Occultation by (152) Atala May 6 Well-Observed

Nine positive chords were fairly well-distributed across the asteroid with negative observations also near both limits

Updated: 2006 May 31

From: David Dunham [dunham@starpower.net]
Sent: Wednesday, May 31, 2006 1:03 AM
To: Dunham, David
Subject: Now 8 Atala chords timed, & close misses north and south

Need to add to this Gary Frishkorn's video obs., & Tolea's miss

      Observations of the occultation of TYC 5558-01048-1 by 152 
Atala show that the path shifted only about 0.3 sigma north, 
according to the second summary below, now with 8 positive chords 
reasonably well-spaced across Atala, and two close miss observations 
near both of the actual limits. 

Steve Preston's 05/05/06 update [the LATEST update] Occultation of 
TYC 5558-01048-1 by 152 Atala on 2006 May 07 (06 EDT) Distance from 
the center of occultation path - in km 
         %
      Proba-  Location
   km bility
  115   16 ** Northern limit plus 1-sigma, occultation quite possible **
   80 F 32 Essex    MD Dale Lehman - No occultation (miss)
   79   32 Baltimore MD Alin Tolea - No occultation (miss)
   59   42 Dayton MD Gary Frishkorn - video, 2.8s occultation
   61 ? 43 Morgntwn WV TomchinObsLittleton - about 3s occ'n, visual
   60 F 44 Columbia, MD     Don Gardner - video, 3.4s occultation
   55   46 ***  Predicted Northern limit  ***
   51 ? 48 GRINNELL IA GRINNELL COLLEGE - photoelectric, 3.6s occ'n
   43 F 52 GORF16IN  Wayne H. Warren Jr. - visual, 3.7s occultation
   38 F 54 GREENBELT MD Joan Dunham - video, 4.1s occultation
    0   63 **** Predicted Centre Line    ****
    0 F 63 Jose Ripero near Madrid, Spain visual, 3s occultation
  -12 M 62 n.w. La Plata, MD Dunham remote - video, 3.0s occultation
  -21 M 61 Chapel Pt. St. Park, MD Joe Sedlak - visual, 2.7s occ'n
  -35 M 56 Dahlgren, VA D. Dunham mobile - video, prob. no occultation
  -55   46 ***  Predicted Southern limit  ***

After reviewing my video tape at Dahlgren, VA closely, the target 
star was recorded.  Just before the occultation, I realized that the 
drive was not working, and at the time of the occultation, as 
reported by Joe Sedlak nearby, I was carefully adjusting the 
telescope (at about the time of possible disappearance, the target 
star was close to the right edge of the field and would have exited 
a second or two later if I had not adjusted), but slowly enough that 
the target star remained visible during the adjustment.  However, it 
was only marginally visible then with my 5" SCT (it was more clearly 
visible in the 8" SCT recordings at Greenbelt and at La Plata), and 
I could have missed detecting a short occultation, of a quarter of a 
second duration or less.  Perhaps with some more sophisticated 
analysis of the tape, a short event might be revealed, or more 
likely found not to exist. 

We have collected I believe all the available timings and 
coordinates, and have made a first analysis of Atala's outline. That 
will be documented here when time permits. It looks like Atala was a 
little smaller than predicted, especially in the direction of 
motion.  Thanks for all who tried to observe this occultation.  

Extensive predictions and plans to observe the occultation are here.
__________________________________________________ 

David Dunham, IOTA   2006 May 31
phones home 301-474-4722; office 240-228-5609; cell  301-526-5590
Home (IOTA) e-mail dunham@starpower.net