A 10.35 second occultation was recorded by Peter Graham, using Video OSD technique.
one clearly observed constraining miss was recorded for this event.
View the TT14 prediction.
Observers: 1(M) A Pennell,Dunedin New Zealand 2 P PB Graham,Martinborough, NZ 3(P) Prediction TT14, May 28
The circle above is plotted at the expected 184 km diameter of Lomia. With one chord and a nearby constraining miss we can be confident of the path of Lomia and that it was south of the predicted line.
The figure below shows the Limovie light curve of the occultation.
Observation details for MP ( 117 ) lomia By Star UCAC4 239-166182 On 2015-06-05 at 18:11:40.0 _______________________________ Observer Ash Pennell Location Dunedin New Zealand Longitude +170:29 Latitude -45:52 Altitude 136 m Datum WGS84 Telescope SCT including Cass and Mak Aperture 35 cm Seeing Slight flickering Clear Camera Type Watec 120N+ PAL/CCIR Camera Delay Timing GPS - time inserted Video with frame analysis Missed Comments: _______________________________ Observer PB Graham Location Martinborough, NZ Longitude +175:29 Latitude -41:14 Altitude 73 m Datum WGS84 Telescope SCT including Cass and Mak Aperture 25 cm Seeing Steady Clear hum bar on video from power supply Camera Type Watec 910BD PAL/CCIR Camera Delay Timing GPS - time inserted Video with frame analysis Disappearance 18:10:43.55 Reappearance 18:10:53.90 Comments: camera delay 1 frame time difference from video stamp to start of exposure -0.040s.