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1532 Inari

From Wikipedia, the free encyclopedia
Main-belt asteroid discovered on 1938-09-16 by Yrjö Väisälä at Turku

1532 Inari
Discovery[1]
Discovered byY. Väisälä
Discovery siteTurku Obs.
Discovery date16 September 1938
Designations
(1532) Inari
Named after
Lake Inari(Finnish lake)[2]
1938 SM · 1933 SZ
1935 BJ · 1936 FP1
main-belt · (outer)
Eos[3][4]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc80.74 yr (29,492 days)
Aphelion3.1618AU
Perihelion2.8486 AU
3.0052 AU
Eccentricity0.0521
5.21yr (1,903 days)
325.80°
0° 11m 21.12s / day
Inclination8.7769°
330.63°
122.85°
Physical characteristics
Dimensions24.439±0.056 km[5]
26.759±0.099 km[6]
28.38 km(derived)[3]
29.53±0.56 km[7]
30.39±3.24 km[8]
25h[9]
0.060±0.003[7]
0.0623±0.0080[6]
0.078±0.011[5]
0.087±0.039[8]
0.1049(derived)[3]
Tholen =S[1][3]
B–V = 0.840[1]
U–B = 0.360[1]
10.8[1][3] · 10.86[8] · 11.50[6][7]

1532 Inari (provisional designation1938 SM) is a stony Eoanasteroid from the outer regions of theasteroid belt, approximately 28 kilometers in diameter. Discovered byYrjö Väisälä atTurku Observatory in 1938, it was later named forLake Inari in northern Finland.[2]

Discovery

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Inari was discovered on 16 September 1938, by Finnish astronomerYrjö Väisälä at theIso-Heikkilä Observatory near Turku, Finland.[10] The asteroid was first identified as1933 SZ atSimeiz Observatory in September 1933, and itsobservation arc begins atNice Observatory in April 1936, more than two years prior to its official discovery observation at Turku.[10]

Orbit and classification

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Inari is a member theEos family (606),[4] one of the asteroid belt's largestfamilies with nearly 10,000 known asteroids.[11]: 23  It orbits the Sun in theouter main belt at a distance of 2.8–3.2 AU once every 5 years and 3 months (1,903 days). Its orbit has aneccentricity of 0.05 and aninclination of 9° with respect to theecliptic.[1]

Physical characteristics

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In theTholen classification,Saimaa is a featureless stonyS-type asteroid.[1][3] The overallspectral type for members of the Eos family is that of aK-type.[11]: 23 

Rotation period

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In January 2008, a fragmentary rotationallightcurve of Inari was obtained from photometric observations by French amateur astronomerRené Roy. Lightcurve analysis gave a longer-than-averagerotation period of 25 hours with a low brightness amplitude of 0.09magnitude (U=1+).[9] As of 2017, no secure period has been obtained.[3]

Diameter and albedo

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According to the surveys carried out by the JapaneseAkari satellite and theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer, Inari measures between 24.439 and 30.39 kilometers in diameter and its surface has analbedo between 0.060 and 0.087.[5][6][7][8] TheCollaborative Asteroid Lightcurve Link derives an albedo of 0.1049 and a diameter of 28.38 kilometers based on anabsolute magnitude of 10.8.[3]

Naming

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Thisminor planet was named afterLake Inari (Inarijärvi), located north of theArctic Circle inLapland, Finland. Lake Inari is the country'sthird-largest lake and one of thelargest lakes in Europe.[2]

The officialnaming citation was published by theMinor Planet Center on 20 February 1976 (M.P.C. 3929).[12]

References

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  1. ^abcdefgh"JPL Small-Body Database Browser: 1532 Inari (1938 SM)" (2017-01-09 last obs.).Jet Propulsion Laboratory. Retrieved9 October 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(1532) Inari".Dictionary of Minor Planet Names.Springer Berlin Heidelberg. p. 121.doi:10.1007/978-3-540-29925-7_1533.ISBN 978-3-540-00238-3.
  3. ^abcdefgh"LCDB Data for (1532) Inari". Asteroid Lightcurve Database (LCDB). Retrieved9 October 2017.
  4. ^ab"Asteroid 1532 Inari – Nesvorny HCM Asteroid Families V3.0".Small Bodies Data Ferret. Retrieved26 October 2019.
  5. ^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. Retrieved9 October 2017.
  6. ^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.
  7. ^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)
  8. ^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. Retrieved9 October 2017.
  9. ^abBehrend, Raoul."Asteroids and comets rotation curves – (1532) Inari".Geneva Observatory. Retrieved9 October 2017.
  10. ^ab"1532 Inari (1938 SM)".Minor Planet Center. Retrieved9 October 2017.
  11. ^abNesvorný, 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.
  12. ^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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