1225 Ariane, provisional designation , is a stony Florian
asteroid
An asteroid is a minor planet of the Solar System#Inner solar system, 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 o ...
from the inner regions of the
asteroid belt
The asteroid belt is a torus-shaped region in the Solar System, located roughly between the orbits of the planets Jupiter and Mars. It contains a great many solid, irregularly shaped bodies, of many sizes, but much smaller than planets, called ...
, approximately 9 kilometers in diameter. It was discovered on 23 April 1930, by Dutch astronomer
Hendrik van Gent at the
Leiden Southern Station, annex to the
Johannesburg Observatory in South Africa.
Orbit and characterization
''Ariane'' orbits the Sun at a distance of 2.1–2.4
AU once every 3 years and 4 months (1,219 days). Its orbit has an
eccentricity of 0.07 and an
inclination
Orbital inclination measures the tilt of an object's orbit around a celestial body. It is expressed as the angle between a Plane of reference, reference plane and the orbital plane or Axis of rotation, axis of direction of the orbiting object ...
of 3
° with respect to the
ecliptic
The ecliptic or ecliptic plane is the orbital plane of the Earth around the Sun. From the perspective of an observer on Earth, the Sun's movement around the celestial sphere over the course of a year traces out a path along the ecliptic agai ...
.
observations made in 2003 at the U.S. Carbuncle Hill Observatory (
912
Year 912 ( CMXII) was a leap year starting on Wednesday (link will display the full calendar) of the Julian calendar.
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Events By place Byzantine Empire
* May 11 – Emperor Leo VI (the Wise) dies after a 26-year reign in wh ...
) near Providence, Rhode Island, give a synodic
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 ...
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