Why are
planets round
Isostatic
adjustment
Thermal
Equilibrium
Hydrostatic
equilibrium
Stes de Necker
Isostatic adjustment
Planets are round because their
gravitational field acts as though it originates from the center of the body
and pulls everything toward it.
With its large body and internal heating
from radioactive elements, a planet behaves like a fluid, and over long periods
of time succumbs to the gravitational pull from its center of gravity. The only
way to get all the mass as close to planet's center of gravity as possible is
to form a sphere.
The technical name for this process is
"isostatic adjustment."
With much smaller bodies, such as asteroids (50 to 500 miles) the gravitational pull is too weak to overcome the asteroid's mechanical
strength. As a result, these bodies do not form spheres. Rather they maintain
irregular, fragmentary shapes.
Thermal Equilibrium
Thermal equilibrium is
the tendency of thermal energy
to flow so that temperature differences
are equalized. Equilibrium applies to gravity, too.
Every part of a planet’s surface has a
gravitational potential energy. This quantity can be expressed as the product
of the object’s mass (m),
the acceleration of
gravity (g), and the height of the object (h):
PEGravity = m * g * h
So potential energy increases with the mass of the planet (because a more massive planet will have a larger value of g), and with the distance from the planet’s center.
PEGravity = m * g * h
So potential energy increases with the mass of the planet (because a more massive planet will have a larger value of g), and with the distance from the planet’s center.
Gravity pulls all the parts of an object
toward its center of mass.
Gravity always works to minimize the
potential energy of
all parts of a planet. High places have a larger gravitational potential energy,
and are pulled downward more strongly than low places.
Take a large tray and cover it with sand or
gravel heaped into "mountains." If you shake the tray, the sand will
quickly settle to a flat surface where the gravitational potential energy is
the same everywhere. This is an example of equilibrium.
Large bodies in the solar system have
enough mass so
that their strong gravity
forces their surfaces to have the same potential energy everywhere.
The result is the most symmetric shape possible: a sphere.
The Earth is as round and smooth as a
billiard ball.
Small asteroids, however, do not have
enough gravity to overcome the strength of the rock they are made of. So they
have irregular shapes.
Asteroid Ida with its tiny moonlet Dactyl
Hydrostatic equilibrium
Planets are round also because their mass
is large enough to trigger hydrostatic equilibrium. Hydrostatic
equilibrium is where an objects own gravity pulls high places down and pushes
low places up until all pressures are equalized and the object is round.
It is very much like a bubble. The
pressure on the inside and outside of a round bubble are the same.
If a part of the bubble is sticking out,
there is more pressure on the outside of the part sticking out than on the
inside of the part sticking out. That pressure pushes the bubble until it
is not sticking out any more. It doesn't keep pushing on that part,
because then there would be more pressure on the inside of the bubble than the
outside, and the part being pushed in would be pushed back out again.
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