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1219 Britta

From Wikipedia, the free encyclopedia
Main-belt asteroid

1219 Britta
Shape model ofBritta from itslightcurve
Discovery[1]
Discovered byM. F. Wolf
Discovery siteHeidelberg Obs.
Discovery date6 February 1932
Designations
(1219) Britta
Named after
unknown[2]
1932 CJ · 1947 XG
1975 FE · A904 SB
A915 BD
main-belt[1][3] · (inner)
Flora[4] · background[5]
Orbital characteristics[3]
Epoch 23 March 2018 (JD 2458200.5)
Uncertainty parameter 0
Observation arc113.51yr (41,461 d)
Aphelion2.4883AU
Perihelion1.9390 AU
2.2136 AU
Eccentricity0.1241
3.29 yr (1,203 d)
131.11°
0° 17m 57.48s / day
Inclination4.4135°
42.543°
23.720°
Physical characteristics
9.86±0.34 km[6]
11.43±0.9 km[7]
11.76±0.30 km[8]
5.573±0.001 h[9]
5.574±0.003 h[10]
5.5750±0.0005 h[11]
5.575±0.001 h[12]
5.575 h[13]
5.575 h[14]
5.57556±0.00001 h[15]
5.57557±0.00002 h[16]
0.223±0.013[8]
0.2267±0.040[7]
0.2629(derived)[4]
0.346±0.041[6]
S(S3OS2)[17]
B–V = 0.913[3]
U–B = 0.514[3]
11.7[3]
11.80[4][6]
11.94[7][8]

1219 Britta, provisional designation1932 CJ, is a stony backgroundasteroid from the inner regions of theasteroid belt, approximately 11 kilometers (7 miles) in diameter. It was discovered on 6 February 1932, by German astronomerMax Wolf at theHeidelberg-Königstuhl State Observatory in southern Germany.[1] The likely elongatedS-type asteroid has arotation period of 5.57 hours.[4] Any reference of its name to a person is unknown.[2]

Orbit and classification

[edit]

Britta is a non-family asteroid of the main belt'sbackground population when applying thehierarchical clustering method to itsproper orbital elements.[5] Based on osculating Keplerianorbital elements, the asteroid has also been classified as a member of theFlora family (402), a giantasteroid family and the largest family of stony asteroids in the main-belt.[4]

It orbits the Sun in theinner main-belt at a distance of 1.9–2.5 AU once every 3 years and 3 months (1,203 days;semi-major axis of 2.21 AU). Its orbit has aneccentricity of 0.12 and aninclination of 4° with respect to theecliptic.[3]

The asteroid was first observed asA904 SB at Heidelberg Observatory in September 1904. The body'sobservation arc begins with its official discovery observation at Heidelberg in February 1932.[1]

Naming

[edit]

Thisminor planet is named after a common German female name. Any reference of this name to a person or occurrence is unknown.[2]

Unknown meaning

[edit]

Among the many thousands ofnamed minor planets,Britta is one of 120 asteroids, for which no official naming citation has been published. All of these low-numbered asteroids have numbers between164 Eva and1514 Ricouxa and were discovered between 1876 and the 1930s, predominantly by astronomersAuguste Charlois,Johann Palisa,Max Wolf andKarl Reinmuth.[18]

Physical characteristics

[edit]

Britta has been characterized as a stonyS-type asteroid in both the Tholen- and SMASS-like taxonomy of theSmall Solar System Objects Spectroscopic Survey (S3OS2).[17]

Rotation period

[edit]

Several rotationallightcurves[a] ofBritta have been obtained from photometric observations since the 1980s.[9][10][11][12][13][14] The consolidated lightcurve analysis results give arotation period of 5.575 hours with a brightness amplitude between 0.48 and 0.75magnitude, indicative of an elongated shape (U=3).[4]

Spin axis

[edit]

Modeled photometric data from the Lowell Photometric Database (LPD) and the robotic BlueEye600 Observatory, gave a concurring period of 5.57556 and 5.57557 hours, respectively.[15][16] Both studies determined twospin axes of (72.0°, −66.0°) and (241.0°, −66.0°), as well as (61.0°, −2.0°) and (223.0°, −68.0°) inecliptic coordinates (λ, β).[15][16]

Diameter and albedo

[edit]

According to the surveys carried out by the Infrared Astronomical SatelliteIRAS, the JapaneseAkari satellite and theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer,Britta measures between 9.860 and 11.76 kilometers in diameter and its surface has analbedo between 0.223 and 0.346.[6][7][8] TheCollaborative Asteroid Lightcurve Link derives an albedo of 0.2629 and a diameter of 11.31 kilometers based on anabsolute magnitude of 11.8.[4]

Notes

[edit]
  1. ^Lightcurve plot of (1219) Britta byR. D. Stephens (2014): rotation period5.573±0.001 hours. 474 data points. Quality Code of 3. Summary figures at theLCDB andCenter for Solar System Studies – CS3 Lightcurves Page

References

[edit]
  1. ^abcd"1219 Britta (1932 CJ)".Minor Planet Center. Retrieved11 January 2018.
  2. ^abcSchmadel, Lutz D. (2007). "(1219) Britta".Dictionary of Minor Planet Names – (1219) Britta.Springer Berlin Heidelberg. p. 102.doi:10.1007/978-3-540-29925-7_1220.ISBN 978-3-540-00238-3.
  3. ^abcdef"JPL Small-Body Database Browser: 1219 Britta (1932 CJ)" (2018-03-27 last obs.).Jet Propulsion Laboratory. Retrieved3 May 2018.
  4. ^abcdefg"LCDB Data for (1219) Britta". Asteroid Lightcurve Database (LCDB). Retrieved3 May 2018.
  5. ^ab"Asteroid 1219 Britta – Proper Elements". AstDyS-2, Asteroids – Dynamic Site. Retrieved28 October 2019.
  6. ^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. Retrieved11 January 2018.
  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. ^abStephens, Robert D. (July 2014)."Asteroids Observed from CS3: 2014 January - March".The Minor Planet Bulletin.41 (3):171–175.Bibcode:2014MPBu...41..171S.ISSN 1052-8091. Retrieved11 January 2018.
  10. ^abBehrend, Raoul."Asteroids and comets rotation curves – (1219) Britta". Geneva Observatory. Retrieved11 January 2018.
  11. ^abKryszczynska, A.; Colas, F.; Polinska, M.; Hirsch, R.; Ivanova, V.; Apostolovska, G.; et al. (October 2012)."Do Slivan states exist in the Flora family?. I. Photometric survey of the Flora region".Astronomy and Astrophysics.546: 51.Bibcode:2012A&A...546A..72K.doi:10.1051/0004-6361/201219199. Retrieved11 January 2018.
  12. ^abKlinglesmith, 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. Retrieved11 January 2018.
  13. ^abBinzel, R. P.; Cochran, A. L.; Barker, E. S.; Tholen, D. J.; Barucci, A.; di Martino, M.; et al. (July 1987)."Coordinated observations of asteroids 1219 Britta and 1972 Yi Xing".Icarus.71 (1):148–158.Bibcode:1987Icar...71..148B.doi:10.1016/0019-1035(87)90169-2.ISSN 0019-1035. Retrieved11 January 2018.
  14. ^abPilcher, Frederick; Binzel, R. P.; Tholen, D. J. (March 1985)."Rotations of 1168 Brandia and 1219 Britta".The Minor Planet Bulletin.12: 10.Bibcode:1985MPBu...12...10P. Retrieved11 January 2018.
  15. ^abcDurech, J.; Hanus, J.; Oszkiewicz, D.; Vanco, R. (March 2016)."Asteroid models from the Lowell photometric database".Astronomy and Astrophysics.587: 6.arXiv:1601.02909.Bibcode:2016A&A...587A..48D.doi:10.1051/0004-6361/201527573. Retrieved11 January 2018.
  16. ^abcDurech, Josef; Hanus, Josef; Broz, Miroslav; Lehký, Martin; Behrend, Raoul; Antonini, Pierre; et al. (April 2018). "Shape models of asteroids based on lightcurve observations with BlueEye600 robotic observatory".Icarus.304:101–109.arXiv:1707.03637.Bibcode:2018Icar..304..101D.doi:10.1016/j.icarus.2017.07.005.
  17. ^ab"Asteroid 1219 Britta – Asteroid Taxonomy V6.0".Small Bodies Data Ferret. Retrieved28 October 2019.
  18. ^Schmadel, Lutz D. (2007). "Appendix 11 – Minor Planet Names with Unknown Meaning".Dictionary of Minor Planet Names – Fifth Revised and Enlarged revision. Springer Berlin Heidelberg. pp. 927–929.ISBN 978-3-540-00238-3.

External links

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