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1460 Haltia

From Wikipedia, the free encyclopedia
Main-belt asteroid

1460 Haltia
Discovery[1]
Discovered byY. Väisälä
Discovery siteTurku Obs.
Discovery date24 November 1937
Designations
(1460) Haltia
Named after
Halti/Haltia[2]
(highest Finnish peak)
1937 WC
main-belt · (middle)
background[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc79.61 yr (29,077 days)
Aphelion3.0202AU
Perihelion2.0643 AU
2.5422 AU
Eccentricity0.1880
4.05yr (1,481 days)
245.72°
0° 14m 35.52s / day
Inclination6.6858°
74.185°
358.22°
Physical characteristics
Dimensions6.57±1.19 km[4]
7.43±0.61 km[5]
8.440±0.225 km[6]
8.97 km(calculated)[7]
3.58682±0.00006h[8]
3.588±0.005 h[8]
3.59 h[7]
0.186±0.032[5]
0.20(assumed)[7]
0.226±0.030[6]
0.36±0.15[4]
S(assumed)[7]
12.60[4][6][7] · 12.7[1] · 12.78±0.14[9] · 13.10[5]

1460 Haltia, provisional designation1937 WC, is a stony backgroundasteroid from the central regions of theasteroid belt, approximately 8 kilometers in diameter. It was discovered on 24 November 1937, by Finnish astronomerYrjö Väisälä at theIso-Heikkilä Observatory in Turku, Finland.[10] The asteroid was named afterHalti (Haltia), Finland's highest peak on the border to Norway.[2]

Orbit and classification

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Haltia is a non-family asteroid of the main belt'sbackground population.[3] It orbits the Sun in thecentral asteroid belt at a distance of 2.1–3.0 AU once every 4 years and 1 month (1,481 days). Its orbit has aneccentricity of 0.19 and aninclination of 7° with respect to theecliptic.[1] The body'sobservation arc begins with its official discovery observation at Turku.[10]

Physical characteristics

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Haltia is an assumed stonyS-type asteroid.[7]

Rotation period

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Two rotationallightcurves ofHaltia were obtained from photometric observations by astronomers Henk de Groot,Raoul Behrend andRené Roy. Lightcurve analysis gave a respectiverotation period of 3.58682 and 3.588 hours with a brightness amplitude of 0.32magnitude (U=3-/3).[8] The Lightcurve Data Base adopts a consolidated period of 3.59 hours.[7]

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,Haltia measures between 6.57 and 8.44 kilometers in diameter and its surface has analbedo between 0.186 and 0.36.[4][5][6]

TheCollaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20 and calculates a diameter of 8.97 based on anabsolute magnitude of 12.6.[7]

Naming

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Thisminor planet was named afterHalti (Haltia), the highest Finnish peak at 1,365 metres (4,478 ft) located on the border between Norway and Finland.[2] The officialnaming citation was published by theMinor Planet Center on 20 February 1976 (M.P.C. 3928).[11]

References

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  1. ^abcd"JPL Small-Body Database Browser: 1460 Haltia (1937 WC)" (2017-07-04 last obs.).Jet Propulsion Laboratory. Retrieved20 October 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(1460) Haltia".Dictionary of Minor Planet Names – (1460) Haltia.Springer Berlin Heidelberg. p. 117.doi:10.1007/978-3-540-29925-7_1461.ISBN 978-3-540-00238-3.
  3. ^ab"Asteroid 1460 Haltia – Proper Elements". AstDyS-2, Asteroids – Dynamic Site. Retrieved29 October 2019.
  4. ^abcdNugent, 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. Retrieved20 October 2017.
  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. ^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. Retrieved20 October 2017.
  7. ^abcdefgh"LCDB Data for (1460) Haltia". Asteroid Lightcurve Database (LCDB). Retrieved20 October 2017.
  8. ^abcBehrend, Raoul."Asteroids and comets rotation curves – (1460) Haltia".Geneva Observatory. Retrieved20 October 2017.
  9. ^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. Retrieved20 October 2017.
  10. ^ab"1460 Haltia (1937 WC)".Minor Planet Center. Retrieved20 October 2017.
  11. ^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

[edit]
Minor planets
Asteroid
Distant minor planet
Comets
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Authority control databasesEdit this at Wikidata
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