2022-03-24 / 4UC 454-033141 / (439) Ohio
# | OBS | Observer | Occ | Meth. | Instr. | CC | TSRC | UT1 | UT2 | UT3 | UT4 | UT2E | UT3E | Dur. | Chrd |
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1 | show | Jerome Delpau | O+ | CCD | L125 | FR | NTP | 22:18:01 | 22:20:13.04 | 22:20:17.74 | 22:22:02 | 0.58 | 0.58 | 4.70 | 59.2 |
2 | show | R. Boninsegna et al | O+ | VID | M305 | BE | GPS++ | 22:18:58 | 22:20:25.97 | 22:20:31.33 | 22:21:56 | 0.08 | 0.08 | 5.36 | 67.5 |
3 | show | Benoit Goffin | O+ | CCD | M250 | BE | GPS++ | 22:16:35 | 22:20:27.23 | 22:20:32.22 | 22:23:33 | 0.09 | 0.09 | 4.99 | 62.9 |
4 | show | Olivier Schreurs | O+ | VID | M406 | BE | GPS++ | 22:19:30 | 22:20:28.88 | 22:20:33.64 | 22:21:31 | 0.04 | 0.04 | 4.76 | 60.0 |
5 | show | Sven Andersson | O+ | CCD | M355 | DE | GPS++ | 22:20:01 | 22:20:45.71 | 22:20:51.11 | 22:21:31 | 0.33 | 0.33 | 5.40 | 68.0 |
6 | show | Konrad Guhl | O+ | CCD | M500 | DE | GPS++ | 22:20:00 | 22:20:45.51 | 22:20:50.76 | 22:21:05 | 0.13 | 0.13 | 5.25 | 66.1 |
7 | show | Olaf Hofschulz | O+ | CCD | L140 | DE | GPS+ | 22:19:38 | 22:20:45.93 | 22:20:51.18 | 22:23:00 | 0.75 | 0.50 | 5.25 | 66.1 |
8 | show | Maciej Borkowski | O+ | VID | M300 | PL | GPS++ | 22:19:01 | 22:21:00.23 | 22:21:02.55 | 22:23:01 | 0.08 | 0.08 | 2.32 | 29.2 |
9 | show | Anna Marciniak | O? | CCD | M350 | PL | GPS+ | 22:19:41 | 22:20:51.52 | 22:20:52.61 | 22:21:58 | 0.25 | 0.25 | 1.09 | 13.7 |
9 observations found in db: euraster
Available (probably) matching predictions (click on the link to switch):JPL#103 : d1997854-3672-4d7c-a3ca-1765a5e90e43 [db: observed] |
Using prediction d1997854-3672-4d7c-a3ca-1765a5e90e43 for map and profile fit
Ellipse and circular profile fits to the timings (chords) |
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Auto-Fit Result: Size = 84 x 64 km a',b' = 41.8, 31.8 km X0,Y0 = 819.7, 20.2 km Mean diameter = 73 km From 9 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: 2022-03-24, 22:19 UT (JD = 2459663.430)
DAMIT | Q | P (h) | λ, β | JD0 | JD-JD0 | φ0 | Version | Modified | Vol-equiv D | Cmnt |
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# 2253 | 1.5 | 37.467 | 39°, -54° | 2.451054e6 | 8609.4 | 0.0° | None | 2018-07-19 | not scaled | 2018-07-18 |
# 2254 | 1.5 | 37.468 | 260°, -30° | 2.451054e6 | 8609.4 | 0.0° | None | 2018-07-19 | not scaled | 2018-07-18 |
Image size: 300px. Transparent image background for copy & paste
Map with groundtrack and observer stations |
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Event Details |
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Occultation UUID [and DB] : d1997854-3672-4d7c-a3ca-1765a5e90e43 [observed] Occultation Date + Time : 2022-03-24 at 22:12:52 UT +/- 0.02 min [1] Object Designation : (439) Ohio Orbit Class : MBA Star Designation : GDR3 3111485969510691968 Star Coordinates (ICRF) : RA = 07 20 07.8451, DE = +00 36 14.912 [2] Star Magnitudes : G = 12.58 mag, RP = 12.15 mag, BP = 12.85 mag Object Magnitude : V = 15.21 mag Estimated Magnitude Drop : 2.7 mag Estimated Max. Duration : 6.1 sec Object Mean Diameter : 77 km (src: astorb) Speed of the shadow : 12.6 km/s Elongation to Moon & Sun : 148° (sunlit = 54%), Sun = 106° Cross-track uncertainty : 1.3 mas = 2 km = 0.03 path-width (1-sig) RUWE and duplicate source : 1.02 mas, dup.src = 0 (0:false, 1:true) Ephemeris Reference : JPL#103 [1] time t0 of closest geocentric approach c/a, [2] including proper motion until t0 |
More Data and Informations |
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(If error 404: link not valid which means no data available)
Aladin Sky Atlas |
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Aladin Lite direct link (has Gaia overlay) |