3169 Ostro

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3169 Ostro
U–B = 0.306[1]
12.73[1][4]

3169 Ostro, provisional designation 1981 LA, is a

Hungaria family asteroid from the innermost regions of the asteroid belt
, approximately 5 kilometers in diameter.

The asteroid was discovered on 4 June 1981, by American astronomer

Edward Bowell at Lowell's Anderson Mesa Station in Flagstaff, Arizona,[3] and named after planetary scientist Steven J. Ostro at JPL.[2]

Orbit and classification

Ostro is a member of the

Hungaria family, which form the innermost dense concentration of asteroids in the Solar System. It orbits the Sun at a distance of 1.8–2.0 AU once every 2 years and 7 months (950 days). Its orbit has an eccentricity of 0.07 and an inclination of 25° with respect to the ecliptic.[1]

Physical characteristics

In the

SMASS taxonomy, Ostro is classified as a TS-type and Xe-type asteroid, respectively.[1] It has also been characterized as an E-type asteroid.[4]

According to the survey carried out by NASA's

albedo of 0.960.[5] The Collaborative Asteroid Lightcurve Link derives an albedo of 0.5152 and a diameter of 5.27 kilometers with an absolute magnitude of 12.73.[4]

In May 2012, a rotational

Naming

This

M.P.C. 11749).[7]

References

  1. ^ a b c d e f g h i j "JPL Small-Body Database Browser: 3169 Ostro (1981 LA)" (2017-06-04 last obs.). Jet Propulsion Laboratory. Archived from the original on 23 April 2017. Retrieved 15 June 2017.
  2. ^ .
  3. ^ a b "3169 Ostro (1981 LA)". Minor Planet Center. Retrieved 15 June 2017.
  4. ^ a b c d e f "LCDB Data for (3169) Ostro". Asteroid Lightcurve Database (LCDB). Retrieved 15 June 2017.
  5. ^ . Retrieved 15 June 2017.
  6. ^ . Retrieved 15 June 2017.
  7. ^ "MPC/MPO/MPS Archive". Minor Planet Center. Retrieved 15 June 2017.

External links