ASTEROIDAL OCCULTATION - REPORT FORM +------------------------------+ +------------------------------+ | EAON | | IOTA/ES | | | | INTERNATIONAL OCCULTATION | | EUROPEAN ASTEROIDAL | | TIMING ASSOCIATION | | OCCULTATION NETWORK | | EUROPEAN SECTION | +------------------------------+ +------------------------------+ 1 DATE: 24 March 2022 STAR: UCAC 484-048632 (13.9 mag) ASTEROID: Suevia No: 417 2 OBSERVER: Name: Marek Zawilski Abbr: Assistance: Mieczyslaw Borkowski and Janusz Bankowski 3 OBSERVING STATION: Nearest cities: Belchatow Station: Kluki Latitude: 51d 20' 23.1" N Longitude: 19d 14' 53.7" E Altitude: 175 m MSL Datum (WGS84 preferred): WGS84 Single, OR Double or Multiple station (Specify observer's name): SINGLE +----------------------------------+ 4 TIMING OF EVENTS: | | | OCCULTATION RECORDED: POSITIVE | | | +----------------------------------+ Type of event Start observation Interrupt-start Disappearance Blink Flash End observation Jnterrupt-end Reappearance Other (specify) Comments Event Time (UT) P.E. Acc. Code HH:MM:SS.ss S.ss S.ss S - 20:13:00 - N/A 1.0 D - 20:13:36.05 0.10 AOTA analysis R - 20:13:38.17 0.40 AOTA analysis E - 20:15:00 - N/A 1.0 Duration : 2.12 sec Mid-event : 20:13:37.11 Predicted mid-event : 24 Mar;20:13:42 UT +/- 7 sec Was your reaction time applied to the above timings? N/A 5 TELESCOPE: Type: Cassegrain Aperture: 203mm Magnification: --- Mount: Equatorial Motor drive: YES Foc.length: 2032mm reduced to 1016mm 6 TIMING & RECORDING: Time source: Laptop time controlled by the GPS Shelyak TimeBox device (time error +0.000 s with 7 satellites). Sensor: ZWO ASI 120MM, shutter set for 200 ms, video time resolution 200 ms, image resolution 1024x768 px, gain 80, brightness 13. Recording: SHARPCAP v.4.0.8667.0 software. 7 OBSERVING CONDITIONS: Atmospheric transparency: very good Wind: none Temperature: +2 deg C Star image stability: good Minor planet visible: yes 8 ADDITIONAL COMMENTS: The light curve analyze using Tangra software and a careful inspection of the screen replay showed a small drop of the star brightness caused by the asteroid. The star image was stable enough both for the occulted and a guiding star. The D and R times according to the AOTA analysis. The observation was made inside the predicted path. The asteroid was brigther than the star. Predicted max. 9.6 sec. duration with 0.5 mag. drop. Event probability at site : 63.2% Distance from center line : 8.2 km in 52° direction, inside the predicted path. Local * conditions (Alt,Az): 45°, @176° in Leo. Moon (Alt, Az): below the horizon.