We are asked to determine the perihelion distance of Halley's comet. To do that we will use the following formula:

Where:

To determine the distance of the semi-major axis we will use Kepler's third law

Where:

Now, we solve for "a" by taking the cubic root on both sides:
![\sqrt[3]{T^2}=a](https://img.qammunity.org/2023/formulas/physics/college/orajz22qy9nb4qw4fk7w30tupf1nzylv1s.png)
Now, we substitute the value of "T":
![\sqrt[3]{(67years)^2}=a](https://img.qammunity.org/2023/formulas/physics/college/dumarasqt3sh5072915p58to0mn5b0azbc.png)
Solving the operations:

Now we substitute this value in the formula for the perihelion:

Solving the operations:

Therefore, the perihelion distance is 0.5 Astronomical Units.