A
A PROBLEM ON THE STABILITY OF SPHERICAL GYROSCOPE (ODNA
USTOICAIVOSTI QIROSKOPA)
ZADACAA
08
Vo1.27,
No.6,
PMM
V.
1963,
V.
SHAROVOQO
pp.f005-1011
KREMENTULO
(MOSCOW) (Received
Under certain
assumptions
we consider scope. for
the
June
on the nature
stability
of
asymptotic the
stability.
case
of
method
The cases
rotation
of
the vertical
By the Liapunov-Chetaev
also
20,
with
of
1963)
the
viscous
rotation
gaseous
of
we obtain
sufficient
astatic
and heavy
variable
angular
shell,
a spherical
gyro-
conditions gyroscopes,
velocity,
and
are treated
in particular. The principal given
LlI.
in
scheme A steel
for
the motion
sphere
of
1 (Figure)
a spherical
is
placed
gyroscope
inside
was
a closed
spherical bowl tionary vertical wall
of
2 rotating with constant angular velocity around a staaxis 0~1. Gas supplied through special holes in the bowl forms a shell completely enveloping the sphere and
the
isolating
it
instant
the
thickness
(equal
the
sphere)
the
geometric
center
from the gaseous
to the
and remains center
the
gaseous
has
inside
axis of vertical
the
shell it
The
bowl.
thus
for
the
sphere
It
is
assumed
a homogeneous between all
shell
the
radii
subsequent coincides,
consequently,
is
time
that
at a certain
with
constant
of
the
of
the motion.
by hypotheses,
a stationary
bowl
and
with
point.
Thus, the
Since
the
viscosity,
the bowl in spinning carries along with it in its turn makes the sphere rotate. The sphere
which
be the
balanced
stability
the
difference
a cylindrical
0 will
of
becomes
groove
symmetry 0~ which 02,. The ellipsoid
point 1.
ing
of
of the bowl and,
gas has a specific
the
wall
shell
of
at the
3 for initial
creating instant
of inertia of the ellipsoid of rotation.
gyroscope. the established
The problem motion
1547
of
a definite coincides
sphere
with
consists the sphere
dynamic with
of
respect
the to
investigatas a rigid
1548
V. V.
body
in which
,pension the
the
center
0 and which
viscous
to the
gaseous
difference
of
is
gravity
acted
shell
Krementulo
coincides
between
the
angular
of
lar
the
the
velocity
instantaneous
velo-
of
the of
[21 prove
K is
of
the
us note
that
gaseous
A
here
the motion
is
the
choice
mentioned
problems
of
such
of
the
only
respect
action
velocity
of
gas is
to point
an induction
in balanced
value
for
considered
0.
Let
creation
The action
of
moment
maintaining
us write
the dynamic
the
a con-
equations
equations
of
A) qr = K (coy -
p),
-$+ qf-r-7’
I=
2 +
(A
-
C) pr=
q),
g
=- f)
K (coy” -
the
moment of
K (07’
-
equatorial of
respect under
moment of the
inertia
sphere,
corresponds
to
to the
p,
axes
investigation
P =
p==q=o,
ry
-
/7,-f
Euler
0
(1.2)
r),
inertia
with
stationary state system (1.2)
_t
and
the
-
Oz,
co-
with
motor,
motion.
sphere in the form of equations of Poisson
not
in connection
w =
a rotation
the
the
7
sphere,
C is
the
the projections
the sphere onto the principal direction cosines of the
Ox, Cb, and Oz, will
COIISL,
of
of
7 and r are
of the instantaneous angular velocity Q of axes of inertia Oxyz, y, y’ and y ‘* are the
which
a numerical
(C
Here A is
vertical
in hydroaero-
$- +
c -dr = rlt axial
of
analogous
our
moment M with to
of motion of the and the kinematic
A
certain
that
shell
rotating angular
the
valid.
M'1s analogous stant
of
the coefficient
solving
efficient
the
velo-
gas.
mechanics
Let
(1.1)
angular
d is the thickness and v is
7he results
that
in
o is the constant anguthe bowl, R is the radius
of
shell
viscosity
sus-
sphere,
of the sphere, gaseous
of
M originating
The
M = -K (!4 - w), K =8g2 city
the point
moment
and proportional
cities of the sphere and the bowl. moment M is taken in the form
where Q is
with
upon by a rotating
respectively.
be the particular
=
sphere
y’
zz 0,
and the
7” =z 1
bowl
The
solution
of
(1.X)
as a wliole
A problem
around
the
depending
on
vertical on p,
whose motion of equations
axis
q,
they (1.2)
0~~.
y,
r,
stability
the
y’
describe allows
of
a spherical
1549
gyroscope
The right-hand sides of equations (1.2)) and y”, show that the mechanical system
is essentially nonconservative. of only one known integral r2 +
7’2 +
TV2 =
The system
const
(1.4)
Let us determine the stability of motion (1.3) in the sense Liapunov with respect to the variables p, q, F, y, y’ and y”. The problem
rotation (1.3) with respect to body with a fixed oint in the Lagrange case, was solved, as is well known, by Chetaev [3 P by the method of constructing Liapunov functions in the form of a linear combination of the integrals of the equations of perturbed motion. In the given case p,
q,
F,
y,
of stability and y” for
of
y’
of vertical a heavy rigid
the number of integrals is not sufficient for the construction of a linear combination; however, we can try to construct a sign-definite combination from specially selected functions such that the conditions of
Liapunov’s Let
stability
us introduce
the projection and the
of
function
theorem
into the
consideration
angular
El
9 =
the kinetic
momentum
energy
G of the sphere
of
onto
the
sphere,
axis
Ozl,
Gz, = Apy + A qy’ + Cry”
+ Aq2 + CF), cll =
P =
satisfied.
0
T = +(Ap2
By denoting
are
the
perturbed
rl,
r=a+L
72 +
7’2 +
motion
7s2
(1.5)
corresponding 7
=
a,
7’
to =
(1.3)
P,
f’
by 1 +
=
6
(1.6)
we can write
F, = A (E” + q2) + CC”+ 2Co5 F, = A (b + qS) + CC6+ C (06 + 5) F, = a2 + p2 i Let
us make a linear
combination 2V =
It
is
not
difficult
2V = A (E” f
q2) -
to 2oA
see
F, that
(&I +
(1.7)
a2 + 26 of
20F,
functions +
2V will
q6) +
The derivative of function I’ taken turbed motion corresponding to motion
(1.7)
in
the
form
Co2F, be a quadratic
Co2 (a” + relative (1.3)
to
form
p”) +
C (< -
the
equations
oQ2 of
(1.8) per-
1.550
(l-9) will be sign-constant of a sign opposite to that of V. The function V, not being sign-definite in all of the variables <, q, <, a, p and 6, will be sign-definite in the variables <, q, a, p and 6 - o< when the condition C > A is satisfied, which indicates that in this case the axis Oz will
be the minor
of
the
ellipsoid
bility
with
stable y” are
with respect to p, q, y, y’ connected during the motion stability
follows
stability
respect
to y”
sequently, respect
the point
respect
all
The derivative general,
it
(1.3). is
is
sufficient
given
by the
asymptotic
with
my” follows
variables not
motion
in
c: = 0.
with
in equality variables
(1.6),
we obtain
it
is
seen
the modulus the
sphere
equals
does
motion not
motion the
function,
under for
therefore, of
with
study of
this
stability
is
theorem
t.hr
if
in detail
derivative
v’ is
between
motion
the
the nature
of
to
in accordance
(1.10)
= ---K/Q -aI2
proportional the
motions,
we <..n solutions except
from perturbations
(r-oy”)2l
state
derivative
to be asymptoti-
be demonstrated
difference
in of
the
asymptotic
we pass
and unperturbed
&n-
F.
be stable
stability
the perturbed
+
there
and y”.
us clarify
(1.9)
and
to
angular
the
square
velocities
of of
and consequently,
when Q = o.
or does
whether
the
vector
sphere
with
to
will
asymptotic
will
I.et of
respect
(1.3)
not wholly contain the corresponding to (1.3))
t_ (q--oy’)2
(1.2) shows that rotations around
except
perturbed
that
the
in perturbed
zero
System motions Y -
of
with y’
motion
(1.3)
If
the
to y and y’
sign-constancy
0 does motion
the original
V’ = --K[ (p-(0~)~ Hence
y,
the
the
itself.
of
the theorem on sta[41, motion (1.3) is
and from stability
[5,1 . On t,he basis
of
region
values
r,
infer
motion
(1.3’)
respect
criterion
establish that the region I’= of the equations of perturbed the
q,
cases
stated of
with to y”,
a sign-definite to
of
variables
stability
the unperturbed
stability
the
C > A, motion p,
possible
theorem
inertia
and r - my”. lhe variables y, y’ by relation (1.4), and therefore,
(1.3)
Such a sufficient
unperturbed
of
respect
condition
in certain for
stable.
solution
1’ is not
However,
cally
of
the
the
a portion
also and r -
under to
to
of
0. Thus, on the basis
respect
from the
to
axis
with
sphere
(1.3). contain
the sphere cannot the vertical with
Hence, the
corresponding for
the
entire
specified
to
accomplish established constant angular velpcity
question
whether
integral
curves
(1.3),
reduces
perturbations
the of
to the
region
the
question
can or cannot
V = 0
equations
of
of
accomplish
A problem
a continuous city
0.
fixed
sequence
In other
axoid
that
the moving bodies
us to
infer
axoid
gives that
achieving
asymptotic
it
is
sion
of
0.
that inertia
the of
Note.
condition
axis
the
C >
A motion
of
vertical
of
rotation
[61,
(1.3)
of
which
will
(1.3)
be the minor respect in
the
same time allows
be asymp-
of K. Consequently,
rotation
was obtained
velo-
that
The kinematics
question
the magnitude
with
at the
cone?
this
of
sphere
result
The results of
inertia
other
of
the
the
2v =
of
symmetry
Section
of
the
body with
assumptions
show that
of
to
of
the
for sphere,
axis
of
the
the point
of
suspen-
[71 by investigating
1 can be extended
rigid
body.
respect
to
Section
function
the
1 remain
satisfied,
in the
motion 2.
(1.3)
variables
of
us assume that dynamic
axis
of
The equations
$ + (C Ag+(A -
A
to
gyroscope. does
the
under not
center
of
It
axes is
Oxyz.
not
re-
The
difficult
to
motion
C) pr = -
(1.3).
stable
the
mgq,r
q,
r,
to
the
Hence,
under
with
equations
of
the unperturbed
conditions
of
the point the
(1.12).
sphere
suspension
is
located
0.
Let
on its
0.
sphere
K (coy +
y,
of
z,, from point
P-1)
p),
cg =
K (of
-
r)
K (07’ - q),
of a stationary solution not’ations, we investigate
respect to p, the functions
in-
Let us proceed to the question of the the action of moment (l.l), in which the
mgz,f +
A) qr =
when the
(1.12)
relative
gravity
of
(1.11)
Pz) + C(c - 06)~
p and 5 - 06
(1.9)
coincide of
a,
state
synnnetry Oz at a distance
when o = const, admit selves to the previous (1.3) with sideration
derivative
the sphere
gravity
the
C>B
be asymptotically
heavy of
we waive
principal
in force.
<, q,
A,
corresponding
will
The
stability center
has the
motion
its
if
B and C be the moments
(AEa + BqP) + Cw2(a2 +
C> perturbed
Let A,
V
At2 + BqZ - 20
Positive definite equal it ies
are
to
some angular
body move such line
a nondegenerate answer
with
rigid
1551
problem.
quirement of
straight
stability
An analogous
linear
to some fixed
the
gyroscope
rotations the
independently
sufficient
spherLcal
a
instantaneous
remains
under
stable
01
can or cannot
a negative
totically
ellipsoid
of
words,
degenerates
rigid
stabrlrty
the
on
y ’ and y”.
(1.3). the
By confining stability of
Let us introduce
into
ourstate con-
1552
Qr = A (5” + %
= A (Eo +
Functions F,
of
qB) +
q2) +
C66 +
Cl;” +
C (06
az and o3 coincide
Section
1.
It
is
easy
with
to
see
+
SCOT, + 6),
2mgz,6,
@a =
(2.2)
a2 + p2 t- h2 _t 26
the corresponding
that
the
functions
derivative
of
the
F, and functions
v, 2V, = taken form
relative (1.9).
to
the
a1 -
equations
The function 2vi
2&,
= A 6”
of
q2) +
+(Co2
motion
of
by virtue
of
asymptotic not
enter
directly
determine axis.
C >
the rate
( 2.4)
A inequalities
above,
motion
into
the damping
Inequalities
case
of
of
will
conditions
may hold (2.4)
are
in case
C < A they
reduce
3.
Ihe
velocity system sphere
case motion
u = o( t ). of
be the for
for
the
[31 when
(2.4)
conditions for the coefficient
motions
any relation
stability of
the h’ does if
the
gyroscope
between
A and C.
we In
to (2.5)
0 condition
We studied rotating
a sphere,
the
(2.3)
0
asymptotic
equivalent
C) 69 + mgz, <
(A -
established
to
has
(2.3)
20 <
the perturbed
to < but
function
As before,
(1.3).
of
by Chetaev
0,
C) to2 + mgz, <
what was stated
stability
(1.3),
(A& + A$ + ~56) + (a2 + fi2 + d2)
sign-definiteness
(A -
for
form
2w
mgz,)
resulting from, a more general form constructed A = - o and P = 0 (in the notations of [31). ‘Ihe conditions
mgz,) CD3
be a quadratic
Cc2 -
-
(Co2 -
perturbed
2V, will
+
+
0
(2.6)
above the stability around the vertical
of the with a
equal to the constant velocity o of the bowl. As shown by in the case o = o(t), the nonstationary motion of the (1.2))
p=q=o,
r =
does not occur. Motion (3. l), of special corrective devices
0
(t),
r = q-’ = 0,
nevertheless, which create
is possible an auxiliary
y” = 1
(3.1)
in the presence moment Mzk( t)
A problem
on the
stability
of
a spherical
gyroscope
1553
around axis 04. In every real gyroscopic system there are usually introduced corrective devices to ensure the realization of some designed motion; this justifies to a known degree the assumptions of the stated problem. If Mzk(t)
satisfy
the condition M*k (t) = Co.(t)
(3.2)
then the system of equations
A g Ag
(3.3)
+ (C - A) Q’ = K (W’ - p), + (A - C)
pF
=
K
admit of the particular we write the equations
(of
c -dr = R (a$
r) +
M*k (t)
solution (3.1). Retaining the adopted notations, of perturbed motion corresponding to (3.1)
df Az+(C-A)q(~+f)=K(
$
oa - 8,
A~+(A--C)((o+t)=K(oB-~),
c$ =K As the Liapunov
-
dt
q),
-
(08 -
function
2V = Fl -
let
Q, us
consider
20 (t) F, + Cd
=fw+~)-q(l+4
z
= E(1+6)--
d6 x
=w
the
-
(a+()
68
combination
(3.4) of
functions
(t) F, + p (t) Fda
by (1.7) and F, = 5. ‘be functions o(t), where F,, F, and F, are defined p(t) are assumed to be bounded, continuous, twice-differentiable on the infinite time interval t > ta; moreover 0-l (t)
a* >
>
0,
o (t) #
‘lbe function V which has been considered with variable coefficients
0 whent>to will
(3.5)
be a quadratic
form
3’ (t, E, 7, 5, a, B, 8) = A (E”+ q2)+ V + p) P -
-
20 (A@ + AT@ + C:8) + Co2 (a2 + fJ2 + d2)
‘Ihe derivative of be a quadratic form V’ = -
(3.6)
taken relative
to equations
(3.4)
(3.6) will
20 (Ea + $J + f6) + a2 (a2 + B” + WI
K IE” + q2 + G2 -
also -
-w~(A~u+A$+C~~)+C~~‘(U~+~~+~~)+&-~(O~-~)+ ++pX2
=
.- KY (t, 5, q, b, a, B, 6)
(3.7)
1554
V. V.
hrementulo
On the basis of Liapunov's theorem on asymptotic stability, the unperturbed motion (3.1) turns out to be asymptotically stable if the function (3.6) is positive-definite and function (3.7) negative-definite in the sense of Liapunov (the requirement of the presence of an infinitely small upper bound in form I’ is satisfied under the given assumptions on the nature of functions o(t) and u(t)). Thus, motion (3.1) is asymptotically stable if Sylvester's conditions are satisfied for the quadratic forms
(Al, A,, A, and A, are positive numbers as small as desired). Each of these forms can be represented as a sum of three forms in the variables (5, a), (n, 13)and (5, 6). The Sy1vester conditions for these two-variable forms are
In order to evaluate the basic results, let us analyze these inequalities when A, = h, = h, = A, = 0. Tn this case inequalities (3.9) give c I> ‘4,
p I-- 0
Inequalities (3.10) reduce to ‘M(A
-c)ow'-11120'2)o,
The first relation in
P'(w2-
(i1.11) (3.12)
,,;$‘j
(3.12) gives (3.13)
Let us now pass to the selection of function u(t) constrained by inequalities (3.11) and (3.12). ""Len
the
A problem
on
the
relation
in
(3.12)
second Taking
(3.11)
into
stability
is
account,
of a spherical
gyroscope
satisfied.
we get
the
following
bounds
(3.15)
inequalities By combining (3.13) and (3.15) we obtain ditions (3.9) and (3.10) reduce when A, = . . . A, = 0
If
the condition
then, the
as is
not
following
state
A, =
. . . = h, = 0 is eliminated to
sufficient
verify,
conditions
to which
from the hypothesis,
inequalities for
the
(3.16)
(3.9)
asymptotic
and (3.10) stability
EQ>$>-4Kc++e,<0,
El, -
(f)‘>o
positive numbers as small where Em, E, and .sJ are strictly Inequalitiei (3.17) define a certain class of asymptotically motions
(3.1).
special
kind
Conditions of
in accordance
(3.17)
function
with
(3.6)
(3.14).
functions
p satisfying
widen
the
of
class
corresponding
by considering
F, + 2hF, -
is
the aid
of
with
CohF, + pFd2 -
some function
conditions
for
Let us examine under (3.1) does occur in the with
p(t)
speaking,
motions
along
as desired. stable
from a consideration
(3.1).
(3.12)
which
This
aim can
a Liapunov
(3.6)
of
were defined we can find
inequalities
stable
(3.17)
can
function
form
2V* = where A = h(t)
generally
differential
asymptotically
be accomplished a more general
were obtained
when the coefficients
However,
other also
give of
(3.1):
C>A +
of
con-
(;)‘>o
O>f>-4Kq,
difficult
on o:
($ )‘>o
$
C>A,
1555
the
2V, =
conditions
A) F,
analogous
to
the
n(t).
what conditions an asymptotically stable motion case of heavy gyroscopes. ‘Ibis problem is solved
quadratic @,
satisfying
2C (o $ -
-
200~
form +
(Gz
-
mgz,) (&
+
p@)4”
(3.18)
where 0,, o2 and o3 are defined in accordance with (2.2) and 0, coincides with F,. As is not difficult to see, the derivative of (3.18) relative to the equations of perturbed motion coincides with (3.7). Along
with
(3.6)
in the
given
case
we obtain
a
1556
I’. 1’. Krrmentulo
The author thanks V.V. numiantsev interest in the work and for helpful
and S.A. Kharlamov for their remarks while it was in progress.
BIBLIOGRAPHY 1.
William scope.
C. Pittman, .4R.S Journal,
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Loitsianskii,
L. G.,
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5,
N.G.,
mekhanike
4.
Akad.
7.
No.
with 4,
(On the
Appel' , P.,
Vol.
84.
Tcoret
gyro-
sfericheskogo bearing).
0. F.,
tela
(giroskopa)
axisymmetric Nauk
86,
pod-
PM! Vol. 19,
po
analiticheskoi
on Analytic
Mechanics).
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a portion
k chasti of
the
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variables).
1957.
No.
N.N., of
3,
icheskaia
Ob ustoichivosti
motion
dvizheniia
in-the-large).
Dokl.
Akad.
1952.
(Theoret
mekhanika
ical
Vol.
Mechanics).
1960. dvizheniia
Ustoichivost’ rigid
Raboty
Papers
respect
stability
Fizmatgiz,
Boichuk,
Akad.
21,
E. A. and Krasovskii,
SSSR,
1, p.
teoriia
a spherical
V. V. , Ob ustoichivosti
v tselov
6.
Mot ion.
Nauk SSSR, p.
MGU,
Barbashin, Nauk
of
dvizheniia. of
(On stability
Vestn. 5.
theory
Ustoichivost’
(Stability
Rumiantsev, nykh
Gidrodinamicheskaia
(Hydrodynamic
spherical
1955.
Chetaev, Izd.
Dynamics of an air-supported Vol. 32, No. 7, 1962.
na sfericheskoi body
(gyroscope)
CfkrSSR, NO. 1,
osesimmetrichnogo
pore
(Stability
of
on a spherical
tverdogo motion
support).
of
an Dokl.
1963.
Translated
by
N.H.C.