2024-08-16 / UCAC4 419-139877 / (1760) Sandra
# | OBS | Observer | Occ | Meth. | Instr. | CC | TSRC | UT1 | UT2 | UT3 | UT4 | UT2E | UT3E | Dur. | Chrd |
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1 | show | Oscar Canales | O+ | CCD | M280 | ES | NTP | 22:13:26 | 22:16:26.34 | 22:16:30.00 | 22:19:26 | 0.45 | 0.45 | 3.66 | 44.3 |
2 | show | Daniel Blazewicz | O+ | VID | M350 | PL | GPS | 22:12:25 | 22:14:07.45 | 22:14:09.38 | 22:16:09 | 0.18 | 0.18 | 1.93 | 23.4 |
3 | show | Leszek Benedyktowicz | O+ | VID | M200 | PL | GPS | 22:11:07 | 22:14:09.100 | 22:14:13.100 | 22:16:16 | 0.40 | 0.40 | 4.00 | 48.4 |
3 observations found in db: sodis
Available (probably) matching predictions (click on the link to switch):JPL#71 : eb671270-c352-11ef-5276-0b38bdf959d3 [db: observed] |
JPL#69 : 2d5f6950-8791-11ef-78cd-40053f7a5844 [db: asteroids] |
Using prediction eb671270-c352-11ef-5276-0b38bdf959d3 for map and profile fit
Ellipse and circular profile fits to the timings (chords) |
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Auto-Fit Result: Size = 56 x 24 km a',b' = 28.2, 11.8 km X0,Y0 = 1591.8, 28.4 km Mean diameter = 36 km From 3 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. |
Map with groundtrack and observer stations |
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Event Details |
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Occultation UUID [and DB] : eb671270-c352-11ef-5276-0b38bdf959d3 [observed] Occultation Date + Time : 2024-08-16 at 22:17:37 UT +/- 0.0 min [1] Object Designation : (1760) Sandra Orbit Class : MBA Star Designation : GDR3 6908248569683442176 Star Coordinates (ICRF) : RA = 20 34 32.6436, DE = -06 19 38.724 [2] Star Magnitudes : G = 14.98 mag, RP = 14.46 mag, BP = 15.33 mag Object Magnitude : V = 15.98 mag Estimated Magnitude Drop : 1.4 mag Estimated Max. Duration : 3.0 sec Object Mean Diameter : 35.9 km (src: astorb) Speed of the shadow : 12.1 km/s Elongation to Moon & Sun : 29° (sunlit = 89%), Sun = 161° Cross-track uncertainty : 0.4 mas = 0 km = 0.02 path-width (1-sig) RUWE and duplicate source : 0.96 mas, dup.src = 0 (0:false, 1:true) Ephemeris Reference : JPL#71 [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) |