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LCROSS / Clues in the shadows

What was hiding in that crater?

A planned impact lifted material into view. Explore the plume, then see why scientists study more than just a photograph.

NASA LCROSS (2009-031B)NORAD: 35316

7.2 GJ Kinetic Impact & Water Ice Discovery

Cabeus Crater Permanently Shadowed Region · Discovered 155 kg of water ice and volatile cocktail

Impact Site

Cabeus Crater (PSR)

40 K (-233°C)

Centaur Impact Energy

7.20 GigaJoules

~1.72 tons TNT equivalent

Water Vapor Detected

155 kg H₂O

5.6% of excavated regolith

Plume Altitude

10 km High

Lit by solar rays above rim

LROC Frame

M119827295RE

NAC Cabeus PSR observation

Centaur Upper Stage Kinetic Energy Calculator

On October 9, 2009, NASA steered the spent 2,305 kg Centaur rocket body directly into Cabeus crater at 2.5 km/s (9,000 km/h). The kinetic explosion excavated a 20-meter crater and threw 350 tons of regolith into the sunlight.

Impact Velocity:2,500 m/s (9,000 km/h)7.20 GigaJoules
1,000 m/s (1.15 GJ)2,500 m/s (Actual LCROSS Velocity: 7.20 GJ)3,500 m/s (14.1 GJ)
T = 00:00 (11:31:19 UTC)

Centaur Kinetic Collision

The 2,305 kg rocket slams into Cabeus crater floor at 9,000 km/h. Ejecta plume launches 10 km into sunlight above the crater rim.

T + 04:00 (Plume Transit)

Shepherding Craft Dives In

Trailing 4 minutes behind, the probe flies through the sunlit debris cloud, its 9 sensors capturing absorption dips of water ice.

T + 04:17 (11:35:36 UTC)

Final Science Impact

After streaming high-speed video and spectra until 2 seconds before collision, the shepherding spacecraft impacts Cabeus, leaving its own monument.

Look deeper: mission background

Authentic NASA Mission Context: LCROSS in Cabeus Crater

On October 9, 2009, NASA sent the LCROSS Centaur upper stage hurtling into the permanently shadowed floor of Cabeus crater near the lunar south pole. The collision excavated a 20-meter crater and launched 350 tons of regolith into the sunlight. Trailing four minutes behind, the shepherding spacecraft flew through the plume, using near-infrared spectrometers to detect the distinctive absorption signatures of water ice at 1.4 µm and 1.9 µm. The mission proved that polar craters on the Moon harbor volatile reservoirs essential for future lunar exploration.