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12621 Alsufi

Main-belt asteroid


Main-belt asteroid

FieldValue
minorplanetyes
name12621 Alsufi
background#D6D6D6
discovery_ref
discovered24 September 1960
discovererC. J. van Houten
I. van Houten-G.
Tom Gehrels
discovery_sitePalomar Obs.
mpc_name(12621) Alsufi
alt_names6585 P-L
named_afterAbd al-Rahman al-Sufi
(astronomer)
mp_categorymain-beltThemis
orbit_ref
epoch4 September 2017 (JD 2458000.5)
uncertainty0
observation_arc56.33 yr (20,576 days)
aphelion3.5148 AU
perihelion2.6980 AU
semimajor3.1064 AU
eccentricity0.1315
period5.48 yr (2,000 days)
mean_anomaly142.13°
mean_motion/ day
inclination2.4308°
asc_node148.06°
arg_peri204.34°
dimensions6.76 km (calculated)
rotationh
albedo0.08 (assumed)
spectral_typeLC
abs_magnitude13.9 (R)14.21

I. van Houten-G. Tom Gehrels (astronomer)

12621 Alsufi, provisionally designated , is a carbonaceous Themistian asteroid from the outer region of the asteroid belt, approximately 7 kilometers in diameter. It was discovered by astronomers during the Palomar–Leiden survey in 1960, and named for medieval Persian astronomer Abd al-Rahman al-Sufi.

Discovery

Alsufi was discovered on 24 September 1960, by Dutch astronomer couple Ingrid and Cornelis van Houten at Leiden, on photographic plates taken by Dutch–American astronomer Tom Gehrels at the U.S. Palomar Observatory, California. No precoveries were taken prior to its discovery observation.

Palomar–Leiden survey

The survey designation "P-L" stands for Palomar–Leiden, named after Palomar Observatory and Leiden Observatory, which collaborated on the fruitful Palomar–Leiden survey in the 1960s. 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 minor planets.

Classification and orbit

It is a member of the Themis family, a dynamical group of outer-belt asteroids with nearly coplanar ecliptical orbits. The C-type asteroid is also classified as a rather rare L-type asteroid by Pan-STARRS large-scale survey. It orbits the Sun in the outer main-belt at a distance of 2.7–3.5 AU once every 5 years and 6 months (2,000 days). Its orbit has an eccentricity of 0.13 and an inclination of 2° with respect to the ecliptic.

Physical characteristics

A rotational lightcurve of this asteroid was obtained from photometric observations made at the U.S. Palomar Transient Factory, California, in January 2012. It gave a rotation period of hours with a brightness amplitude of in magnitude (). The Collaborative Asteroid Lightcurve Link assumes an albedo of 0.08 and calculates a diameter of 6.8 kilometers with an absolute magnitude of 14.21.

Naming

This minor planet is named in honor of 10th-century Persian astronomer Abd al-Rahman al-Sufi (A.D. 903–986), also known by his western name, Azophi. Working in Isfahan, he produced his influential star atlas around A.D. 963. The atlas is based on both, Ptolemy's Almagest and on pre-Islamic star lore, and contains the earliest description of the Andromeda Galaxy. The approved naming citation was published by the Minor Planet Center on 22 January 2008 (M.P.C. 61764). The lunar crater Azophi is also named in his honour.

References

Info: Wikipedia Source

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