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2022-06-22 / 4UC 387-113992 / (29603) 1998 MO44

#OBSObserverOccMeth.Instr.CC TSRCUT1UT2UT3UT4UT2EUT3EDur.Chrd
1 show Sven Andersson O+ CCD M355 DE GPS++ 23:17:01 23:17:47.70 23:17:49.25 23:19:01 0.04 0.04 1.55 28.4
2 show Christian Weber O+ VID M203 DE GPS++ 23:16:10 23:17:48.20 23:17:49.40 23:19:01 0.08 0.08 1.20 22.0
3 show Anna Marciniak O- CCD M350 PL 23:16:31 23:18:30
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: euraster

Available (probably) matching predictions (click on the link to switch):
JPL#40 : 6d16c1aa-83b6-48f4-b355-818d5ba8c76e [db: observed]

Using prediction 6d16c1aa-83b6-48f4-b355-818d5ba8c76e 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 = 2319.3, 0.3 km
Circular diameter = 30 km

From 2 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).

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Map with groundtrack and observer stations

Event Details
 Occultation UUID [and DB] : 6d16c1aa-83b6-48f4-b355-818d5ba8c76e [observed]

 Occultation Date + Time   : 2022-06-22 at 23:19:29 UT +/- 0.05 min  [1]
 Object Designation        : (29603) 1998 MO44
 Orbit Class               : JTRO
 Star Designation          : GDR3 4102717653523641472
 Star Coordinates (ICRF)   : RA = 18 54 50.8231, DE = -12 38 23.987  [2]
 Star Magnitudes           : G = 11.85 mag, RP = 10.96 mag, BP = 12.68 mag
 Object Magnitude          : V = 18.02 mag
 Estimated Magnitude Drop  : 6.2 mag
 Estimated Max. Duration   : 1.1 sec
 Object Mean Diameter      : 20 km  (src: astorb)
 Speed of the shadow       : 18.3 km/s
 Elongation to Moon & Sun  : 100° (sunlit = 31%), Sun = 164°
 Cross-track uncertainty   : 8.7 mas = 25 km = 1.28 path-width (1-sig)
 RUWE and duplicate source : 0.87 mas, dup.src = 0  (0:false, 1:true)

 Ephemeris Reference       : JPL#40

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

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