1815 Beethoven

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1815 Beethoven
Discovery
U–B = 0.330[2]
11.33[5]
11.36[1][2][6][7][8][10][11][13]

1815 Beethoven, provisional designation 1932 CE1, is a carbonaceous background

rotation period of 54 hours (tentative).[13] It was named after Ludwig van Beethoven.[1]

Orbit and classification

Beethoven is a non-

602), a very large family of carbonaceous asteroids, named after 24 Themis.[3][13]

It orbits the Sun in the

semi-major axis of 3.15 AU). Its orbit has an eccentricity of 0.19 and an inclination of 3° with respect to the ecliptic.[2] The body's observation arc begins with its official discovery observation at Heidelberg in January 1992.[1]

Naming

This

M.P.C. 3935).[14]

Physical characteristics

In the

Tholen classification, Beethoven is an uncommon, carbonaceous F-type asteroid,[2] while in the Barucci taxonomy, it is a C0 type.[3]

Rotation period

In January 2005, a fragmentary rotational

Diameter and albedo

According to the surveys carried out by the Infrared Astronomical Satellite

albedo between 0.04 and 0.10.[5][6][7][8][9][10][11]

The Collaborative Asteroid Lightcurve Link adopts the results obtained by IRAS, that is, an albedo of 0.0548 and a diameter of 30.36 kilometers based on an absolute magnitude of 11.36.[13]

References

  1. ^ a b c d e f g h "1815 Beethoven (1932 CE1)". Minor Planet Center. Retrieved 7 December 2018.
  2. ^ a b c d e f g h "JPL Small-Body Database Browser: 1815 Beethoven (1932 CE1)" (2018-09-10 last obs.). Jet Propulsion Laboratory. Retrieved 7 December 2018.
  3. ^ a b c d e "Asteroid 1815 Beethoven". Small Bodies Data Ferret. Retrieved 7 December 2018.
  4. ^ a b "Asteroid (1815) Beethoven – Proper elements". AstDyS-2, Asteroids – Dynamic Site. Retrieved 4 December 2018.
  5. ^ .
  6. ^ .
  7. ^ . Retrieved 17 October 2019.
  8. ^ . Retrieved 7 December 2018.
  9. ^ .
  10. ^ )
  11. ^ )
  12. ^ .
  13. ^ a b c d e "LCDB Data for (1815) Beethoven". Asteroid Lightcurve Database (LCDB). Retrieved 7 December 2018.
  14. .

External links