2026-07-05 / UCAC4 459-074335 / (921) Jovita
| # | OBS | Observer | Occ | Meth. | Instr. | CC | TSRC | UT1 | UT2 | UT3 | UT4 | UT2E | UT3E | Dur. | Chrd |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| 1 | show | Alfonso Noschese | O+ | VID | M450 | IT | GPS | 01:26:06 | 01:26:30.1 | 01:26:36.7 | 01:27:04 | 1.200 | 0.300 | 6.60 | 57.4 |
| 2 | show | Antonio Vecchione | O+ | VID | M250 | IT | GPS | 01:26:09 | 01:26:32.1 | 01:26:36.7 | 01:27:05 | 1.400 | 0.300 | 4.60 | 40.0 |
2 observations found in db: sodis
Available (probably) matching predictions (click on the link to switch):| JPL95 : 66cda690-d9a9-11f1-43f3-b67ae7fea6cb [db: observed] |
Using prediction 66cda690-d9a9-11f1-43f3-b67ae7fea6cb for map and profile fit
| Ellipse and circular profile fits to the timings (chords) |
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Auto-Fit Result: X0,Y0 = 6.1, 17.9 km Circular diameter = 70 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] : 66cda690-d9a9-11f1-43f3-b67ae7fea6cb [observed] Occultation Date + Time : 2026-07-05 at 01:33:26 UT +/- 0.01 min [1] Object Designation : (921) Jovita Orbit Class : MBA Star Designation : GDR3 4468174565318884480 Star Coordinates (ICRF) : RA = 18 06 30.8516, DE = +01 38 15.009 [2] Star Magnitudes : G = 14.83 mag, RP = 14.0 mag, BP = 15.54 mag Object Magnitude : V = 13.75 mag Estimated Magnitude Drop : 0.3 mag Estimated Max. Duration : 6.7 sec Object Mean Diameter : 58.5 km (src: astorb) Speed of the shadow : 8.7 km/s Elongation to Moon & Sun : 70° (sunlit = 77%), Sun = 153° Cross-track uncertainty : 1.0 mas = 1 km = 0.02 path-width (1-sig) RUWE and duplicate source : 1.01 mas, dup.src = 0 (0:false, 1:true) Ephemeris Reference : JPL95 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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