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1520 Imatra

From Wikipedia, the free encyclopedia
Main-belt asteroid

1520 Imatra
Discovery[1]
Discovered byY. Väisälä
Discovery siteTurku Obs.
Discovery date22 October 1938
Designations
(1520) Imatra
Named after
Imatra(Finnish town)[2]
1938 UY · 1938 YH
main-belt · (outer)[3]
Ursula[4]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc78.53 yr (28,682 days)
Aphelion3.4132AU
Perihelion2.8113 AU
3.1123 AU
Eccentricity0.0967
5.49yr (2,005 days)
179.71°
0° 10m 46.2s / day
Inclination15.241°
253.40°
116.83°
Physical characteristics
Dimensions53.41 km(derived)[3]
53.42±19.70 km[5]
53.435±0.370 km[6]
53.61±1.4 km[7]
53.79±14.73 km[8]
55.55±0.60 km[9]
56.094±1.824 km[10]
58.63±0.70 km[11]
5.23h(dated)[12]
18.609±0.004 h[13]
18.635±0.004 h[14]
0.039±0.009[11]
0.04±0.03[8]
0.0428(derived)[3]
0.05±0.06[5]
0.0561±0.0109[10]
0.058±0.002[9]
0.0615±0.003[7]
0.062±0.006[6]
SMASS =C[1] · C[3]
10.0[7][9][10] · 10.30[8][11] · 10.40±0.35[15] · 10.4[1][3] · 10.43[5]

1520 Imatra (provisional designation1938 UY) is a carbonaceous Ursulaasteroid from the outer region of theasteroid belt, approximately 54 kilometers in diameter. It was discovered on 22 October 1938, by Finnish astronomerYrjö Väisälä atTurku Observatory in Southwest Finland, who named after the Finnish town ofImatra.[2][16]

Orbit

[edit]

Imatra is a member of theUrsula family (631),[4] a largefamily ofC- andX-type asteroids, named after its parent body,375 Ursula.[17]: 23  It orbits the Sun in theouter main-belt at a distance of 2.8–3.4 AU once every 5 years and 6 months (2,005 days;semi-major axis of 3.11 AU). Its orbit has aneccentricity of 0.10 and aninclination of 15° with respect to theecliptic.[1] Noprecoveries and no prior identifications were made. Imatra'sobservation arc begins at Turku, 3 weeks after its official discovery observation.[16]

Physical characteristics

[edit]

Imatra is aC-type asteroid in theSMASS taxonomy.[1]

Rotation period

[edit]

In July 2008, American astronomerBrian Warner obtained a rotationallightcurve of Imatra at his Palmer Divide Observatory in Colorado. It gave arotation period of 18.635 hours with a brightness variation of 0.28magnitude (U=3-),[14] superseding a period of 5.23 hours from observations at Italian and French observatories in the 1990s (U=2).[12] In September 2014, photometric observations by French amateur astronomersLaurent Bernasconi, Romain Montaigut and Arnaud Leroy gave a period of 18.609 hours with an amplitude of 0.27 magnitude (U=2+).[13]

Diameter and albedo

[edit]

According to the surveys carried out by the Infrared Astronomical SatelliteIRAS, the JapaneseAkari satellite, and NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE mission, Imatra measures between 53.42 and 58.63 kilometers in diameter, and its surface has analbedo between 0.039 and 0.062.[5][6][7][8][9][10][11] TheCollaborative Asteroid Lightcurve Link derives an albedo of 0.0428 and a diameter of 53.41 kilometers using anabsolute magnitude of 10.4.[3]

Naming

[edit]

Thisminor planet is named for the south-eastern Finnish townImatra, located inSouth Karelia near the Russian border, about halfway betweenSt Petersburg and Finland's capitalHelsinki.[2] The officialnaming citation was published by theMinor Planet Center on 20 February 1976 (M.P.C. 3929).[18]

References

[edit]
  1. ^abcdef"JPL Small-Body Database Browser: 1520 Imatra (1938 UY)" (2017-05-02 last obs.).Jet Propulsion Laboratory. Retrieved5 June 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(1520) Imatra".Dictionary of Minor Planet Names.Springer Berlin Heidelberg. p. 121.doi:10.1007/978-3-540-29925-7_1521.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (1520) Imatra". Asteroid Lightcurve Database (LCDB). Retrieved3 January 2017.
  4. ^ab"Asteroid 1520 Imatra – Nesvorny HCM Asteroid Families V3.0".Small Bodies Data Ferret. Retrieved26 October 2019.
  5. ^abcdNugent, 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.arXiv:1606.08923.Bibcode:2016AJ....152...63N.doi:10.3847/0004-6256/152/3/63.
  6. ^abcMasiero, Joseph R.; Grav, T.; Mainzer, A. K.; Nugent, C. R.; Bauer, J. M.; Stevenson, R.; et al. (August 2014)."Main-belt Asteroids with WISE/NEOWISE: Near-infrared Albedos".The Astrophysical Journal.791 (2): 11.arXiv:1406.6645.Bibcode:2014ApJ...791..121M.doi:10.1088/0004-637X/791/2/121. Retrieved3 January 2017.
  7. ^abcdTedesco, E. F.; Noah, P. V.; Noah, M.; Price, S. D. (October 2004)."IRAS Minor Planet Survey V6.0".NASA Planetary Data System.12: IRAS-A-FPA-3-RDR-IMPS-V6.0.Bibcode:2004PDSS...12.....T. Retrieved22 October 2019.
  8. ^abcdNugent, C. R.; Mainzer, A.; Masiero, J.; Bauer, J.; Cutri, R. M.; Grav, T.; et al. (December 2015)."NEOWISE Reactivation Mission Year One: Preliminary Asteroid Diameters and Albedos".The Astrophysical Journal.814 (2): 13.arXiv:1509.02522.Bibcode:2015ApJ...814..117N.doi:10.1088/0004-637X/814/2/117. Retrieved3 January 2017.
  9. ^abcdUsui, 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)
  10. ^abcdMainzer, 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.arXiv:1109.6407.Bibcode:2011ApJ...741...90M.doi:10.1088/0004-637X/741/2/90.
  11. ^abcdMasiero, 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. Retrieved3 January 2017.
  12. ^abde Sanctis, M. C.; Barucci, M. A.; Angeli, C. A.; Fulchignoni, M.; Burchi, R.; Angelini, P. (October 1994)."Photoelectric and CCD observations of 10 asteroids".Planetary and Space Science.42 (10):859–864.Bibcode:1994P&SS...42..859D.doi:10.1016/0032-0633(94)90066-3.ISSN 0032-0633. Retrieved3 January 2017.
  13. ^abBehrend, Raoul."Asteroids and comets rotation curves – (1520) Imatra".Geneva Observatory. Retrieved3 January 2017.
  14. ^abWarner, Brian D. (January 2009)."Asteroid Lightcurve Analysis at the Palmer Divide Observatory: 2008 May - September".The Minor Planet Bulletin.36 (1):7–13.Bibcode:2009MPBu...36....7W.ISSN 1052-8091. Retrieved3 January 2017.
  15. ^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. Retrieved3 January 2017.
  16. ^ab"1520 Imatra (1938 UY)".Minor Planet Center. Retrieved3 January 2017.
  17. ^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.
  18. ^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.

External links

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