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An 8.4 second occultation was recorded by John Broughton, using video OSD technique.
View the updated prediction.
Observers:
1(M) J Broughton,Reedy Creek, QLD,AU
2 J Broughton,Brunswick Heads, QLD,AU
3(P) Prediction 5 April
Discussion:
The circle above is plotted at the expected 69 km diameter of Happelia.
With only one chord it is not possible to determine whether John's mobile station
was north or south of the central line of the event.
However, assuming the updated prediction was approximately correct the longer than
expected chord of about 78 km would suggest that the chord might lie close to
the central portion of the asteroid.
An observation with 5 chords on 2005 May 23 in USA indicated an elongated object
82 km by 57 km which is consistent with this observation.
Observational Data:
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Observation details for MP (578 ) Happelia
By Star UCA 2U20751392
On 2009-05-15 at 17:03:16.0
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Observer J Broughton
Location Reedy Creek, QLD 4227, Australia
Longitude +153:23:52.9
Latitude -28:06:30.4
Altitude 66 m
Datum WGS84
Telescope Newtonian
Aperture 51 cm
Seeing Slight flickering Clear
Timing Image analysis + time signal Drift scan
Missed
Comments: : Unattended drift-scan observation.
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Observer J Broughton
Location Brunswick Heads, QLD , Australia
Longitude +153:32:55.4
Latitude -28:33:4.8
Altitude 5 m
Datum WGS84
Telescope SCT
Aperture 25 cm
Seeing Slight flickering Clear
Timing GPS - time inserted Video with frame analysis
Disappearance 17:03:05.80
Reappearance 17:03:14.20
Comments: : Mobile observation using a Watec 120N+ at 16X integration (0.64sec).
: I overdid the integration as a result of forgeting to attach a focal reducer.
: Without it, the image scale was different from that of my ScanTracker printout
: and I couldn't recognize the star patterns until after the drift through.
: The integration was supposed to be reduced once the target was identified.
: Not until later in the day when I replayed the video was I able to ascertain
: that the target did actually drift through the field and was occulted.
: The times are estimates of where within the 16X integrations D and R occurred.