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4. R.larivislic p.nub.rions (Lsrnd. & Chlpronl-Tou?J 1982).<br />

5- Penurb.tuG du. to tidd afccis (villim3.t. a! l97E).<br />

6. Molion of the efccnce frde conside&d wilh spect to m in€rrigl fime of<br />

consideradon ol all lhese pelturbarioB esuhs in<strong>lo</strong> rime series fomlla for geocentric<br />

<strong>lo</strong>ngitude, IatiMe .rd disra@ of 0E M@n at nds $e numh.r of lcm !o 15:37.<br />

An al€natc ro this ther€icrl appro&h is !o rcpr€*nl1hc coordinai.s explicilly<br />

6 tinc ledes fomule. This epEs.rolion of tlie tinc sed€s is dcr<strong>lo</strong>ped by Chap6n!<br />

Touzi ind Chapront (Chapront-Touu & Chaprcnq l9tl, pp. l0) und ha bcc. !*d in<br />

fiis work. The mjor fomula used in rhh vork due !o $es authob de lkrcd be<strong>lo</strong>Nl<br />

Tbe ge@entric <strong>lo</strong>ngitude<br />

'/h.xpesed<br />

as:<br />

'/=218.31665416+48126?.8813424'r-0,00011268'r:<br />

+0.000001856tr'<br />

0.0000000r534.r1+,5. +(s; +/ 1si +r' xsi/1oo0o)/l0oo<br />

(2.2.t)<br />

wh€rc<br />

I = h in iulian centuies sinceJ2000.0<br />

s, =tv,sr,(dj') +d|),,+ao *r' xro I +ao)'/r xr0' +d|,.rr xro r)<br />

I = )':st(o;'' -a:"' '4<br />

(2.2.21<br />

(2 2.r\<br />

si = tv;,s,,(d;,o + dnD.r) (2.2 4)

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