From spencer Thu Nov 2 10:24:26 1995 From spencer Thu Nov 2 10:24:26 1995 To: oleroemer Subject: Jupiter viewing times X-Sun-Charset: US-ASCII Content-Length: 4483 X-Lines: 102 Status: RO I just got this from John Rogers, leader of the Jupiter section of the British Astronomical Association. It's not directly relevant to the Satellites Discipline, but there might be someone on the list who can help with these important observations, so here's the information... Our last hope for Io remote sensing during the December Io flyby, a high-res equatorial scan with the radiometer, will not be done after all. However, as far as I know, the particles and fields measurements are still likely to take place, and will return very valuable data. John. _____________________________________________ NOTE FOR IJW, sent Oct.31: LONGITUDE OF PROBE ENTRY SITE So far I have only seen the Probe entry longitude given in System III. However, in this latitude region on the NEBs edge, everything moves with System I - all large and small features, from the visible cloudtops down to the 5-micron regions. System I (\1) diverges from System III (\3) by 7.4 degrees/day. Therefore it is essential to track the Probe entry site in System I. Below will be an adaptation of Glenn's table of viewing times, for \1 = 7.4. This is the point of entry, around 50 nanobars, based on the value of \3 = 5.0 given by the Galileo team (by coincidence, \1 = \3 a few hours before entry). However after 2 min deceleration, descent through the cloud layers will be at \1 ~ 4.0 (+/- 1 degree). This longitude is deduced from the Galileo project statement that the Probe will be fully entrained by local winds after E + 2 min, and will cross the terminator at E + 42 min. (The stated times appear to be UT at the spacecraft, rather than Earth-received time). If anyone sees any errors in these figures, please let me know. Thus: ----------------------------------------------------- Entry E+2m E+42m (0.1 bar) (12 bar) ------- ------- ------- Time UT at spacecraft 22:04 22:06 22:46 Time UT at Earth 22:56 22:58 23:38 Longitude Sys.I 7.4 4.0 4.0 Longitude Sys.III 5.0 1.6 1.4 Latitude 'centric +6.6 ? ? Latitude 'graphic +7.5 ? ? ----------------------------------------------------- In July-August, \1 = 4 happened to be the location of a large, persistent 'NEBs dark projection' (visible), presumably a 'hotspot' (5 microns). This was one of only two such features on an otherwise messy NEBs; we will try to establish whether it is still there. However, even if such a feature appears stable, it can change suddenly within 1-2 days, and the probe might fly through a billowing white updraft and/or an adjacent dark 'hotspot'. Therefore, extrapolated data will be no substitute for observations on the exact day of the Galileo entry. -- John Rogers British Astronomical Association. ------------------------------------------------------------ UT date Jupiter-Sun PES (\1=7.4) CM Angle (deg.) Crossing Time (UT) ------------------------------------------------------------ Dec. 1.0 14.1 7:42 17:33 Dec. 2.0 13.3 3:24 13:15 23:05 Dec. 3.0 12.6 8:56 18:47 Dec. 4.0 11.7 4:37 14:28 Dec. 5.0 11.0 0:18 10:09 20:00 Dec. 6.0 10.2 5:50 15:41 Dec. 7.0 9.4 1:32 11:23 21:13 Dec. 8.0 8.6 7:04 16:54 Dec. 9.0 7.8 2:45 12:36 22:27 Dec. 10.0 7.0 8:17 ------------------------------------------------------------ ##########################################################################