Collaborative Occultation Resources and Archive (CORA)


Occultations | Observations | Reports | Info + Credits | JOA | Admin | Login

2023-09-25 / UCAC4 553-005449 / (595) Polyxena

#OBSObserverOccMeth.Instr.CC TSRCUT1UT2UT3UT4UT2EUT3EDur.Chrd
1 show Jean-Francois Pittet O+ VID M254 DE GPS 19:24:34 19:25:59.92 19:26:04.80 19:27:32 0.13 0.15 4.88 43.4
2 show Andreas Tazreiter O+ CCD L180 AT GPS 19:23:17 19:25:55.7 19:26:06.3 19:31:17 0.9 1.0 10.60 94.3
3 show Marian Urbanik O+ VID T400 SK GPS 19:24:12 19:25:42.4 19:25:55.21 19:27:11 0.3 0.17 12.81 114.0
UT1/UT4: Begin/End of observation | UT2/UT3: Begin/End of occultation | Dur: Reported duration in seconds | Chrd: Corresponding chord length in km | More

3 observations found in db: sodis

Available (probably) matching predictions (click on the link to switch):
JPL#104 : b68f1d63-9f28-403b-8ec1-60ed87b30c8e [db: observed]

Using prediction b68f1d63-9f28-403b-8ec1-60ed87b30c8e 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 = 132 x 85 km
a',b' = 66.1, 42.5 km
X0,Y0 = -973.4, 34.2 km
Mean diameter = 106 km

From 3 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: 2023-09-25, 19:25 UT (JD = 2460213.309)

DAMITQP (h)λ, βJD0JD-JD0φ0VersionModifiedVol-equiv DCmnt
# 228None11.794 42°, 8° 2.449187e611026.30.0° preliminary model, agrees well with occultation data http://www.asteroidoccultation.com/observations/Results/Data2015/20150415_PolyxenaProfileDAMIT228.gif2015-08-25 not scaled 2008-09-16
# 229None11.794 222°, -4° 2.449187e611026.30.0° preliminary model, probably wrong pole solution, does not agree with occultation data http://www.asteroidoccultation.com/observations/Results/2015-08-25 not scaled 2008-09-16
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] : b68f1d63-9f28-403b-8ec1-60ed87b30c8e [observed]

 Occultation Date + Time   : 2023-09-25 at 19:15:06 UT +/- 0.06 min  [1]
 Object Designation        : (595) Polyxena
 Orbit Class               : MBA
 Star Designation          : GDR3 0085138002837333504
 Star Coordinates (ICRF)   : RA = 02 48 51.4436, DE = +20 29 03.701  [2]
 Star Magnitudes           : G = 12.25 mag, RP = 11.75 mag, BP = 12.59 mag
 Object Magnitude          : V = 13.18 mag
 Estimated Magnitude Drop  : 1.3 mag
 Estimated Max. Duration   : 12.2 sec
 Object Mean Diameter      : 109 km  (src: astorb)
 Speed of the shadow       : 8.9 km/s
 Elongation to Moon & Sun  : 94° (sunlit = 82%), Sun = 136°
 Cross-track uncertainty   : 10.7 mas = 18 km = 0.17 path-width (1-sig)
 RUWE and duplicate source : 1.18 mas, dup.src = 0  (0:false, 1:true)

 Ephemeris Reference       : JPL#104

 
 [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
(If error 404: link not valid which means no data available)

Aladin Sky Atlas
Aladin Lite direct link (has Gaia overlay)