Astronomy:1518 Rovaniemi

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1518 Rovaniemi
1518Rovaniemi (Lightcurve Inversion).png
Lightcurve-based 3D-model of Rovaniemi
Discovery[1]
Discovered byY. Väisälä
Discovery siteTurku Obs.
Discovery date15 October 1938
Designations
(1518) Rovaniemi
Named afterRovaniemi (Finnish city)[2]
1938 UA · 1928 TL
1951 SH
Minor planet categorymain-belt · (inner)
Flora[3][4]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc88.74 yr (32,412 days)
|{{{apsis}}}|helion}}2.5449 AU
|{{{apsis}}}|helion}}1.9053 AU
2.2251 AU
Eccentricity0.1437
Orbital period3.32 yr (1,212 days)
Mean anomaly246.56°
Mean motion0° 17m 49.2s / day
Inclination6.7137°
Longitude of ascending node27.804°
37.101°
Physical characteristics
Dimensions7.46±1.30 km[5]
7.76±0.71 km[6]
8.480±0.167 km[7]
8.98 km (calculated)[3]
9.019±0.070 km[8]
Rotation period5.247±0.001 h[9]
5.249±0.002 h[10]
Geometric albedo0.24 (assumed)[3]
0.2631±0.0374[8]
0.295±0.063[7]
0.31±0.17[5]
0.340±0.195[6]
S[3]
Absolute magnitude (H)12.3[8] · 12.34[6] · 12.4[1][3] · 12.68[5]


1518 Rovaniemi, provisional designation 1938 UA, is a stony Florian asteroid from the inner regions of the asteroid belt, approximately 8 kilometers in diameter. Discovered by Yrjö Väisälä at the Turku Observatory in 1938, the asteroid was later named after the Finnish city of Rovaniemi.

Discovery

Rovaniemi was discovered on 15 October 1938, by Finnish astronomer Yrjö Väisälä at the Turku Observatory in Southwest Finland. Six nights later, it was independently discovered by Belgian astronomer Eugène Delporte at Uccle Observatory on 21 October 1938. The Minor Planet Center, however, only recognizes the first discoverer.[2][11]

The asteroid was first identified as 1928 TL at Simeiz Observatory on 7 October 1928.[lower-alpha 1] The body's observation arc begins two weeks later at Simeiz on 21 October 1928, almost 10 years prior to the asteroid's official discovery observation at Turku.[11]

Orbit and classification

Rovaniemi is a member of the Flora family (402), a giant asteroid family and the largest family of stony asteroids in the main-belt.[3][4][12]:23 It orbits the Sun in the inner main-belt at a distance of 1.9–2.5 AU once every 3 years and 4 months (1,212 days). Its orbit has an eccentricity of 0.14 and an inclination of 7° with respect to the ecliptic.[1]

Physical characteristics

Rovaniemi is an assumed stony S-type asteroid,[3] which corresponds to the overall spectral type of the Flora family.[12]:23

Rotation period

In January 2009, two rotational lightcurves of Rovaniemi were obtained from photometric observations by René Roy at Blauvac Observatory (627) in France, and by Brian Warner at the Palmer Divide Observatory (716) in Colorado, United States. Lightcurve analysis gave a rotation period of 5.247 and 5.249 hours with a brightness amplitude of 0.26 and 0.25 magnitude, respectively ({{{1}}}).[9][10]

Spin axis

In 2013, an international study modeled a lightcurve from various data sources including the Uppsala Asteroid Photometric Catalogue and the Palomar Transient Factory survey. The lightcurve gave a concurring period of 5.25047 hours and allowed for the determination of two spin axis of (62.0°, 60.0°) and (265.0°, 45.0°) in ecliptic coordinates (λ, β).[13]

Diameter and albedo

According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Rovaniemi measures between 7.46 and 9.019 kilometers in diameter and its surface has an albedo between 0.2631 and 0.340.[5][6][7][8]

The Collaborative Asteroid Lightcurve Link assumes an albedo of 0.24 – derived from 8 Flora, the Flora family's largest member and namesake – and calculates a diameter of 8.98 kilometers based on an absolute magnitude of 12.4.[3]

Naming

This minor planet was named after the Finnish city of Rovaniemi, located just six kilometers south of the Arctic Circle.[2] The official naming citation was published by the Minor Planet Center on 20 February 1976 (M.P.C. 3929).[14]

Notes

  1. ↑ Alternatively to the Simeiz Observatory, it is also possible that observations at the Italian Turin Observatory on 13 and 14 October 1928, lead to the assignment of Rovaniemi's first provisional designation, 1928 TL.

References

  1. ↑ 1.0 1.1 1.2 1.3 "JPL Small-Body Database Browser: 1518 Rovaniemi (1938 UA)". Jet Propulsion Laboratory. https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2001518. 
  2. ↑ 2.0 2.1 2.2 Schmadel, Lutz D. (2007). "(1518) Rovaniemi". Dictionary of Minor Planet Names. Springer Berlin Heidelberg. p. 121. doi:10.1007/978-3-540-29925-7_1519. ISBN 978-3-540-00238-3. 
  3. ↑ 3.0 3.1 3.2 3.3 3.4 3.5 3.6 3.7 "LCDB Data for (1518) Rovaniemi". Asteroid Lightcurve Database (LCDB). http://www.minorplanet.info/PHP/generateOneAsteroidInfo.php?AstInfo=1518%7CRovaniemi. 
  4. ↑ 4.0 4.1 "Asteroid 1518 Rovaniemi – Nesvorny HCM Asteroid Families V3.0". Small Bodies Data Ferret. https://sbntools.psi.edu/ferret/SimpleSearch/results.action?targetName=1518+Rovaniemi#Asteroid%201518%20RovaniemiEAR-A-VARGBDET-5-NESVORNYFAM-V3.0. 
  5. ↑ 5.0 5.1 5.2 5.3 Nugent, C. R.; Mainzer, A.; Bauer, J.; Cutri, R. M.; Kramer, E. A.; Grav, T. et al. (September 2016). "NEOWISE Reactivation Mission Year Two: Asteroid Diameters and Albedos". The Astronomical Journal 152 (3): 12. doi:10.3847/0004-6256/152/3/63. Bibcode: 2016AJ....152...63N. 
  6. ↑ 6.0 6.1 6.2 6.3 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. doi:10.1088/2041-8205/759/1/L8. Bibcode: 2012ApJ...759L...8M. http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2012ApJ...759L...8M. Retrieved 6 September 2017. 
  7. ↑ 7.0 7.1 7.2 Masiero, Joseph R.; Mainzer, A. K.; Grav, T.; Bauer, J. M.; Cutri, R. M.; Dailey, J. et al. (November 2011). "Main Belt Asteroids with WISE/NEOWISE. I. Preliminary Albedos and Diameters". The Astrophysical Journal 741 (2): 20. doi:10.1088/0004-637X/741/2/68. Bibcode: 2011ApJ...741...68M. http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2011ApJ...741...68M. Retrieved 6 September 2017. 
  8. ↑ 8.0 8.1 8.2 8.3 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. doi:10.1088/0004-637X/741/2/90. Bibcode: 2011ApJ...741...90M. 
  9. ↑ 9.0 9.1 Behrend, Raoul. "Asteroids and comets rotation curves – (1518) Rovaniemi". Geneva Observatory. http://obswww.unige.ch/~behrend/page4cou.html#001518. 
  10. ↑ 10.0 10.1 Warner, Brian D. (July 2009). "Asteroid Lightcurve Analysis at the Palmer Divide Observatory: 2008 December - 2009 March". The Minor Planet Bulletin 36 (3): 109–116. ISSN 1052-8091. Bibcode: 2009MPBu...36..109W. http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2009MPBu...36..109W. Retrieved 6 September 2017. 
  11. ↑ 11.0 11.1 "1518 Rovaniemi (1938 UA)". Minor Planet Center. https://www.minorplanetcenter.net/db_search/show_object?object_id=1518. 
  12. ↑ 12.0 12.1 Nesvorný, D.; Broz, M.; Carruba, V. (December 2014). "Identification and Dynamical Properties of Asteroid Families". Asteroids IV. pp. 297–321. doi:10.2458/azu_uapress_9780816532131-ch016. ISBN 978-0-8165-3213-1. Bibcode: 2015aste.book..297N. 
  13. ↑ Hanus, J.; Durech, J.; Broz, M.; Marciniak, A.; Warner, B. D.; Pilcher, F. et al. (March 2013). "Asteroids' physical models from combined dense and sparse photometry and scaling of the YORP effect by the observed obliquity distribution". Astronomy and Astrophysics 551: 16. doi:10.1051/0004-6361/201220701. Bibcode: 2013A&A...551A..67H. http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2013A&A...551A..67H. Retrieved 6 September 2017. 
  14. ↑ Schmadel, Lutz D. (2009). "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. 

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