ASTEROIDAL OCCULTATION - REPORT FORM +------------------------------+ +------------------------------+ | EAON | | IOTA/ES | | | | INTERNATIONAL OCCULTATION | | EUROPEAN ASTEROIDAL | | TIMING ASSOCIATION | | OCCULTATION NETWORK | | EUROPEAN SECTION | +------------------------------+ +------------------------------+ 1 DATE: 20 September 2021 STAR: TYC 3565-01175-1 (10.5 mag) ASTEROID: 2008 YB3 No: 342842 2 OBSERVER: Name: Marek Zawilski Abbr: E-mail: marek.zawilski@p.lodz.pl Address: ul.Julianowska 5/7 m.322, 91-473 Lodz, Poland 3 OBSERVING STATION: Nearest cities: Lodz and Poddebice Station: Tobolice Latitude: 51d 54' 48.3" N Longitude: 19d 03' 22.4" E Altitude: 140m MSL Datum (WGS84 preferred): WGS84 Single, OR Double or Multiple station (Specify observer's name): SINGLE +----------------------------------+ 4 TIMING OF EVENTS: | | | OCCULTATION RECORDED: NEGATIVE | | | +----------------------------------+ 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 - 22:18:24 - N/A - 1 : I - 22:18:50 - N/A - 1 : J - 22:19:03 - N/A - 1 : I - 22:19:21 - N/A - 1 : J - 22:19:26 - N/A - 1 : D - - : R - - : E - 22:29:40 - N/A - 1 : Duration : no occultation Mid-event : (20 Sep; 22:29:05) i.e. 10s earlier than predicted according to the positive observation by M.Harman Predicted mid-event : 20 Sep.; 22:29:15 UT +/- 27 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 TimeBox device (time error 0.000 s). Sensor: ZWO ASI 120MM, shutter set for 500 ms, image resolution 1024x768 px, gain 60. Recording: SHARPCAP v.3.2.6383.0 software 7 OBSERVING CONDITIONS: Atmospheric transparency: good but with passing thin clouds Wind: none Temperature: +5 deg C Star image stability: good within periods without clouds Minor planet visible: no 8 ADDITIONAL COMMENTS: The light curve analyze using Tangra software and a careful inspection of the screen replay showed no longer remarkable rapid drop of the star brightness caused by the asteroid. The star image was not stable enough for the occulted star because of passing thin clouds; however, because the star was detectable on the recording in the periods stated above, there was no occultation longer than 0.5s and the observation has been classified as negative. Predicted max 1.9 sec duration with 10.6 mag drop. Event probability at site : 6.0 % Distance from center line : 210.5 km in 344° direction, outside the predicted path, inside the 1-sigma limit Local * conditions (Alt,Az): 54°, @290° in Cygnus Moon (Alt,Az): 33°, @174°, near full moon but did not disturbe the star view.