While the Earth’s atmosphere can play a role through factors such as such as wind and water erosion in erasing the visual evidence of impact craters it is a secondary mechanism.
The size of an impact crater is a function of the kinetic energy KE of the object striking the surface.
The KE is defined by the equation KE = 0.5mv² where m and v are the mass and velocity of the object respectively.
When the object such as an asteroid enters the atmosphere it rapidly decelerates forming a high pressure air front with comparatively little pressure behind or to the sides of the object.
This places the object under considerable stress.
If the pressure build up is considerable, air is forced into the pores and cracks causing the object to fragment with pieces distributing themselves laterally.
This is known as the "pancake effect."
The collection of smaller pieces has a larger front-facing surface area, causing even more stress build up.
In very short order, a runaway fragmentation cascade disintegrates the object, where the loss of KE through deceleration is converted into the KE of individual fragments flying through the atmosphere which may impact the Earth.
The absence of large meteorite craters on Earth compared to what is found on the moon is therefore due to a reduction in the KE through loss of mass and reduction of velocity.
An extreme case occurs where the object explodes above the surface and leaves no crater.
This occurred in 1908 known as the Tunguska event which flattened an estimated 80 million trees over an area of 2,150 km² of forest.
On a less spectacular note a few years ago I observed a bolide which was brighter than the full moon and had a greenish colour probably due to an iron-nickel meteor.
The bolide broke up into a number of fragments each leaving a trail in the sky and was accompanied by a thunderclap sound.
The size of an impact crater is a function of the kinetic energy KE of the object striking the surface.
The KE is defined by the equation KE = 0.5mv² where m and v are the mass and velocity of the object respectively.
When the object such as an asteroid enters the atmosphere it rapidly decelerates forming a high pressure air front with comparatively little pressure behind or to the sides of the object.
This places the object under considerable stress.
If the pressure build up is considerable, air is forced into the pores and cracks causing the object to fragment with pieces distributing themselves laterally.
This is known as the "pancake effect."
The collection of smaller pieces has a larger front-facing surface area, causing even more stress build up.
In very short order, a runaway fragmentation cascade disintegrates the object, where the loss of KE through deceleration is converted into the KE of individual fragments flying through the atmosphere which may impact the Earth.
The absence of large meteorite craters on Earth compared to what is found on the moon is therefore due to a reduction in the KE through loss of mass and reduction of velocity.
An extreme case occurs where the object explodes above the surface and leaves no crater.
This occurred in 1908 known as the Tunguska event which flattened an estimated 80 million trees over an area of 2,150 km² of forest.

On a less spectacular note a few years ago I observed a bolide which was brighter than the full moon and had a greenish colour probably due to an iron-nickel meteor.
The bolide broke up into a number of fragments each leaving a trail in the sky and was accompanied by a thunderclap sound.
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