The Earth-Moon system is unique, and it believed that without our Moon life would not have had a chance to form. However how the Moon came to exist is a bit of a mystery. One theory is they formed together each sweeping up material as the pair orbit the Sun. Yet another theory is a large impact on Earth tore away a nice sized chunk of debris that later evolved to become our Moon. A new theory has been published in Nature Magazine in that a large Mars sized body struck the Earth and two large chunks appeared eventually coming together to form our Moon. This could explain why the side of the Moon facing us has many low lying areas and the far side of the Moon has a thicker crust ans is more cratered. Below is the article from Nature.
Earth once had two moons, which merged in a slow-motion collision that took several hours to complete, researchers propose in Nature today.
Both satellites would have formed from debris that was ejected when a Mars-size protoplanet smacked into Earth late in its formation period. Whereas traditional theory states that the infant Moon rapidly swept up any rivals or gravitationally ejected them into interstellar space, the new theory suggests that one body survived, parked in a gravitationally stable point in the Earth–Moon system.
Several such ‘Lagrangian’ points exist, but the two most stable are in the Moon’s orbit, 60° in front or 60° behind.
Traces of this ‘other’ moon linger in a mysterious dichotomy between the Moon’s visible side and its remote farside, says Erik Asphaug, a planetary scientist at the University of California, Santa Cruz, who co-authored the study with Martin Jutzi, now of the University of Berne.
The Moon’s visible side is dominated by low-lying lava plains, whereas its farside is composed of highlands. But the contrast is more than skin deep. The crust on the farside is 50 kilometres thicker than that on the nearside. The nearside is also richer in potassium (K), rare-earth elements (REE) and phosphorus (P) — components collectively known as KREEP. Crust-forming models show that these would have been concentrated in the last remnants of subsurface magma to crystallize as the Moon cooled.
What this suggests, Asphaug says, is that something ‘squished’ the late-solidifying KREEP layer to one side of the Moon, well after the rest of the crust had solidified. An impact, he believes, is the most likely explanation.
“By definition, a big collision occurs only on one side,” he says, “and unless it globally melts the planet, it creates an asymmetry.”
Asphaug and Jutzi have created a computer model showing that the Moon’s current state can be explained by a collision with a sister moon about one-thirtieth the Moon’s mass, or around 1,000 kilometres in diameter.
Such a moon could have survived in a Lagrangian point long enough for its upper crust and that of the Moon to solidify, even as the Moon’s deeper KREEP layer remained liquid.
Meanwhile, tidal forces from Earth would have been causing both moons to migrate outward. When they reached about one-third of the Moon’s present distance (a process that would take tens of millions of years), the Sun’s gravity would have become a player in their orbital dynamics.
“The Lagrange points become unstable and anything trapped there is adrift,” Asphaug says. Soon after, the two moons collided. But because they were in the same orbit, the collision was at a relatively low speed.
“It’s not a typical cratering event, where you fire a ‘bullet’ and excavate a crater much larger than the bullet,” Asphaug says. “Here, you make a crater only about one-fifth the volume of the impactor, and the impactor just kind of splats into the cavity.”
Like A Pancake
In the hours after the impact, gravity would have crushed the impactor to a relatively thin layer, pasted on top of the Moon’s existing crust. “You end up with a pancake,” Asphaug says. The impact would have pushed the still-liquid KREEP layer to the Moon’s opposite side.
Apshaug’s theory isn’t the only attempt to explain the lunar dichotomy. Others have invoked tidal effects from Earth’s gravity, or convective forces from cooling rocks in the Moon’s mantle.
“The fact that the nearside of the Moon looks so different to the farside has been a puzzle since the dawn of the space age,” says Francis Nimmo, one of the authors of a 2010 paper in Science proposing tidal forces as the cause.
But despite his competing model, Nimmo (a colleague of Asphaug’s at Santa Cruz, but not an author of the new study) calls the new theory “elegant”.
And Peter Schultz of Brown University in Providence, Rhode Island, calls it “interesting” and “provocative”, despite his own theory involving a high-angle collision at the Moon’s south pole, which he believes would have pressed crustal material northward to form the farside highlands.
“All this is great fun and tells us that there are very fundamental questions that remain about the Moon,” he says.
NASA’s upcoming GRAIL mission, designed to probe the Moon’s interior using precise measurements of its gravity, may help figure out what happened billions of years ago. “But in the end,” Schultz says, “new lunar samples may be necessary.”
Author: Richard Lovett