ASTEROIDAL OCCULTATION - REPORT FORM +------------------------------+ +------------------------------+ | EAON | | IOTA/ES | | | | INTERNATIONAL OCCULTATION | | EUROPEAN ASTEROIDAL | | TIMING ASSOCIATION | | OCCULTATION NETWORK | | EUROPEAN SECTION | +------------------------------+ +------------------------------+ 1 DATE: 14 September 2021 STAR: UCAC4 471_110652 (12.8 mag) ASTEROID: Pretoria No: 790 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: Koło Station: Brdów Latitude: 52d 20' 41.0" N Longitude: 18d 43' 57.9" E Altitude: 105 m 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 - 22:44:43 - N/A - 1 : D - - : R - - : E - 22:46:40 - N/A - 1 : Duration : no occultation Mid-event : Predicted mid-event : 14 Sep ; 22:45:23 UT +/- 12 sec Was your reaction time applied to the above timings? N/A 5 TELESCOPE: Type: Cassegrain Aperture: 203 mm Magnification: --- Mount: Equatorial Motor drive: YES Foc.length: 2032 mm reduced to 1016 mm 6 TIMING & RECORDING: Time source: Laptop time controlled by the GPS TimeBox device (steady time delay 0.190 s, considered in Tangra). Sensor: ZWO ASI 120MM, shutter set for 500 ms, image resolution 1024x768 px, gain 70. Recording: SHARPCAP v.3.2.6383.0 software 7 OBSERVING CONDITIONS: Atmospheric transparency: good Wind: none Temperature: +12 deg C Star image stability: average Minor planet visible: yes (as approaching to the star gradually) 8 ADDITIONAL COMMENTS: A remote mobile station. The light curve analysis using Tangra and AOTA software and a careful inspection of the screen replay showed no remarkable rapid drop of the star brightness caused by the asteroid to the expected level of brightness (i.e. to about a half of the summed combined brightness of the star and asteroid - Pretoria's magnitude was 13.1). The star image was not very stable both for the occulted and a guiding star; however, there was no occultation longer than 0.5s and the observation has been classified as negative. The lightdrop around 22:45:30 coincides with the prediction plus a 3-6s delay obtained by other positive observations but it could not be confirmed by the AOTA analysis as a real occultation. Predicted max 32.0 sec duration at the central line with 0.9 mag drop. Event probability at site : 70 % Distance from center line : 61 km in 140° direction, inside the predicted path, not far from the eastern limit Local * conditions (Alt,Az): 24°, @242° in Aquila Moon below the horizon.