Upload
jean-claude-picot
View
215
Download
0
Embed Size (px)
Citation preview
7/25/2019 Bicknell, P. J. - The Shape of the Cosmos in Empedocles
1/1
THE
SHAPE
OF
TFIE
COSMOS
IN EMPEDOCI,trS
Accorcling
to
Aetius
as reporterl
by
John
of Stobi,
Empedocles
helil
the
follorving
orinions:
to {ou
ra .n
"c
Til
ei
tv
ot:pat,t,
itcg
otiv .g"
4p"ib
A,j"tcj.-
oc, n)'eiovu
ei.tctt r,.t
y,a,r,
r n).n,o
torctatt,
xut,
rata
ro
oi.pcl,ya
p.,)),o,t
.vutien^cu:,:tou
c
r
t nupan).qai.a
rv
xap.ov
xeio0..
G,thrie
2
lielieves
that
this
rotion
$as suggested
to
Empeclocles
'not
by
any observecl
facts,
but by
the poems
o{ the
Orphics, in
lvhose
cosmogony
&
r,vorld
egg g-ar,e
birth
to the
generative
power
of
Love
be{ore
the
existerce
of
heavc' a.cl
earth,
which
rvere
sub-
sequently
formecl
from
the tr,r'o
iralves
of the
egg'.
This explanation
is
surely
unacceptable.
Even if
it
can be
grantecl
that
orphic cosmogo'ies
irvolvi'g
a
rvorld
egg artedated
Empedocles,
and this
is
far
from
certain,3
it
is harrl
to
creilit
that
any
amou't
of
Orphic
plejuclice
coulcl
have
led
him
to go
against
the
facts
of
observation.
Tliis
Empeclocles
rvould have
had
to
do if he
rrelcl
that
an egg-shaped
cosmos
rotated
about
its shorter
axis. Accorcling
to
bis
vielv the
cosmos
lvas
bourrded
by
a solid,
crystalline
heaven
to
lvliich the
fixed stars
rvere attachecl.a
If
this
heaven
lvas egg-shaped,
then
to
observers
on
the
earth
the stals
near
to the
horizon
at
two
opposite
qur'te's
of it
rvo,lcl
apper'
to
be
closer
than those
at
the
other
tr,vo
quarte's.
As
lfeath
s
sarv,
such
a
cliffic'lty
could
o'ly
have
I
Aetius
2.31.
4
(DK
3.
^.50).
2
W.
K. C.
Gurrrnrr,
A l,Iistorl,
oJ
Greelc
Phlosoph,, lI
(Cnmbridge,
1965),
pp.
190-91;
a
sinrilar
vierv
has
been
taken
by
many
othcrs.
3
'I'he
mo-.l
ltalancecl
cliscussions
of
Lhe
qucstion
o{ ear.ly
Op|ict
cosrnogorries
is that
b Gurunrr,
ortheus
coul
Greelt,
Religion,
chapter
4.
Thc
co-.rrric
egg
at
Aristophancs'
Birds
93 f1. has,
o-[ course,
litle
cviclential
valur:
si.ce
the
cosrlogory
lhele
is that
of the
rircls,
a
Aeti.s
2. ll.2
(DK
31. A.5l)
ncl
2.13.
ll
(DK
31.4.54).
5
Sir Trror,r.rs [h.xtu,
Aristarcltos
oJ
TIIIiJ
SLIPI.]
OF'I}II
(OSN'IOS
IN EIPI'DOC]LIS
been
avoicled
if
Emireclocles
hacl
supposed
his ovoicl cosmos
to
rotate
rbout
its longer
axis, so that
tbe
plane containing
the surface
of
the
errth
coukl
be circuar.
Horvever,
if
this
rvere
the case
the
stars at
the zenith rvoultl
appeal
to
ar
obsetvel
to
be
{arther tlot
llearer
than
those at
the
horizon.
Empedocles,
thctr,
catrnot
liave
saicl
that tire
cosmos
was
ovoid.
ZeTler
6
rvas colrect
in
mair.rtaining that
he regardecl
it
as an
oblate
spheroicl
ancl that
the egg
comparison
is introducecl
only
to
make
the
point
that
the broadest
section of
the
spheroid is coinciilent
rvith
the
celestial
equator'.
Ihe
cosmos
lies as an
egg does
'lvhen
placecl
on a
flat sur{ace.
The
reason
for Empedocles
thus liolcling
that the
worlcl
rvas
a
flattened
rather than a
per{ect sphere was
no
doubt empirical.
Owing
to
their
greater brightness
tlie stars
overhead usually
seem
a
little
nearer
than
those
near tire horizon. Consequently,
tbe visible
portion
of
the
celestial
sphere appeals
to be a
flattened rather
than
a
hemisphericai
clome.
It
is
notervorthy
that
Empetlocles'
forced
adoption
of
an
oblate
spheroicl
lor
the shape of
the cosuros
led him
into
theoretical
complications.
Had he
been able
to
suppose that
the
cosmos,
formed
cluring
the transition
from
the rule
of
Love
to that
o{
Stri{e
over
the
{ortr roots
in the
spl.rere
o{
the All, rvas a
per{ect
srhere,
he could
quite
economically
and logically
have
made
it
anri
the
sphere
of
the All coterminous.
Sirrce
Parmenicles'
lroof
7
that
lhe
totality of
rvhat
is
mrtst be a
perfect
sphere
prevented him
{rom
allowing
the
ll even
temporarily to
lose
its
sphericity,
he was
committed
to
maintaining
that
his
notr'spherical cosmos
't\as
mol'e
or less
buried within
the
sphere
o{
the
;\ll
and surrouncled
by matter
rvhich
had
not
become
involveil
it.t cosmogony.
This
is clearly
strteil in
a
passage
o{
\etiusB rvhic]r
somee
irave
founcl
puzzling:
'l pn:oz). 6
zo-r.ov
pv v,
o
pvtot
r
nv
va
r
xap"o't,
)J.r
).Lyov
r,t ro
n.vr
rpo;,
t
onv
a,y'p
t t)'1t.
Parn
J.
BrcrNnn
Sro,s
(Orforcl,
191.3),
p.87,
note
1.
6
F.'ltttt'ttn, Die
Philosopltie tlcr Crie'
clrcn,
I,
erl. 7
cnlargctl
by
\V.
NESTLU,
p.
980,
note
2.
7
Parmenitle-',
I)K
28.B.81ines,12-{9.
I
-A.etius
1.5.2
(DK
31.A..47).
s
Sec
CurIInIr,
HGP,
lI,
p.
180.
I19