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12848 Agostino

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12848 Agostino
Discovery
Discovered byA. Boattini
Discovery siteCampo Imperatore
Discovery date10 July 1997
Designations
MPC designation(12848) Agostino
Named afterAgostino Boattini
(discoverer's father)
Alternative designations1997 NK10 · 1993 QQ10
Minor planet categorymain-belt · Eunomia
Orbital characteristics
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc66.88 yr (24,428 days)
Aphelion2.8514 AU
Perihelion2.3537 AU
Semi-major axis2.6025 AU
Eccentricity0.0956
Orbital period (sidereal)4.20 yr (1,534 days)
Mean anomaly183.78°
Mean motion0° 14 5.28 / day
Inclination15.066°
Longitude of ascending node172.84°
Argument of perihelion249.89°
Physical characteristics
Dimensions4.55 km (calculated)
4.864±0.120 km
Synodic rotation period6.3225±0.0052 h
6.3350±0.0258 h
Geometric albedo0.21 (assumed)
0.225±0.033
Spectral typeS
Absolute magnitude (H)13.6 · 13.54±0.32 · 13.8 · 13.537±0.006 (R) · 13.574±0.007 (R) · 14.02

12848 Agostino, provisional designation 1997 NK10, is a stony Eunomia asteroid from the central region of the asteroid belt, approximately 5 kilometers in diameter.

The asteroid was discovered on 10 July 1997, by Italian astronomer Andrea Boattini at the Campo Imperatore Observatory in the Gran Sasso massif of central Italy. It was named after the father of the discoverer, Agostino Boattini.

Orbit and classification

Agostino is a member of the Eunomia family, a large group of stony S-type asteroids and the most prominent family in the intermediate main-belt. It orbits the Sun at a distance of 2.4–2.9 AU once every 4 years and 2 months (1,534 days). Its orbit has an eccentricity of 0.10 and an inclination of 15° with respect to the ecliptic.

The body's observation arc begins 47 years prior to its official discovery observation with a precovery taken at Palomar Observatory in June 1950.

Physical characteristics

Two rotational lightcurves of Agostino were obtained in the R-band from photometric observations by astronomers at the Palomar Transient Factory in August 2010, and February 2012, respectively. Lightcurve analysis gave a rotation period of 6.3350 and 6.3225 hours with a respective brightness variation of 0.51 and 0.84 in magnitude (U=2/2).

According to the NEOWISE mission of NASA's space-based Wide-field Infrared Survey Explorer, Agostino measures 4.9 kilometers in diameter and its surface has an albedo of 0.23. The Collaborative Asteroid Lightcurve Link assumes an albedo of 0.21 – derived from 15 Eunomia, the family's largest member and namesake – and calculates a diameter of 4.6 kilometers with an absolute magnitude of 14.02.

Naming

This minor planet was named after Agostino Boattini (born 1932), the father of the discoverer. The approved naming citation was published by the Minor Planet Center on 9 May 2001 (M.P.C. 42673).

References

  1. ^ "JPL Small-Body Database Browser: 12848 Agostino (1997 NK10)" (2017-05-05 last obs.). Jet Propulsion Laboratory. Retrieved 24 June 2017.
  2. ^ Schmadel, Lutz D. (2007). "(12848) Agostino". Dictionary of Minor Planet Names – (12848) Agostino. Springer Berlin Heidelberg. p. 789. doi:10.1007/978-3-540-29925-7_8689. ISBN 978-3-540-00238-3.
  3. ^ "LCDB Data for (12848) Agostino". Asteroid Lightcurve Database (LCDB). Retrieved 2 May 2016.
  4. ^ 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 2 May 2016.
  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. ^ Waszczak, Adam; Chang, Chan-Kao; Ofek, Eran O.; Laher, Russ; Masci, Frank; Levitan, David; et al. (September 2015). "Asteroid Light Curves from the Palomar Transient Factory Survey: Rotation Periods and Phase Functions from Sparse Photometry". The Astronomical Journal. 150 (3): 35. arXiv:1504.04041. Bibcode:2015AJ....150...75W. doi:10.1088/0004-6256/150/3/75. Retrieved 2 May 2016.
  7. 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 2 May 2016.
  8. ^ "12848 Agostino (1997 NK10)". Minor Planet Center. Retrieved 2 May 2016.
  9. "MPC/MPO/MPS Archive". Minor Planet Center. Retrieved 2 May 2016.

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