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5430 Luu

From Wikipedia, the free encyclopedia
Main-belt asteroid

5430 Luu
Discovery[1]
Discovered byC. Shoemaker
E. M. Shoemaker
Discovery sitePalomar Obs.
Discovery date12 May 1988
Designations
(5430) Luu
Named after
Jane Luu
(American astronomer)[2]
1988 JA1 · 1970 OL
main-belt · Phocaea[3][4]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc46.86 yr (17,114 days)
Aphelion2.8929AU
Perihelion1.8356 AU
2.3642 AU
Eccentricity0.2236
3.64yr (1,328 days)
20.073°
0° 16m 15.96s / day
Inclination23.894°
123.00°
122.11°
Physical characteristics
Dimensions6.508±0.029 km[5]
6.659±0.043[6]
7.63 km(calculated)[3]
8.05±0.22 km[7]
8.27±0.25 km[8]
4.44±0.05 h[9]
13.55±0.02h[10]
0.212±0.012[7]
0.215±0.036[8][6]
0.23(assumed)[3]
0.3826±0.0839[5]
S[3]
12.6[5] · 12.70[8] · 12.8[1][3][7] · 13.45±0.87[11]

5430 Luu, provisional designation1988 JA1, is a stony Phocaeaasteroid from the inner regions of theasteroid belt, approximately 7 kilometers in diameter. It was discovered on 12 May 1988, by American astronomer coupleCarolyn andEugene Shoemaker atPalomar Observatory, California, and later named after astronomerJane Luu.[2][12]

Orbit and classification

[edit]

Luu is a member of thePhocaea family (701).[4] It orbits the Sun in theinner main-belt at a distance of 1.8–2.9 AU once every 3 years and 8 months (1,328 days). Its orbit has aneccentricity of 0.22 and aninclination of 24° with respect to theecliptic.[1] The firstprecovery was taken atCrimea–Nauchnij in 1970, extending the asteroid'sobservation arc by 18 years prior to its discovery.[12]

Physical characteristics

[edit]

Luu has been characterized as a commonS-type asteroid.[3]

Rotation period

[edit]

In April 2006,photometric observations ofLuu collected by American astronomerBrian D. Warner at his Palmer Divide Station, Colorado, show arotation period of13.55±0.02 hours with a brightness variation of0.06±0.02magnitude (U=2).[10] A second, tentativelightcurve was obtained by French astronomerRené Roy in July 2007. It gave a period of4.44±0.05 hours and an amplitude of 0.05 in magnitude (U=2-).[9]

Diameter and albedo

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According to the surveys carried out by the JapaneseAkari satellite and NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE mission,Luu measures 6.5 and 8.3 kilometers in diameter and its surface has analbedo between 0.21 and 0.26.[5][6][7][8]

TheCollaborative Asteroid Lightcurve Link assumes an albedo of 0.23 – derived from25 Phocaea, the family's most massive member and namesake – and calculates a diameter of 7.6 kilometers with anabsolute magnitude of 12.8.[3]

Naming

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Thisminor planet is named in honor of Vietnamese-American astronomerJane X. Luu (born 1963) for her research and discovering the first and subsequent members of theKuiper Belt.[13] She also studied the physical properties of these bodies and thecoma of potentiallyExtinct comets.[2] The approved naming citation was published by theMinor Planet Center on 1 July 1996 (M.P.C. 27459).[14]

References

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  1. ^abcd"JPL Small-Body Database Browser: 5430 Luu (1988 JA1)" (2017-06-06 last obs.).Jet Propulsion Laboratory. Retrieved20 June 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(5430) Luu".Dictionary of Minor Planet Names – (5430) Luu.Springer Berlin Heidelberg. p. 464.doi:10.1007/978-3-540-29925-7_5209.ISBN 978-3-540-00238-3.
  3. ^abcdefg"LCDB Data for (5430) Luu". Asteroid Lightcurve Database (LCDB). Retrieved14 August 2016.
  4. ^ab"Asteroid 5430 Luu – Nesvorny HCM Asteroid Families V3.0".Small Bodies Data Ferret. Retrieved27 October 2019.
  5. ^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. Retrieved14 August 2016.
  6. ^abcMasiero, 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. Retrieved5 December 2016.
  7. ^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)
  8. ^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. Retrieved14 August 2016.
  9. ^abBehrend, Raoul."Asteroids and comets rotation curves – (5430) Luu".Geneva Observatory. Retrieved14 August 2016.
  10. ^abWarner, Brian D. (December 2006), "Asteroid lightcurve analysis at the Palmer Divide Observatory - March - June 2006",The Minor Planet Bulletin,33 (4):85–88,Bibcode:2006MPBu...33...85W.
  11. ^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. Retrieved14 August 2016.
  12. ^ab"5430 Luu (1988 JA1)".Minor Planet Center. Retrieved14 August 2016.
  13. ^John Keith Davies (2001).Beyond Pluto: Exploring the Outer Limits of the Solar System.Cambridge University Press. p. 219.ISBN 9781139428774. Retrieved1 June 2012.5430 Luu.
  14. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved14 August 2016.

External links

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