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1474 Beira

From Wikipedia, the free encyclopedia
Asteroid
1474 Beira
Discovery[1]
Discovered byC. Jackson
Discovery siteJohannesburg Obs.
Discovery date20 August 1935
Designations
(1474) Beira
Named after
Beira[2]
(city in Mozambique)
1935 QY · 1950 DQ
Mars-crosser[1][3][4]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc81.06 yr (29,606 d)
Aphelion4.0740AU
Perihelion1.3920 AU
2.7330 AU
Eccentricity0.4907
4.52yr (1,650 days)
19.609°
0° 13m 5.16s / day
Inclination26.683°
323.50°
84.070°
Physical characteristics
Dimensions8.73 km(calculated)[4]
14.9±1.5 km[5]
15±2 km[6]
15.46±1.55 km[7]
4.184±0.001h[8][9][a]
4.184±0.002 h[10]
0.06±0.01[6]
0.064±0.013[7]
0.07±0.01[5]
0.20(assumed)[4]
Tholen =FX[1]
SMASS =B[1][4]
B–V = 0.620[1]
U–B = 0.245[1]
12.66[1][4][5][6][7]

1474 Beira, provisional designation1935 QY, is a bright carbonaceousasteroid and largeMars-crosser on an eccentric orbit from theasteroid belt, approximately 15 kilometers in diameter. It was discovered on 20 August 1935, by South African astronomerCyril Jackson at theUnion Observatory in Johannesburg.[3] The asteroid was named after the port city ofBeira in Mozambique.[2]

Orbit and classification

[edit]

Beira is aMars-crossing asteroid, a dynamically unstable group between themain belt and thenear-Earth populations, crossing the orbit of Mars at 1.666 AU. It orbits the Sun at a distance of 1.4–4.1 AU once every 4 years and 6 months (1,650 days). Its orbit has a higheccentricity of 0.49 and aninclination of 27° with respect to theecliptic.[1] The body'sobservation arc begins with its official discovery observation at Johannesburg in 1935.[3]

Physical characteristics

[edit]

In theSMASS classification,Beira is a bright carbonaceousB-type asteroid, while in theTholen classification itsspectral type is ambiguous, closest to anF-type and somewhat similar to that of anX-type asteroid.[1]

Rotation period

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Three rotationallightcurves ofBeira were obtained from photometric observations. Lightcurve analysis gave a well-definedrotation period of 4.184 hours with a brightness amplitude between 0.15 and 0.24magnitude (U=3/3/3).[8][9][10][a]

Diameter and albedo

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According to the survey carried out by theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer,Beira measures between 14.9 and 15.46 kilometers in diameter and its surface has a lowalbedo between 0.06 and 0.07.[5][6][7] Conversely, theCollaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20 and consequently calculates a smaller diameter of 8.73 kilometers using anabsolute magnitude of 12.66.[4]

With a diameter close to 15 kilometers,Beira is larger than most sizeableMars-crossing asteroids such as1065 Amundsenia (9.75 km),1139 Atami (9.35 km),1011 Laodamia (7.39 km),1727 Mette (est 9 km),1131 Porzia (7.13 km),1235 Schorria (est. 9 km),985 Rosina (8.18 km)1310 Villigera (15.24 km), and1468 Zomba (7 km); but still smaller than the largest members of this dynamical group, namely,132 Aethra,323 Brucia,1508 Kemi,2204 Lyyli and512 Taurinensis, which are larger than 20 kilometers in diameter (in one or other given source).

Naming

[edit]

Thisminor planet was named after the port city ofBeira in Mozambique.[2] The officialnaming citation was published by theMinor Planet Center in April 1953 (M.P.C. 909).[11]

Notes

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  1. ^abLightcurve plot of (1474) Beira, Robert Koff, Antelope Hills Observatory (H09). Summary figures atLCDB

References

[edit]
  1. ^abcdefghij"JPL Small-Body Database Browser: 1474 Beira (1935 QY)" (2016-09-09 last obs.).Jet Propulsion Laboratory. Retrieved21 October 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(1474) Beira".Dictionary of Minor Planet Names – (1474) Beira.Springer Berlin Heidelberg. p. 118.doi:10.1007/978-3-540-29925-7_1475.ISBN 978-3-540-00238-3.
  3. ^abc"1474 Beira (1935 QY)".Minor Planet Center. Retrieved21 October 2017.
  4. ^abcdef"LCDB Data for (1474) Beira". Asteroid Lightcurve Database (LCDB). Retrieved21 October 2017.
  5. ^abcdAlí-Lagoa, V.; Licandro, J.; Gil-Hutton, R.; Cañ; ada-Assandri, M.; Delbo', M.; et al. (June 2016)."Differences between the Pallas collisional family and similarly sized B-type asteroids".Astronomy and Astrophysics.591: 11.Bibcode:2016A&A...591A..14A.doi:10.1051/0004-6361/201527660.hdl:11336/63614. Retrieved21 October 2017.
  6. ^abcdAlí-Lagoa, V.; de León, J.; Licandro, J.; Delbó, M.; Campins, H.; Pinilla-Alonso, N.; et al. (June 2013)."Physical properties of B-type asteroids from WISE data".Astronomy and Astrophysics.554: 16.arXiv:1303.5487.Bibcode:2013A&A...554A..71A.doi:10.1051/0004-6361/201220680. Retrieved21 October 2017.
  7. ^abcdAlí-Lagoa, V.; Delbo', M. (July 2017)."Sizes and albedos of Mars-crossing asteroids from WISE/NEOWISE data"(PDF).Astronomy and Astrophysics.603: 8.arXiv:1705.10263.Bibcode:2017A&A...603A..55A.doi:10.1051/0004-6361/201629917. Retrieved21 October 2017.
  8. ^abStrabla, Luca; Quadri, Ulisse; Girelli, Robert (April 2013)."Asteroid Observed from Bassano Bresciano Observatory 2012 August-September".The Minor Planet Bulletin.40 (2):83–84.Bibcode:2013MPBu...40...83S.ISSN 1052-8091. Retrieved21 October 2017.
  9. ^abKoff, Robert A. (June 2004)."Lightcurve photometry of Mars-crossing asteroids 1474 Beira and 3674 Erbisbuhl".The Minor Planet Bulletin.31 (2):33–34.Bibcode:2004MPBu...31...33K.ISSN 1052-8091. Retrieved21 October 2017.
  10. ^abApostolovska, Gordana; Ivanova, Violeta; Borisov, Galin (June 2004)."Lightcurves and rotational periods of 1474 Beira, 1309 Hyperborea, and 2525 O'Steen".The Minor Planet Bulletin.31 (2):44–45.Bibcode:2004MPBu...31...44A.ISSN 1052-8091. Retrieved21 October 2017.
  11. ^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

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