2026-09-22 / UCAC4 399-071546 / (216) Kleopatra
| # | OBS | Observer | Occ | Meth. | Instr. | CC | TSRC | UT1 | UT2 | UT3 | UT4 | UT2E | UT3E | Dur. | Chrd |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| 1 | show | Jean-Francois Pittet | O+ | VID | M254 | DE | GPS | 19:49:55 | 19:50:51.6 | 19:50:57.0 | 19:51:55 | 0.400 | 0.400 | 5.40 | 90.2 |
| 2 | show | Joachim Siegert | O+ | VID | M279 | DE | GPS | 19:49:50 | 19:50:48.019 | 19:50:52.219 | 19:51:50 | 0.704 | 0.704 | 4.20 | 70.1 |
| 3 | show | Jiri Polak | O+ | VID | M300 | CZ | NTP | 19:48:52 | 19:50:51.1 | 19:50:55.7 | 19:52:52 | 0.300 | 0.300 | 4.60 | 76.8 |
| 4 | show | Jiri Kubanek | O+ | VID | M303 | CZ | GPS | 19:49:53 | 19:50:51.6 | 19:50:56.6 | 19:51:54 | 0.800 | 0.800 | 5.00 | 83.5 |
| 5 | show | Jiri Kubanek | O+ | VID | M200 | CZ | GPS | 19:49:53 | 19:50:51.9 | 19:50:56.9 | 19:51:53 | 0.900 | 0.900 | 5.00 | 83.5 |
| 6 | show | Zdenek Moravec | O+ | CCD | T600 | CZ | GPS | 19:49:50 | 19:50:48.8 | 19:50:53.1 | 19:51:48 | 0.300 | 0.400 | 4.30 | 71.8 |
| 7 | show | Serge Vasseur | O+ | VID | M406 | FR | GPS | 19:45:00 | 19:50:09.47 | 19:50:13.22 | 19:55:00 | 0.770 | 0.770 | 3.75 | 62.6 |
| 8 | show | Deborah Smith | O- | VID | M300 | ES | GPS | 19:49:38 | :: | :: | 19:51:39 | ||||
| 9 | show | Deborah Smith | O- | VID | M250 | ES | GPS | 19:49:35 | :: | :: | 19:51:36 | ||||
| 10 | show | Andreas Schweizer | O- | VID | M250 | CH | GPS | 19:49:46 | :: | :: | 19:51:45 | ||||
| 11 | show | Stefan Meister | O- | VID | M500 | CH | GPS | 19:50:24 | :: | :: | 19:51:09 |
11 observations found in db: sodis
Available (probably) matching predictions (click on the link to switch):| JPL157 : e43ba930-d9b1-11f1-43f3-09febfbea233 [db: observed] |
Using prediction e43ba930-d9b1-11f1-43f3-09febfbea233 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 = 120 km From 7 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. |
Sky projection (artificial light) for occ. time: 2026-09-22, 19:49 UT (JD = 2461306.326)
| DAMIT | Q | P (h) | λ, β | JD0 | JD-JD0 | φ0 | Version | Modified | Vol-equiv D | Cmnt |
|---|---|---|---|---|---|---|---|---|---|---|
| # 1826 | 4.0 | 5.385 | 74°, 20° | 2.44450276914e6 | 16803.6 | 0.0° | None | 2017-06-19 | 124.0 +/- 5.0 km | 2017-06-16 |
Image size: 300px. Transparent image background for copy & paste
| Map with groundtrack and observer stations |
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| Event Details |
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Occultation UUID [and DB] : e43ba930-d9b1-11f1-43f3-09febfbea233 [observed] Occultation Date + Time : 2026-09-22 at 19:49:29 UT +/- 0.0 min [1] Object Designation : (216) Kleopatra Orbit Class : MBA Star Designation : GDR3 4164091091225062144 Star Coordinates (ICRF) : RA = 17 47 08.3205, DE = -10 12 01.170 [2] Star Magnitudes : G = 13.98 mag, RP = 13.05 mag, BP = 14.89 mag Object Magnitude : V = 12.27 mag Estimated Magnitude Drop : 0.2 mag Estimated Max. Duration : 8.1 sec Object Mean Diameter : 135.1 km (src: astorb) Speed of the shadow : 16.7 km/s Elongation to Moon & Sun : 49° (sunlit = 85%), Sun = 87° Cross-track uncertainty : 1.0 mas = 1 km = 0.01 path-width (1-sig) RUWE and duplicate source : 1.02 mas, dup.src = 0 (0:false, 1:true) Ephemeris Reference : JPL157 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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