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2091 Sampo

From Wikipedia, the free encyclopedia
Main-belt asteroid

2091 Sampo
Discovery[1]
Discovered byY. Väisälä
Discovery siteTurku Obs.
Discovery date26 April 1941
Designations
(2091) Sampo
Named after
Sampo
(Finnish mythology)[2]
1941 HO · 1931 MG
1938 UF1 · 1951 GA1
1952 LB · 1956 EP
1971 BH1 · 1978 NB
A924 BB
main-belt · (outer)
Eos[3][4]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc93.06 yr (33,989 days)
Aphelion3.1985AU
Perihelion2.8300 AU
3.0143 AU
Eccentricity0.0611
5.23yr (1,911 days)
359.61°
0° 11m 17.88s / day
Inclination11.378°
114.53°
318.84°
Physical characteristics
Dimensions23.024±0.474 km[5]
23.493±0.240 km[6]
30.25 km(derived)[3]
30.48±1.3 km[7]
35.47±0.45 km[8]
71.34±0.05h[9]
0.118±0.003[8]
0.1218(derived)[3]
0.1582±0.014[7]
0.2683±0.0325[6]
0.277±0.019[5]
S[3]
10.2[6][7][8] · 10.5[1][3]

2091 Sampo (provisional designation1941 HO), is a stonyEosasteroid and relativelyslow rotator from the outer region of theasteroid belt, approximately 30 kilometers in diameter. It was discovered on 26 April 1941, by Finnish astronomerYrjö Väisälä atTurku Observatory, Finland, and named afterSampo from Finnish mythology.[10]

Orbit and classification

[edit]

Sampo is a member of theEos family (606), the largestasteroid family in theouter main belt consisting of nearly 10,000 asteroids.[4][11]: 23  It orbits the Sun in at a distance of 2.8–3.2 AU once every 5 years and 3 months (1,911 days). Its orbit has aneccentricity of 0.06 and aninclination of 11° with respect to theecliptic.[1]

Physical characteristics

[edit]

TheS-type asteroid measures between 23.0 and 35.5 kilometers in diameter, and its surface has analbedo between 0.118 and 0.277, according to the surveys carried out byIRAS,Akari, andNEOWISE.[5][6][7][8]

A rotationallightcurve ofSampo was obtained from photometric observations made by astronomersRené Roy,Laurent Bernasconi and Stéphane Charbonnelat in March 2003. It gave a potentially longrotation period of71.34±0.05 hours with a brightness variation of 0.38magnitude (U=2).[9]

Naming

[edit]

Thisminor planet was named after the wonder-objectSampo from Finnish mythology. It is mentioned in the national oral folklore and mythology epic,Kalevala, after which the minor planet1454 Kalevala is named. Sampo was to produce every kind of fortune. When Kalevala and Pohjola(also see3606 Pohjola) were fighting for its possession it broke into pieces.[2] The official naming citation was published by theMinor Planet Center on 1 August 1980 (M.P.C. 5450).[12]

References

[edit]
  1. ^abcd"JPL Small-Body Database Browser: 2091 Sampo (1941 HO)" (2017-02-17 last obs.).Jet Propulsion Laboratory. Retrieved11 June 2017.
  2. ^abSchmadel, Lutz D. (2007). "(2091) Sampo".Dictionary of Minor Planet Names.Springer Berlin Heidelberg. pp. 169–170.doi:10.1007/978-3-540-29925-7_2092.ISBN 978-3-540-00238-3.
  3. ^abcde"LCDB Data for (2091) Sampo". Asteroid Lightcurve Database (LCDB). Retrieved7 December 2016.
  4. ^ab"Asteroid 2091 Sampo – 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.
  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. ^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.
  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. ^abBehrend, Raoul."Asteroids and comets rotation curves – (2091) Sampo".Geneva Observatory. Retrieved7 December 2016.
  10. ^"2091 Sampo (1941 HO)".Minor Planet Center. Retrieved7 December 2016.
  11. ^Nesvorný, 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. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved7 December 2016.


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