1840 Hus

1840 Hus (prov. designation: Template:Mp) is a stony Koronis asteroid from the outer regions of the asteroid belt, approximately in diameter. It was discovered on 26 October 1971, by Czech astronomer Luboš Kohoutek at the Bergedorf Observatory in Hamburg, Germany. The S-type asteroid has a rotation period of 4.8 hours and is likely elongated in shape. It was later named after 15th-century theologian Jan Hus.

Orbit and classification

Hus is a core member of the Koronis family (605), a very large asteroid family of almost 6,000 known asteroids with nearly co-planar ecliptical orbits. It orbits the Sun in the outer main-belt at a distance of 2.9–3.0 AU once every 5 years (1,821 days; semi-major axis of 2.92 AU). Its orbit has an eccentricity of 0.02 and an inclination of 2° with respect to the ecliptic. Hus was first observed as Template:Mp at the Lowell Observatory in October 1931. The body's observation arc begins with its observation as Template:Mp at the Goethe Link Observatory in January 1953, more than 18 years prior to its official discovery observation at Hamburg.

Naming

This minor planet was named after Czech Jan Hus (1372–1415), a fifteenth century Bohemian theologian, rector of Charles University in Prague and forerunner of the protestant reformation. He was condemned to death by the Council of Constance and burned at the stake for his reformation ideas. Jan Hus is also known as John Huss in the English speaking world. The official Template:MoMP was published by the Minor Planet Center on 20 December 1974 (M.P.C. 3757).

Physical characteristics

Based on the asteroid's membership to the Koronis family and its relatively high geometric albedo determined by the Wide-field Infrared Survey Explorer (WISE), Hus is very likely a stony S-type asteroid.

Rotation period and pole

In June 2006, a rotational lightcurve of Hus was obtained from photometric observations taken by Maurice Clark at the Chiro Observatory Template:Obscode in Western Australia. Lightcurve analysis gave a rotation period of hours with a high brightness variation of 0.85 magnitude (U=2-), strongly indicative of an elongated, non-spherical shape. In March 2016, a synthetic lightcurve gave a similar period of hours, using sparse-in-time photometry data from the Lowell Photometric Database (U=n.a.). More recent lightcurve analysis during observations of the 1840 Hus apparition in 2020, from the MIT Koronis Family Asteroids Rotation Lightcurve Observing Program, gave a secure rotation period of hours.

Diameter and albedo

According to the survey carried out by NASA's WISE telescope with its subsequent NEOWISE mission, Hus measures 12.4 and 12.6 kilometers in diameter, and its surface has an albedo of 0.261 and 0.255, respectively. Conversely, the Collaborative Asteroid Lightcurve Link assumes a standard albedo for carbonaceous asteroids of 0.057, rather than one for a stony body, as indicated by WISE/NEOWISE – and calculates therefore a twice as large diameter of 25.4 kilometers, as the lower the albedo, the larger the body's diameter for a constant absolute magnitude.

External links

• A Simple Guide to NEOWISE Data Problems, Nathan Myhrvold, 25 May 2016
• 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:PAGENAMEBASE at the JPL Small-Body DatabaseTemplate:EditAtWikidata