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Asteroid impacts happen when a rocky object from space crosses Earth’s orbit and enters the atmosphere at very high speed. Most incoming objects are small and burn up as meteors, but larger ones can survive the trip and strike the surface. Understanding impacts matters because they shape planetary surfaces, affect ecosystems, and represent a real natural hazard.

Scientists study asteroid paths so they can estimate impact risk and plan possible defenses.

Key Facts

  • Impact speed near Earth is often about 11 km/s to 72 km/s.
  • Kinetic energy is KE = 1/2 mv^2, so speed has a huge effect on impact energy.
  • Earth’s escape speed at the surface is about 11.2 km/s, which sets a minimum natural impact speed for falling objects from space.
  • Atmospheric drag force increases with speed and cross-sectional area, approximately Fd = 1/2 ρv^2CdA.
  • A meteoroid becomes a meteor when it glows in the atmosphere, and any surviving piece that reaches the ground is a meteorite.
  • Impact frequency decreases as asteroid size increases, so small impacts are common while giant impacts are rare.

Vocabulary

Asteroid
A rocky or metallic object that orbits the Sun, usually smaller than a planet and often found in the asteroid belt.
Meteoroid
A small rocky or metallic object traveling through space before it enters a planet’s atmosphere.
Meteor
The bright streak of light produced when a meteoroid heats up and glows as it passes through the atmosphere.
Meteorite
A fragment of a meteoroid or asteroid that survives atmospheric entry and lands on a planet’s surface.
Impact crater
A bowl-shaped depression formed when a high-speed object strikes a solid planetary surface.

Common Mistakes to Avoid

  • Calling every space rock a meteorite is wrong because it is only a meteorite after it reaches the ground.
  • Assuming friction alone makes the glow is incomplete because compression of air in front of the object also heats the gas and surface strongly.
  • Ignoring velocity in impact energy gives poor estimates because KE = 1/2 mv^2 means doubling speed makes four times the kinetic energy.
  • Thinking large asteroids fall straight down is wrong because they enter with orbital motion, so their paths are usually curved and angled relative to the surface.

Practice Questions

  1. 1 A meteoroid has a mass of 200 kg and enters the atmosphere at 20,000 m/s. Calculate its kinetic energy using KE = 1/2 mv^2.
  2. 2 An asteroid travels 60,000 km in 1 hour as it approaches Earth. What is its average speed in km/s?
  3. 3 Explain why a small asteroid may explode in the atmosphere while a larger or denser asteroid can reach the ground and form a crater.