2025-12-31 / UCAC4 469-001414 / (7226) Kryl
| # | OBS | Observer | Occ | Meth. | Instr. | CC | TSRC | UT1 | UT2 | UT3 | UT4 | UT2E | UT3E | Dur. | Chrd |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| 1 | show | Michael Kohl | O+ | VID | M200 | CH | GPS | 17:51:35 | 17:52:31.320 | 17:52:31.920 | 17:53:21 | 0.050 | 0.050 | 0.60 | 9.4 |
| 2 | show | Gregor Krannich | O+ | VID | M350 | DE | GPS | 17:51:57 | 17:52:41.129 | 17:52:41.933 | 17:53:27 | 0.005 | 0.005 | 0.80 | 12.5 |
| 3 | show | Andreas Schweizer | O- | VID | M250 | CH | GPS | 17:51:59 | :: | :: | 17:52:59 | ||||
| 4 | show | Stefan Meister | O- | VID | M200 | CH | GPS | 17:52:08 | :: | :: | 17:52:53 |
4 observations found in db: sodis
Available (probably) matching predictions (click on the link to switch):| JPL68 : 3f03aa90-d997-11f1-43f3-a9fdfdb6daf9 [db: observed] |
Using prediction 3f03aa90-d997-11f1-43f3-a9fdfdb6daf9 for map and profile fit
| Ellipse and circular profile fits to the timings (chords) |
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Auto-Fit Result: X0,Y0 = 1693.6, 33.8 km Circular diameter = 18 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] : 3f03aa90-d997-11f1-43f3-a9fdfdb6daf9 [observed] Occultation Date + Time : 2025-12-31 at 17:50:19 UT +/- 0.0 min [1] Object Designation : (7226) Kryl Orbit Class : MBA Star Designation : GDR3 2551853444529265536 Star Coordinates (ICRF) : RA = 01 01 45.6429, DE = +03 39 09.220 [2] Star Magnitudes : G = 11.53 mag, RP = 10.88 mag, BP = 12.02 mag Object Magnitude : V = 17.86 mag Estimated Magnitude Drop : 6.3 mag Estimated Max. Duration : 0.6 sec Object Mean Diameter : 9.4 km (src: astorb) Speed of the shadow : 15.6 km/s Elongation to Moon & Sun : 48° (sunlit = 90%), Sun = 95° Cross-track uncertainty : 1.0 mas = 1 km = 0.18 path-width (1-sig) RUWE and duplicate source : 1.13 mas, dup.src = 0 (0:false, 1:true) Ephemeris Reference : JPL68 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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