Answer:
We can use the conservation of angular momentum to solve this problem. According to this principle, the angular momentum of a planet in its elliptical orbit is conserved, meaning that the product of its orbital velocity and its distance from the star is constant.
Let's denote the planet's speed when it is closest to the star by v1, and its speed when it is farthest from the star by v2. Similarly, let's denote the planet's distance from the star when it is closest and farthest by r1 and r2, respectively.
Using the conservation of angular momentum, we can write:
v1 * r1 = v2 * r2
Plugging in the values given in the problem, we get:
v1 * 46 million km = 38 km/s * 85 million km
Solving for v1, we get:
v1 = (38 km/s * 85 million km) / 46 million km
v1 = 70 km/s
Therefore, the planet is moving at a speed of 70 km/s when it is closest to the star.