3548 Eurybates

3548 Eurybates
Eurybates and its satellite Queta (circled) imaged by the Hubble Space Telescope in 2019–2020
Discovery
Discovered byC. J. van Houten
I. van Houten-G.
Tom Gehrels
Discovery sitePalomar Obs.
Discovery date19 September 1973
Designations
(3548) Eurybates
Pronunciation/jʊˈrɪbətz/
Named after
Eurybates
(Greek mythology)
1973 SO · 1954 CB
1957 JX · 1978 EE5
1985 TZ
Jupiter trojan
Greek
Eurybates

binary
AdjectivesEurybatian
Orbital characteristics
Epoch 25 February 2023 (JD 2460000.5)
Uncertainty parameter 0
Earliest precovery date9 February 1954
Aphelion5.680 AU
Perihelion4.733 AU
5.206 AU
Eccentricity0.0909
11.88 yr (4,339 d)
27.507°
0° 4m 58.682s / day
Inclination8.054°
43.542°
27.481°
Jupiter MOID0.1092 AU
TJupiter2.972
Physical characteristics
Dimensions77.5 × 71.3 × 61.8 km
69.3±1.4 km (area equivalent)
Mass(1.51±0.03)×1017 kg
Mean density
1.1±0.3 g/cm3
8.7027283±0.0000029 h
150° (wrt ecliptic)
158° (wrt orbit)
−60°
320°
0.044±0.003
C
B–V = 0.739±0.026
V–R = 0.384±0.021
V–I = 0.355±0.015
16.2 to 18.1
9.800±0.007

    3548 Eurybates (/jʊˈrɪbətz/ yə-RIB-ə-teez) is a carbonaceous Jupiter trojan from the Greek camp and the parent body of the Eurybates family, approximately 68 kilometers (42 miles) in diameter. It is a target to be visited by the Lucy mission in August 2027. Discovered during the second Palomar–Leiden Trojan survey in 1973, it was later named after Eurybates from Greek mythology. This C-type asteroid is among the 60 largest known Jupiter trojans and has a rotation period of 8.7 hours. Eurybates has one kilometer-sized satellite, named Queta, that was discovered in images taken by the Hubble Space Telescope in September 2018.