मराठी

Biochemical Origin of Life - Second step: Origin of Molecules and Simple Inorganic Compounds

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Estimated time: 8 minutes
CISCE: Class 12

Early Earth Conditions

  • Temperature of primitive Earth was extremely high (about 5000–6000°C).
  • Under such high temperature, elements like hydrogen, oxygen, carbon, and nitrogen could not remain in a free state.
  • These elements combined to form simple inorganic compounds such as oxides, carbides, and nitrides.
  • Water was present as superheated steam, not as liquid.
CISCE: Class 12

Formation of Simple Inorganic Compounds

Reactive elements (H, C, O, and N) combined due to high-energy conditions.

Formed basic inorganic compounds:

  • Oxides (from oxygen)
  • Carbides (from carbon)
  • Nitrides (from nitrogen)

These were among the earliest chemical substances on Earth and formed the base for later chemical evolution.

CISCE: Class 12

Cooling of Earth and Formation of Oceans

  • Gradual cooling of Earth allowed superheated steam to condense into rain.
  • Continuous rainfall over a long period led to the accumulation of water on the surface.
  • Hot boiling seas/oceans were formed.

These early oceans contained:

  • Dissolved gases (methane, ammonia)
  • Minerals and salts.
CISCE: Class 12

Composition and Nature of Primitive Atmosphere

Around 3600 million years ago, Earth had:

  • Solid crust
  • Active volcanic eruptions
  • Hot oceans.

Atmosphere was reducing in nature (no free oxygen).

Major gases present:

  • Hydrogen (H₂)
  • Methane (CH₄)
  • Ammonia (NH₃)
  • Carbon dioxide (CO₂)
  • Nitrogen (N₂)
  • Water vapour (H₂O).
CISCE: Class 12

Key Points: Origin of molecules and simple inorganic compounds

  • Due to extremely high temperatures on early Earth, elements like hydrogen, carbon, oxygen, and nitrogen combined to form simple inorganic compounds such as oxides, carbides, and nitrides.
  • As the Earth cooled, water vapour condensed into rain, leading to the formation of oceans containing dissolved gases like methane, ammonia, minerals, and salts.
  • The primitive Earth had a reducing atmosphere rich in hydrogen, methane, ammonia, carbon dioxide, and water vapour, with no free oxygen present.
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