Planets and Moons  ID: 3533

How LRO Will Find Safe Landing Sites on the Moon (No Narration)

The first attempt to land humans on the moon - Apollo 11 - was a triumph that almost ended in disaster. At just 400 feet from the lunar surface, with only about a minute's worth of fuel remaining, astronauts Neil Armstrong and Edwin 'Buzz' Aldrin saw that their ship's computer was taking them directly into a crater the size of a football field, strewn with SUV-sized boulders. They quickly took control from the computer, flew over the crater and touched down in a smoother area beyond, cutting the engine with just 30 seconds of fuel left.

In general, good landing sites need to be level and free from large boulders that could damage or tip the spacecraft as it attempts to land. And it's up to LRO to make those landings as safe as possible.

Astronauts will want to avoid places with steep slopes that could tip the spacecraft, so LRO includes a laser ranging system that will build an elevation map to show the contours of the polar surface. The instrument, called the Lunar Orbiter Laser Altimeter (LOLA), records the time it takes for a laser pulse to travel from the spacecraft to the lunar surface and back to calculate the height of the lunar terrain. After a year in orbit aboard LRO, LOLA will have created an elevation map of the polar regions that is accurate to within a half-meter (20 inches) vertically and 50 meters (about 160 feet) horizontally.

LRO will also use data from another instrument that measures temperatures to double-check the safe zone map. Temperatures change more rapidly in areas with loose materials (lots of rocks). By analyzing how quickly temperatures change in potential landing zones, planners using the instrument, named Diviner, can rule out areas that appear smooth but actually are likely to be rocky.

LRO also carries a pair of eagle-eyed cameras, called the Narrow Angle Cameras (NACs) which together can take images that reveal details as small as a half-meter (almost 20 inches) over swaths 10 kilometers (about 6.2 miles) wide. As LRO orbits over the poles, the moon rotates beneath the spacecraft, and the NACs will gradually build up a detailed picture of the region. It will be used to identify safe landing zones free of large boulders and craters, allowing astronauts to avoid surprises like Apollo 11.

LRO is scheduled to launch in 2009.

For a 3D stereo version of this visualization, please visit animation #3567: How LRO Will Find Safe Landing Sites on the Moon - Stereoscopic version

For a feature version of this visualization with narration and music, please visit Goddard Multimedia #10349: LRO Scouts for Safe Landing Sites


For More Information

http://www.nasa.gov/mission_pages/LRO/news/safe_landing.html


Visualization Credits

Alex Kekesi (GST): Lead Animator
Wade Sisler (NASA/GSFC): Producer
Andrew Freeberg (NASA/GSFC): Producer
John Keller (NASA/GSFC): Scientist
William Steigerwald (NASA/GSFC): Writer
Please give credit for this item to:
NASA/Goddard Space Flight Center Scientific Visualization Studio Reference DEM data provided by: Jay Friedlander (QSS, Code 672)

Short URL to share this page:
http://svs.gsfc.nasa.gov/3533

Mission:
LRO (Lunar Reconnaissance Orbiter)

Data Used:
LRO/Diviner
LRO/LROC
LRO/LOLA
Note: While we identify the data sets used in these visualizations, we do not store any further details nor the data sets themselves on our site.

This item is part of this series:
LRO - Animations

Keywords:
SVS >> HDTV
SVS >> Hyperwall
SVS >> Lunar Reconnaissance Orbiter
NASA Science >> Planets and Moons
SVS >> Presentation