e
E
o
G
hiJ
a:ill/::f¡
",ill,~
giwn ;
lo
ftl/(l I·j¡ ¡IJce
in
:h:
,cíip–
t~c,
11·(
d.;
o[
I h(
monlh, od
"lile
tf
Ih" d! . Ihollgh
1"'J
h./J ,dI br<ll lll ,-Rdllfy
Ihe gloSe for Ihe Ittiludo
l nd zenilh, and fn Ihe
~ uad
r.ntof alti lude
10
Ihe givt1l
l l'mulh inIbe horiloo ;
k~~oin"
il there, lurn Ihe
gl~be
(>11
ils axis until Ihe ecliplic 'cu;s
Ih~
qu.drlnl ia Ihe gi–
reo
altilude: Ih' I poinl of Ihe ecliplic whieh CUISIbe
~nadrant
Ihere, will be the fua's place; aod Ihe day of
the
01001"
anfwfring
therel~,
lI'ill be fonnd over the like
1
lace of the fu n on Ihe wooden horilOn.
Keep Ihe
quadranl of oltitude inIhdt pofilion; and, having broughl
Ihe fun's plJce to Ibe brafen meridiJn, and thehour-indcx
10
XII
at noon, lurnbaek Ihe glube, unli! Ihe fun's
pl.cecuts the quadraot of
allilud~
osain, and Ibe illJex will
fnelV th: hour.
Any
111'0
POinl! of the ecliptic, which are equidifianl
from the beginoing of Cancel'
01'
of Capricoln, will h" 'e
the fame altitude and az;muth al the fame
h~ur,
thonbh
Ihe months be difIeren!; and therefore it reqaires fome
care in this problem, not lOmlll,ke bOlh Ihe mooth and
Ihe day of the monlh; lOaroid which, obferve, thdt
{rom Ihe 20th of M.reh tO the 2111of June, that part
of the ecliptic which is .(Jelween lhe beginning of Aries
and beginning of Canea is lObe ufcd: from the 2In
cf June
10
the 23d of September, belw,eo Ihe beginning
of Caneer and beginning of Libra : fromIhe 23d of Sep–
tem~er
to the 21fl of December,
b~tween
the beginning
.of Libra and Ihe beginning of Capricorn ; and from the
21fi of December to the 20th of March,
belw~eo
tbe
beginning of Capricorn and beginaiag of Aries. And:u
one can oever be at a lors
10
knowinwhat quaner of lhe
year he takes Ihe fuo 's altilude aod alimuth, the abol'e
caution wilh regard to the quaners of Ihe ediptic will
keep him right as to the mOnth and day lhereor.
PROB.
XXV.
To¡ nd
11"
/wg/h o[ /h, /ongej/ day
al an; givw plaa .-I f
the place be on lhe nonh fide of
me equator (fi nd ilSlatitude by Probo
l.)
and elevate Iho
nonh pole to that latilUde; lhen, bring the beginning
oC
Cancel' to the bUlcn meridian, and fet the hour,in–
dex to
XII
at noon. But if the given place
be
on the
fomh fide of Ihe equalor, elel'ate Ihe fouth poleto its la–
titude, and bring the beginniog of Capricom to lbe
brafs meridian, and lhe hour-index lOXI I. This done,
turn lhe glob. wdlward, unlil the beginning of Cancel'
or Capricom (as lhe laliludeis nonh or fou lh ) comes to
the horizon; and the index will Ihea point out the lime
of fun-fetting, for it lI'ill have gone over all the after.
noon hours, betweea mid-day aod fun fet; whichlength of
time being doubled, will give the ",hole lengthof tbeday
from fun- rifi ng tOlun-felllng. For, in aUI.Hiludes, lbe
fun rifes as long befure mid day, as he fets after it.
PRono
XXVI.
To find ill 'Wha / IIIlillldr Ihd Mg–
tjJ
d.1!
iI,
,¡
afIJ giv,n I"'glh, lifi //'."
24
houn.- If
Ihe I"ilude be oonh, briog lhe beginning of CatÍce,
10
the b,.f.n meritlan, and devale the nonh poie lOa–
bout
('6~
degrlcs; hut if tI,e lalilude be fou[h, bling lhe
be~inning
of Cap' icorn 'o tlle meridian, and elevm ,he
{oulh poi. to abollt 66{ degrees; becaufe Ihe loogell day
in r.orth lalitude is, wlren lhe fun is in Ihe fidl poinl of
Caneer; and in fomh Idtilude, ",hen he is in the firfl
p~jtU
of C.pricorn. Thcn fel ule hour-inJtK to XIl at
p
H
Y.
no,r., an,1turn thc globe \VeflwarJ, untu tbe¡odex poinl1
al h, lf
tlr~
nUll1ber 01 hou,s giyeo; which done, k<tp lhe
~¡"be
from turning on ils aXIS, and Rid. lhe lIItrrdiolJl
down
in
lbe nOleh", unt il the
aforef.idpoiot of the e.
cl'Plic
(,.iz.
Caneer O( Cap' icorn) comel to Ihe horizon;
[hen, Ih. demioo of the pole \ViU be equallo Ihe lati.
tude ,equired.
Pr.OB.
XXVII.
Tlu lalitud,
o/
an, plaa, nol rr–
mding
6H
dtgrm, brillg givrn:
lo
fi~d
in 'Whal cli.
mate th, place
ÍJ.- Find Ihe length of [he loogell d,y at
the gil'eo place, by Probo
XXV.
aod, whatever be the
number of hours whereby il exeeedelh lwelve. doubie
llrat number, and tire fumwill give the'climate io whieb
the place is_
PRO Bo
XXV lIl.
The lalillldr, alld Ihe da, of lhe
1IIM/h, kú ng
gi.rn; lo
f.nd16,
ha/lr o[ Ih, do, 'When
Ih,
fin
jhimJ
.- Sel the woodcn borizon truly level, and
the b,afeo melidian due oonh and fOUlb by a m.,incr',
eompafs: Ihen, having retli6ed the
globe,
fiiek a fmall
f.IViog-otedle iotO tbe fun's rlace in lhe ecJiplic, perpen–
dicul" to lhat pan of lhe furface of theglobe : this dooe,
turn lhe globe
00
ils axis, un,il the needle comes lOlhe
brafeo moridian, and fel the hour-index toXII at nooo
¡
then, tum the globe on ils axis, until the needle poinlS
exatlly towards the fun (which it wiU do wheo il cans
DO
fhadow
00
t~e glo~e),
and the iodex willlhew Ihe hour
of the day.
r ile Ufo
o¡
Ihe Celeflial G/obe.
H AV' NC
done for the pr& nt with the terrellri.I
globe, we fhall proceed to lhe ufe of me celellial ;
-6d1
prelllifing, that as the equalor, ecliptic, lropies, polar–
circles, horiloo, aod brafen meridiao, are exatlly aIike
on both gloues, all the former problems coneerning tbe
fuo are folved Ihe fame way by bOlh globes. The me·
thod alfo of retlifying [he celellial globe is the fame as
reélifyiog Ihe terreflnal.
N..
B.
The fuo's place for aoy day of the year lIand,
dirdtly over thal day on thehorizonof the celefliaJ globe,
as it does on that of the ,errellrial.
T he
lalitud,
and
longilude
of the flars,
01'
of all o·
ther cdellial pheoomeod, are reckoned in a , ery differ.
enl manoer from the latilude and longilude of places
o~
the eaTth : for all terrell rial laliludes are reckooed from
the equalor; and longitudes from the meridian of fome
remarkable place, as of Loodoo by the Britifh, aod
Dí
Paris by the French. But the allronomers of all na–
tions agree in reekooing lhe lalitude! of tbe moon, flm,
plaoets, aod comel!, from Ihe ecliplic; and lheir loogi–
tudes from the equinotlial colure, in lhat femi circle of
it whiehCUlSIheecliptic at the beginoing of Aries; and
theoce eafiward, quile rouod, tOIhe fame feOli-circle a.
gain. Confequently thofe lIars ,,·hieh lie bttlVeeo Ihe e·
quinotlialand Ihe nonhernhalf of lhe ecliplie, hal'eoOltl.
decl lnation aod foulh lalitude ; Ihofe which lie betlVCCll
tire equi notlial and the foulhern half of ,he ediptie, have
fouth declioalion and nonh lalilude
¡
and ,11 tlrofe ...hieh
!ie between the lropies and poles, have their dcclinalion.
and lali ludes of Ihe f,me denomin"ion.
Tbere are fiKg1'<al circks UII ,he edefiill
~Io~e,
whicl,