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2025-04-21 / TYC 1911-00434-1 / (77) Frigga

#OBSObserverOccMeth.Instr.CC TSRCUT1UT2UT3UT4UT2EUT3EDur.Chrd
1 show Jordi Marco O+ CCD M235 ES NTP 19:34:30 19:35:59.644 19:36:02.197 19:37:28 0.017 0.017 2.55 58.9
2 show Joan Aragones O+ CCD M250 ES NTP 19:34:30 19:35:59.47 19:36:02.08 19:37:52 0.1 0.1 2.61 60.3
3 show Jorge JUAN, Carles Schnabel O+ VID M410 ES GPS 19:34:28 19:35:58.15 19:36:00.67 19:37:31 0.04 0.04 2.52 58.2
UT1/UT4: Begin/End of observation | UT2/UT3: Begin/End of occultation | Dur: Reported duration in seconds | Chrd: Corresponding chord length in km | More

3 observations found in db: sodis

Available (probably) matching predictions (click on the link to switch):
JPL#108 : c5966330-852b-11ef-78cd-0f96db3fa65d [db: asteroids]

Using prediction c5966330-852b-11ef-78cd-0f96db3fa65d 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:
Size = 66 x 3 km
a',b' = 32.8, 1.7 km
X0,Y0 = -589.9, 6.1 km
Mean diameter = 15 km

From 3 chords (VID,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).

Check SiMDA for size and mass data.

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Map with groundtrack and observer stations

Event Details
 Occultation UUID [and DB] : c5966330-852b-11ef-78cd-0f96db3fa65d [asteroids]

 Occultation Date + Time   : 2025-04-21 at 19:34:33 UT +/- 0.0 min  [1]
 Object Designation        : (77) Frigga
 Orbit Class               : MBA
 Star Designation          : GDR3 0868070344301213184
 Star Coordinates (ICRF)   : RA = 07 35 26.7741, DE = +23 25 02.731  [2]
 Star Magnitudes           : G = 10.0 mag, RP = 9.3 mag, BP = 10.54 mag
 Object Magnitude          : V = 13.71 mag
 Estimated Magnitude Drop  : 3.8 mag
 Estimated Max. Duration   : 3.0 sec
 Object Mean Diameter      : 69.2 km  (src: astorb)
 Speed of the shadow       : 23.1 km/s
 Elongation to Moon & Sun  : 161° (sunlit = 42%), Sun = 80°
 Cross-track uncertainty   : 0.7 mas = 1 km = 0.02 path-width (1-sig)
 RUWE and duplicate source : 0.85 mas, dup.src = 0  (0:false, 1:true)

 Ephemeris Reference       : JPL#108

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

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