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1127 Mimi

From Wikipedia, the free encyclopedia
Main-belt asteroid

1127 Mimi
Modelled shape ofMimi from itslightcurve
Discovery[1]
Discovered byS. Arend
Discovery siteUccle Obs.
Discovery date13 January 1929
Designations
(1127) Mimi
Named after
"Mimi" Delporte
(wife ofEugène Delporte)[2]
1929 AJ · 1948 PU
A906 OA
Orbital characteristics[3]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc87.10 yr (31,812 days)
Aphelion3.2821AU
Perihelion1.9104 AU
2.5962 AU
Eccentricity0.2642
4.18yr (1,528 days)
122.26°
0° 14m 8.16s / day
Inclination14.745°
128.63°
281.95°
Physical characteristics
46.006±0.305 km[6]
46.18±10.10 km[7]
46.84±4.9 km[8][9]
48.198±0.465 km[10]
49.53±0.67 km[11]
50.67±13.81 km[12]
8.5410±0.0004 h[13]
8.541±0.1 h[14]
12.749±0.003 h[15]
(224.0°, −57.0°) (λ11)[5]
0.031±0.001[11]
0.0317±0.0133[10]
0.0336±0.008[8][9]
0.034±0.005[6]
0.04±0.02[7][12]
10.6[1][3][8][9][11]

1127 Mimi (prov. designation:1929 AJ) is a darkbackground asteroid from the central regions of theasteroid belt. It was discovered on 13 January 1929, by Belgian astronomerSylvain Arend at theRoyal Observatory of Belgium in Uccle.[1] The carbonaceousC-type asteroids (CX) has arotation period of 12.7 hours and measures approximately 47 kilometers (29 miles) in diameter. Through a glitch in the naming process, the asteroid received the name "Mimi" instead of "Robelmonte" as originally intended by the discoverer.[2]

Orbit and classification

[edit]

Mimi is a non-family asteroid of the main belt'sbackground population when applying thehierarchical clustering method to itsproper orbital elements.[4][5] It orbits the Sun in thecentral asteroid belt at a distance of 1.9–3.3 AU once every 4 years and 2 months (1,528 days). Its orbit has aneccentricity of 0.26 and aninclination of 15° with respect to theecliptic.[3] The asteroid was first observed asA906 OA atHeidelberg Observatory in July 1906. The body'sobservation arc begins at Uccle in May 1934, more than 5 years after its official discovery observation.[1]

Naming

[edit]

Thisminor planet was named after "Mimi" the wife of Belgian astronomerEugène Delporte. Through an error, the names intended for 1127 Mimi (wife of Delporte) and1145 Robelmonte (birthplace of Arend) had been switched, and each name had been proposed by the discoverer of the other asteroid. Thenaming was mentioned inThe Names of the Minor Planets byPaul Herget in 1955 (H 105).[2]

Physical characteristics

[edit]

Mimi has been characterized as a darkP-type asteroid by theWide-field Infrared Survey Explorer (WISE). In theTholen classification, no unambiguous type could by assigned. Numerical color analysis showed that it is closest to theC-type asteroids and somewhat similar to theX-type asteroids (CX).[3]

Rotation period and pole

[edit]

In January 2004, the best-rated rotationallightcurve ofMimi was obtained fromphotometric observations by astronomer John Menke at his Menke Observatory in Barnesville, Maryland (no obs. code). Lightcurve analysis gave a well-definedrotation period of 12.749 hours with a brightness amplitude of 0.72magnitude (U=3).[15] Two other lightcurves gave a shorter period of 8.541 hours with an amplitude of 0.93 and 0.95 magnitude, respectively (U=2/2).[13][14]

A 2016-published lightcurve, using modeled photometric data from the Lowell Photometric Database (LPD), gave a concurring period of 12.74557 hours, as well as a spin axis of (224.0°, −57.0°) inecliptic coordinates (λ, β).[16]

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,Mimi measures between 46.006 and 50.67 kilometers in diameter and its surface has analbedo between 0.031 and 0.04.[6][7][8][10][11][12]

TheCollaborative Asteroid Lightcurve Link adopts the results obtained by IRAS, that is, an albedo of 0.0336 and a diameter of 46.84 kilometers based on anabsolute magnitude of 10.95.[9]

References

[edit]
  1. ^abcde"1127 Mimi (1929 AJ)".Minor Planet Center. Retrieved31 August 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(1127) Mimi".Dictionary of Minor Planet Names. Springer Berlin Heidelberg. p. 96.doi:10.1007/978-3-540-29925-7_1128.ISBN 978-3-540-00238-3.
  3. ^abcdefgh"JPL Small-Body Database Browser: 1127 Mimi (1929 AJ)" (2017-07-03 last obs.).Jet Propulsion Laboratory. Retrieved31 August 2017.
  4. ^ab"Asteroid 1127 Mimi – Proper Elements". AstDyS-2, Asteroids – Dynamic Site. Retrieved14 March 2020.
  5. ^abc"Asteroid 1127 Mimi".Small Bodies Data Ferret. Retrieved14 March 2020.
  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.S2CID 119293330. Retrieved31 August 2017.
  7. ^abcNugent, 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.
  8. ^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. Retrieved14 March 2020.
  9. ^abcde"LCDB Data for (1127) Mimi". Asteroid Lightcurve Database (LCDB). Retrieved31 August 2017.
  10. ^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.S2CID 35447010.
  11. ^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)
  12. ^abcNugent, 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. Retrieved31 August 2017.
  13. ^abBehrend, Raoul."Asteroids and comets rotation curves – (1127) Mimi".Geneva Observatory. Retrieved31 August 2017.
  14. ^abMaleszewski, Chester; Clark, Maurice (December 2004)."Bucknell University Observatory lightcurve results for 2003-2004"(PDF).Minor Planet Bulletin.31 (4):93–94.Bibcode:2004MPBu...31...93M.ISSN 1052-8091.
  15. ^abMenke, John L. (September 2005)."Lightcurves and periods for asteroids 471 Papagena, 675 Ludmilla, 1016 Anitra, 1127 Mimi, 1165 Imprinetta, 1171 Rustahawelia, and 2283 Bunke"(PDF).Minor Planet Bulletin.32 (3):64–66.Bibcode:2005MPBu...32...64M.ISSN 1052-8091.
  16. ^Ďurech, J.; Hanuš, J.; Oszkiewicz, D.; Vančo, R. (March 2016). "Asteroid models from the Lowell photometric database".Astronomy and Astrophysics.587: A48.arXiv:1601.02909.Bibcode:2016A&A...587A..48D.doi:10.1051/0004-6361/201527573.ISSN 0004-6361.S2CID 118427201.

External links

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