.png) A three-dimensional model of 669 Kypria based on its light curve | |
| Discovery | |
|---|---|
| Discovered by | August Kopff |
| Discovery site | Heidelberg |
| Discovery date | 20 August 1908 |
| Designations | |
| (669) Kypria | |
| Pronunciation | /ˈkɪpriə/[1] |
| 1908 DQ | |
| Orbital characteristics[2] | |
| Epoch 31 July 2016 (JD 2457600.5) | |
| Uncertainty parameter 0 | |
| Observation arc | 110.22 yr (40258 d) |
| Aphelion | 3.2452 AU (485.48 Gm) |
| Perihelion | 2.7840 AU (416.48 Gm) |
| 3.0146 AU (450.98 Gm) | |
| Eccentricity | 0.076496 |
| 5.23yr (1911.8d) | |
| 277.943° | |
| 0° 11m 17.88s / day | |
| Inclination | 10.794° |
| 170.761° | |
| 114.672° | |
| Physical characteristics | |
| 15.875±0.65km | |
| 14.283 h (0.5951 d) | |
| 0.1405±0.012 | |
| 10.24 | |
669 Kypria is aminor planet orbiting theSun that was discovered by German astronomerAugust Kopff on August 20, 1908.
This is a member of the dynamicEos family of asteroids that most likely formed as the result of a collisional breakup of a parent body.[3]
_mathilde.jpg) | This article about an asteroid native to theasteroid belt is astub. You can help Wikipedia byexpanding it. |
