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4760 Jia-xiang

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Background asteroid from the inner regions of the asteroid belt

4760 Jia-xiang
Discovery 
Discovered byHarvard College Obs.
Discovery siteOak Ridge Obs.
Discovery date1 April 1981
Designations
MPC designation(4760) Jia-xiang
Named afterZhang Jiaxiang
(Chinese astronomer)
Alternative designations1981 GN1 · 1981 GP1
1982 SE5
Minor planet categorymain-belt  · (inner)
background
Orbital characteristics
Epoch 23 March 2018 (JD 2458200.5)
Uncertainty parameter 0
Observation arc62.47 yr (22,817 d)
Aphelion2.6236 AU
Perihelion2.0279 AU
Semi-major axis2.3258 AU
Eccentricity0.1281
Orbital period (sidereal)3.55 yr (1,296 d)
Mean anomaly37.063°
Mean motion0° 16 40.44 / day
Inclination9.8513°
Longitude of ascending node177.82°
Argument of perihelion130.44°
Physical characteristics
Mean diameter4.71 km (calculated)
4.79±1.41 km
5.137±0.036 km
5.16±1.28 km
Synodic rotation period14.96±0.0006 h
14.9601 h
Geometric albedo0.13±0.06
0.20 (assumed)
0.21±0.15
0.227±0.042
0.2275±0.0418
Spectral typeS (assumed)
Absolute magnitude (H)13.56±0.40 · 13.7 · 13.90 · 14.0 · 14.29

4760 Jia-xiang, provisional designation 1981 GN1, is a background asteroid from the inner regions of the asteroid belt, approximately 5 kilometers (3 miles) in diameter. It was discovered on 1 April 1981, by astronomers at Harvard University's Oak Ridge Observatory in Massachusetts, United States. The presumed stony S-type asteroid was named after Chinese astronomer Zhang Jiaxiang. It has a rotation period of 14.96 hours.

Orbit and classification

Jia-xiang is a non-family asteroid from the main belt's background population. It orbits the Sun in the inner main-belt at a distance of 2.0–2.6 AU once every 3 years and 7 months (1,296 days; semi-major axis of 2.33 AU). Its orbit has an eccentricity of 0.13 and an inclination of 10° with respect to the ecliptic. The body's observation arc begins with a precovery taken at Palomar Observatory in January 1955, or 26 years prior to its official discovery observation at Oak Ridge.

Physical characteristics

Rotation period

In 2017, two rotational lightcurves of Jia-xiang were obtained from photometric observations by Czech astronomer Petr Pravec at Ondřejov Observatory. Lightcurve analysis gave a rotation period of 14.96 and 14.9601 hours with a brightness amplitude of 0.55 and 0.63 magnitude, respectively (U=3/3).

Diameter and albedo

According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Jia-xiang measures between 4.79 and 5.16 kilometers in diameter and its surface has an albedo between 0.13 and 0.2275.

The Collaborative Asteroid Lightcurve Link assumes an albedo of 0.20 and calculates a diameter of 4.71 kilometers based on an absolute magnitude of 14.0.

Naming

This minor planet was named after Chinese astronomer Zhang Jiaxiang (born 1932). The official naming citation was published by the Minor Planet Center on 21 November 1991 (M.P.C. 19339).

Notes

  1. ^ Pravec (2017) web: rotation period 14.96±0.02 and 14.9601±0.0006 hours with a brightness amplitude of 0.55±0.02 and 0.63±0.02 mag. Quality Code is 3/3. Summary figures at the LCDB and Pravec, P.; Wolf, M.; Sarounova, L. (2017)
  2. ^ Lightcurve plot A and plot B of (4760) Jia-xiang, from Ondrejov data obtained by the NEO Photometric Program and collaborating projects

References

  1. ^ "4760 Jia-xiang (1981 GN1)". Minor Planet Center. Retrieved 3 April 2018.
  2. ^ "JPL Small-Body Database Browser: 4760 Jia-xiang (1981 GN1)" (2017-07-05 last obs.). Jet Propulsion Laboratory. Retrieved 3 April 2018.
  3. ^ "LCDB Data for (4760) Jia-xiang". Asteroid Lightcurve Database (LCDB). Retrieved 3 April 2018.
  4. ^ "Asteroid 4760 Jia-xiang – Proper Elements". AstDyS-2, Asteroids – Dynamic Site. Retrieved 29 October 2019.
  5. ^ Nugent, 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.
  6. ^ Masiero, Joseph R.; Mainzer, A. K.; Grav, T.; Bauer, J. M.; Cutri, R. M.; Dailey, J.; et al. (November 2011). "Main Belt Asteroids with WISE/NEOWISE. I. Preliminary Albedos and Diameters". The Astrophysical Journal. 741 (2): 20. arXiv:1109.4096. Bibcode:2011ApJ...741...68M. doi:10.1088/0004-637X/741/2/68. S2CID 118745497.
  7. ^ Mainzer, 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.
  8. ^ Nugent, 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.
  9. 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.
  10. "MPC/MPO/MPS Archive". Minor Planet Center. Retrieved 3 April 2018.

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