SCIENTIFIC ABSTRACT FESENKOV, V.G. - FESENKOV, V.G.

• Document Type: CREST
• Collection: Scientific Abstracts
• Document Number (FOIA) /ESDN (CREST): CIA-RDP86-00513R000412920010-2
• Release Decision: RIF
• Original Classification: S
• Document Page Count: 99
• Document Creation Date: November 2, 2016
• Document Release Date: August 23, 2000
• Sequence Number: 10
• Publication Date: December 31, 1967
• Content Type: SCIENTIFIC ABSTRACT

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FESENKOV, V.G.; ROZHKOVSKIY, D.A.
Th-e origin of the stars. Dokl. Akad. Nauk OSSR 84, No-5, 917-18 152.
(FA 56 no.66825270 133) (MLRA 5:7)

~PHASE I TREASURE ISLAND BIBLIOGRAPHICAL REPORT AID 384 - I
BOOK Call No.: QB981.F4
.Author: FESENKGV V. G., Academican
Full Tit 1;-=- DEVELOPMENT OF CELESTIAL BODIES FROM
. CONTEMPORARY DATA
Transliterated Title: Proiskhozhdeniye i razvitiye nebeanykh tel
po sovremennym dannym.
Publishing Data
Originating Agency; Academy of Sciences of the U.S.S.R.
Publishing House: Publishing House of the Academy of Sciences, U.S.S.R.
Date: 1953 No. pp.: 64 No. of copies; 25,000
Editorial Staff
Editor: None Tech. Ed.: None
Editor-in-Chief: None Appraiser: None
Text Data
Coverage: The book is a popular treatise in cosmogony. Some of the
information appears to be of interest: 1) the results of observa-
tions made with the meniscoun telescope (photoprint of the tele-
scope on p. 6 with not other details given) of D. D. Maksutov, con-
structed by B. K. Ioannisiani and installed in 1950 at an 1500 m.
altitude in the Alma-Ata Mountain astro-physical observatory, which
is claimed to detect stars with a luminosity 1 million times smaller
V3

Proiskhczhdeniye i razvitiye nebesnykh tel AID 384 - I
po sovremennym dannym
than those visible to the naked eye (p. 25). Pictures were taken of
nebulae, in the red Fz line and with a yellow filter. 2) Academi-
cian G. A. Shayn and V. F. Gaze, of the Crimean astro-physical ob-
servatory, using special very sensitive photoplates with a red
filter, isolated the emission of the red hydrogen line k, and this
made possible for G. A. Shayn to discover many new gas and dust
nebulae (see "Izvestiya Krymskoy Astrofizicheskoy Observatorii'll
and also to establish some new structural properties of known
galaxies (pp. 24-25). 20 photoplates, graphs and diagrams are
given in the book, some of them deserve attention.
The book Is well written and descripe8 the gaseous and dust theory.
(without giving credit to von Weizsacker, G. P. Kuipe.r, D. ter Haar)
of the origin and development of the Universe, disregarding the new
nuclear reaction theory. No references are made to foreign scientists.
TABLE OF CONTENTS PAGES
Introduction 3-4
Our Stellar System the Galaxy 5-12
Nature of Stars 13-22
Origin of Stars 23-38
2/3

Proiskhozhdeniye i razvitiye nebesnykh tel AID 384 - I
po sovremennym dannym.
PAGES
Development of Gaseous and Dust Nebulae 39-47
Origin of the So,lar-System 48-63
Purpose: For popular information
Facilities: None
No. of Russian and Slavic References: Only names in the text, all
Russian.
Available: Library of Congress.
3/3

71zsrlari.c~", V. o. i zk

V. G.
"Cbnference Held on Ifte Alma-AtA on the' Problem of Possibility of Life on other
Planets, in C6n-nedtion-'vith'~l6~ks-~of-the',")ecti6'n of Asti
-ob6tarq,, _azakh`SSR Guided
by the Presidium of the Academy of Sciences, Kazakh SSRj 2547 September 1952.,11 by
V. G. Fesenkov., Astr Zhur, Vol 30., No 2, pp 244, 14ar/Apr, 53.
Reports on-topics wwo made by G. A. Tikhov,, N.- 1. Kucherov, A. P. Kutyreva,
o. 7.,Troitskaya., V. G. Fesenkov., L. B. Golosnitskiy. OpLnions d-Iffered.
~51T:L2.

USSR/Astronomy Polar Radiation, Breaking Effect NOV/11ec 53
uBreaking Effect of Polar Radiation on Non-Spherical Bodies," V. V. Radzievskiy
.and Y. F. Razbttnaya, Taroslavl State pedagogical Inst it Ushinekly
Astron Zhur, Vol 301 No 6, vp 616-618
'Attempts to prove that formula obtained by H.~Robsrtson (M. N. 97. No 6 (1937)
and V. G, 79senkov (tbid 23, 6 (1946)- equating the tint after which a black
spherical body will fall on the sun,~due to the breaking affect of solar rad-
iation, my also be aimlied to nonspherical bodies. Roe 2 Kar 53

KRINOV, Te.L.; FXSJNKOV, V.G., akademik.
Certain regularities.in the falling of stone meteoriteo. Dokl.,AH Sm
90 no.6:979-982 Js 153. (MLRA 6:6)
L Akademiya nauk 353R (for Fesenkov). (Meteorites)

IDLIS, G.H.; Y=TKOV. V.G., akademik.
Criteria of~gravitational resistance and distribution of spheroidal clusters
In galaxies and sturs in spheroidal clusters. Dok.AN SSSR 91 no.6:i.)05-
1308 Ag 133. (MIJUL 6:8
1. Akademiya nauk SM (for Fesenkov). 2. Astrofizicheski.V institut Akademii
Nuuk Kazakhakoy SSR. (Hii4 way)

Tiw Z;*=ittee on Stal Itt Prizes OrAr tLe 1;o~il of kInIxters LZZR~ L'I Qe 'I'leid 6 4t
am
Inv"tIand *an&Auc*a "t We fall*wing setwitific vorks, papAar aeieu-
titt-i booke, and textboots Uve been 611Wd1tU4 for wiVetition for Stalin Prizes ror
thin pasa 1952 8AA 4~53# (30"twifta rwiturs. Mu"ww, No. 22-401, ZO Fab - 3 Apr 1954)
Title crVork,
Fesenkov, V.G. Research on the processes os Acadexy of Sciences. Kazakh SSR
Rozhkovskiy, D.A. the origin and development of
stars (series f articles)
July 1.j-,-4

od-tattlelated, by
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S., Asta viai'j, Problem, M the. counfor
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of the Coiantq4q~r. ~~FL-vlku~" V. G:. Gaseous tilil of the earth [ditlerlm" -
M. ".'Tho tattue of the zwnterglow-. E)i B, Tho p~~wwro of
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~ollvct-~d ald tr
4phe?a tiid the Ru--lan pJ
of ~abavd, cited Rwisiaii paPerg _p~IMU-4he fi~it'LdOoll
war " eo.
ho campktia',fiaea ationioUtheAst, :palier-s- all I UVC,

6mt reru-se (Vw~sdmlt the pos-Alillt of A gaswmi "Wrl

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- - - - - -- - - -

VEM .; TULENKOVA, L.No
wpn~-
Motion of the Sikhote-Alin' meteorite through the solax system.
Metaoritika no.11:138-152 154, WaL 8:3)
: : (Meteorites) "' . ''

AID P-56
Subject USSR/Astronomy
Card 1/2
Authors Fesenko
G., Academician, and Rozhkovskiy, D. A.
Title On the Radiation Energy from the Filaments of Nebulae
and on the Narrow Stellar Trails connected with them.
Periodical Astron. zhur., V. XXXI, 1, 3-14, Ja - F 1954
Abstract Results of photometric determination of 20 stars in 4
stellar trails in filaments of the gaseous-cloudy
nebula in Cygnus between NGC6960 and 6992-5 are given.
The stars areassumed to be sub-giants. Radiation
and evaluation of space density are estimated. Two
photo negatives of the trailB, shown on 2 plates, were,,
made with D.' D. Makautov's neniscus telescope (opening'
500 mm, light power 2.4) insk;aTLled in 1950 in the
Gornaya Astronomical Observatory. 3 graphs show
samples of these stellar trails. The article is based
on works by J. Chamberlin, Hynek, and E. R. Mustell.
The bibliography lists 4 references, of which 2 are
Russian..

Astron. zhur., V. XXXI, 1, 3-14, -Ja F 1954. A lb
(additional. card)
Ca rd 2/2
Institution Gornaya Astrophys. Obs. of the Acad. of Sci. Kaz SSR
Submitted November 4, 1953

AID P - 372
Subject USSR/Astronomy
Card 1/1 Pub. 8 2/12
Authors Fesenkov, V. G., Kazachevskiy, V. 14. and Tulenkovaj L. N.
.Title 0~ ~W~ i~tLn of Filaments of Nebulae NGC 6960 and
NGC 6992-5 in the Constellation of Cygnus
Periodical Astron. zhur., V. 31, 3, 224-230, My-Je 1954
Abstraci In comparing the photographs of nebulae NGc 696o and
NGC 6992-5, made at intervals of 22 and 50 years respec-
tively, the displacement of individual very clearly dis-
tinguishable filaments was established. The velocities
are considerable (in tens km. per see.) and there is a
tendency in some parts to spread out. Two photoplates,
two sketches, and equations. 4 references of which one
is Russian.
Institution Academy of Sciences, Kazakstan SSR, Astrophysical Institute
Submitted April 3, 1954

AID P - 423
Subject USSR/Aetronomy
Card 1/1 Pub. 8, 2/16
Author Fesenkov, V. 0.
Title Luminosity of a Hydrogen Nebula under the Action of
Many Stars
Periodical : Astron. zhur., v. 31-4, 312-317, Jl-Ag 1954
Abstract : Determination of density of a mainly hydrogen nebula,
activated by radiant energy, can be done by determining
not only the number of ions and free electrons, but also
the number of neutral atoms. A special formula of ioniza-
tion is given by the'author, which, when applied to the
fibrous nebulae in Cygnus, permits the determination of
their significant densities. 1 graph and 7 references.
Institution Institute of Astrophysics, Acad. of Sci., Kaz. SSR
Submitted May 26, 1954

KURMOV, V.; FMZNKOV V,G.; ROZHKOVSKjy, D.A.
1--! -*-
On V.Xurganovlo article IV.G.Fesenkoy and D.A.Rozhkovskii's
research in the development of stare from filaments of gao-dust
nebulae 0 Astron.shur 31 no.6:556-557 M-D 154. (mm 8a)
(itars) (Nebula;)

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FESZNKOV. V,,G.. demik.
Visibility of narrow stellar paths conneoted with filawnts of
gaseous and dust nebulas. DokI.AN SSSR 95 no.2:2)3-2)6 Kr '54.
(KL'RA 7-3)
1. Institut astrofiziki Akademli nauk Kasakhokoy SSR.
(Stars-Clusters) (Nebulas)

-li,' %Al=tA V& V~w "
!?A~ . - L - _

FESENKOV, V.G..
Principal scientific achievements of the Institute of
Astrophysics of the Academy of Sciences of the Kazakh
S.S.R. Isy. Astrofts.Inst. AN Kasakb.SSR I no.1/2:3-24
155. (MLEL 9M)
(Kazakhstan--Astrophysics)

Phenomena observable on Jupiter; origin of the dark belts.
Izv. Astrofts.Inst. AN Kazakh.SSIt I no.1/2:239-251 '55.
(nu 9: 10)
(Jupiter (Planet))

Zr-
TONNKOVI.G.. almdemik
On the problem of micrometeorites. Meteoritika RO.12:3-13 155.
(Meteorites) (MIRA 8:10)
8 I-WHIMPIRMI,~10, RUQZR
~6i 'AR

IN,
PBSMOV,V.G. akacl*mik
Observations on the motion of the Sikhots-AlAn meteorite in the
atmosphere. Mateoritika no.12:72-74 155. (MLRA 8:10)
(Meteorites)

T.G., ajmdmik.,
Idyances In meteoritics daring 1952. Xoteeritikit se.13:9-14 1555..
(Meteorites) (KrJIA 9:2)
J7

YSSENKOIF.V.G.
On the theory of diurnal sky brightness in the case of a spherical
earth. Astroneshur. 32 no.3:265-281 My-Je '55. (KERA 8:8)
1. Astrofisicheekly Institut1kadeall neuk iazakhokoy SSR
(SoUr radiation)

Problem of the origiu of stars. Astron.zhur.32 no.4:314-325
Jl-Ag'55- (MIRA 8:10)
1. Institut astrofizild Akademii uauk K&z.SSR
(Staro)

Rro age",

phas.but -takIn

th_-
ing-', o-. a *a

on Ifi; the M,

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PstH 2 2- %b*-,22:---: ,16X.1
Jul 688A

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or.
the ~. biltin -is
-from. the -sun - - th
~46f6rance: -.(3-944)~
Natitution f- -~U
-v- 7

--SBVMYY. Andrey Boripovich;'"" akademik, otvetetveaW
redaktorl YAFMOV. Tu.I., redaktor x atellstva; USHIQ, R.S.,
tekWAchookly rodaktor
CSO14r pbyotcal Piiiks solntsa. Kookwa, Ir-d-vo Akademit rAuk
SSSRV, 1156,:158~~Ps (MLRA 10-2)

OPARIN, Aleksandr Ivanovich: J29MRV, Vamilig Gricorlyvvich; PIRRILI, Ta.G.,
redaktor; POLYANDVA, TI,B., to es N&Lktor.
[Life in the universe] Zhiznl vo Toelennoi. Nookya, Izd-To Akadoull
nauk SSSR, 1956. ~22 OM 19: 6).

w-
I .
11sur Uhe Certaine Bande d'Adsorption dans 1e Spectre du Ciel Diurne,"
Spectralphotometric observations: made by the Obsen~atory of the
Astrophysical Institute., Alma Ata,, USSR$ confirm the existence of a weak adsorption
band at 7,436a in thh spectrum of the night sky. It is supposed that this is
produced primarily from floating dust in the high portions of our atmosphere.
A paper presented at the 7th International Astrophysical Colloquium,, Liege,
july 12-14,, 1956
SO: 568946

Sam
ftsur la Composante Atmospherique de la Lumiere Zodiacale,n a papei-
presented at the 7th International Astrophysical Colloquium, Liege, Jul 12-14,, 1956.
Photometric,abservations of the zodiacal light made by expeditions
of the Astrophysical Institute at Alma Ata, USSR, point to eonsiderable charge in the
aspect of this phenomenon depending upon the position of the ecliptic with respect
to the horizon,
SO: 568946

Sm.
,
f

tv
'a
w, I ~,,
vil-s tbig slucs1iiiiii A,I:
t

-, ~6
614-521
, Enghz-.I., UIIIIL:kf..
.
The wth~~, iuvestig~jcs die nit.-tion u! aoici, in tht

gravita
yova; field of (I spherej having all ;oullk)~phk lv! of
dr-i- force i5 ;l%:;ujiwd it~ 1-.t
proplDrUpp to tha,vCocity re afive t.) th-, -ttiu
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reswti;:Pbf~in~&d the first
rather d ffictzlt I r- In I f t hv 'I
MISIstant "It-dwol

FF,sENNOV, V.G., almdemik.
Introduction. Irv,,Astrofts.Inst. AN Kazakh. SSR 3 no.4:
4-6 156. (paju 9.-,10)
(KazakhatI#in-Astronoa7)

"Ils in. Achievements of tlx! Astrophysics Institute in the Peroid
of its &xistence ('1945-1955)"
Izvestiym Astrofizicheskogo Isntituta, Vol III, i1c 4, 1956, PP 33-45
Translation M-3,053,054, 4 Jan 57
-i-A-1 LI-1 haa
UR

-FESEMOV, V. G.
On the origin of stars. I.zv.Astrof ix. Inst. AN Kazakh. , SSR
3 no.4:53-67 156. (Mrl?A 9::L0)
(Stars)

akademik.
Origin of the soL&r or-stem and the problem of life il the
universe. Va8tAN Xuakh.SSR 12 no.2-3-13 7 156.
(SO3Ar BYltem)(PlUralitir of world@) (MIRA 9:6)

FXSBNKOV, -'.G., akademik,
Advances in meteoritics in 1953 and 1954. Notooritika no,14t-5-13 1156,
j,. (KMA 101: 1)
Nteorites)

YES . I or" - - f~~ mik.
... I,
Various aspects of occurence of cosmic dust. Meteoritika no.14:92-
1010 0560' (MLRL 10:1)
(Cosmic dust)

FESINKOV, Y.G.
Mateorit as and thoir role in the cosmogony of the eolar system.
Izv.Krym.astrofis,.ob8er. 16:228-238 '56. (MINA 13:4)
1. Institut astrofisiki AN K"SSR.
(Metsolrites) (solar system)

Colloquy on molecular astrophysics in Liege. Vest. AN SSSR
26 no.10:52-54 0 156. (MLRA 9:11.)
(Liege-Aoirophysice--Congresees)

FESMKOV V G - DIVARI, N.3.
~ ~, 1W
The problem of zodiacal light in connection with the International
Geophysical Year. Aistron.zhur.33 no.3.*391-403 '56. (MLRA 9:10)
l.Astrofizicheskiy Institut Akademii nauk KFtsSSR.
(Zodincal light)

FESMOV V.G
The problem of lifet on Mars. lstron..zhur.3.3 no-3:440-443 My-JP
'56. (MLRA 9:10)
l.Astrofizicheakiy institut Akademli nauk KazSSR.
(Hars (Planet) I'

Chomaoterls-ilis of,'!~bs ~t on d a itatisg..~q4y- in a rise isting
VAT
33....uqG'.4;.614-62i nAg--156.: (JURA 9:11)
I. lusittat "tiotillik Akadnmii nmk Usakhskoy SM

YESLINKOV V G
Atmospheric com ponent of zodiacal light. Astron.zhur- 33 no.5:
708-714 S-0 156. (MLU 9:12)
1. Institut fiziki atmoefery Akademil nauk SSSR.
(Zodiacal light)

FESENEDV. V.G.
Meteorites in studying the cosmogony of the solar system.
Astron.xbur. 33 no.5".1767-777.4-4 156. (MLRA 9:12)
(Meteorites) (solar system)

---- - ------
FESENKOV, YtGI. . ~
'wMw- - -
Seventh international colloquy on "Molecules in cosmic bodissO
in Liege. Astron.shur. 33 n0-51779-784 S-0 '56. (HLRA 9M)
(Liage--Astrophysics--Cor,gresses)

-- i -- - - - - - -- -- -. --- - -- - --- - - -
FBSBNKOV, V.,6-1
q~,-
Observing the total lunar eclipse of May 24, 1956. Astronetsir #
no.1?2-.19 Ag 156. (MMA 10:1)
(Iolipses, Imnar-1956)

IDLIS, GrigoAy Hoisayevichi starshiy asuchnyy sotrudaik. SlIK21g.T.G.,
akademik, otyatotvennyy redaktor; PMLI, Yu.G., redaktor
izdatelletva; HOVIKOVA, B.G., tekhaicheakiy redaktor
(Cosmic matterl.tosmichaskala materiia. Moskva, Izd-vo 4Lkademii
nauk SSSR. i957- 124 p- (HLRA 10:3)
l..Al=-Ata. Xamenskoye plato, Astrofizichaskiy inatitut Akademii
nauk Kuz,SBR (for Idlis)
(Cosmography)

,,.ZLaZCQV, V. G.
"Development of Astronomy in Kazakhstan," p 2477. in Science in Kazakhstan durinfi
the Forty Years of tbe Soviet Regime. Alma-ata, Izd-vO All Kazakhskoy SSR, 1957. 452P.
Te-d. Satpayer, K.-17.-
'This is a collection of ar.ticles (20) compiled by 24, authors on various aspects of
scienatific progress in Soviet Kazakhstan. One third of the articles also deal with the
progress made in *the main fields of indust.rial endeavor. The articles on the development
of science survey the main.aontributior~s made in the respective branches by Kazakh
scientists, and enumerat-e and describe the existing scientific institutes, organizations,
and universities. A large number of scientists are mentioned and their fields of interest
stated.

---- ------ -
F ESEITKOV, V.G.
"On Star Chains and Dark Filaments in Galactic Nebulae) 4 p.
paper submitted for Third sMosiuw Ion Cosmical Gas Dytiaraics, Cambridge (I'lass
24-.29 June 1957.
Trans. .Available
B-3,101,248, 1 Apr 58
~-4
, NOW -0-
H PIN

- FIE GENKOV. -7-. - G --- - - ---- - ---- - - - -- - -- -

N YN' V,
AUTHOR: Krinov Ye L.
TITLE: Chronicle: International Conference on Interplanetary Matter
-
(Khronika: htezhdunarodnaya Konferentsiya po iziezhplanetnoy
materii)
PERIODICAL: Geokhimiyat 1956f Nr 1, pp. 96-96 (USSR)
ABSTRACT: The International Congress on Interplanetary Matter took place
at Jena, German lemocratic Republic from October r tq_October
11?2, 195 . It was organized by the German Academy of Sciences.
,c-About 100 representatives of 11 countries took part in.it.
The Soviet Union was represented by Ye. L. Krinov, Scientific
Secretary of the Comittee for Meteorite Science of the AN
USSR9.by the Scientific Assistant of this comittee L. G.
Kvasha, and by V. S. Safronov, Scientific Assistant of the
Institute for Geophysics of the All USSR.
.The Soviet delegation gave ten of the thirty reports'heard
there-'
V. G. Fesenkov, Member of the All USSR: The Northern Zodiacal
Light
V. G. Fesenkovt Member of the AN USSR: The Pressure Wave at
Card 1/3 ______~_the Fall of the Tungusska Meteor in 19o8

Chronicle: International Conference on Interplanetary Matter 7-1-11/12
Ye. L. Krinov: The Mechanism of the Destruction of Meteoric
Bodies in the Atmosphere, and qheir Original
Forms
L. G. Kvasha: Certain Types of Stone Meteors
B. Yu. Levin: On the History of the Investigation of the
Variation of Meteorite Frequency
B. Yu. Levin: The Origin of Meteors and Comets
A. P. Vinogradov, Member of the AN USSR, I. K. Zadorozhnyy and
K. P. Florenskiy: The Contents of Inert Gases in the Sikhote-
Alin Iron Meteor (published in GC, 1957, no. 6)
N. N. Pariyakiyand L. M. Gindilis: Investigation of the
Luminiscence of the Green Band 5577 in the
Night Sky in the Counter-Glov Region
(Idaledovaniye svecheniya zelenoy linii 5577
nochnogo neba v oblasti protivosiyaniya)
1. S. Shklovskiy: The State of Ionization of Interplanetary
Gas and Its Significance for Certain Geophysical,
'Problems
The conference decided to publish all reports in special
editions of the following periodicals:
Card 2/3 Astronomical reports in: "Die Sterne";

Chronicle: International Conference on Interplanetary Matter 7-1-11/12
Reports on the material consistency of meteorites in;
Tk~emie der Erde".
AVAILABLE: Library of Congress
1. Reports-Bibliograpby .2. USSR
Card 3/3

FISINKOV, V~091 akademike
Observation of Mars during favorable opposition in 1956s Vest*
AN ZmakheSSI 13 noml(142)1?2-31 A 157. (KLRA 10: 4)
(Kars (Pla"t)-opposition,1956)

'AUTHOR: - F6senko -V.- G.---
TITLE: The early thermal history of the Earth. (K voprosy o
ranney termicheskoy-istorii zemli).
PERIODICAL: Astronomicheskii Zhurnal, 1959., Vol-34, No.1, pp.105-119.
ABSTRACT: An attempt is made to collect together known geological
and astronomical facts relating to the early thermal history
of the Earth.
The continents consist, in the main, of granite, and the
origin of the latter must be considered first. It appears
that the only PO Bsible explanation is that the granite
crystallised out 'qf,hotmagma. This should take place at
temperatures in excess of 10000. -The problem is -considered
in ref a., (2.
The origin. Of -the 'continents must also be consideried: in.
connection with the general problem of the formation of the
Earth as awhole.,_-~The problem.iB considered in refs..0 10)
but -no unique:conc-lusion has been reached.
The problem of the evolution of the Rarthl.s atmoST)here
and the formation of oceanic basins must also be 6onsiZLered
in connection with the earliest thermal hist2 of the Earth.
,
The -atmosphere has ~a . secondary origin. As is noimoxygen
was -originally produced by 'green plants and by pl$xnkton in
the oceans. Nitrogen originated partly from plants but
mainly in the interior of the Earth. Of the original
atmosphere. only an insignificant, admixture of inert gases
The water of the oceans is supposed to have originated
in the interior of the. Earth a~ the latter was cooling down.
Thus, for exa .mplel.during a volcanic eruption a great amount
of water is emitted, and this later returns as rain. It has
been shown that mg,gma is Capable of containing up j;o 10% of
water vapour (by yite) under a suitably high pressure* However,
a similar process would be possible with an originally cool
th
Ear
which was gradually warmed up through radioactive
disintegrations. Thus, the existence of the oceans is a
Fst-Or-TOf -the Earth. (Cont.)
strong argument in support of the hypothesis of an original 1y
hot surface of oU37 ]planet. (12 - 14).
'Deep furrows, valleys, and mountains should also have a
direct relation to thethermal history of the Earth. They
exist at the bottom of the oceans, in addition to the great
canyons. These Canyons can be assumed to have been caused
by gigantic underwater currents which were caused by the
collapse of continental masses in the different periods in
the Earth's history,, E.G. at the end of the glacial periods,
during a rapid melting of ice, or during earthquakes. The
effect of great convective currents under the Earth's crust
is considered by Mellard (19). (See also refs. 15-18).
The distribution of radioactive elements is of interest
from the point of view.of the evolution of the globe.. The
main radioactive elements (Uranium and Thorium) ar
trated in th e donoen-
e upper~4yers.of_the Earth. Goldschmidt (21)
considers that the 43LtOms Of uranium and thorium are too bulky
to enter into' sili -
Cate lattices during the process of
crystallisation. Thus; as the internal parts of the Earth
_~-the
began to cool down,- atoms Of uranium and thorium were
Squeezed out" in the out-ward direction. This would e=lain
4-1- Z- -4-V.-%~._A__- ___: - _ ___ , .-

The early thermal history of th-e-Earth~.-(Gan-t----)
produced when a dispersed medium contracts to a smaller
volume (potential energy transformed into kinetic energy);
(ii) Radioactive disintegration; (iii) Transformation of
chemical energy into heat (refs. 33-34); (iv) The differen-
tiation of the terrestrial matter according to its density
may have some effect on the thermal regime of the Globe.
One can easily show that, even if the Earth was formed
in a single gravitational condensation, enough energy must
have been produced to bring it into a molten state. In such,
an incandescent wtss convection currents are inevitably
produced and lead to a sufficiently rapid cooling. As was
shown aboye, radioactive elements are brought to the surfqce
during this process.,'and so their influence on the thermal
state of the Earth become minimal.
The origin o:C the Earth is considered to be not in a
quasi-meteoric dust-cloud captured by the Sun from a
hypothetical dust nebula, but in a medium consisting of both
gas and dust, which surrounded the original Sun and has a
chemical structure identical.with it (refs.35-4i).
Spitzer s theory of the differences between blars and the
Earth K42) are summarised. It is thought that the absence of
water on Mars is.probably a result of volcanic eruptions
which occurred after the complete cooling down of this planet.
43 references, 20 of which are Russian.
I I Reed. Dec. 7, 1956.

414
New of the Astrophysics Institute (Cont.) 382-3
Idmiso G~X. Basic Features of the Observed Astronomical Universe
,Xnhabitable - Cosmic System
~W Typical Characteristics of an: 39:
NikollsIdyj G.Me' Problei of Night Glow in the Red and Green Lines 55
Nikollskiy, G.Sh. Indicatrix of Ught Scattering in the Ai=osphere
in the Nearest Infrared Region ofthe Spectrum -65
Tulenkova., LiN Deteridnation of' the Oscillation of Star TM80i
According to Obser7ationa of the Observatory of the Astrophysical Institute 74
Obashev, S.O. Polarization of tk.* Prismtic Spectrograph 79
B4)yko,, P.N.. Reflectability of WMagnesium Screen 82
Griforlyeva,, N.B. Investigation:'of Clusters NOC 752 and NCIC 6940 90
KVAILAZZI: Library of Congress I-
Card 3/3
7-15 )0

CRLOV, Sergey Vladlmirovich; -,akndemlkg otvatetvenrqy- red.;
NOVIKOVA, Ye.N., red izd-va;SMCMMO, L.T., red. izd-va.
Cibture of 'Comets] 0 prirode komet. goskva, Is& vo Akad. nauk SSSR,
1958. 187 ps' (MIRL 11--7))
(comets)
77~
3- -,A,R lip
. =jg,

-4-(
-A -)v
t PHASE I BOOK M(PLOITATION SOV/31388
SOV/37-M-15
Akademiya nauk SSSR., p0 meteoritam
statey,, v3rP. 15. (Meteoritiasj Collection of
Articles, No 15) Mosoowp 1958. 193 P. 1,300 copies printed.,
Errata slipinserted in No 16 for No 15.
I _y.G._Feser*M Academiolani Deputy Reep. Ed,: Ye.L. krinov;
Ed.
Ed. of Publishing House: I.Ye, R&Winj Tech. Ed.: A.P.
Guseva.
PU9POSE: This publication is.,intended for astronomers., geophysi-
cists, astrophysicists, and other scientifio'personnel rooncerined
with meteoritic phenormna.1
COVERAGE: This ~s a colleotion.of 12,artioles on problems in meteo-
Four artiolegi describe the characteristics of fourdif-
.ferent.meteorites which fell on the USSR, and the conditions and
phenomena accompanyini; theirflight.and fall. Four articles
discuss the chemical'and physical properties of meteorites and
Card 1/4
TNI
, 0 , I
R-0

Meteoritics,; Collection (Cont.) SOV/3888
the analytical technitlues used in their study. Individual arti-
cles discuss American and international organizations for the
study oflmeteoiites. A catalog of Soviet and non-Soviet meteo-
rites kept.in the Department of Geology,,'Leningrad State Univer-,
sity is presented. References accompany individual articles.
TABLE OF CONENTS:
Astapovich,,-I.S. An Investigation of the Conditions Surrounding
the Flight of the Stone Meteorite,"Staroye Peslyanoye" 3
Aotapovich.,.I.S. Conditions Surrounding the Fall of the Stone-
.Meteoritic Rain "Pervomayakiy Poiselok" 31
.Zotkin, I.T., and Ye L.'Krinov. Investigation of-the Conditions.
Surrounding the Fall of the Stone MeteoriteRain "Xunashak"" 51
Card 2/4

Meteoritics; Collection (Pont.) SOV/3888
Zotkin, I.T., and Ye.L.,Kri4qv~ Investigating the Conditions.
Surrounding the,Fall of the St;ne Meteo.rJte "Nikollskoyell 82
IV
M
. asha,,L.G,, Petrographic Analysis of the Stone Meteorite
--uAkollskoyo" 9T
Iravnell., A.A,:-Clasa1fy1n9-Neteor1tea by,Their Components 215:
Yavnel'.. A*jk,,., and MoL,Dlyakonova. Chemical Composition of
Meteorites
1favnell, AA*j and K9I 01yxkqnqv&, - IdentifyIng Different, Types
of Irnan In Stone N~t60;1t4s--:.. 152
Idikheyev,-v,I, doeeased),,and A.I.'Winin, Applyjng the.Roont-
Senometria Method to'the Study of the Xater~aa Composition'of
Meteorites 156
'Kass
al skaya,, K.P. Internitional Organizations for the Study,of
'Meteorites 180
Massallskaya X.P. Organizations for the Study of Meteorites in
Card 3/4

2-
PASE I B" E(PLOITATION SOV/3887
scv/37-m-16
.'~ta~ya nauk SSSR. Xcuitet po meteoritm
Meteoritika; sbornik statey, VYP. 16 '(Hfte6ritics; Collection of Articles, No. 16)
Moscow, 1958- 209 p.' Errata alip inserted. Errata sUp inserted for No. 15-
i,3W, copies printed.
Edo: VoGoFeaenkorl Academician; Deputy Reap. Edo: Ye.L.Krinov; Ed. of Publish-
ing Rollse: L.K. Nikolayeva; Tech. Tech* Ed#: T.V. Polyakova.
FLWOSE: This publication is intended for astr'onaners, geophysicists, astrc-
physleibts., and other specialists concerned with meteoritic phenomena.
COVERAGE:, This collection contains 4 articles, a bibliographic index e m&'-IerifLI-cr-
meteorites., and. 23 'Abstrapts and reports, of papers presented at the Seventh Caz-
fereace on Meteorites organized by the Committee on Meteorites, Academy of
Scli~nces USSR , held in Moscov, November%14-oI6, 1956. The reportsand articles
d-,&l with the origin and conposition of meteorites and their relation to other
.elements in the solar system, the itaperties of stone meteorites, mete6riti!
C4rd 1/ 6

Meteoritics; Collection of'Articles., No. 16 SOV/3887
=&ters on the earth and the moon., and specific meteorites such as t4ose vhieh
fell in the Ukraine and in Mongolia. Seyeral reports are devoted to the
Sikhote-Alin' meteoric shower., its trajectory, checd4cal amd mineral compw:d~-
ti=O structure, and the circumstances attending its fall. A brief note de-
s--xl.bes the activities of the Center for Meteorite Study, Division of Astron-
cm;y,, Institute of Physics, Bulgarian Academy of Sciences. No personal-ttied
sre mentioned.
TABLE W2 CONTENTS:
TRANSACTIONS OF.THE SEVENTH CONFERENCE ON METEORITES
Fesenkzr, V-G. Academiciaz%Advances in Meteoritics 5
YaTn91119 A.A. Regularities in the Composition of Meteoritic Substance
ahd Conlitions For the Forzation of Meteorites (Summary of a Report) 11
Fewnenkcm, V.G. Aciademiciam Scme Problems in Meteoritics and Astronmy 13
. . . . ......
Gerziag, and L.K. Levskly. Origin of Inert Gases In Stone
-Meteorites 24
(,vaxd 2/6

iteoritics; Collection of Articles, No. 16 SW/3887
Levin, B*Yuo, and G.L, Slonimakiyo On the Problem of the Origin of Metmoritlc
Chondrules 30
Divari, N.B. Firuil Elements in the Atmospheric Trajectory of the -
Sikhote-Alin' Meteorite (Swmary of a Report) Y7
Krinw, Ye.L. Circumstances Attending the Fall of the Sikhote-Alin' Iron
Meteorite Shower (Suw~ary of &'#epo~t) 39
D"Yakonova, M.I. Chemical Composition of the Sikhote-Alin' Meteorite 41-1
Kvasha, L.G. -'Mineral Caupoeitiam~ and Structmv of the Sikhote-Alin!
Iron Meteorite (S 49
MUL17 Of a RQpWt)
Koltmenskiy, V.D.,-and I.A. Yudin. Mineral Cemp1wition of the Crust af
the Sikhote-Alint Meteorite and of Meteoritic and Meteoric Dust 59
Alekseyeva, K.N. Physical Properties of Stone Meteorites and Their In-
terpretation in the Light of Hypotheses on the Origin of Meteorites 67
Cezd 3/6

Meteoritics; Collection or Articles, No. 16 SOV/3887
YwUn. 1.A. Opaque Minera.1s in Stone Meteorites
.Dreyzin, R.L. Results of a Study of the Circumstances During the Fs-7.2.
of the Krjmkb, Stone Metdorite Shower
Aaoe, A. Recent Data on Meteoritic Craters on the Island of Saaremaa in
the Estonskaya SSR ~jj
Bonev., N. [Corresponding Wmberiof the Bulgarian Academy of Sciences].
The Meteoritic Hypothesis of the Origin of Lunar Craters 1.15
Zotkin., I.T. The Popularization of Meteoritics (Abridged Report)
Fokehivnitskiy, G.S., The Morasko Meteorite 323
Starik, I.Ye., K.A. Petrxhak, N.M. Shats, I.N. Sewenyushkin. and M.A.
Bak. Oce-ur7exlcd or Uranium In Meteorites and Its Isotopic bmTwition 126
Rotko -9 M.A. The Study of Minerals in Meteorites by the Metho-i of
Luminescence Analysis 131
Card 4/6

iteoritics; Collection of Articles, No, 16 SCq/W7
Vordblyev, G.G., and 0., Namnandorzh. Mongolian Meteorites 134
Bushitskiy, P.Is Results of a Study of a Bolide Observed in the Ukraine
on June 30, 1954 137
Yudin, I.A. Bolides in the Urals 140
Bonev, N.[Correepcoding Member of the Bulgarian Acadwy of Sciences]. k
New Center for the Study or Meteorites in I Bulgaria
ARMCLES
C-
Fesenkov, VwF* Acadam! clan. Considerations on the Energy of Formation of
Cra;t5rs-a"n-cT-on the Velocity of the Sikhote-Alin' Meteorite 147
Kvashal, L.G. Thermal Metamorphosis of Scue Types of Stone Mateorites 156
Yavnell., A.A.) and B.Se Pontow Mechanical Strength of the Sikhote-A21n'
Meteorite 175
Card 5/6

Meteoritics; Collection of Articles, No. 16 sov/3887
Dlyakonova, M.I. Nic1ml Content in Smyles of Iran Meteorites in the
Collection of the AcadmW of Sciences USSR 179
BIBLIOGRAPffr
Massallskaya~ K.P. Bibliographic Index of Material on Meteoritics 151
AVAILABLE: Ldbriu7 of Congress
JA/edV,Ipp
Card 616 7-25-6o

SOV/169-59-5-5380
Translation from -Referativnyy zhurnal-,,Geofizika, 1959, Nr 5, pp 142 143
(USSR)
AUTHOR: Fesenkov, V.G.
TITLE: Expedition-of AS USSR Into the Egyptian Region of OAR for
observing the Zodiacal Lijklit
-;FERIODICAL: Mezhdunar. geofiz. god. Inform. byul., 1958, Nr 5, PP 82 85
ABSTRACT: Prdliminary results of an expedition of,AS USSR into the
Egyptian region of OAR_for observing the Zodiacal light according
to the,IGY program are described. The expedition was working in
October - November 1957 near Assuan. In addition to 5 Soviet
scientists, 2s cientists of OAR participated in the expedition
work. Photoelectric and visual observations of the Zodiacal
light and of the daytime s1q were carried out. The observa-
tions of the Zodiacal light made it possible to obtain iso-
phots of. the evening and morning cones of the Zodiacal light,
to measure the degree of polarization of the Zodiacal light for
Card 1/2 various elongations of the Sun, to determine the possible

SOV/169-59-5-5380
Expedition of-AS USSR.Into-the.Egyptian Region of OAR:for Observing the
Zodiacal Light
Intensification of emission lines of the night sky with the Zodiacal light.
Thb daytime observations served to study the optical characteristics of the
atmosphere, to determine the coefficient of transparency, the degree of
Yolarization and the indicatrix of.dispersion of the day sky. A preliminary
processing of the obtained material enables one to draw the conclusion that
'the Zodiacal light is almost entirely due to the scattering of solar radiation
by dust particles In the interplanetary space. Electrons are not likely to
have any essential. effect In the origination of the Zodiacal light. The day-
time observations have shown that the optical characteristics of the atmosphere
tire very steady in Egypt.
N.B. Divari
Card a/2

sov/30-58-6-16/45
AUTHOR: Fesenkov, V. G., Memberg Academy of Sciences, USSR
TITLE: Investigati:ons on the Zodiacal Light (Iseledovaniya zodiakalt-
nogo sveta) Provisional Results Obtained by the Observations
of the Soviet Expedition in Egypt (Predvaritelonyye rezultaty
nablyudeniy sovetskoy ekspeditaii v Yegipte)
PERIODICAL: Vestnik Akaaemii nauk SSSR, 1958, Nr 6, pp. 89 - 91 (USSR)
ABSTRACT: In September-1957, an expedition of the AS USSR was sent to
Egypt in order to carry out investigations of the nature of
the zodiacal light, as well as on the properties of the
terrestrial atmosphere according to the work program of the
International Geophysioal Year. The appearance of the zo-
diaoal light depends on the inclination of the ecliptic with
respect to the horizon. Egypto where in autilmn, before sun-
rise, the zodiacal light can be seen almost vertically to
the horizon under the Tropic of Cancer, - whereas completely
different outlines can be seen in the shape of a largely in-
q~ined branch in the eVening of the same days, in the West -is
Card 1/3 especially fit for these observations. The Soviet-Expedition

-----------I
sov/3o-58-6-16/45
Investigations on the Zodiacal Light. Provisional Results Obtained by the
Observations of the Soviet Expedition in Egypt
has built az id tested special equipment for this purpose.
The expedition oonsisted of 5 Soviet experts and 2 Egyptian
specialists: the astrophysicist of the observatory, Kheluan
Adli Asaadq as well as the physicist Emar Sayed from the
Gelliopolis University (Cairo). The equipment of the expe-
.dition was built up in the Libyan Desert, approximately 25 km
south of Assuan, Altogether 30 000 measurements were carried
out from October 16 to November 24- It was found that the
matutinal branch of the zodiacal light corresponds compara-
tively exactly to its real appearancep whereas its evening
branch is considerably distorted by the influence of the zo-
diacal twilight. Based -upon the results obtained by the ex.-
pedition, it may be asserted that the zodiacal light is al-
,most exclusively produced by dust particles which penetrate
continuously into the interplanetary space as a result of the
disintegration of asteroids. Hitherto it has been assumed
that a highly polarized dull light cannot be produced by
cosmic dust, whereas the observations made by Ye. V.
Pyaskovskaya-Fesenkova in the Libyan Desert have shown that
Card 2/3 in case of a solar angle of 90 09 the degree of polarization