![]() A three-dimensional model of 690 Wratislavia based on its light curve | |
Discovery | |
---|---|
Discovered by | Joel Hastings Metcalf |
Discovery site | Taunton, Massachusetts |
Discovery date | 16 October 1909 |
Designations | |
(690) Wratislavia | |
Pronunciation | /vrætɪˈslɑːviə/ |
Named after | Wrocław |
1909 HZ | |
Orbital characteristics[1] | |
Epoch 31 July 2016 (JD 2457600.5) | |
Uncertainty parameter 0 | |
Observation arc | 113.75 yr (41547 d) |
Aphelion | 3.7163 AU (555.95 Gm) |
Perihelion | 2.5737 AU (385.02 Gm) |
3.1450 AU (470.49 Gm) | |
Eccentricity | 0.18166 |
5.58 yr (2037.2 d) | |
53.487° | |
0° 10m 36.192s / day | |
Inclination | 11.266° |
253.160° | |
114.819° | |
Physical characteristics | |
Mass | (1.28±0.03)×1019 kg[2] |
Mean density | 7.81±1.77 g/cm3[2] |
8.64 h (0.360 d) | |
0.0604±0.004 | |
8.02 | |
690 Wratislavia is a minor planet orbiting the Sun. Wratislavia was discovered on October 16, 1909.[1] IRAS data shows it is about 135 km in diameter.[1]
Wratislavia has been studied by radar.[3]
Carry2012
was invoked but never defined (see the help page).