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1393 Sofala

From Wikipedia, the free encyclopedia
Main-belt asteroid

1393 Sofala
Discovery[1]
Discovered byC. Jackson
Discovery siteJohannesburg Obs.
Discovery date25 May 1936
Designations
(1393) Sofala
Named after
Sofala
(Province in Mozambique)[2]
1936 KD · 1928 FB
1951 GL · 1956 TE
1958 CA · 1971 SJ
1975 UB
main-belt · (inner)
Vestian[3] · background[4]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc89.54 yr (32,703 days)
Aphelion2.6997AU
Perihelion2.1685 AU
2.4341 AU
Eccentricity0.1091
3.80yr (1,387 days)
146.78°
0° 15m 34.2s / day
Inclination5.8476°
56.701°
183.46°
Physical characteristics
Dimensions11.214±0.495 km[5]
11.30 km(calculated)[3]
7.8h(poor)[6]
16.5931±0.0005 h[7]
108.259±0.7031 h[8]
0.20(assumed)[3]
0.223±0.046[5]
S(assumed)[3]
11.835±0.002(R)[8] · 12.00[5] · 12.1[1][3] · 12.42±0.78[9]

1393 Sofala, provisional designation1936 KD, is a Vestianasteroid from the inner regions of theasteroid belt, approximately 11 kilometers in diameter. It was discovered on 25 May 1936, by South African astronomerCyril Jackson at theUnion Observatory in Johannesburg.[10] The asteroid was named after the province ofSofala in Mozambique.[2]

Orbit and classification

[edit]

Sofala is a member of theVesta family (401),[3] the second-largest asteroid family of the main-belt by number of members. However, it is also considered to be a non-family asteroid of the main belt'sbackground population when applying theHierarchical Clustering Method to itsproper orbital elements.[4] It orbits the Sun in theinner asteroid belt at a distance of 2.2–2.7 AU once every 3 years and 10 months (1,387 days). Its orbit has aneccentricity of 0.11 and aninclination of 6° with respect to theecliptic.[1]

The asteroid was first identified as1928 FB atHeidelberg Observatory in March 1928. The body'sobservation arc begins with its official discovery observation at Johannesburg in 1936.[10]

Physical characteristics

[edit]

Sofala is an assumed stonyS-type asteroid.[3]

Rotation period

[edit]

The asteroid has an ambiguouslightcurve. While a lightcurve, obtained at thePalomar Transient Factory in September 2013, gave arotation period of 108.259 hours with a brightness amplitude of 0.48magnitude (U=2),[8] another lightcurve modeled from combined dense and sparse photometry gave a sidereal period of 16.5931 hours.(U=2).[7] If the first result were correct,Sofala would be one of few hundred knownslow rotators with a period above 100 hours. The Lightcurve Data Base, however, adopts the shorter period from the modeled lightcurve.[3] A third lightcurve with a period of 7.8 hours byRené Roy from 2008 has received a poor rating.[6]

Diameter and albedo

[edit]

According to the survey carried out by theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer,Sofala measures between 11.21 kilometers in diameter and its surface has analbedo of 0.223.[5]

TheCollaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20 and calculates a diameter of 11.30 kilometers based on anabsolute magnitude of 12.1.[3]

Naming

[edit]

Thisminor planet was named afterSofala Province in central-eastern Mozambique. It is the country's largest province.[2] Its capital city isBeira after which the Mars-crosser1474 Beira, another discovery by Cyril Jackson, is named. The officialnaming citation was published by theMinor Planet Center in April 1953 (M.P.C. 909).[11]

References

[edit]
  1. ^abcd"JPL Small-Body Database Browser: 1393 Sofala (1936 KD)" (2017-09-29 last obs.).Jet Propulsion Laboratory. Retrieved24 October 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(1393) Sofala".Dictionary of Minor Planet Names – (1393) Sofala.Springer Berlin Heidelberg. p. 113.doi:10.1007/978-3-540-29925-7_1394.ISBN 978-3-540-00238-3.
  3. ^abcdefghi"LCDB Data for (1393) Sofala". Asteroid Lightcurve Database (LCDB). Retrieved24 October 2017.
  4. ^ab"Asteroid 1393 Sofala – Proper Elements". AstDyS-2, Asteroids – Dynamic Site. Retrieved29 October 2019.
  5. ^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. Retrieved24 October 2017.
  6. ^abBehrend, Raoul."Asteroids and comets rotation curves – (1393) Sofala".Geneva Observatory. Retrieved24 October 2017.
  7. ^abHanus, J.; Durech, J.; Broz, M.; Marciniak, A.; Warner, B. D.; Pilcher, F.; et al. (March 2013). "Asteroids' physical models from combined dense and sparse photometry and scaling of the YORP effect by the observed obliquity distribution".Astronomy and Astrophysics.551: 16.arXiv:1301.6943.Bibcode:2013A&A...551A..67H.doi:10.1051/0004-6361/201220701.
  8. ^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. Retrieved24 October 2017.
  9. ^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. Retrieved24 October 2017.
  10. ^ab"1393 Sofala (1936 KD)".Minor Planet Center. Retrieved24 October 2017.
  11. ^Schmadel, Lutz D. "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]
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