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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