10251 Mulisch

Source: Wikipedia, the free encyclopedia.

10251 Mulisch
Discovery
Perihelion
2.1299 AU
2.3333 AU
Eccentricity0.0872
3.56 yr (1,302 d)
147.36°
0° 16m 35.4s / day
Inclination2.0659°
250.96°
205.49°
Physical characteristics
Mean diameter
2.398±0.559 km[4]
0.337±0.158[4]
15.2[2]

10251 Mulisch, provisional designation 3089 T-1, is a bright background

Cornelis van Houten at Leiden, and Tom Gehrels at Palomar Observatory in California, United States. The asteroid was named after Dutch writer Harry Mulisch.[1]

Orbit and classification

Mulisch is a non-

semi-major axis of 2.33 AU). Its orbit has an eccentricity of 0.09 and an inclination of 2° with respect to the ecliptic.[2] The body's observation arc begins at Palomar on 26 March 1971, two nights prior to its official discovery observation.[1]

Palomar–Leiden Trojan survey

The

Palomar–Leiden Trojan survey, named after the fruitful collaboration of the Palomar and Leiden Observatory in the 1960s and 1970s. Gehrels used Palomar's Samuel Oschin telescope (also known as the 48-inch Schmidt Telescope), and shipped the photographic plates to Ingrid and Cornelis van Houten at Leiden Observatory where astrometry was carried out. The trio are credited with the discovery of several thousand asteroid discoveries.[5]

Physical characteristics

The asteroid has an

rotation period, pole and shape remain unknown.[2]

Diameter and albedo

According to the survey carried out by the

albedo of 0.337.[4]

Naming

This

M.P.C. 56959).[6]

References

  1. ^ a b c d e f "10251 Mulisch (3089 T-1)". Minor Planet Center. Retrieved 1 May 2018.
  2. ^ a b c d e f "JPL Small-Body Database Browser: 10251 Mulisch (3089 T-1)" (2017-04-28 last obs.). Jet Propulsion Laboratory. Retrieved 1 May 2018.
  3. ^ a b "Asteroid 10251 Mulisch – Proper Elements". AstDyS-2, Asteroids – Dynamic Site. Retrieved 29 October 2019.
  4. ^ . Retrieved 1 May 2018.
  5. ^ "Minor Planet Discoverers". Minor Planet Center. 2018. Retrieved 1 May 2018.
  6. ^ "MPC/MPO/MPS Archive". Minor Planet Center. Retrieved 1 May 2018.

External links