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13006 Schwaar

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Phocaea asteroid

13006 Schwaar
Discovery
Discovered byB. A. Skiff
Discovery siteAnderson Mesa Stn.
Discovery date12 January 1983
Designations
MPC designation(13006) Schwaar
Named afterPierre–Yves Schwaar
(American amateur astronomer)
Alternative designations1983 AC1 · 1990 DH
Minor planet categorymain-belt · Phocaea
Orbital characteristics
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc34.21 yr (12,495 days)
Aphelion2.7336 AU
Perihelion1.8143 AU
Semi-major axis2.2739 AU
Eccentricity0.2021
Orbital period (sidereal)3.43 yr (1,252 days)
Mean anomaly29.457°
Mean motion0° 17 14.64 / day
Inclination28.523°
Longitude of ascending node129.27°
Argument of perihelion358.22°
Physical characteristics
Dimensions5.04 km (calculated)
5.325±0.052
5.892±0.113 km
Synodic rotation period6.8 h
Geometric albedo0.182±0.038
0.1850±0.0281
0.23 (assumed)
Spectral typeS
Absolute magnitude (H)13.6 · 13.7 · 13.97±0.22

13006 Schwaar, provisional designation 1983 AC1, is a stony Phocaea asteroid from the inner regions of the asteroid belt, approximately 5 kilometers in diameter. It was discovered on 12 January 1983, by American astronomer Brian Skiff at Lowell's Anderson Mesa Station in Flagstaff, Arizona. The asteroid was named after amateur astronomer Pierre–Yves Schwaar.

Orbit and classification

Schwaar is a member of the Phocaea family (701), a rather small group of asteroids with similar orbital characteristics, named after its largest member, 25 Phocaea. It orbits the Sun in the inner main-belt at a distance of 1.8–2.7 AU once every 3 years and 5 months (1,252 days). Its orbit has an eccentricity of 0.20 and an inclination of 29° with respect to the ecliptic. No precoveries were taken. The asteroid's observation arc begins 20 days after its discovery.

Physical characteristics

Schwaar has been characterized as a S-type asteroid by Pan-STARRS photometric survey.

Lightcurves

A rotational lightcurve of Schwaar was obtained from photometric observations made at the Hunters Hill Observatory (E14), Australia, and collaborating stations in December 2006. The lightcurve gave a rotation period of 6.8 hours with a brightness variation of 0.17 in magnitude (U=3-).

Diameter and albedo

According to the survey carried out by the NEOWISE mission of NASA's space-based Wide-field Infrared Survey Explorer, Schwaar measures 5.3 and 5.9 kilometers in diameter and its surface has an albedo of 0.182 and 0.185, respectively, while the Collaborative Asteroid Lightcurve Link assumes a standard albedo for members of the Phocaea family of 0.23, and calculates a diameter of 5.0 kilometers with an absolute magnitude of 13.7.

Naming

This minor planet was named in memory amateur astronomer Pierre–Yves Schwaar (1946–2000), member of the Saguaro Astronomy Club (SAC), telescope maker, and photographer of the night sky. The official naming citation was published by the Minor Planet Center on 9 January 2001 (M.P.C. 41939). The native Swiss amateur astronomer and immigrant to the U.S. was also an inventor and master craftsman, a model rocketeer, an USAF aircraft mechanic, a Vietnam veteran, and an eclipse chaser.

References

  1. ^ "JPL Small-Body Database Browser: 13006 Schwaar (1983 AC1)" (2017-03-29 last obs.). Jet Propulsion Laboratory. Retrieved 24 June 2017.
  2. ^ Schmadel, Lutz D. (2007). "(13006) Schwaar". Dictionary of Minor Planet Names – (13006) Schwaar. Springer Berlin Heidelberg. p. 791. doi:10.1007/978-3-540-29925-7_8722. ISBN 978-3-540-00238-3.
  3. ^ "LCDB Data for (13006) Schwaar". Asteroid Lightcurve Database (LCDB). Retrieved 25 May 2016.
  4. ^ "Asteroid 13006 Schwaar – Nesvorny HCM Asteroid Families V3.0". Small Bodies Data Ferret. Retrieved 27 October 2019.
  5. ^ Masiero, Joseph R.; Mainzer, A. K.; Grav, T.; Bauer, J. M.; Cutri, R. M.; Dailey, J.; et al. (November 2011). "Main Belt Asteroids with WISE/NEOWISE. I. Preliminary Albedos and Diameters". The Astrophysical Journal. 741 (2): 20. arXiv:1109.4096. Bibcode:2011ApJ...741...68M. doi:10.1088/0004-637X/741/2/68. Retrieved 3 December 2016.
  6. ^ Mainzer, A.; Grav, T.; Masiero, J.; Hand, E.; Bauer, J.; Tholen, D.; et al. (November 2011). "NEOWISE Studies of Spectrophotometrically Classified Asteroids: Preliminary Results". The Astrophysical Journal. 741 (2): 25. arXiv:1109.6407. Bibcode:2011ApJ...741...90M. doi:10.1088/0004-637X/741/2/90. Retrieved 25 May 2016.
  7. ^ Higgins, David; Oey, Julian (September 2007). "Asteroid Lightcurve Analysis at Hunters Hill Observatory and Collaborating Stations - December 2006 - April 2007". The Minor Planet Bulletin. 34 (3): 79–80. Bibcode:2007MPBu...34...79H. ISSN 1052-8091. Retrieved 25 May 2016.
  8. ^ 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:1506.00762. Bibcode:2015Icar..261...34V. doi:10.1016/j.icarus.2015.08.007. Retrieved 25 May 2016.
  9. ^ "13006 Schwaar (1983 AC1)". Minor Planet Center. Retrieved 25 May 2016.
  10. "MPC/MPO/MPS Archive". Minor Planet Center. Retrieved 25 May 2016.

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