Astronomy:120375 Kugel

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120375 Kugel
Discovery[1]
Discovered byC. Rinner
Discovery siteOttmarsheim Obs.
Discovery date10 August 2005
Designations
(120375) Kugel
Named afterFrançois Kugel[1]
(French astronomer)
2005 PB6 · 1998 SM108
2001 KE74
Minor planet categorymain-belt[1][2] · (inner)
background[3][4] · near-Flora[5]
Orbital characteristics[2]
Epoch 1 July 2021 (JD 2459396.5)
Uncertainty parameter 0
Observation arc22.53 yr (8,228 d)
|{{{apsis}}}|helion}}2.8289 AU
|{{{apsis}}}|helion}}1.8077 AU
2.3183 AU
Eccentricity0.2202
Orbital period3.53 yr (1,289 d)
Mean anomaly189.77°
Mean motion0° 16m 45.12s / day
Inclination2.7591°
Longitude of ascending node229.91°
97.616°
Physical characteristics
Mean diameter1.05 km (calculated)[5]
Rotation period6.923±0.0085 h[6]
Geometric albedo0.24 (assumed)[5]
S/Q (SDSS-MOC)[7]
Absolute magnitude (H)16.619±0.003 (R)[6]
16.7[2] · 17.07[5]


120375 Kugel, provisional designation: 2005 PB6, is a background asteroid from the inner regions of the asteroid belt, approximately 1 kilometer (0.6 miles) in diameter. It was discovered on 10 August 2005, by French amateur astronomer Claudine Rinner at her Ottmarsheim Observatory (224) in France.[1] The stony S/Q-type asteroid in the region of the Florian clan has a tentative rotation period of 6.9 hours.[5] It was named after French astronomer François Kugel.[1]

Orbit and classification

Kugel is a non-family asteroid of the main belt's background population when applying the hierarchical clustering method to its proper orbital elements.[3][4] Based on osculating Keplerian orbital elements, the asteroid has also been considered a member of the Flora family (402), a giant asteroid clan and the largest family of stony asteroids in the main belt.[5]

It orbits the Sun in the inner asteroid belt at a distance of 1.8–2.8 AU once every 3 years and 6 months (1,289 days; semi-major axis of 2.32 AU). Its orbit has an eccentricity of 0.22 and an inclination of 3° with respect to the ecliptic.[2] The body's observation arc begins with its first observation as 1998 SM108 at Lincoln Laboratory ETS in September 1998, nearly 7 years prior to its official discovery observation at Ottmarsheim.[1]

Naming

This minor planet was named after French amateur astronomer François Kugel (born 1959), an active observer of comets and a collaborator of the discoverer. He has founded the Chante-Perdrix Observatory (A77) in 2005.[1] The official naming citation was published by the Minor Planet Center on 6 August 2009 (M.P.C. 66728).[8]

Physical characteristics

In the SDSS-based taxonomy, Kugel has an SQ-type that transitions between the common S-type and less common Q-type asteroids.[7]

Rotation period

In August 2012, a rotational lightcurve of Kugel was obtained from photometric observations in the R-band by astronomers at the Palomar Transient Factory in California. Lightcurve analysis gave a tentative rotation period of 6.923±0.0085 hours with a weak brightness amplitude of 0.09 magnitude ({{{1}}}).[6] As of 2021, no secure period has been obtained.[5]

Diameter and albedo

Kugel has not been observed by any of the space-based surveys such as the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, the Akari satellite or IRAS. The Collaborative Asteroid Lightcurve Link assumes an albedo of 0.24 – derived from 8 Flora the parent body of the Flora family – and calculates a diameter of 1.05 kilometers based on an absolute magnitude of 17.07.[5]

References

  1. 1.0 1.1 1.2 1.3 1.4 1.5 1.6 "120375 Kugel (2005 PB6)". Minor Planet Center. https://www.minorplanetcenter.net/db_search/show_object?object_id=120375. Retrieved 4 April 2018. 
  2. 2.0 2.1 2.2 2.3 "JPL Small-Body Database Browser: 120375 Kugel (2005 PB6)". Jet Propulsion Laboratory. https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2120375. Retrieved 4 April 2018. 
  3. 3.0 3.1 "Asteroid 120375 Kugel – Nesvorny HCM Asteroid Families V3.0". Small Bodies Data Ferret. https://sbntools.psi.edu/ferret/SimpleSearch/results.action?targetName=120375+Kugel. Retrieved 15 July 2021. 
  4. 4.0 4.1 "Asteroid 120375 Kugel – Proper Elements". AstDyS-2, Asteroids – Dynamic Site. https://newton.spacedys.com/astdys/index.php?pc=1.1.6&n=120375. 
  5. 5.0 5.1 5.2 5.3 5.4 5.5 5.6 5.7 "LCDB Data for (120375) Kugel". Asteroid Lightcurve Database (LCDB). http://www.minorplanet.info/PHP/generateOneAsteroidInfo.php?AstInfo=120375%7CKugel. Retrieved 4 April 2018. 
  6. 6.0 6.1 6.2 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. doi:10.1088/0004-6256/150/3/75. Bibcode2015AJ....150...75W. http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2015AJ....150...75W. Retrieved 4 April 2018. 
  7. 7.0 7.1 Carvano, J. M.; Hasselmann, P. H.; Lazzaro, D.; Mothé-Diniz, T. (February 2010). "SDSS-based taxonomic classification and orbital distribution of main belt asteroids". Astronomy and Astrophysics 510: 12. doi:10.1051/0004-6361/200913322. Bibcode2010A&A...510A..43C. https://sbnarchive.psi.edu/pds3/non_mission/EAR_A_I0035_5_SDSSTAX_V1_1/data/sdsstax_ast_table.tab. Retrieved 15 July 2021.  (PDS data set)
  8. "MPC/MPO/MPS Archive". Minor Planet Center. https://www.minorplanetcenter.net/iau/ECS/MPCArchive/MPCArchive_TBL.html. Retrieved 4 April 2018. 

External links