2019-08-03 / 4UC 365-082756 / (415) Palatia
# | OBS | Observer | Occ | Meth. | Instr. | CC | TSRC | UT1 | UT2 | UT3 | UT4 | UT2E | UT3E | Dur. | Chrd |
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1 | show | Gregor Krannich | O+ | CCD | L72 | DE | GPS++ | 20:44:03 | 20:46:37.47 | 20:46:45.47 | 20:48:14 | 0.25 | 0.25 | 8.00 | 48.8 |
2 | show | Marek Zawilski | O+ | CCD | M203 | PL | NTP | 20:41:00 | 20:43:50.8 | 20:44:01.8 | 20:45:00 | 0.8 | 0.8 | 11.00 | 67.1 |
3 | show | Pietro Baruffetti | O- | VID | M300 | IT | 20:43:24 | 20:47:21 | |||||||
4 | show | Jiri Kubanek | O- | VID | M203 | CZ | 20:42:05 | 20:47:04 | |||||||
5 | show | Jiri Polak | O- | VID | M303 | CZ | 20:42:40 | 20:46:42 |
5 observations found in db: euraster
Available (probably) matching predictions (click on the link to switch):JPL#84 : f8ab38c5-8e0a-4259-b5a4-541d863191dd [db: observed] |
Using prediction f8ab38c5-8e0a-4259-b5a4-541d863191dd for map and profile fit
Ellipse and circular profile fits to the timings (chords) |
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Auto-Fit Result: Circular profile fit was not successful ... 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. |
Map with groundtrack and observer stations |
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Event Details |
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Occultation UUID [and DB] : f8ab38c5-8e0a-4259-b5a4-541d863191dd [observed] Occultation Date + Time : 2019-08-03 at 20:56:05 UT +/- 0.02 min [1] Object Designation : (415) Palatia Orbit Class : MBA Star Designation : GDR3 4135660022638645632 Star Coordinates (ICRF) : RA = 17 10 15.6461, DE = -17 01 16.317 [2] Star Magnitudes : G = 12.89 mag, RP = 12.34 mag, BP = 13.28 mag Object Magnitude : V = 15.17 mag Estimated Magnitude Drop : 2.4 mag Estimated Max. Duration : 12.5 sec Object Mean Diameter : 76 km (src: astorb) Speed of the shadow : 6.1 km/s Elongation to Moon & Sun : 88° (sunlit = 11%), Sun = 127° Cross-track uncertainty : 0.7 mas = 1 km = 0.02 path-width (1-sig) RUWE and duplicate source : 0.87 mas, dup.src = 0 (0:false, 1:true) Ephemeris Reference : JPL#84 [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) |