2026-09-30 / UCAC4 510-010411 / (164110) 2003 XM16
| # | OBS | Observer | Occ | Meth. | Instr. | CC | TSRC | UT1 | UT2 | UT3 | UT4 | UT2E | UT3E | Dur. | Chrd |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| 1 | show | Peter Nosal | O+ | VID | M250 | SK | NTP | 02:41:57 | 02:43:07.340 | 02:43:08.390 | 02:44:11 | 0.050 | 0.050 | 1.05 | 5.1 |
| 2 | show | Tomas Janik | O+ | CCD | T600 | CZ | GPS | 02:41:05 | 02:41:40.76 | 02:41:41.35 | 02:42:29 | 0.030 | 0.030 | 0.59 | 2.9 |
| 3 | show | Peter Nosal, Paula Libic | O- | VID | M200 | SK | NTP | 02:42:03 | :: | :: | 02:44:15 |
3 observations found in db: sodis
Available (probably) matching predictions (click on the link to switch):| JPL41 : fb3f9410-d9b2-11f1-43f3-c3a29bfdfc93 [db: observed] |
Using prediction fb3f9410-d9b2-11f1-43f3-c3a29bfdfc93 for map and profile fit
| Ellipse and circular profile fits to the timings (chords) |
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Auto-Fit Result: Circular profile fit was not successful ... 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] : fb3f9410-d9b2-11f1-43f3-c3a29bfdfc93 [observed] Occultation Date + Time : 2026-09-30 at 02:51:25 UT +/- 0.06 min [1] Object Designation : (164110) 2003 XM16 Orbit Class : MBA Star Designation : GDR3 3388007543255229184 Star Coordinates (ICRF) : RA = 05 12 24.5242, DE = +11 58 18.370 [2] Star Magnitudes : G = 12.47 mag, RP = 11.9 mag, BP = 12.86 mag Object Magnitude : V = 20.38 mag Estimated Magnitude Drop : 7.9 mag Estimated Max. Duration : 0.6 sec Object Mean Diameter : 2.9 km (src: astorb) Speed of the shadow : 4.9 km/s Elongation to Moon & Sun : 31° (sunlit = 86%), Sun = 108° Cross-track uncertainty : 2.3 mas = 3 km = 1.33 path-width (1-sig) RUWE and duplicate source : 1.02 mas, dup.src = 0 (0:false, 1:true) Ephemeris Reference : JPL41 Note : FP:true [1] time t0 of closest geocentric approach c/a, [2] including proper motion until t0 |
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