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2433 Sootiyo

From Wikipedia, the free encyclopedia
Main-belt asteroid

2433 Sootiyo
Discovery[1]
Discovered byE. Bowell
Discovery siteAnderson Mesa Stn.
Discovery date5 April 1981
Designations
(2433) Sootiyo
Named after
"star boy"(Hopi language)[2]
1981 GJ · 1939 KA
1960 KA · 1969 QF
1974 VZ1 · 1978 SG6
1978 UL
main-belt · (middle)[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc63.40 yr (23,157 days)
Aphelion3.1849AU
Perihelion2.0276 AU
2.6062 AU
Eccentricity0.2220
4.21yr (1,537 days)
195.45°
0° 14m 3.48s / day
Inclination10.366°
188.27°
71.294°
Physical characteristics
Dimensions12.076±0.136 km[1][4]
12.946±0.103 km[5]
14.85±0.37 km[6]
14.89 km(calculated)[3]
7h[7][a]
7.2298±0.0002 h[8]
0.156±0.009[6]
0.20(assumed)[3]
0.2690±0.0630[5]
0.304±0.062[1][4]
LS[9] · S[3]
11.5[1][3][5] · 11.80[6] · 11.86±0.62[9]

2433 Sootiyo, provisional designation1981 GJ, is a stonyasteroid from the middle region of theasteroid belt, approximately 13 kilometers in diameter. It was discovered on 5 April 1981, by American astronomerEdward Bowell at Lowell'sAnderson Mesa Station near Flagstaff, Arizona.[10] The asteroid was named "Sootiya" meaning "star boy" in theHopi language.[2]

Orbit and classification

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Sootiyo orbits the Sun in thecentral main-belt at a distance of 2.0–3.2 AU once every 4 years and 3 months (1,537 days). Its orbit has aneccentricity of 0.22 and aninclination of 10° with respect to theecliptic.[1] The first usedprecovery was taken atPalomar Observatory in 1953, extending the asteroid'sobservation arc by 28 years prior to its discovery observation.[10]

Physical characteristics

[edit]

PanSTARRS photometric survey characterizedSootiyo as a LS-type, an intermediary between the stonyS-type and rareL-type asteroids.[9]

Rotation period

[edit]

French amateur astronomerRené Roy obtained a rotationallightcurve from photometric observations in October 2007. It gave arotation period of7.2298 hours with a brightness variation of 0.54magnitude (U=2+), superseding observations by Brazilian Cláudia Angeli and by the Spanish ECLA project, which both gave a period of 7 hours with an amplitude of 0.57 and 0.4 magnitude, respectively (U=1/2).[7][a]

Diameter and albedo

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According to the survey carried out by the JapaneseAkari satellite, the asteroid measures 14.9 kilometers in diameter and its surface has analbedo of 0.156,[6] while two different data sets from NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE mission give a diameter of 12.1 and 12.9 kilometers with an albedo of 0.269 and 0.304, respectively.[4][5]

TheCollaborative Asteroid Lightcurve Link agrees with the results obtained by Akari, assuming a standard albedo for stony asteroids of 0.20 and calculating a diameter of 14.9 kilometers with anabsolute magnitude of 11.5.[3]

Naming

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Thisminor planet is named "Sootiya" which means "star boy" in thelanguage of theHopi Tribe of northern Arizona. Correspondingly, the Vestian asteroid2432 Soomana stands for "star girl".[2] Naming citation was proposed by Michael Lomatewama and Ekkehart Malotki and published on 8 February 1982 (M.P.C. 6650).[11]

Notes

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  1. ^abECLA (2011) web: rotation period hours with a brightness amplitude of mag. Summary figures for (2433) Sootiyo atCollaborative Asteroid Lightcurve Link (CALL) andProyecto ECLA (Silvia Alonso Perez) (2011)

References

[edit]
  1. ^abcdef"JPL Small-Body Database Browser: 2433 Sootiyo (1981 GJ)" (2017-03-05 last obs.).Jet Propulsion Laboratory. Retrieved13 June 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(2433) Sootiyo".Dictionary of Minor Planet Names – (2433) Sootiyo.Springer Berlin Heidelberg. p. 198.doi:10.1007/978-3-540-29925-7_2434.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (2433) Sootiyo". Asteroid Lightcurve Database (LCDB). Retrieved1 September 2016.
  4. ^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. Retrieved1 September 2016.
  5. ^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.
  6. ^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)
  7. ^abAngeli, C. A.; Guimarã; es, T. A.; Lazzaro, D.; Duffard, R.; Fernández, S.; et al. (April 2001)."Rotation Periods for Small Main-Belt Asteroids From CCD Photometry".The Astronomical Journal.121 (4):2245–2252.Bibcode:2001AJ....121.2245A.doi:10.1086/319936. Retrieved1 September 2016.
  8. ^Behrend, Raoul."Asteroids and comets rotation curves – (2433) Sootiyo".Geneva Observatory. Retrieved1 September 2016.
  9. ^abcVeres, 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. Retrieved1 September 2016.
  10. ^ab"2433 Sootiyo (1981 GJ)".Minor Planet Center. Retrieved1 September 2016.
  11. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved1 September 2016.

External links

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