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1424 Sundmania

From Wikipedia, the free encyclopedia
Large asteroid and rather slow rotator

1424 Sundmania
Shape model ofSundmania from itslightcurve
Discovery[1]
Discovered byY. Väisälä
Discovery siteTurku Obs.
Discovery date9 January 1937
Designations
(1424) Sundmania
Named after
Karl F. Sundman[2][3]
(Finnish mathematician)
1937 AJ · 1929 SS
1929 UB · 1931 AD
1938 FP · A918 WA
main-belt · (outer)[4]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc98.53 yr (35,989 days)
Aphelion3.3831AU
Perihelion2.9966 AU
3.1899 AU
Eccentricity0.0606
5.70yr (2,081 days)
196.29°
0° 10m 22.8s / day
Inclination9.1784°
42.988°
301.53°
Physical characteristics
64.691±0.254 km[5]
68.169±1.767 km[6]
70.56 km(derived)[4]
70.75±2.5 km[7]
73.40±0.86 km[8]
74.46±16.37 km[9]
80.20±28.15 km[10]
84.67±0.64 km[11]
93.73±0.03 h[12]
  • (51.0°, 76.0°) (λ11)[13]
  • (275.0°, 58.0°) (λ22)[13]
0.030±0.004[11]
0.03±0.01[9]
0.03±0.04[10]
0.0426(derived)[4]
0.052±0.001[8]
0.0559±0.004[7]
0.0602±0.0136[6]
SMASS =X[1] · P[6] · C[4]
9.50[6][7][8] · 9.80[4][11] · 9.90[1][9] · 10.03±0.38[14] · 10.07[10]

1424 Sundmania (prov. designation:1937 AJ) is a largeasteroid and ratherslow rotator from thebackground population of the outer regions of theasteroid belt. It was discovered on 9 January 1937, by astronomerYrjö Väisälä at theTurku Observatory in southwest Finland.[15] The darkX-type asteroid has a notably longrotation period of 93.7 hours and measures approximately 70 kilometers (43 miles) in diameter. It was named after Finnish astronomer and mathematicianKarl F. Sundman.[2]

Orbit and classification

[edit]

Sundmania is a non-family asteroid of the main belt'sbackground population when applying thehierarchical clustering method to itsproper orbital elements. It orbits the Sun in theouter main-belt at a distance of 3.0–3.4 AU once every 5 years and 8 months (2,081 days). Its orbit has aneccentricity of 0.06 and aninclination of 9° with respect to theecliptic.[1] The body'sobservation arc begins with its first identification asA918 WA atHeidelberg Observatory in November 1918, more than 18 years prior to its official discovery observation at Turku.[15]

Naming

[edit]

Thisminor planet was named after Finnish mathematicianKarl F. Sundman (1873–1949), who intensively worked on then-body problem. Sundman worked as an astronomer at several observatories all over Europe. He became director of theHelsinki University Observatory and was appointed professor of astronomy at theUniversity of Helsinki in 1907. The asteroids1558 Järnefelt and1559 Kustaanheimo were also named after astronomers from the University of Helsinki.[2][3] Thenaming was mentioned inThe Names of the Minor Planets byPaul Herget in 1955 (H 129). The lunar craterSundman was also named in his honor.[2]

Physical characteristics

[edit]

In theSMASS classification,Sundmania is anX-type asteroid.[1] It has also been characterized as a primitiveP-type by theWide-field Infrared Survey Explorer (WISE).[6] The Lightcurve Data Base assumes it to be a carbonaceousC-type asteroid.[4]

Rotation period

[edit]

Sundmania is a ratherslow rotator as most minor planets have arotation period of less than 20 hours.

In April 2012, a rotationallightcurve ofSundmania was obtained fromphotometric observations by American astronomerRobert Stephens at the Goat Mountain Astronomical Research Station (G79) in California. Lightcurve analysis gave a rotation period of 93.73 hours with a brightness amplitude of 0.42magnitude (U=2+).[12] Observations by French amateur astronomersLaurent Bernasconi andRené Roy gave a period of 36 and 47 hours, of which the latter seems to be half the period solution obtained by Stephens (U=1/1+).[16]

Spin axis

[edit]

In 2016, an international study modeled a lightcurve with a period of94.537±0.005 hours and found twospin axes of (51.0°, 76.0°) and (275.0°, 58.0°) inecliptic coordinates (λ, β).[13]

Diameter and albedo

[edit]

According to the surveys carried out by the Infrared Astronomical SatelliteIRAS, the JapaneseAkari satellite and theNEOWISE mission of NASA's WISE telescope,Sundmania measures between 64.691 and 84.67 kilometers in diameter and its surface has analbedo between 0.030 and 0.0602.[5][6][7][8][9][10][11] TheCollaborative Asteroid Lightcurve Link derives an albedo of 0.0426 and a diameter of 70.56 kilometers based on anabsolute magnitude of 9.8.[4]

References

[edit]
  1. ^abcdef"JPL Small-Body Database Browser: 1424 Sundmania (1937 AJ)" (2017-06-04 last obs.).Jet Propulsion Laboratory. Retrieved20 September 2017.
  2. ^abcdSchmadel, Lutz D. (2007). "(1424) Sundmania".Dictionary of Minor Planet Names.Springer Berlin Heidelberg. p. 114.doi:10.1007/978-3-540-29925-7_1425.ISBN 978-3-540-00238-3.
  3. ^abHannu Karttunen."Observatory museum Biographies: 1900s — Sundman, Karl Frithiof (1873–1949)". University of Helsinky. Archived fromthe original on 16 June 2011.
  4. ^abcdefg"LCDB Data for (1424) Sundmania". Asteroid Lightcurve Database (LCDB). Retrieved20 September 2017.
  5. ^abMasiero, 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.S2CID 119293330. Retrieved20 September 2017.
  6. ^abcdefMainzer, 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.S2CID 35447010.
  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. ^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.S2CID 9341381. Retrieved20 September 2017.
  10. ^abcdNugent, C. R.; Mainzer, A.; Bauer, J.; Cutri, R. M.; Kramer, E. A.; Grav, T.; et al. (September 2016)."NEOWISE Reactivation Mission Year Two: Asteroid Diameters and Albedos".The Astronomical Journal.152 (3): 12.arXiv:1606.08923.Bibcode:2016AJ....152...63N.doi:10.3847/0004-6256/152/3/63.
  11. ^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.S2CID 46350317. Retrieved20 September 2017.
  12. ^abStephens, Robert D. (October 2012)."Asteroids Observed from Santana, CS3 and GMARS Observatories: 2012 April - June"(PDF).Minor Planet Bulletin.39 (4):226–228.Bibcode:2012MPBu...39..226S.ISSN 1052-8091. Retrieved16 March 2020.
  13. ^abcHanus, J.; Durech, J.; Oszkiewicz, D. A.; Behrend, R.; Carry, B.; Delbo, M.; et al. (February 2016). "New and updated convex shape models of asteroids based on optical data from a large collaboration network".Astronomy and Astrophysics.586: 24.arXiv:1510.07422.Bibcode:2016A&A...586A.108H.doi:10.1051/0004-6361/201527441.S2CID 119112278.
  14. ^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.S2CID 53493339. Retrieved20 September 2017.
  15. ^ab"1424 Sundmania (1937 AJ)".Minor Planet Center. Retrieved20 September 2017.
  16. ^Behrend, Raoul."Asteroids and comets rotation curves – (1424) Sundmania".Geneva Observatory. Retrieved20 September 2017.

External links

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