3290 Azabu

3290 Azabu, provisional designation Template:Mp, is a dynamical Hildian asteroid from the outermost regions of the asteroid belt, approximately in diameter. It was discovered on 19 September 1973, by Dutch astronomers Ingrid and Cornelis van Houten at Leiden, and Tom Gehrels the Palomar Observatory. The asteroid has a rotation period of 7.67 hours. It was named after the former city district of Tokyo, Azabu.

Orbit and classification

Azabu is a member of the dynamical Hilda group, located beyond the actual core region of the asteroid belt, and locked in a 3:2 orbital resonance with the gas giant Jupiter. This means that for every 2 orbits Jupiter completes around the Sun, a Hildian asteroid will complete 3 orbits. While it belongs to the dynamical Hilda group, Azabu, is not a member of the Hilda family (001), but an asteroid of the background population.

This asteroid orbits the Sun in the outer main-belt at a distance of 3.5–4.5 AU once every 7 years and 11 months (2,891 days; semi-major axis of 3.97 AU). Its orbit has an eccentricity of 0.13 and an inclination of 3° with respect to the ecliptic. The body's observation arc begins with a precovery taken at Palomar in April 1954, or 29 years prior to its official discovery observation.

Palomar–Leiden Trojan survey

Despite being discovered during the second Palomar–Leiden Trojan survey in 1973, Azabu has not received a provisional survey designation starting with "T-2". This may be related to the swapped naming rights proposed by Tom Gehrels (see below). The survey was a fruitful collaboration between the Palomar and Leiden observatories during the 1960s and 1970s. Gehrels used Palomar's Samuel Oschin telescope (also known as the 48-inch Schmidt Telescope), and shipped the photographic plates to Ingrid and Cornelis van Houten at Leiden Observatory where astrometry was carried out. The trio are credited with the discovery of several thousand asteroid discoveries.

Physical characteristics

The asteroid has been characterized as an XL-type by Pan-STARRS and in the SDSS-based taxonomy. It is also characterized as a carbonaceous C-type asteroid in the SDSS-MFB (Masi Foglia Binzel) taxonomy.Template:Efn

Rotation period

In April 2017, a rotational lightcurve of Azabu was obtained from photometric observations by Brian Warner and Robert Stephens at the Center for Solar System Studies in California. Lightcurve analysis gave a secure rotation period of 7.670 hours with a brightness amplitude of 0.23 magnitude (U=3-),Template:Efn superseding a measurement of approximately 12 hours from the 1990s (U=1).

Diameter and albedo

According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Azabu measures 10.2 kilometers in diameter and its surface has an albedo between 0.32. The Collaborative Asteroid Lightcurve Link assumes a much lower carbonaceous standard albedo of 0.057 (based on the Masi Foglia Binzel taxonomy) and consequently calculates a much larger diameter of 21.16 kilometers with an absolute magnitude of 12.1.

Naming

This minor planet was named after Azabu, a former district of the city of Tokyo, where the Tokyo Astronomical Observatory was previously located. The official naming citation was published by the Minor Planet Center on 16 December 1986 (M.P.C. 11442).

Based on a proposal by the discoverer Tom Gehrels, the naming right for this asteroid were swapped with 3291 Dunlap (discovered by Japanese astronomers), in order to create a quartet of sequentially named asteroids named after Template:MoMP (numbers 3291–3294).

External links

• Asteroid Lightcurve Database (LCDB), query form (info Template:Webarchive)
• Dictionary of Minor Planet Names, Google books
• Asteroids and comets rotation curves, CdR – Observatoire de Genève, Raoul Behrend
• Discovery Circumstances: Numbered Minor Planets (1)-(5000) – Minor Planet Center
• Template:AstDys
• Template:PAGENAMEBASE at the JPL Small-Body DatabaseTemplate:EditAtWikidata