined ro
- Sun, and are alI oF em nearts in che Tame Plain.
- CMaF P lalet.
Cite
Lexicon Technicum: Or, An Universal English Dictionary Of Arts And Sciences, fol. - . Machine transcription, not an edition: Leibniz Legible (model FoNDUE-GD_v2_ft_Leibniz, run 74). https://leibnizlegible.com/page/806933011:0455?run=74