G
E
o
11'1
E T
R
Y.
Wh,'d'm ,
by
lhe
3d
cafe of trigooo!llwy, BC, tbe di- the clemeots) tO contrive metilotls for this purprl e, ac'
Hance
fou~ht,
wllI be fou0'1.
cordiog tO die occ.fion: fo that there is no oeed of
atl~-
P
p
O P O S 1
T
IO N
XVr.
iog any more of Ihis fOrt. We
{hall
fubjoin hm a m' ·
F,e ,
~O.
ro nlr4/1rr Ih, drjl"nct o[ /wo p/acú
A thod by whidl (he oi:uneter of the earth Illay be luu"d
M.1lJ,
o[
,vhic~
o,,,
ÍI
aCCffiblt,
~)'
Iht gr6pr.ollulrr.-
OUt.
Let there be ereaed at two points A aod C, fuflicienrly
PRO P O S
1
T
ION
XIX.
dirhnt, twO vifible ligos ; then (by Ihe t2n, prop. of tbis
PLA,.. CXVL F,c.
1.
r ofind Iht diam"tr
.¡
Il,.
pan)
Id tbe tWO angles BAC, !JCA be t:>.ken by tite
earln[rol/l o/u Obftrvalion,-Let
there
be
chofeo a high
~r"phometer.
Let the dilfance of thellations A aod C hill AR, oear the Cea-OlOre, and !et tbe obCer·vator vn
be meafured witll a chain. Then the thiro angle B being the top 01 it, with ao' exatl quarlrant divided iuto mi–
koo.,n, aoo Ibe fide AC being likewiCe known; there- nUles and fecoods by traofvcrCe divifions, and filtCd with
fore, by tbe 6rn cafe of trigonomctry, the dillance re-
B
telcfeope in place of tbe common figlm, meafure ,he
quired, AB, will be fouod.
the aogle ABE cootaioed uoder the righl lioe AB, whkh
PRO
P
O
S {
T
ION
XVU.
goes to tbe ceotre, and the right lioe HE dralVn to the
Flc . 2t.
r o",'af¡rt Ay
Ihe
groph' lntltr, Int di·
Cea, a tangeot to the globe at
E;
let tber.e be drawo
jla/lrt
of
I,v. plam, /ltilhtr o[ 'W!Jich
JI
aCCfJ!ih/t.-
Crom A perpeodicular 10 BD, the lioe AF meetiog BE
Let
(11'0
Ihtioos C aod D be cbofeo, from each of which io F. Now in Ihe rigbt.angled Iriaogle BAF all
tI~
ao–
the plms may be feeo whofe dillance is fought : let tbe gles are giveo, alfo the fide AB, the Iteight of,the bill .
Rogle5 ACD, ACB, BCD, aod likewiCe the aogles whicb is 10 be found by fome
oC
the foregoiog Dltlbods:
BDC, BDA, CDA, be meafured by tbe grlphomelcr; as exaélly as pollible; and
(by
lrigonometry) the fidco
let Ihe dill.oce of the
Ilatio~s
C aod D be meaCured by a BF aod
AF
are foun.d , But, by eor. 36tb
3,
Euc!. AF
cbaio, or (if it be oeceffary) by the precediag praélice. ;s equal to FE; tberefore
BE
will be koown, More–
Now, io the triangle ACD, there are giveo tWO aogles over, by 361h
3. Elle!.
tbe rellangle under BA aod BO
ACD and
A
OC; tbereíore, the third CAD is likewife is equal tO tbe fquare of BE, And thenee, by 17lh
giveo ; moreover the fiele CD is giveo ; therefore, by the
6. Euc!,
as AB : BE :: BE :
8
D. Therefore, ,fioce
6rll caCe of Higooometry, the fide AD will be found . AB aod BE are already ginn, BD will be Cound bJ rrth,
After Ihe fame maooer, in tbe triaogle BCD, from all
6.
Euc!. or by "le rule of three; ood
Cubr~2éting
BA,
the aogles aod ooe lirle CD given, tl:e Gde BD is fouod, there 'l/ill remain AD the diamelar of tbe eanh fought.
Whercfore, io the triangle ADB, from lhe given fioes
S
e
H
o
L 1 U M.
DA
aod DH, aod rhe aogle ADB contaioed by them,
Many otber metbods might be propofed for meaCuring
the fide AS (the di(laoce Cought) is found by tbe 4tb the diameter of the earth. The mofl ex,él is that pro-
cafe
of
trigonometry of oblique.angled triaogles.
pofed by Mr Picart of lhe acade/TIy of Ceieoees at Paris.
PRO P O S 1
T ION XVIII,
" Accordiog te Mr Pi<:art, a degree of lbe meridian
FI
C. 22.
1I
iJ
rf</uird'by1ht grophol/ul<r and 9ua-
"al the lati'tude of 49° 21 ', was 57,060 Freoch toiCes,
¿ronl, lo II/tajl/r¡ an awJ!iblr hrighl
AB,
plaud jo on a
"eaeh
oC
whicbCOntaiM
fix
Ceet of rhe fa me meaCure'
jlup, Ihat ont con n,ilhtr go n,or
it
in an horizonlal
"from which it follow!, that, iC Ihe earth
be
an exad
plant, mr ruede[ronl i/, al 'v< juppofld in Ihtjo/ulian
"fphere, lbe circumfereoce of a great cirele of it will
o/'tht
14/h
P,op.-Let
there be chofen '1oy Í1tuation as "be 123,249,600 Paris fm, and the femidiameter of
C, aod .notber D; where let fome mark be ere@.ed: "the earth r9.6t5,800 feet: but the l'rench malhe–
let tbe angles ACD aod ADC be fouod by Ibe grapbo- "maticiaos, who of late have ·cxamined Mr
Picart~s
0-
meter; then the third aogle DAC Vlill be koown. Let "perations, alfure us, That Ihe ckgree io thar latitude
the fide CD, the dillance of the (la,ions, be Oleafu red "is 57,183 10iCes. They menCured
-a
degree inLap–
with a chaio, aod theoce (by trigoo.) the fide AC will he "lood, in the la!ilUde of 66° 20', and fouod it of
found. Again, io the triaogle ACB, rigbt aogled at B, "570438 toiCes .• By comparing rbefe degrecs, as wcll
naviog fouod by the 9uadraot the aogle ACB, the other .. as by the obCervatioos 00 peodulums, and Ihe thenry
angle CAS is knolVo like"..iCe: but the fide AC io lbe "of gravity, it appears Ihat Ibe earth is ao olilate fphe–
triangle ADC is already known; therefore Ihe heighl "roid; aorl (fuppofing thoCe degrees
10
be accurmly
req uir~d
AB will be found by tbe 4tb cafe of righ t·aogled "meafured) Ihe axis or diameler that palfes through the
triangles. If theheight of ¡he tower is waoled, the ao· .. poles will be to tite diameter of tbe equator, as
177
10
glc BC!" wilJ be fouod by the quadrant; wbicb being "1 ¡8i or thecarth will bc 22 miles higher at the equator
takeo froOl me angle ACB already koowo, the angle "than at tbe poles.
A
degree bas likell'ife ['eeo mN–
ACF \ViII remain: but tbe aosle
FAC
w;tS koowo before ; "fured 1.t tbe cquator, ami found 10 be confidmbly
I~(s
tberefore Ihe reOlaining aogle AFC will be konwo. But "tbao al the I.,titurle of Paris ; whicb
c()nfirm~
r!,c ob.
tbe fine AC lilas alCo knowo before; Ihcrefore, in the "late fi gure of
Ih~
eallh, Bur an accouot 01' this IJI!
triangle AFC, .11 the aoglcs aod ooe of the fides AC be- "meofurat;oo has OOt beco ptlbliOll'o as reto
If Ibe
iog koowo, Af, the beight of the tower l.bove the hill, " e3lth was
uf
ao I:oiformdeoÍlty from Ihe «rrface
tu
will be founJ by trip,onoOletry.
.. the
ce~lre,
!llro, accordiog to Ihe thco,y oCgra l'il,",
S
e
f!
o
L 1 U M.
"
the OIcridian \Vould be an exaél ellil'fis, aod the axis
lt
werc cafy tO add 0I30y other
Ill~th()ds
of meafl!ring "would be 10 Ihe t1iameler of the c9t1ator as 1,0 10
~eigh:s
and diflaoces ; but, ir what is aboye be tloder- "23r ; aroJ Ihc .!ilI'crence of Ihe fcmi,li'lm",'r oi' the
¡¡uod, it will hc e"fy (. rpetially for ooe th.1 is ..rCld in .. cqtlalor aod f"mi,xis abotlr 17 miles,"
VOL .
JI.
No,
Sí,
2
l'
7 N
La