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2011-11-22 / 2UC 42217550 / (22) Kalliope

#OBSObserverOccMeth.Instr.CC TSRCUT1UT2UT3UT4UT2EUT3EDur.Chrd
1 show Michael Parl O+ VID M203 DE RAD+ 02:37:00 02:42:10.31 02:42:26.55 02:47:00 0.12 0.12 16.24 133.2
2 show Oliver Kloes O+ VID M254 DE GPS++ 02:38:01 02:42:53.97 02:43:04.67 02:46:00 0.02 0.02 10.70 87.7
3 show Josef Mueller O+ VID M300 DE GPS++ 02:42:00 02:42:58.61 02:43:11.22 02:44:00 0.05 0.05 12.61 103.4
4 show Bernd Brinkmann O+ VID L30 DE GPS++ 02:41:58 02:43:09.8 02:43:16.3 02:45:00 0.2 0.2 6.50 53.3
5 show Pietro Baruffetti O- VID M200 IT 02:41:27 02:42:30
6 show Bernard Tregon O- VID M200 FR 02:38:42 02:49:52
7 show Eric Barbotin O- CCD M225 FR 02:39:09 02:47:30
8 show Stefano Sposetti O- VID M400 CH 02:35:40 02:51:15
9 show GB Casalnuovo et al O- VID M300 IT 02:40:00 02:44:00
10 show Maurice Audejean O- CCD M320 FR 02:39:05 02:49:05
11 show J. Berthier et al O- VID M180 FR 02:35:00 02:54:00
12 show Rolf Apitzsch O- VID M355 DE 02:42:15 02:42:56
13 show Otto Farago O- VID M406 DE 02:40:30 02:44:30
14 show F. Van Den Abbeel O- CCD M200 BE 02:41:01 02:45:01
15 show R. Decellier/G. Huys O- VIS M300 BE 02:39:15 02:47:04
16 show Rene Bourtembourg O- VIS M254 BE 02:42:00 02:46:00
17 show A. Tudorica et al O- CCD M500 DE 02:30:00 02:50:00
18 show Harrie Rutten O- VID M356 NL 02:41:00 02:46:30
UT1/UT4: Begin/End of observation | UT2/UT3: Begin/End of occultation | Dur: Reported duration in seconds | Chrd: Corresponding chord length in km | More

18 observations found in db: euraster

Available (probably) matching predictions (click on the link to switch):
JPL#122 : 7e7d7b51-5dc9-4554-88a6-ef02a49a2845 [db: observed]

Using prediction 7e7d7b51-5dc9-4554-88a6-ef02a49a2845 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 = 191 x 125 km
a',b' = 95.3, 62.7 km
X0,Y0 = -1616.6, 27.5 km
Mean diameter = 155 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).
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.

Check Johnston Archive for satellites.

Sky projection (artificial light) for occ. time: 2011-11-22, 02:42 UT (JD = 2455887.613)

DAMITQP (h)λ, βJD0JD-JD0φ0VersionModifiedVol-equiv DCmnt
# 121None4.148 196°, 3° 2.436258e619629.60.0° None2011-04-11 143.0 +/- 10.0 km 2011-03-28
# 18274.04.148 196°, 2° 2.436258e619629.60.0° None2017-06-19 157.0 +/- 6.0 km 2017-06-06
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] : 7e7d7b51-5dc9-4554-88a6-ef02a49a2845 [observed]

 Occultation Date + Time   : 2011-11-22 at 02:40:31 UT +/- 0.02 min  [1]
 Object Designation        : (22) Kalliope
 Orbit Class               : MBA
 Star Designation          : GDR3 3434486442383195392
 Star Coordinates (ICRF)   : RA = 06 35 03.4633, DE = +29 35 09.726  [2]
 Star Magnitudes           : G = 10.83 mag, RP = 10.02 mag, BP = 11.54 mag
 Object Magnitude          : V = 10.9 mag
 Estimated Magnitude Drop  : 0.8 mag
 Estimated Max. Duration   : 22.0 sec
 Object Mean Diameter      : 181 km  (src: astorb)
 Speed of the shadow       : 8.2 km/s
 Elongation to Moon & Sun  : 98° (sunlit = 14%), Sun = 141°
 Cross-track uncertainty   : 2.0 mas = 2 km = 0.01 path-width (1-sig)
 RUWE and duplicate source : 0.92 mas, dup.src = 0  (0:false, 1:true)

 Ephemeris Reference       : JPL#122

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

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