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2006-10-08 / TYC 1722-00810-1 / (409) Aspasia

#OBSObserverOccMeth.Instr.CC TSRCUT1UT2UT3UT4UT2EUT3EDur.Chrd
1 show G. Busi/C. Frisoni O+ VID M400 IT RAD++ 21:24:00 21:24:54.52 21:25:00.28 21:30:00 0.24 0.24 5.76 69.7
2 show Roberto Di Luca O+ VID M250 IT RAD++ 21:20:00 21:24:48.92 21:25:00.84 21:30:00 0.04 0.04 11.92 144.2
3 show Paolo Corelli O+ CCD M450 IT NTP 21:24:15 21:24:32.80 21:24:41.95 21:25:15 0.3 0.3 9.15 110.7
4 show Bernd Gaehrken O+ VID L120 AT RAD 21:24:20 21:24:21.40 21:24:36.12 21:28:00 14.72 178.1
5 show Michael Schmid O+ VID L300 AT RAD 21:20:00 21:24:07.88 21:24:14.84 21:25:10 0.15 0.10 6.96 84.2
6 show Gerhard Dangl O+ VID M254 AT GPS++ 21:20:50 21:24:06.10 21:24:20.94 21:27:41 0.01 0.01 14.84 179.6
7 show Ladislav Smelcer O+ CCD M280 CZ RAD 21:23:52.8 21:24:01.5 1.0 1.0 8.70 105.3
8 show E. Frappa/A. Klotz O- CCD M250 FR 21:24:28 21:27:35
9 show Andrea Manna O- VIS M300 CH 21:18:00 21:40:00
10 show Stefano Sposetti O- CCD M400 CH 21:21:30 21:28:30
11 show Wieslaw Slotwinski O- VIS M200 PL 21:18:00 21:30:00
12 show Libor Smid O- VID M355 CZ 21:21:00 21:26:00
13 show Otta Sandor O- VIS M200 CZ 21:21:02 21:29:22
14 show Tomas Janik O- VIS M200 CZ 21:23:32 21:24:31
15 show Jerzy Speil O- VIS M250 PL 21:21:30 21:26:30
UT1/UT4: Begin/End of observation | UT2/UT3: Begin/End of occultation | Dur: Reported duration in seconds | Chrd: Corresponding chord length in km | More

15 observations found in db: euraster

Available (probably) matching predictions (click on the link to switch):
JPL#124 : ff9ef757-db82-402d-bd94-a792ae0c509f [db: observed]

Using prediction ff9ef757-db82-402d-bd94-a792ae0c509f 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 = 183 x 167 km
a',b' = 91.7, 83.3 km
X0,Y0 = 1871.1, 26.0 km
Mean diameter = 175 km

From 7 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).

Check SiMDA for size and mass data.

Check Johnston Archive for satellites.

Sky projection (artificial light) for occ. time: 2006-10-08, 21:23 UT (JD = 2454017.391)

DAMITQP (h)λ, βJD0JD-JD0φ0VersionModifiedVol-equiv DCmnt
# 215None9.021 3°, 30° 2.44431e69707.40.0° None2011-04-11 173.0 +/- 17.0 km 2011-03-28
# 7154.09.021 4°, 29° 2.44431e69707.40.0° None2017-06-19 164.0 +/- 3.0 km 2017-06-19
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] : ff9ef757-db82-402d-bd94-a792ae0c509f [observed]

 Occultation Date + Time   : 2006-10-08 at 21:26:56 UT +/- 0.02 min  [1]
 Object Designation        : (409) Aspasia
 Orbit Class               : MBA
 Star Designation          : GDR3 2770755012641480448
 Star Coordinates (ICRF)   : RA = 23 55 16.8632, DE = +15 03 50.495  [2]
 Star Magnitudes           : G = 10.49 mag, RP = 9.97 mag, BP = 10.84 mag
 Object Magnitude          : V = 11.45 mag
 Estimated Magnitude Drop  : 1.3 mag
 Estimated Max. Duration   : 13.4 sec
 Object Mean Diameter      : 162 km  (src: astorb)
 Speed of the shadow       : 12.1 km/s
 Elongation to Moon & Sun  : 36° (sunlit = 95%), Sun = 162°
 Cross-track uncertainty   : 2.7 mas = 3 km = 0.02 path-width (1-sig)
 RUWE and duplicate source : 1.13 mas, dup.src = 1  (0:false, 1:true)

 Ephemeris Reference       : JPL#124

 Object is a Gaia mass determination target !
[1] time t0 of closest geocentric approach c/a, [2] including proper motion until t0

More Data and Informations
SiMDA | 3D Asteroid Catalogue | Johnston Archive | Star at CDS (Vizier) | JPL Small-Body Node | Minor Planet Center | Wikipedia
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