15374 Teta

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15374 Teta
Discovery
Synodic rotation period
2.820±0.005 h[5]
2.8204±0.0005 h[6]
0.30 (assumed)[4]
E/S[4]
14.3[1] · 14.44±0.30[4][7]

15374 Teta, provisional designation 1997 BG, is bright, stony Hungaria asteroid from the inner regions of the asteroid belt, about 3.3 kilometers in diameter. It was discovered by Czech astronomers Miloš Tichý and Zdeněk Moravec at Kleť Observatory in South Bohemia on 16 January 1997.[3] It is named after Teta from Czech mythology.[2]

Orbit and classification

Teta is a bright

Hungaria family, which form the innermost dense concentration of asteroids in the Solar System. It orbits the Sun in the inner main-belt at a distance of 1.7–2.3 AU once every 2 years and 10 months (1,028 days). Its orbit has an eccentricity of 0.16 and an inclination of 32° with respect to the ecliptic.[1] A first precovery was obtained during Digitized Sky Survey at Palomar Observatory in 1950, extending the body's observation arc by 47 years prior to its discovery.[3]

Physical characteristics

In 2014, an improved rotational

The Collaborative Asteroid Lightcurve Link assumes an albedo of 0.30 – a compromise value between 0.4 and 0.2, corresponding to the Hungaria asteroids both as family and orbital group – and calculates a diameter of 3.35 kilometers using an absolute magnitude of 14.4.[4]

Naming

This

M.P.C. 41573).[8]

References

  1. ^ a b c d e "JPL Small-Body Database Browser: 15374 Teta (1997 BG)" (2017-05-03 last obs.). Jet Propulsion Laboratory. Retrieved 5 July 2017.
  2. ^ .
  3. ^ a b c "15374 Teta (1997 BG)". Minor Planet Center. Retrieved 27 April 2016.
  4. ^ a b c d e f "LCDB Data for (15374) Teta". Asteroid Lightcurve Database (LCDB). Retrieved 27 April 2016.
  5. ^
    ISSN 1052-8091
    . Retrieved 14 January 2016.
  6. ^ . Retrieved 14 January 2016.
  7. . Retrieved 27 April 2016.
  8. ^ "MPC/MPO/MPS Archive". Minor Planet Center. Retrieved 27 April 2016.

External links