2026-04-17 / UCAC4 383-065030 / (309) Fraternitas
| # | OBS | Observer | Occ | Meth. | Instr. | CC | TSRC | UT1 | UT2 | UT3 | UT4 | UT2E | UT3E | Dur. | Chrd |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| 1 | show | Antonio Catapano | O+ | VID | T500 | IT | GPS | 21:15:06 | 21:16:03.1 | 21:16:06.2 | 21:17:02 | 0.300 | 0.200 | 3.10 | 36.6 |
| 2 | show | Alfonso Noschese | O+ | VID | M450 | IT | GPS | 21:15:22 | 21:16:01.2 | 21:16:02.9 | 21:16:50 | 0.200 | 0.300 | 1.70 | 20.1 |
| 3 | show | Ettore Marmo | O- | VID | M300 | IT | GPS | 21:14:41 | :: | :: | 21:18:11 |
3 observations found in db: sodis
Available (probably) matching predictions (click on the link to switch):| JPL#88 : 8dc56800-33c3-11f1-6999-12477f7fbd1a [db: asteroids] |
Using prediction 8dc56800-33c3-11f1-6999-12477f7fbd1a for map and profile fit
| Ellipse and circular profile fits to the timings (chords) |
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Auto-Fit Result: X0,Y0 = -1214.9, 23.7 km Circular diameter = 43 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] : 8dc56800-33c3-11f1-6999-12477f7fbd1a [asteroids] Occultation Date + Time : 2026-04-17 at 21:11:17 UT +/- 0.0 min [1] Object Designation : (309) Fraternitas Orbit Class : MBA Star Designation : GDR3 3607175807359584512 Star Coordinates (ICRF) : RA = 13 37 09.6354, DE = -13 24 16.918 [2] Star Magnitudes : G = 14.56 mag, RP = 14.09 mag, BP = 14.85 mag Object Magnitude : V = 14.08 mag Estimated Magnitude Drop : 0.5 mag Estimated Max. Duration : 3.9 sec Object Mean Diameter : 45.3 km (src: astorb) Speed of the shadow : 11.8 km/s Elongation to Moon & Sun : 174° (sunlit = 0%), Sun = 177° Cross-track uncertainty : 1.0 mas = 1 km = 0.03 path-width (1-sig) RUWE and duplicate source : 0.91 mas, dup.src = 0 (0:false, 1:true) Ephemeris Reference : JPL#88 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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(If error 404: link not valid which means no data available)
| Aladin Sky Atlas |
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| Aladin Lite direct link (has Gaia overlay) |