Domina Eberle Spencer and Uma Y. Shama- Stellar Aberration and the Postulates on the Velocity of...
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Physics Essays volume 9, number 3, 1996
S t e l la r A b e r r a t i o n a n d t h e P o s t u l a t e s o n th e V e l o c i t y o f L i g h t
D o m i n a E b e rl e S p e n c e r a n d U m a Y . S h a m a
A b s t r a c t
This pap er presents a s im ple pr oo f of the validity o f the universal t ime postulate on theveloci ty o f light based on the experimental d ata on s tel lar aberrat ion observed by Bradley in
1728. I t is demonstrated that Eins tein's postulate on the veloci ty o f l ight predicts s tel lar
aberration correctly in coordinate systems in wh ich the star is stationary bu t fa lls to pre dict
the pheno meno n at al l in the earthbound coordinate sys tem in which i t is observed.
Ke y word s : ve loc i ty of l igh t , s t e ll a r aberra t ion , pos tu la tes on the ve loc i ty of l igh t
1 . I N T R O D U C T I O N
This paper c l a r if i e s the re l a tionship be twee n the three pos tu-
l a tes on the ve loc i ty of l igh t sugges ted by Eins te in (1905), R i t z(1908), and M oon an d Spencer (1956) . I t summ ar izes the
previous a t tempts to de te rmine which p os tu la te i s cor rec t : t he
ana lysi s of the da ta on b inary s t ars, t he Micbe l son-M or ley
exper iment , t he Miche l son-Gale exper iment , and the Sagnac
exper iment . The paper then desc r ibes the phenomen on of s t e ll a r
aber ra t ion in two coordina te sys tems and demons t ra tes tha t on ly
one o f the three pos tu lates on the ve loc i ty of l igh t i s t enable in
Eucl idea n space.
2 . T H E P O S T U L A T E S O N T H E V E L O C I T Y O F L I G H T
The f i rs t scient is t who had the fores ight to real ize that a
formal pos tu la te on the ve loc i ty of l igh t was neces sa ry was
Eins tein. In 1905 Ein s tein 1) propo sed:
Pos tu la te I : The v e loc i ty of l igh t in f ree space i s a lways a
cons tan t c i r respec tive of the m ot ion o f the source or rece iver.
As a resu l t o f th i s postu late , un iversa l t ime no lon ger had an y
meaning except in l abora tori es whose re l a tive ve loc i ty was ze ro .
Eins te in h imm lf recognized tha t Pos tu la te I w as n ot en t i re ly
satis factory. On ly two years la ter he sug gested that i t be
mo dified, 29 His revised postulate is essent ial ly equivalent to wha t
has been ca l ledO)
Pos tu la te I* : The ve loc i ty of l igh t in f ree space i s a cons tan ti r respec t ive of the ve loc i ty of source or rece iver in any ine r t i a l
coordinate sys tem.
This means tha t in any ine r t i a l coord ina te sys tem x ,y , z l ight
emit ted at t im e rI t rave ls outw ards in spheres o f radius r x,
Fi g . 1 ,
r = c ( t - r l ) , ( I )
who se cente r a lway s rema ins at the point/~(ri ), ,l (Zi) ,~r wh ere
the source was a t the ins tan t of em i~ io n r I . Th e equa t ion for any
poin t x , y , z on th i s spher ica l wave f ront a t t im e t i s
I x - ~ ( r z ) ] 2 + [ y - n ( r z ) ] 2 + [ z - ? % ) 1 2 _ _ ( r z ) 2 . ( 2 )
Solving for r t we have
r z = ( [ x - ~ ( r i ) ] : + l y - , l ( r z ) ] ~ + [ z - r ( r z ) ] ~ ) ~ a . O )
Accordins to the pos tu la te , c locks cannot be sy nchronized unless
the re is no re l a tive mot ion be tween source and rece iver . T hus
the concept of un iversal t ime becom es untenable for l abora tor i es
that are in relat ive motion.
Eins te in ' s pos tu la te was not imm edia te ly accepted . The
in tu i tive ly a tt rac tive concept of un iversa l t ime w as n ot l igh t ly
abandoned. In 1908 the Swiss physicis t Ri tz ,(4) wh o was w orkin g
at Got t ingen , was unw i l ling to accept th is pos tu la te an d propo sed
a bal lis tic pos tulate of his o wn :
Pos tu la te H : The ve loc i ty of l igh t in f ree space i s a cons tan t c
wi th respec t to the source a t the ins tan t o f emis s ion .
Acc ording to Postulate II , l igh t emit ted at t ime r n t ravels
outward in spher ica l waves o f rad ius r n , F ig . 2 ,
rn = c(t - 7n). (4)
Ritz mad e the ball is t ic assum ption that the cen ter o f thesespheres mov es a t the ve loc i ty tha t the source had a t the ins tan
of emis sion . Thus the pos i t ion of the cen te r a t time t i s
l i ( r ~ ) + (t - r T T ) ( d U d r ) ( r T T ) ,
~ l ( rn ) + ( t - 7 n ) ( d T I I d r ) ( r u ) ,
~ra ) + (t - rn)(dr
Thus , accord ing to Pos tu la te I I , t he equ a t ion for any poin t on the
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Domina Eborle Spencer and Uma Y. Shama
Figure 1. Postulate I*.
spherical wave front is
Ix - ~(rn ) - ( t - r 1 1 ) ( d ~ / d z ) ( T n ) ] 2
+ [y - n(r n) - ( t - r n ) ( d n / d r ) ( r n ) l 2
+ [z - ~(rn ) - ( t - r u ) ( d ~ / d r ) ( r u ) ] 2 = (rn) 2.
Or, solving for riI,
rn =
lx2
1/2
(5)
(6)
third postulate on the velocity o f light:
According to this postulate, clocks can be synchronized if thelaboratories are moving at a constant relative velocity. Thus if
Postulate II is valid, universal time must be abandoned only for
accelerated laboratories. With Postulate II the concept of
universal time can be extended to all laboratories whose relative
velocity is a constant.
It was not until 1956 that another important postulate on the
velocity o f light w as prop osed. Moo n and Spencer ~3 asked
whether there is any postulate on the velocity of light that will
permit the concept of u n i v e r s a l t i me to be established for a ll
l a b o r a t o r i e s , e v e n t h o s e t h a t a r e a c c e l e ra t e d . T h u s was born the
Pos tulate in : In any coordinate system in which the light source
is stationary, the velocity of light in free space is a constant c.
Postulate III reduces to Postulate II w henever there is noacceleration of source or receiver. It was subsequently found
necessary 3) to modify Postulate III by inserting the wo rd
"inertial," just as in Postulate I*:
Pos tulate i n . : In an inertial coordinate system that is no
moving with respect to the source, the velocity of light in free
space is a constant c.
In an inertial coordinate system in which the source is always
at the origin, light travels at velocity c, so if light is emitted at
time rim the wav e front is a sphere with center at the origin and
radius, Fig. 3,
r m = c(t - rm). (7)
In an inertial coordinate system x ' , y ' , z ' in which the source is
stationary, the equation of the sphere is
(X, )2 + (y, )2 + (Z, )2 = ( rm)2 . (8 )
However, in an inertial coordinate system x , y , z in which the
source moves along a path ~(t),~(t),~(t),
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Stellar Aberration and the Postulates on the Velocity of Light
Figure 2. Postulate II .
x ' = x -
y ' = y -
z ' = z -
Thus the equation of the spherical wave front, Eq. (8), becomes
[x - ~(t)] 2 + [y - 17(012 + [Z - ~ t ) ] 2 = ( r l l l ) 2 , (9 )
or, solving for rm,
r m -- (Ix - ~( t)l 2 + LY - ~( t) l 2 + [z - ['(0 ]2) 112. (10)
The light emitted from the source at time r m travels outward in
a sphere of ever-increasing radius rm w hose center always
remains at the source no matter how the source moves. Postu-
late III is the o nly postulate that permits clocks to b e
synchronized even in accelerated laboratories. (5,~ Thus it can be
called the "universal time postulate."
In 1989 Moon et al. (6) first showed that all three of these
postulates can be expressed mathematically by the same equa-
tion,
(r)R = C(t -- l"p.), (11)
if the radii (r)R are suitably defined as shown in Fig. 4. For
Postulate I*, (r)x is the distance from where the source was at
the time of emission ri to where the receiver is at time t. For
Postulate II , (r) n is the distance from wh ere the source woul d
have been at the time of reception t, if it had continued to move
at the velocity with which it was moving at the time of emission
zn, to where the receiver is at time t. For Postulate III , (r) m is
the distance from where the source is at time of reception t towhere the receiver is at time t.
3 . W H I C H P O S T U L A T E IS C O R R E C T ?
It is one thing to formulate a postulate. It is quite a different
problem to determine whether or not a postulate is consistent
with experimental evidence.
The serious consideration of any postulate other than Postu-
late I was nipped in the bud in 1913 when de Sitter~7) poi nte d out
that according to Postulate II , distant binary stars should exhibit
very strange behavior that had not been observed: infinite
Doppler shifts, multiple images, and apparent variation in
magnitude.
For the next forty years Einstein's postulate on the velocity of
light reigned unchallenged. In 1953 Moon and Spencer~s
reexamined the data on binary stars. I t was shown that Postu-
late II need not necessarily be abandoned: there are two possibil-
ities. The data on binary stars could be explained if
(1) Postulate I is employed in Euclidean space;
(2) Postulate U is employed in Riemannian space.
The analysis of the binary star data considering all three pos-
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Domina Eborle Spencer and Urea Y. Shama
Figure 3. Postulate III*.
tulates on the velocity of l ight was undertaken by Moo n et a l p )
in 1989. This paper showed that
(1) both P ostulates I a nd III were consistent with all the data on
binary stars in Eu clidean space;
(2) Postulate II must be abandoned unless space was assumed tobe Riem~nnlan.
The famous Michelson-Morley<1~ experiment of 1887 was
~nalyzed by Mo on n) in 1993 from the point of view of each of
the three postulates on th e velocity of light. I f the experiment
was analyzed in a coordinate system attached to the laboratory,
all three postulates on the velocity o f light were show n to predict
the null fringe shift that was observed experimentally. If the
experiment was described in a coordinate system moving at a
constant velocity relative to the laboratory, the result was
entirely different. Postulate I does not predict the null fringe
shift unless the FitzGerald contraction of length, which is a
function of velocity, is introduced. Howev er, with Postulates IIand HI the mill effect is predicted in co ordinate systems that are
mov ing at a constant velocity relative to the laboratory without
any need fo r contraction o f length.
In linearly accelerated coordinate systems the situation is
different. Postulate I requires a FitzGerald-type contraction that
is a function o f both velocity an d acceleration. Postulate ILl
necessitates the introduction o f a FitzGerald-type contraction that
is a fu nction of acceleration. OMy Postulate 111predicts the null
frin ge shift with out any nee d fo r a l'~tzGerald-type contraction
even in linearly accelerated coordinate systems. Thus there are
three possible conclusions that are cott~istent with the
Michelson-Mofley experiment:
(1) Postulate I: Distance is an invariant only in stationary coor-
dinate systems but is contracted in any moving coordinate
system.(2) Postulate II: Distance is an invariant on ly in u uaccelerated
coordinate systems and is contracted in accelerated co-
ordinate systems.
(3) Postulate III: Distance is an invariant in all coordinate
systems, even those that are linearly accelerated.
The Michelson -Gale 12) experiment was analyzed by M oo n et
al. ~ in 1990. This experiment could not be explained by either
Postulate I or Postulate HI unless they were both modified to
exclude rotating coordinate systems. Thus the Michelson-Gale
experiment necessitated the introduction o f Po stulates I* ~nd
III*. Both o f these modified postulates permitted the p rediction
of precisely the fringe shift measured by M ichelson and Gale.The Sagnac(13) expe rimen t also pro duc es a me asurab le frin ge
shift. Analysis of this experiment by Mo on et al . (14) has shown
that the experimental fringe shifts are predicted by bo th Po stu-
lates 1" and III*.
4 . STELLAR ABERRATION IN THE STELLAR COORDI-
N A T E SY ST E MThe phenom enon of stellar aberration has been ably treated by
Hayden,o5) who questioned the Einstein equations, wh ich wer e
supposed to explain the well-known result. The phen om enon o
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Stellar Aberration and the Postulates on the V elocity of Light
v ( t )n ( x ) + V y ( ~ ) ( t - ~ n ) , v(* ~n ) ~ ' - - . . .
( t '
v ( x ( t ) , y ( t ) ,
r i
z ( t )
Figure 4 . The three postula tes on the ve loci ty of l ight .
s te l la r aberra t ion w as discovered by Bradley, (103 wh o found tha t
t he t e le scope mus t b e t i pped fo rward b y an ang l e
= ( v / c ) s i n 0 ( 1 2 )
wh en the te lescope is moving a t a re la t ive ve loci ty v toward the
star and the star i s a t an angle 0 above the hor izonta l . The
maximum orb i ta l ve loc i t y o f t he Ea r th i s abou t 1 0 -4c , so t he
max imum va lue o f v t c i s approximate ly 10 -4 tad , or approx -imate ly 20.5".
In a coordinate system in which the star i s s ta t ionary the
analysis i s the same for Pos tula tes I* , I I , and I I I* , Fig . 5 . Light
t ravels f rom the star a t ve loci ty c a t angle 0 wi th the hor izonta l.
Howeve r , i f t he t e l e scope i s i n mot ion a t ve loc i t y v i n t he
horizonta l d i rec tion, the te lescope mus t be or iented a t angle (0 -
A0). From the l aw o f s i nes ,
vAt /sin A0 = cAt /sin (0 - A0) , (13)
where ~t i s the t ime requi red for l ight to t raverse the length of
the te lescope. Since A0 is smal l compared to 0 and v << c ,
AO ~ , ( v l c ) s in0 , , V s in0 (14)1 + ( v / c ) cos 0 c
jus t a s was found by B rad l ey .
This i s essent ia l ly the explanat ion of s te l la r aberra t ion given
by Bergmann. (17) Th us w e can c onclu de that, since in a stellar
coordinate system a l l three postula tes on the ve loci ty of l ight
predic t tha t the ve loci ty of l ight i s c , a l l three are in agreement
wi th Bradley 's exper imenta l resul t .
5 . S T E L L A R A B E R R A T I O N I N A N E A R T H B O U N D
C O O R D I N A T E S Y S T E M
But ast ronomical measurements are ac tual ly made in e a r t h -
b o u n d labora tor ies . I t i s necessary to be able to expla in them
both in coordinate systems in wh ich the star i s s ta t ionary and in
coordinate systems in which the te lescope i s s ta t ionary.
As shown in F ig . 6 , i n an ea r thbound coord ina t e sys t em Pos-
tula te I* predic ts an ent i re ly di f ferent resul t f rom Postula tes I I
and II I* . The star i s a t angle 0 abov e the hor izon a t t ime ofemission r . In th is coordinate system the star i s t ravel ing to the
lef t a t ve loci ty v . According to Postula te I* , l ight t ravels f rom
where the star was a t t ime r to where the te lescope i s a t t ime t
a long t he d is t ance r I shown in F ig . 6 . The subsequen t mot ion o f
the star does n ot a ffec t the d istance r I . T herefore , P o s t u l a t e I *
p r e d i c t s e r r o n e o u s l y t h a t t h e r e i s n o s t e l l a r a b e r r a t i o n i n t h e
e a r t h b o u n d c o o r d i n at e s y s t e m .
Since the pa th of the star i s approximate ly l inear o ver the t ime
interval to be co nsidered, P ostula tes I I and II I* cannot b e
dist inguished in this exper iment . According to both postula tes,
the distance r n = r m is measu red f ro m whe re the star i s a t t ime
t to where the te lescope i s a t t ime t as shown in Fig. 6 . Theangle A0 betw een the di rec t ion r I and the di rec t ion of r~ and rm
of Fig. 4 i s the ansle o f s te l la r aberra t ion. To pro ve this , we
have o nly to use e lementary t r igonom etry. Since r n = r m =
c ( t - r n) = c ( t - r il l) and the star has mo ved a distance v( t -
rn) = v( t - rm) betw een t ime rn = rm and l ime t , by the law
of sines,
v ( t - r ) = c ( t - r ) (15
sin A0 sin (0 - A0) '"
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D o m i n a E b o r le S p o n c er a n d U r e a Y . S h a m s
Star
C
T e l e s c o p e
V A t
O-AO
0
Figu re 5. Stel lar aberrat ion in a coord inate sys tem in wh ich the s tar is s ta tionary and the te lescope is in m otion , Postulates I*, II ,
and I I I* .
But s ince A0 is a very smal l angle and s ince A0 << 0 and
v < < c ,
AO ~ v /cs inO. (16)
Th us Po stulates 11 and III* both pred ict exactly the stellar
aberrat ion discovered by Bradley in 1728. But Postulate l ' fa i l s
to pre dic t any stellar aberration in an earthbound coordinate
system.
6 . C O N C L U S I O N S
Since a cont rad ic tion has been demon s t ra ted , i f t he phenom
enon o f s t e l la r aber ra t ion i s ana lyzed in s t e ll a r and ea r thboun
coordinate sys tems, Postulate I* must be rejected. Postulate I
mus t be re j ec ted because o f the b inary s t a r da ta unless we
assume that space is Riemannian rather than Eucl idean.
Thus the only postulate on the velocity of l ight that is in
agreement with all the experiments hitherto analyzed on a
comparative basis is Postulate III*. This postulate is consis ten
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Stellar Aberration and the Postulates o n the Ve locity of Ligh t
P o s t u l a t e I * P o s t u l a t e s II a n d I I I*
S t a r S t a rv _ v ( t - ~ , , , )
131
C
C
rn = r~H
r I = C( t - T i ) - - C ( t - z i I )
0 / J / J \ 0
t - t
F i g u r e 6 . S t e l l a r a b e r r a t i o n i n a c o o r d i n a t e s y s t e m i n w h i c h t h e s t a r i s m o v i n g a n d t h e t e l e s c o p e i s s t a t i o n a r y .
w i t h t h e b i n a r y s t a r d a t a e v e n i n E u c l i d e a n s p a c e . I t p r e d i c t s t h e
n u l l re s u lt o f th e M i c b e l s o n - M o f l e y e x p e r im e n t w i t h o u t th e
n e c e s s i t y f o r a F i t z G e r a l d c o n t r a c t i o n . I t a l s o p r e d i c t s t h e c o r r e c t
f r i n g e s h i f t f o r b o t h t h e M i c h e l s o n - G a l e a n d t h e S a g n a c e x p e r i -
m e n t s . A n d i t p r e d i c t s t h e s t e l la r a b e r r a t i o n o b s e r v e d b y B r a d l e y .
O n t h e b a s i s o f th e e x p e r i m e n t a l r e s u l t s h i t h e r to a n a l y z e d w e
c a n c o n c l u d e t h a t u n i v e r s a l t i m e i s a t e n a b l e c o n c e p t , d i s t a n c e i s
a n i n v a f i a n t , s p a c e i s E u c l i d e a n , a n d t h e a n g l e b e t w e e n r I a n d r l a
s h o w n i n F i g . 4 i s t h e a n g l e o f a b e r r a t i o n t h a t a s t r o n o m e r s h a v e
b e e n o b s e r v i n g f o r n e a r ly t h r e e c e n t u r ie s . U n l e s s f u r t h e r a n a l y s i s
o f o t h e r e x p e ri m e n t s p r o d u c e s c o n t r a d i c t o r y e v i d e n c e , w e c a n
c o n c l u d e t h a t the velocity o f light is not a constant in al l
coordinate systems but is a constant in any inertial coordinate
system in which the source of light is stationary.
R e c e i v e d 2 4 A p r i l 1 9 9 5 .
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Domina Eberle Spencer and U rea Y. Shama
R 6 s u m 6Cet art ic le pr~sente une preuve sim ple de la val idi t~ du po stula t d 'universe l temps s ur la
v i tesse de la lumi~re ~ part i r d es donn~es exp~rimentales sur l 'aber rat ion ste l laire observ~e
pa r Bradley en 1728. I I est ds que le pos tulat d 'Einste in sur la v i tesse de la lumi~re
donne une pred ic t i on adequa te dans un sy s t~ne de co ord onn ~ dans l aqueUe l '~ to i le e s t
s tat ionnaire mais la pr~ l ic t ion est compl~tement erron~e lorsqu'observ~ pa r ra ppor t r un
syst~Vne de coordonn ~es li~ au r~f~ rentiel terrestre.
R ef erences
1. A. Einstein, Ann. Phys. 17, 891 (1905).
2 . Idem, Jahrbnch Radioaktivitat IV , 42 2; V, 98 (Berichti-
gunsen, 1907).
3. P. M oon, D.E . Spencer, and E.E. M oon, Phys. Essays 3,
431 (1990).
4. W. Ritz, Ann. Chim. Phys. 13, 145 (1908).
5. P. M oon and D.E. Spencer, Phi los . Sci . 23, 216 (1956).
6. P. Moon, D.E. Spencer, and E.E. Moon, Phys. Essays 2,
268 (1989).7. W . de Sitter, Phys. Z. 14, 1267 (1913).
8. P. M oona nd D.E. Spencer, J . Op t . Soc. Am. 43, 635 (1953).
9. P. Moon, D.E. Spencer, and E.E. Moon, Phys. Essays 2,
275 (1989).
D o m i n a E b e r l e Sp en ce r
University of Connecticut
Storrs , C onnecticut 06268 U .S.A.
U m a Y . S h a m a
Bridgewater State College
Bridgewater, Massachusetts 02324 U.S.A.
10. A.A. Michelson and E.H. Morley, Am. J . Sci . 34, 333
( 1 8 8 7 ) .
I I. E . E . M o o n , P h y s . E s s a y s 6 , 4 8 7 ( 1 9 9 3 ).
12. A.A . M ichelson, Astrophys. I. 6 1, 137 (1925); A.A .
Michelson and H.G . G ale, ibid. , 140.
13. G. Sagnac, C. R. Acad. Sci. 1 57, 708, 141 0 (1913).
14. P. M oon, D.E . Spencer, and U.Y . S h~m a, Phys. Essays 4,
249 (1991).
15. H.C . H ayden, "Stellar Aber ration," to be published;
"Stellar Aberration and the Street-Lamp Pa rado x," G alilean
Electrodyn., to be published.
16. J. Bradley, philos. Trans. 35, 637 (1728).
17. P.G. Bermnann, Introduct ion to the T heory o f Relat iv ity
(Prentice-Hall, NY, 1942).
48 3