2025-02-02 / UCAC4 506-052374 / (672) Astarte
# | OBS | Observer | Occ | Meth. | Instr. | CC | TSRC | UT1 | UT2 | UT3 | UT4 | UT2E | UT3E | Dur. | Chrd |
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1 | show | Olivier Schreurs, Manon Lecossois, +1 | O+ | VID | M200 | BE | GPS | 21:31:48 | 21:32:48.55 | 21:32:50.29 | 21:33:49 | 0.04 | 0.04 | 1.74 | 18.6 |
2 | show | Konrad Guhl | O+ | CCD | L100 | DE | GPS | 21:31:26 | 21:32:17.523 | 21:32:20.375 | 21:33:18 | 0.127 | 0.127 | 2.85 | 30.5 |
3 | show | Peter Lindner | O+ | CCD | M300 | DE | GPS | 21:29:31 | 21:32:09.61 | 21:32:12.2 | 21:33:59 | 0.04 | 0.04 | 2.59 | 27.7 |
4 | show | Philip Denyer | O- | VID | M235 | GB | GPS | 21:30:49 | 21:33:51 |
4 observations found in db: sodis
Available (probably) matching predictions (click on the link to switch):JPL#63 : 787f6780-8617-11ef-78cd-ee02efedb301 [db: asteroids] |
Using prediction 787f6780-8617-11ef-78cd-ee02efedb301 for map and profile fit
Ellipse and circular profile fits to the timings (chords) |
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Auto-Fit Result: Size = 35 x 16 km a',b' = 17.7, 8.0 km X0,Y0 = -653.5, 9.1 km Mean diameter = 24 km From 3 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. |
Map with groundtrack and observer stations |
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Event Details |
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Occultation UUID [and DB] : 787f6780-8617-11ef-78cd-ee02efedb301 [asteroids] Occultation Date + Time : 2025-02-02 at 21:26:10 UT +/- 0.0 min [1] Object Designation : (672) Astarte Orbit Class : MBA Star Designation : GDR3 3871270116575081728 Star Coordinates (ICRF) : RA = 10 52 59.2791, DE = +11 00 05.926 [2] Star Magnitudes : G = 11.42 mag, RP = 10.77 mag, BP = 11.92 mag Object Magnitude : V = 15.86 mag Estimated Magnitude Drop : 4.5 mag Estimated Max. Duration : 3.3 sec Object Mean Diameter : 34.8 km (src: astorb) Speed of the shadow : 10.7 km/s Elongation to Moon & Sun : 148° (sunlit = 23%), Sun = 154° Cross-track uncertainty : 0.7 mas = 0 km = 0.03 path-width (1-sig) RUWE and duplicate source : 0.93 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) |