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Contents

   



(Top)
 


1 Classification and orbit  





2 Physical characteristics  



2.1  Lightcurves  





2.2  Diameter and albedo  







3 Naming  





4 References  





5 External links  














1044 Teutonia






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From Wikipedia, the free encyclopedia
 


1044 Teutonia
Discovery[1]
Discovered byK. Reinmuth
Discovery siteHeidelberg Obs.
Discovery date10 May 1924
Designations

MPC designation

(1044) Teutonia
Pronunciation/tjˈtniə/

Named after

Land of the Teutons[2]

Alternative designations

1924 RO · 1925 XF
1929 RP · 1949 KX
1954 UY1 · 1958 RG
1958 UP · A907 EE

Minor planet category

main-belt · (middle)
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc109.95 yr (40,158 days)
Aphelion2.9470 AU
Perihelion2.2044 AU

Semi-major axis

2.5757 AU
Eccentricity0.1442

Orbital period (sidereal)

4.13 yr (1,510 days)

Mean anomaly

147.35°

Mean motion

0° 14m 18.24s / day
Inclination4.2515°

Longitude of ascending node

59.962°

Argument of perihelion

228.45°
Physical characteristics
Dimensions15.20±1.3km[3]
15.30 km (derived)[4]
16.85±0.61km[5]
17.511±0.213km[6]
17.929±0.192km[7]

Synodic rotation period

2.84±0.04h[8]
3.140±0.0010h[9]
3.153±0.003 h[10]
3.157±0.001h[11]
3.158±0.001h[12]
3.18±0.02h[10]

Geometric albedo

0.2449±0.0196[7]
0.251±0.049[6]
0.273±0.021[5]
0.3340±0.063[3]
0.3613 (derived)[4]

Spectral type

S[4]

Absolute magnitude (H)

10.533±0.002 (R)[9] · 10.8[1][4] · 10.9[3][5][7]

1044 Teutonia, provisional designation 1924 RO, is a stony asteroid from the central regions of the asteroid belt, approximately 16 kilometers in diameter. It was discovered on 10 May 1924, by astronomer Karl ReinmuthatHeidelberg Observatory in southwest Germany.[13] The asteroid was named after the land inhabited by the Teutonic people.[2]

Classification and orbit[edit]

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

The asteroid's observation arc begin 17 years prior to its official discovery observation, with its first identification as A907 EE at Taunton Observatory (803) in March 1907.[13]

Physical characteristics[edit]

Lightcurves[edit]

Images of the object made during 2007 were used to produce a light 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 in magnitude over the course of each rotation.[8]

Diameter and albedo[edit]

According to the surveys carried out by the Infrared Astronomical Satellite IRAS, the Japanese Akari satellite, and NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, Teutonia measures between 15.20 and 17.929 kilometers in diameter and its surface has an albedo between 0.2449 and 0.3340.[3][5][6][7] The Collaborative Asteroid Lightcurve Link derives an albedo of 0.3613 and a diameter of 15.30 kilometers based on an absolute magnitude of 10.8.[4]

Naming[edit]

This minor planet was named for the land once inhabited by the Teutons, a Germanic tribe that lived in what is now Jutland. The name was proposed by astronomer Gustav Stracke.[2]

References[edit]

  1. ^ a b c d "JPL Small-Body Database Browser: 1044 Teutonia (1924 RO)" (2017-02-24 last obs.). Jet Propulsion Laboratory. Retrieved 30 June 2017.
  • ^ a b c Schmadel, 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.
  • ^ a b c d Tedesco, 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. Retrieved 22 October 2019.
  • ^ a b c d e "LCDB Data for (1044) Teutonia". Asteroid Lightcurve Database (LCDB). Retrieved 30 June 2017.
  • ^ a b c d Usui, 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)
  • ^ a b c Masiero, 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. Retrieved 30 June 2017.
  • ^ a b c d Mainzer, 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.
  • ^ a b Betzler, 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. Retrieved 30 June 2017.
  • ^ a b Waszczak, 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. Retrieved 30 June 2017.
  • ^ a b Behrend, Raoul. "Asteroids and comets rotation curves – (1044) Teutonia". Geneva Observatory. Retrieved 30 June 2017.
  • ^ 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. Retrieved 30 June 2017.
  • ^ 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. Retrieved 30 June 2017.
  • ^ a b "1044 Teutonia (1924 RO)". Minor Planet Center. Retrieved 30 June 2017.
  • External links[edit]


    Retrieved from "https://en.wikipedia.org/w/index.php?title=1044_Teutonia&oldid=1191754879"

    Categories: 
    Minor planet object articles (numbered)
    Background asteroids
    Discoveries by Karl Wilhelm Reinmuth
    Named minor planets
    Astronomical objects discovered in 1924
    Hidden categories: 
    Use dmy dates from October 2019
    Webarchive template wayback links
    Articles with JPL SBDB identifiers
    Articles with MPC identifiers
     



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