• Source: 702 Alauda

702 Alauda , provisional designation 1910 KQ, is a carbonaceous asteroid and binary system from the outer asteroid belt, approximately 190 kilometers in diameter. It is the parent body of the Alauda family. Discovered in 1910 by German astronomer Joseph Helffrich at Heidelberg Observatory, it was named after the lark (alauda). Its small moon, named Pichi üñëm, was discovered in 2007.




Satellite


Alauda's satellite Pichi üñëm, provisionally known as S/2007 (702) 1, was discovered on 26 July 2007 from observations using adaptive-optics imaging with the European Southern Observatory (ESO) 8-m Very Large Telescope (VLT) on Cerro Paranal, Chile. It is about 3.5 km in diameter (assuming it has the same albedo as the primary) and orbits Alauda in a nearly circular orbit at a distance of 1226.5±24 km. Pichi üñëm takes 4.91 days to complete one orbit.
It was named Pichi üñëm (Mapuche pronunciation: [ˈpɪtʃi ɨˈɲɘm], approximately ), meaning "little bird" in the Mapuche language of Chile, the country from which the moon was discovered.




Orbital characteristics


Alauda has been identified as the largest member of the Alauda family, a dynamical family of bright carbonaceous asteroids with more than a thousand known members.: 23  Other members of this family include: 581 Tauntonia, 1101 Clematis, 1838 Ursa, 3139 Shantou, 3325 TARDIS, 4368 Pillmore, 5360 Rozhdestvenskij, 5815 Shinsengumi, and many others. Alauda's moon may be a result of the collision that created the asteroid family.




Physical characteristics


The discovery and tracking of Alauda's moon enabled Alauda's mass to be determined. The discoverers of the moon, Patricio Rojo and Jean-Luc Margot, estimated Alauda's mass to be (6.057±0.36)×1018 kg and its density to be 1.57±0.5 g/cm3.




= Occultations

=
Alauda has been observed to occult stars on several occasions, providing important information on its size and shape. It produced occultations on 2001-07-12 and 2004-04-21. It may have occulted an apparent magnitude 9.5 star in the constellation of Gemini on 2009-10-17 at 08:18 UT. This event should have been visible from Uruguay, Argentina, and Chile.




References






External links


Asteroids with Satellites, Robert Johnston, johnstonsarchive.net
702 Alauda at AstDyS-2, Asteroids—Dynamic Site
Ephemeris · Observation prediction · Orbital info · Proper elements · Observational info
702 Alauda at the JPL Small-Body Database

Kata Kunci Pencarian:

• 702 Alauda
• Meanings of minor-planet names: 1–1000
• Joseph Helffrich
• List of Solar System objects by size
• Asteroid family
• List of minor planets: 1–1000
• List of exceptional asteroids
• 3325 TARDIS
• 581 Tauntonia
• Minor-planet moon