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2023-05-08 / UCAC4 619-035010 / (117) Lomia

#OBSObserverOccMeth.Instr.CC TSRCUT1UT2UT3UT4UT2EUT3EDur.Chrd
1 show Daniel Blazewicz O+ CCD M350 PL GPS 21:20:54 21:21:42.66 21:21:47.36 21:23:53 0.15 0.15 4.70 168.7
2 show Leszek Benedyktowicz O+ VID M200 PL GPS 21:20:31 21:21:43.3 21:21:47.5 21:22:43 0.3 0.3 4.20 150.8
3 show Marcin Filipek O+ VID M250 PL GPS 21:21:01 21:21:42.590 21:21:47.290 21:22:30 0.1 0.1 4.70 168.7
4 show Marek Zawilski, Mieczyslaw Borkowski O+ VID M200 PL GPS 21:21:09 21:21:38.4 21:21:43.3 21:22:25 0.20 0.20 4.90 175.9
5 show Daniel Antuszewicz O+ VID M203 PL NTP 21:20:44 21:21:36.96 21:21:40.20 21:22:41 0.20 0.20 3.24 116.3
6 show Petr Zeleny O- VID M250 CZ GPS 21:19:00 21:25:00
7 show Anna Marciniak O- CCD M350 PL GPS 21:20:30 21:22:58
UT1/UT4: Begin/End of observation | UT2/UT3: Begin/End of occultation | Dur: Reported duration in seconds | Chrd: Corresponding chord length in km | More

7 observations found in db: sodis

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

JPL#141 : 970c5e20-ddb3-11f0-547e-3f28dededba8 [db: observed]
Using prediction 970c5e20-ddb3-11f0-547e-3f28dededba8 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 = 193 x 124 km
a',b' = 96.7, 62.1 km
X0,Y0 = -1197.7, 17.1 km
Mean diameter = 155 km

From 5 chords (CCD,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: 2023-05-08, 21:21 UT (JD = 2460073.390)

DAMITQP (h)λ, βJD0JD-JD0φ0VersionModifiedVol-equiv DCmnt
# 838None9.124 117°, -19° 2.446333e613740.40.0° NoneNone not scaled 2016-01-04
# 839None9.124 323°, -57° 2.446333e613740.40.0° 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] : 970c5e20-ddb3-11f0-547e-3f28dededba8 [observed] Occultation Date + Time : 2023-05-08 at 21:20:27 UT +/- 0.0 min [1] Object Designation : (117) Lomia Orbit Class : MBA Star Designation : GDR3 0941398767623502336 Star Coordinates (ICRF) : RA = 06 36 04.4318, DE = +33 40 56.618 [2] Star Magnitudes : G = 13.91 mag, RP = 13.39 mag, BP = 14.26 mag Object Magnitude : V = 14.07 mag Estimated Magnitude Drop : 0.8 mag Estimated Max. Duration : 4.1 sec Object Mean Diameter : 148.7 km (src: astorb) Speed of the shadow : 35.9 km/s Elongation to Moon & Sun : 169° (sunlit = 88%), Sun = 50° Cross-track uncertainty : 0.7 mas = 1 km = 0.01 path-width (1-sig) RUWE and duplicate source : 1.2 mas, dup.src = 0 (0:false, 1:true) Ephemeris Reference : JPL#141 Note : FP:true [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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