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1513 Mátra

From Wikipedia, the free encyclopedia
Main-belt asteroid

1513 Mátra
Discovery[1]
Discovered byG. Kulin
Discovery siteKonkoly Obs.
Discovery date10 March 1940
Designations
(1513) Matra
Named after
Mátra(mountain range)[2]
1940 EB · 1940 EO
main-belt · Flora[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc66.67 yr (24,351 days)
Aphelion2.4085AU
Perihelion1.9763 AU
2.1924 AU
Eccentricity0.0986
3.25yr (1,186 days)
324.55°
0° 18m 12.96s / day
Inclination3.9773°
136.22°
27.140°
Physical characteristics
Dimensions4.96±0.70 km[4]
5.19±0.92 km[5]
5.85 km(calculated)[3]
6.603±0.271 km[6]
24h[7]
0.189±0.024[6]
0.24(assumed)[3]
0.31±0.19[5]
0.34±0.13[4]
S[3]
13.33[1][3][5][6] · 13.43[4]

1513 Mátra (provisional designation1940 EB) is a stony Florianasteroid from the inner regions of theasteroid belt, approximately 5 kilometers in diameter. It was discovered on 10 March 1940, by Hungarian astronomerGyörgy Kulin atKonkoly Observatory in Budapest, Hungary.[8] It was later named after theMátra mountain range.[2]

Orbit and classification

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Mátra is a member of theFlora family, a large group of stonyS-type asteroids in the inner main-belt. It orbits the Sun at a distance of 2.0–2.4 AU once every 3 years and 3 months (1,186 days). Its orbit has aneccentricity of 0.10 and aninclination of 4° with respect to theecliptic.[1]

One day prior to Mátra's official discovery observation at Konkoly, aprecovery was taken atNice Observatory. However, the body'sobservation arc begins 10 years later in 1950, when it was observed at theLa Plata Observatory in Argentina.[8]

Physical characteristics

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Rotation period

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American astronomerRichard P. Binzel obtained a rotationallight-curve of Mátra from photometric observation in the 1980s. It gave a tentativerotation period of 24 hours with a brightness variation of 0.1magnitude (U=1).[7] As of 2017, a secure period still has yet to be determined.[3]

Diameter and albedo

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According to the survey carried out by NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE mission, Mátra measures between 4.96 and 6.60 kilometers in diameter and its surface has analbedo between 0.189 and 0.34.[4][5][6]

TheCollaborative Asteroid Lightcurve Link assumes an albedo of 0.24 – derived from the family's largest body and namesake, the asteroid8 Flora – and calculates a diameter of 5.85 kilometers with anabsolute magnitude of 13.33.[3]

Naming

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Thisminor planet was named after theMátra mountain range in northern Hungary, where the outstation of the discovering Konkoly Observatory is located.[2] The official naming citation was published by theMinor Planet Center on 1 February 1980 (M.P.C. 5182).[9]

References

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  1. ^abcd"JPL Small-Body Database Browser: 1513 Matra (1940 EB)" (2017-02-14 last obs.).Jet Propulsion Laboratory. Retrieved5 June 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(1513) Mátra".Dictionary of Minor Planet Names – (1513) Mátra.Springer Berlin Heidelberg. p. 120.doi:10.1007/978-3-540-29925-7_1514.ISBN 978-3-540-00238-3.
  3. ^abcdefg"LCDB Data for (1513) Mátra". Asteroid Lightcurve Database (LCDB). Retrieved4 January 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. ^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. Retrieved4 January 2017.
  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.S2CID 46350317. Retrieved4 January 2017.
  7. ^abBinzel, R. P.; Mulholland, J. D. (December 1983)."A photoelectric lightcurve survey of small main belt asteroids".Icarus.56 (3):519–533.Bibcode:1983Icar...56..519B.doi:10.1016/0019-1035(83)90170-7.ISSN 0019-1035. Retrieved4 January 2017.
  8. ^ab"1513 Matra (1940 EB)".Minor Planet Center. Retrieved4 January 2017.
  9. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved4 January 2017.

External links

[edit]
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