1889 Pakhmutova

1889 Pakhmutova

A three-dimensional model of 1889 Pakhmutova based on its light curve.
Discovery [1]
Discovered by L. Chernykh
Discovery site CrAO - Nauchnyj
Discovery date 24 January 1968
Designations
MPC designation 1889 Pakhmutova
Named after
 Aleksandra Pakhmutova
(composer)[2]
1968 BE · 1942 JM
1966 US · 1969 JM
main-belt · (outer) [3]
Orbital characteristics [1]
Epoch 13 January 2016 (JD 2457400.5)
Uncertainty parameter 0
Observation arc 49.38 yr (18037 days)
Aphelion 3.4326 AU (513.51 Gm)
Perihelion 2.7456 AU (410.74 Gm)
3.0891 AU (462.12 Gm)
Eccentricity 0.11120
5.43 yr (1983.1 d)
284.43°
0° 10m 53.508s / day
Inclination 13.182°
55.160°
84.379°
Earth MOID 1.79881 AU (269.098 Gm)
Jupiter MOID 1.76283 AU (263.716 Gm)
Jupiter Tisserand parameter 3.176
Physical characteristics
Dimensions 33.53 km[4]
37.47±0.84 km[5]
35.24±0.63 km[6]
33.45 km (derived)[3]
Mean radius
 16.765 ± 0.9 km
17.490 h (0.7288 d)[1][7]
17.5157±0.0005 h[8]
17.5226±0.0113 h[9]
0.0752[4]
0.061±0.003[5]
0.057±0.013[6]
0.0629 (derived)[3]
0.0752 ± 0.009[1]
C [3]
11.1

    1889 Pakhmutova, provisional designation 1968 BE, is a dark, carbonaceous asteroid from the outer region of the asteroid belt, about 34 kilometers in diameter. It was discovered by Russian astronomer Lyudmila Chernykh at the Crimean Astrophysical Observatory in Nauchnyj on 24 January 1968.[10]

    The C-type asteroid orbits the Sun at a distance of 2.7–3.4 AU once every 5 years and 5 months (1,984 days). Its orbit shows an eccentricity of 0.11 and is inclined by 13 degrees to the plane of the ecliptic. It has a well-defined rotation period of 17.5 hours.[7][8][9] Its albedo is in the range of 0.06–0.08, as measured by the Akari, IRAS and WISE/NEOWISE surveys.[4][5][6]

    The asteroid is named in honor of the Russian composer Aleksandra Pakhmutova, one of the best known figures in Soviet and later Russian popular music.[2]

    References

    1. 1 2 3 4 "JPL Small-Body Database Browser: 1889 Pakhmutova (1968 BE)" (2015-10-22 last obs.). Jet Propulsion Laboratory. Retrieved 20 April 2016.
    2. 1 2 Schmadel, Lutz D. (2003). Dictionary of Minor Planet Names – (1889) Pakhmutova. Springer Berlin Heidelberg. p. 151. ISBN 978-3-540-29925-7. Retrieved November 2015.
    3. 1 2 3 4 "LCDB Data for (1889) Pakhmutova". Asteroid Lightcurve Database (LCDB). Retrieved November 2015.
    4. 1 2 3 Tedesco, E. F.; Noah, P. V.; Noah, M.; Price, S. D. (October 2004). "IRAS Minor Planet Survey V6.0". NASA Planetary Data System. Bibcode:2004PDSS...12.....T. Retrieved November 2015.
    5. 1 2 3 Usui, Fumihiko; Kuroda, Daisuke; Müller, Thomas G.; Hasegawa, Sunao; Ishiguro, Masateru; Ootsubo, Takafumi; et al. (October 2011). "Asteroid Catalog Using Akari: AKARI/IRC Mid-Infrared Asteroid Survey". Publications of the Astronomical Society of Japan 63 (5): 1117–1138. Bibcode:2011PASJ...63.1117U. doi:10.1093/pasj/63.5.1117. Retrieved November 2015.
    6. 1 2 3 Masiero, Joseph R.; Mainzer, A. K.; Grav, T.; Bauer, J. M.; Cutri, R. M.; Nugent, C.; Cabrera, M. S. (November 2012). "Preliminary Analysis of WISE/NEOWISE 3-Band Cryogenic and Post-cryogenic Observations of Main Belt Asteroids". The Astrophysical Journal Letters 759 (1): 5. arXiv:1209.5794. Bibcode:2012ApJ...759L...8M. doi:10.1088/2041-8205/759/1/L8. Retrieved November 2015.
    7. 1 2 Warner, Brian D. (December 2006). "Asteroid lightcurve analysis at the Palmer Divide Observatory - February - March 2006". The Minor Planet Bulletin 33 (4): 82–84. Bibcode:2006MPBu...33...82W. ISSN 1052-8091. Retrieved November 2015.
    8. 1 2 Hanus, J.; Durech, J.; Broz, M.; Warner, B. D.; Pilcher, F.; Stephens, R.; et al. (June 2011). "A study of asteroid pole-latitude distribution based on an extended set of shape models derived by the lightcurve inversion method". Astronomy & Astrophysics 530: 16. arXiv:1104.4114. Bibcode:2011A&A...530A.134H. doi:10.1051/0004-6361/201116738. Retrieved November 2015.
    9. 1 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. arXiv:1504.04041. Bibcode:2015AJ....150...75W. doi:10.1088/0004-6256/150/3/75. Retrieved November 2015.
    10. ↑ "1889 Pakhmutova (1968 BE)". Minor Planet Center. Retrieved November 2015.

    External links


    This article is issued from Wikipedia - version of the Wednesday, May 04, 2016. The text is available under the Creative Commons Attribution/Share Alike but additional terms may apply for the media files.