1503 Kuopio
![]() Lightcurve-based 3D-model of Kuopio | |
Discovery [1] | |
---|---|
Discovered by | Y. Väisälä |
Discovery site | Turku Obs. |
Discovery date | 15 December 1938 |
Designations | |
(1503) Kuopio | |
Named after | Kuopio (Finnish town)[2] |
1938 XD · 1935 EF 1953 LH | |
Minor planet category | main-belt · (middle) Eunomia [3][4] |
Orbital characteristics [1] | |
Epoch 4 September 2017 (JD 2458000.5) | |
Uncertainty parameter 0 | |
Observation arc | 82.34 yr (30,075 days) |
Aphelion | 2.8995 AU |
Perihelion | 2.3499 AU |
2.6247 AU | |
Eccentricity | 0.1047 |
4.25 yr (1,553 days) | |
154.93° | |
0° 13m 54.48s / day | |
Inclination | 12.369° |
316.98° | |
177.92° | |
Physical characteristics | |
Dimensions | 18.43±1.5 km[5] 18.54 km (derived)[3] 22.33±0.34 km[6] 22.985±0.964 km[7] |
9.577±0.0004 h[8] 9.957±0.006 h[8] 9.9586±0.0005 h[9][10] 9.96±0.05 h[8] 9.98 h[11] | |
0.223±0.008[6] 0.2995±0.056[5] 0.3243 (derived)[3] 0.399±0.262[7] | |
S [3] | |
Absolute magnitude (H) | 9.81[7] · 10.5[1][3] · 10.60[5][6] · 10.65±0.69[12] |
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.[13] The asteroid was named for the Finnish town of Kuopio.[2]
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.[3][4][14]: 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.[1]
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.[13]
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).[8][11]
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.).[9][10]
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, Kuopio measures between 18.43 and 22.99 kilometers in diameter and its surface has an albedo between 0.223 and 0.399.[5][6][7]
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.[3]
Naming[]
This minor planet was named after the town of Kuopio in central Finland.[2] The official naming citation was published by the Minor Planet Center on 20 February 1976 (M.P.C. 3928).[15]
References[]
- ^ Jump up to: a b c d "JPL Small-Body Database Browser: 1503 Kuopio (1938 XD)" (2017-07-04 last obs.). Jet Propulsion Laboratory. Retrieved 8 September 2017.
- ^ Jump up to: a b c Schmadel, Lutz D. (2007). "(1503) Kuopio". Dictionary of Minor Planet Names – (1503) Kuopio. Springer Berlin Heidelberg. p. 120. doi:10.1007/978-3-540-29925-7_1504. ISBN 978-3-540-00238-3.
- ^ Jump up to: a b c d e f g "LCDB Data for (1503) Kuopio". Asteroid Lightcurve Database (LCDB). Retrieved 8 September 2017.
- ^ Jump up to: a b "Asteroid 1503 Kuopio – Nesvorny HCM Asteroid Families V3.0". Small Bodies Data Ferret. Retrieved 31 October 2019.
- ^ Jump up to: a b c d Tedesco, E. F.; Noah, P. V.; Noah, M.; Price, S. D. (October 2004). "IRAS Minor Planet Survey V6.0". NASA Planetary Data System – IRAS-A-FPA-3-RDR-IMPS-V6.0. Bibcode:2004PDSS...12.....T. Retrieved 17 October 2019.
- ^ Jump up to: a b c d 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. (online, AcuA catalog p. 153)
- ^ Jump up to: a b c d Masiero, Joseph R.; Mainzer, A. K.; Grav, T.; Bauer, J. M.; Cutri, R. M.; Nugent, C.; et al. (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 8 September 2017.
- ^ Jump up to: a b c d Behrend, Raoul. "Asteroids and comets rotation curves – (1503) Kuopio". Geneva Observatory. Retrieved 8 September 2017.
- ^ Jump up to: a b 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 8 September 2017.
- ^ Jump up to: a b Hanus, J.; Broz, M.; Durech, J.; Warner, B. D.; Brinsfield, J.; Durkee, R.; et al. (November 2013). "An anisotropic distribution of spin vectors in asteroid families". Astronomy and Astrophysics. 559: 19. arXiv:1309.4296. Bibcode:2013A&A...559A.134H. doi:10.1051/0004-6361/201321993. Retrieved 8 September 2017.
- ^ Jump up to: a b Székely, P.; Kiss, L. L.; Szabó, Gy. M.; Sárneczky, K.; Csák, B.; Váradi, M.; et al. (August 2005). "CCD photometry of 23 minor planets". Planetary and Space Science. 53 (9): 925–936. arXiv:astro-ph/0504462. Bibcode:2005P&SS...53..925S. doi:10.1016/j.pss.2005.04.006. Retrieved 8 September 2017.
- ^ Veres, Peter; Jedicke, Robert; Fitzsimmons, Alan; Denneau, Larry; Granvik, Mikael; Bolin, Bryce; et al. (November 2015). "Absolute magnitudes and slope parameters for 250,000 asteroids observed by Pan-STARRS PS1 - Preliminary results". Icarus. 261: 34–47. arXiv:1506.00762. Bibcode:2015Icar..261...34V. doi:10.1016/j.icarus.2015.08.007. Retrieved 8 September 2017.
- ^ Jump up to: a b "1503 Kuopio (1938 XD)". Minor Planet Center. Retrieved 8 September 2017.
- ^ Nesvorný, 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.
- ^ Schmadel, Lutz D. "Appendix – Publication Dates of the MPCs". Dictionary of Minor Planet Names – Addendum to Fifth Edition (2006–2008). Springer Berlin Heidelberg. p. 221. doi:10.1007/978-3-642-01965-4. ISBN 978-3-642-01964-7.
External links[]
- Asteroid Lightcurve Database (LCDB), query form (info Archived 16 December 2017 at the Wayback Machine)
- Dictionary of Minor Planet Names, Google books
- Asteroids and comets rotation curves, CdR – Observatoire de Genève, Raoul Behrend
- Discovery Circumstances: Numbered Minor Planets (1)-(5000) – Minor Planet Center
- 1503 Kuopio at AstDyS-2, Asteroids—Dynamic Site
- 1503 Kuopio at the JPL Small-Body Database
- Minor planet object articles (numbered)
- Eunomia asteroids
- Discoveries by Yrjö Väisälä
- Minor planets named for places
- Named minor planets
- Astronomical objects discovered in 1938