Minorplanet: | yes |
1242 Zambesia | |
Background: |
|
Discovered: | 28 April 1932 |
Mpc Name: | (1242) Zambesia |
Alt Names: | 1932 HL1947 TE 1948 AC1967 EF A908 BF |
Named After: | Zambezi basin |
Epoch: | 4 September 2017 (JD 2458000.5) |
Uncertainty: | 0 |
Observation Arc: | 109.42 yr (39,966 days) |
Perihelion: | 2.2201 AU |
Semimajor: | 2.7385 AU |
Eccentricity: | 0.1893 |
Period: | 4.53 yr (1,655 days) |
Mean Motion: | / day |
Inclination: | 10.163° |
Asc Node: | 350.01° |
Arg Peri: | 52.968° |
Dimensions: | km 47.54 km km km km km km km |
Rotation: | h h > h |
Albedo: | 0.0541 |
Abs Magnitude: | 10.1010.4010.4110.87 |
1242 Zambesia (prov. designation:) is a dark background asteroid from the central regions of the asteroid belt, approximately 48km (30miles) in diameter. It was discovered on 28 April 1932, by South African astronomer Cyril Jackson at the Union Observatory in Johannesburg. The asteroid was named for the large Zambezi basin in southern Africa.
Zambesia is a non-family asteroid from the main belt's background population. It orbits the Sun in the central main-belt at a distance of 2.2–3.3 AU once every 4 years and 6 months (1,655 days; semi-major axis of 2.74 AU). Its orbit has an eccentricity of 0.19 and an inclination of 10° with respect to the ecliptic.
The asteroid was first observed as at Taunton Observatory in January 1908. The body's observation arc begins at the United States Naval Observatory in February 1908, more than 26 years prior to its official discovery observation at Johannesburg.
This minor planet was named after the Zambezi river valley, partially part of the former British Central Africa Protectorate. The official naming citation was mentioned in The Names of the Minor Planets by Paul Herget in 1955 . The large Zambezi basin stretches across modern Angola, Botswana, Mozambique, Namibia, Zambia and Zimbabwe.
In both the Tholen- and SMASS-like taxonomy of the Small Solar System Objects Spectroscopic Survey (S3OS2),, Zambesia is a common, carbonaceous C-type asteroid.
In October 2015, a rotational lightcurve of Zambesia was obtained by a group of Spanish astronomers. Lightcurve analysis gave a rotation period of 15.72 hours with a brightness variation of 0.15 magnitude . Previous photometric observations gave a divergent period of 17.305 and 24+ hours .
According to the surveys carried out by the Infrared Astronomical Satellite IRAS, the Japanese Akari satellite and the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Zambesia measures between 42.16 and 72.818 kilometers in diameter and its surface has an albedo between 0.0252 and 0.0708.
The Collaborative Asteroid Lightcurve Link derives an albedo of 0.0541 and a diameter of 47.54 kilometers based on an absolute magnitude of 10.4.