2020-11-04 / 4UC 557-034202 / (971) Alsatia
# | OBS | Observer | Occ | Meth. | Instr. | CC | TSRC | UT1 | UT2 | UT3 | UT4 | UT2E | UT3E | Dur. | Chrd |
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1 | show | Peter Tickner | O+ | CCD | M356 | UK | GPS | 00:34:27 | 00:37:13.90 | 00:37:25.11 | 00:40:27 | 0.55 | 0.25 | 11.21 | 69.5 |
2 | show | Simon Kidd | O+ | CCD | M350 | UK | GPS++ | 00:36:30 | 00:37:24.43 | 00:37:31.70 | 00:38:45 | 0.19 | 0.22 | 7.27 | 45.1 |
3 | show | Pierre Le Cam | O- | CCD | M250 | FR | 00:34:10 | 00:38:10 | |||||||
4 | show | John Talbot | O- | VID | M303 | UK | 00:36:31 | 00:38:28 | |||||||
5 | show | Tim Haymes | O- | CCD | M279 | UK | 00:34:00 | 00:41:00 |
5 observations found in db: euraster
Available (probably) matching predictions (click on the link to switch):JPL#63 : b5576832-6a9a-407d-846e-6bbd12f4fdfd [db: observed] |
Using prediction b5576832-6a9a-407d-846e-6bbd12f4fdfd for map and profile fit
Ellipse and circular profile fits to the timings (chords) |
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Auto-Fit Result: X0,Y0 = 3280.7, 50.9 km Circular diameter = 72 km From 2 chords (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. |
Map with groundtrack and observer stations |
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Event Details |
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Occultation UUID [and DB] : b5576832-6a9a-407d-846e-6bbd12f4fdfd [observed] Occultation Date + Time : 2020-11-04 at 00:36:29 UT +/- 0.03 min [1] Object Designation : (971) Alsatia Orbit Class : MBA Star Designation : GDR3 3378344072999467776 Star Coordinates (ICRF) : RA = 06 50 18.6917, DE = +21 19 23.017 [2] Star Magnitudes : G = 14.19 mag, RP = 13.44 mag, BP = 14.78 mag Object Magnitude : V = 13.87 mag Estimated Magnitude Drop : 0.6 mag Estimated Max. Duration : 10.4 sec Object Mean Diameter : 64 km (src: astorb) Speed of the shadow : 6.2 km/s Elongation to Moon & Sun : 22° (sunlit = 90%), Sun = 120° Cross-track uncertainty : 1.7 mas = 1 km = 0.03 path-width (1-sig) RUWE and duplicate source : 4.75 mas, dup.src = 0 (0:false, 1:true) Ephemeris Reference : JPL#63 [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) |