Richard Nugent Records 3 Asteroidal Occultations in First Two Nights of 2003; Other Recent Observations

New: 2003 Jan. 6; Updated Jan. 7
      The past week has already been very active with asteroidal 
occultation observations, indicating that 2003 could surpass even 
last year's record.  The occultation by the prototypical outer belt 
asteroid (153) Hilda was timed from at least 4 stations in Japan on 
December 31, capping 2002's efforts.  But right away, the first 
asteroidal occultation of 2003, by (233) Asterope, was video taped 
at 3h UT of Jan. 1 by Paul Maley and Richard Nugent from two 
locations in Texas.  And the next night, Richard recorded two more 
asteroidal occultations, by (196) Philomela and (44) Nysa, from near 
Jai, New Mexico, the first time anyone has observed 3 asteroidal 
occultations in 2 nights, and the second time that anyone has 
observed 2 of these events in 1 night [the first time that was done 
was on Jan. 17, 1999, when T. Kojima in Japan timed occultations by 
(510) Mabella and (820) Adriana].  And Paul recorded a 2.3-second 
occultation by (726) Joella Jan. 3 UT near Preston's central line at 
Cash, Texas, north of Dallas, making 4 events already observed 
during the first 3 days of 2003!  Also observed since my last 
general message was the occultation by (334) Chicago from at least 8 
stations from Pennsylvania to Alberta on Dec. 24 (read more about
it here), and the occultation of HIP 21529 A by 
(392) Wilhelmina on Dec. 27, by Frank Anet in California 
and Roger Venable in South Carolina.  The occultation by (44) Nysa 
on Jan. 2 was also video recorded by Peter Armstrong at his 
observatory in Limpia, Texas. 

     Below is my message to Richard Nugent congratulating him
on his observation of three asteroidal occultations in one night,
and his message with the reports of the events.

Richard,
     Many thanks for your reports below of the occultations 
that you video recorded of
(233) Asterope on Jan. 1,
(196) Philomela on Jan. 2, and
(44) Nysa on Jan. 2

You wrote:

"Three (3) asteroid report form attached. That makes 7 in a row for 
me since Athor 10-15-02, which included 2 last night. I'm really 
feeling lucky now, so I'm going out to buy a lottery ticket."

As far as I know, nobody else has previously observed 3
asteroidal occultations during 2 nights, and the first
2 nights of 2003 at that!  The only other case of an
observer timing two asteroidal occultations in one night
that I know of was by T. Kojima in Japan on 1999 Jan. 17,
when he observed an occultation of 9.8-mag. SAO 117797
by (510) Mabella and of 5.7-mag. SAO 119508 by (820)
Adriana.  

David
________________________________________________________________

                 IOTA ASTEROIDAL OCCULTATION REPORT FORM

Asteroid (or other object): 233 Asterope  Star:  TYC 726-00419-1
Date (U.T.):01 Jan 2003    Predicted Time (U.T.): 3:15:08
Observer Name: Richard Nugent    1-800-753-6977 
                      Cell Phone:  713-805-7344
Postal Address:  P.O. Box 131034, Houston, Texas 77219
E-mail Address: JackiesDad@weblore.com Fax:  (713)524-1993
TELESCOPE: Aperture: 4"   Focal length: 1000mm f/10  Type:Meade 2045D 
Eyepiece Power: n/a   Observing site name: 5 miles east of 
                      Carizzo Springs, TX on Hwy 85 at Pinic area.
Longitude: West 99deg 45min 15.2sec Latitude: 28deg 32min 58.8sec N.
Determined by Garmin GPS model "Venture" unit. DATUM: WGS84             
Height above sea level: 504 m   How determined?:Garmin GPS 
model "etrex" NOTE: This GPS unit quoted accuracy to 5 meters.

Sky Transparency (Circle one, or delete two): Very Good, Stars
m = 6.5 visible. 
Star Image Stability ("seeing"; as above): good, images were steady
Other Conditions:  (Wind, Clouds, Lights, etc.): Temperature during 
occultation approx. 50 F.  No wind.

Time Source:   WWV 5,000 kHz   Recording method: Image intensified video
                               Supercircuits PC-164C and WWV direct feed
                               simultaneously into camcorder.
Was the Asteroid Visible in your Scope? It was faintly visible on video.

EVENT TIMINGS:  (All times in Universal Time)
         Universal Time  Estimated  Accuracy,  Reaction (estimated error)
                                 h   m   s         Time  
  Started Recording:             3: 14: 45             
  Star and Object Merged:        
  Disappearance:                 3: 16: 17.8     +/- 0.1 sec 
  Reappearance:                  3: 16: 26.8     +/- 0.1 sec 
  Star and Object Separated:                                            
  Stopped Recording:             3: 18: 15.0

  DURATION OF EVENT: 9.0 +/- 0.1 seconds
   ---"D" and "R" both instantaneous----

Was your reaction time applied to the above timings?   Yes, reductions 
done from video

ADDITIONAL COMMENTS: Drove to Carrizo Springs, TX and set up at 
picnic area on Hwy 85. Good seeing, steady images. Both "D" and "R" 
were instantaneous. No other events seen during recording interval. 
This event made 5 in a row. 
________________________________________________________________

                 IOTA ASTEROIDAL OCCULTATION REPORT FORM

Asteroid (or other object): 196 Philomela  Star:  TAC +05 00062
Date (U.T.):02 Jan 2003    Predicted Time (U.T.): 1:13:10
Observer Name: Richard Nugent    1-800-753-6977 
E-mail Address: JackiesDad@weblore.com Fax:  (713)524-1993

TELESCOPE: Aperture: 4"   Focal length: 1000mm f/10  Type:Meade 2045D 
Eyepiece Power: n/a   Observing site name: 5 miles west of Jai,NM
                                           on Hwy 128
Longitude: West 103deg 16min 46.4sec Latitude: 32deg 8min 14.2sec North.
Determined by Garmin GPS model "Venture" unit. DATUM: WGS84             
Height above sea level: 956 m   How determined?:Garmin GPS 
model "etrex" NOTE: This GPS unit quoted accuracy to 5 meters.

Sky Transparency (Circle one, or delete two): Very Good, Stars
m = 6.5 visible. 
Star Image Stability ("seeing"; as above): good, images were steady
Other Conditions:  (Wind, Clouds, Lights, etc.): Temperature during 
occultation approx. 45 F.  Sustained winds of 20-25 mph prevailed.

Time Source:   WWV 5,000 kHz   Recording method: Image intensified video
                               Supercircuits PC-164C and WWV direct feed
                               simultaneously into camcorder.
Was the Asteroid Visible in your Scope? It was faintly visible on video.

EVENT TIMINGS:  (All times in Universal Time)
                               Universal Time   Accuracy
                                 h   m   s       
  Started Recording:             1: 10: 45             
  Star and Object Merged:        
  Disappearance:                 1: 13: 15.7    +/- 0.1 sec 
  Reappearance:                  1: 13: 17.8    +/- 0.2 sec 
     (this time was difficult due to shakey video view)
  Star and Object Separated:                                            
  Stopped Recording:             1: 15: 10.0

  DURATION OF EVENT: 2.1 +/- 0.1 seconds
Was your reaction time applied to the above timings?   Yes, 
reductions done from video 

ADDITIONAL COMMENTS: Drove to Ft. Davis, and then drove to site. 
Some difficulty was experienced in locating the star since sunset 
was less than 60 minutes prior to event. Following this occultation, 
stayed at site to observe 44 Nysa some 3.5 hours later, which was 
successful also. 

Video field of view was a little shakey due to the wind even though 
telescope was set up shielded by car.  
________________________________________________________________

                 IOTA ASTEROIDAL OCCULTATION REPORT FORM

Asteroid (or other object): 44 Nysa  Star:  TYC 654-00755
Date (U.T.):02 Jan 2003    Predicted Time (U.T.): 4:55:00
Observer Name: Richard Nugent    1-800-753-6977 
E-mail Address: JackiesDad@weblore.com Fax:  (713)524-1993

TELESCOPE: Aperture: 4"   Focal length: 1000mm f/10  Type:Meade 2045D 
Eyepiece Power: n/a   Observing site name: 5 miles west of Jai,NM
                                           on Hwy 128
Longitude: West 103deg 16min 46.4sec Latitude: 32deg 8min 14.2sec North.
Determined by Garmin GPS model "Venture" unit. DATUM: WGS84             
Height above sea level: 956 m   How determined?: Garmin GPS 
model "etrex" NOTE: This GPS unit quoted accuracy to 5 meters.

Sky Transparency (Circle one, or delete two): Very Good, Stars
m = 6.5 visible. 
Star Image Stability ("seeing"; as above): good, images were steady
Other Conditions:  (Wind, Clouds, Lights, etc.): Temperature during 
occultation approx. 45 F.  Some wind.

Time Source:   WWV 5,000 kHz   Recording method: Image intensified video
                               Supercircuits PC-164C and WWV direct feed
                               simultaneously into camcorder.
Was the Asteroid Visible in your Scope? It was faintly visible on video.

EVENT TIMINGS:  (All times in Universal Time)
                               Universal Time    Accuracy
                                 h   m   s        
  Started Recording:             4: 51: 45             
  Star and Object Merged:        
  Disappearance:                 4: 54: 51.1     +/- 0.1 sec 
  Reappearance:                  4: 55: 06.9     +/- 0.1 sec 
  Star and Object Separated:                                            
  Stopped Recording:             4: 57: 10.0

  DURATION OF EVENT: 15.8 +/- 0.1 seconds

Was your reaction time applied to the above timings?   Yes, 
reductions done from video 

ADDITIONAL COMMENTS: 2nd occultation observed in same night. Wind 
died down considerably, making the small mag. drop of 0.9 easier to 
see. This success makes 2 in one night. 
________________________________________________________________