2024-12-31 / UCAC4 453-000016 / (137) Meliboea
| # | OBS | Observer | Occ | Meth. | Instr. | CC | TSRC | UT1 | UT2 | UT3 | UT4 | UT2E | UT3E | Dur. | Chrd |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| 1 | show | Alberto Ossola | O+ | VID | M230 | CH | GPS | 18:10:13 | 18:11:49.65 | 18:11:55.41 | 18:13:00 | 0.32 | 0.32 | 5.76 | 136.5 |
| 2 | show | Andrea Manna | O+ | VID | M200 | CH | GPS | 18:09:05 | 18:11:49.84 | 18:11:54.68 | 18:14:53 | 0.08 | 0.12 | 4.84 | 114.7 |
| 3 | show | Stefano Sposetti | O+ | VID | M420 | CH | GPS | 18:09:00 | 18:11:50.205 | 18:11:54.912 | 18:15:00 | 0.051 | 0.051 | 4.71 | 111.6 |
3 observations found in db: sodis
Available (probably) matching predictions (click on the link to switch):| JPL#145 : e525e390-ddb5-11f0-547e-6c88a5bf501a [db: observed] |
Using prediction e525e390-ddb5-11f0-547e-6c88a5bf501a for map and profile fit
| Ellipse and circular profile fits to the timings (chords) |
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Auto-Fit Result: Ellipse profile fit was not successful. Trying circular fit. Circular diameter = 155 km From 3 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 |
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| Event Details |
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Occultation UUID [and DB] : e525e390-ddb5-11f0-547e-6c88a5bf501a [observed] Occultation Date + Time : 2024-12-31 at 18:10:00 UT +/- 0.0 min [1] Object Designation : (137) Meliboea Orbit Class : MBA Star Designation : GDR3 2738218195832102016 Star Coordinates (ICRF) : RA = 00 00 29.0028, DE = +00 27 33.608 [2] Star Magnitudes : G = 13.25 mag, RP = 12.59 mag, BP = 13.76 mag Object Magnitude : V = 13.84 mag Estimated Magnitude Drop : 1.1 mag Estimated Max. Duration : 6.1 sec Object Mean Diameter : 145.4 km (src: astorb) Speed of the shadow : 23.7 km/s Elongation to Moon & Sun : 70° (sunlit = 1%), Sun = 80° Cross-track uncertainty : 0.7 mas = 1 km = 0.01 path-width (1-sig) RUWE and duplicate source : 1.01 mas, dup.src = 0 (0:false, 1:true) Ephemeris Reference : JPL#145 Note : FP:true [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) |