CONTEMPORARY WORK IN CELESTIAL MECHANICS
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Collection:
Document Number (FOIA) /ESDN (CREST):
CIA-RDP80T00246A012500080001-4
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RIPPUB
Original Classification:
C
Document Page Count:
8
Document Creation Date:
December 22, 2016
Document Release Date:
February 24, 2011
Sequence Number:
1
Case Number:
Publication Date:
March 22, 1961
Content Type:
REPORT
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i i 1 II I'_ III _
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/CENTRAL INTELLIGENCE AGENCY
ntains information affecting the National Defense of the United States within the meaning of the Espionage, Laws, Title
Contemporary Work in Celestial Mechanics DATE DISTR.
DATE OF
INFO.
PLACE &
DATE AC
STATE I I ARMY
(report entitled 'report to Commission
7 about the work accomplished in the USSR in 1958=1960"? M mission 7 is
that part of the International Astronomical Union concerned with celestial
mechanics. Tie report was prepared by M. F. Subbotin, director of the
Institute of Theoretical Astronomy,, Leningrad. Its bibliography contains
46 references. am C?0=N F-I D-E=ST-T-I-A-L? 50X1-HUM
116-\ C* I
LNAVY
AIR
AEC
0
22 Mar 61
U
INFORMATION REPORT ANFORMATION RERORT
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WJ. W016
R E P O R T
to Commission 7 about the work accomplished in the USSR in
1958 - 1960.
No attempt is made either to give a complete bibliography
of published papers (especially of those pertaining also
to the Commission 4, 17, 20 and 22 ) or to describe theo-
retical work in detail.
PROBL OF THREE BODIES
At the Institute of Theoretical Astronomy at Leningrad
the investigations on the final motion in this problem was
continued and some interesting results for the case when the
constant of energy is negative were obtained by G.A.Merman
C13. He has obtained also [23 a new general solution of the
problem of three bodies in the form of convergent series,quite
different from that of sandman. V.A.iirumberg [33 has studied
the relativistic problem of three bodies and has found{ 43
the corresponding corrections for the motion of the loon with
a completeness not yet attained. some particular cases of the
problem of three bodies related to the study of the Trojan
group of minor planets and to the Rabe's hypothesis on their
origin were investigated by t.*.A. Chebotarev and his collaborat-
ore [5,6,7, . dome cases of temporal capture in the elliptical
restricted .problem were found.by V.F.Froskurin and L. I.
itumianceva [93 .
At Sternberg Astronomical Institute, Moscow University,
some special aspects of the restricted problem were considered
by late N.D.Noiseiev 410J 13.K.shohigolev { 11j investigated
the "second Hill's intermediate orbit? as- a possible starting
poiat for the solution of the Bate lltte. problel.
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ware ao&eidor.et bar
2.
was-, P4:t4 to e.t..
ary an a , :1 . t `` these j*:erat;,.o a r er. ..do 'ed
by Y . rtie.!v 1
}
p story 4the a for s ol~tt 63
rasrcxted ' o b by
i1Z?~.w`'
THEORY
has proposed a new form of the development
of the disturb i ?' ,ction suitable for any value of the
mutual iocIina nn and more convenient than the form given
by 'Xisa:er d.
G.M.Bazhenov C183 has published two methode,baaed on
the Tshebyshev' a approximation, for computing the absolute
perturbations of a minor planet.
I.S. Jarow;-Jarowoi {193 has constructed some new prin-
ciples of the approximate theory of Ceres, which proved to be
in esbonl' al e$peement with the observation for the years
do
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UM B s
ha wo:rci n.t the principles
t e ,oat urn,.
4MPX-O'Ving the orbits, Of the
o 't rasa the o beervat ions witkh` sc r6x`
out by U.K.Kulikov and Yu. V. Batrakov-
of the artificial satellites were published by Yu. V.Batrakov
t 38J and I.D.Zongolkvitch CJ
1.I?dedov (40) has given a general survey of the
orbits towards the Moon.
G.N.Daboshin C 41, has studied the rotational mouveasnts
of the artificial celestial bodies.
74blsms of orbit determination of these
:liter were considered by Yu. V.Batrakov ~36J and T
M
.
.
M-neev 0373 .
Some results from the discussion of the observations
MISCEI4LA OUS WORK
M .S.Petrowekaja [42j by a generalization of the A.
" " rya oma1 orbit are actually convergent for
iher's method has shown that the Hill's aeries renraaont{Me
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L.$ bbott 43] He has also or
modification of the conventional
8 parabolic orbits,.
method for. the c' pat,4i; a
name ric`al,
character07
.itivsly
diflg el*?rs His theory confirms q;
1-knO n result of u.Brouwer that after a
K3/2 .
&nrest igated the aocumalatfon' of.
e or9 ; with the regard on the ranida.
The practical application
theory was investigated by A. S. tiochilina [46] .
order of
rid #i `'eretI:a , `eet:loa o .
of this
k B F R H S N C L S
Norman G.J. Bu11.Inet. aetr.Leningrad, 6, 687-712,1958.
L 2J Merman U.A. Bull. Inst . astr. Leningrad, 6,713-7322 1958.
C33 Bromberg V.A. A.Zh.35, 893-903,1959.
C41 Bromberg V.A. Bull. Inet . astr. Leningrad, 6, 733-756,1958.
t 1.
C gj
Chebotarev
C61 Chebotarev
C7~
Cho bo t arev
u.A. and Bozhkova A.J. Bu1l.Inet.astr.
Leningrad,7, 186-201,1959.
u.A. and Volkov M.S. Bull.Inst.aetr.
Leningrad, 7, 202-207,1959.
U.A. and Volkov M. S.Bu11.Inst. astr.
Le,mi.agrad, 7, 420- 421,1959.
83. Che botar. G.A. and Bozhkova a. J. Bull.Inst. aet r.
581-587,1960.
,c?va L.I.Bu11.Inat.aetr.
'?+ 92,l959.
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L 11} ihohigole B.M; . P zb
0127;.. go ov-''.A4 .1f
[14]. PoloZova
4 y3! , .A.. Bu1.l.l et. , tr.tie ingr?aa, 7s 4,22 44Q 959.
[16 Thor .~~ ,, Pu1:l. Ine>i . ate tr.. +aui rad, 7 r 64-9-6574 1960.
[151 PalQzova
18 Ba Ono* Ei. ., l nst. tr.I,eningradf7 X3..7].1959.
19 J ap at*'WO I.S. Publ. Sternberg astr.Inst.,28,25.-9O
i
1.
L203 Dub_os x. (~..N. Pabl. Sternberg astr.Inst. 28 121-148 1960.
[13 LuboshiA G. N. Pub 1. Sternberg aatr. Inst. , 28,14,9-160.1960.
~22J iuboahln G.N. Publ.Sternberg astr.Inet, 28, 161-170,1960.
C23] mybakov A.I .Publ . Sternberg aetr., Inst . , 28,171-202,1960.
C24j. Kybakov &.I. P ubl. Sternberg astr.Ins t . , 28, 203-248,1960.
L15j ?ybakov? A .I. Publ.Sternberg aatr.Inet., 28, 249-275, 1960.
[2'6] Yosaehevsky M.P. Publ. Sternberg aetr.Inst, 28, 277_2911960.
[273 Xasachevak,y M.P. yubl.Sternberg aetr,Inet., 28,293-304,
1960.
C28.1 Z'ofgolovitoh, ILA), J iill.Inst . ast r. Leningrad 7, 521-536
1960.
C2?] Pra ke ~l8 V. v u t I t. aa.t '.. a , -
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6.
L311 Jarow-Jarowoi M.S-Ball.Inet.astr.Leningrad,7,552-553,
1960.
c321 neletzky V. V.Artif.5atellites of the Barth Moscow I,
25-43,1958.
[3'3j Beletzky V. V.Artif.uate111tes of the Parth,Moscow, 3,
13-31,1959.
[34] Kislin M.i).Artif.5atellitee of, the Barth ,Moscow
3 .. W7, 1960.
C35] Sulikov, L.K. and batrakov, Y u. V. .8all.Inst. aetr
.Lenin_
C6]
[37]
r38.]
ft.
L3
9
[40
[41.
[42.J
C43 7
T4r
55.3
[46 ~
grad, 7, 554-569,1960.
batrakov Yu.V. Bull.Inst.ast.r.Leningrad, 7, 570-578,1960.
tsneev T.M.Artif.Uatellitee of the 1sarth,M1oecow, 4,
43-55,1960.
batrakov ru. V, Bull.Inst.aetr.Lontngrad,7)503-510,1960.
Zhongolovitch I.y.Bull.of the stations for the obser-
vation of the artif.Satellites,Moscow,12,196U
aedov L.I.Artif.Satellites of the 8arth,Moecow, 5,3-15
1960.
Duboshin G.A.Bu11.Inst.aetr.Leningrad, 7,511-520,1960.
Petrowekaja M.S.Bull.Inet.astr.Leningrad, 7,441-465,1959
Subbotin M.F. Bull.Inet.astr.Leningrad, 7) 407_415,1959.
Subbotin X.F.Bull.Inst.astr.Leningrad.7.416-419,1959.
Myachin Y.F. Bull.Inst . ast r. Leningrad, 7, 257-280,1959.
Soohilina J.S. Bull.Inet.estr. Leningrad,7, 281-286,1959.
. ~.F.Sub~otin
Director of the Inetit'ut?
of The.oretioal Astronomy
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