669 Kypria

In this article, we will explore the different aspects related to 669 Kypria, understanding its importance and its impact on today's society. From its origins to its current situation, we will analyze how 669 Kypria has managed to influence different aspects of daily life. We will address different perspectives and opinions on 669 Kypria, seeking to understand its relevance in different contexts. Additionally, we will examine potential challenges and opportunities related to 669 Kypria, and how these may impact the future. Through this article, we will seek to shed light on the role of 669 Kypria in the contemporary world and how it continues to shape our reality.

669 Kypria
A three-dimensional model of 669 Kypria based on its light curve
Discovery
Discovered byAugust Kopff
Discovery siteHeidelberg
Discovery date20 August 1908
Designations
(669) Kypria
Pronunciation/ˈkɪpriə/[1]
1908 DQ
Orbital characteristics[2]
Epoch 31 July 2016 (JD 2457600.5)
Uncertainty parameter 0
Observation arc110.22 yr (40258 d)
Aphelion3.2452 AU (485.48 Gm)
Perihelion2.7840 AU (416.48 Gm)
3.0146 AU (450.98 Gm)
Eccentricity0.076496
5.23 yr (1911.8 d)
277.943°
0° 11m 17.88s / day
Inclination10.794°
170.761°
114.672°
Physical characteristics
15.875±0.65 km
14.283 h (0.5951 d)
0.1405±0.012
10.24

669 Kypria is a minor planet orbiting the Sun that was discovered by German astronomer August Kopff on August 20, 1908.

This is a member of the dynamic Eos family of asteroids that most likely formed as the result of a collisional breakup of a parent body.[3]

References

  1. ^ "Cyprian". Oxford English Dictionary (Online ed.). Oxford University Press. (Subscription or participating institution membership required.)
  2. ^ Yeomans, Donald K., "669 Kypria", JPL Small-Body Database Browser, NASA Jet Propulsion Laboratory, retrieved 5 May 2016.
  3. ^ Veeder, G. J.; et al. (March 1995), "Eos, Koronis, and Maria family asteroids: Infrared (JHK) photometry" (PDF), Icarus, vol. 114, pp. 186–196, Bibcode:1995Icar..114..186V, CiteSeerX 10.1.1.31.2739, doi:10.1006/icar.1995.1053.