| Show in iiii nun i j biby I 1 wm 0 affa ff a syr 1 r go 19 ji J 44 tae y per af 4 p prows body at iak 4 san the alk embr I 1 dival Div 4 R aby the periodic Por iodie time and the cab 21 will be the r require velocity 0 second 1 7 I 7 I 1 EX EXAMPLE AMPLE I 1 wafa the k 00 0 earth carlli at its mean distance ja period I 1 meau mean solar days I 1 I 1 I 1 4 WV I 1 1 I 1 I 1 t V evaa am 10 per P second EXAMPLE 2 L whit W afie of mercury q mt at its istance its being 87 1 w aids kyp 1 I i t 1 hf I 0 I 1 1 I 1 r I 1 M r I 1 1 1 I 1 I 1 i t 1 5 t 1 1 T 8 0 ec ond 4 T 3 i r roie 1111 I 1 t if I 1 I 1 ifil u d ih bis twice 1 41 of a planetary body I 1 from the 8 u s u I 1 ay hen boly velocity Velo cily y per er secondi second 1 I 1 ii given i 4 D divia 1 14 1 aj w by th q I 1 t w oy ol of bp I 1 V velo alo I 1 city 1 abick I afi 4 dt r w wk be e atlie h I 1 e I 1 n I 1 disa I 1 a I 1 in 11 ml milf 1 I fak I 1 I 1 E ra P L P I 1 4 t 1 the M win distance n ce of t the he E vr 11 J 1 I tieta I 1 t W its ferocity Ve rocity at that dis 1 talice being behig mv miles iles por per si second I 1 I 1 it air r I 1 r tar 1 j i 2 i T r JaW i hp I 1 I 1 I 1 I 1 s EXA whit DI df 4 the pl pt aitel 4 iP i ibe sun its velocity vel oel tv at thit that ai distance beino 30 1 e it per 1 second ig r t I 1 ka i I 1 v 1 I 1 T r I 1 II I 1 1 li 2 1 I 1 1 I ault TV IV it p 1 1 x II 11 1 I 1 ill J I 1 i 1 I ri to fi find ald the Velocity per a plane twy 1 body alien kiil oivi tg mean D caf is given I 1 by bap gean lean di distance a twice and the a quo go k 4 j hp e tile the I 1 velocity per second EXAMPLE D 1 I 1 Vel velocity oaty parea perk I 1 0 o nd of ite aarti atthe mean distance instance of 95 miles 1 iati i I 1 ft fi f v i r 1 1 93 4 1 I 1 leg per second I 1 2 what is the Volo velocity rity per ajic 1 I ond of the planet et mercury bep mep at the mean distance of play iles A t L 1101 1 I 1 0 I 1 I 1 I 1 if I 1 85 1 15 1 1 I 1 I 1 it a miles second K 7 8 1 per I 1 the constant nt quail titles days and 85 III fir the he fore golli ig arulas bitne periodic iwan d distance I 1 froma brorn the sun situ at which a planetary body would moe I 1 with thelva ity ty af 0 I 1 arvile er second I 1 I 1 i i iiii aie are A far T mt more ore I 1 a sl 1 I mple than any annj that hist I 1 have ever before seen it is hoppi hoped that their i publication in in your valuable paper will vill render es vent ting t t acir inquiries cone arning the laws and harj har hr j m 1 I P the y bodies i j tile like those 0 f epler do not irace brace tiie the ai from the dif j fereri of the tha massa af pf the several seral Pla pets liets but bui these masses twing j t of the aundo nn dp got no affect amat the co lution toady to any I 1 1 D i 1 I 1 1 airs ws anost PRATT son san G S L city ta 11 1854 |
