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2024-12-24 / UCAC4 633-014472 / (109990) 2001 SS58

#OBSObserverOccMeth.Instr.CC TSRCUT1UT2UT3UT4UT2EUT3EDur.Chrd
1 show Alberto Ossola O+ VID M230 CH GPS 20:06:24 20:07:56.13 20:07:56.29 20:08:48 0.08 0.08 0.16 1.7
2 show Peter Nosal, Paula Libic O+ VID M200 SK NTP 20:05:08 20:06:42.89 20:06:43.29 20:07:46 0.02 0.03 0.40 4.3
UT1/UT4: Begin/End of observation | UT2/UT3: Begin/End of occultation | Dur: Reported duration in seconds | Chrd: Corresponding chord length in km | More

2 observations found in db: sodis

Available (probably) matching predictions (click on the link to switch):
JPL#40 : cd9c0a60-ddb5-11f0-547e-4c24efffbcb0 [db: observed]

Using prediction cd9c0a60-ddb5-11f0-547e-4c24efffbcb0 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 = 318.8, 30.5 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).

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Map with groundtrack and observer stations

Event Details
 Occultation UUID [and DB] : cd9c0a60-ddb5-11f0-547e-4c24efffbcb0 [observed]

 Occultation Date + Time   : 2024-12-24 at 20:06:50 UT +/- 0.01 min  [1]
 Object Designation        : (109990) 2001 SS58
 Orbit Class               : MBA
 Star Designation          : GDR3 0220027605460078336
 Star Coordinates (ICRF)   : RA = 03 51 16.4948, DE = +36 24 24.638  [2]
 Star Magnitudes           : G = 11.97 mag, RP = 11.17 mag, BP = 12.65 mag
 Object Magnitude          : V = 19.83 mag
 Estimated Magnitude Drop  : 7.9 mag
 Estimated Max. Duration   : 0.4 sec
 Object Mean Diameter      : 4.0 km  (src: astorb)
 Speed of the shadow       : 10.8 km/s
 Elongation to Moon & Sun  : 139° (sunlit = 32%), Sun = 146°
 Cross-track uncertainty   : 2.3 mas = 4 km = 1.03 path-width (1-sig)
 RUWE and duplicate source : 1.04 mas, dup.src = 0  (0:false, 1:true)

 Ephemeris Reference       : JPL#40
 Note                      : FP:true

 
 [1] time t0 of closest geocentric approach c/a, [2] including proper motion until t0

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