2591 Dworetsky

2591 Dworetsky
Discovery [1]
Discovered by K. Reinmuth
Discovery site Heidelberg Obs.
Discovery date 2 August 1949
Designations
MPC designation 2591 Dworetsky
Named after
Michael Dworetsky
(British astronomer)[2]
1949 PS · 1929 RH1
1934 RD · 1949 QU
1952 DC1 · 1962 BD
1962 EH · 1969 OC
1973 GQ · 1975 TU4
1978 GX3 · 1979 OD14
1981 YL2 · 1982 BO
main-belt · (outer)[3]
Orbital characteristics[1]
Epoch 13 January 2016 (JD 2457400.5)
Uncertainty parameter 0
Observation arc 81.45 yr (29748 days)
Aphelion 3.0613 AU (457.96 Gm)
Perihelion 2.8158 AU (421.24 Gm)
2.9385 AU (439.59 Gm)
Eccentricity 0.041773
5.04 yr (1839.9 d)
119.20°
 11m 44.376s / day
Inclination 1.5431°
356.27°
273.79°
Earth MOID 1.79869 AU (269.080 Gm)
Jupiter MOID 1.96872 AU (294.516 Gm)
Jupiter Tisserand parameter 3.272
Physical characteristics
Dimensions 13.269±0.195 km[4]
15.60 km (calculated)[3]
12.77 h (0.532 d)[5]
0.2792±0.0310[4]
0.20 (assumed)[3]
S[3]
11.5[1]

    2591 Dworetsky, provisional designation 1949 PS, is a stony asteroid from the outer region of the asteroid belt, about 14 kilometers in diameter. It was discovered on 2 August 1949, by German astronomer Karl Reinmuth at the Heidelberg Observatory in southern Germany.[6]

    The S-type asteroid orbits the Sun at a distance of 2.8–3.1 AU once every 5.04 years (1,840 days). Its orbit shows an eccentricity of 0.04 and is nearly coplanar to the ecliptic, tilted by 2 degrees only. It has a rotation period of 12.8 hours[5] and an albedo of 0.28, based on observations made by Wide-field Infrared Survey Explorer.[4] The Collaborative Asteroid Lightcurve Link assumes a somewhat lower albedo of 0.20.[3]

    The minor planet was named in honor of British astronomer Michael M. Dworetsky, senior lecturer at University College London (UCL). He is an active member of the International Astronomical Union, affiliated to several divisions, including "Education, Outreach and Heritage".[7] His research involve the stellar abundances of the mercury group of elements and has also taken a large part in the development of the undergraduate astronomy degree program. The asteroid's name was proposed by Conrad Bardwell (also see 1615 Bardwell), who made the identifications involving this minor planet.[2]

    References

    1. 1 2 3 "JPL Small-Body Database Browser: 2591 Dworetsky (1949 PS)" (2015-11-15 last obs.). Jet Propulsion Laboratory. Retrieved 15 April 2016.
    2. 1 2 Schmadel, Lutz D. (2003). Dictionary of Minor Planet Names – (2591) Dworetsky. Springer Berlin Heidelberg. p. 211. ISBN 978-3-540-29925-7. Retrieved 10 December 2015.
    3. 1 2 3 4 5 "LCDB Data for (2591) Dworetsky". Asteroid Lightcurve Database (LCDB). Retrieved 10 December 2015.
    4. 1 2 3 Mainzer, 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:1109.6407Freely accessible. Bibcode:2011ApJ...741...90M. doi:10.1088/0004-637X/741/2/90. Retrieved 10 December 2015.
    5. 1 2 Behrend, Raoul. "Asteroids and comets rotation curves – (2591) Dworetsky". Geneva Observatory. Retrieved 10 December 2015.
    6. "2591 Dworetsky (1949 PS)". Minor Planet Center. Retrieved 10 December 2015.
    7. "Michael M. Dworetsky". International Astronomical Union (IAU). Retrieved 10 December 2015.

    External links


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