2025-10-12 / UCAC4 676-009110 / (433) Eros
| # | OBS | Observer | Occ | Meth. | Instr. | CC |
TSRC | UT1 | UT2 | UT3 | UT4 | UT2E | UT3E | Dur. | Chrd |
| 1 |
show |
Mikel Martínez |
O+ |
CCD |
M280 |
ES |
NTP |
01:12:10 |
01:14:06.443 |
01:14:11.454 |
01:16:08 |
0.087 |
0.087 |
5.01 |
27.6 |
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: 2025-10-12, 01:14 UT (JD = 2460960.551)
| DAMIT | Q | P (h) | λ, β | JD0 | JD-JD0 | φ0 | Version | Modified | Vol-equiv D | Cmnt |
| # 3083 | 5.0 | 5.270 |
17°, 11° |
2.451545e6 | 9415.6 | 32.64° |
Shape model from PDS (433 EROS PLATE MODEL MSI 1708), rotation state from Konopliv et al. (2002) | 2019-03-09 |
16.897 +/- 0.0 km |
2019-03-08 |
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] : 8eee7ac0-ddb8-11f0-547e-80ffd63f2414 [observed]
Occultation Date + Time : 2025-10-12 at 01:16:34 UT +/- 0.02 min [1]
Object Designation : (433) Eros
Orbit Class : NEO
Star Designation : GDR3 0350403433673313664
Star Coordinates (ICRF) : RA = 01 45 06.7104, DE = +45 07 20.802 [2]
Star Magnitudes : G = 12.18 mag, RP = 11.45 mag, BP = 12.77 mag
Object Magnitude : V = 10.45 mag
Estimated Magnitude Drop : 0.2 mag
Estimated Max. Duration : 5.3 sec
Object Mean Diameter : 28.8 km (src: astorb)
Speed of the shadow : 5.5 km/s
Elongation to Moon & Sun : 50° (sunlit = 69%), Sun = 142°
Cross-track uncertainty : 10.3 mas = 3 km = 0.13 path-width (1-sig)
RUWE and duplicate source : 1.0 mas, dup.src = 0 (0:false, 1:true)
Ephemeris Reference : JPL#659
Note : FP:true
[1] time t0 of closest geocentric approach c/a, [2] including proper motion until t0
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