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1397 Umtata

From Wikipedia, the free encyclopedia
Main-belt asteroid

1397 Umtata
Discovery[1]
Discovered byC. Jackson
Discovery siteJohannesburg Obs.
Discovery date9 August 1936
Designations
(1397) Umtata
Named after
Mthatha[2]
(South-African town)
1936 PG · 1931 GK
1945 QF · 1945 RC
1948 EB1
main-belt · (middle)[3]
background[4]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc81.14 yr (29,638 days)
Aphelion3.3646AU
Perihelion1.9967 AU
2.6806 AU
Eccentricity0.2551
4.39yr (1,603 days)
173.37°
0° 13m 28.56s / day
Inclination3.5109°
77.437°
206.53°
Physical characteristics
Dimensions20.35±0.30 km[5]
20.40 km(derived)[3]
20.798±0.292 km[6]
22.895±0.285 km[7]
30h[8]
0.0794±0.0140[7]
0.084±0.046[6]
0.10(assumed)[3]
0.112±0.004[5]
S/C[3]
B–V = 0.690[1]
U–B = 0.210[1]
11.47[1][5] · 11.57[3][7][8]

1397 Umtata, provisional designation1936 PG, is anasteroid from thebackground population of theasteroid belt's central region, approximately 21 kilometers in diameter. It was discovered by South-African astronomerCyril Jackson at theUnion Observatory in Johannesburg on 9 August 1936.[9] The asteroid was named after the South-African town ofMthatha, formerly known as Umtata.[2]

Orbit and classification

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Umtata is a non-family asteroid of the main belt'sbackground population.[4] It orbits the Sun in thecentral asteroid belt at a distance of 2.0–3.4 AU once every 4 years and 5 months (1,603 days). Its orbit has aneccentricity of 0.26 and aninclination of 4° with respect to theecliptic.[1]

The asteroid was first identified as1931 GK at theLowell Observatory in April 1931. The body'sobservation arc begins with its official discovery observation at Johannesburg.[9]

Physical characteristics

[edit]

The asteroid'sspectral type is unknown. The Lightcurve Data Base assumes anS- orC-type to be equally likely, using an average albedo of 0.10(see below).[3][a]

Rotation period

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In May 1984, a rotationallightcurve ofUmtata was obtained from photometric observations by American astronomerRichard Binzel. Analysis of the fragmentary lightcurve gave arotation period of 30 hours with a brightness amplitude of 0.13magnitude (U=1).[8] As of 2017, no secure period has been obtained.[3]

Diameter and albedo

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According to the surveys carried out by the JapaneseAkari satellite and theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer,Umtata measures between 20.35 and 22.895 kilometers in diameter and its surface has analbedo between 0.0794 and 0.112.[5][6][7]

TheCollaborative Asteroid Lightcurve Link assumes an albedo of 0.10 – a compromise value between thestony (0.20) andcarbonaceous asteroid's, both abundant in the main belt's central region – and derives a diameter of 20.40 kilometers based on anabsolute magnitude of 11.57.[3]

Naming

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Thisminor planet was named after South-African town ofMthatha, formerly known as Umtata. It is the capital town of theOR Tambo District Municipality and theKing Sabata Dalindyebo Local Municipality.[2] The officialnaming citation was published by theMinor Planet Center in April 1953 (M.P.C. 909).[10]

Notes

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  1. ^Asteroid Lightcurve Data Base (LCDB) – 2. Taxonomic Class, orbital class, and albedo. The LCDB generically assumes aS/C-type with an albedo of 0.10 for non-family main belt asteroids with asemi-major axis between 2.6 and 2.7.

References

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  1. ^abcdef"JPL Small-Body Database Browser: 1397 Umtata (1936 PG)" (2017-10-01 last obs.).Jet Propulsion Laboratory. Retrieved17 October 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(1397) Umtata".Dictionary of Minor Planet Names – (1397) Umtata.Springer Berlin Heidelberg. p. 113.doi:10.1007/978-3-540-29925-7_1398.ISBN 978-3-540-00238-3.
  3. ^abcdefgh"LCDB Data for (1397) Umtata". Asteroid Lightcurve Database (LCDB). Retrieved17 October 2017.
  4. ^ab"Asteroid 1397 Umtata – Proper Elements". AstDyS-2, Asteroids – Dynamic Site. Retrieved29 October 2019.
  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. ^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. Retrieved17 October 2017.
  7. ^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.
  8. ^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. Retrieved17 October 2017.
  9. ^ab"1397 Umtata (1936 PG)".Minor Planet Center. Retrieved17 October 2017.
  10. ^Schmadel, Lutz D. (2009). "Appendix – Publication Dates of the MPCs".Dictionary of Minor Planet Names – Addendum to Fifth Edition (2006–2008). Springer Berlin Heidelberg. p. 221.doi:10.1007/978-3-642-01965-4.ISBN 978-3-642-01964-7.

External links

[edit]
Minor planets
Asteroid
Distant minor planet
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Authority control databasesEdit this at Wikidata
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