Answered: Use Kuiper Belt Object Haumea's… | bartleby

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a) Dp =
Da =
b) p² =
a³-

Use Kuiper Belt Object Haumea's eccentricity; e = 0.189, semimajor axis, a = 43.3
AU, and Period, P = 285 yrs, values to
a) calculate its perihelion and aphelion distances with Dp = a (1 e) and D₂ = a (1 + e),
b) verify if Haumea's a and P satisfy Kepler's third law for all objects orbiting the Sun:
p2 = a³.
Show your work.
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a) Dp=
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b) p2=
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