COLLIDE-2 is an investigation into planetary dust rings. A follow on to COLLIDE-1, which flew on STS-90, COLLIDE-2 performed low-velocity (~1cm/sec) impact experiments into simulated dusty regoliths in microgravity. These impacts simulate the conditions in planetary rings and early protoplanetary disks. The experiment will give scientists a look at the dynamics, origin and evolution of planetary ring systems. Rings are collisionally evolved systems. Collisions sculpt the ring, leading to spreading, transfer of annular momentum, release of dust particles and damping of waves and wakes. The rate of evolution depends on dissipation of energy in collisions. COLLIDE-2 results also can be applied to the lifecycles of planetary dust rings.
The purpose of the COLLIDE-2 is to better understand the release of dust from the surfaces of small particles in planetary rings and protoplanetary disks, by spring/launching Teflon spheres into trays of powdered basaltic rock. The experiment performed six impacts of small spheres into trays of lunar regolith at velocities from 1 centimeter/second to 100 centimeters/second. The ejects from these impacts were measured with video camcorders for quantity, launch angle, and velocity distribution.
Experimental Objectives:
- Measure the impact velocities and resulting rebound velocities to high precision (within 1 percent).
- Identify the transition regime form low-velocity collisions where no mass is ejected to conditions where craters are formed and mass is ejected as a result of the impact.
- Determine the mass and velocity distribution of the ejected material as a function of impact parameters.
- Determine the dependence of coefficient of restitution (a measurement of how well the projectile "sticks" to the target material) on impact velocities for velocities ranging between 1 and 100 cm/sec.