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2006-12-22 / TYC 0675-00594-1 / (2934) Aristophanes

#OBSObserverOccMeth.Instr.CC TSRCUT1UT2UT3UT4UT2EUT3EDur.Chrd
1 show Rene Bourtembourg O+ VIS M254 BE RAD 18:29:00 18:31:09.25 18:31:10.78 18:34:00 0.50 0.50 1.53 17.1
2 show E. Frappa/A. Klotz O- CCD M250 FR 18:31:21 18:34:28
3 show Stefano Sposetti O- CCD M400 CH 18:28:30 18:34:30
4 show Arnaud Leroy O- VID M355 FR 18:28:00 18:34:00
5 show Olivier Dechambre O- VID M279 FR 18:27:00 18:40:00
6 show F. Van Den Abbeel O- CCD M200 BE 18:31:00 18:31:50
7 show Thierry Pauwels O- CCD M850 BE 18:19:10 18:43:20
UT1/UT4: Begin/End of observation | UT2/UT3: Begin/End of occultation | Dur: Reported duration in seconds | Chrd: Corresponding chord length in km | More

7 observations found in db: euraster

Available (probably) matching predictions (click on the link to switch):
JPL#54 : c82926e8-1a6a-47a8-b964-3b18fa9d2799 [db: observed]
JPL#54 : ba746652-8f22-4ec2-91dc-66159625b8fe [db: observed]

Using prediction c82926e8-1a6a-47a8-b964-3b18fa9d2799 for map and profile fit

Get observations as KML file (reduced site location resolution)


Map with groundtrack and observer stations

Event Details
 Occultation UUID [and DB] : c82926e8-1a6a-47a8-b964-3b18fa9d2799 [observed]

 Occultation Date + Time   : 2006-12-22 at 18:34:40 UT +/- 0.04 min  [1]
 Object Designation        : (2934) Aristophanes
 Orbit Class               : MBA
 Star Designation          : GDR3 3304135250100217344
 Star Coordinates (ICRF)   : RA = 04 16 58.4608, DE = +11 52 39.475  [2]
 Star Magnitudes           : G = 16.06 mag, RP = 15.33 mag, BP = 16.54 mag
 Object Magnitude          : V = 16.79 mag
 Estimated Magnitude Drop  : 1.2 mag
 Estimated Max. Duration   : 2.5 sec
 Object Mean Diameter      : 27 km  (src: astorb)
 Speed of the shadow       : 11.2 km/s
 Elongation to Moon & Sun  : 125° (sunlit = 6%), Sun = 152°
 Cross-track uncertainty   : 1.1 mas = 1 km = 0.07 path-width (1-sig)
 RUWE and duplicate source : 1.06 mas, dup.src = 0  (0:false, 1:true)

 Ephemeris Reference       : JPL#54

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

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