2026-09-17 / UCAC4 422-128988 / (7603) Salopia
| # | OBS | Observer | Occ | Meth. | Instr. | CC | TSRC | UT1 | UT2 | UT3 | UT4 | UT2E | UT3E | Dur. | Chrd |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| 1 | show | Jiri Kubanek | O+ | VID | M303 | CZ | GPS | 18:51:32 | 18:52:30.0 | 18:52:30.68 | 18:53:33 | 0.300 | 0.180 | 0.68 | 3.8 |
| 2 | show | Jiri Kubanek | O+ | VID | M303 | CZ | GPS | 18:51:32 | 18:52:31.130 | 18:52:32.210 | 18:53:33 | 0.180 | 0.090 | 1.08 | 6.0 |
| 3 | show | Tomas Janik | O- | CCD | T600 | CZ | GPS | 18:51:22 | :: | :: | 18:53:20 |
3 observations found in db: sodis
Available (probably) matching predictions (click on the link to switch):| JPL61 : fd4d5050-d9b0-11f1-43f3-372bdbef8471 [db: observed] |
Using prediction fd4d5050-d9b0-11f1-43f3-372bdbef8471 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] : fd4d5050-d9b0-11f1-43f3-372bdbef8471 [observed] Occultation Date + Time : 2026-09-17 at 19:06:13 UT +/- 0.06 min [1] Object Designation : (7603) Salopia Orbit Class : MBA Star Designation : GDR3 6908343574360179840 Star Coordinates (ICRF) : RA = 20 32 56.4156, DE = -05 47 07.607 [2] Star Magnitudes : G = 14.32 mag, RP = 13.63 mag, BP = 14.86 mag Object Magnitude : V = 17.89 mag Estimated Magnitude Drop : 3.6 mag Estimated Max. Duration : 1.5 sec Object Mean Diameter : 8.1 km (src: astorb) Speed of the shadow : 5.6 km/s Elongation to Moon & Sun : 58° (sunlit = 40%), Sun = 133° Cross-track uncertainty : 1.0 mas = 1 km = 0.19 path-width (1-sig) RUWE and duplicate source : 0.98 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 |
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