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1248 Jugurtha

Main-belt asteroid


Main-belt asteroid

FieldValue
minorplanetyes
name1248 Jugurtha
background#D6D6D6
image001248-asteroid shape model (1248) Jugurtha.png
captionShape model of Jugurtha from its lightcurve
discovery_ref
discovererC. Jackson
discovery_siteJohannesburg Obs.
discovered1 September 1932
mpc_name(1248) Jugurtha
alt_names1932 RO1930 DU
A901 VEA915 XB
pronounced
named_afterJugurtha
(King of Numidia)
mp_category{{plainlist
* main-belt<ref name"MPC-object" /(middle)
* background<ref name"AstDys-object" /}}
orbit_ref
epoch27 April 2019 (JD 2458600.5)
uncertainty0
observation_arc116.94 yr (42,713 d)
aphelion2.7671 AU
perihelion2.6769 AU
semimajor2.7220 AU
eccentricity0.0166
period4.49 yr (1,640 d)
mean_anomaly32.971°
mean_motion/ day
inclination9.1387°
asc_node79.381°
arg_peri345.85°
mean_diameter
rotation
albedo
spectral_typeSMASS S
abs_magnitude9.70
9.80
9.9

A901 VEA915 XB (King of Numidia)

  • main-belt(middle)
  • background}}

9.80 9.9

1248 Jugurtha (prov. designation: ) is a stony background asteroid from the central regions of the asteroid belt, approximately 29 km 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.

Discovery

Jugurtha was discovered on 1 September 1932, by South African astronomer Cyril Jackson at the Union Observatory in Johannesburg. On 29 September 1932, it was independently determined by Soviet astronomer Grigory Neujmin at the Simeiz Observatory on the Crimean peninsula. The Minor Planet Center only recognizes the first discoverer.

Orbit and classification

Jugurtha is a non-family asteroid from the main belt's background population. 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. The body's observation arc begins with its first observation as at Heidelberg Observatory in November 1901, nearly 31 years prior to its official discovery, .

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 was mentioned in The Names of the Minor Planets by Paul Herget in 1955 (H 115).

Physical characteristics

In the SMASS classification, Jugurtha is a common, stony S-type asteroid.

Rotation period

Several rotational lightcurves of Jugurtha have been obtained from photometric observations since 2001. Analysis of the best-rated lightcurve gave a rotation period of hours with a brightness amplitude between 0.70 and 1.40 magnitude (), indicative of an elongated, non-spherical shape. 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).

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. 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.

Notes

References

References

  1. {{MW. Jugurtha
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