2023-09-05 / UCAC4 400-124523 / (25307) 1998 XU77
# | OBS | Observer | Occ | Meth. | Instr. | CC | TSRC | UT1 | UT2 | UT3 | UT4 | UT2E | UT3E | Dur. | Chrd |
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1 | show | Gregor Krannich | O+ | VID | M350 | DE | GPS | 20:38:25 | 20:39:53.300 | 20:39:54.740 | 20:41:25 | 0.16 | 0.16 | 1.44 | 7.3 |
2 | show | Zdenek Moravec, Bohuslav Matouš | O+ | CCD | T432 | CZ | GPS | 20:38:12 | 20:39:10.79 | 20:39:12.26 | 20:40:12 | 0.10 | 0.12 | 1.47 | 7.5 |
3 | show | Zdenek Sikac | O- | VID | T150 | CZ | NTP | 20:37:01 | 20:41:00 | ||||||
4 | show | Anna Marciniak | O- | CCD | M350 | PL | GPS | 20:37:45 | 20:39:49 |
4 observations found in db: sodis
Available (probably) matching predictions (click on the link to switch):JPL#48 : 1cb3a868-a424-4544-95e6-135d0ed8db2a [db: observed] |
JPL#55 : 3bd5fb90-c33f-11ef-5276-07d27dd91b8f [db: observed] |
Using prediction 1cb3a868-a424-4544-95e6-135d0ed8db2a for map and profile fit
Ellipse and circular profile fits to the timings (chords) |
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Auto-Fit Result: X0,Y0 = 2411.6, 17.9 km Circular diameter = 8 km From 2 chords (CCD,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] : 1cb3a868-a424-4544-95e6-135d0ed8db2a [observed] Occultation Date + Time : 2023-09-05 at 20:52:50 UT +/- 0.09 min [1] Object Designation : (25307) 1998 XU77 Orbit Class : MBA Star Designation : GDR3 4193462001733379328 Star Coordinates (ICRF) : RA = 19 49 11.3936, DE = -10 10 20.487 [2] Star Magnitudes : G = 13.74 mag, RP = 13.22 mag, BP = 14.08 mag Object Magnitude : V = 18.62 mag Estimated Magnitude Drop : 4.9 mag Estimated Max. Duration : 1.3 sec Object Mean Diameter : 6.8 km (src: astorb) Speed of the shadow : 5.1 km/s Elongation to Moon & Sun : 122° (sunlit = 61%), Sun = 133° Cross-track uncertainty : 4.0 mas = 6 km = 1.00 path-width (1-sig) RUWE and duplicate source : 1.01 mas, dup.src = 0 (0:false, 1:true) Ephemeris Reference : JPL#48 [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) |