2026-08-18 / UCAC4 419-082798 / (58211) 1992 HF4
| # | OBS | Observer | Occ | Meth. | Instr. | CC | TSRC | UT1 | UT2 | UT3 | UT4 | UT2E | UT3E | Dur. | Chrd |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| 1 | show | Ferran Casarramona | O+ | VID | M200 | ES | GPS | 00:27:02 | 00:27:56.31 | 00:27:57.05 | 00:29:02 | 0.140 | 0.140 | 0.74 | 3.6 |
| 2 | show | Ferran Casarramona | O+ | VID | M200 | ES | GPS | 00:27:02 | 00:27:58.55 | 00:27:58.71 | 00:29:02 | 0.080 | 0.080 | 0.16 | 0.8 |
| 3 | show | Deborah Smith | O- | VID | M300 | ES | GPS | 00:26:46 | :: | :: | 00:28:46 |
3 observations found in db: sodis
Available (probably) matching predictions (click on the link to switch):| JPL53 : 0b1098d0-d9ae-11f1-43f3-82e47f7fa229 [db: observed] |
Using prediction 0b1098d0-d9ae-11f1-43f3-82e47f7fa229 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] : 0b1098d0-d9ae-11f1-43f3-82e47f7fa229 [observed] Occultation Date + Time : 2026-08-18 at 00:29:16 UT +/- 0.02 min [1] Object Designation : (58211) 1992 HF4 Orbit Class : MBA Star Designation : GDR3 4256027443186663424 Star Coordinates (ICRF) : RA = 18 33 25.1938, DE = -06 18 06.978 [2] Star Magnitudes : G = 12.33 mag, RP = 10.97 mag, BP = 14.61 mag Object Magnitude : V = 17.13 mag Estimated Magnitude Drop : 4.8 mag Estimated Max. Duration : 0.8 sec Object Mean Diameter : 3.7 km (src: astorb) Speed of the shadow : 4.8 km/s Elongation to Moon & Sun : 70° (sunlit = 30%), Sun = 131° Cross-track uncertainty : 1.1 mas = 0 km = 0.21 path-width (1-sig) RUWE and duplicate source : 1.16 mas, dup.src = 0 (0:false, 1:true) Ephemeris Reference : JPL53 Note : FP:true [1] time t0 of closest geocentric approach c/a, [2] including proper motion until t0 |
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