2026-07-13 / UCAC4 325-186295 / (1194) Aletta
| # | OBS | Observer | Occ | Meth. | Instr. | CC | TSRC | UT1 | UT2 | UT3 | UT4 | UT2E | UT3E | Dur. | Chrd |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| 1 | show | Ferran Casarramona | O+ | VID | M200 | ES | GPS | 21:28:02 | 21:30:17.78 | 21:30:22.30 | 21:33:02 | 0.044 | 0.044 | 4.52 | 55.6 |
| 2 | show | Deborah Smith | O+ | VID | M300 | ES | GPS | 21:29:22 | 21:30:20.564 | 21:30:25.043 | 21:31:23 | 0.016 | 0.016 | 4.48 | 55.1 |
| 3 | show | Deborah Smith | O+ | VID | M250 | ES | GPS | 21:29:25 | 21:30:22.668 | 21:30:27.080 | 21:31:25 | 0.017 | 0.017 | 4.41 | 54.2 |
3 observations found in db: sodis
Available (probably) matching predictions (click on the link to switch):| JPL74 : 75e7f6c0-d9aa-11f1-43f3-3a477ffb846e [db: observed] |
Using prediction 75e7f6c0-d9aa-11f1-43f3-3a477ffb846e for map and profile fit
| Ellipse and circular profile fits to the timings (chords) |
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Auto-Fit Result: Size = 58 x 25 km a',b' = 29.1, 12.5 km X0,Y0 = -984.0, 23.3 km Mean diameter = 38 km From 3 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] : 75e7f6c0-d9aa-11f1-43f3-3a477ffb846e [observed] Occultation Date + Time : 2026-07-13 at 21:25:37 UT +/- 0.0 min [1] Object Designation : (1194) Aletta Orbit Class : MBA Star Designation : GDR3 4073461611954143104 Star Coordinates (ICRF) : RA = 18 42 48.9618, DE = -25 09 55.120 [2] Star Magnitudes : G = 11.76 mag, RP = 10.8 mag, BP = 12.72 mag Object Magnitude : V = 14.81 mag Estimated Magnitude Drop : 3.1 mag Estimated Max. Duration : 4.5 sec Object Mean Diameter : 55.4 km (src: astorb) Speed of the shadow : 12.3 km/s Elongation to Moon & Sun : 175° (sunlit = 0%), Sun = 168° Cross-track uncertainty : 0.7 mas = 0 km = 0.02 path-width (1-sig) RUWE and duplicate source : 0.85 mas, dup.src = 0 (0:false, 1:true) Ephemeris Reference : JPL74 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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