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7346 Boulanger

From Wikipedia, the free encyclopedia
Koronian asteroid from the outer regions of the asteroid belt

7346 Boulanger
Discovery[1]
Discovered byE. W. Elst
Discovery siteCERGA Obs.
Discovery date20 February 1993
Designations
(7346) Boulanger
Named after
Nicolas Boulanger
(French naturalist)
1993 DQ2 · 1981 UC16
1986 TK5 · 1986 TX10
1990 RN18
main-belt[1][2] · (outer)
Koronis[3]
Orbital characteristics[2]
Epoch 23 March 2018 (JD 2458200.5)
Uncertainty parameter 0
Observation arc63.01yr (23,016 d)
Aphelion3.1060AU
Perihelion2.6453 AU
2.8757 AU
Eccentricity0.0801
4.88 yr (1,781 d)
169.09°
0° 12m 7.56s / day
Inclination3.1808°
119.00°
254.01°
Physical characteristics
7.378±0.081 km[4]
0.270±0.066[4]
S(SDSS-MOC)[5]
12.8[1][2]

7346 Boulanger, provisional designation1993 DQ2, is a Koronianasteroid from the outer regions of theasteroid belt, approximately 7.4 kilometers (4.6 miles) in diameter. It was discovered on 20 February 1993, by Belgian astronomerEric Elst at theCERGA Observatory in Caussols, southeastern France. It was named after French Enlightenment philosopherNicolas Boulanger.[1]

Orbit and classification

[edit]

Boulanger is a member of theKoronis family (605),[3] a very large outerasteroid family with nearly co-planar ecliptical orbits.[6] It orbits the Sun in theouter main-belt at a distance of 2.6–3.1 AU once every 4 years and 11 months (1,781 days;semi-major axis of 2.88 AU). Its orbit has aneccentricity of 0.08 and aninclination of 3° with respect to theecliptic.[2]

The body'sobservation arc begins with aprecovery taken atPalomar Observatory in April 1955, nearly 38 years prior to its official discovery observation at Caussols.[1]

Physical characteristics

[edit]

In theSDSS-based taxonomy,Boulanger is a common, stonyS-type asteroid,[5] which agrees with the overallspectral type for Koronian asteroids.[6]: 23  It has anabsolute magnitude of 12.8.[1][2] As of 2018, no rotationallightcurve ofBoulanger has been obtained fromphotometric observations. The body'srotation period,pole and shape remain unknown.[2]

Diameter and albedo

[edit]

According to the survey carried out by theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer,Boulanger measures 7.378 kilometers in diameter and its surface has analbedo of 0.270.[4]

Naming

[edit]

Thisminor planet was named afterEnlightenment philosopher and geologistNicolas Antoine Boulanger (1722–1759).[1] The official naming citation was published by theMinor Planet Center on 24 June 2002 (M.P.C. 46008).[7]

References

[edit]
  1. ^abcdefg"7346 Boulanger (1993 DQ2)".Minor Planet Center. Retrieved27 May 2018.
  2. ^abcdef"JPL Small-Body Database Browser: 7346 Boulanger (1993 DQ2)" (2018-04-21 last obs.).Jet Propulsion Laboratory. Retrieved27 May 2018.
  3. ^ab"Asteroid 7346 Boulanger".Small Bodies Data Ferret. Retrieved27 May 2018.
  4. ^abcMasiero, 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.
  5. ^abCarvano, 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.Bibcode:2010A&A...510A..43C.doi:10.1051/0004-6361/200913322. Retrieved30 October 2019.(PDS data set)
  6. ^abNesvorný, D.; Broz, M.; Carruba, V. (December 2014). "Identification and Dynamical Properties of Asteroid Families".Asteroids IV. pp. 297–321.arXiv:1502.01628.Bibcode:2015aste.book..297N.doi:10.2458/azu_uapress_9780816532131-ch016.ISBN 9780816532131.
  7. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved27 May 2018.

External links

[edit]
Minor planets
Asteroid
Distant minor planet
Comets
Other
Authority control databasesEdit this at Wikidata
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