Misplaced Pages

6980 Kyusakamoto

Article snapshot taken from Wikipedia with creative commons attribution-sharealike license. Give it a read and then ask your questions in the chat. We can research this topic together.

6980 Kyusakamoto
Discovery 
Discovered byK. Endate
K. Watanabe
Discovery siteKitami Obs.
Discovery date16 September 1993
Designations
MPC designation(6980) Kyusakamoto
Named afterKyu Sakamoto
(Japanese singer)
Alternative designations1993 SV1 · 1979 WH7
1988 RU13
Minor planet categorymain-belt · Koronis
Orbital characteristics
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc36.98 yr (13,508 days)
Aphelion2.9663 AU
Perihelion2.7030 AU
Semi-major axis2.8347 AU
Eccentricity0.0464
Orbital period (sidereal)4.77 yr (1,743 days)
Mean anomaly62.052°
Mean motion0° 12 23.4 / day
Inclination3.2909°
Longitude of ascending node97.461°
Argument of perihelion211.58°
TJupiter3.3080
Physical characteristics
Dimensions8.791±0.081 km
8.98 km (calculated)
Synodic rotation period3.2526±0.0042 h (R)
3.2529±0.0042 h (S)
Geometric albedo0.24 (assumed)
0.301±0.037
Spectral typeS
Absolute magnitude (H)12.2 · 12.367±0.002 (R) · 12.4 · 12.45±0.07 · 12.966±0.003 (S)

6980 Kyusakamoto, provisional designation 1993 SV1, is a stony Koronis asteroid from the outer region of the asteroid belt, approximately 9 kilometers in diameter. It was discovered by Japanese astronomers Kin Endate and Kazuro Watanabe at Kitami Observatory on 16 September 1993. The asteroid was named after Japanese singer Kyu Sakamoto.

Orbit and classification

Kyusakamoto is a member of the Koronis family, which is named after 158 Koronis and consists of about 300 known bodies with nearly ecliptical orbits. It orbits the Sun in the outer main-belt at a distance of 2.7–3.0 AU once every 4 years and 9 months (1,743 days). Its orbit has an eccentricity of 0.05 and an inclination of 3° with respect to the ecliptic.

In November 1979, it was first identified as 1979 WH7 at Crimea–Nauchnij, extending the body's observation arc by 14 years prior to its official discovery observation at Kitami.

Physical characteristics

Rotation period

In August 2012, a rotational lightcurve of Kyusakamoto was obtained through photometric observations at the Palomar Transient Factory, California. The lightcurve showed a period of 3.2529±0.0042 hours with a brightness amplitude of 0.40 in magnitude (U=2). In the Mould-R filter (R), a different photometric band, the observations rendered a nearly identical period of 3.2526±0.0042 hours with an amplitude of 0.41 (U=2).

Diameter and albedo

According to the survey carried out by the NEOWISE mission of NASA's space-based Wide-field Infrared Survey Explorer, Kyusakamoto measures 8.8 kilometers in diameter and its surface has a high albedo of 0.30, while the Collaborative Asteroid Lightcurve Link assumes a stony albedo of 0.24 and calculates a slightly larger diameter of 9.0 kilometers.

Naming

This minor planet was named in memory of Japanese popular singer Kyu Sakamoto (1941–1985), who died in the crash of Japan Air Lines Flight 123, the deadliest single-aircraft accident in history. Adored as "Kyu-chan", he is best known for his hit, I Look Up As I Walk ("Sukiyaki"), which became a worldwide bestseller. The naming also refers to his collaborators Rokusuke Ei and Hachidai Nakamura, songwriter and pianist, respectively. The official naming citation was published by the Minor Planet Center on 5 October 1998 (M.P.C. 32789).

References

  1. ^ "JPL Small-Body Database Browser: 6980 Kyusakamoto (1993 SV1)" (2016-11-10 last obs.). Jet Propulsion Laboratory. Retrieved 21 June 2017.
  2. ^ Schmadel, Lutz D. (2007). "(6980) Kyusakamoto". Dictionary of Minor Planet Names – (6980) Kyusakamoto. Springer Berlin Heidelberg. p. 569. doi:10.1007/978-3-540-29925-7_6220. ISBN 978-3-540-00238-3.
  3. ^ "LCDB Data for (6980) Kyusakamoto". Asteroid Lightcurve Database (LCDB). Retrieved 19 May 2016.
  4. ^ 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. Retrieved 19 May 2016.
  5. ^ 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. Retrieved 5 December 2016.
  6. ^ Waszczak, Adam; Chang, Chan-Kao; Ofek, Eran O.; Laher, Russ; Masci, Frank; Levitan, David; et al. (September 2015). "Asteroid Light Curves from the Palomar Transient Factory Survey: Rotation Periods and Phase Functions from Sparse Photometry". The Astronomical Journal. 150 (3): 35. arXiv:1504.04041. Bibcode:2015AJ....150...75W. doi:10.1088/0004-6256/150/3/75. Retrieved 19 May 2016.
  7. 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. Retrieved 19 May 2016.
  8. ^ "6980 Kyusakamoto (1993 SV1)". Minor Planet Center. Retrieved 16 April 2016.
  9. "MPC/MPO/MPS Archive". Minor Planet Center. Retrieved 19 May 2016.

External links

Minor planets navigator
Small Solar System bodies
Minor planets
Asteroid
Distant minor planet
Comets
Other
Categories: