167 Urda Explained

Minorplanet:yes
167 Urda
Background:
  1. D6D6D6
Discoverer:C. H. F. Peters
Discovery Site:Clinton, New York
Discovered:28 August 1876
Mpc Name:(167) Urda
Alt Names:A876 QA; 1899 KC;
1905 QA; 1906 WA
Named After:Urd
Mp Category:main belt (Koronis asteroid family)
Epoch:31 July 2016 (JD 2457600.5)
Semimajor:2.8538511AU
Perihelion:2.7493497AU
Aphelion:2.9583526abbr=onNaNabbr=on
Eccentricity:0.0366177
Period:4.82 yr (1760.9 d)
Inclination:2.212408°
Asc Node:166.21859°
Arg Peri:133.03586°
Mean Anomaly:37.607175°
Rotation:13.07abbr=onNaNabbr=on
Spectral Type:S
Abs Magnitude:9.1
Mean Motion: / day
Observation Arc:132.01 yr (48218 d)
Uncertainty:0
Moid:1.73392AU
Jupiter Moid:2.10867AU
Tisserand:3.302

167 Urda is a main-belt asteroid that was discovered by German-American astronomer Christian Heinrich Friedrich Peters on August 28, 1876, in Clinton, New York, and named after Urd, one of the Norns in Norse mythology. In 1905, Austrian astronomer Johann Palisa showed that the asteroid varied in brightness.

Photometric observations of this asteroid at the Palmer Divide Observatory in Colorado Springs, Colorado, during 2007–8 gave a light curve with a period of 13.06133 ± 0.00002 hours. This S-type asteroid is a member of the Koronis family of asteroids that share similar orbital elements.

In 2002, a diameter estimate of 37.93 ± 3.17 km was obtained from the Midcourse Space Experiment observations, with an albedo of 0.2523 ± 0.0448.

A stellar occultation by Urda was observed from Japan on July 23, 2001.[1]

External links

Notes and References

  1. Web site: Observed Minor Planet Occultation Events - Asteroidal Occultations. 2018-10-14.