In polar coordinates (r = solar radii; PA: north up increasing eastwardfrom north) the center of Venus, seen against the Sun from ACRIMSAT, in fiveminute increments during solar visibilities (based upon a satellite ephemerisgenerated from the the 8 June 2004 two-line element set) are as follows:

UT/HM    Sol_rad   PA(N)
05:15    1.01960    115.62
05:20    1.00690   116.63
05:25    0.99537   117.76
05:30    0.98423   118.92
05:35    0.97134   120.29
05:40    0.96110   121.50
05:45    0.94497   122.73
05:50    0.93318   123.97
05:55    0.91738   125.04
06:00    0.90050   126.21
       
06:40    0.76651   132.87
06:45    0.75741   134.06
06:50    0.74865   135.47
06:55    0.74413   137.00
07:00    0.73766   138.56
07:05    0.73445   140.33
07:10    0.73332   142.19
07:15    0.72948   144.19
07:20    0.72753   146.10
07:25    0.72333   147.94
07:30    0.71912   149.78
07:35    0.71326   151.77
07:40    0.70668   153.40
 
08:20    0.63920   166.44
08:25    0.64047   168.07
08:30    0.64366   169.88
08:35    0.64974   171.39
08:40    0.65911   173.36
08:45    0.66939   175.12
08:50    0.68368   176.99
08:55    0.69520   178.63
09:00    0.70730   180.50
09:05    0.71655   182.17
09:10    0.72490   184.09
09:15    0.73211   185.84
       
09:55    0.75884   198.52
10:00    0.76927   199.70
10:05    0.77950   200.88
10:10    0.79308   202.00
10:15    0.80949   202.87
10:20    0.82839   203.77
10:25    0.84895   204.85
10:30    0.86986   205.61
10:35    0.89012   206.49
10:40    0.90983   207.48
10:45    0.92742   208.38
10:50    0.94457   209.40
10:55    0.96138   210.52