.
Kepler's first law
Kepler's third law
The Law of Equal Areas
The Law of Inertia
The mass of the sun
The mass of Earth
The mass of the central object
The mass of the orbiting object
A1 = A2.
Delta t1 > delta t2.
If delta t1 = delta t2, then the orbit is circular.
If delta t1 = delta t2, then A1 = A2.
It would increase by a factor of 2.
It would increase by a factor of 4.
It would decrease by a factor of 2.
The speed would not change.
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