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2685 Masursky

Small Eunomian Asteroid


Small Eunomian Asteroid

FieldValue
minorplanetyes
name2685 Masursky
background#D6D6D6
imageAsteroid 2685Masurky.png
caption*Masursky* imaged by *Cassini–Huygens* in January 2000
discovery_ref
discovererE. Bowell
discovery_siteAnderson Mesa Stn.
discovered3 May 1981
mpc_name(2685) Masursky
alt_names1981 JN1950 VO
1973 QF
1977 KU
pronounced
named_afterHarold Masursky
(American planetary geologist)
mp_categorymain-belt(middle)
Eunomia
orbit_ref
epoch23 March 2018 (JD 2458200.5)
uncertainty0
observation_arc44.58 yr (16,282 d)
aphelion2.8522 AU
perihelion2.2874 AU
semimajor2.5698 AU
eccentricity0.1099
period4.12 yr (1,505 d)
mean_anomaly54.965°
mean_motion/ day
inclination12.129°
asc_node215.36°
arg_peri288.47°
mean_diameter
albedo
spectral_typeS
abs_magnitude12.1

1973 QF 1977 KU (American planetary geologist) Eunomia

2685 Masursky, provisional designation , is a stony Eunomian asteroid from the central regions of the asteroid belt, approximately 11 km in diameter. It was discovered on 3 May 1981, by American astronomer Edward Bowell at the Anderson Mesa Station near Flagstaff, Arizona, and named after American planetary geologist Harold Masursky. In January 2000, the Cassini space probe observed the S-type asteroid from afar during its coast to Saturn.

Orbit and classification

Masursky is a member of the Eunomia family (502), a prominent family of stony asteroids and the largest one in the intermediate main belt with more than 5,000 members.

It orbits the Sun in the central main-belt at a distance of 2.3–2.9 AU once every 4 years and 1 month (1,505 days; semi-major axis of 2.57 AU). Its orbit has an eccentricity of 0.11 and an inclination of 12° with respect to the ecliptic. The asteroid was first observed as at McDonald Observatory in November 1950. The body's observation arc begins with its observation as at Cerro El Roble Observatory in August 1973, nearly 8 years prior to its official discovery observation at Anderson Mesa.

Cassini–Huygens flyby

Little was known about Masursky until the Cassini–Huygens space probe, en route to Jupiter and Saturn, flew past it on 23 January 2000. Because Cassini passed the asteroid at a distance of 1.6 million kilometers (approximately 4 lunar distances), the images it returned showed nothing more than a dot.

Physical characteristics

Cassini's observations had cast some doubt on its composition, but later ground-based spectroscopy has confirmed its stony S-type spectrum, which is also the Eunomia family's overall spectral type.

Diameter and albedo

During its flyby in January 2000, Cassini–Huygens estimated a mean diameter of approximately 15–20 kilometers, based on an angular diameter of 0.81–1.08 arcseconds just hours before its closest approach. According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Masursky measures 10.744 kilometers in diameter and its surface has an albedo of 0.114.

Rotation period

As of 2018, no rotational lightcurve of Masursky has been obtained from photometric observations. The body's rotation period, spin-axis and shape remain unknown.

Naming

This minor planet was named after Harold Masursky (1922–1990), a planetary geologist at the USGS Astrogeology Science Center of the U.S. Geological Survey, in Flagstaff, Arizona. Masursky worked on numerous space missions and programs including Ranger, Surveyor, Lunar Orbiter, Apollo, Mariner 9, Viking, Pioneer Venus, Voyager, as well as on the Galileo and Magellan spacecraft. The official naming citation was published by the Minor Planet Center on 4 August 1982 (M.P.C. 7158).

References

Info: Wikipedia Source

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