Traces of Indigenous Gas Found in Meteorite to Shed Light on Moon’s Origin

The most popular theory about the formation of the Moon is that it is the result of a collision between Earth and another celestial object. Now, a study has suggested that the Moon may have a deeper relationship with the Earth. Scientists from the ETH Zurich have concluded that Moon inherited some noble gases, such as neon and helium, deep from the Earth’s mantle. The discovery was made by analysing lunar meteorites found in Antarctica.

The team found that the traces of noble gases in the meteorites matched those in the solar gases. The findings are likely to help astronomers understand the process through which Earth, Moon, and other celestial bodies were formed.

In the study, published in Science Advances, doctoral researcher Patrizia Will obtained six samples of the lunar meteorites found in Antarctica and studied them. These celestial bodies consist of basalt rock that is formed after magma spews out of the Moon’s interior and cools rapidly. They remained covered by multiple basalt layers, protecting them from the cosmic rays, especially solar wind. This cooling process led to the formation of lunar glass particles along with other materials found in the magma.

Upon analysing the glass particles, the team found chemical fingerprints or isotopic signatures of the solar gases in them. These included helium and neon that are present in the Moon’s interior. “Finding solar gases, for the first time, in basaltic materials from the Moon that are unrelated to any exposure on the lunar surface was such an exciting result,” said Will.

The team used a state-of-the-art noble gas mass spectrometer at the Noble Gas Laboratory of ETH Zurich. They used the instrument to measure the sub-millimeter glass particles and were able to rule out solar winds as the possible source of the detected gases.

“I am strongly convinced that there will be a race to study heavy noble gases and isotopes in meteoritic materials,” said ETH Zurich Professor Henner Busemann, one of the world’s leading scientists in the field of extra-terrestrial noble gas geochemistry.

The professor added that while such gases are not necessary for the survival of life, it would be fascinating to unravel how they survived the brutal formation of the Moon. It is also likely to help scientists create more new models explaining the process.


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Researchers to Scan Ocean Floor for Meteorite That Crashed on Earth in 2014

A mysterious object from space crashed into the ocean off the coast of Papua New Guinea in 2014. Called the CNEOS 2014-01-08, the meteorite has still kept scientists puzzled about its origin but initially, it was speculated that it could be an interstellar object. After its discovery, researchers namely then graduate Amir Siraj, and Harvard professor Avi Loeb first suspected its possible interstellar origin. Now, they are chalking up plans to scan the ocean floor for the object and have described their idea in a new research paper.

The object is estimated to be some half-metre wide and researchers have used catalog data on the object’s trajectory to dig out information on it. They noted the high heliocentric velocity of the object and concluded that it could belong to a place beyond our solar system. This meant that with such speed, it was indicative that the meteorite was not bound by the gravity of the Sun. Siraj and Loeb used data from a US Department of Defense spy satellite to measure the object’s impact on Earth.

However, the satellite is used for monitoring Earthly military activities and the exact error values of measurement taken by it are not in the public domain. Hence, this makes it difficult to confidently declare CNEOS 2014-01-08 as an interstellar object.

The findings of Siraj and Loeb were echoed by the US Space Force’s Space Operations Command’s Chief Scientist, Joel Mozer in 2019. He, after analysing the data on the object “confirmed that the velocity estimate reported to NASA is sufficiently accurate to indicate an interstellar trajectory.”

6/ “I had the pleasure of signing a memo with @ussfspoc‘s Chief Scientist, Dr. Mozer, to confirm that a previously-detected interstellar object was indeed an interstellar object, a confirmation that assisted the broader astronomical community.” pic.twitter.com/PGlIOnCSrW

— U.S. Space Command (@US_SpaceCom) April 7, 2022

Now, researchers have aimed at searching for the fragments of the meteorite that could be scattered on the ocean floor. For this, the tracking data from the satellite and wind and ocean current data can help narrow down their search.

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Planet Formation Theory Upset After New Study Of Mars Meteorite

The planetary formation theory that scientists have been referring to for decades seems to have been jeopardised by a recent study regarding an old meteorite. The theory explained how rocky planets like the Earth and Mars acquire volatile elements such as hydrogen, carbon, oxygen, nitrogen and noble gases during the formative stages. During the research, scientists observed minute quantities of krypton isotopes in samples of the meteorite. The low abundance of krypton isotopes makes it more difficult to measure. Hence, in order to find out the origin of these isotopes, researchers used a new method set up at the UC Davis Noble Gas Laboratory.

According to Sandrine Péron, a postdoctoral scholar working with Professor Sujoy Mukhopadhyay in the Department of Earth and Planetary Sciences, University of California, Davis, “A basic assumption about planet formation is that planets first collect these volatiles from the nebula around a young star.” But the recent study contradicts the process.

Scientists found that the krypton isotopes in the meteorite suggest that they originated from meteorites and not from the solar nebula. This suggests that meteorites were delivering volatile elements to planets at a much earlier formative stage, even in the presence of the solar nebula, which is contradictory to what was previously believed.

The new study indicates that the growth of Mars was completed before the radiation from the sun dissipated the nebula. But the irradiation should also have blown off the nebular atmosphere on Mars. This means that atmospheric krypton must have been preserved in some way, either by being trapped underground or stored in polar ice caps.

Professor Mukhopadhyay said, “However, that would require Mars to have been cold in the immediate aftermath of its accretion. While our study clearly points to the chondritic gases in the Martian interior, it also raises some interesting questions about the origin and composition of Mars’ early atmosphere.”

Krypton, among other noble gases, is instrumental in discovering the source of volatile materials on planets.

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