15374 Teta

15374 Teta
Discovery[1]
Discovered by M. Tichý
Z. Moravec
Discovery site Kleť Obs.
Discovery date 16 January 1997
Designations
MPC designation 15374 Teta
Named after
Teta (Czech mythology)[2]
1997 BG
main-belt · Hungaria[3]
Orbital characteristics[1]
Epoch 16 February 2017 (JD 2457800.5)
Uncertainty parameter 0
Observation arc 65.55 yr (23,943 days)
Aphelion 2.3155 AU
Perihelion 1.6708 AU
1.9932 AU
Eccentricity 0.1617
2.81 yr (1,028 days)
218.09°
 21m 1.08s / day
Inclination 32.403°
131.98°
190.29°
Earth MOID 0.6602 AU
Physical characteristics
Dimensions 3.35 km (calculated)[3]
2.820±0.005 h[4]
2.8204±0.0005 h[5]
0.30 (assumed)[3]
E[3]
14.3[1] · 14.44±0.30[6]

    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.[7]

    The bright E-type asteroid 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 1.7–2.3 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.of 1.7–2.3 AU once every 2 years and 10 months (1,028 days). Its orbit is heavily tilted by 32° to the plane of the ecliptic and shows an eccentricity of 0.16.[1] The first precovery was obtained during Digitized Sky Survey at Palomar Observatory in 1950, extending the asteroid's observation arc by 47 years prior to its discovery.[7]

    In 2014, a photometric light-curve observation with an improved period solution over a 2009-analysis at the U.S. Palmer Divide Observatory, Colorado, rendered a rotation period of 2.820±0.005 hours with a brightness amplitude of 0.30 in magnitude (U=3-).[5][4] The Collaborative Asteroid Lightcurve Link assumes a high albedo of 0.30, a typical value for the bright E-class asteroid, such as the family's largest member and namesake, 434 Hungaria.[3]

    The minor planet was named from Czech mythology after Teta, the fortune-teller, heathen priestess, and member of the Přemyslid dynasty. She is the second daughter of Duke Krok and sister of Libuše, who, according to legend, founded the city of Prague (also see 2367 Praha) in the 8th century, and after whom the minor planets 264 Libussa and 3102 Krok were named, respectively.[2] Naming citation was published on 11 November 2000 (M.P.C. 41573).[8]

    References

    1. 1 2 3 4 "JPL Small-Body Database Browser: 15374 Teta (1997 BG)" (2016-01-30 last obs.). Jet Propulsion Laboratory. Retrieved 3 December 2016.
    2. 1 2 Schmadel, Lutz D. (2007). Dictionary of Minor Planet Names – (15374) Teta. Springer Berlin Heidelberg. p. 823. ISBN 978-3-540-00238-3. Retrieved 27 April 2016.
    3. 1 2 3 4 5 "LCDB Data for (15374) Teta". Asteroid Lightcurve Database (LCDB). Retrieved 27 April 2016.
    4. 1 2 Warner, Brian D. (July 2014). "Asteroid Lightcurve Analysis at CS3-Palmer Divide Station: 2014 January-March". The Minor Planet Bulletin. 41 (3): 144–155. Bibcode:2014MPBu...41..144W. ISSN 1052-8091. Retrieved 14 January 2016.
    5. 1 2 Warner, Brian D. (January 2010). "Asteroid Lightcurve Analysis at the Palmer Divide Observatory: 2009 June-September". The Minor Planet Bulletin. 37 (1): 24–27. Bibcode:2010MPBu...37...24W. ISSN 1052-8091. Retrieved 14 January 2016.
    6. Veres, Peter; Jedicke, Robert; Fitzsimmons, Alan; Denneau, Larry; Granvik, Mikael; Bolin, Bryce; et al. (November 2015). "Absolute magnitudes and slope parameters for 250,000 asteroids observed by Pan-STARRS PS1 - Preliminary results". Icarus. 261: 34–47. arXiv:1506.00762Freely accessible. Bibcode:2015Icar..261...34V. doi:10.1016/j.icarus.2015.08.007. Retrieved 27 April 2016.
    7. 1 2 "15374 Teta (1997 BG)". Minor Planet Center. Retrieved 27 April 2016.
    8. "MPC/MPO/MPS Archive". Minor Planet Center. Retrieved 27 April 2016.

    External links

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