2099 Öpik

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2099 Öpik
Discovery 
U–B = 0.350[1]
15.18[1][4] · 15.22[5]

2099 Öpik, provisional designation 1977 VB, is a dark and eccentric

Mars-crosser from the inner regions of the asteroid belt
, approximately 5.1 kilometers in diameter.

The asteroid was discovered on 8 November 1977, by American astronomer

Eleanor Helin at the Palomar Observatory in California, and named after Estonian astronomer Ernst Öpik.[3]

Orbit and classification

Öpik orbits the Sun in the inner main-belt at a distance of 1.5–3.1 AU once every 3 years and 6 months (1,277 days). Its orbit has an eccentricity of 0.36 and an inclination of 27° with respect to the ecliptic.[1] The first used precovery was taken at the discovering observatory in 1970, extending the asteroid's observation arc by 7 years prior to its discovery.[3]

Physical characteristics

Originally, the asteroid's

albedo (below).[1]

Diameter and albedo

According to the survey carried out by NASA's

albedo of 0.05.[5] The Collaborative Asteroid Lightcurve Link assumes a standard albedo for carbonaceous asteroids of 0.057 and calculates a diameter of 5.12 kilometers with an absolute magnitude of 15.18.[4]

Rotation period

In 2005, a photometric

Naming

This

M.P.C. 4548).[8]

References

  1. ^ a b c d e f g h i j "JPL Small-Body Database Browser: 2099 Opik (1977 VB)" (2017-03-05 last obs.). Jet Propulsion Laboratory. Retrieved 11 June 2017.
  2. ^ .
  3. ^ a b c "2099 Opik (1977 VB)". Minor Planet Center. Retrieved 7 December 2016.
  4. ^ a b c d e "LCDB Data for (2099) Öpik". Asteroid Lightcurve Database (LCDB). Retrieved 7 December 2016.
  5. ^ .
  6. ^ a b Behrend, Raoul. "Asteroids and comets rotation curves – (2099) Öpik". Geneva Observatory. Retrieved 7 December 2016.
  7. ^ . Retrieved 27 April 2016.
  8. .

External links