Short Jarnefelt occultation timed in Topeka March 27

Updated: 2001 March 28
The below is another confirmation of Federspiel's and Preston's 
predictions, better than expected, within a path-width.  
This was a grazing occultation, and apparently at least two
occultations of the star by features on the asteroid occurred.
There have been several similar reports for other asteroidal
occultations.
 - David Dunham, IOTA
__________________________________________________________________ 

Subject:	1558 Jarnefelt Mar. 27th occ'n final report
Date: Sat, 31 Mar 2001 21:38:52 -0600
To: Dunham@erols.com
From: Wilds 

Hi Dave:  Just a second copy to make sure you got it.  Please notice that
we have some interesting event action just before the main event, but the
seeing made certainty very difficult.  However, the number of quick events
just before the main event does make one suppect that they may be real.
Therefore, we put them in with comments to cover our concerns.  Your
comments that they may be the result of a graze experience along the
northern edge of the asteroid were taken as the most probable arguement.
Thank You!

                 IOTA ASTEROIDAL OCCULTATION REPORT FORM

Asteroid (or other object):_1558 Jarnefelt__  Star:PPM 160656=HIP 70660_____

Date (U.T.):_27 March 2001____________  Predicted Time (U.T.):_05:58:04UT___
Richard P. Wilds, Heartland Astronomical Research Team
Observer Name:__Craig McManus, Rex Easton__  Telephone:_(785)478-1868_______

Postal Address:_7328 SW 23rd Terrace, Topeka, Kansas 66614-6060 USA__________

E-mail Address:_Wilds@networksplus.net__________  Fax:______________________

TELESCOPE:  Aperture:_18 CM_  Focal length:162CM_  Type:_Refractor__________
Used Image intensified CCD Video yielding 13th magnitude in a 1 degree field.
    Eyepiece Power:________  Observing site name: Topeka, Kansas____________

    Longitude:_95d 47m 37.3s_(W)______  Latitude:_39d 01m 25.4s_(N)_________

    Height above sealevel:_315(M)_ How determined?:_GPS_____________________

Sky Transparency (Circle one, or delete two):            Good       

Star Image Stability ("seeing"; as above):        Fair              

Other Conditions:  (Wind, Clouds, Lights, etc.):_______City Lights__________

EVENT TIMINGS:  (All times in Universal Time)

Time Source:GPS Time Insertion WWV 5.0  Recording method:_VHS VCR___________

Was the Asteroid Visible in your Scope? __No__  Approx. Limiting Mag.:_13___

                               Universal Time  Estimated  Accuracy, Remarks
                                 h   m    s    Reaction
                                                Time,
  Started Observing:           _05:_50:_00.00_  (sec.)  ____________________

  Star and Object Merged:      ___:___:___.___          ____________________

Observed BLINK at (D at 58:01.12 and R at 58:01.15) Quick & Uncertain.
Observed BLINK at (D at 58:01.78 and R at 58:01.82) Quick & Uncertain.
Observed Fade Out at 58:02.18 and Fade In at 58:02.20 Fair seeing made the
	certainty of the observation unsure.

  Disappearance:               _05:_58:_02.23_  __.___  ____________________

  Estimated Closest Approach:  _____________________________________________
                  (if no D/R)
  Reappearance:                _05:_58:_04.55_  __.___  Began Fade 58:04.48_

  Star and Object Separated:   ___:___:___.___          ____________________

  Stopped Observing:           _06:_05:_00.00_          ____________________

  Was your reaction time applied to the above timings? _No______

If you could tell, did the object pass NORTH, SOUTH, EAST, or WEST of the
star (cicle one, or delete three)?  If possible,
estimate the distance of closest approach in arc seconds: _______

Additional comments: _Both "D" and "R" were observed as fade events lasting
     ~0.05 seconds.  The time inserter is accurate to 0.03 seconds. Fair
     seeing made timing and certainty of the quick events a difficult task.

Send         Jan Manek                Fax:     +420-2-61216822              
report to:   Stefanik Observatory     E-mail:  jmanek@mbox.vol.cz           
             Petrin 205               If an occultation is timed, copy to:  
             118 46  Praha 1                   dunham@erols.com           
             Czech Republic      


------
"...indeed the business of the universe is to make such a fool of you that
you will know yourself for one, and so begin to be wise!"  Quote of Mr.
Raven(The Librarian, The Sexton or Adam) from Lilith, by George MacDonald.

Richard and Tatyana Wilds
7328 SW 23rd Terrace
Topeka, Kansas 66614-6060 USA
(785)478-1868 Home
(785)575-6910 Work

E-mail: Wilds@networksplus.net		Home
	rwilds@topeka.k12.ks.us		Work

Observatory Director,
	Kansas Flint Hills Observatory Complex
	A Tech
	629 SE Quincy, Suite 204
	Topeka, Kansas 66603-3927 USA

Research Coordinator,
	Heartland Astronomical Research Team--HART
	P.O. Box 3938
	Topeka, Kansas 66604-6938 USA
	WWW: http://www.skygazer.org/hart/

Writer for Grazing Occultation Services,
	International Occultation Timing Association--IOTA
	2760 SW Jewell Ave
	Topeka, Kansas 66611-1614 USA
	E-Mail: IOTA@inlandnet.net
	WWW: http://www.occultations.org
	     
American Astronomical Society
		WWW: http://www.aas.org/
	Planetary Sciences Division
		WWW: http://www.aas.org/~dps/dps.html
	Historical Astronomy Division
		WWW: http://www.aas.org/divisions/had.html