2026-03-06 / UCAC4 313-081901 / (972) Cohnia
| # | OBS | Observer | Occ | Meth. | Instr. | CC | TSRC | UT1 | UT2 | UT3 | UT4 | UT2E | UT3E | Dur. | Chrd |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| 1 | show | Marek Harman | O+ | VID | M350 | SK | NTP | 02:19:26 | 02:21:18.180 | 02:21:24.800 | 02:23:22 | 0.050 | 0.050 | 6.62 | 36.4 |
| 2 | show | Peter Delincak | O+ | VID | M400 | SK | NTP | 02:19:16 | 02:21:14.521 | 02:21:20.312 | 02:22:40 | 0.040 | 0.040 | 5.79 | 31.8 |
| 3 | show | Anna Marciniak | O+ | CCD | M400 | PL | GPS | 02:18:59 | 02:20:59.8 | 02:21:10.1 | 02:23:14 | 0.300 | 0.400 | 10.30 | 56.7 |
3 observations found in db: sodis
Available (probably) matching predictions (click on the link to switch):| JPL#71 : ed6da4c0-de6e-11f0-4858-528ff3df177e [db: asteroids] |
Using prediction ed6da4c0-de6e-11f0-4858-528ff3df177e for map and profile fit
| Ellipse and circular profile fits to the timings (chords) |
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Auto-Fit Result: Size = 238 x 9 km a',b' = 119.1, 4.5 km X0,Y0 = -2591.4, 0.8 km Mean diameter = 46 km From 3 chords (VID,CCD) 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] : ed6da4c0-de6e-11f0-4858-528ff3df177e [asteroids] Occultation Date + Time : 2026-03-06 at 02:35:59 UT +/- 0.03 min [1] Object Designation : (972) Cohnia Orbit Class : MBA Star Designation : GDR3 6213450812560020480 Star Coordinates (ICRF) : RA = 15 30 44.6273, DE = -27 27 40.435 [2] Star Magnitudes : G = 12.24 mag, RP = 11.41 mag, BP = 12.97 mag Object Magnitude : V = 15.86 mag Estimated Magnitude Drop : 3.7 mag Estimated Max. Duration : 13.7 sec Object Mean Diameter : 75.7 km (src: astorb) Speed of the shadow : 5.5 km/s Elongation to Moon & Sun : 40° (sunlit = 93%), Sun = 108° Cross-track uncertainty : 0.3 mas = 0 km = 0.01 path-width (1-sig) RUWE and duplicate source : 1.15 mas, dup.src = 0 (0:false, 1:true) Ephemeris Reference : JPL#71 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) |