Collisional and dynamic evolution of dust from the asteroid belt

Details Collisional and dynamic evolution of dust from the asteroid belt Collisional and dynamic evolution of dust from the asteroid belt

Dec 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992acm..proc..223g&link_type=abstract

In Lunar and Planetary Inst., Asteroids, Comets, Meteors 1991 p 223-226 (SEE N93-19113 06-90)

Physics

3

Asteroid Belts, Asteroids, Interplanetary Dust, Particle Size Distribution, Poynting-Robertson Effect, Spatial Distribution, Drag, Meteoroids, Solar System, Space Debris

Scientific paper

The size and spatial distribution of collisional debris from main belt
asteroids is modeled over a 10 million year period. The model dust and
meteoroid particles spiral toward the Sun under the action of
Poynting-Robertson drag and grind down as they collide with a static
background of field particles.

Affiliated with

Also associated with

No associations

Rating

Collisional and dynamic evolution of dust from the asteroid belt does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Collisional and dynamic evolution of dust from the asteroid belt, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Collisional and dynamic evolution of dust from the asteroid belt will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1112584