10979 Fristephenson
   HOME

TheInfoList



OR:

10979 Fristephenson, provisional designation , is a carbonaceous Sulamitis
asteroid An asteroid is a minor planet of the inner Solar System. Sizes and shapes of asteroids vary significantly, ranging from 1-meter rocks to a dwarf planet almost 1000 km in diameter; they are rocky, metallic or icy bodies with no atmosphere. ...
from the inner regions of the asteroid belt, approximately in diameter. It was discovered during the Palomar–Leiden Trojan survey on 29 September 1973, by Ingrid and Cornelis van Houten at Leiden, and
Tom Gehrels Anton M.J. "Tom" Gehrels (February 21, 1925 – July 11, 2011) was a Dutch–American astronomer, Professor of Planetary Sciences, and Astronomer at the University of Arizona, Tucson. Biography Youth and education Gehrels was born at Haa ...
at
Palomar Observatory Palomar Observatory is an astronomical research observatory in San Diego County, California, United States, in the Palomar Mountain Range. It is owned and operated by the California Institute of Technology (Caltech). Research time at the observat ...
in California, United States. The dark C-type asteroid was named for British historian of astronomy Francis Richard Stephenson.


Orbit and classification

''Fristephenson'' is a member of the Sulamitis family (), a small family of 300 known carbonaceous asteroids named after 752 Sulamitis. It orbits the Sun in the
inner Interior may refer to: Arts and media * ''Interior'' (Degas) (also known as ''The Rape''), painting by Edgar Degas * ''Interior'' (play), 1895 play by Belgian playwright Maurice Maeterlinck * ''The Interior'' (novel), by Lisa See * Interior de ...
main-belt at a distance of 2.3–2.7  AU once every 3 years and 10 months (1,407 days;
semi-major axis In geometry, the major axis of an ellipse is its longest diameter: a line segment that runs through the center and both foci, with ends at the two most widely separated points of the perimeter. The semi-major axis (major semiaxis) is the long ...
of 2.46 AU). Its orbit has an eccentricity of 0.08 and an inclination of 6 ° with respect to the ecliptic. The body's observation arc begins at Palomar on 19 September 1973, ten days after its official discovery observation.


Palomar–Leiden Trojan survey

The
survey designation Provisional designation in astronomy is the naming convention applied to astronomical objects immediately following their discovery. The provisional designation is usually superseded by a permanent designation once a reliable orbit has been calcu ...
"T-2" stands for the second Palomar–Leiden Trojan survey, named after the fruitful collaboration of the Palomar and Leiden Observatory during the 1960s and 1970s. Gehrels used Palomar's Samuel Oschin telescope (also known as the 48-inch Schmidt Telescope), and shipped the
photographic plate Photographic plates preceded photographic film as a capture medium in photography, and were still used in some communities up until the late 20th century. The light-sensitive emulsion of silver salts was coated on a glass plate, typically thinn ...
s to Ingrid and Cornelis van Houten at Leiden Observatory where
astrometry Astrometry is a branch of astronomy that involves precise measurements of the positions and movements of stars and other celestial bodies. It provides the kinematics and physical origin of the Solar System and this galaxy, the Milky Way. His ...
was carried out. The trio are credited with the discovery of several thousand asteroid discoveries.


Physical characteristics

''Fristephenson'' has an absolute magnitude of 15.1. Based on the Moving Object Catalog (MOC) of the
Sloan Digital Sky Survey The Sloan Digital Sky Survey or SDSS is a major multi-spectral imaging and spectroscopic redshift survey using a dedicated 2.5-m wide-angle optical telescope at Apache Point Observatory in New Mexico, United States. The project began in 2000 a ...
, the asteroid has a spectral type of a carbonaceous C-type asteroid, which agrees with its classification into the Sulamitis family, as well as with its low Geometric albedo measured by the Wide-field Infrared Survey Explorer. As of 2018, no rotational lightcurve has been obtained from photometric observations. The body's
rotation period The rotation period of a celestial object (e.g., star, gas giant, planet, moon, asteroid) may refer to its sidereal rotation period, i.e. the time that the object takes to complete a single revolution around its axis of rotation relative to the ...
, pole and shape remain unknown.


Diameter and albedo

According to the survey carried out by the NEOWISE mission of NASA's WISE telescope, ''Fristephenson'' measures 5.327 kilometers in diameter and its surface has an albedo of 0.057.


Naming

This minor planet was named after Francis Richard Stephenson (born 1941), a British
historian of astronomy Astronomy is the oldest of the natural sciences, dating back to antiquity, with its origins in the religious, mythological, cosmological, calendrical, and astrological beliefs and practices of prehistory: vestiges of these are still found in ...
at
Durham University , mottoeng = Her foundations are upon the holy hills (Psalm 87:1) , established = (university status) , type = Public , academic_staff = 1,830 (2020) , administrative_staff = 2,640 (2018/19) , chancellor = Sir Thomas Allen , vice_chan ...
. The official naming citation was published by the
Minor Planet Center The Minor Planet Center (MPC) is the official body for observing and reporting on minor planets under the auspices of the International Astronomical Union (IAU). Founded in 1947, it operates at the Smithsonian Astrophysical Observatory. Function ...
on 26 November 2004 ().


References


External links


Asteroid Lightcurve Database (LCDB)
query form

)
Dictionary of Minor Planet Names
Google books

– Minor Planet Center * * {{DEFAULTSORT:Fristephenson 010979 Discoveries by Cornelis Johannes van Houten Discoveries by Ingrid van Houten-Groeneveld Discoveries by Tom Gehrels 4171 Named minor planets 4386 19730929