Discovery | |
---|---|
Discovered by | Robert Luther |
Discovery date | 14 March 1885 |
Designations | |
(247) Eukrate | |
Pronunciation | /juːˈkreɪtiː/[a] |
Named after | Eucrate |
A885 EB, 1901 TB 1947 TA, 1960 TC | |
Main belt | |
Orbital characteristics[1] | |
Epoch 31 July 2016 (JD 2457600.5) | |
Uncertainty parameter 0 | |
Observation arc | 131.09 yr (47880 d) |
Aphelion | 3.4086 AU (509.92 Gm) |
Perihelion | 2.0778 AU (310.83 Gm) |
2.7432 AU (410.38 Gm) | |
Eccentricity | 0.24257 |
4.54 yr (1659.5 d) | |
Average orbital speed | 18.0 km/s |
75.9892° | |
0° 13m 0.948s / day | |
Inclination | 24.991° |
0.16410° | |
54.969° | |
Physical characteristics | |
130.935±0.505 km[1] | |
61580 km2[b] | |
Volume | 1.361×106 km3[c] |
Mass | (1.99 ± 0.830/0.62)×1018 kg[2] |
Mean density | 1.693 ± 0.706/0.527 g/cm3[2][d] |
12.093 h (0.5039 d) | |
0.064±0.012[1] | |
CP | |
8.20[1] | |
247 Eukrate is a rather large main-belt asteroid. It is dark and probably a primitive carbonaceous body. The asteroid was discovered by Robert Luther on March 14, 1885, in Düsseldorf. It was named after Eucrate, a Nereid in Greek mythology.
In 2001, the asteroid was detected by radar from the Arecibo Observatory at a distance of 1.18 AU. The resulting data yielded an effective diameter of 134 ± 15 km.[3]
There have been 9 occultation observations of this asteroid since 2004.[4] The latest of 2018 May 12 was a 5 chord observation that allows, using Occult (Software), the scaling of the DAMIT model 1207, to yield a mean volume-equivalent diameter of 137.5 km and a mean surface-equivalent diameter of 140.0 km.
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