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1044 Teutonia

From Wikipedia, the free encyclopedia
Main-belt asteroid

1044 Teutonia
Discovery[1]
Discovered byK. Reinmuth
Discovery siteHeidelberg Obs.
Discovery date10 May 1924
Designations
(1044) Teutonia
Pronunciation/tjˈtniə/
Named after
Land of theTeutons[2]
1924 RO · 1925 XF
1929 RP · 1949 KX
1954 UY1 · 1958 RG
1958 UP · A907 EE
main-belt · (middle)
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc109.95 yr (40,158 days)
Aphelion2.9470AU
Perihelion2.2044 AU
2.5757 AU
Eccentricity0.1442
4.13yr (1,510 days)
147.35°
0° 14m 18.24s / day
Inclination4.2515°
59.962°
228.45°
Physical characteristics
Dimensions15.20±1.3 km[3]
15.30 km(derived)[4]
16.85±0.61 km[5]
17.511±0.213 km[6]
17.929±0.192 km[7]
2.84±0.04 h[8]
3.140±0.0010 h[9]
3.153±0.003h[10]
3.157±0.001 h[11]
3.158±0.001 h[12]
3.18±0.02 h[10]
0.2449±0.0196[7]
0.251±0.049[6]
0.273±0.021[5]
0.3340±0.063[3]
0.3613(derived)[4]
S[4]
10.533±0.002(R)[9] · 10.8[1][4] · 10.9[3][5][7]

1044 Teutonia, provisional designation1924 RO, is a stonyasteroid from the central regions of theasteroid belt, approximately 16 kilometers in diameter. It was discovered on 10 May 1924, by astronomerKarl Reinmuth atHeidelberg Observatory in southwest Germany.[13] The asteroid was named after the land inhabited by theTeutonic people.[2]

Classification and orbit

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Teutonia orbits the Sun in thecentral main-belt at a distance of 2.2–2.9 AU once every 4 years and 2 months (1,510 days). Its orbit has aneccentricity of 0.14 and aninclination of 4° with respect to theecliptic.[1]

The asteroid'sobservation arc begin 17 years prior to its official discovery observation, with its first identification asA907 EE at Taunton Observatory (803) in March 1907.[13]

Physical characteristics

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Lightcurves

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Images of the object made during 2007 were used to produce alight curve that gave a synodic period of 2.84 ± 0.04 h. However, a study made in 2006 gave a period of 3.153 ± 0.003, which can not yet be ruled out. The brightness of the object varied by 0.20 ± 0.03 inmagnitude over the course of each rotation.[8]

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,Teutonia measures between 15.20 and 17.929 kilometers in diameter and its surface has analbedo between 0.2449 and 0.3340.[3][5][6][7] TheCollaborative Asteroid Lightcurve Link derives an albedo of 0.3613 and a diameter of 15.30 kilometers based on anabsolute magnitude of 10.8.[4]

Naming

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Thisminor planet was named for the land once inhabited by theTeutons, a Germanic tribe that lived in what is nowJutland. The name was proposed by astronomer Gustav Stracke.[2]

References

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  1. ^abcd"JPL Small-Body Database Browser: 1044 Teutonia (1924 RO)" (2017-02-24 last obs.).Jet Propulsion Laboratory. Retrieved30 June 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(1044) Teutonia".Dictionary of Minor Planet Names – (1044) Teutonia.Springer Berlin Heidelberg. p. 89.doi:10.1007/978-3-540-29925-7_1045.ISBN 978-3-540-00238-3.
  3. ^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.
  4. ^abcde"LCDB Data for (1044) Teutonia". Asteroid Lightcurve Database (LCDB). Retrieved30 June 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. ^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. Retrieved30 June 2017.
  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.
  8. ^abBetzler, Alberto Silva; Ferreira, Diogo Henrique; Dos Santos, Tarcio Henrique Ribeiro; Novaes, Alberto Brum (March 2008)."Lightcurve and Rotation Period of 1044 Teutonia".The Minor Planet Bulletin.35 (1): 26.Bibcode:2008MPBu...35...26B.ISSN 1052-8091. Retrieved30 June 2017.
  9. ^abWaszczak, Adam; Chang, Chan-Kao; Ofek, Eran O.; Laher, Russ; Masci, Frank; Levitan, David; et al. (September 2015)."Asteroid Light Curves from the Palomar Transient Factory Survey: Rotation Periods and Phase Functions from Sparse Photometry".The Astronomical Journal.150 (3): 35.arXiv:1504.04041.Bibcode:2015AJ....150...75W.doi:10.1088/0004-6256/150/3/75. Retrieved30 June 2017.
  10. ^abBehrend, Raoul."Asteroids and comets rotation curves – (1044) Teutonia".Geneva Observatory. Retrieved30 June 2017.
  11. ^Klinglesmith, Daniel A. III; Hanowell, Jesse; Risley, Ethan; Turk, Janek; Vargas, Angelica; Warren, Curtis Alan (July 2014)."Lightcurves for Inversion Model Candidates".The Minor Planet Bulletin.41 (3):139–143.Bibcode:2014MPBu...41..139K.ISSN 1052-8091. Retrieved30 June 2017.
  12. ^Klinglesmith, Daniel A. III (January 2017)."Asteroid Photometry Results from Etscorn Observatory".The Minor Planet Bulletin.44 (1):69–72.Bibcode:2017MPBu...44...69K.ISSN 1052-8091. Retrieved30 June 2017.
  13. ^ab"1044 Teutonia (1924 RO)".Minor Planet Center. Retrieved30 June 2017.

External links

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