6498 Ko

Last updated

6498 Ko
Discovery  [1]
Discovered by K. Endate
K. Watanabe
Discovery site Kitami Obs.
Discovery date26 October 1992
Designations
(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 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc 62.24 yr (22,734 days)
Aphelion 2.6660 AU
Perihelion 1.8955 AU
2.2807 AU
Eccentricity 0.1689
3.44 yr (1,258 days)
149.16°
0° 17m 9.96s / day
Inclination 7.9910°
149.63°
156.73°
Physical characteristics
Dimensions3.99 km (calculated) [3]
500 h [lower-alpha 1] [lower-alpha 2]
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. The asteroid was discovered on 26 October 1992, by Japanese amateur astronomers Kin Endate and Kazuro Watanabe at Kitami Observatory on eastern Hokkaidō, Japan. [5] It was named for Japanese scientist Ko Nagasawa. [2]

    Contents

    Orbit and classification

    Ko is a member of the Flora family, one of the largest groups of stony asteroids in the main-belt. It orbits the Sun in the inner main-belt 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 ecliptic. [1]

    A first precovery was taken at Palomar Observatory in 1954, extending the asteroid's observation arc by 38 years prior to its discovery. [5]

    Minor-planet close approaches

    Although Ko 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]

    Physical characteristics

    Slow rotator

    A rotational lightcurve of Ko 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] [lower-alpha 2]

    Diameter and albedo

    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 with an absolute magnitude of 14.16. [3]

    Naming

    This minor planet was named in honor of Japanese scientist Ko Nagasawa (born 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. [2]

    At the Dodaira Station, after which the minor planet 14313 Dodaira is named, Ko 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] The approved naming citation was published by the Minor Planet Center on 20 June 1997 ( M.P.C. 30099). [6]

    Notes

    1. 1 2 3 Pravec (2012): 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 for (6498) Ko at Collaborative Asteroid Lightcurve Link (CALL) and Pravec, P.; Wolf, M.; Sarounova, L. (2012)
    2. 1 2 Pravec (2012): alternative lightcurve plot with a period of 250 hours at Pravec, P.; Wolf, M.; Sarounova, L. (2012)

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    References

    1. 1 2 3 4 5 "JPL Small-Body Database Browser: 6498 Ko (1992 UJ4)" (2017-02-16 last obs.). Jet Propulsion Laboratory . Retrieved 21 June 2017.
    2. 1 2 3 4 Schmadel, Lutz D. (2007). "(6498) Ko". Dictionary of Minor Planet Names – (6498) Ko. Springer Berlin Heidelberg. p. 537. doi:10.1007/978-3-540-29925-7_5909. ISBN   978-3-540-00238-3.
    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: 1506.00762 . 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.
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