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

In summary, when a smaller asteroid collides with a larger asteroid at a small angle, the resulting vectors will have a large parallel component and a smaller perpendicular component. If the perpendicular energy is absorbed, the remaining debris will mostly move in the same direction, leading to clusters of orbiting particles. Eventually, these clusters can coalesce into one larger body, while retaining the original velocities of the two objects. However, in some cases, external forces like tidal disruption can prevent this coalescence from occurring, as seen in the asteroid belt between Mars and Jupiter.
  • #1
Novawatcher
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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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  • #2
Did you have a question?
 
  • #3
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.
 

What is the process of dust attraction in space?

The process of dust attraction in space refers to the way in which small particles in space, such as dust and gas, are attracted to each other and form larger bodies.

What factors contribute to the formation of larger bodies in space?

There are several factors that contribute to the formation of larger bodies in space, including gravity, electromagnetic forces, and collisions between particles.

How do scientists study the formation of larger bodies in space?

Scientists study the formation of larger bodies in space through various methods, including observations from telescopes, computer simulations, and experiments in reduced gravity environments.

Can dust attraction lead to the formation of planets?

Yes, dust attraction can lead to the formation of planets. As the dust particles continue to attract and collide, they can form larger bodies, eventually leading to the formation of planets.

Are there any potential applications or implications of understanding dust attraction in space?

Yes, understanding dust attraction in space can have practical applications in fields such as planetary science and space exploration. It can also provide insights into the formation and evolution of our own solar system and other planetary systems in the universe.

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