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12848 Agostino

From Wikipedia, the free encyclopedia
Main-belt asteroid

12848 Agostino
Discovery[1]
Discovered byA. Boattini
Discovery siteCampo Imperatore
Discovery date10 July 1997
Designations
(12848) Agostino
Named after
Agostino Boattini
(discoverer's father)[2]
1997 NK10 · 1993 QQ10
main-belt · Eunomia[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc66.88 yr (24,428 days)
Aphelion2.8514AU
Perihelion2.3537 AU
2.6025 AU
Eccentricity0.0956
4.20yr (1,534 days)
183.78°
0° 14m 5.28s / day
Inclination15.066°
172.84°
249.89°
Physical characteristics
Dimensions4.55 km(calculated)[3]
4.864±0.120 km[4][5]
6.3225±0.0052h[6]
6.3350±0.0258 h[6]
0.21(assumed)[3]
0.225±0.033[4][5]
S[3]
13.6[1] · 13.54±0.32[7] · 13.8[4] · 13.537±0.006(R)[6] · 13.574±0.007(R)[6] · 14.02[3]

12848 Agostino, provisional designation1997 NK10, is a stony Eunomiaasteroid from the central region of theasteroid belt, approximately 5 kilometers in diameter.

The asteroid was discovered on 10 July 1997, by Italian astronomerAndrea Boattini at theCampo Imperatore Observatory in the Gran Sasso massif of central Italy.[8] It was named after the father of the discoverer, Agostino Boattini.[2]

Orbit and classification

[edit]

Agostino is a member of theEunomia family, a large group of stonyS-type asteroids and the most prominent family in theintermediate 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 aneccentricity of 0.10 and aninclination of 15° with respect to theecliptic.[1]

The body'sobservation arc begins 47 years prior to its official discovery observation with aprecovery taken atPalomar Observatory in June 1950.[8]

Physical characteristics

[edit]

Two rotationallightcurves ofAgostino were obtained in the R-band from photometric observations by astronomers at thePalomar Transient Factory in August 2010, and February 2012, respectively. Lightcurve analysis gave arotation period of6.3350 and6.3225 hours with a respective brightness variation of 0.51 and 0.84 inmagnitude (U=2/2).[6]

According to theNEOWISE mission of NASA's space-basedWide-field Infrared Survey Explorer,Agostino measures 4.9 kilometers in diameter and its surface has analbedo of 0.23.[4] TheCollaborative Asteroid Lightcurve Link assumes an albedo of 0.21 – derived from15 Eunomia, thefamily's largest member and namesake – and calculates a diameter of 4.6 kilometers with anabsolute magnitude of 14.02.[3]

Naming

[edit]

Thisminor planet was named after Agostino Boattini (born 1932), the father of the discoverer.[2] The approved naming citation was published by theMinor Planet Center on 9 May 2001 (M.P.C. 42673).[9]

References

[edit]
  1. ^abcd"JPL Small-Body Database Browser: 12848 Agostino (1997 NK10)" (2017-05-05 last obs.).Jet Propulsion Laboratory. Retrieved24 June 2017.
  2. ^abcSchmadel, 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. ^abcdef"LCDB Data for (12848) Agostino". Asteroid Lightcurve Database (LCDB). Retrieved2 May 2016.
  4. ^abcdMainzer, 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. Retrieved2 May 2016.
  5. ^abMasiero, 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. Retrieved3 December 2016.
  6. ^abcdeWaszczak, 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. Retrieved2 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. Retrieved2 May 2016.
  8. ^ab"12848 Agostino (1997 NK10)".Minor Planet Center. Retrieved2 May 2016.
  9. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved2 May 2016.

External links

[edit]
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