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( 4 11 )'

An.l6jj. Sept. ij 8h <)' 4o // . at Grcentvich, Mr. Flamßeed observed ths>Eirst Satellite to begin to Emerge ; that is 8* 1 ()' x6" . at London.

d.

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N. I.

N. II.

1677.

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102, y

Sept.

17

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4 JZ

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147, 7

Sept.

7

18 48

ziyy

248, 0

/Equat. I.

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3

/Equat. 2.

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S - 37

x 73

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1 3y

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Sunimora

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2-4' 9

Eejual Time

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Apparent T.

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Error

I 21

An Immersion of this Satellite bemg computed aster the fame rnannef^ac* -cording to thde Tables, ought to have happen’d. /hi. HiSg. Nov. go.i6 h 5 ‘tJ 7/'. but I observed it at- 16 lx 48^ 40" to that the Error was»-

— i si'■

Again, M. Casini ofeserv’d an Emerson at Paris. An. 169g. Jan. 14^"' 10^**

40^ 28'' that ir, at London i e E go/ 4 5 ". Which- thde Tablesgive at ioh^go 7 59V. and -tbereforo the Error was no more.than -+■ 9//.

After this mannet I have compared thde Tables wich many goed and cer--tain Obfervations» and searce ever find them Err above g or 4 Minutos of;

Time; which Errors are exceeding finali in compari ton of. the ftiorc Time-thac’the Satellites have been di/covered.

In the Constrpction os the Tab!e, which shews the.H.;li Continuance, of/thefe Eclipses , the Semidiameter öf the Shadow of Jupiter is made by Casinijust 10 Deg, and. that of the Satellite gc/; and the Satellite’s Ajcending Node,-being luppofed in 1 y° of Aquarius , : at the End of this Century, ( that is-y y°

2:c/ before tlie Pcribclion ot Jupiter ) it will thence follow, that Nam. I. be—ing 116, or 7 . 102 , Jupiter pafies the Nodes of the Satellites Orb» and conte-'quently thde Eclipses ■ are Central, and of the.Greatest Duration. ButNum. I. being 2. 1 y, or 1481, the Satellite pafles the Shadow with the Crea- •test Obliquity,,vjy. z 0, y.y' frorn the Center, whcnce the S animor a becomesof,all the {hortest.

3. The Tables of the other g Satellites not being tb perfect or exact as of tbevthtr 5.thole of the. First, are here given insanother. Form. Tne Pericds ot-their Satellites.Revolutions to Jupiter s Shade areas follows.. 1 '