Dark background asteroid of primitive composition
1330 Spiridonia , provisional designation 1925 DB , is a dark background asteroid of primitive composition, located in the outer regions of the asteroid belt , approximately 65 kilometers in diameter. It was discovered on 17 February 1925, by Soviet astronomer Vladimir Albitsky at the Simeiz Observatory on the Crimean peninsula.[ 16] The asteroid was named after the discoverer's brother-in-law, Spiridon Zaslavskij.[ 2]
Orbit and classification
Spiridonia is a non-family asteroid from the main belt's background population .[ 4] It orbits the Sun in the outer asteroid belt at a distance of 2.9–3.4 AU once every 5 years and 8 months (2,061 days; semi-major axis of 3.17 AU). Its orbit has an eccentricity of 0.08 and an inclination of 16° with respect to the ecliptic .[ 1]
The asteroid was first identified as A922 SA at Heidelberg Observatory in September 1922. The body's observation arc begins at Yerkes Observatory in October 1934, more than 9 years after its official discovery observation at Simeiz.[ 16]
Physical characteristics
In the Tholen classification , Spiridonia is a primitive P-type asteroid .[ 1] [ 3]
Rotation period
Several rotational lightcurves of Spiridonia have been obtained from photometric observations since 2004.[ 12] [ 13] [ 14] Analysis of the best-rated lightcurve by American photometrist Robert Stephens at the Santana Observatory (646 ) from April 2005, gave a rotation period of 9.67 hours with a brightness amplitude of 0.16 magnitude (U=3 ).[ 1] [ 13]
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 , Spiridonia measures between 50.73 and 78.496 kilometers in diameter and its surface has an albedo between 0.029 and 0.06.[ 5] [ 6] [ 7] [ 8] [ 9] [ 10] [ 11]
The Collaborative Asteroid Lightcurve Link derives an albedo of 0.0580 and a diameter of 55.17 kilometers based on an absolute magnitude of 10.0.[ 3]
1330 Spiridonia has been observed to occult 5 stars between 1993 and 2023.
Naming
This minor planet was named after the discoverer's brother-in-law, Spiridon Zaslavskij (1883–1942), who was also the uncle of Viktorovich Zaslavskij (1925–1944), after whom the discoverer named the asteroid 1030 Vitja .[ 2] The official naming citation was published by the Minor Planet Center on 15 July 1968 (M.P.C. 2882 ).[ 17]
References
^ a b c d e f g h i "JPL Small-Body Database Browser: 1330 Spiridonia (1925 DB)" (2017-11-02 last obs.). Jet Propulsion Laboratory . Retrieved 29 November 2017 .
^ a b c Schmadel, Lutz D. (2007). "(1330) Spiridonia". Dictionary of Minor Planet Names – (1330) Spiridonia . Springer Berlin Heidelberg . p. 108. doi :10.1007/978-3-540-29925-7_1331 . ISBN 978-3-540-00238-3 .
^ a b c d e f g "LCDB Data for (1330) Spiridonia" . Asteroid Lightcurve Database (LCDB). Retrieved 29 November 2017 .
^ a b "Asteroid 1330 Spiridonia – Proper Elements" . AstDyS-2, Asteroids – Dynamic Site. Retrieved 29 October 2019 .
^ a b c d Nugent, 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 . S2CID 9341381 . Retrieved 29 November 2017 .
^ a b c d 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. arXiv :1606.08923 . Bibcode :2016AJ....152...63N . doi :10.3847/0004-6256/152/3/63 .
^ 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 .
^ a b c Masiero, 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 . S2CID 119293330 .
^ a b c d 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. arXiv :1109.6407 . Bibcode :2011ApJ...741...90M . doi :10.1088/0004-637X/741/2/90 . S2CID 35447010 .
^ 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 )
^ a b c d Masiero, Joseph R.; Nugent, C.; Mainzer, A. K.; Wright, E. L.; Bauer, J. M.; Cutri, R. M.; et al. (October 2017). "NEOWISE Reactivation Mission Year Three: Asteroid Diameters and Albedos" . The Astronomical Journal . 154 (4): 10. arXiv :1708.09504 . Bibcode :2017AJ....154..168M . doi :10.3847/1538-3881/aa89ec .
^ a b Stephens, Robert D. (January 2013). "Asteroids Observed from Santana and CS3 Observatories: 2012 July - September" . The Minor Planet Bulletin . 40 (1): 34– 35. Bibcode :2013MPBu...40...34S . ISSN 1052-8091 . Retrieved 29 November 2017 .
^ a b c Stephens, Robert D. (September 2005). "Asteroid lightcurve photometry from Santana Observatory - winter 2005" . The Minor Planet Bulletin . 32 (3): 66– 68. Bibcode :2005MPBu...32...66S . ISSN 1052-8091 . Retrieved 29 November 2017 .
^ a b c d Behrend, Raoul. "Asteroids and comets rotation curves – (1330) Spiridonia" . Geneva Observatory. Retrieved 29 November 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 . S2CID 53493339 . Retrieved 29 November 2017 .
^ a b "1330 Spiridonia (1925 DB)" . Minor Planet Center . Retrieved 29 November 2017 .
^ 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. Bibcode :2009dmpn.book.....S . doi :10.1007/978-3-642-01965-4 . ISBN 978-3-642-01964-7 .
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