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1889 Pakhmutova
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Carbonaceous main-belt asteroid
October 2019
yes
1889 Pakhmutova
#D6D6D6
1889Pakhmutova (Lightcurve Inversion).png
Lightcurve-based 3D-model of Pakhmutova padding: 5px 0; line-height: 1.3em;
24 January 1968
L. Chernykh
Crimean Astrophysical Obs.
(1889) Pakhmutova
1968 BE1942 JM1966 US1969 JM
Aleksandra Pakhmutova(Russian composer)
main-belt(outer)
4 September 2017 (JD 2458000.5)
0
50.53 yr (18,455 days)
3.4349 AU
2.7452 AU
3.0901 AU
0.1116
5.43 yr (1,984 days)
33.156°
0.1814 ms / day
13.183°
55.153°
84.606°
33.41 km (derived)33.53 1.8 km35.24 0.63 km35.45 10.87 km37.47 0.84 km37.68 14.19 km
17.490 0.004 hlightcurve-plot17.5157 0.0005 h17.5226 0.0113 h
0.05 0.040.057 0.0130.0574 (derived)0.06 0.090.061 0.0030.0752 0.009
C
10.8010.969 0.002 (R)11.011.111.1211.29 0.37
1889 Pakhmutova, provisional designation 1968 BE, is a carbonaceous asteroid from the outer region of the asteroid belt, approximately 35 kilometers in diameter.
It was discovered by Russian astronomer Lyudmila Chernykh at the Crimean Astrophysical Observatory in Nauchnyj on 24 January 1968. The asteroid was named after Russian composer Aleksandra Pakhmutova.
Orbit and classification
Pakhmutova orbits the Sun in the outer main-belt at a distance of 2.7–3.4 AU once every 5 years and 5 months (1,984 days). Its orbit has an eccentricity of 0.11 and an inclination of 13° with respect to the ecliptic. It was first identified as 1942 JM at Johannesburg Observatory in 1942. Its first used observation was made in 1968, when it was identified as 1966 US at the discovering observatory, extending the body's observation arc by 2 years prior to its official discovery observation.
Physical characteristics
Pakhmutova has been characterized as a carbonaceous C-type asteroid.
Diameter and albedo
This asteroid has a mean-diameter between 33.53 and 37.68 kilometers, and an albedo between 0.05 and 0.0752, as measured by the space-based Akari, IRAS and WISE/NEOWISE surveys. The Collaborative Asteroid Lightcurve Link derives an albedo of 0.0574 and a diameter of 33.41 kilometers with an absolute magnitude of 11.1.
Rotation period and poles
In February 2006, a rotational lightcurvelightcurve-plot was obtained by American astronomer Brian Warner at his Palmer Divide Observatory (716) in Colorado. Lightcurve analysis gave a rotation period of 17.490 hours with a brightness variation of 0.50 in magnitude (U=3-). Photometric observations at the Palomar Transient Factory in February 2012, gave a period of 17.5226 hours and an amplitude of 0.49 magnitude (U=2).
In 2011, a modeled lightcurve using data from the Uppsala Asteroid Photometric Catalogue (UAPC) and other sources gave a period 17.5157 hours, as well as a spin axis of (22.0°, –76.0°; 167.0°, –40.0°) in ecliptic coordinates (λ, β) (U=2).
Naming
This minor planet was named in honor of the Russian composer Aleksandra Pakhmutova, one of the best known figures in Soviet and later Russian popular music. The official 1889 naming citation was published by the Minor Planet Center on 20 February 1976 (M.P.C. 3936).
Notes
lightcurve-plot Lightcurve plot of 1889 Pakhmutova with a rotation period 17.490 0.004 hours with a brightness amplitude of 0.50 0.02 by B. D. Warner at the Palmer Divide Observatory (2006). Summary figures at LCDB
References
30em 2017-04-30 last obs.
JPL Small-Body Database Browser: 1889 Pakhmutova (1968 BE)
https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2001889
Jet Propulsion Laboratory
9 June 2017
Dictionary of Minor Planet Names – (1889) Pakhmutova
Schmadel Lutz D.
Springer Berlin Heidelberg
151
2007
978-3-540-00238-3
10.1007/978-3-540-29925-7_1890 (1889) Pakhmutova
1889 Pakhmutova (1968 BE)
Minor Planet Center
https://www.minorplanetcenter.net/db_search/show_object?object_id=1889
11 December 2016
Dictionary of Minor Planet Names – Addendum to Fifth Edition (2006–2008)
Appendix – Publication Dates of the MPCs
Schmadel Lutz D.
2009
Springer Berlin Heidelberg
221
978-3-642-01964-7
10.1007/978-3-642-01965-4 2009dmpn.book.....S
1889
11 December 2016
6
Fumihiko Usui
Daisuke Kuroda
Thomas G. Müller
Sunao Hasegawa
Masateru Ishiguro
Takafumi Ootsubo
Daisuke Ishihara
Hirokazu Kataza
Satoshi Takita
Shinki Oyabu
Munetaka Ueno
Hideo Matsuhara
Takashi Onaka
October 2011
Asteroid Catalog Using Akari: AKARI/IRC Mid-Infrared Asteroid Survey
Publications of the Astronomical Society of Japan
63
5
1117–1138
2011PASJ...63.1117U
10.1093/pasj/63.5.1117
free
(online, AcuA catalog p. 153)
E. F. Tedesco
P. V. Noah
M. Noah
S. D. Price
October 2004
IRAS Minor Planet Survey V6.0
https://sbnarchive.psi.edu/pds3/iras/IRAS_A_FPA_3_RDR_IMPS_V6_0/data/diamalb.tab
NASA Planetary Data System – IRAS-A-FPA-3-RDR-IMPS-V6.0
2004PDSS...12.....T
17 October 2019
6
Joseph R. Masiero
A. K. Mainzer
T. Grav
J. M. Bauer
R. M. Cutri
C. Nugent
M. S. Cabrera
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Preliminary Analysis of WISE/NEOWISE 3-Band Cryogenic and Post-cryogenic Observations of Main Belt Asteroids
http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2012ApJ...759L...8M
The Astrophysical Journal Letters
759
1
5
2012ApJ...759L...8M
10.1088/2041-8205/759/1/L8
1209.5794
46350317 11 December 2016
Warner, Brian D.
December 2006
Asteroid lightcurve analysis at the Palmer Divide Observatory - February - March 2006
http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2006MPBu...33...82W
The Minor Planet Bulletin
33
4
82–84
1052-8091
2006MPBu...33...82W
11 December 2016
6
Hanus, J.
Durech, J.
Broz, M.
Warner, B. D.
Pilcher, F.
Stephens, R.
Oey, J.
Bernasconi, L.
Casulli, S.
Behrend, R.
Polishook, D.
Henych, T.
Lehký, M.
Yoshida, F.
Ito, T.
June 2011
A study of asteroid pole-latitude distribution based on an extended set of shape models derived by the lightcurve inversion method
http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2011A&A...530A.134H
Astronomy & Astrophysics
530
16
2011A&A...530A.134H
10.1051/0004-6361/201116738
1104.4114
11 December 2016
6
Adam Waszczak
Chan-Kao Chang
Eran O. Ofek
Russ Laher
Frank Masci
David Levitan
Jason Surace
Yu-Chi Cheng
Wing-Huen Ip
Daisuke Kinoshita
George Helou
Thomas A. Prince
Shrinivas Kulkarni
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Asteroid Light Curves from the Palomar Transient Factory Survey: Rotation Periods and Phase Functions from Sparse Photometry
http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2015AJ....150...75W
The Astronomical Journal
150
3
35
2015AJ....150...75W
10.1088/0004-6256/150/3/75
1504.04041
8342929 11 December 2016
6
Peter Veres
Robert Jedicke
Alan Fitzsimmons
Larry Denneau
Mikael Granvik
Bryce Bolin
Serge Chastel
Richard J. Wainscoat
William S. Burgett
Kenneth C. Chambers
Heather Flewelling
Nick Kaiser
Eugen A. Magnier
Jeff S. Morgan
Paul A. Price
John L. Tonry
Christopher Waters
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http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2015Icar..261...34V
Icarus
261
34–47
2015Icar..261...34V
10.1016/j.icarus.2015.08.007
1506.00762
53493339 11 December 2016
6
C. R. Nugent
A. Mainzer
J. Masiero
J. Bauer
R. M. Cutri
T. Grav
E. Kramer
S. Sonnett
R. Stevenson
E. L. Wright
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NEOWISE Reactivation Mission Year One: Preliminary Asteroid Diameters and Albedos
http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2015ApJ...814..117N
The Astrophysical Journal
814
2
13
2015ApJ...814..117N
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1509.02522
9341381 9 June 2017
6
C. R. Nugent
A. Mainzer
J. Bauer
R. M. Cutri
E. A. Kramer
T. Grav
J. Masiero
S. Sonnett
E. L. Wright
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The Astronomical Journal
152
3
12
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External links
Asteroid Lightcurve Database (LCDB), query form (info https://web.archive.org/web/20171216050541/http://www.minorplanet.info/lightcurvedatabase.html 16 December 2017 )
Dictionary of Minor Planet Names, Google books
Asteroids and comets rotation curves, CdR https://web.archive.org/web/20160729213840/http://obswww.unige.ch/~behrend/page_cou.html 29 July 2016 – Observatoire de Genève, Raoul Behrend
Discovery Circumstances: Numbered Minor Planets (1)-(5000) – Minor Planet Center
1889
1888 Zu Chong-Zhi 1889 1890 Konoshenkova
001889
Category:Discoveries by Lyudmila Chernykh
Category:Named minor planets
19680124