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1093 Freda

From Wikipedia, the free encyclopedia
Carbonaceous main-belt asteroid

1093 Freda
Discovery[1]
Discovered byB. Jekhovsky
Discovery siteAlgiers Obs.
Discovery date15 June 1925
Designations
(1093) Freda
Named after
Fred Prévost
(French engineer)[2]
1925 LA · A898 VE
main-belt · (outer)[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc88.15 yr (32,198 days)
Aphelion3.9776AU
Perihelion2.2809 AU
3.1293 AU
Eccentricity0.2711
5.54yr (2,022 days)
175.72°
0° 10m 41.16s / day
Inclination25.215°
55.635°
251.42°
Physical characteristics
Dimensions88.01±27.85 km[4]
101.67±1.45 km[5]
116.73±2.9 km[6]
126.04±43.76 km[7]
10.73±0.05h[8]
10.73±0.05 h[8]
19.67±0.01 h[9][a]
19.701±0.0148 h[10]
0.03±0.02[7]
0.0381±0.002[6]
0.051±0.002[5]
0.06±0.05[4]
Tholen =C[1][3]
B–V = 0.679[1]
U–B = 0.356[1]
8.49±0.42[11] · 8.83[1][3][5][6][7] · 8.88[4] · 8.882±0.001(R)[10]

1093 Freda, provisional designation1925 LA, is a carbonaceousasteroid from the outer regions of theasteroid belt'sbackground population, approximately 110 kilometers in diameter. It was discovered on 15 June 1925, by astronomerBenjamin Jekhowsky at theAlgiers Observatory in Algeria, North Africa.[12] The asteroid was named after French engineerFred Prévost.[2]

Orbit and classification

[edit]

Freda is a non-family asteroid of the main belt'sbackground population. It orbits the Sun in theouter main-belt at a distance of 2.3–4.0 AU once every 5 years and 6 months (2,022 days). Its orbit has aneccentricity of 0.27 and aninclination of 25° with respect to theecliptic.[1]

In November 1998, the asteroid was first identified asA898 VE at theBoyden Station of the Harvard Observatory in Peru. The body'sobservation arc begins atYerkes Observatory in February 1929, almost four years after its official discovery observation at Algiers.[12]

Physical characteristics

[edit]

In theTholen classification,Freda is a common carbonaceousC-type asteroid.[1][3]

Rotation period

[edit]

Several rotationallightcurves ofFreda were obtained from photometric observations byBrian Warner, Federico Manzini, and at thePalomar Transient Factory since 2007.[8][9][10] Best-rated lightcurve analysis gave arotation period of 19.67 hours with a brightness amplitude of 0.21magnitude (U=3).[9][a]

Diameter and albedo

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According to the surveys carried out by the Infrared Astronomical SatelliteIRAS, the JapaneseAkari satellite and theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer,Freda measures between 88.01 and 126.04 kilometers in diameter and its surface has analbedo between 0.03 and 0.06.[4][5][6][7]

TheCollaborative Asteroid Lightcurve Link adopts the results obtained by IRAS, that is, an albedo of 0.0381 and a diameter of 116.73 kilometers based on anabsolute magnitude of 8.83.[3]

Naming

[edit]

Thisminor planet was named after Fred Prévost, a French civil engineer of mines and benefactor of the Faculty of sciences of Bordeaux. The official naming citation was mentioned inThe Names of the Minor Planets byPaul Herget in 1955 (H 103).[2]

Notes

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  1. ^abLightcurve plot of 1093 Freda, Palmer Divide Observatory, Brian D. Warner (2008). Summary figures for (1093) Freda at theLCDB

References

[edit]
  1. ^abcdefgh"JPL Small-Body Database Browser: 1093 Freda (1925 LA)" (2017-03-30 last obs.).Jet Propulsion Laboratory. Archived fromthe original on 18 September 2020. Retrieved25 September 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(1093) Freda".Dictionary of Minor Planet Names – (1093) Freda.Springer Berlin Heidelberg. p. 93.doi:10.1007/978-3-540-29925-7_1094.ISBN 978-3-540-00238-3.
  3. ^abcde"LCDB Data for (1093) Freda". Asteroid Lightcurve Database (LCDB). Retrieved25 September 2017.
  4. ^abcdNugent, 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.
  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. ^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.
  7. ^abcdNugent, 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. Retrieved25 September 2017.
  8. ^abcBehrend, Raoul."Asteroids and comets rotation curves – (1093) Freda".Geneva Observatory. Retrieved25 September 2017.
  9. ^abcWarner, Brian D. (October 2008)."Asteroid Lightcurve Analysis at the Palmer Divide Observatory: February-May 2008".The Minor Planet Bulletin.35 (4):163–166.Bibcode:2008MPBu...35..163W.ISSN 1052-8091. Retrieved25 September 2017.
  10. ^abcWaszczak, 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.S2CID 8342929. Retrieved25 September 2017.
  11. ^Veres, 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.S2CID 53493339. Retrieved25 September 2017.
  12. ^ab"1093 Freda (1925 LA)".Minor Planet Center. Retrieved25 September 2017.

External links

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