14.5
CONFLUENT
HYPERGEOMETRIC
FUNCTIONS
423
His observation
of
the variation
of
the proper
motion
of
the stars Sirius and Procyon
led
him to posit the existence
of
nearby, large, low-luminosity stars called dark companions.
Between1821and1833he cataloguedthe positionsof about75,000stars,publishing his
measurements in detail. One
of
his
most
important contributions to astronomy was the
determinationof the distanceto a starusingparallax.This methoduses triangulation,or the
determinationof theapparentpositions of a distant objectviewedfrom twopointsa known
distanceapart,in thiscasetwodiametrically opposedpointsoftheEarth's orbit.The angle
subtended by the baseline
of
Earth's orbit, viewed from the star's perspective, is known
as the star's parallax. Before Bessel's measurement, stars were assumed to be so distant
that their parallaxeswere too smallto measure,and it was further assumedthatbright stars
(thoughtto be nearer) would have the largest parallax. Besselcorrectly reasoned that stars
with large proper motions were
more
likely to be nearby ones and selected such a star, 61
Cygni, for his historic measurement. His measured parallaxfor that stardiffers by less than
8% from the currently acceptedvalue.
Given such an impressive record in astronomy, it seems only fitting that the famous
functions that bearBessel's
name
grew out
of
his investigations
of
perturbationsin planetary
systems. He showed that such perturbations could be divided into two effects and treated
separately: the obvious direct attraction due to the perturbing planet and an indirect effect
caused by the
sun's
response to theperturber's force.
The
so-called Bessel functions then
appear as coefficients
in the series treatment
of
the indirectperturbation. Although special
cases
of
Bessel functions were discovered by Bernoulli,Euler, and Lagrange, the systematic
treatment by Bessel clearly established his preeminence, a fitting tribute to the creator
of
the
most
famous functions in mathematicalphysics.
14.5.1 BesselFunctions
Bessel
differential
The Bessel
differential
equation
is usually written as
equalion
1/
I,
( V
2)
W +
-w
+
1-
- w = 0
Z Z2
(14.41)
As in the example above, the substitution
w =
zI'e-~'
f(z)
transforms (14.41)
inlo
d
2
f
(2/k
+I )
df
[/k
2
- v
2
~(2/k
+I) 2
IJ
f 0
-+---2~-+
-
+~+
=,
di
z ~
~
z
which, if we set /k =v and
~
=i, reduces to
r +
CV:
I _
2i)
f'
_
(2V;
I);
f =
O.
Making the further substitution 2;z = t, and multiplying
out
by t, we obtain
d
2f
df
t-
2
+(2v+I-t)--(v+!)f=O,
dt
dt