Английская Википедия:1248 Jugurtha
Шаблон:Use dmy dates Шаблон:Infobox planet
1248 Jugurtha (prov. designation: Шаблон:Mp) is a stony background asteroid from the central regions of the asteroid belt, approximately Шаблон:Convert in diameter. Discovered by Cyril Jackson at the Union Observatory in 1932, the asteroid was named after Jugurtha, the ancient North African king of Numidia. The S-type asteroid is likely elongated in shape and has a rotation period of 12.9 hours.[1]
Discovery
Jugurtha was discovered on 1 September 1932, by South African astronomer Cyril Jackson at the Union Observatory in Johannesburg.[2] On 29 September 1932, it was independently by Soviet astronomer Grigory Neujmin at the Simeiz Observatory on the Crimean peninsula.[3] The Minor Planet Center only recognizes the first discoverer.[2]
Orbit and classification
Jugurtha is a non-family asteroid from the main belt's background population.[4][5] It orbits the Sun in the central asteroid belt at a distance of 2.7–2.8 AU once every 4 years and 6 months (1,640 days; semi-major axis of 2.72 AU). Its orbit has an eccentricity of 0.02 and an inclination of 9° with respect to the ecliptic.[6] The body's observation arc begins with its first observation as Шаблон:Mp at Heidelberg Observatory in November 1901, nearly 31 years prior to its official discovery, .[2]
Naming
This minor planet was named after Jugurtha (160–104 BC), a king of Numidia in North Africa, opposed to and defeated by Rome in the Jugurthine War (112–106 BC). The official Шаблон:MoMP was mentioned in The Names of the Minor Planets by Paul Herget in 1955 (Шаблон:Small).[3]
Physical characteristics
In the SMASS classification, Jugurtha is a common, stony S-type asteroid.[4][1]
Rotation period
Several rotational lightcurves of Jugurtha were obtained from photometric observations since 2001.[1][7][8]Шаблон:Efn Analysis of the best-rated lightcurve gave a rotation period of Шаблон:Val hours with a brightness amplitude between 0.70 and 1.40 magnitude (Шаблон:Small), indicative of an elongated, non-spherical shape.[9] A modeled lightcurve, using photometric data from the Lowell Photometric Database, gave a concurring period of 12.19047 hours, as well as a spin axis of (254.0°, −89.0°) in ecliptic coordinates (λ, β).[10]
Diameter and albedo
According to the surveys carried out by the Japanese Akari satellite and the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Jugurtha measures between 27.46 and 33.559 kilometers in diameter and its surface has an albedo between 0.2073 and 0.282.[11][12][13][14][15] The Collaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20 and calculates a diameter of 31.12 kilometers based on an absolute magnitude of 9.9.[1]
Notes
References
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
Шаблон:Minor planets navigator Шаблон:Small Solar System bodies
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