The oceans of early Earth were significantly different from modern oceans in terms of composition and conditions. They were likely more acidic and rich in dissolved metals, with higher concentrations of gases like carbon dioxide and lesser amounts of oxygen. Additionally, early oceans were influenced by volcanic activity and lacked the diverse ecosystems found today, as life was just beginning to emerge. Over time, biological processes and geological changes led to the development of the more stable and diverse oceans we see now.
there were meteorites, a lot of space debris and lightning and liquid water eventually made the oceans.
the Earth's early history when water vapor was released from volcanic activity and comets colliding with the planet. This water then accumulated in the Earth's crust and eventually formed the oceans through various geological processes.
Cro-Magnon were early modern humans. Other than living in the stone age, they were just like us.
The water vapor in the early atmosphere of Earth likely condensed and fell as rain, contributing to the formation of the oceans. This process, known as the "water cycle," involves the continuous movement of water between the atmosphere, land, and oceans through processes like evaporation, condensation, and precipitation. Over time, the oceans became the primary reservoir for water on Earth, where it remains today.
One piece of evidence is the presence of ancient rocks found on continents that show evidence of having been formed in marine environments. Additionally, the chemical composition of Earth's oldest rocks suggests interaction with seawater, indicating the existence of oceans. Isotope ratios in certain minerals also provide clues about the early presence of oceans on Earth.
Condensed water vapor formed the oceans as rain fell on Earth's surface over millions of years, filling depressions in the land and creating bodies of water. Additionally, water was brought to Earth by comets and asteroids during its early formation. The accumulation of water in these depressions eventually led to the formation of the oceans as we know them today.
As the early Earth cooled, the water vapor in the atmosphere condensed and fell as rain, leading to the formation of the Earth's oceans. This process is known as the "primordial rainout" and it played a crucial role in shaping the planet's surface and creating the conditions for life to emerge.
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The Earth's atmosphere likely developed from gases released during volcanic eruptions. Outgassing also contributed to the formation of the Earth's early atmosphere and the oceans through the release of water vapor and other volatile compounds.
Water vapor condensed to form oceans on Earth's surface early in Earth's history, as the planet cooled down and the atmospheric temperature decreased to a point where the water vapor could no longer remain in its gaseous state.
Water vapour (produced rain-rivers, lakes, oceans) carbon dioxide nitrogen
dissolved solids were carried from land into oceans