Английская Википедия:924 Toni

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924 Toni (prov. designation: Шаблон:Mp or Шаблон:Mp) is a large background asteroid, approximately Шаблон:Convert in diameter, from the outer regions of the asteroid belt. It was discovered on 20 October 1919, by German astronomer Karl Reinmuth at the Heidelberg-Königstuhl State Observatory. The X-type asteroid has a rotation period of 19.4 hours. It was named "Toni", a common German female name unrelated to the discoverer's contemporaries, that was taken from the almanac Lahrer Hinkender Bote.

Orbit and classification

Toni is a non-family asteroid of the main belt's background population when applying the hierarchical clustering method to its proper orbital elements. It orbits the Sun in the outer asteroid belt at a distance of 2.5–3.4 AU once every 5.04 years (1,840 days; semi-major axis of 2.94 AU). Its orbit has an eccentricity of 0.15 and an inclination of 9° with respect to the ecliptic. The asteroid was first observed as Шаблон:Mp (Шаблон:Mp) at Heidelberg Observatory on 20 January 1906, where the body's observation arc begins two days later on 20 January 1906, more than 13 years prior its official discovery observation.

Naming

This minor planet was named "Toni", after a female name picked from the Lahrer Hinkender Bote, published in Lahr, southern Germany. A Hinkender Bote (lit. "limping messenger") was a very popular almanac, especially in the alemannic-speaking region from the late 17th throughout the early 20th century. The calendar section contains feast days, the dates of important fairs and astronomical ephemerides. The German name day analogue is given next to the protestant and catholic entries in the calendar of saints (entry not found).

Reinmuth's calendar names

As with 22 other asteroids – starting with 913 Otila, and ending with 1144 Oda – Reinmuth selected names from this calendar due to his many asteroid discoveries that he had trouble thinking of proper names. These names are not related to the discoverer's contemporaries. Lutz Schmadel, the author of the Dictionary of Minor Planet Names learned about Reinmuth's source of inspiration from private communications with Dutch astronomer Ingrid van Houten-Groeneveld, who worked as a young astronomer at Heidelberg.

Physical characteristics

In the Bus–Binzel SMASS classification, Toni is an X-type asteroid, while in the Tholen classification, it is closest to a common, carbonaceous C-type asteroid and somewhat similar to an X-type (CX).

Rotation period

In July 2014, a rotational lightcurve of Toni was obtained from photometric observations by Frederick Pilcher at the Organ Mesa Observatory Шаблон:Obscode in New Mexico.Шаблон:Efn Lightcurve analysis gave a well-defined rotation period of Шаблон:Val hours with a brightness amplitude of Шаблон:Val magnitude (Шаблон:Small). This result supersedes previous observations with tentative period determinations by French amateur astronomers René Roy and Laurent Bernasconi (Шаблон:Small).

Diameter and albedo

According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer (WISE), the Japanese Akari satellite, and the Infrared Astronomical Satellite IRAS, Toni measures (Шаблон:Val), (Шаблон:Val) and (Шаблон:Val) kilometers in diameter and its surface has a low albedo of (Шаблон:Val), (Шаблон:Val) and (Шаблон:Val), respectively. The Collaborative Asteroid Lightcurve Link adopts the results obtained by IRAS, that is, an albedo of 0.0432 and a diameter of 85.49 km based on an absolute magnitude of 9.37. Further published mean-diameters and albedos by the WISE team include (Шаблон:Val) and (Шаблон:Val) and albedos of (Шаблон:Val) and (Шаблон:Val).

External links

• Lightcurve Database Query (LCDB), at www.minorplanet.info
• Dictionary of Minor Planet Names, Google books
• Asteroids and comets rotation curves, CdR – Geneva Observatory, Raoul Behrend
• Discovery Circumstances: Numbered Minor Planets (1)-(5000) – Minor Planet Center
• Шаблон:AstDys
• Шаблон:JPL small body