Answer:
1.

2.

3.

Step-by-step explanation:
The apparent brightness is inversally proportional to the square of distance, and it can be written as:

Where, for instance, state 1 is the Earth (given, known values) and state 2 is the unknown value. Knowing a new distance leads to a known apparent brightness, and viceversa.
This is a very simple proportionallity law, so, rearranging the equation:

1. For a distance of half the distance from the Sun (i.e., 0.5 AU, regardless its actual value since we are using AU multiples):

2. Similarly, for r2=2AU:

3. Finally, for r2=7AU:
