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1113 Katja

From Wikipedia, the free encyclopedia
Background asteroid

1113 Katja
Discovery[1]
Discovered byP. Shajn
Discovery siteSimeiz Obs.
Discovery date15 August 1928
Designations
(1113) Katja
Named after
Ekaterina Iosko[2]
(assistant at Simeiz Observatory)
1928 QC · A909 DH
main-belt · (outer)[3]
background[4]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc108.74 yr (39,719 days)
Aphelion3.5537AU
Perihelion2.6687 AU
3.1112 AU
Eccentricity0.1422
5.49yr (2,004 days)
341.95°
0° 10m 46.56s / day
Inclination13.280°
324.54°
119.15°
Physical characteristics
Dimensions38.20±0.58 km[5]
38.50±2.0 km[6]
38.65 km(derived)[3]
44.792±0.626 km[7]
51.949±1.531 km[8]
18±1h[9]
18.42±0.02 h[9]
18.465±0.010 h[10]
18.47±0.05 h[9]
0.1144±0.0266[8]
0.168±0.026[7]
0.195±0.018[11]
0.2071±0.023[6]
0.211±0.008[5]
0.2253(derived)[3]
C(assumed)[3]
9.30[1][3][7] · 9.40[5][6][8] · 9.49±0.20[12]

1113 Katja (provisional designation1928 QC) is a backgroundasteroid from the outer regions of theasteroid belt, approximately 39 kilometers in diameter. It was discovered byPelageya Shajn at theSimeiz Observatory in 1928, and named after Ekaterina Iosko, a staff member at the discovering observatory.[2][13]

Discovery

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Katja was discovered on 15 August 1928, by Soviet astronomerPelageya Shajn at theSimeiz Observatory on the Crimean peninsula.[13] Nine nights later, it was independently discovered byMax Wolf at the GermanHeidelberg Observatory on 24 August 1928. TheMinor Planet Center only recognizes the first discoverer.[2] The asteroid was first observed asA909 DH at Heidelberg in February 1909.[13]

Orbit and classification

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Katja is a non-family asteroid of the main belt'sbackground population.[4] It orbits the Sun in theouter asteroid belt at a distance of 2.7–3.6 AU once every 5 years and 6 months (2,004 days;semi-major axis of 3.11 AU). Its orbit has aneccentricity of 0.14 and aninclination of 13° with respect to theecliptic.[1] The body'sobservation arc begins at Heidelberg, 10 days after its official discovery observation at Simeiz.[13]

Physical characteristics

[edit]

AlthoughKatja is an assumed, carbonaceousC-type asteroid, it is rather of stony composition due to its high albedo.[3]

Rotation period

[edit]

Between 2002 and 2011, several rotationallightcurves of Katja were obtained from photometric observations by French amateur astronomers Maurice Audejean,René Roy and Laurent Brunetto (U=2/2/2-).[9] Best rated lightcurve, however, was obtained at theSunflower (739), Blackberry (929) and Universidad de Monterrey (720) observatories in January 2002. Lightcurve analysis gave a well-defined synodicrotation period of 18.465 hours with a brightness amplitude of 0.17magnitude (U=3).[10]

Diameter and albedo

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According to the surveys carried out by the Infrared Astronomical SatelliteIRAS, the JapaneseAkari satellite and theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer, Katja measures between 38.20 and 51.949 kilometers in diameter and its surface has analbedo between 0.1144 and 0.211.[5][6][7][8][11]

TheCollaborative Asteroid Lightcurve Link derives an albedo of 0.2253 and a diameter of 38.65 kilometers based on anabsolute magnitude of 9.3.[3]

Naming

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Thisminor planet was named for Ekaterina ("Katja") Iosko, a laboratory assistant and orbit calculator at the discoveringSimeiz Observatory (AN 238, 149). She was the daughter of Iosif Gavrilovich Iosko, who also worked as a mechanician at the observatory.[2]

References

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  1. ^abcd"JPL Small-Body Database Browser: 1113 Katja (1928 QC)" (2017-11-25 last obs.).Jet Propulsion Laboratory. Retrieved26 January 2018.
  2. ^abcdSchmadel, Lutz D. (2007). "(1113) Katja".Dictionary of Minor Planet Names – (1113) Katja.Springer Berlin Heidelberg. p. 94.doi:10.1007/978-3-540-29925-7_1114.ISBN 978-3-540-00238-3.
  3. ^abcdefg"LCDB Data for (1113) Katja". Asteroid Lightcurve Database (LCDB). Retrieved26 January 2018.
  4. ^ab"Asteroid 1113 Katja – Proper Elements". AstDyS-2, Asteroids – Dynamic Site. Retrieved28 October 2019.
  5. ^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)
  6. ^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.
  7. ^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. Retrieved26 January 2018.
  8. ^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.
  9. ^abcdBehrend, Raoul."Asteroids and comets rotation curves – (1113) Katja". Geneva Observatory. Retrieved26 January 2018.
  10. ^abRobinson, L. E.; Sada, P. V.; Cooney, W. R. Jr. (September 2002)."CCD Photometry of Asteroid 1113 Katja".The Minor Planet Bulletin.29: 54.Bibcode:2002MPBu...29...54R. Retrieved26 January 2018.
  11. ^abMasiero, 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.
  12. ^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. Retrieved26 January 2018.
  13. ^abcd"1113 Katja (1928 QC)".Minor Planet Center. Retrieved26 January 2018.

External links

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