2000-08-07 / HIP 11333 / (372) Palma
# | OBS | Observer | Occ | Meth. | Instr. | CC | TSRC | UT1 | UT2 | UT3 | UT4 | UT2E | UT3E | Dur. | Chrd |
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1 | show | Arturo Ramirez | O+ | VIS | M250 | ES | RAD | 03:24:58.0 | 03:25:05.5 | 7.50 | 177.0 | ||||
2 | show | Jose Ripero | O+ | VIS | ES | 03:24:58.7 | 03:25:07.7 | 9.00 | 212.4 | ||||||
3 | show | Maylis Lavayssiere | O+ | VIS | L127 | FR | RAD | 03:25:00 | 03:25:17 | 03:25:21.7 | 03:26:00 | 4.70 | 110.9 | ||
4 | show | Gino Farroni | O+ | CCD | M410 | FR | 03:24:00 | 03:44:00 | |||||||
5 | show | Gilles Regheere | O+ | VIS | B80 | FR | RAD | 03:15:00 | 03:25:46.5 | 03:25:49.0 | 03:28:00 | 1.5 | 1 | 2.50 | 59.0 |
6 | show | Patrick Degrelle | O+ | VIS | M153 | FR | RAD++ | 03:15:29 | 03:25:51 | 03:25:54 | 03:32:07 | 1 | 1 | 3.00 | 70.8 |
7 | show | C. Eliche et al | O- | CCD | M810 | ES | |||||||||
8 | show | Juan Pastor | O- | VIS | M114 | ES | 03:15:00 | 03:36:00 | |||||||
9 | show | Hilari Pallares | O- | VIS | M200 | ES | 02:50:00 | 04:05:00 | |||||||
10 | show | Oscar Canales | O- | VIS | M120 | ES | 03:19:30 | 03:31:30 | |||||||
11 | show | Alain Klotz | O- | CCD | M200 | FR | 03:21:45 | 03:31:45 | |||||||
12 | show | Nick Quinn | O- | VIS | M90 | UK | 03:24:00 | 03:28:00 | |||||||
13 | show | Andrew Elliott | O- | VID | M254 | UK | 03:15:00 | 03:35:00 |
13 observations found in db: euraster
Available (probably) matching predictions (click on the link to switch):JPL#108 : 75225ef8-51f0-445d-a336-87c1b78ce509 [db: observed] |
Using prediction 75225ef8-51f0-445d-a336-87c1b78ce509 for map and profile fit
Ellipse and circular profile fits to the timings (chords) |
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Auto-Fit Result: Size = 329 x 117 km a',b' = 164.7, 58.7 km X0,Y0 = 2020.1, -26.5 km Mean diameter = 197 km From 5 chords (VIS) 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: 2000-08-07, 03:23 UT (JD = 2451763.641)
DAMIT | Q | P (h) | λ, β | JD0 | JD-JD0 | φ0 | Version | Modified | Vol-equiv D | Cmnt |
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# 298 | None | 8.582 | 221°, -47° | 2.443889e6 | 7874.6 | 0.0° | None | 2011-05-02 | 187.0 +/- 20.0 km | 2011-02-18 |
# 299 | None | 8.582 | 44°, 17° | 2.443889e6 | 7874.6 | 0.0° | None | 2011-05-02 | 198.0 +/- 26.0 km | 2011-02-18 |
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] : 75225ef8-51f0-445d-a336-87c1b78ce509 [observed] Occultation Date + Time : 2000-08-07 at 03:25:42 UT +/- 0.03 min [1] Object Designation : (372) Palma Orbit Class : MBA Star Designation : GDR3 0328338090729271040 Star Coordinates (ICRF) : RA = 02 25 49.9419, DE = +37 00 49.246 [2] Star Magnitudes : G = 6.44 mag, RP = 5.41 mag, BP = 7.54 mag Object Magnitude : V = 12.46 mag Estimated Magnitude Drop : 6.0 mag Estimated Max. Duration : 8.0 sec Object Mean Diameter : 189 km (src: astorb) Speed of the shadow : 23.6 km/s Elongation to Moon & Sun : 154° (sunlit = 51%), Sun = 89° Cross-track uncertainty : 6.7 mas = 11 km = 0.06 path-width (1-sig) RUWE and duplicate source : 1.26 mas, dup.src = 0 (0:false, 1:true) Ephemeris Reference : JPL#108 [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) |