2025-09-01 / UCAC4 619-024419 / (1642) Hill
| # | OBS | Observer | Occ | Meth. | Instr. | CC |
TSRC | UT1 | UT2 | UT3 | UT4 | UT2E | UT3E | Dur. | Chrd |
| 1 |
show |
Simon Kidd |
O+ |
VID |
M350 |
GB |
GPS |
00:52:00 |
00:52:55.81 |
00:52:56.53 |
00:54:00 |
0.040 |
0.040 |
0.72 |
18.6 |
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: 2025-09-01, 00:52 UT (JD = 2460919.536)
| DAMIT | Q | P (h) | λ, β | JD0 | JD-JD0 | φ0 | Version | Modified | Vol-equiv D | Cmnt |
| # 4668 | 1.0 | 6.043 |
117°, 64° |
2.45723e6 | 3689.5 | 0.0° |
None | 2020-10-05 |
not scaled |
2019-10-23 |
| # 4669 | 1.0 | 6.043 |
276°, 33° |
2.45723e6 | 3689.5 | 0.0° |
None | 2020-10-05 |
not scaled |
2019-10-23 |
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] : 5c3e3620-ddb7-11f0-547e-8afbecdbfcdb [observed]
Occultation Date + Time : 2025-09-01 at 00:54:53 UT +/- 0.0 min [1]
Object Designation : (1642) Hill
Orbit Class : MBA
Star Designation : GDR3 3449478828889091456
Star Coordinates (ICRF) : RA = 05 35 18.0738, DE = +33 41 52.353 [2]
Star Magnitudes : G = 14.14 mag, RP = 13.52 mag, BP = 14.59 mag
Object Magnitude : V = 16.29 mag
Estimated Magnitude Drop : 2.3 mag
Estimated Max. Duration : 1.0 sec
Object Mean Diameter : 26.1 km (src: astorb)
Speed of the shadow : 25.8 km/s
Elongation to Moon & Sun : 171° (sunlit = 57%), Sun = 74°
Cross-track uncertainty : 0.2 mas = 0 km = 0.02 path-width (1-sig)
RUWE and duplicate source : 1.01 mas, dup.src = 0 (0:false, 1:true)
Ephemeris Reference : JPL#73
Note : FP:true
[1] time t0 of closest geocentric approach c/a, [2] including proper motion until t0
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