2003 Jan. Bathilde Occ'n - 2 remote videos & Maryland expedition results
New: 2003 Feb. 21The January 11th occultation of SAO 117679 by (441) Bathilde was the first one where unattended telescopes at two sites successfully recorded the target star during the appulse. You know about Roger Venable's successful remote recording of the occultation, while several miles away he also timed the occultation visually with a pair of binoculars, the first remote video/attended visual observation of an asteroidal occultation (in contrast, for the two other remote successes, mine with 9 Metis in Sept. 2001 and Steve Preston's with the occultation of 26 Gem by 701 Oriola in April 2002, video recordings were made at all stations). On January 11th, I also ran a remote video station, and it recorded the target star during the minute surrounding the closest approach, but that station was outside the occultation path and had no occultation. I obtained permission from a homeowner on the north side of Glennville, Georgia, to set up a C-8 in his yard, about 100 feet east of the north-south highway US301 and overlooking a large dark field. Alin Tolea and I set up the telescope with f/3.3 focal reducing lens and Watec 902H camera about 2 hours before the appulse, and at just the right time, we aimed the telescope at a distinctive group of stars near Procyon, aimed at the same declination as the target star but two hours of R.A. less. That is, it was pointed at the altitude and azimuth that the target star would have at the time of the appulse so that we would not have to worry about the accuracy of a clock drive; the telescope's clamps were locked and it was not driven. Then several miles south of Glennville, we couldn't find any houses with awake occupants near US301, but we found a small deserted building and set up a C-5 at the edge of woods near it, and focused the video and aligned the finder scope, using another f/3.3 reducer and PC-164C camera. Then we drove several miles north of Glennville, where Alin and Magda Tolea stayed, setting up their 4-inch refractor with another PC-164C and a reducing lens. On the way back to the C-5, I stopped at the C-8, and 30 minutes before the occultation I started the video recording, then went to the C-5, got the video running there, and located the target star a few minutes before the occultation. In summary, our expedition from Maryland obtained the following negative observations at 3 sites near US301 in Georgia: Distance (determined with W. Warren's Magellan GPS) from W. center, Longitude Latitude Height Location Observer km deg. ' deg. , feet 25N 81 54.562 +32 03.576 150 near Midway Alin Tolea 14N 81 55.396 +31 57.070 156 n. Glennville none (remote) 3N 81 55.840 +31 51.250 39 s. of Glennville David Dunham The target star crossed the video field at the remote site from 3h 54m 10s to 3h 55m 57s UTC. The closest approach time there was 3h 55.5m, but the target star arrived in the field a little earlier (that is, the observation interval was not symmetric about the closest approach time) because we did not take into account the difference between solar and sidereal rates. David Dunham