Movatterモバイル変換


[0]ホーム

URL:


Jump to content
WikipediaThe Free Encyclopedia
Search

1428 Mombasa

From Wikipedia, the free encyclopedia
Main-belt asteroid

1428 Mombasa
Discovery[1]
Discovered byC. Jackson
Discovery siteJohannesburg Obs.
Discovery date5 July 1937
Designations
(1428) Mombasa
Named after
Mombasa(city, port)[2]
1937 NO · 1933 WO
1949 FA · 1957 YZ
main-belt · (middle)
Orbital characteristics[1]
Epoch 16 February 2017 (JD 2457800.5)
Uncertainty parameter 0
Observation arc82.74 yr (30,219 days)
Aphelion3.2039AU
Perihelion2.4154 AU
2.8096 AU
Eccentricity0.1403
4.71yr (1,720 days)
263.81°
0° 12m 33.48s / day
Inclination17.305°
115.72°
252.61°
Physical characteristics
Dimensions52.464±0.268 km[3]
53.35±13.28 km[4]
55.34±0.70 km[5]
56.63±2.0 km[6]
56.83 km(derived)[7]
57.59±19.41 km[8]
62.45±0.73 km[9]
127.203±29.18 km[10]
16.67±0.01 h[a]
17.12±0.01h[11]
17.6±0.2 h[12]
0.0010±0.0099[10]
0.0240±0.002[6]
0.025±0.001[5]
0.038±0.004[9]
0.04±0.04[8]
0.0415(derived)[7]
0.06±0.06[4]
SMASS = Xc[1] · P[10] · C[7]
9.95±0.74[13] · 10.20[8][9] · 10.27[4] · 10.3[1][7] · 10.9[5][6][10]

1428 Mombasa, provisional designation1937 NO, is a darkasteroid from the middle region of theasteroid belt, approximately 56 kilometers in diameter.

It was discovered on 5 July 1937, by English-born South African astronomerCyril Jackson atJohannesburg Observatory, South Africa, and later named afterMombasa, Kenya.[2][14]

Orbit and classification

[edit]

Mombasa orbits the Sun at a distance of 2.4–3.2 AU once every 4 years and 9 months (1,720 days). Its orbit has aneccentricity of 0.14 and aninclination of 17° with respect to theecliptic.[1]Mombasa was first identified as1933 WO atLowell Observatory, extending the body'sobservation arc by 4 years prior to its official discovery at Johannesburg.[14]

Physical characteristics

[edit]

Rotation period

[edit]

American astronomerRobert Stephens obtained a rotationallightcurve ofMombasa in June 2012. Light-curve analysis gave arotation period of 16.67 hours with a brightness variation of 0.16magnitude (U=2+).[a] Previous lightcurves were obtained by French amateur astronomerRené Roy in February 2006 (17.6 hours, Δ0.15 mag;U=2),[12] as well as by Scot Hawkins and Richard Ditteon atOakley Observatory in May 2007 (17.12 hours, Δ0.25 mag;U=2).[11]

Spectral type, diameter and albedo

[edit]

On theSMASS taxonomic scheme,Mombasa is aXc-type, an intermediate between the carbonaceousC andX-type, while it is also described as a darkerP-type asteroid.[10] According to the surveys carried out by the Infrared Astronomical SatelliteIRAS, the JapaneseAkari satellite, and NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE mission,Mombasa measures between 52.46 and 62.45 kilometers in diameter, ignoring a preliminary result of 127 km,[10] and its surface has analbedo of 0.025 and 0.06.[3][4][5][6][8][9] TheCollaborative Asteroid Lightcurve Link derives an albedo of 0.0415 and a diameter of 56.83 kilometers with anabsolute magnitude of 10.3.[7]

Naming

[edit]

Thisminor planet was named afterMombasa, chief-port and second largest city ofKenya on the coast of East Africa.[2] The officialnaming citation was published by theMinor Planet Center in April 1953 (M.P.C. 909).[15]

Notes

[edit]
  1. ^abStephens (2012) web: rotation period16.67±0.01 hours with a brightness amplitude of0.16 mag. Notes: "A half-period of 8.38 h cannot be formally excluded". Summary figures atCollaborative Asteroid Lightcurve Link (CALL) for (1428) Mombasa

References

[edit]
  1. ^abcde"JPL Small-Body Database Browser: 1428 Mombasa (1937 NO)" (2016-08-13 last obs.).Jet Propulsion Laboratory. Archived fromthe original on 20 August 2020. Retrieved6 January 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(1428) Mombasa".Dictionary of Minor Planet Names – (1428) Mombasa.Springer Berlin Heidelberg. p. 115.doi:10.1007/978-3-540-29925-7_1429.ISBN 978-3-540-00238-3.
  3. ^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.S2CID 119293330. Retrieved6 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. ^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. ^abcde"LCDB Data for (1428) Mombasa". Asteroid Lightcurve Database (LCDB). Retrieved6 January 2017.
  8. ^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. Retrieved6 January 2017.
  9. ^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. Retrieved6 January 2017.
  10. ^abcdefMainzer, 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.S2CID 35447010.
  11. ^abHawkins, Scot; Ditteon, Richard (March 2008)."Asteroid Lightcurve Analysis at the Oakley Observatory - May 2007".The Minor Planet Bulletin.35 (1):1–4.Bibcode:2008MPBu...35....1H.ISSN 1052-8091. Retrieved6 January 2017.
  12. ^abBehrend, Raoul."Asteroids and comets rotation curves – (1428) Mombasa".Geneva Observatory. Retrieved6 January 2017.
  13. ^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. Retrieved6 January 2017.
  14. ^ab"1428 Mombasa (1937 NO)".Minor Planet Center. Retrieved6 January 2017.
  15. ^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.Bibcode:2009dmpn.book.....S.doi:10.1007/978-3-642-01965-4.ISBN 978-3-642-01964-7.

External links

[edit]
Minor planets
Asteroid
Distant minor planet
Comets
Other
Authority control databasesEdit this at Wikidata
Retrieved from "https://en.wikipedia.org/w/index.php?title=1428_Mombasa&oldid=1313036777"
Categories:
Hidden categories:

[8]ページ先頭

©2009-2025 Movatter.jp