![]() | There goes the neighborhood! This is an artist's illustration of a supposed asteroid impact on Earth about 250 million years ago. This impact, off the northwestern coast of Australia, left a 125 mile diameter crater and caused massive extinctions. (NASA image, Continental Dynamics Workshop/NSF). |
| Impulsive Technique | Description |
| Conventional Explosive (surface) | Detonate on impact |
| Conventional Explosive (subsurface) | Drive explosive device into PHO, and then detonate |
| Nuclear Explosive (standoff) | Detonate on flyby using a proximity fuse |
| Nuclear Explosive (surface) | Impact, detonate using a contact fuse |
| Nuclear Explosive (delayed) | Land on surface, detonate at an optimum time |
| Nuclear Explosive (subsurface) | Drive explosive device into PHO, and then detonate |
| Kinetic Impact | High velocity impact |
| Slow Push Technique | Description |
| Focused Solar | Use a large mirror to focus solar energy on a spot to vaporize material |
| Pulsed Laser | Rendezvous, position spacecraft near PHO and focus a laser on surface to vaporize material |
| Mass Driver | Rendezvous, land, attach, mine material and eject material from the PHO at high velocity |
| Gravity Tractor | Rendezvous with PHO and fly in close proximity for extended period, Gravitational attraction provides a small force |
| Asteroid Tug | Rendezvous with the PHO, attach to the PHO and push |
| Yarkovsky Effect | Change the albedo of a rotating PHO. Radiation from sun-heated material will provide a small force as the body rotates |