1. PROGUBB IV 1*97. 



* in breadth, ll- |--r*IMr|K*> 



**l remark al 



it had a tr 



ublful If 



.o 11)11. h, ft- '!:.- linage Of 



fifth fwitdllti* WM meastr 



places agreeing with Mar' ell. 



ith 



lift* ilHrr- 

 ''rml ami poln 



:!..! .H51. 



The n|.|Min-iit diameter* generally 



; 



notion la 



Considerable areunu-r. The 

 400*1* ai. 



uotiaa to only half a second of an . 







>, Jupiter f%"fr 



it has i^rii I.-L Kven in IK H 



aay - eooH u at any 



been ohBnrcl at aitMhrr rHum it ai. ..ulr be a*- 



h ..- r '.'.. I- s aj '- ... - :--:. 



.nit an.l in coo*irable icmth 



cpni drtectloo there to 



i .;. i- aj W - ' '-' :- : 



iHirrnM-hrlll.. II: , - ' ^ 



iiaknl rye onlr. Always to the iodiac and 



. ii. wji ' . : 



.11 Januarv. IHII . 



n f riff i"ii:il \< .ir \-> i ) -I. an !: ! v l-- ~ n .r .'! 

 in the ncighttorlKMil of 



I another a.Miti. n t the long list 

 comets. It wn- 



1 >eo. 8, 1806. It hail a star- 



I 



th.- ink- .1 \. . I 1 .- -! m< :.'-. v i MI one par- 

 tr a close resemblance to those of t h.- 



nts of 

 both are ph^ed aide by aide for comparison : 



I Hjeara, 



being generally about to* in 



IT K 



odfaral band V .r h eitrnding from it 



h the morning and ereolnf iiiaraJ lighu 



ran, aa haa aUo Prof. Srarle. -f llananl r^lew 



nriianl ha* mrnllT deetrftud m 



.. tiii'til Journal." So. 408. May, 



{raranrr* a* follow*: - Wbeii 



<n in autumn it is unaccoaspejiied by A 



codiaral baml. but later, when it* right mctfAm 



in (^ 0. it beoomea elli|>li<-al and the band apprara 



to the aiirxee of the evening and mum* 



ingrodUcal li|>ht. There appear* a 1 m. 



an oecillation cast and wet of al.ut 1 . ith a 



tend* - leaa longitude than 180*. It im- 



.mi on any hrpotheato the caoae of 



this light < r n ral 



* them not r*, after much i 



follow i i 



of 

 that it is caused by refracted ai 



n the same manner as the red 



thrtM :trth's atiu.-p) 



Utween sunlight and dark 



a 



fractetl dowrn ui n the Moon and then feebly re* 

 rendering her visible, all boajrh 

 thr Krth- shadow. In tbu 



the Moon that to the reflector, but in the 

 dost that to 

 all 



-.*/ /.*f/7 / .This c- 



parabola, ai 



case of the OefMisrAeiii it t> 



can ever visit our system the ^N,H| time. It rle- the refl.t ti.r. that <>ur atin<-| 

 menu arr 



tied in the order of perihelion pass,, 



.tion. 146 H S4-9'; 

 distance Earth 



prrpiated with dust, to conceded by all 

 kronomeri That the light is alw.rs oppoaite the 

 - a significant point In favor of this hypothe- 

 sis. The subject is att racttof incraasvd attenrion, 

 and there to hope that the cause of this strange 



;l , (bond il tin LMi Otmrrnton h r. 



riMonJonaSa, 



- 1' 46" 29*. This to its terent h r. 

 since ita dtocm \rr.-t in iv.i. It is the 



nt of nil the snort-period comets and often 

 anafea deie^ion. thofn alwaji atrafM raj lfy 



Tt ti<dletto Attran M : ,, hi M a W9I 



..llU'h ill*rs|| tfa t|,,M !% 1. >, Imlohf 



hail previously suggested the probable 



it of I^xall. and re- 



quested astronomera to obtain aa long a seriea of 



elliptical elements with th* utmost accuracv. Those 



Uf it iToother po*f^nl n. equally 

 tnapttoAbli S ptriMfi h fi ' ' 



Oqfi****. to the Bodiaoal light, visible aa a broad 

 conical luminous beam to the west a? 

 during the autumn ami winter months and to the 

 .....'. . ,. . . .._..,... __ . ... | , , 



MII^BMI^IIII l*m.m nan lit ! Wjt^M lkt I K<. Iirt4<t { 



pecwvecope nas recenuy anown inai me iigni 



.n.;cf.- r. :'. -, ! '-. ::. : , tt . ' 



t rented, therefore, as a luminous ring 



eK.r1hin*te.lofUwSun. 

 I n IHcat Ion of Tine. ThetotofMtkoalunifica- 



o has been adopted in nearlv 1 

 try eept Framv. S ( in. an.l PortupU. En^and. 

 Belgium^ IMlJ.i. and Luxemburg we western 

 European time. Central time to adopted by Italy. 

 Hand. Germany. iK-nmark. Xorwav, and 

 Sweden. Knivia. Koumania. Bulgaria, and Euro- 



