The frictional force between two surfaces is given by:

where

is the coefficienct of friction

is the force with which one surface is pushed against the other one
Looking at the formula, we see that there are two possible ways to increase the friction:
1) by increasing the coefficient of friction

(for instance, by making the surfaces more "rough"
2) by increasing

, the force with which one surface is pushed against the other
Similarly, in order to decrease the friction, the two possible ways are:
1) by reducing the coefficient of friction
2) by reducing the force
Answer:

Explanation:
The Stefan–Boltzmann law for a black body (as stars are treated) can be written as
, where
is the total energy radiated per unit surface area across all wavelengths per unit time,
the absolute temperature and
is the Stefan–Boltzmann constant.
If we multiply
by the surface area
of the star we get the total energy radiated across all wavelengths per unit time, which is the total power radiated, so we can write:

where we have used the formula for the surface area of a sphere 
Solving for r we have:

... Extreme temperature changes between seasons.
... Extreme changes in length of daylight and darkness.
... Larger areas around both poles where daylight/darkness
can last more than a whole day.
Altogether, these areas cover half of the planet.