2024-12-29 / UCAC4 589-021820 / (2509) Chukotka
| # | OBS | Observer | Occ | Meth. | Instr. | CC | TSRC | UT1 | UT2 | UT3 | UT4 | UT2E | UT3E | Dur. | Chrd |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| 1 | show | Carles Schnabel | O+ | VID | M400 | ES | GPS | 02:19:27 | 02:21:26.25 | 02:21:27.8 | 02:23:14 | 0.16 | 0.2 | 1.55 | 18.8 |
| 2 | show | Antoni Selva, Carlos Perello | O+ | VID | M500 | ES | GPS | 02:20:26 | 02:21:25.560 | 02:21:27.170 | 02:22:26 | 0.10 | 0.10 | 1.61 | 19.5 |
2 observations found in db: sodis
Available (probably) matching predictions (click on the link to switch):| JPL#67 : 64154c80-ddb2-11f0-547e-2b571feeadfd [db: observed] |
| JPL#67 : 64157390-ddb2-11f0-547e-5096fbe914e6 [db: observed] |
Using prediction 64157390-ddb2-11f0-547e-5096fbe914e6 for map and profile fit
| Ellipse and circular profile fits to the timings (chords) |
|---|
|
|
Auto-Fit Result: X0,Y0 = -5242.8, 7689.1 km Circular diameter = 22 km From 2 chords (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 |
|---|
| Event Details |
|---|
Occultation UUID [and DB] : 64157390-ddb2-11f0-547e-5096fbe914e6 [observed] Occultation Date + Time : 2024-12-29 at 02:19:06 UT +/- 0.0 min [1] Object Designation : (2509) Chukotka Orbit Class : MBA Star Designation : GDR3 3443030919042501888 Star Coordinates (ICRF) : RA = 05 49 05.9496, DE = +27 44 45.315 [2] Star Magnitudes : G = 12.51 mag, RP = 11.56 mag, BP = 13.42 mag Object Magnitude : V = 16.48 mag Estimated Magnitude Drop : 4.0 mag Estimated Max. Duration : 0.7 sec Object Mean Diameter : 8.8 km (src: astorb) Speed of the shadow : 12.1 km/s Elongation to Moon & Sun : 168° (sunlit = 4%), Sun = 169° Cross-track uncertainty : 0.3 mas = 0 km = 0.04 path-width (1-sig) RUWE and duplicate source : 1.03 mas, dup.src = 0 (0:false, 1:true) Ephemeris Reference : JPL#67 Note : FP:true [1] time t0 of closest geocentric approach c/a, [2] including proper motion until t0 |
| More Data and Informations |
|---|
(If error 404: link not valid which means no data available)
| Aladin Sky Atlas |
|---|
| Aladin Lite direct link (has Gaia overlay) |