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5855 Yukitsuna

Main-belt asteroid


Main-belt asteroid

FieldValue
minorplanetyes
name5855 Yukitsuna
background#D6D6D6
discovery_ref
discovererA. Natori
T. Urata
discovery_siteJCPM Yakiimo Stn.
discovered26 October 1992
mpc_name(5855) Yukitsuna
alt_names1943 UF
named_after
(Japanese general)
mp_categorymain-belt(middle)
MariaEunomia
orbit_ref
epoch23 March 2018 (JD 2458200.5)
uncertainty0
observation_arc74.49 yr (27,207 d)
aphelion2.9480 AU
perihelion2.1566 AU
semimajor2.5523 AU
eccentricity0.1551
period4.08 yr (1,489 d)
mean_anomaly124.59°
mean_motion/ day
inclination15.509°
asc_node20.596°
arg_peri323.91°
mean_diameter
(calculated)
rotation
albedo(assumed)
spectral_typeS (assumed)
abs_magnitude11.8
12.1

T. Urata

(Japanese general) MariaEunomia (calculated)

12.1

5855 Yukitsuna, provisional designation , is a stony Marian asteroid from the central regions of the asteroid belt, approximately 11 km in diameter. It was discovered on 26 October 1992, by Japanese astronomers Akira Natori and Takeshi Urata at the JCPM Yakiimo Station. The likely elongated S-type asteroid has a rotation period of 19 hours. It was named for , a Japanese general during the Heian era.

Orbit and classification

Yukitsuna is a core member of the Maria family (506), a large intermediate belt family of stony asteroids. Alternatively, it has also been assigned to the stony Eunomia family (502), one of the most prominent families in the intermediate main belt with more than 5,000 members.

It orbits the Sun in the central main-belt at a distance of 2.2–2.9 AU once every 4 years and 1 month (1,489 days; semi-major axis of 2.55 AU). Its orbit has an eccentricity of 0.16 and an inclination of 16° with respect to the ecliptic.

The asteroid was first observed as at Heidelberg Observatory in October 1943. The body's observation arc begins as at Crimea–Nauchnij in March 1974, more than 17 years prior to its official discovery observation at Yakiimo.

Physical characteristics

Yukitsuna is an assumed S-type asteroid, as is the overall spectral type of both the Maria and Eunomia family.

Rotation period

In January 2006, a rotational lightcurve of Yukitsuna was obtained from photometric observations by Federico Manzini at the Sozzago Astronomical Station in Italy. Lightcurve analysis gave a rotation period of 19.2 hours with a brightness variation of 0.8 magnitude (). In September 2008, a more refined period of 19.04 hours and an amplitude of 0.80 magnitude was measured at the Oakley Southern Sky Observatory and Oakley Observatory (). The high brightness variation of 0.8 magnitude is indicative for an elongated, non-spherical shape.

Diameter and albedo

According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Yukitsuna measures between 10.585 and 11.100 kilometers in diameter and its surface has an albedo between 0.273 and 0.3002.

The Collaborative Asteroid Lightcurve Link assumes an albedo of 0.21 – derived from 15 Eunomia, the parent body of the Eunomia family – and calculates a diameter of 11.03 kilometers based on an absolute magnitude of 12.1.

Naming

This minor planet was named after , a general of the late Heian period of Japanese history. The official naming citation was published by the Minor Planet Center on 14 December 1997 (M.P.C. 31024).

References

Info: Wikipedia Source

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