2026-07-28 / UCAC4 639-101360 / (206956) 2004 RL327
| # | OBS | Observer | Occ | Meth. | Instr. | CC | TSRC | UT1 | UT2 | UT3 | UT4 | UT2E | UT3E | Dur. | Chrd |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| 1 | show | Jorge JUAN, Carles Schnabel | O+ | VID | M410 | ES | GPS | 20:50:35 | 20:53:37.46 | 20:53:37.76 | 20:56:08 | 0.070 | 0.080 | 0.30 | 3.9 |
| 2 | show | Antoni Selva, Carlos Perello | O+ | VID | M500 | ES | GPS | 20:52:37 | 20:53:35.93 | 20:53:36.33 | 20:54:37 | 0.040 | 0.040 | 0.40 | 5.2 |
2 observations found in db: sodis
Available (probably) matching predictions (click on the link to switch):| JPL37 : d7231940-d9ac-11f1-43f3-410fe7cf0c2c [db: observed] |
Using prediction d7231940-d9ac-11f1-43f3-410fe7cf0c2c for map and profile fit
| Ellipse and circular profile fits to the timings (chords) |
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Auto-Fit Result: X0,Y0 = 533.8, 20.1 km Circular diameter = 6 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] : d7231940-d9ac-11f1-43f3-410fe7cf0c2c [observed] Occultation Date + Time : 2026-07-28 at 20:48:08 UT +/- 0.01 min [1] Object Designation : (206956) 2004 RL327 Orbit Class : MBA Star Designation : GDR3 1868706602255198208 Star Coordinates (ICRF) : RA = 21 14 31.8624, DE = +37 43 18.634 [2] Star Magnitudes : G = 13.86 mag, RP = 13.18 mag, BP = 14.38 mag Object Magnitude : V = 19.16 mag Estimated Magnitude Drop : 5.3 mag Estimated Max. Duration : 0.3 sec Object Mean Diameter : 3.9 km (src: astorb) Speed of the shadow : 13.0 km/s Elongation to Moon & Sun : 64° (sunlit = 99%), Sun = 123° Cross-track uncertainty : 1.7 mas = 2 km = 0.60 path-width (1-sig) RUWE and duplicate source : 0.98 mas, dup.src = 0 (0:false, 1:true) Ephemeris Reference : JPL37 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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