2025-11-29 / UCAC4 636-017796 / (1927) Suvanto
| # | OBS | Observer | Occ | Meth. | Instr. | CC |
TSRC | UT1 | UT2 | UT3 | UT4 | UT2E | UT3E | Dur. | Chrd |
| 1 |
show |
Stefano Sposetti |
O+ |
VID |
M420 |
CH |
GPS |
17:15:00 |
17:15:58.7 |
17:15:59.52 |
17:17:00 |
0.200 |
0.100 |
0.82 |
9.0 |
UT1/UT4: Begin/End of observation | UT2/UT3: Begin/End of occultation | Dur: Reported duration in seconds | Chrd: Corresponding chord length in km |
More
1 observation found in db: sodis
Available (probably) matching predictions (click on the link to switch):
Sky projection (artificial light) for occ. time: 2025-11-29, 17:15 UT (JD = 2461009.219)
| DAMIT | Q | P (h) | λ, β | JD0 | JD-JD0 | φ0 | Version | Modified | Vol-equiv D | Cmnt |
| # 546 | None | 8.162 |
278°, 23° |
2.451027e6 | 9982.2 | 0.0° |
None | None |
not scaled |
2013-02-11 |
| # 547 | None | 8.162 |
74°, 73° |
2.451027e6 | 9982.2 | 0.0° |
None | None |
not scaled |
2013-02-11 |
Q: model quality flag (0-5, 5=highest) | P: rotation period | λ,β: ecl. lon. and lat. of spin axis (J2000) | JD: initial time (epoch) | φ0: initial rotation angle for JD0
Image size: 300px. Transparent image background for copy & paste
| Map with groundtrack and observer stations |
| Event Details |
|
Occultation UUID [and DB] : ce23d0a0-ddb8-11f0-547e-5e15fa379242 [observed]
Occultation Date + Time : 2025-11-29 at 17:08:21 UT +/- 0.0 min [1]
Object Designation : (1927) Suvanto
Orbit Class : MBA
Star Designation : GDR3 0177523097268513792
Star Coordinates (ICRF) : RA = 04 22 05.5536, DE = +37 01 44.343 [2]
Star Magnitudes : G = 14.5 mag, RP = 13.37 mag, BP = 15.85 mag
Object Magnitude : V = 15.23 mag
Estimated Magnitude Drop : 1.2 mag
Estimated Max. Duration : 1.2 sec
Object Mean Diameter : 13.0 km (src: astorb)
Speed of the shadow : 11.0 km/s
Elongation to Moon & Sun : 75° (sunlit = 65%), Sun = 165°
Cross-track uncertainty : 1.0 mas = 1 km = 0.08 path-width (1-sig)
RUWE and duplicate source : 0.98 mas, dup.src = 0 (0:false, 1:true)
Ephemeris Reference : JPL#77
Note : FP:true
[1] time t0 of closest geocentric approach c/a, [2] including proper motion until t0
|
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