Intrinsic Water Formation vs. Asteroid Delivery on Early Earth - Episode Hero Image

Intrinsic Water Formation vs. Asteroid Delivery on Early Earth

Original Title: Did Earth’s Water Come From Space?

TL;DR

  • Earth's water likely originated from carbonaceous chondrite asteroids, not comets, due to matching deuterium-to-hydrogen ratios, implying a significant early solar system material shuffling mechanism.
  • The formation of water internally on Earth is a viable hypothesis, involving reactions between a hydrogen-rich atmosphere and a molten magma ocean during the planet's early stages.
  • Lab experiments using diamond anvil cells confirm that water can be synthesized from iron oxides and hydrogen gas under high pressure and temperature conditions, supporting internal formation theories.
  • The debate over Earth's water origin highlights the dynamic nature of early solar system formation, where gas giant gravitational interactions likely redistributed water-rich materials inward.
  • Understanding Earth's water origin is crucial for identifying potentially habitable exoplanets, as it informs whether water is delivered externally or formed intrinsically on planets.

Deep Dive

The origin of water on Earth remains a fiercely debated topic in astrobiology, with compelling evidence now supporting the idea that water may have formed intrinsically during Earth's early stages rather than solely being delivered by comets or asteroids. This shift in understanding has profound implications for how we search for life beyond Earth, suggesting that water-rich worlds might be more common than previously assumed.

Historically, the prevailing scientific view posited that Earth formed "bone dry" due to its proximity to the hot, inner solar system, and that water was subsequently delivered by icy objects from beyond the "snow line" -- the region where water could condense into ice. Initially, comets were considered the primary delivery mechanism, but analysis of the deuterium-to-hydrogen (D/H) ratios in cometary water did not match Earth's water. This led to a re-evaluation, with certain types of carbonaceous chondrite asteroids, which formed beyond the snow line and possess a compatible D/H ratio, becoming the favored candidates. Dynamical simulations suggest that the gravitational influence of gas giants like Jupiter and Saturn could have scattered these water-rich asteroids inward, delivering a significant portion of Earth's water.

However, a more recent and increasingly compelling hypothesis suggests that water could have been generated on Earth itself during its formation. This theory posits that Earth's early environment, characterized by a molten magma ocean and a thick atmosphere of hydrogen gas, contained the necessary ingredients. The reaction between hydrogen gas (H2) and iron oxides (Fe-O) present in the molten rock could have produced water (H2O). Experimental evidence, using a diamond anvil cell to replicate the high pressures and temperatures of early Earth, has now demonstrated that this reaction is indeed feasible in a laboratory setting. This "in-situ" water formation theory challenges the long-held assumption that Earth's building materials were inherently dry.

The implications of this debate are significant for the search for extraterrestrial life. If water can be intrinsically generated during planet formation, then water-rich worlds might be far more common across the galaxy than if water delivery from specific extraterrestrial sources was the only viable pathway. Future telescopes capable of analyzing exoplanet atmospheres could test these hypotheses by searching for signs of water, helping to distinguish between planets that received water from external delivery versus those that formed with it internally. This refined understanding of water's origin on Earth directly informs our strategy and optimism in identifying potentially habitable exoplanets.

Action Items

  • Audit water origin hypotheses: Compare deuterium-to-hydrogen ratios for Earth, comets, and carbonaceous chondrites to identify primary delivery mechanisms.
  • Design laboratory experiment: Replicate water formation from hydrogen gas and iron oxides under high pressure and temperature conditions (ref: diamond anvil cell).
  • Measure isotopic ratios: Obtain precise deuterium-to-hydrogen measurements for 5-10 diverse asteroid samples to refine delivery models.
  • Analyze exoplanet data: Search for signs of water-rich worlds among 20-30 nearby exoplanets to test universal water formation theories.

Key Quotes

"Currently planetary scientists are taught that water wasn't really present when our planet was forming we thought that earth was like pretty bone dry to begin with so it had to be delivered from somewhere else in the solar system."

Michael Wong, an astrobiologist and planetary scientist, explains the prevailing scientific understanding that Earth was initially dry and required external delivery of water. This perspective shaped early hypotheses about the origin of Earth's water.


"And we noticed that comets and asteroids have very different ratios of deuterium to hydrogen or different amounts of hdo mixed in the regular h2o and you can compare that to the amount of hdo that we find here on earth you get a rough sort of estimate for like what the d to h ratio is for the earth you compare that to the d to h ratios for comets oops they don't match at all and then you go to the d to h ratio for these specific kinds of asteroids called carbonaceous chondrites which are these asteroids that are rich in carbon but also very rich in water and you say oh that kind of looks the same."

Wong highlights the significance of the deuterium-to-hydrogen ratio as a key clue in tracing the origin of water. He notes that this ratio in comets does not match Earth's, while certain types of carbonaceous chondrite asteroids show a similar ratio, suggesting a potential source of Earth's water.


"We think that the gas giants may have been actually responsible for this... JUPITER AND SATURN DO MOST OF THE HEAVY LIFTING BUT... SOMETIMES URANUS AND NEPTUNE IN THESE WHAT WE CALL DYNAMICAL SIMULATIONS... AND JUPITER AND SATURN JUST WRECK HAVOC ON THE ENTIRE SOLAR SYSTEM SOMETIMES URANUS AND NEPTUNE ACTUALLY SORT OF FLIP PLACES."

Wong discusses the role of gas giants in planetary science, explaining that their gravitational influence, as shown in dynamical simulations, could have disrupted the solar system. This chaos may have been responsible for flinging water-rich material from the outer solar system inward to Earth.


"The idea that okay you form a terrestrial planet and along with that formation process you create water may have been the original way that people just thought water spawned on a planet because we didn't know that we didn't know about asteroids and comets and so you know this idea that the water had to be delivered from somewhere else only came about once we realized that okay the initial material of the earth was bone dry it was just too hot here for there to be water intrinsically but you could form that water shortly after the planet was created out of bone dry material."

Wong describes an earlier hypothesis where water was thought to form concurrently with a terrestrial planet's creation. This idea emerged before the understanding of asteroids and comets, and before the realization that early Earth's conditions made intrinsic water formation unlikely.


"Basically if you go right to the beginning of planet earth you've got a magma ocean... and the plane is sort of the spacecraft of our imagination is soaring not in an atmosphere of mostly nitrogen and oxygen as we have today but a hot thick atmosphere of hydrogen gas... and the combination of hydrogen gas h2 and this magma ocean which is full of what we call iron oxides basically iron bonded to oxygen those two components iron oxides and hydrogen gas can react together or so the theory went to basically rip the oxygen off of the iron oxide and deposit it in hydrogen therefore creating water."

Wong explains a theoretical mechanism for water formation on early Earth, involving a magma ocean and a thick atmosphere of hydrogen gas. He posits that the reaction between iron oxides in the molten rock and hydrogen gas could have produced water.


"People have come up with this theoretical model of taking iron oxides and hydrogen and oh yeah you should just be able to make water out of that but this paper shows that you actually can in the lab and they used a very clever technique called a diamond anvil cell to do it."

Wong references a recent scientific paper that experimentally validates the theoretical model of water creation. He notes that researchers used a diamond anvil cell, a technique that applies extreme pressure and temperature, to demonstrate this reaction in a laboratory setting.

Resources

External Resources

Books

  • "The Origin of Water on Earth" by Michael Wong - Mentioned as a theoretical paper on water formation.

Articles & Papers

  • "Diamond Anvil Cell" (Unspecified Publication) - Discussed as a laboratory technique used to simulate planetary conditions for water formation research.

People

  • Michael Wong - Astrobiologist and planetary scientist at Carnegie Science, guest on the podcast discussing the origin of water on Earth.

Organizations & Institutions

  • Carnegie Science - Institution where Michael Wong is an astrobiologist and planetary scientist.
  • NPR - The public radio network producing the podcast "Shortwave."
  • LinkedIn Ads - Sponsor of the podcast, offering advertising services for B2B marketing.
  • Edward Jones - Sponsor of the podcast, a financial advisory firm.
  • Capella University - Sponsor of the podcast, an online university.
  • Bombas - Sponsor of the podcast, a company selling engineered socks.
  • Indiana University - Sponsor of the podcast, a university with industry partnerships.

Other Resources

  • Deuterium to Hydrogen Ratio - Used as a clue to determine the origin of water by comparing ratios in comets, asteroids, and Earth.
  • Protoplanetary Disk - The swirling disk of gas and dust from which planets form.
  • Snow Line - The point in a protoplanetary disk where water can condense into ice.
  • Asteroids - Celestial bodies discussed as a potential source of Earth's water.
  • Comets - Celestial bodies discussed as a potential source of Earth's water.
  • Carbonaceous Chondrites - A specific type of asteroid rich in carbon and water, discussed as a source of Earth's water.
  • Gas Giants (Jupiter, Saturn, Uranus, Neptune) - Planets whose gravitational influence may have shuffled material in the early solar system, potentially delivering water-rich asteroids to Earth.
  • Dynamical Simulations - Computer models used to understand the motion of planets and their effect on solar system material.
  • Oort Cloud - A theoretical shell of icy objects surrounding the solar system, mentioned in the context of scattering material inward.
  • Kuiper Belt - A region of icy bodies beyond Neptune, mentioned in the context of scattering material inward.
  • Magma Ocean - A molten layer of rock on the early Earth's surface, discussed as a component in water formation.
  • Hydrogen Gas (H2) - A component of Earth's early atmosphere, discussed as a reactant in water formation.
  • Iron Oxides - Compounds found in Earth's early rocks, discussed as a reactant in water formation.
  • Exoplanets - Planets outside our solar system, mentioned as potential locations to test hypotheses about water worlds.

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