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http://en.wikipedia.org/wiki/Pictor
<<Pictor is a small, faint constellation located between brilliant Canopus and the Large Magellanic Cloud.
"Pictor" literally means "painter". The name is an abbreviation of EQUULEUS Pictoris, "painter's *EASEL* ".>>
*EASEL* , n. [D. ezel ass, donkey, hence, easel, or G. esel; akin to E. ass. See Ass.]
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http://en.wikipedia.org/wiki/Beta_Pictoris
Planetesimal belts: <<The dust around Beta Pictoris may be produced by the collisions of large planetesimals. In 2003, imaging of the inner region of the Beta Pictoris system with the Keck II telescope revealed the presence of several features which are interpreted as being belts or rings of material. Belts at approximately 14, 28, 52 and 82 astronomical units from the star were detected, which alternate in inclination with respect to the main disk.>>
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Titus-Bode law:
. belt a : 21 + 60 AU = 81 AU
. belt b : 21 + 30 AU = 51 AU
. [belt c : 21 + 15 AU ?]
. belt d : 21 + 7.5 AU = 28.5 AU
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Pictors in Space:
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http://en.wikipedia.org/wiki/Beta_Pictoris
<<In 2000, observations made with the Advanced Meteor Orbit Radar facility revealed the presence of a stream of particles coming from the direction of Beta Pictoris, which appears to be the dominant source of interstellar meteoroids in our solar system. The particles in the Beta Pictoris dust stream are relatively large, with radii exceeding 20 microns, and their velocities suggest that they must have left the Beta Pictoris system at roughly 25 km/s. These particles may have been ejected from the Beta Pictoris debris disk as a result of the migration of gas giant planets within the disk and may be an indication that the Beta Pictoris system is forming an Oort cloud. Numerical modelling of dust ejection also suggests radiation pressure may also be responsible and suggests that planets further than about 1 AU from the star cannot directly cause the dust stream. On the other hand, planets in close-in orbits around Beta Pictoris better fit the planetary scenario for the stream's origin.>>
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