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2826 Ahti

From Wikipedia, the free encyclopedia
Main-belt asteroid

2826 Ahti
Discovery[1]
Discovered byY. Väisälä
Discovery siteTurku Obs.
Discovery date18 October 1939
Designations
(2826) Ahti
Named after
Ahti(Finnish mythology)[2]
1939 UJ · 1942 FH
1950 TG3 · 1968 UT2
1979 RG · 1980 VK1
main-belt · (outer)[1]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc77.63 yr (28,355 days)
Aphelion3.3789AU
Perihelion3.0708 AU
3.2248 AU
Eccentricity0.0478
5.79yr (2,115 days)
2.3046°
0° 10m 12.72s / day
Inclination15.466°
33.671°
150.83°
Physical characteristics
Dimensions36.60 km(derived)[3]
36.71±2.7 km(IRAS:24)[4]
39.975±0.157[5]
42.16±0.62 km[6]
42.373±0.121 km[7]
55.33±0.29 km[8]
24h[9]
0.023±0.004[8][5]
0.0471±0.0122[7]
0.0479(derived)[3]
0.049±0.002[6]
0.0628±0.010(IRAS:24)[4]
C[3]
11.1[1][3] · 10.80[4][6][7] · 11.00[8] · 11.25±0.25[10]

2826 Ahti, provisional designation1939 UJ, is a carbonaceousasteroid from the outer region of theasteroid belt, about 37 kilometers in diameter. The asteroid was discovered on 18 October 1939, by Finnish astronomerYrjö Väisälä atTurku Observatory, Southwest Finland.[11] It was named afterAhti from Finnish mythology.[2]

Orbit and classification

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Ahti orbits the Sun in theouter main-belt at a distance of 3.1–3.4 AU once every 5 years and 9 months (2,115 days). Its orbit has aneccentricity of 0.05 and aninclination of 15° with respect to theecliptic.[1]

Physical characteristics

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Ahti has been characterized as a darkC-type asteroid.[3]

Rotation period

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A photmetriclightcurve analysis by French astronomerPierre Antonini in 2006, gave a longer than averagerotation period of 24 hours (U=1). The result, however, is considered to be only provisional.[3][9]

Diameter and albedo

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According to the surveys carried out by the Infrared Astronomical SatelliteIRAS, the JapaneseAkari satellite, and NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE mission,Ahti measures between 36.71 and 55.33 kilometers in diameter and its surface has a lowalbedo between 0.023 and 0.0628.[4][5][6][7][8]

TheCollaborative Asteroid Lightcurve Link agrees best with the results obtained by IRAS, and derives a diameter of 36.60 kilometers with an albedo of 0.0479 and anabsolute magnitude of 11.1.[3]

Naming

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Thisminor planet was named for the god of the sea and of fishing,Ahti (also known as Ahto), mentioned in theKalevala, a 19th-century work of epic poetry from Karelian and Finnish oral folklore and mythology.

The asteroid1454 Kalevala is named after the Finishnational epic. Ahti is also a common masculine name in Finland.[2] The official naming citation was published by theMinor Planet Center on 26 May 1983 (M.P.C. 7949).[12]

References

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  1. ^abcde"JPL Small-Body Database Browser: 2826 Ahti (1939 UJ)" (2017-06-05 last obs.).Jet Propulsion Laboratory. Retrieved14 June 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(2826) Ahti".Dictionary of Minor Planet Names – (2826) Ahti.Springer Berlin Heidelberg. p. 231.doi:10.1007/978-3-540-29925-7_2827.ISBN 978-3-540-00238-3.
  3. ^abcdefg"LCDB Data for (2826) Ahti". Asteroid Lightcurve Database (LCDB). Retrieved1 May 2016.
  4. ^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.
  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. Retrieved6 December 2016.
  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. ^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. Retrieved1 May 2016.
  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. Retrieved1 May 2016.
  9. ^abBehrend, Raoul."Asteroids and comets rotation curves – (2826) Ahti".Geneva Observatory. Retrieved1 May 2016.
  10. ^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. Retrieved1 May 2016.
  11. ^"2826 Ahti (1939 UJ)".Minor Planet Center. Retrieved1 May 2016.
  12. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved5 August 2016.

External links

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Distant minor planet
Comets
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