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1255 Schilowa

From Wikipedia, the free encyclopedia
Main-belt asteroid

1255 Schilowa
Discovery[1][2]
Discovered byG. Neujmin
Discovery siteSimeiz Obs.
Discovery date8 July 1932
Designations
(1255) Schilowa
Named after
Maria Zhilova
(Russian astronomer)
1932 NC · 1933 VB
A905 UC
main-belt · (outer)[3]
background[4]
Orbital characteristics[2]
Epoch 27 April 2019 (JD 2458600.5)
Uncertainty parameter 0
Observation arc113.54yr (41,472 d)
Aphelion3.6891AU
Perihelion2.5983 AU
3.1437 AU
Eccentricity0.1735
5.57 yr (2,036 d)
122.84°
0° 10m 36.48s / day
Inclination8.5473°
237.62°
133.51°
Physical characteristics
32.52±1.6 km[5]
33.669±0.718 km[6]
35.846±2.824 km[7]
36.49±0.51 km[8]
37.24±4.78 km[9]
29.536±0.006 h[3][10][11]
0.071±0.031[9]
0.111±0.004[8]
0.1144±0.0263[7]
0.130±0.027[6]
0.1389±0.015[5]
S(assumed)[3]
10.20[5][7][8]
10.3[1][2][3]
10.63[9]

1255 Schilowa, provisional designation1932 NC, is a backgroundasteroid from the outer regions of theasteroid belt, approximately 34 kilometers (21 miles) in diameter. It was discovered on 8 July 1932, by Soviet astronomerGrigory Neujmin at theSimeiz Observatory on the Crimean peninsula.[1] The asteroid has a longer-than averagerotation period of 29.5 hours. It was named afterMariya Zhilova (Schilowa), who was Russia's first professional female astronomer.[12]

Orbit and classification

[edit]

Schilowa is a non-family asteroid from the main belt'sbackground population.[4] It orbits the Sun in theouter main-belt at a distance of 2.6–3.7 AU once every 5 years and 7 months (2,036 days;semi-major axis of 3.14 AU). Its orbit has aneccentricity of 0.17 and aninclination of 9° with respect to theecliptic.[2]

The asteroid was first observed asA905 UC atHeidelberg Observatory in October 1905. The body'sobservation arc began one week later at Heidelberg in November 1905, almost 27 years prior to its official discovery observation at Simeiz.[1]

Naming

[edit]

Thisminor planet was named afterMariya Vasilyevna Zhilova (1870–1934), also known Mariya Shilova or Schilowa, a Russian astronomer at thePulkovo Observatory near Saint Petersburg. She was Russia's first professional female astronomer and awarded for her work oncelestial mechanics by the Russian Astronomical Society in 1905. The official naming citation was mentioned inThe Names of the Minor Planets byPaul Herget in 1955 (H 115).[12]

Physical characteristics

[edit]

Schilowa is an assumedS-type asteroid.[3]

Rotation period

[edit]

Between 2005 and 2009, three rotationallightcurves ofSchilowa were obtained from photometric observations by European astronomersPierre Antonini,Laurent Bernasconi,René Roy,Reiner Stoss,Jaime Nomen,Salvador Sánchez,Raoul Behrend. Lightcurve analysis gave arotation period of 29.536 hours (also 24 h and 29.7 h) with a brightness amplitude between 0.09 and 0.15magnitude (U=2 and 2/2-).[10]

Spin axis

[edit]

In 2013, an international study modeled a lightcurve from various data sources including the Uppsala Asteroid Photometric Catalogue and thePalomar Transient Factory survey. The lightcurve gave a sidereal period of 29.4674 hours and allowed for the determination of two spin axis of (156.0°, −4.0°) and (338.0°, 15.0°) inecliptic coordinates (λ, β).[13]

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,Schilowa measures between 32.52 and 37.24 kilometers in diameter and its surface has analbedo between 0.071 and 0.1389.[5][6][7][8][9] TheCollaborative Asteroid Lightcurve Link derives an albedo of 0.1273 and a diameter of 32.44 kilometers based on anabsolute magnitude of 10.3.[3]

References

[edit]
  1. ^abcd"1255 Schilowa (1932 NC)".Minor Planet Center. Retrieved4 November 2019.
  2. ^abcd"JPL Small-Body Database Browser: 1255 Schilowa (1932 NC)" (2019-05-11 last obs.).Jet Propulsion Laboratory. Retrieved4 November 2019.
  3. ^abcdef"LCDB Data for (1255) Schilowa". Asteroid Lightcurve Database (LCDB). Retrieved27 December 2017.
  4. ^ab"Asteroid 1255 Schilowa – Proper Elements". AstDyS-2, Asteroids – Dynamic Site. Retrieved29 October 2019.
  5. ^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.
  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.
  7. ^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.
  8. ^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)
  9. ^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. Retrieved27 December 2017.
  10. ^abBehrend, Raoul."Asteroids and comets rotation curves – (1255) Schilowa". Geneva Observatory. Retrieved27 December 2017.
  11. ^"Asteroid 1255 Schilowa".Small Bodies Data Ferret. Retrieved4 November 2019.
  12. ^abSchmadel, Lutz D. (2007). "(1255) Schilowa".Dictionary of Minor Planet Names – (1255) Schilowa.Springer Berlin Heidelberg. p. 104.doi:10.1007/978-3-540-29925-7_1256.ISBN 978-3-540-00238-3.
  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.arXiv:1301.6943.Bibcode:2013A&A...551A..67H.doi:10.1051/0004-6361/201220701.

External links

[edit]
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