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Дата изменения: Mon Jun 28 22:37:32 2004
Дата индексирования: Mon Oct 1 23:14:52 2012
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Apparent Encounters of the Outermost Satellites of Jupiter
Varfolomeev M. I., Emelianov N. V.
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Description:
The higher accuracy of observations is reached at the periods
of apparent encounters of satellites when two satellites fall within
the same CCD frame. This paper presents the precalculated
circumstances of the apparent encounters of the outermost satellites
of Jupiter for the years 2005 through 2010.
Ephemerides were divided into six parts, according to periods of Jupiter's
observability and placed into tables 3 to 8 where apparent angular
distances between two satellites for the beginning of each date are given.
Each line contains ephemerides for a single moment of time. Each column
(beginning from the 7th) corresponds to a pair of satellites.
One column may contain data for different pairs of satellites if their
close encounters do no coincide in time. Numbers of satellites,
to which apparent angular distances relate, are given in the first line
of the column segment. The mutual angular distances between pairs
of satellites are given in arcminutes.

File Summary:
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FileName Lrecl Records Explanations
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ReadMeT.txt 80 . This file
table3.dat 128 319 Ephemerides of the apparent encounters for 2005
table4.dat 92 320 Ephemerides of the apparent encounters for 2006
table5.dat 92 322 Ephemerides of the apparent encounters for 2007
table6.dat 98 323 Ephemerides of the apparent encounters for 2008
table7.dat 86 329 Ephemerides of the apparent encounters for 2009
table8.dat 98 266 Ephemerides of the apparent encounters for 2010
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Byte-by-byte Description of files: table3.dat to table8.dat
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Bytes Format Units Label Explanations
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1- 4 I4 --- YYYY Year of the date
6- 7 I2 --- MM Month of the date
9- 10 I2 d DD Day of the date
12- 15 I4 d JD* Julian day of the date DJ*=JD-2450000.5
17- 20 F4.2 --- Moon Phase of the Moon, 1.00 is a Full Moon
22- 26 F4.1 degrees MD Apparent distance between Moon and Jupiter
28- 32 A5 arcmin D See Note (1)
34- 38 A5 arcmin D See Note (1)
40- 44 A5 arcmin D See Note (1)
46- 50 A5 arcmin D See Note (1)
52- 56 A5 arcmin D See Note (1)
58- 62 A5 arcmin D See Note (1)
64- 68 A5 arcmin D See Note (1)
70- 74 A5 arcmin D See Note (1)
76- 80 A5 arcmin D See Note (1)
82- 86 A5 arcmin D See Note (1)
88- 92 A5 arcmin D See Note (1)
94- 98 A5 arcmin D See Note (1)
100-104 A5 arcmin D See Note (1)
106-110 A5 arcmin D See Note (1)
112-116 A5 arcmin D See Note (1)
118-122 A5 arcmin D See Note (1)
124-128 A5 arcmin D See Note (1)
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Note (1):
*: No data
N1-N2: N1 - number of first satellite, N2 - number of second satellite of event
DD.DD: The value of the apparent distance between the satellites in arcmin
at 0 h (TT) of the date
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Acknowledgements: This work was supported by the Russian Foundation for Basic
Research, project no. 03-02-17441.

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(End) 01-Jan-2004