On the formation of larger bodies in space after dust attraction.

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SUMMARY

The discussion centers on the dynamics of asteroid collisions and their role in the formation of larger celestial bodies. When a 50-meter asteroid 'A' collides with a 500-meter asteroid 'B' at a small angle, the collision generates two vectors: one parallel and one perpendicular to asteroid 'B'. The energy from the perpendicular vector is absorbed, leaving only the parallel vector, which contributes to the clustering of debris in the solar system. This clustering can lead to coalescence, although factors like tidal disruption from nearby massive bodies, such as Jupiter, can prevent the formation of planets from these clusters, as seen in the asteroid belt.

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  • Understanding of basic physics principles related to vector dynamics
  • Knowledge of celestial mechanics and orbital dynamics
  • Familiarity with asteroid composition and collision outcomes
  • Awareness of the gravitational influences of large bodies like Jupiter
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  • Research the physics of asteroid collisions and energy transfer
  • Study the formation and dynamics of the asteroid belt between Mars and Jupiter
  • Explore the effects of tidal forces on celestial bodies
  • Investigate the processes of coalescence in space debris aggregation
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Astronomers, astrophysicists, and space scientists interested in the formation of celestial bodies and the dynamics of asteroid collisions.

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When a (say 50 meters) asteroid 'A' strikes a larger (say 500 meters) ‘equally hard’ asteroid 'B' at a small angle to the asteroid 'B' would have two vectors, one large vector parallel to the asteroid 'B', another second small vector perpendicular to the asteroid 'B'.
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If the small amount of energy of the perpendicular vector is diminished or absorbed by the asteroid (other than asteroid 'A' being absorbed or bouncing off at an opposed angle), all that remains would be the vector parallel to the asteroid 'B' path.
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Thus, since the great majority of debris in the solar system has the same orbital direction, this would result in clusters of particles (asteroids) moving in orbit together.
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Sooner or later the result would be the cluster slowly coalescing. Any original velocities of the two objects ('A' & 'B') would retained but a conjunctive focus for a third order interception point would be created. Ω
 
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An example I can think of is the asteroid belt between Mars and Jupiter. Those bodies will never coallesce to form a planet to due tidal disruption from Jupiter.
 

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