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1503 Kuopio
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Main-belt asteroid
October 2019
yes
1503 Kuopio
#D6D6D6
File:1503Kuopio (Lightcurve Inversion).png
Lightcurve-based 3D-model of Kuopio
Y. Väisälä
Turku Obs.
15 December 1938
(1503) Kuopio
1938 XD1935 EF1953 LH
Kuopio (Finnish town)
main-belt(middle)Eunomia
4 September 2017 (JD 2458000.5)
0
82.34 yr (30,075 days)
2.8995 AU
2.3499 AU
2.6247 AU
0.1047
4.25 yr (1,553 days)
154.93°
0.2318 ms / day
12.369°
316.98°
177.92°
18.43 1.5 km18.54 km (derived)22.33 0.34 km22.985 0.964 km
9.577 0.0004 h9.957 0.006 h9.9586 0.0005 h9.96 0.05 h9.98 h
0.223 0.0080.2995 0.0560.3243 (derived)0.399 0.262
S
9.8110.510.6010.65 0.69
1503 Kuopio (provisional designation 1938 XD) is a stony Eunomian asteroid from the central region of the asteroid belt, approximately 19 kilometers in diameter. It was discovered on 15 December 1938, by astronomer Yrjö Väisälä at the Turku Observatory in Southwest Finland. The asteroid was named for the Finnish town of Kuopio.
Orbit and classification
Kuopio is a member of the Eunomia family (502), a prominent family of stony S-type asteroid and the largest one in the intermediate main belt with more than 5,000 members.23 It orbits the Sun at a distance of 2.3–2.9 AU once every 4 years and 3 months (1,553 days). Its orbit has an eccentricity of 0.10 and an inclination of 12° with respect to the ecliptic plane.
The body's observation arc begins with its first identification as 1935 EF at Yerkes Observatory in March 1935, more than 3 years prior to its official discovery observation at Turku.
Physical characteristics
Rotation period
Several rotational lightcurves of Kuopio were obtained from photometric observations since 2001. Analysis of these lightcurves gave a rotation period between 9.577 and 9.98 hours with a brightness variation of 0.01 to 0.05 magnitude (U=3/3/2/2/3).
Poles
In 2011 and 2013, a modeled lightcurve using data from the Uppsala Asteroid Photometric Catalogue (UAPC) and other sources was published. In both studies, the modeled lightcurve gave a concurring period 9.9586 hours. The 2013-publication also determined two spin axis of (170.0°, −86.0°) and (27.0°, −61.0°) in ecliptic coordinates (λ, β) (U=n.a.).
Diameter and albedo
According to the surveys carried out by the Infrared Astronomical Satellite IRAS, the Japanese Akari satellite and the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer (WISE) program, Kuopio measures between 18.43 and 22.99 kilometers in diameter and its surface has an albedo between 0.223 and 0.399.
The Collaborative Asteroid Lightcurve Link derives an albedo of 0.3243 and a diameter of 18.54 kilometers based on an absolute magnitude of 10.5.
Naming
This minor planet was named after the town of Kuopio in central Finland. The official 1503 naming citation was published by the Minor Planet Center on 20 February 1976 (M.P.C. 3928).
References
30em 2017-07-04 last obs.
JPL Small-Body Database Browser: 1503 Kuopio (1938 XD)
https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2001503
Jet Propulsion Laboratory
8 September 2017
Schmadel Lutz D.
Dictionary of Minor Planet Names Springer Berlin Heidelberg
120
2007
978-3-540-00238-3
10.1007/978-3-540-29925-7_1504 (1503) Kuopio
1503 Kuopio (1938 XD)
Minor Planet Center
https://www.minorplanetcenter.net/db_search/show_object?object_id=1503
8 September 2017
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
Asteroids and comets rotation curves – (1503) Kuopio
Behrend
Raoul
Geneva Observatory
https://obswww.unige.ch/~behrend/page4cou.html#001503
8 September 2017 October 2026 InternetArchiveBot
Asteroid 1503 Kuopio – Nesvorny HCM Asteroid Families V3.0
Small Bodies Data Ferret
https://sbntools.psi.edu/ferret/SimpleSearch/results.action?targetName=1503+Kuopio#Asteroid%201503%20KuopioEAR-A-VARGBDET-5-NESVORNYFAM-V3.0
31 October 2019
https://web.archive.org/web/20200820060751/https://sbntools.psi.edu/ferret/SimpleSearch/results.action?targetName=1503+Kuopio#Asteroid%201503%20KuopioEAR-A-VARGBDET-5-NESVORNYFAM-V3.0
20 August 2020
dead
D. Nesvorný
M. Broz
V. Carruba
December 2014
Identification and Dynamical Properties of Asteroid Families
Asteroids IV
297–321
2015aste.book..297N
10.2458/azu_uapress_9780816532131-ch016
1502.01628
9780816532131
1503
8 September 2017
6
Joseph R. Masiero
A. K. Mainzer
T. Grav
J. M. Bauer
R. M. Cutri
C. Nugent
M. S. Cabrera
November 2012
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
8 September 2017
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
(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
P. Székely
L. L. Kiss
Gy. M. Szabó
K. Sárneczky
B. Csák
M. Váradi
Sz. Mészáros
August 2005
CCD photometry of 23 minor planets
http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2005P&SS...53..925S
Planetary and Space Science
53
9
925–936
2005P&SS...53..925S
10.1016/j.pss.2005.04.006
astro-ph/0504462
8 September 2017
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
8 September 2017
6
J. Hanus
M. Broz
J. Durech
B. D. Warner
J. Brinsfield
R. Durkee
D. Higgins
R. A. Koff
J. Oey
F. Pilcher
R. Stephens
L. P. Strabla
Q. Ulisse
R. Girelli
November 2013
An anisotropic distribution of spin vectors in asteroid families
http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2013A&A...559A.134H
Astronomy and Astrophysics
559
19
2013A&A...559A.134H
10.1051/0004-6361/201321993
1309.4296
8 September 2017
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
November 2015
Absolute magnitudes and slope parameters for 250,000 asteroids observed by Pan-STARRS PS1 - Preliminary results
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
8 September 2017
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/20241208174218/http://obswww.unige.ch/~behrend/page_cou.html 8 December 2024 – Observatoire de Genève, Raoul Behrend
Discovery Circumstances: Numbered Minor Planets (1)-(5000) – Minor Planet Center
1503
1502 Arenda 1503 1504 Lappeenranta
001503
Category:Discoveries by Yrjö Väisälä
Category:Named minor planets
19381215