Oldest Earth Rock Found In Lunar Exile

When our young planet was taking a beating by massive impacts, bits were ejected into space—and some ended up on the moon.

An artist’s impression of what our planet probably looked like over 4 billion years ago, during the violent Hadean epoch [Simone Marchi (SwRI), SSERVI, NASA]

This is an interesting thought: When Apollo astronauts were busy exploring the lunar surface, it wasn’t just moon rocks that were crunching beneath their moon boots—bits of Earth were there too. But how did Earth stuff get mixed-in with moon stuff?

According to a new study published in the journal Earth and Planetary Science Letters, this question may be a controversial one, but it’s not without some compelling evidence.

During the Apollo 14 moon landing in February 1971, when NASA astronauts Alan Shepard and Ed Mitchell were exploring the Fra Mauro Highlands, they scooped up some moon rocks and returned them to Earth for study. Fast-forward 48 years and an international group of researchers think that a 2 gram shard of rock in one of their scoops has terrestrial origins. That is a cool find in itself, but this particular sample is ancient, and possibly the oldest sample of Earth rock ever found, heralding from a time when the Earth was a very different place.

Between 4 and 4.6 billion years ago, our planet was a mess. Still in the process of forming, it was getting pummeled by an incessant barrage of asteroids and comets. Many parts of the Earth’s surface would have been molten, all of it would have been cratered, and none of the continents or oceans that we are familiar with today would have been present (see the image at the top of this page for an imagining of what it may have looked like). This was the Hadean epoch — named after the Greek god of the underworld, Hades — and it would have been a hellish time.

Apollo 14’s Ed Mitchell using a map during an EVA [NASA]

With all these impacts, large and small, it seems logical to think that a few of these impacts would have been large enough to launch a sizable quantity of debris into space. Back then, the moon orbited Earth much closer than it does now — four times closer in fact (which is a cool thought; the moon would have loomed four times larger in Hadean skies than it does now). As the moon was closer, there would have been higher odds of the terrestrial collision debris to come crashing down on the lunar surface. And this was the beginning of the epic journey of the 2 gram shard of rock that was returned to Earth and now lives in a lab.

The international team of researchers are associated with the Center for Lunar Science and Exploration, a part of NASA’s Solar System Exploration Research Virtual Institute, and they carried out a new analysis technique to search for Earth rocks in the Apollo moon samples. In one of the samples was a piece that is composed of quartz, feldspar, and zircon. These minerals are all common on Earth, but not on the lunar surface. Their interest was piqued. Further chemical analysis of the sample revealed how the rock formed: it crystallized in an oxidized atmosphere at temperatures more akin to Earth’s at the time. Moon rock typically crystallized at much higher temperatures devoid of an oxygen-rich atmosphere. The implication is clear: this particular sample didn’t form on the moon, it formed on Hadean Earth. But its journey from the Earth to the moon and into an Apollo astronaut’s sample scoop is quite the epic story.

A sample of moon rock collected by Apollo 14 astronauts [NASA]

Through the chemical analysis on the sample, a surprising amount of detail about the hows and whens could be deduced. First, after considering the mineral components of the sample, the rock must have formed around 20 kilometers under the surface, in young Earth’s crust, approximately 4.1 billion years ago. At the time, it wasn’t uncommon for massive impacts to excavate craters thousands of kilometers wide. These impact events would have easily have reached 20 kilometers deep, blasting some Earth stuff into space. The 2-gram sample was likely part of a bigger chunk that eventually collided with the moon, creating its own lunar crater, where it remained, in relative peace for a couple of hundred million years. Then, around 3.9 billion years ago, another lunar impact pummeled the sample, partially melting it, burying it deeper under the moon’s surface.

This sample holds this incredible record of geological history of a time when massive impacts were very common, when planets were accreting mass and life was just beginning to emerge on an embryonic Earth. After that lunar impact, the sample remained buried in moon rock for a few billion years.

Then, 26 million years ago, a comparatively small meteoroid slammed into the moon to create the 340-meter wide Cone Crater. The 2-gram sample was once again kicked onto the moon’s surface where it was randomly scooped by Shepard or Mitchell in 1971. The photograph below shows the boulders at the rim of Cone Crater where the sample was collected:

A photo taken on the Apollo 14 mission in the Fra Mauro highlands of the moon showing a cluster of boulders on the rim of Cone Crater during EVA-2 [NASA]

Although it may be logical to assume that ancient rocky debris from Earth likely ended up on the moon’s surface, it’s phenomenal that a tiny piece of Hadean Earth was discovered in an Apollo 14 sample. This could be an indicator as to how common it is; Earth rock preserved for billions of years on a world with no weather or tectonic processes continually erasing signs of the geological past, helping us better understand how our planet evolved.

Doomsday, Whenever: Massive Asteroid Impacts Probably Happen at Random

We always seem to be “overdue” a devastating asteroid impact, but how can we be overdue if asteroids don’t have an impact schedule?

Don Davis/NASA

Humans are naturally tuned to seek out patterns in seemingly random events. It’s an evolutionary trait that has helped us become the smart Homo sapiens we are today.

This ability to spot patterns and predict cyclical events continues to dominate our everyday lives. For example, geologists chart seismic activity in hopes of seeing a tell-tail earthquake signal before the “big one” happens; farmers track seasonal cycles in an attempt to predict periods of drought; Wall Street traders use complex numerical models to warn of the next financial crisis (or, indeed, profit from the downturn). Also, astronomers try to find patterns in cosmic occurrences that could pose an existential threat.

We are, of course, talking asteroid impacts — cataclysmic events that have shaped all of the planets in our solar system. Although Earth’s atmosphere is very good at eroding away ancient impact craters, evidence for asteroid impacts in the geological history of our planet is very common. Frankly, it’s perfectly natural to be hit by large asteroids and comets; that’s how planets accrete rocky material, collect water and accumulate organic chemistry for life (on Earth, at least).

But should we get hit by a massive asteroid in the near future, it could be curtains for our civilization. So it sure would be handy if we could somehow use the geologic record of our planet, see how often we get punched, spot a cycle or some kind of pattern, predict then the next impact is likely to happen and — hopefully — plan for the next marauding space rock to make an appearance in our skies! (Whether we’ll be able to do anything about it is an entirely different matter.)

Although seeking out cycles in asteroid and comet strikes is a doomsayer’s favorite hobby, scientists have had a challenging time at pinning down any kind of pattern in historic asteroid impacts and, as a new study published in the journal Monthly Notices of the Royal Astronomical Society dramatically concludes, there may be no pattern at all.

But what could drive periodic asteroid or comet impacts in the first place? One hypothesis claims that the solar system’s “wobble” through the galactic plane may destabilize comets in the Oort Cloud periodically, causing an uptick in massive planetary impacts. Also, the much hyped solar twin, Nemesis, could gravitationally jumble asteroids during its long orbit around the sun. But neither hypothesis stands up to scrutiny and the existence of an extremely dim solar partner is becoming increasingly unlikely.

Regardless, previous studies have suggested that extinction-level impacts (of the magnitude of the one that wiped out, or at least greatly contributed to the extinction of the dinosaurs) occur roughly every 26 million years (the cause of which is open to debate), but researchers from ETH Zurich and Lund University in Sweden now refute this claim.

“We have determined … that asteroids don’t hit the Earth at periodic intervals,” Matthias Meier, of ETH Zurich’s Institute of Geochemistry and Petrology, said in a statement.

After studying precisely-dated impact craters around the world that were formed in the past 500 million years, Meier and Sanna Holm-Alwmark of Lund University dated some 22 craters with dates of impacts known to a precision of one percent.

Then, using a technique known as circular spectral analysis (CSA), they attempted to find the approximate-26 million year period in this set of craters. They found no such period.

Interestingly, Meier and Holm-Alwmark also found that some of the impact craters were of the same age, hinting at a common source. “Some of these craters could have been formed by the collision of an asteroid accompanied by a moon,” said Meier. “But in other cases, the impact sites are too far away from each other for this to be the explanation.”

One interesting example is the apparent close similarity in age of the famous 66 million-year-old, 110 mile-wide Chicxulub Crater in Mexico (that has been linked with the extinction of the dinosaurs) and the 15 mile-wide Boltysh Crater in the Ukraine. As pointed out by the researchers, although a definitive explanation for this coincidence isn’t immediately clear, the two impactors may have originated from a collision in the asteroid belt, sending fragments to Earth, hitting the planet within a very short period of one another.

And it’s these kinds of clustering impacts that the researchers have identified as being potential problems with previous statistical studies — they assumed each impact is distinct, when in fact, they happened at the same time, possibly skewing results and creating a pattern when, in fact, there wasn’t one.

“Our work has shown that just a few of these so-called impact clusters are enough to suggest a semblance of periodicity,” said Meier.

I have little doubt that these new findings will be disputed, spawning more studies pointing to other statistical techniques and a bigger impact crater data set, but it is interesting to think that, as far as extinction-level impact events go, there really may be no pattern to their occurrence.

We know that a doomsday asteroid is out there, and it will hit us, but it has a random impact date that is only known to our planet’s geological future.

Mars’ Ancient Mega-Floods Are Still Etched Into the Red Planet

Around 3.5 billion years ago — when basic life was just gaining a foothold on Earth — the Tharsis region on Mars was swamped with vast floods that scar the landscape to this day.

Rendered perspective view of Worcester Crater using Mars Express elevation data. The dramatic crater rim was carved by the flow of ancient floodwater (ESA)

Mars wears its geological history like a badge of honor — ancient craters remain unchanged for hundreds of millions of years and long-extinct volcanoes look as if they were venting only yesterday. This is the nature of Mars’ thin, cold atmosphere; erosional processes that rapidly delete Earth’s geological history are largely absent on the Red Planet, creating a smorgasbord of features that provide planetary scientists with an open book on Mars’ ancient past.

In this latest observation from the European Mars Express mission, a flood of biblical proportions has been captured in all its glory. But this flood didn’t happen recently, this flood engulfed a vast plain to the north of the famous Valles Marineris region billions of years ago.

It is believed that a series of volcanic eruptions and tectonic upheavals in the Tharsis region caused several massive groundwater releases from Echus Chasma, a collection of valleys some 100 kilometers (62 miles) long and up to 4 kilometers (2.5 miles) deep. These powerful bursts of water carved vast outflow channels into the adjacent Lunae Planum, contributing to the formation of the Kasei Valles outflow channels, releasing water into the vast Chryse Planitia plains which acted as a “sink.” Smaller “dendritic” channels can be seen throughout the plain, indicating that there were likely many episodic bursts of water flooding the region.

This context image shows a region of Mars where Kasei Vallis empties into the vast Chryse Planitia (NASA MGS MOLA Science Team)
This context image shows a region of Mars where Kasei Vallis empties into the vast Chryse Planitia (NASA MGS MOLA Science Team)

These floods happened between 3.4 to 3.6 billion years ago, less than a billion years after the most basic lifeforms started to appear on Earth (a period of time known as the Paleoarchean era).

In the middle of what was likely a powerful, vast and turbulent flows of water is Worcester Crater that was created before the Tharsis floods and, though its crater rim stands to this day and retains its shape, it was obviously affected by the flow of water, with a “tail” of sediment downstream.

ESA Mars Express observation of the mouth of Kasei Valles, as it transitions into Chryse Planitia. The large crater in the lower left is Worcester Crater. (ESA/DLR/FU Berlin)
ESA Mars Express observation of the mouth of Kasei Valles, as it transitions into Chryse Planitia. The large crater in the lower left is Worcester Crater (ESA/DLR/FU Berlin)

Also of note are smaller “fresh” craters that would have appeared long after the flooding took place, excavating the otherwise smooth outflow channels. These younger craters have tails that seem to be pointed in the opposite direction of the flow of water. These tails weren’t caused by the flow of water, but by the prevailing wind direction.

From orbital observations by our armada of Mars missions, it is well known that these channels contain clays and other minerals associated with the long-term presence of water. Although the Red Planet is now a very dry place, as these beautiful Mars Express images show, this certainly hasn’t always been the case.

Shock and Awe: Curiosity Laser-Blasts First Mars Rock

The laser-zapped rock "Coronation" -- inset image was taken by the ChemCam instrument, featuring the small laser burn. Credit: NASA/JPL-Caltech
The laser-zapped rock “Coronation” — inset image was taken by the ChemCam instrument, featuring the small laser burn. Credit: NASA/JPL-Caltech

After Mars rover Curiosity’s thunderous landing on Aug. 5/6, any hypothetical Martian on the surface would have been forgiven for being a little confused.

Setting down on the flat plain called Aeolis Palus inside Gale Crater, the six-wheeled, one-ton, nuclear-powered rover would have looked more like an alien battle tank being dropped off by a rather ominous-looking “Flying Saucer” than a scientific mission. But after the famous “sky crane” maneuver that lowered the rover with the precision of a Harrier Jump Jet, the “alien” robot didn’t start rolling over the Martian landscape zapping Mars rocks with its laser. Instead, it just sat there. For days. Occasionally there’d be a bit of action — such as Curiosity’s cameras swiveling, mast raising and high-gain antenna tracking the sky — but apart from that, our hypothetical Martians would probably not have thought much of this lack-luster invasion by an airdropped tank.

But that all changed today. Curiosity blasted a rock with its laser, marking the beginning of Curiosity’s Mars domination! Shock and awe, Mars rover style.

Alas, this isn’t a military exercise, but it is significant. Today marks the first day that one of our interplanetary robotic emissaries have used a laser on another planet in the name of science. NASA mission operators gave the go-ahead to carry out a test-run of the Chemistry and Camera instrument, or ChemCam, targeting a small rock (called “Coronation”) with 30 pulses of its laser over a 10-second period. According to the JPL press release, each pulse delivered more than a million watts of power for about five one-billionths of a second.

The fist-sized Mars rock -- called "Coronation", previously designated "N165" -- has become the first casualty scientific target of Curiosity's ChemCam intrument. Credit: NASA/JPL-Caltech
The fist-sized Mars rock — called “Coronation”, previously designated “N165” — has become the first casualty of war scientific target of Curiosity’s ChemCam instrument. Credit: NASA/JPL-Caltech

“We got a great spectrum of Coronation — lots of signal,” said ChemCam Principal Investigator Roger Wiens of Los Alamos National Laboratory, N.M. “Our team is both thrilled and working hard, looking at the results. After eight years building the instrument, it’s payoff time!”

The laser works by vaporizing the surface layers of exposed rock. Under the intense heating by such focused energy, a tiny sample of material rapidly turns into plasma. The the flash of light generated by the small, rapidly dissipating cloud of plasma can then by analyzed from afar by the ChemCam’s spectrometer. The light reveals what kinds of elements are contained in the sample, aiding Curiosity’s studies of the Red Planet. And the best thing is that ChemCam appears to be working better than expected.

“It’s surprising that the data are even better than we ever had during tests on Earth, in signal-to-noise ratio,” said ChemCam Deputy Project Scientist Sylvestre Maurice of the Institut de Recherche en Astrophysique et Planetologie (IRAP) in Toulouse, France. “It’s so rich, we can expect great science from investigating what might be thousands of targets with ChemCam in the next two years.”

To find out more about this landmark day for Curiosity and Mars exploration, read the JPL press release: “Rover’s Laser Instrument Zaps First Martian Rock

Sol 3: Beautiful, Beautiful Mars Dirt. In Color.

Rocks and regolith strewn over the ground near Mars rover Curiosity. Credit: NASA/JPL-Caltech
Rocks and regolith strewn over the ground near Mars rover Curiosity. Credit: NASA/JPL-Caltech

It looks like rocks and dust, right? Actually, it resembles the dusty parking lot near a beach where my family used to holiday when I was young — a sandy, ruddy, dusty patch devoid of grass where cars had worn down the top layer of dirt, exposing smoothed rock underneath. However, this isn’t a parking lot. Actually, scrub that, it IS a parking lot — Mars rover Curiosity’s parking lot in Aeolis Palus, a remarkably smooth plain inside Gale Crater on Mars.

I don’t have an awful lot to say about these new high-resolution images that have just been uploaded to the Mars Science Laboratory (MSL) mission site except that I really wish I were a geologist! I get the feeling that these images from a never before seen region of Mars will keep geologists busy for some time to come.

As Curiosity undergoes a software upgrade preparing it for surface operations, we’ve been patiently waiting for the mission site to upload new images (beyond the color thumbnail teasers) of the surrounding area. And it seems that on Saturday night that happened. Here are some of my favorite views from Curiosity’s Mastcam:

Curiosity's sundial on its deck reads: "Mars 2012 -- To Mars To Explore"
Curiosity’s sundial on its deck reads: “Mars 2012 — To Mars To Explore”

Discoloration in the top soil in the location of a crater formed by Curiosity's Sky Crane rockets. Credit: NASA/JPL-Caltech
Discoloration in the top soil in the location of a crater formed by Curiosity’s Sky Crane rockets. Credit: NASA/JPL-Caltech

The deployed high-gain antenna. Credit: NASA/JPL-Caltech
The deployed high-gain antenna. Credit: NASA/JPL-Caltech

The crater rim and detail of undulating terrain -- possibly dunes. Credit: NASA/JPL-Caltech
The crater rim and detail of undulating terrain — possibly dunes. Credit: NASA/JPL-Caltech