4760 Jia-xiang
Discovery [1] | |
---|---|
Discovered by | Harvard College Obs. |
Discovery site | Oak Ridge Obs. |
Discovery date | 1 April 1981 |
Designations | |
(4760) Jia-xiang | |
Named after | Zhang Jiaxiang [1] (Chinese astronomer) |
1981 GN1 · 1981 GP1 1982 SE5 | |
main-belt [1][2] · (inner)[3] background [4] | |
Orbital characteristics [2] | |
Epoch 23 March 2018 (JD 2458200.5) | |
Uncertainty parameter 0 | |
Observation arc | 62.47 yr (22,817 d) |
Aphelion | 2.6236 AU |
Perihelion | 2.0279 AU |
2.3258 AU | |
Eccentricity | 0.1281 |
3.55 yr (1,296 d) | |
37.063° | |
0° 16m 40.44s / day | |
Inclination | 9.8513° |
177.82° | |
130.44° | |
Physical characteristics | |
4.71 km (calculated)[3] 4.79±1.41 km[5] 5.137±0.036 km[6][7] 5.16±1.28 km[8] | |
14.96±0.0006 h[a][b] 14.9601 h[a][b] | |
0.13±0.06[8] 0.20 (assumed)[3] 0.21±0.15[5] 0.227±0.042[6] 0.2275±0.0418[7] | |
S (assumed)[3] | |
13.56±0.40[9] · 13.7[7] · 13.90[5] · 14.0[2][3] · 14.29[8] | |
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.[1] The presumed stony S-type asteroid was named after Chinese astronomer Zhang Jiaxiang. It has a rotation period of 14.96 hours.[a][b]
Orbit and classification
Jia-xiang is a non-family asteroid from the main belt's background population.[4] 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.[2] 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.[1]
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).[a][b]
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.[5][6][7][8]
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.[3]
Naming
This minor planet was named after Chinese astronomer Zhang Jiaxiang (born 1932).[1] The official naming citation was published by the Minor Planet Center on 21 November 1991 (M.P.C. 19339).[10]
Notes
- ^ a b c d 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)
- ^ a b c d Lightcurve plot A and plot B of (4760) Jia-xiang, from Ondrejov data obtained by the NEO Photometric Program and collaborating projects
References
- ^ a b c d e f "4760 Jia-xiang (1981 GN1)". Minor Planet Center. Retrieved 3 April 2018.
- ^ a b c d "JPL Small-Body Database Browser: 4760 Jia-xiang (1981 GN1)" (2017-07-05 last obs.). Jet Propulsion Laboratory. Retrieved 3 April 2018.
- ^ a b c d e f "LCDB Data for (4760) Jia-xiang". Asteroid Lightcurve Database (LCDB). Retrieved 3 April 2018.
- ^ a b "Asteroid 4760 Jia-xiang – Proper Elements". AstDyS-2, Asteroids – Dynamic Site. Retrieved 29 October 2019.
- ^ a b c d 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.
- ^ a b c 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.
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: CS1 maint: multiple names: authors list (link) - ^ a b c d 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.
- ^ a b c d 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.
{{cite journal}}
: CS1 maint: unflagged free DOI (link) - ^ 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.
- ^ "MPC/MPO/MPS Archive". Minor Planet Center. Retrieved 3 April 2018.
External links
- Asteroid Lightcurve Database (LCDB), query form (info)
- Dictionary of Minor Planet Names, Google books
- Asteroids and comets rotation curves, CdR – Observatoire de Genève, Raoul Behrend
- Discovery Circumstances: Numbered Minor Planets (1)-(5000) – Minor Planet Center
- 4760 Jia-xiang at AstDyS-2, Asteroids—Dynamic Site
- 4760 Jia-xiang at the JPL Small-Body Database