Everyone has seen the full Moon in the
night sky. The familiar dark splotches called ‘maria,’ Latin for seas, create
patterns on the lunar surface. Some people see a man’s face, the Man in the
Moon. Others imagine a frog or a rabbit. Whatever you might picture when you
look at the full Moon, the pattern of large, dark areas overlying lighter
material is quite obvious. The maria are composed of lava that poured out from
asteroid impacts and covered the lighter surface material.
The Lunar Nearside, credit NASA
From Earth, we only see the one side of the Moon, so you
might assume this arrangement of maria over lighter material continues on the
far side of the Moon. Astronomers assumed that, too, until the Russian Luna 3
spacecraft sent back the first, grainy pictures of the lunar far side in 1959.
Although there were a few dark patches, they were quite a bit smaller than the
familiar maria of the near side and didn’t cover much of the far side surface.
The Lunar Farside, credit NASA
Subsequent studies of the Moon revealed that the crust on
the far side is as much as 10 miles (ca. 16 km) thicker than the near side crust. Because
of this, asteroids can’t so easily puncture the far side crust, so fewer and
smaller maria formed there. For decades, astronomers puzzled as to what might
have caused this. Until recently, the best idea was that we originally had two
moons. Very early on, the two collided at low speed on the far side. The
material from the smaller impacting moon flowed over that side, creating the
thicker crust.
Measurements
made by the Gravity Recovery and Interior Laboratory (GRAIL) mission in 2012
provided more data, suggesting an impact from an outsider. "The
detailed gravity data obtained by GRAIL has given new insight into the
structure of the lunar crust underneath the surface," said Meng Hua Zhu, a
co-author on the new paper on the subject and a scientist at Macau University
of Science and Technology in China. Using computers, the researchers modeled
360 different collisions and compared all the results to what we know about the
moon today. The best fit with our Moon suggests that a collision of an object 500-560 miles (ca. 805-901 km) across could have done the trick.
Artists concept of Lunar Farside collision, credit NASA
Luckily for us, there are no other such
large objects wandering around near our orbit today.
On or about the first Tuesday of each month, I write an
astronomy-related column piece for the Oklahoman newspaper. On the following
day, I post that same column to my blog page.
This is reprinted by permission from the Oklahoman and www.newsok.com.