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2024-11-28 / UCAC4 367-062199 / (324) Bamberga

#OBSObserverOccMeth.Instr.CC TSRCUT1UT2UT3UT4UT2EUT3EDur.Chrd
1 show Jordi Marco O+ CCD M235 ES NTP 05:40:04 05:42:58.3 05:43:02.1 05:44:01 0.4 0.4 3.80 136.0
2 show Oscar Canales O+ CCD M280 ES GPS 05:41:26 05:42:53.52 05:43:00.02 05:44:26 0.17 0.17 6.50 232.7
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#166 : a25fc0a0-858a-11ef-78cd-5ea67bdb19d1 [db: asteroids]
JPL#166 : bac1f680-826b-11ef-6618-47b6d1ebb568 [db: asteroids]

Using prediction a25fc0a0-858a-11ef-78cd-5ea67bdb19d1 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 = -1263.0, 19.4 km
Circular diameter = 234 km

From 2 chords (CCD)








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] : a25fc0a0-858a-11ef-78cd-5ea67bdb19d1 [asteroids]

 Occultation Date + Time   : 2024-11-28 at 05:45:30 UT +/- 0.0 min  [1]
 Object Designation        : (324) Bamberga
 Orbit Class               : MBA
 Star Designation          : GDR3 3604273539043532928
 Star Coordinates (ICRF)   : RA = 13 26 52.9492, DE = -16 36 22.418  [2]
 Star Magnitudes           : G = 12.59 mag, RP = 12.17 mag, BP = 12.86 mag
 Object Magnitude          : V = 13.88 mag
 Estimated Magnitude Drop  : 1.6 mag
 Estimated Max. Duration   : 6.4 sec
 Object Mean Diameter      : 229 km  (src: astorb)
 Speed of the shadow       : 35.8 km/s
 Elongation to Moon & Sun  : 8° (sunlit = 8%), Sun = 41°
 Cross-track uncertainty   : 0.7 mas = 2 km = 0.01 path-width (1-sig)
 RUWE and duplicate source : 1.07 mas, dup.src = 0  (0:false, 1:true)

 Ephemeris Reference       : JPL#166

 Object is a Gaia mass determination target !
[1] time t0 of closest geocentric approach c/a, [2] including proper motion until t0

More Data and Informations
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