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1079 Mimosa

From Wikipedia, the free encyclopedia
Main-belt asteroid

1079 Mimosa
Discovery[1]
Discovered byG. van Biesbroeck
Discovery siteYerkes Obs.
Discovery date14 January 1927
Designations
(1079) Mimosa
Pronunciation/mɪˈmzə,-sə/[2]
Named after
Mimosa(flowering plant)[3]
1927 AD · 1961 AM
main-belt · (outer)
Koronis[4] · Karin[5]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc90.80 yr (33,165 days)
Aphelion3.0127AU
Perihelion2.7332 AU
2.8729 AU
Eccentricity0.0486
4.87yr (1,779 days)
253.25°
0° 12m 8.64s / day
Inclination1.1764°
329.37°
106.35°
Physical characteristics
Dimensions19.01±1.20 km[6]
20.67 km(derived)[4]
20.69±2.7 km[1][5]
7.3h[7]
24 h[8]
64.6±0.5 h[9]
0.1332(derived)[4]
0.1367±0.044[1]
0.174±0.025[6]
Tholen =S[1][4] · S[10]
B–V = 0.800[1]
U–B = 0.393[1]
11.1[1] · 11.18±0.02[9] · 11.20[6] · 11.23[4][7] · 11.30±0.26[10]

1079 Mimosa, provisional designation1927 AD, is a stony Karin or Koronianasteroid from the outer regions of theasteroid belt, approximately 20 kilometers in diameter. It was discovered on 14 January 1927, by Belgian–American astronomerGeorge Van Biesbroeck at theYerkes Observatory in Williams Bay, Wisconsin.[11] The asteroid was named after the flowering plantMimosa.[3]

Orbit and classification

[edit]

Based on theHierarchical Clustering Method, which uses the object'sproper orbital elements,Mimosa is a member of the stonyKarin family (610),[5] a mid-sized asteroid family named after its parent body832 Karin.[12]: 23  The asteroid has also been grouped into the much largerKoronis family (605).[4][5]

Mimosa orbits the Sun in theouter asteroid belt at a distance of 2.7–3.0 AU once every 4 years and 10 months (1,779 days;semi-major axis of 2.87 AU). Its orbit has aneccentricity of 0.05 and aninclination of 1° with respect to theecliptic.[1] The body'sobservation arc begins with its official discovery observation at Williams Bay in January 1927.[11]

Physical characteristics

[edit]

In theTholen classification,Mimosa is a stonyS-type asteroid, which matches the overallspectral type of both the Karin and Koronis family.[1][4]Pan-STARRS' photometric survey also characterized the asteroid as a common S-type.[10]

Rotation period

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Several fragmentary rotationallightcurves ofMimosa have been obtained from photometric observations since 1983.[7][8][9] Lightcurve analysis gave a consolidatedrotation period of 64.6 hours with a brightness amplitude between 0.07 and 0.13magnitude (U=2-).[4] While not being aslow rotator, this is a notably longer-than average period as most asteroids take less than 20 hours to complete a full rotation. However, the period is based on a fragmentary lightcurve and still may change significantly. As of 2017, no secure period has been obtained.[4]

Diameter and albedo

[edit]

According to the surveys carried out by the Infrared Astronomical SatelliteIRAS (PDS IMPS) and the JapaneseAkari satellite,Mimosa measures between 19.01 and 20.69 kilometers in diameter and its surface has analbedo between 0.1367 and 0.174.[1][5][6] TheCollaborative Asteroid Lightcurve Link derives an albedo of 0.1332 and a diameter of 20.67 kilometers based on anabsolute magnitude of 11.23.[4]

Naming

[edit]

Thisminor planet was named after the flowering plantMimosa, a genus of herbs and shrubs of the legume familyFabaceae(also see list of minor planets named after animals and plants). The official naming citation was mentioned inThe Names of the Minor Planets byPaul Herget in 1955 (H 102).[3]

References

[edit]
  1. ^abcdefghijk"JPL Small-Body Database Browser: 1079 Mimosa (1927 AD)" (2017-11-02 last obs.).Jet Propulsion Laboratory. Retrieved29 November 2017.
  2. ^"mimosa".Oxford English Dictionary (Online ed.). Oxford University Press. (Subscription orparticipating institution membership required.)
  3. ^abcSchmadel, Lutz D. (2007). "(1079) Mimosa".Dictionary of Minor Planet Names.Springer Berlin Heidelberg. p. 92.doi:10.1007/978-3-540-29925-7_1080.ISBN 978-3-540-00238-3.
  4. ^abcdefghij"LCDB Data for (1079) Mimosa". Asteroid Lightcurve Database (LCDB). Retrieved29 November 2017.
  5. ^abcde"Asteroid 1079 Mimosa – Nesvorny HCM Asteroid Families V3.0".Small Bodies Data Ferret. Retrieved26 October 2019.
  6. ^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)
  7. ^abcBinzel, R. P. (October 1987)."A photoelectric survey of 130 asteroids".Icarus.72 (1):135–208.Bibcode:1987Icar...72..135B.doi:10.1016/0019-1035(87)90125-4.ISSN 0019-1035. Retrieved29 November 2017.
  8. ^abBehrend, Raoul."Asteroids and comets rotation curves – (1079) Mimosa". Geneva Observatory. Retrieved29 November 2017.
  9. ^abcSlivan, Stephen M.; Binzel, Richard P.; Boroumand, Shaida C.; Pan, Margaret W.; Simpson, Christine M.; Tanabe, James T.; et al. (May 2008)."Rotation rates in the Koronis family, complete to H≈11.2".Icarus.195 (1):226–276.Bibcode:2008Icar..195..226S.doi:10.1016/j.icarus.2007.11.019. Retrieved29 November 2017.
  10. ^abcVeres, 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. Retrieved29 November 2017.
  11. ^ab"1079 Mimosa (1927 AD)".Minor Planet Center. Retrieved29 November 2017.
  12. ^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.

External links

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