5751 Zao Explained

Minorplanet:yes
Background:
  1. FFC2E0
5751 Zao
Discovery Ref:[1]
Discoverer:M. Koishikawa
Discovery Site:Ayashi Station
Discovered:5 January 1992
Mpc Name:(1992) AC
Alt Names:MPO 319156, 1989 EN1
Named After:Mount Zaō
Mp Category:
NEO
Orbit Ref:[2]
Uncertainty:0
Epoch:13 January 2016 (JD 2457400.5)
Observation Arc:9792 days (26.81 yr)
Aphelion:2.994076221abbr=onNaNabbr=on
Perihelion:1.21174819AU
Semimajor:2.102912204AU
Eccentricity:0.423776140
Period:3.05 yr (1113.9 d)
Inclination:16.0739405°
Asc Node:121.691193°
Mean Anomaly:300.120144°
Mean Motion: / day
Arg Peri:25.2587992°
Moid:0.244159AU
Rotation:76abbr=onNaNabbr=on
Albedo:0.36
Abs Magnitude:14.8

5751 Zao, provisional designation, is an Amor asteroid discovered by Japanese astronomer M. Koishikawa at the Ayashi Station of the Sendai Astronomical Observatory on 5 January 1992

Physical properties

Zao has been observed by several groups to determine its rotational period. Its light curve was observed by Pravec, et al. between 1992 and 1995 with the intention of determining its rotational period. From its nearly constant brightness it was determined that the asteroid is roughly spherical and has a rotational period of ≥ 21.7 hr.[3] Another group led by Wisniewski conducted an approximately 5 hour observation and were unable to conclude a rotational period.[4] Zao was again observed in 2001 by Delbó, et al. using the Keck telescope. They were able to determine the asteroid's albedo of 0.36 and re-classify the asteroid from X-type to E-type.[5] Using the asteroid's albedo and the Near Earth Asteroid Thermal Model (NEATM) the asteroid's diameter was estimated to be 2.3 km.[5] Further study of the asteroid by the Ondrejov Asteroid Photometry Project concludes that a rotational period of 76 hours is consistent with earlier measurements.[6] [7]

External links

Notes and References

  1. Web site: (5751) Zao = 1992 AC = 1989 EN1. Minor Planet Center. 2015-06-04.
  2. Web site: 5751 Zao (1992 AC) . . . 13 April 2016.
  3. The Near-Earth Objects Follow-Up Program . P. . Pravec . . December 1997 . 130 . 2 . 275–286 . 10.1006/icar.1997.5816 . 1997Icar..130..275P. etal.
  4. Photometric Observations of 125 Asteroids . W. Z. . Wisniewski . MichaŁowski, T. M.. Harris, A. W.. McMillan, R. S.. April 1997 . . 126 . 2 . 395–449 . 10.1006/icar.1996.5665 . 1997Icar..126..395W.
  5. Keck observations of near-Earth asteroids in the thermal infrared . Marco . Delbó . Harris, Alan W.. Binzel, Richard P.. Pravec, Petr. Davies, John K. . November 2003 . . 166 . 1 . 116–130 . 10.1016/j.icarus.2003.07.002 . 2003Icar..166..116D.
  6. Web site: 5751 Zao . European Asteroid Research Node . 2008-03-30 . https://web.archive.org/web/20140227010907/http://earn.dlr.de/nea/005751.htm . 2014-02-27 . dead .
  7. Web site: Ondrejov Asteroid Photometry Project: Summary of Prepublished Data .