2685 Masursky

2685 Masursky, provisional designation Template:Mp, is a stony Eunomian asteroid from the central regions of the asteroid belt, approximately Template:Convert 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.<ref name="MPC-object" /> In January 2000, the Cassini space probe observed the S-type asteroid from afar during its coast to Saturn.<ref name="Cassini-flyby" />

Orbit and classification

Masursky is a member of the Eunomia family (Template:Small),<ref name="Ferret" /> a prominent family of stony asteroids and the largest one in the intermediate main belt with more than 5,000 members.<ref name="Nesvorny-2014" />

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.<ref name="jpldata" /> The asteroid was first observed as Template:Mp at McDonald Observatory in November 1950. The body's observation arc begins with its observation as Template:Mp at Cerro El Roble Observatory in August 1973, nearly 8 years prior to its official discovery observation at Anderson Mesa.<ref name="MPC-object" />

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.<ref name="Cassini-flyby" />

Physical characteristics

Cassini's observations had cast some doubt on its composition,<ref name="Cassini-flyby" /> but later ground-based spectroscopy has confirmed its stony S-type spectrum,<ref name="Lazzaro-1999" /> which is also the Eunomia family's overall spectral type.<ref name="Nesvorny-2014" />Template:Rp

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.<ref name="Cassini-flyby" /> 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.<ref name="Masiero-2014" /><ref name="Masiero-2012" />

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.<ref name="jpldata" />

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.<ref name="MPC-object" /> The official naming citation was published by the Minor Planet Center on 4 August 1982 (Template:Small).<ref name="MPC-Circulars-Archive" />

External links

• New Cassini Images of Asteroid Available, 11 Feb 2000
• Asteroid Lightcurve Database (LCDB), query form (info Template:Webarchive)
• Dictionary of Minor Planet Names, Google books
• Discovery Circumstances: Numbered Minor Planets (1)-(5000) – Minor Planet Center
• Template:AstDys
• Template:JPL small body