2024-07-17 / UCAC4 405-108887 / (35420) 1998 AG6
# | OBS | Observer | Occ | Meth. | Instr. | CC | TSRC | UT1 | UT2 | UT3 | UT4 | UT2E | UT3E | Dur. | Chrd |
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1 | show | Daniel Blazewicz | O+ | VID | M350 | PL | GPS | 01:36:44 | 01:37:24.84 | 01:37:25.09 | 01:38:27 | 0.03 | 0.02 | 0.25 | 3.0 |
2 | show | Anna Marciniak, Bartosz Ziolkowski, +1 | O+ | CCD | M400 | PL | GPS | 01:36:19 | 01:37:23.060 | 01:37:23.170 | 01:37:57 | 0.06 | 0.06 | 0.11 | 1.3 |
3 | show | Rui Goncalves | O- | VID | M256 | PT | GPS | 01:37:04 | 01:41:02 | ||||||
4 | show | Lionel Rousselot | O- | VID | M200 | FR | GPS | 01:36:32 | 01:39:32 |
4 observations found in db: sodis
Available (probably) matching predictions (click on the link to switch):JPL#51 : 1786cb70-c34e-11ef-5276-1462f7df56e4 [db: observed] |
Using prediction 1786cb70-c34e-11ef-5276-1462f7df56e4 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] : 1786cb70-c34e-11ef-5276-1462f7df56e4 [observed] Occultation Date + Time : 2024-07-17 at 01:43:32 UT +/- 0.0 min [1] Object Designation : (35420) 1998 AG6 Orbit Class : MBA Star Designation : GDR3 4204153068710661760 Star Coordinates (ICRF) : RA = 19 09 02.1590, DE = -09 02 52.005 [2] Star Magnitudes : G = 11.71 mag, RP = 10.54 mag, BP = 13.17 mag Object Magnitude : V = 17.89 mag Estimated Magnitude Drop : 6.2 mag Estimated Max. Duration : 0.5 sec Object Mean Diameter : 6 km (src: astorb) Speed of the shadow : 12.2 km/s Elongation to Moon & Sun : 50° (sunlit = 79%), Sun = 165° Cross-track uncertainty : 0.2 mas = 0 km = 0.05 path-width (1-sig) RUWE and duplicate source : 1.15 mas, dup.src = 0 (0:false, 1:true) Ephemeris Reference : JPL#51 [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) |