2026-02-26 / UCAC4 529-046450 / (2535) Hameenlinna
| # | OBS | Observer | Occ | Meth. | Instr. | CC | TSRC | UT1 | UT2 | UT3 | UT4 | UT2E | UT3E | Dur. | Chrd |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| 1 | show | Piotr Walczak | O+ | VID | M130 | PL | GPS | 18:11:44 | 18:12:43.68 | 18:12:45.08 | 18:13:49 | 0.180 | 0.120 | 1.40 | 7.1 |
| 2 | show | Marcin Górko | O+ | VID | L152 | PL | GPS | 18:12:15 | 18:12:42.707 | 18:12:44.158 | 18:13:15 | 0.040 | 0.040 | 1.45 | 7.4 |
| 3 | show | Nikolai Wuensche | O+ | VID | M300 | DE | GPS | 18:12:12 | 18:13:36.33 | 18:13:37.89 | 18:15:12 | 0.050 | 0.050 | 1.56 | 8.0 |
3 observations found in db: sodis
Available (probably) matching predictions (click on the link to switch):| JPL#73 : bae94360-de73-11f0-4858-b80867fdb41f [db: asteroids] |
Using prediction bae94360-de73-11f0-4858-b80867fdb41f for map and profile fit
| Ellipse and circular profile fits to the timings (chords) |
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Auto-Fit Result: Size = 26 x 3 km a',b' = 12.8, 1.3 km X0,Y0 = -1107.8, 25.9 km Mean diameter = 8 km From 3 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] : bae94360-de73-11f0-4858-b80867fdb41f [asteroids] Occultation Date + Time : 2026-02-26 at 17:58:52 UT +/- 0.01 min [1] Object Designation : (2535) Hameenlinna Orbit Class : MBA Star Designation : GDR3 0652634509855883648 Star Coordinates (ICRF) : RA = 08 29 09.8052, DE = +15 40 10.233 [2] Star Magnitudes : G = 11.22 mag, RP = 10.78 mag, BP = 11.49 mag Object Magnitude : V = 15.2 mag Estimated Magnitude Drop : 4.0 mag Estimated Max. Duration : 2.2 sec Object Mean Diameter : 11.0 km (src: astorb) Speed of the shadow : 5.1 km/s Elongation to Moon & Sun : 29° (sunlit = 75%), Sun = 147° Cross-track uncertainty : 0.6 mas = 0 km = 0.05 path-width (1-sig) RUWE and duplicate source : 2.76 mas, dup.src = 0 (0:false, 1:true) Ephemeris Reference : JPL#73 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) |