2026-11-05 / UCAC4 556-011026 / (1315) Bronislawa
| # | OBS | Observer | Occ | Meth. | Instr. | CC | TSRC | UT1 | UT2 | UT3 | UT4 | UT2E | UT3E | Dur. | Chrd |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| 1 | show | Jiri Polak | O+ | VID | M300 | CZ | NTP | 04:53:08 | 04:55:02.18 | 04:55:07.93 | 04:57:08 | 0.020 | 0.030 | 5.75 | 63.8 |
| 2 | show | Michal Rottenborn | O+ | VID | M254 | CZ | GPS | 04:54:08 | 04:55:02.140 | 04:55:08.020 | 04:56:08 | 0.040 | 0.040 | 5.88 | 65.3 |
| 3 | show | Emmanuel Foguenne | O+ | VID | M235 | BE | GPS | 04:53:01 | 04:55:42.35 | 04:55:49.14 | 04:59:01 | 0.063 | 0.063 | 6.79 | 75.4 |
3 observations found in db: sodis
Available (probably) matching predictions (click on the link to switch):| JPL95 : 4c85ef70-d9b5-11f1-43f3-ccc15b320bd7 [db: observed] |
Using prediction 4c85ef70-d9b5-11f1-43f3-ccc15b320bd7 for map and profile fit
| Ellipse and circular profile fits to the timings (chords) |
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Auto-Fit Result: Size = 89 x 20 km a',b' = 44.6, 10.0 km X0,Y0 = 798.6, 3.9 km Mean diameter = 42 km From 3 chords (VID) You can enter space separated chord numbers (example: 11 4 8) or a method like VIS to ignore all visual timings, or a time source like RAD and NTP (but not GPS). If the plot disappears, then there are less than 2 chords left (too much ignored, go back with browser). Check SiMDA for size and mass data. Check Johnston Archive for satellites. |
| Map with groundtrack and observer stations |
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| Event Details |
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Occultation UUID [and DB] : 4c85ef70-d9b5-11f1-43f3-ccc15b320bd7 [observed] Occultation Date + Time : 2026-11-05 at 05:02:00 UT +/- 0.01 min [1] Object Designation : (1315) Bronislawa Orbit Class : MBA Star Designation : GDR3 3411863166006762112 Star Coordinates (ICRF) : RA = 04 48 06.0295, DE = +21 00 44.171 [2] Star Magnitudes : G = 12.89 mag, RP = 12.01 mag, BP = 13.69 mag Object Magnitude : V = 15.49 mag Estimated Magnitude Drop : 2.7 mag Estimated Max. Duration : 5.7 sec Object Mean Diameter : 63.5 km (src: astorb) Speed of the shadow : 11.1 km/s Elongation to Moon & Sun : 101° (sunlit = 17%), Sun = 150° Cross-track uncertainty : 0.3 mas = 0 km = 0.01 path-width (1-sig) RUWE and duplicate source : 0.96 mas, dup.src = 0 (0:false, 1:true) Ephemeris Reference : JPL95 Note : FP:true [1] time t0 of closest geocentric approach c/a, [2] including proper motion until t0 |
| More Data and Informations |
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