6498 Ko

6498 Ko
Discovery[1]
Discovered by K. Endate
K. Watanabe
Discovery site Kitami Obs.
Discovery date 26 October 1992
Designations
MPC designation 6498 Ko
Named after
Ko Nagasawa
(Japanese scientist)[2]
1992 UJ4 · 1964 PM
1971 QK3 · 1994 CD4
main-belt · Flora[3]
Orbital characteristics[1]
Epoch 31 July 2016 (JD 2457600.5)
Uncertainty parameter 0
Observation arc 61.56 yr (22,484 days)
Aphelion 2.6661 AU
Perihelion 1.8962 AU
2.2811 AU
Eccentricity 0.1688
3.45 yr (1,258 days)
34.669°
 17m 9.96s / day
Inclination 7.9909°
149.64°
156.78°
Physical characteristics
Dimensions 3.99 km (calculated)[3]
500 h[lower-alpha 1]
0.24 (assumed)[3]
S[3]
13.5[1]
13.71[lower-alpha 1]
13.92±0.47[4]
14.16[3]

    6498 Ko, provisional designation 1992 UJ4, is a stony Flora asteroid and exceptionally slow rotator from the inner regions of the asteroid belt, approximately 4 kilometers in diameter. It was discovered on 26 October 1992, by Japanese amateur astronomers Kin Endate and Kazuro Watanabe at Kitami Observatory on eastern Hokkaidō, Japan.[5]

    The S-type asteroid is a member of the Flora family, one of the largest groups of stony asteroids in the main-belt. It orbits the Sun at a distance of 1.9–2.7 AU once every 3 years and 5 months (1,258 days). Its orbit has an eccentricity of 0.17 and an inclination of 8° with respect to the plane of the ecliptic.[1] The first precovery was taken at Palomar Observatory in 1954, extending the asteroid's observation arc by 38 years prior to its discovery.[5]

    Although the asteroid does not cross the orbit of any planet, it does make close approaches to other large asteroids, such as 29 Amphitrite, which it approached within 0.038 AU in 1915. Further close approaches will take place in 2025 and 2135 at a distance of 0.012 and 0.009 AU, respectively. On 14 November 2009, the asteroid also made a close encounter with 3 Juno at a distance of about 0.047 AU.[1]

    A rotational light-curve for this asteroid was obtained from photometric observations by Czech astronomer Petr Pravec at the Ondřejov Observatory in June 2012. It rendered an exceptionally long rotation period of 500 hours with a brightness amplitude of 0.6 in magnitude (U=2).[lower-alpha 1] The Collaborative Asteroid Lightcurve Link assumes an albedo of 0.24, derived from the Flora family's largest member and namesake, the asteroid 8 Flora, and calculates a diameter of 4.0 kilometers based on an absolute magnitude of 14.16.[3]

    The minor planet was named in honor of Japanese scientist Ko Nagasawa (b.1932), who became a keen researcher of meteors and workes for the Public Information Office at the National Astronomical Observatory of Japan, after retiring from the Earthquake Research Institute, University of Tokyo in 1994. At the Dodaira Station, after which the minor planet 14313 Dodaira is named, he has obtained numerous photographic spectra of the 1965-Leonid meteor shower. The minor planet's name was proposed by the second discoverer, Kazuro Watanabe, following a suggestion by Japanese astronomer Kōichirō Tomita.[2] Naming citation was published on 20 June 1997 (M.P.C. 30099).[6]

    References

    1. 1 2 3 Pravec (2012) web: rotation period of 500 hours with a brightness amplitude of 0.6 magnitude. CALL assigned a quality-code Q of 2 to the measurement, which means, that the result is based on less than full coverage, and that the period may be wrong by 30 percent or so. Summary figures at Collaborative Asteroid Lightcurve Link (CALL) for (6498) Ko and Pravec, P.; Wolf, M.; Sarounova, L. (2012)
    1. 1 2 3 4 5 "JPL Small-Body Database Browser: 6498 Ko (1992 UJ4)" (2016-06-11 last obs.). Jet Propulsion Laboratory. Retrieved 4 July 2016.
    2. 1 2 Schmadel, Lutz D. (2007). Dictionary of Minor Planet Names – (6498) Ko. Springer Berlin Heidelberg. p. 537. ISBN 978-3-540-00238-3. Retrieved 4 July 2016.
    3. 1 2 3 4 5 6 "LCDB Data for (6498) Ko". Asteroid Lightcurve Database (LCDB). Retrieved 4 July 2016.
    4. 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:1506.00762Freely accessible. Bibcode:2015Icar..261...34V. doi:10.1016/j.icarus.2015.08.007. Retrieved 4 July 2016.
    5. 1 2 "6498 Ko (1992 UJ4)". Minor Planet Center. Retrieved 4 July 2016.
    6. "MPC/MPO/MPS Archive". Minor Planet Center. Retrieved 4 July 2016.

    External links

    This article is issued from Wikipedia - version of the 9/23/2016. The text is available under the Creative Commons Attribution/Share Alike but additional terms may apply for the media files.