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1368 Numidia

From Wikipedia, the free encyclopedia
Asteroid

1368 Numidia
Modelled shape ofNumidia from itslightcurve
Discovery[1]
Discovered byC. Jackson
Discovery siteJohannesburg Obs.
Discovery date30 April 1935
Designations
(1368) Numidia
Pronunciation/njˈmɪdiə/[2]
Named after
Numidia[3]
(ancient Berber kingdom)
1935 HD · 1928 SN
1931 JF · 1935 KB
1936 QN · 1953 YK
main-belt · (inner)[4]
background[5] · Maria[6]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc86.45 yr (31,577 days)
Aphelion2.6814AU
Perihelion2.3673 AU
2.5243 AU
Eccentricity0.0622
4.01yr (1,465 days)
146.05°
0° 14m 44.52s / day
Inclination14.823°
18.130°
264.36°
Physical characteristics
Dimensions15.93±0.37 km[7]
19.24 km(derived)[4]
19.29±0.9 km[8]
19.591±0.213 km[9]
19.899±0.110 km[10]
20.66±0.82 km[11]
3.64h[12]
3.640739 h[13]
3.640740 h[14]
0.177±0.016[11]
0.1838±0.0295[10]
0.1918(derived)[4]
0.2035±0.019[8]
0.298±0.021[7]
S(assumed)[4]
B–V = 0.860[1]
U–B = 0.360[1]
10.92[1][7][8][11] · 10.99[4][10][12]

1368 Numidia, provisional designation1935 HD, is a stonybackground asteroid from the central regions of theasteroid belt, approximately 19 kilometers in diameter. It was discovered on 30 April 1935, by South African astronomerCyril Jackson at theUnion Observatory in Johannesburg.[15] The asteroid was named after the ancient North African kingdom ofNumidia.[3]

Orbit and classification

[edit]

Based on thehierarchical clustering method,Numidia has both been classified as a non-family asteroid from the main belt'sbackground population (Nesvorný),[5] and as a core member of theMaria family (Milani and Knežević).[6] It orbits the Sun in theintermediate asteroid belt at a distance of 2.4–2.7 AU once every 4.01 years (1,465 days;semi-major axis of 2.52 AU). Its orbit has aneccentricity of 0.06 and aninclination of 15° with respect to theecliptic.[1]

The asteroid was first identified as1928 SN atUccle Observatory in September 1928. The body'sobservation arc begins at Johannesburg in May 1931, three weeks after its official discovery observation.[15]

Naming

[edit]

Thisminor planet was named after the ancientBerber kingdom ofNumidia, that was located in North Africa, in what is now Algeria. The official naming citation was mentioned inThe Names of the Minor Planets byPaul Herget in 1955 (H 124).[3]

Physical characteristics

[edit]

Numidia is an assumed stonyS-type asteroid.[4]

Rotation period and poles

[edit]

In May 1983, a first rotationallightcurve ofNumidia was obtained from photometric observations by American astronomerRichard Binzel. Lightcurve analysis gave a well-definedrotation period of 3.64 hours with a brightness amplitude of 0.35magnitude (U=3).[12]

Modeling of the asteroid's lightcurve gave a concurring sidereal period of 3.640739 and 3.640740 hours, respectively.[13][14] In 2016, modeling also determined a pole of (201.0°, −62.0°) inecliptic coordinates (λ, β).[13]

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,Numidia measures between 15.93 and 20.66 kilometers in diameter and its surface has analbedo between 0.177 and 0.298.[7][8][9][10][11]

TheCollaborative Asteroid Lightcurve Link derives an albedo of 0.1918 and a diameter of 19.24 kilometers based on anabsolute magnitude of 10.99.[4]

References

[edit]
  1. ^abcdef"JPL Small-Body Database Browser: 1368 Numidia (1935 HD)" (2017-11-01 last obs.). Jet Propulsion Laboratory. Retrieved9 November 2017.
  2. ^"Numidian".Oxford English Dictionary (Online ed.). Oxford University Press. (Subscription orparticipating institution membership required.)
  3. ^abcSchmadel, Lutz D. (2007). "(1368) Numidia".Dictionary of Minor Planet Names – (1368) Numidia. Springer Berlin Heidelberg. p. 111.doi:10.1007/978-3-540-29925-7_1369.ISBN 978-3-540-00238-3.
  4. ^abcdefg"LCDB Data for (1368) Numidia". Asteroid Lightcurve Database (LCDB). Retrieved9 November 2017.
  5. ^ab"Small Bodies Data Ferret".Nesvorny HCM Asteroid Families V3.0. Archived fromthe original on 2 August 2017. Retrieved9 November 2017.
  6. ^ab"Asteroid 1368 Numidia – Proper Elements". AstDyS-2, Asteroids – Dynamic Site. Retrieved29 October 2019.
  7. ^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. Retrieved9 November 2017.
  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. Retrieved22 October 2019.
  9. ^abMasiero, 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. Retrieved9 November 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.
  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. ^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. Retrieved9 November 2017.
  13. ^abcHanus, J.; Durech, J.; Oszkiewicz, D. A.; Behrend, R.; Carry, B.; Delbo, M.; et al. (February 2016). "New and updated convex shape models of asteroids based on optical data from a large collaboration network".Astronomy and Astrophysics.586: 24.arXiv:1510.07422.Bibcode:2016A&A...586A.108H.doi:10.1051/0004-6361/201527441.
  14. ^abHanus, J.; Durech, J.; Broz, M.; Warner, B. D.; Pilcher, F.; Stephens, R.; et al. (June 2011)."A study of asteroid pole-latitude distribution based on an extended set of shape models derived by the lightcurve inversion method".Astronomy & Astrophysics.530: 16.arXiv:1104.4114.Bibcode:2011A&A...530A.134H.doi:10.1051/0004-6361/201116738. Retrieved9 November 2017.
  15. ^ab"1368 Numidia (1935 HD)".Minor Planet Center. Retrieved9 November 2017.

External links

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