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7449 Döllen

From Wikipedia, the free encyclopedia
Main-belt asteroid

7449 Döllen
Discovery[1]
Discovered byK. Reinmuth
Discovery siteHeidelberg Obs.
Discovery date21 August 1949
Designations
(7449) Döllen
Named after
Wilhelm Döllen[1]
(German astronomer)
1949 QL · 1949 QZ
1969 TV3
main-belt[1][2] · (inner)
Flora[3][4]
Orbital characteristics[2]
Epoch 23 March 2018 (JD 2458200.5)
Uncertainty parameter 0
Observation arc68.68yr (25,085 d)
Aphelion2.6599AU
Perihelion1.7865 AU
2.2232 AU
Eccentricity0.1964
3.31 yr (1,211 d)
230.21°
0° 17m 50.28s / day
Inclination6.2648°
335.74°
26.045°
Physical characteristics
3.389±0.151 km[5][6]
3.74 km(calculated)[3]
10±2.0 h[7]
0.24(assumed)[3]
0.465±0.064[5][6]
S(Flora family)[3]
13.8[6]
14.3[2][3]

7449 Döllen, provisional designation1949 QL, is a stony Florianasteroid from the inner regions of theasteroid belt, approximately 3.5 kilometers (2.2 miles) in diameter. It was discovered on 21 August 1949, by German astronomerKarl Reinmuth at theHeidelberg Observatory in southwest Germany.[1] The likelyS-type asteroid has arotation period of 10 hours.[3] It was named after German astronomerWilhelm Döllen.[1]

Orbit and classification

[edit]

Döllen is a member of theFlora family (402),[4] a giantasteroid family and the largest family of stony asteroids in the main-belt.[8]

It orbits the Sun in theinner asteroid belt at a distance of 1.8–2.7 AU once every 3 years and 4 months (1,211 days;semi-major axis of 2.22 AU). Its orbit has aneccentricity of 0.20 and aninclination of 6° with respect to theecliptic.[2] The body'sobservation arc begins atLowell Observatory in Flagstaff, the night prior to its official discovery observation at Heidelberg.[1]

Physical characteristics

[edit]

Döllen is an assumedS-type asteroid,[3] which corresponds to the overallspectral type for Florian asteroids.[8]: 23 

Rotation period

[edit]

In September 2012, a rotationallightcurve ofDöllen was obtained fromphotometric observations by French amateur astronomerRené Roy. Lightcurve analysis gave a tentativerotation period of 10 hours with a brightness amplitude of 0.10magnitude (U=2-).[3][7]

Diameter and albedo

[edit]

According to the survey carried out by theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer,Döllen measures 3.389 kilometers in diameter and its surface has analbedo of 0.465,[5][6] while theCollaborative Asteroid Lightcurve Link assumes an albedo of 0.24 – derived from8 Flora, theparent body of the Flora family – and calculates a diameter of 3.74 kilometers based on anabsolute magnitude of 14.3.[3]

Naming

[edit]

Thisminor planet was named after German astronomerWilhelm Döllen (1820–1897), for his discussion on errors of heliometer observations. Döllen was an assistant ofFriedrich Georg Wilhelm von Struve at theDorpat Observatory (Tartu Observatory) in Estonia. He also worked on geodetic problems at thePulkovo Observatory near Saint Petersburg, Russia.[1] The official naming citation was suggested byLutz Schmadel and published by theMinor Planet Center on 6 August 2009 (M.P.C. 66724).[9]

References

[edit]
  1. ^abcdefg"7449 Dollen (1949 QL)".Minor Planet Center. Retrieved27 May 2018.
  2. ^abcd"JPL Small-Body Database Browser: 7449 Dollen (1949 QL)" (2018-04-25 last obs.).Jet Propulsion Laboratory. Retrieved27 May 2018.
  3. ^abcdefghi"LCDB Data for (7449) Döllen". Asteroid Lightcurve Database (LCDB). Retrieved27 May 2018.
  4. ^ab"Asteroid 7449 Döllen".Small Bodies Data Ferret. Retrieved27 May 2018.
  5. ^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.
  6. ^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. (catalog)
  7. ^abBehrend, Raoul."Asteroids and comets rotation curves – (7449) Döllen". Geneva Observatory. Retrieved27 May 2018.
  8. ^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.S2CID 119280014.
  9. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved27 May 2018.

External links

[edit]
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