2026-09-22 / UCAC4 464-001966 / (3885) Bogorodskij
| # | OBS | Observer | Occ | Meth. | Instr. | CC | TSRC | UT1 | UT2 | UT3 | UT4 | UT2E | UT3E | Dur. | Chrd |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| 1 | show | Michael OConnell | O+ | VID | M350 | ES | NTP | 22:06:09 | 22:07:08.6 | 22:07:09.8 | 22:08:09 | 0.200 | 0.200 | 1.20 | 12.0 |
| 2 | show | Juan Collada Barcena, Alfonso Coya | O+ | CCD | M356 | ES | GPS | 22:05:54 | 22:06:51.091 | 22:06:53.081 | 22:07:54 | 0.136 | 0.136 | 1.99 | 19.9 |
2 observations found in db: sodis
Available (probably) matching predictions (click on the link to switch):| JPL61 : 588f6f70-d9b1-11f1-43f3-8ed6f73d9457 [db: observed] |
Using prediction 588f6f70-d9b1-11f1-43f3-8ed6f73d9457 for map and profile fit
| Ellipse and circular profile fits to the timings (chords) |
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Auto-Fit Result: X0,Y0 = 3033.3, 38.4 km Circular diameter = 20 km From 2 chords (CCD,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] : 588f6f70-d9b1-11f1-43f3-8ed6f73d9457 [observed] Occultation Date + Time : 2026-09-22 at 22:05:26 UT +/- 0.0 min [1] Object Designation : (3885) Bogorodskij Orbit Class : MBA Star Designation : GDR3 2559380705428161408 Star Coordinates (ICRF) : RA = 01 28 25.8403, DE = +02 36 44.952 [2] Star Magnitudes : G = 14.69 mag, RP = 13.76 mag, BP = 15.59 mag Object Magnitude : V = 16.93 mag Estimated Magnitude Drop : 2.4 mag Estimated Max. Duration : 0.9 sec Object Mean Diameter : 8.7 km (src: astorb) Speed of the shadow : 10.0 km/s Elongation to Moon & Sun : 67° (sunlit = 85%), Sun = 158° Cross-track uncertainty : 0.7 mas = 0 km = 0.10 path-width (1-sig) RUWE and duplicate source : 0.97 mas, dup.src = 0 (0:false, 1:true) Ephemeris Reference : JPL61 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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