SCIENTIFIC ABSTRACT VSEKHSVYATSKIY, S.K. - VSESLOVSKIY, I.A.

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• Collection: Scientific Abstracts
• Document Number (FOIA) /ESDN (CREST): CIA-RDP86-00513R001961220008-2
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• Document Creation Date: November 2, 2016
• Document Release Date: September 1, 2001
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• Publication Date: December 31, 1967
• Content Type: SCIENTIFIC ABSTRACT

VS21H57YATSKIY, S.K, tVsekhsv7ats'kyif.S*KJ, doktor fit.-mat.nauk
!nternsti'6nal Geoph7vical Year. flaulm i ztqttia 7 no.6:21-24
Je 157. (MIRA 12:10)
kInternational Oeophysical fear, 1957-1958)

33-4-T9
AUTHOR: Vsekhavyatskiy, S. K. and Mashcheryakova-Babich, 0* .
TITLE: --D-i`i-tribution of th-e---if~ments of Orbits in the Eruption
Theory. (Raqredeleniye elementov orbit v teorii
izverzheniya).
PERIODICAL: Astronomicheskiy Zhurnal, 1957, Vol.34, No.4. PP-568-580
(USSR).
ABSTRACT: Vsekhsvyatskiy (Refs. 3 and 4) has shown that the
eruption theory can explain orbital characteristics of
short-period and periodic comets. Duklmovskii (Ref-5)
has argued against these conclusions but his results
are inadmissible because of elementary mistakes.
Dukhnovskii maintains that Soviet Astronomers have only
worked out the plane problem while already in 1934
Vsekhsvyatskiy had worked out the spatial case and
obtained results which clearly supported the eruption
theory.
The alm of the present work is to establish the
theoretical distribution of elements of orbits of short
lj~riod comets on the basis of eruption theory. The
following-problem is taken up-. to find the distribution
of elements of orbits of the eruption products which,
on the boundary of the sphere of influence of Jupiter,
Card 1/3 have a uniform distribution of directions and magnitudes

3-3-4-6/19
Distribution of the Elements of Orbits in the Eruption WneOXY-
of relative vi~]_ocities, if the latter lie within certain
limits. The upper limit is taken as 8.5 km/sec and the
lower as zero. The contra of the distribution of the
relative velocities is taken to be coincident with the
centre of the planet, i.e. the linear dimensions of the
sphere of influence are assumed to be small -compared
with planet - sun distance. The planet is assumed to
move in a circle and the attraction due to the planet
is neglected beyond the boundary of the sphere of
influence. These simplifications should not lead to
any essential errors.
A theoretical expression for the above distribution is
obtained and is in good agreement with observations.
A comparison of the theoretical and observed distributions
indicates that during the last two centuries short
period comets were formed as a result of eruption
processes in Jupiter's system. The value of the relative
velocity did not in the mean, exceed H = 0.23
(i.e. 6.9 km/sec5. This corresponds to a maxirmim
possible velocity on the surface of the satellites of the
Card 2/3 order of 7-9 km/sec.

33-4-6/19
Distribution of the Elements of Orbits in the Eruption Theory.
Using the known number of short period comets in the
Jupiter family (65 comets) the total number of cometary
objects thrown out from that family may be estimated.
This is of the order of 600-800.- It was found that
the number of short-period comets as a f)6n
.�tion of the
perihelion distance is proportional to q * , and
increases rapidly towards Jupiter's orbit for r>, A.U.
It is shown that Dubyago's hypothesis (Ref.9) of
condensation of short period comets in -the zone of
motion of Jupiter is inconsistent and erroneous.
There are 7 figures, 7 tables, and 9 references, 7 of
which are Slavic.
SUBMITTED: September 17, 1956.
ASSOCIATION: Department of Astronomy of the Kiev State University.
(Kafedra Astronomii Kiyevskogo Gosuderstvennogo
Universiteta)
AV AILABLE: Library of Congress
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VSXKMVYATSKIT, S.K.
Arend-Rolandis comet (1956 b). Astron.tair. no.180:10 My '57.
(MIRA 13:4)
(Comets--1956)

VSAMTYATBKIY. 3 -X~ -, ~ , - -
I , n-I - ~- -
..
. Brightness of Arend-Roland's comet (1956 h). Astron, tair. no.182:
1-2 Je 157. (MIRA Ilt3)
1. Kafedra astronomli Kiyevskogo universitata Imeni T.G. Shevchanko.
(comets--1956)

s r~l
E -0m; TIKHOV; KFIAVTASI; BAKHMV;
TEMO; ZVERNV; VASILIYFV; PARSHIN; V-S.--K-HSVYA A
LAZASVSKIY
MrkoB' comet (1957 d). Astron.tair. no.184:1-3 S 157.
(mIRA 11:4)
(Comets--1957)

VSEXU"ATSKIY, S.K.
Observntions of Area-Roland's comet. Astron.tair. no.154:7-10 S
(MIRA 11:4)
1. KafedrA astronomii Kiyevskogo gosudaretvennogo universitetn im.
T.G. Shevehenko.
(Comets--1956)

VSMSVTATSKIT, S.K.
Visual observations and evaluations of the brightness of Prkos'
comet (1957 d). Astron.tsir. no.185:6-8 0 157. (MIRA 11:4)
1.1[afedra astronomii Kiyevokogo univeraiteta im. T.S. Shevchenko.
(Comets--1957)

VSWSVYATS' PETRUSENED, A.M.
P.M. Lebedev, outstanding physicist and materialist (OP.N. Lebedev.
outstanding ph7sicist and materialist" by A.V. Shugalin. Revievied
b7 S.K. Veakhsviatelkyl, A.M. Petrusenko). Vienyk AN L%U 28 no.7:
73-76 Jl '57. (MIRA 11:1)
(Lebedev, Petr Nikolaevich, 1866-1912)

., and G. M. ITIKOL'SKIY
VSEaWIPU=LrL. S - _K
"Structure of the Solar Corona of' June 30, 195h"
(Total Ecllpse of the Sun, February 25, 3.952 and June 3D, 1954, TTanmetions of the
Expedition to ObBerve Bolar- Eclipsee) Moacow) IrA-ve Ali W8Rj 1958, 357 P.

y-KQAjt3atjnpvich [Vaekhaviatalkyi. S.K.J. Prof.:
M-MINMY, T.T. [Uziutynalkyi, V.-T.), red.; YMSOV, T.G.
ClUraeov, V.H.I. otv. za vypusk
(Contemporary science on the origin and evolution of celestial
bodies; data for lectures] Suchasna nauka pro pokhodzbowda
i rozvytok nebesnykh til;.materialy do laktaii. Kyiv. 1958.
24 p. (Tovarystvo dlia poshyrennia politychnykh i naukovykh
znan' Ukraino'kol HER, Uer.10, no.ZO).
(MIRA 14:1)
(Cosmogony)

~M PHASE I BOOK EXPLOITATION SOV/1692
Vsekhsvyatakiy, Sergey KonstantInovich
Malyye tela solnechnoy sistemy (Small Bodies in the Solar System)
Moscow, GostekhIzdat, 1958. 47 p. 25,000 copies printed,
I
Ed.: V.A. Mezentsev; Tech. Ed.: K.F. Brudno
PURPOSE: This popular-science booklet Is Intended for the general
reader.
COVERAGE: The author, a Soviet astronomer who specializes in comets,
describes small cosmic bodies such as comets, meteors, asteroids
and cosmic dust, and gives an explanation as to their or.igin, No
personalities are mentioned. No references are given.
TAUB OF CONTENTS:
I
Introduction
3
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.:Small Bodies in the Solar System sov/1692
Small Bodies in the Solar System 7
The Physical Nature of Comets 17
Comets, Asteroids, and Metisoric Bodies 23
The "'Age" of Meteoric Particles 26
The Origin of Comets, Meteoric Dust, and Cosmic Rocks
in the Solar System 28
Short-Period Comets and Thdr Formation 35
The Eruption Theory and the Solar System 44
AVAILABLE: Library of Congress
Card 2/2 M/Tax
6-18-59

PHASE I BOOK EXPLOITATION 666
Vsekhsvyatskly, Sergey Konstantinovich
Fizicheskiye kharakteristiki komet (Physical Characteristics of Comets)
Moscow., Gos. izd-vo fiziko-mat. lit-ry, 1958. 575 p. 2,000 copies printed.
Ed.: Samsonenko., L.V.; abch. Ed.: Akhlamov, S.N.
PURPOSE: This book is intended for astronomers, students, and graduate students
in astronomy. It can also be useful to others interested in comets, their
observation, and the history of astronomy.
COVERAGE: The book contains data on the nature of comets, their origin and
evolution., and a catalog of every comet ever known. The main part of the
book is devoted to a detailed description of the physical characteristics of
comets and the circumstances under which they were discovered. The book also
covers photometric study of comets and the results of a statistical study of
the absolute magnitude of comets. The last part of the book on the obser-
vation of comets is not a complete study, nor was it intended to be such. Re-
cognition for help in compiling the book is given to the author's wife, E. I.
Vsekhsvyatskaya, and to T. A. Vodoplyanovaya, G. M. Nikollskiy, and S. A. Glebcva
Card 113

Physical Characteristics of Comets
666
of the Department of Astronomy, Kiev University. There are 155 references for
Parts I and 11, 89 Soviet, 31 English, 25 German, 7 French, 2 Dutch, 1 Italian.
Six Soviet sources and 114 non-Russian language sources were used in the com-
pilation of Part III. In this section, by far the main part of the book, the
source material is listed after each entry of the individual comet Ix-ing studied.
TABLE OF CONTENTS:
Foreword
PART I. GENERAL DATA ON COMETS
5
Ch. I. The Nature of Comets 7
Comets in the solar system 7
The nature of comets and theories of their form 12
The physics and chemistry of comets 14
The evolution and origin of comets 17
Processes occuring on planets and the origin of comets 20
Ch. II. Photometry of Comets
History of photometric study of comets
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Ehysical Characteristics of Comets 666
Observation errors and the patterns of change in the luminosit-j
of comets 28
Works of N. Bobrovnikoff on photometric study of comets 32
Ch. III. Results of Statistical Analysis of the Elements of an
Orbit and the PIWaical Characteristics of Comets
Long-period and "parabolic" comets 37
Periodic and short-period comets 45
PART II.CATALOG OF ABSOLUTE MAGNITUDES OF COMETS 51
PART III,OBSERVATIONS AND PHYSICAL CHARACTERISTICS OF COMETS 83
Index of names
Index of comets
AVfJJABI;E: Library of Congress
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BK/fal
3a-4-58
557
571

VSEMaVYATSKZ, S.K. (Vaekbaviatalkyi.. S.K.)
I
Photographic and visual observations of Arend-RoIAWIB cftet-
' kh. no. 1:125-127 '58.
Visnyk Kyiv. un, Ser. astron.,, mat. ta me (MIM 3-4: 5)
(Comets-1956)

AUTH011:
TITLE:
Vsekhsvyatskiy, S.K.
8/035/61/000/003/045/o48
A001/A101
Luminosity of the comet 1956 h (Arend-Roland)
PERIODICAL: Referativnyy zhurnal. Astronomiya i Geodeziya, no. 3, 1961, 63-64,
abstract 3A576 "'Visnyk Kyvivs'k. un-tu", 1958, no. 1, Ser. astron,
matem. ta mekhan., no. 1, 129 - 130)
TEXT: The luminosity and magnitude of the comet were estimated from ob-
serva tions with field glasses (50 mmx7) and a binocular tube and a comparison with
off-focus images of the neighboring stars. The observations were conducted in
Moscow, Kiyev and Crimea (Crimean Astrophysical Observator-J) from Januury 23~to
June-4, 1957. The maximum luminosity of dn took place on April 25, and by the end
of June the luminosity decreased down to 7M8.
S. V.
[Abstracter's note; Complete translation]
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S/035/6 1/000/003/046 /0 4 8
A0011A101
AUTHOR., Vsekhsvyatskiy, S.K.
TITLE: Visual observations and estimates of luminosity of' the c0met 1957
(Mrkos)
PERIODICAL: Referativnyy zhurnal. Astronomiya i Geodeziya, no, 3, 1961, 54, ab-
stract 3A580 ("Visnyk Kyvivslk un-tu", 1958, no. 1, Ser. astron,,
matem. ta mekhan., no. 1, 131-133, Ukrainian, Russian summary)
TEXT: The comet 1957 d was observed in Kiyev from August 7 to September 14,
1957. Field glasses (50 mm x 7) and a 70-mm tube were usef for estimating its
luminosity. Its stellar magnitude varied from 2TO (on August 7) to 5T2 (on Septem
ber 14). The tail length and the color of the comotar~j head were noted. During
the first days the nucleus was bright-yellow, the tail and the head were of a.red-
dish shade; the parabolic outline of the head was well visible, On August 9,
with magnification 100, elongation of the nucleus in direction perpendicular to
the tail axis was noticed.
S. V.
(Abstracter's note: Complete translation]
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VSEKMVYATSKIY S.K. [VsekhavigLtslkyi, S.K.)
Photometry of comets. Visnyk-Kyiv. un. Ser. "tron., mat, ta
mekh. no. 1:135-14A '58- (MMA 14:5)
(Photometrys, Astronomical)

AUTHOR. 3ablch, 0.1. and 33-35-35-1
Kazyutinskiy, 7.V.
TITLEs On the 'elie-stior Con3ern-Ing the Capture Hypothesis of the
Formation of 3hort-Periodi,~, Comets 'K voprosm. o gipoteze
obrazovaniya korctkoperiodiche5kikh komet putem zakhvata)
PERIODICAL: Astronomiche5kiy zhurnal, 1958, 1101 35, Nr 39PP 4730-478 (USSR)
ABSTRACT: The present paper has a polemic character. Starting from the
captuze hyp-ithesizi Shteyzis ERef 71 tried in 1957 to explain the
absen--e of r6trograde motiGns for short-periodic comets by
th-:,ir disintegration and obt-gin,3d rebults contradictory to
Nevrton~s wall'.-known resulta [Ref 61 . These contradictory re-
sults cause the authors to investigate the distribution of the
capti.ired orbits in the plane of the Jupiter orbit. It was sup-
posed s A c!rcul,%r orbJ.- for Jupiter, disturbances by the sun
and othar plaw-,ts can br, neglected et-.. The method of Laplace
(transit'~r~n to the planetc-central motion) vas used. The cal-
culation of 216 orbits showed, %
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On the Question t-te Cept-,:,re Hyp0thesis
of the Formation of Sh.)Tt-Periodi,; Comets
parabolas hyperbolas
O,n,6 - I , 0;5 > 1 V05
33-35-3-16/27
ellipses
G