http://science.nasa.gov/science-news/science-at-nasa/2013/16may_lunarimpact/
 
Bright Explosion on the Moon
NASA Science News
May 17, 2013

For the past 8 years, NASA astronomers have been monitoring the Moon for signs 
of explosions caused by meteoroids hitting the lunar surface. "Lunar meteor 
showers" have turned out to be more common than anyone expected, with hundreds 
of 
detectable impacts occurring every year.

They've just seen the biggest explosion in the history of the program.

"On March 17, 2013, an object about the size of a small boulder hit the lunar 
surface in Mare Imbrium," says Bill Cooke of NASA's Meteoroid Environment 
Office. 
"It exploded in a flash nearly 10 times as bright as anything we've ever seen 
before."

Anyone looking at the Moon at the moment of impact could have seen the 
explosion--no 
telescope required.  For about one second, the impact site was glowing like a 
4th magnitude 
star.

Ron Suggs, an analyst at the Marshall Space Flight Center, was the first to 
notice the 
impact in a digital video recorded by one of the monitoring program's 14-inch 
telescopes.  
"It jumped right out at me, it was so bright," he recalls.

The 40 kg meteoroid measuring 0.3 to 0.4 meters wide hit the Moon traveling 
56,000 mph.  
The resulting explosion1 packed as much punch as 5 tons of TNT.

Cooke believes the lunar impact might have been part of a much larger event.

"On the night of March 17, NASA and University of Western Ontario all-sky 
cameras picked 
up an unusual number of deep-penetrating meteors right here on Earth," he says. 
"These 
fireballs were traveling along nearly identical orbits between Earth and the 
asteroid belt."

This means Earth and the Moon were pelted by meteoroids at about the same time.

"My working hypothesis is that the two events are related, and that this 
constitutes a 
short duration cluster of material encountered by the Earth-Moon system," says 
Cooke.

One of the goals of the lunar monitoring program is to identify new streams of 
space debris 
that pose a potential threat to the Earth-Moon system.  The March 17th event 
seems to be a 
good candidate.

Controllers of NASA's Lunar Reconnaissance Orbiter have been notified of the 
strike.  The 
crater could be as wide as 20 meters, which would make it an easy target for 
LRO the next 
time the spacecraft passes over the impact site.  Comparing the size of the 
crater to the 
brightness of the flash would give researchers a valuable "ground truth" 
measurement to 
validate lunar impact models.

Unlike Earth, which has an atmosphere to protect it, the Moon is airless and 
exposed.  
"Lunar meteors" crash into the ground with fair frequency. Since the monitoring 
program 
began in 2005, NASA's lunar impact team has detected more than 300 strikes, 
most orders of 
magnitude fainter than the March 17th event.  Statistically speaking, more than 
half of 
all lunar meteors come from known meteoroid streams such as the Perseids and 
Leonids.  The 
rest are sporadic meteors--random bits of comet and asteroid debris of unknown 
parentage.

U.S. Space Exploration Policy eventually calls for extended astronaut stays on 
the lunar 
surface. Identifying the sources of lunar meteors and measuring their impact 
rates gives 
future lunar explorers an idea of what to expect. Is it safe to go on a 
moonwalk, or not?  
The middle of March might be a good time to stay inside.

"We'll be keeping an eye out for signs of a repeat performance next year when 
the Earth-Moon 
system passes through the same region of space," says Cooke. "Meanwhile, our 
analysis of the 
March 17th event continues."

For updates stay tuned to science.nasa.gov.

Footnote: 
(1)  The Moon has no oxygen atmosphere, so how can something explode? 
Lunar meteors don't require oxygen or combustion to make themselves visible. 
 They hit the ground with so much kinetic energy that even a pebble can 
make a crater several feet wide.  The flash of light comes not from combustion 
but rather from the thermal glow of molten rock and hot vapors at the 
impact site.

Credits:

Author: Dr. Tony Phillips 
Production editor: Dr. Tony Phillips |
Credit: Science@NASA

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