Answer:
v = 2.75 10⁴ m / s
Step-by-step explanation:
For this exercise we must use Kepler's third law which is an application of Newton's second law to the solar system
F = ma
where force is the force of gravity
F =
acceleration is centripetal
a =
we substitute
G m M / r² = m v² / r
= v²
v =
indicate that the radius of the orbit is r = 1.17 AU, let's reduce to the SI system
r = 1.17 AU (1.496 10¹¹ m / 1 AI) = 1.76 10¹¹ m
let's calculate
v =
Ra (6.67 10-11 1.991 10 30 / 1.76 10 11
v =
ra 7.5454 10 8
v = 2.75 10⁴ m / s