No turtles lay up to 90 egggs
Accretionary collisions during Earth's formation did cause some heat loss, as the kinetic energy from impacts was converted into heat. However, the heat loss from these collisions was likely not the primary contributor to the overall heating of the early Earth, as other processes such as radioactive decay and gravitational compression played larger roles in generating heat.
Evaporation
Lord Kelvin's
heat loss at the surface of the earth
heat loss at the surface of the earth
Heat loss varies all over the Earth due to differences in surface characteristics, such as land vs. water, altitude, and vegetation cover. Factors like sunlight angle, cloud cover, and atmospheric circulation patterns also play a role in how heat is distributed and lost across different regions. Patterns of heat loss are further influenced by ocean currents, prevailing winds, and the Earth's tilt and rotation.
The Earth retains heat better due to its thicker atmosphere and higher heat capacity compared to the moon. The atmosphere acts as a barrier, trapping heat on Earth, while the moon has no atmosphere to retain heat, causing rapid heat loss at night.
heat loss
They slow the loss of heat
Heat loss by electromagnetic radiation & by convection
the thicker the insulation is then there will be less heat loss. The material also affects heat loss
The Earth cooled down after its formation due to the loss of heat from its interior through a process called radiative cooling. As the Earth's surface solidified, heat continued to be transferred to the surface and eventually dissipated into space, causing the Earth's overall temperature to decrease gradually over time.