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7548 Engström

From Wikipedia, the free encyclopedia
Main-belt asteroid

7548 Engström
Discovery[1]
Discovered byC.-I. Lagerkvist
Discovery siteLa Silla Obs.
Discovery date16 March 1980
Designations
(7548) Engström
Named after
Albert Engström
(Swedish artist)[2]
1980 FW2 · 1993 QA4
1999 TS324
main-belt · Themis[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc36.88 yr (13,470 days)
Aphelion3.6490AU
Perihelion2.6410 AU
3.1450 AU
Eccentricity0.1603
5.58yr (2,037 days)
151.48°
0° 10m 36.12s / day
Inclination0.3170°
346.66°
296.30°
Physical characteristics
Dimensions7.70 km(calculated)[3]
9.43±3.04 km[4]
11.067±0.129 km[5][6]
5.2309±0.0059h[7]
0.057±0.009[5][6]
0.06±0.05[4]
0.08(assumed)[3]
C[3]
13.5[1][5] · 13.93[3] · 13.477±0.005(R)[7] · 13.64±0.21[8] · 13.75[4]

7548 Engström, provisional designation1980 FW2, is dark Themistianasteroid from the outer region of theasteroid belt, approximately 9 kilometers in diameter. It was discovered on 16 March 1980, by Swedish astronomerClaes-Ingvar Lagerkvist atESO'sLa Silla Observatory site in northern Chile.[9] The asteroid was later named after Swedish artistAlbert Engström.[2]

Classification and orbit

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Engström is a member of theThemis family, a dynamical family ofouter-belt asteroids with nearly coplanarecliptical orbits. It orbits the Sun at a distance of 2.6–3.6 AU once every 5 years and 7 months (2,037 days). Its orbit has aneccentricity of 0.16 and aninclination of 0° with respect to the ecliptic.[1]

The asteroid'sobservation arc begins with its official discovery observation at La Silla.[9]

Physical characteristics

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Engström is an assumed carbonaceousC-type asteroid.[3]

Rotation period

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In September 2010,photometric observations by astronomers at thePalomar Transient Factory in California gave a rotationallightcurve with aperiod of5.2309 hours and a brightness amplitude of 0.35magnitude (U=2).[7]

Diameter and albedo

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According to the survey carried out by theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer,Engström measures 9.43 and 11.1 kilometers in diameter and its surface has a lowalbedo of 0.057 and 0.060, respectively,[5][6] while theCollaborative Asteroid Lightcurve Link (CALL) assumes an albedo of 0.08 and calculates a smaller diameter of 7.7 kilometers, based on anabsolute magnitude of 13.93.[3]

Naming

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Thisminor planet was named afterAlbert Engström (1869–1940), Swedish artist and author, who became a member of the esteemedSwedish academy in 1922. He was born in Lönneberga,Småland. After his studies of Greek and Latin atUppsala University, he went on toValand School of Fine Arts inGothenburg. Renowned painter of caricatures and founder of the humor magazineStrix, he is best known for his black and white illustrations.[2] The official naming citation was published on 11 April 1998 (M.P.C.31611).[10]

References

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  1. ^abcd"JPL Small-Body Database Browser: 7548 Engstrom (1980 FW2)" (2017-01-31 last obs.).Jet Propulsion Laboratory. Retrieved4 July 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(7548) Engström".Dictionary of Minor Planet Names – (7548) Engström.Springer Berlin Heidelberg. p. 603.doi:10.1007/978-3-540-29925-7_6547.ISBN 978-3-540-00238-3.
  3. ^abcdefg"LCDB Data for (7548) Engstrom". Asteroid Lightcurve Database (LCDB). Retrieved14 April 2016.
  4. ^abcNugent, C. R.; Mainzer, A.; Bauer, J.; Cutri, R. M.; Kramer, E. A.; Grav, T.; et al. (September 2016)."NEOWISE Reactivation Mission Year Two: Asteroid Diameters and Albedos".The Astronomical Journal.152 (3): 12.arXiv:1606.08923.Bibcode:2016AJ....152...63N.doi:10.3847/0004-6256/152/3/63.
  5. ^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.S2CID 35447010. Retrieved17 May 2016.
  6. ^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.S2CID 118745497. Retrieved4 December 2016.
  7. ^abcWaszczak, 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.S2CID 8342929. Retrieved17 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.S2CID 53493339. Retrieved17 May 2016.
  9. ^ab"7548 Engstrom (1980 FW2)".Minor Planet Center. Retrieved14 April 2016.
  10. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved17 May 2016.

External links

[edit]
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