2026-10-15 / HIP 12893 / (61784) 2000 QL178
| # | OBS | Observer | Occ | Meth. | Instr. | CC | TSRC | UT1 | UT2 | UT3 | UT4 | UT2E | UT3E | Dur. | Chrd |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| 1 | show | Björn Kattentidt | O+ | VID | T50 | DE | GPS | 02:41:31 | 02:42:17.265 | 02:42:17.580 | 02:43:31 | 0.015 | 0.015 | 0.32 | 2.7 |
| 2 | show | Björn Kattentidt | O+ | VID | T50 | DE | GPS | 02:41:29 | 02:42:17.068 | 02:42:17.592 | 02:43:29 | 0.009 | 0.009 | 0.52 | 4.3 |
| 3 | show | Björn Kattentidt | O- | VID | T50 | DE | GPS | 02:41:25 | :: | :: | 02:43:25 | ||||
| 4 | show | Björn Kattentidt | O- | VID | T50 | DE | GPS | 02:41:28 | :: | :: | 02:43:27 |
4 observations found in db: sodis
Available (probably) matching predictions (click on the link to switch):| JPL47 : e6c79950-d9b3-11f1-43f3-73e4afdd9fc1 [db: observed] |
Using prediction e6c79950-d9b3-11f1-43f3-73e4afdd9fc1 for map and profile fit
| Ellipse and circular profile fits to the timings (chords) |
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Auto-Fit Result: X0,Y0 = 871.7, 24.6 km Circular diameter = 5 km From 2 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] : e6c79950-d9b3-11f1-43f3-73e4afdd9fc1 [observed] Occultation Date + Time : 2026-10-15 at 02:50:12 UT +/- 0.01 min [1] Object Designation : (61784) 2000 QL178 Orbit Class : MBA Star Designation : GDR3 0081875206377503488 Star Coordinates (ICRF) : RA = 02 45 43.1138, DE = +17 01 16.633 [2] Star Magnitudes : G = 6.77 mag, RP = 5.94 mag, BP = 7.49 mag Object Magnitude : V = 18.61 mag Estimated Magnitude Drop : 11.8 mag Estimated Max. Duration : 0.4 sec Object Mean Diameter : 3.0 km (src: astorb) Speed of the shadow : 8.3 km/s Elongation to Moon & Sun : 151° (sunlit = 19%), Sun = 158° Cross-track uncertainty : 1.0 mas = 1 km = 0.35 path-width (1-sig) RUWE and duplicate source : 0.91 mas, dup.src = 0 (0:false, 1:true) Ephemeris Reference : JPL47 Note : FP:true [1] time t0 of closest geocentric approach c/a, [2] including proper motion until t0 |
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