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2017-10-08 / TYC 5632-00827-1 / (173) Ino

#OBSObserverOccMeth.Instr.CC TSRCUT1UT2UT3UT4UT2EUT3EDur.Chrd
1 show Carlo Gualdoni O+ VID M250 IT GPS++ 18:27:00 18:27:23.43 18:27:27.71 18:28:00 0.20 0.08 4.28 144.7
2 show Alberto Ossola O+ VID M230 CH GPS++ 18:25:27 18:27:22.68 18:27:27.09 18:28:25 0.17 0.17 4.41 149.1
3 show Stefano Sposetti O+ VID M200 CH GPS++ 18:21:36 18:27:22.09 18:27:26.45 18:31:10 0.02 0.02 4.36 147.4
4 show Andrea Manna O+ VID M200 CH GPS++ 18:26:48 18:27:22.38 18:27:26.54 18:28:23 0.16 0.16 4.16 140.6
5 show Dariusz Miller O- VIS M202 PL 18:27:20 18:28:00
UT1/UT4: Begin/End of observation | UT2/UT3: Begin/End of occultation | Dur: Reported duration in seconds | Chrd: Corresponding chord length in km | More

5 observations found in db: euraster

Available (probably) matching predictions (click on the link to switch):
JPL#121 : 2552c6de-b7ed-4c35-be73-cde8cfc15630 [db: observed]

Using prediction 2552c6de-b7ed-4c35-be73-cde8cfc15630 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 = 152 x 44 km
a',b' = 76.1, 21.8 km
X0,Y0 = -1778.5, 28.5 km
Mean diameter = 81 km

From 4 chords (VID)








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).
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Map with groundtrack and observer stations

Event Details
 Occultation UUID [and DB] : 2552c6de-b7ed-4c35-be73-cde8cfc15630 [observed]

 Occultation Date + Time   : 2017-10-08 at 18:26:28 UT +/- 0.0 min  [1]
 Object Designation        : (173) Ino
 Orbit Class               : MBA
 Star Designation          : GDR3 4331316879834142208
 Star Coordinates (ICRF)   : RA = 16 35 54.2617, DE = -11 05 04.952  [2]
 Star Magnitudes           : G = 10.8 mag, RP = 10.1 mag, BP = 11.32 mag
 Object Magnitude          : V = 13.93 mag
 Estimated Magnitude Drop  : 3.2 mag
 Estimated Max. Duration   : 4.6 sec
 Object Mean Diameter      : 154 km  (src: astorb)
 Speed of the shadow       : 33.8 km/s
 Elongation to Moon & Sun  : 166° (sunlit = 88%), Sun = 54°
 Cross-track uncertainty   : 1.0 mas = 2 km = 0.02 path-width (1-sig)
 RUWE and duplicate source : 1.75 mas, dup.src = 1  (0:false, 1:true)

 Ephemeris Reference       : JPL#121

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

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