2026-03-28 / UCAC4 491-056395 / (37732) 1996 TY68
| # | OBS | Observer | Occ | Meth. | Instr. | CC | TSRC | UT1 | UT2 | UT3 | UT4 | UT2E | UT3E | Dur. | Chrd |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| 1 | show | Deborah Smith | O+ | VID | M300 | ES | GPS | 20:24:58 | 20:25:58.532 | 20:25:59.782 | 20:26:58 | 0.138 | 0.138 | 1.25 | 20.0 |
| 2 | show | Wolfgang Beisker | O+ | VID | M360 | PT | GPS | 20:26:00 | 20:26:19.14 | 20:26:20.53 | 20:27:00 | 0.110 | 0.070 | 1.39 | 22.2 |
| 3 | show | Deborah Smith | O- | VID | M250 | ES | GPS | 20:24:59 | :: | :: | 20:26:59 |
3 observations found in db: sodis
Available (probably) matching predictions (click on the link to switch):| JPL#41 : 9192f150-de7d-11f0-4858-7993f9fb05ad [db: asteroids] |
Using prediction 9192f150-de7d-11f0-4858-7993f9fb05ad for map and profile fit
| Ellipse and circular profile fits to the timings (chords) |
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Auto-Fit Result: X0,Y0 = -428.9, 21.2 km Circular diameter = 24 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] : 9192f150-de7d-11f0-4858-7993f9fb05ad [asteroids] Occultation Date + Time : 2026-03-28 at 20:22:08 UT +/- 0.04 min [1] Object Designation : (37732) 1996 TY68 Orbit Class : JTRO Star Designation : GDR3 3818657076436556416 Star Coordinates (ICRF) : RA = 11 17 48.4727, DE = +08 08 04.671 [2] Star Magnitudes : G = 14.47 mag, RP = 14.02 mag, BP = 14.74 mag Object Magnitude : V = 19.02 mag Estimated Magnitude Drop : 4.6 mag Estimated Max. Duration : 0.9 sec Object Mean Diameter : 14.0 km (src: astorb) Speed of the shadow : 16.0 km/s Elongation to Moon & Sun : 30° (sunlit = 81%), Sun = 159° Cross-track uncertainty : 10.0 mas = 30 km = 2.20 path-width (1-sig) RUWE and duplicate source : 1.05 mas, dup.src = 0 (0:false, 1:true) Ephemeris Reference : JPL#41 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) |