Some observations made on Sunday evening (local time) [UT date Feb 28]: I observed the Chandra spacecraft (99-040B, 25867) using a 10-inch reflector. Chandra was low in the south, rising up after perigee passage less than an hour earlier. Its brightness was consistent with the 8th magnitude predicted using the standard magnitude of 3.0 in the Mccants.tle file. It was moving relatively slowly through the star field (about 1 degree per minute) so I was able to follow it and obtain a very good positional observation: at 4:59:25.0 UTC Feb 28 2000 Chandra passed directly over the 9th mag star SAO 178543 (J2000 position from GUIDE 7 is 10h13m07s, -30d11m56s). A 10th mag star 1.4 arcmin to the NW made a wide double with the convergent Chandra and SAO 178543, so I estimate that the position given above is good to better than 0.5 arcminute. I continued to follow the spacecraft with the telescope for another 10 minutes as it slowly rose higher in the south. Finally it dimmed as it began to enter eclipse, and it disappeared in the 10 inch at 5:10:17 UTC. My method for locating Chandra was to obtain a state vector from JPL Horizons (telnet to ssd.jpl.nasa.gov, port 6775), use VEC2TLE to convert it to an SGP tle, and then use the eleset with GUIDE 7 to plot the path through the starfield. Chandra was running only about 5 seconds late relative to the JPL horizons SSD ephemeris that was loaded on Feb 1st! I have found the JPL ephemeris to be considerably more accurate than the predictions generated using NORAD elements from GSFC. I also found that if you try to propagate the NORAD elset with the "original" SDP4 model (as you can find in Spacetrack Report No. 3) you will get large errors; but the NORAD elsets for Chandra give good agreement with the JPL ephemeris if you use SGP. Prior to the Chandra observations, I took a look at TDRS 4 (89-021B, 19883) with the 10 inch. For several minutes prior to entering eclipse the TDRS was VERY bright. As it passed near 5th magnitude delta sextantis it was equal in brightness to that star. It got even brighter (about 4th mag) and I could actually see it with the naked eye. This was so unbelievable that I got out my 7x50 binoculars and watched the stars slowly drift past it to be sure I was really seeing the TDRS. I switched back to the scope and observed TDRS 4 do a very slow fade and finally disappear in the 10 inch at 2:31:13 UTC. This was quite a site! Note: Observing site was the Texas Astronomical Society site in Atoka county, Oklahoma. My postion was: long -96.1399 deg, lat 34.1844 deg, elev 0.170km. Curtis Haase Dallas, Tx 73007.2024@compuserve.com PS: the generated Chandra elset I used is: Chandra 1 25867U 99040B 00059.20759045 .00000000 00000-0 00000-0 0 09 2 25867 29.9572 173.2996 7867482 287.8116 3.5344 0.37780175 03 ----------------------------------------------------------------- Unsubscribe from SeeSat-L by sending a message with 'unsubscribe' in the SUBJECT to SeeSat-L-request@lists.satellite.eu.org http://www2.satellite.eu.org/seesat/seesatindex.html
This archive was generated by hypermail 2b29 : Mon Feb 28 2000 - 10:09:40 PST