2026-10-08 / UCAC4 484-130525 / (1031) Arctica
| # | OBS | Observer | Occ | Meth. | Instr. | CC | TSRC | UT1 | UT2 | UT3 | UT4 | UT2E | UT3E | Dur. | Chrd |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| 1 | show | Ferran Casarramona | O+ | VID | M200 | ES | GPS | 23:25:02 | 23:29:48.374 | 23:29:54.288 | 23:35:00 | 0.432 | 0.432 | 5.91 | 59.1 |
| 2 | show | Deborah Smith | O+ | VID | M300 | ES | GPS | 23:28:50 | 23:29:46.385 | 23:29:53.009 | 23:30:50 | 0.344 | 0.344 | 6.62 | 66.2 |
| 3 | show | Deborah Smith | O- | VID | M250 | ES | GPS | 23:28:47 | :: | :: | 23:30:47 |
3 observations found in db: sodis
Available (probably) matching predictions (click on the link to switch):| JPL81 : 408753a0-d9b3-11f1-43f3-7c6dfd7c7787 [db: observed] |
Using prediction 408753a0-d9b3-11f1-43f3-7c6dfd7c7787 for map and profile fit
| Ellipse and circular profile fits to the timings (chords) |
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Auto-Fit Result: X0,Y0 = -2768.4, 26.7 km Circular diameter = 80 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] : 408753a0-d9b3-11f1-43f3-7c6dfd7c7787 [observed] Occultation Date + Time : 2026-10-08 at 23:36:17 UT +/- 0.08 min [1] Object Designation : (1031) Arctica Orbit Class : MBA Star Designation : GDR3 2701175747876542720 Star Coordinates (ICRF) : RA = 21 42 02.8367, DE = +06 38 15.970 [2] Star Magnitudes : G = 15.13 mag, RP = 14.52 mag, BP = 15.58 mag Object Magnitude : V = 14.77 mag Estimated Magnitude Drop : 0.6 mag Estimated Max. Duration : 7.5 sec Object Mean Diameter : 75.5 km (src: astorb) Speed of the shadow : 10.0 km/s Elongation to Moon & Sun : 150° (sunlit = 3%), Sun = 131° Cross-track uncertainty : 1.3 mas = 2 km = 0.03 path-width (1-sig) RUWE and duplicate source : 1.04 mas, dup.src = 0 (0:false, 1:true) Ephemeris Reference : JPL81 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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| Aladin Sky Atlas |
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