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2024-11-02 / UCAC4 535-020708 / (2382) Nonie

#OBSObserverOccMeth.Instr.CC TSRCUT1UT2UT3UT4UT2EUT3EDur.Chrd
1 show Matthieu Conjat O+ VID L500 FR GPS 02:28:16 02:28:50.26 02:28:50.87 02:29:14 0.03 0.03 0.61 7.9
UT1/UT4: Begin/End of observation | UT2/UT3: Begin/End of occultation | Dur: Reported duration in seconds | Chrd: Corresponding chord length in km | More

1 observation found in db: sodis

Available (probably) matching predictions (click on the link to switch):

JPL#70 : 9dba3290-ddb5-11f0-547e-5ff8f65e30a8 [db: observed]
Using prediction 9dba3290-ddb5-11f0-547e-5ff8f65e30a8 for map and profile fit
Get observations as KML file (reduced site location resolution)

Sky projection (artificial light) for occ. time: 2024-11-02, 02:28 UT (JD = 2460616.603)

DAMITQP (h)λ, βJD0JD-JD0φ0VersionModifiedVol-equiv DCmnt
# 1114None15.112 205°, 52° 2.446509e614107.60.0° NoneNone not scaled 2016-01-04
Q: model quality flag (0-5, 5=highest) | P: rotation period | λ,β: ecl. lon. and lat. of spin axis (J2000) | JD: initial time (epoch) | φ0: initial rotation angle for JD0

 
Image size: 300px. Transparent image background for copy & paste

Map with groundtrack and observer stations
Event Details
Occultation UUID [and DB] : 9dba3290-ddb5-11f0-547e-5ff8f65e30a8 [observed] Occultation Date + Time : 2024-11-02 at 02:31:32 UT +/- 0.0 min [1] Object Designation : (2382) Nonie Orbit Class : MBA Star Designation : GDR3 3349692719827047040 Star Coordinates (ICRF) : RA = 05 54 21.0895, DE = +16 54 54.433 [2] Star Magnitudes : G = 12.1 mag, RP = 11.68 mag, BP = 12.35 mag Object Magnitude : V = 16.88 mag Estimated Magnitude Drop : 4.8 mag Estimated Max. Duration : 1.1 sec Object Mean Diameter : 14.1 km (src: astorb) Speed of the shadow : 12.9 km/s Elongation to Moon & Sun : 137° (sunlit = 0%), Sun = 131° Cross-track uncertainty : 0.5 mas = 0 km = 0.06 path-width (1-sig) RUWE and duplicate source : 2.65 mas, dup.src = 0 (0:false, 1:true) Ephemeris Reference : JPL#70 Note : FP:true [1] time t0 of closest geocentric approach c/a, [2] including proper motion until t0

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