Enstatite dendrites are good objects of study for investigating the planet's origin and the early solar system. They are likely made up of the same materials that formed young Earth. Previous research found that both rocky bodies share striking isotopic similarities: Enstatite chondrites have similar oxygen, calcium and titanium isotopes as Earth, which indicates that their hydrogen and nitrogen isotopes are similar as well.
However, most geoscientists assumed that enstatite chrondites formed too close to the sun. As a result, the rocks were often considered dry, prompting scientists to avoid any exhaustive search of hydrogen in them.
For the study, the researchers examined pristine enstatite chondrites -- rocks that were neither altered on Earth nor on their asteroid during the early years of the solar system.
Using conventional mass spectrometry and secondary ion mass spectrometry, the team was able to measure the content and composition of hydrogen in the meteorites. Because hydrogen reacts with oxygen to produce water, knowing how much hydrogen is in the rocks would indicate how much water the rocks contributed to young Earth.
The researchers found that the amount of hydrogen in the rocks could contribute to three times more than the current volume of today's ocean waters. They also posited that a large amount of atmospheric nitrogen, the most abundant gas in Earth's atmosphere, could have come from the pristine rocks.
These findings show that enstatite chondrites, identified to be the building blocks of the planet, may explain the origin of Earth's water.
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