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1915 Quetzálcoatl

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1915 Quetzálcoatl, provisional designation 1953 EA, is a very eccentric, stony asteroid classified as near-Earth object, about half a kilometer in diameter. It was discovered on 9 March 1953, by American astronomer Albert George Wilson at Palomar Observatory, California.[4] It was named for Quetzalcoatl from Aztec mythology.[3]

1915 Quetzálcoatl
Discovery[1]
Discovered byA. G. Wilson
Discovery sitePalomar Obs.
Discovery date9 March 1953
Designations
(1915) Quetzálcoatl
Pronunciation/ˌkɛtsælkoʊˈɑːtəl/[2]
Named after
Quetzalcoatl
(Mesoamerican deity)[3]
1953 EA
NEO · Amor[1][4] · Alinda
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc51.59 yr (18,842 days)
Aphelion3.9958 AU
Perihelion1.0928 AU
2.5443 AU
Eccentricity0.5705
4.06 yr (1,482 days)
12.497°
Inclination20.402°
162.95°
347.88°
Earth MOID0.1102 AU · 42.9 LD
Physical characteristics
Dimensions0.40 km[5]
0.5 km[1]
4.9 h[6]
0.21[1]
0.31[5]
Tholen = SMU[1] · SMU[7]
B–V = 0.784[1]
U–B = 0.430[1]
18.88[7] · 18.88±0.11[8][9] · 18.90[5] · 18.97[1]

Orbit and classification

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Quetzálcoatl is an Amor asteroid – a subgroup of near-Earth asteroids that approach the orbit of Earth from beyond, but do not cross it – and a member of the Alinda family of highly eccentric asteroids. It orbits the Sun at a distance of 1.1–4.0 AU with a period of around 4 years. The osculating orbit as of 2017 has a period just over 4 years, but the period varies because Quetzálcoatl is near the 3:1 orbital resonance with Jupiter (and possibly because it is near the 1:4 resonance with Earth). Its orbit has an eccentricity of 0.57 and an inclination of 20° with respect to the ecliptic.[1]

When it was discovered in March 1953 it had a magnitude around 15, but in recent times its magnitude rarely dips below 20 because even when it is near perihelion it is far from Earth. After the 1953 close approach there were others every four years until March 1981, but the next one will not be until 77 years (19 orbits averaging 4,05 years) later, in February 2062, when its magnitude will be about 17. Its magnitude will get to around 16 (a bit less bright than in 1953) 52 years (13 orbits) later in 2114. Another close approach will occur 39 years (10 orbits) later in 2153 (average period 3.9 years). In the 285 years from 1953 to 2238 it makes 72 orbits, giving an average period of 3.96 years (quite close to a third of Jupiter's period, which comes to 3.95 years).[10]

Its Earth Minimum orbit intersection distance (MOID) is 0.1102 AU which translates into 42.9 lunar distances. On 24 February 2062, it will make a close approach and pass by Earth at a distance of 0.1339 AU (20,000,000 km).[1]

Physical characteristics

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In the Tholen classification, Quetzálcoatl is classified as a rare SMU-subtype of the broader S-type asteroids.[1] Its mean-diameter is between 0.4 and 0.5 kilometers.[5][1] It has a rotation period of 4.9 hours[6] and an albedo of 0.21–0.31.[5] In 1981, this object was observed with radar from the Arecibo Observatory at a distance of 0.09 AU. The measured radar cross-section was 0.02 km2.[11]

Naming

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This minor planet is named after the "feathered serpent" Quetzalcoatl, the Mesoamerican deity of wisdom and culture who brought learning to the Toltec people.[3] The official naming citation was published by the Minor Planet Center on 1 June 1975 (M.P.C. 3827).[12]

References

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  1. ^ a b c d e f g h i j k l m "JPL Small-Body Database Browser: 1915 Quetzalcoatl (1953 EA)" (2004-10-09 last obs.). Jet Propulsion Laboratory. Retrieved 9 June 2017.
  2. ^ "Quetzalcoatl". Oxford English Dictionary (Online ed.). Oxford University Press. (Subscription or participating institution membership required.)
  3. ^ a b c Schmadel, Lutz D. (2007). "(1915) Quetzálcoatl". Dictionary of Minor Planet Names – (1915) Quetzálcoatl. Springer Berlin Heidelberg. p. 154. doi:10.1007/978-3-540-29925-7_1916. ISBN 978-3-540-00238-3.
  4. ^ a b "1915 Quetzálcoatl (1953 EA)". Minor Planet Center. Retrieved 10 December 2016.
  5. ^ a b c d e Harris, Alan W. (February 1998). "A Thermal Model for Near-Earth Asteroids". Icarus. 131 (2): 291–301. Bibcode:1998Icar..131..291H. doi:10.1006/icar.1997.5865. Retrieved 10 December 2016.
  6. ^ a b Binzel, R. P.; Tholen, D. J. (September 1983). "The rotation, color, phase coefficient, and diameter of 1915 Quetzalcoatl". Icarus. 55 (3): 495–497. Bibcode:1983Icar...55..495B. doi:10.1016/0019-1035(83)90118-5. ISSN 0019-1035. Retrieved 10 December 2016.
  7. ^ a b "LCDB Data for (1915) Quetzálcoatl". Asteroid Lightcurve Database (LCDB). Retrieved 10 December 2016.
  8. ^ Pravec, Petr; Harris, Alan W.; Kusnirák, Peter; Galád, Adrián; Hornoch, Kamil (September 2012). "Absolute magnitudes of asteroids and a revision of asteroid albedo estimates from WISE thermal observations". Icarus. 221 (1): 365–387. Bibcode:2012Icar..221..365P. doi:10.1016/j.icarus.2012.07.026. Retrieved 10 December 2016.
  9. ^ Harris, A. W.; Young, J. W. (October 1989). "Asteroid lightcurve observations from 1979-1981". Icarus. 81 (2): 314–364. Bibcode:1989Icar...81..314H. doi:10.1016/0019-1035(89)90056-0. ISSN 0019-1035. Retrieved 10 December 2016.
  10. ^ NASA ephemeris calculator
  11. ^ Ostro, S. J.; Campbell, D. B.; Chandler, J. F.; Shapiro, I. I.; Hine, A. A.; Velez, R.; et al. (October 1991). "Asteroid radar astrometry". Astronomical Journal. 102: 1490–1502. Bibcode:1991AJ....102.1490O. doi:10.1086/115975. ISSN 0004-6256. Retrieved 10 December 2016.
  12. ^ 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.
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