998 Bodea

998 Bodea (prov. designation: Template:Mp or Template:Mp) is a dark background asteroid from the outer regions of the asteroid belt, approximately Template:Convert in diameter. It was discovered on 6 August 1923, by astronomer Karl Reinmuth at the Heidelberg Observatory in southern Germany. The presumed C-type asteroid with an irregular shape has a rotation period of 8.6 hours. It was named after German astronomer Johann Elert Bode (1747–1826).

Orbit and classification

Bodea 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 2.5–3.8 AU once every 5 years and 6 months (2,012 days; semi-major axis of 3.12 AU). Its orbit has an eccentricity of 0.21 and an inclination of 16° with respect to the ecliptic. The body's observation arc begins at Heidelberg on 8 August 1923, just two days after its official discovery observation.

Naming

This minor planet was named after Johann Elert Bode (1747–1826), German astronomer, author of the Berliner Astronomisches Jahrbuch, known for the empirical Titius–Bode law about the sequence of planetary distances. Bode also was the director of the Berlin Observatory in 1780. The asteroid's name was proposed by Swedish astronomer Bror Asplind (see citation for Template:MoMP). The official Template:MoMP was mentioned in The Names of the Minor Planets by Paul Herget in 1955 (H 95). The lunar crater Bode is also named in his honor.

Physical characteristics

Bodea is an assumed C-type asteroid. Due to its very low albedo of 0.03 or less, it could also be a P- or D-type asteroid which are very common in the outer asteroid belt and among the Jupiter trojan population.

Rotation period

File:998Bodea (Lightcurve Inversion).png

Lightcurve-based 3D-model of Bodea

In September 2006, a rotational lightcurve of Bodea was obtained from photometric observations by Italian astronomers Roberto Crippa and Federico Manzini at the Sozzago Astronomical Station Template:Obscode. Lightcurve analysis gave a well defined rotation period of Template:Val hours with a relatively high brightness amplitude of Template:Val magnitude (U=3), which is indicative of an elongated, irregular shape.Template:Efn

Poles

Modeled photometric data from the Lowell Photometric Database (LPD) and WISE thermal data, gave a concurring sidereal rotation period of 8.57412 hours. Each modeled lightcurve also determined the object's spin axes. Durech gives only one pole, namely (7.0°, −59.0°), while Hanus determined two lower rated poles at (336.0°, −70.0°) and (72.0°, −56.0°) in ecliptic coordinates (λ, β).

Diameter and albedo

According to the survey carried out by the NEOWISE mission of NASA's WISE telescope, Bodea measures Template:Val kilometers in diameter and its surface has an albedo of Template:Val. Results from the Japanese Akari satellite are in agreement with Template:Val and an albedo of Template:Val. Only the Infrared Astronomical Satellite IRAS gave a larger diameter of Template:Val and, correspondingly, a lower albedo of Template:Val. The Collaborative Asteroid Lightcurve Link adopts an albedo of 0.0304 and derives a diameter of 38.23 kilometers based on an absolute magnitude of 11.5.

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
• Template:AstDys
• Template:JPL small body