2026-10-08 / UCAC4 304-251417 / (1947) Iso-Heikkila
| # | OBS | Observer | Occ | Meth. | Instr. | CC | TSRC | UT1 | UT2 | UT3 | UT4 | UT2E | UT3E | Dur. | Chrd |
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| 1 | show | Carles Schnabel | O+ | VID | M400 | ES | GPS | 18:58:32 | 19:00:10.54 | 19:00:12.94 | 19:02:06 | 0.100 | 0.100 | 2.40 | 41.5 |
| 2 | show | Jorge JUAN, Carles Schnabel | O+ | VID | M410 | ES | GPS | 18:58:11 | 19:00:10.11 | 19:00:12.41 | 19:02:03 | 0.100 | 0.100 | 2.30 | 39.8 |
2 observations found in db: sodis
Available (probably) matching predictions (click on the link to switch):| JPL77 : 3d201750-d9b4-11f1-43f3-8454b6ff9b30 [db: observed] |
Using prediction 3d201750-d9b4-11f1-43f3-8454b6ff9b30 for map and profile fit
| Ellipse and circular profile fits to the timings (chords) |
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Auto-Fit Result: X0,Y0 = 557.2, 6.7 km Circular diameter = 41 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] : 3d201750-d9b4-11f1-43f3-8454b6ff9b30 [observed] Occultation Date + Time : 2026-10-08 at 18:58:10 UT +/- 0.01 min [1] Object Designation : (1947) Iso-Heikkila Orbit Class : MBA Star Designation : GDR3 6760945515146637824 Star Coordinates (ICRF) : RA = 19 02 19.0475, DE = -29 21 46.298 [2] Star Magnitudes : G = 12.3 mag, RP = 11.76 mag, BP = 12.67 mag Object Magnitude : V = 17.11 mag Estimated Magnitude Drop : 4.8 mag Estimated Max. Duration : 1.7 sec Object Mean Diameter : 29.4 km (src: astorb) Speed of the shadow : 17.3 km/s Elongation to Moon & Sun : 111° (sunlit = 4%), Sun = 88° Cross-track uncertainty : 0.3 mas = 0 km = 0.02 path-width (1-sig) RUWE and duplicate source : 0.9 mas, dup.src = 0 (0:false, 1:true) Ephemeris Reference : JPL77 Note : FP:true [1] time t0 of closest geocentric approach c/a, [2] including proper motion until t0 |
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