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2023-09-05 / UCAC4 400-124523 / (25307) 1998 XU77

#OBSObserverOccMeth.Instr.CC TSRCUT1UT2UT3UT4UT2EUT3EDur.Chrd
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
UT1/UT4: Begin/End of observation | UT2/UT3: Begin/End of occultation | Dur: Reported duration in seconds | Chrd: Corresponding chord length in km | More

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]

Using prediction 1cb3a868-a424-4544-95e6-135d0ed8db2a for map and profile fit

Get observations as KML file (reduced site location resolution)

Ellipse and circular profile fits to the timings (chords)

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).

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Map with groundtrack and observer stations

Event Details
 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      : 7 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

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