Using the center-of-mass equations or the Center of Mass Calculator (under Binary-Star Basics, above), you will investigate a specific binary-star system. Assume that Star 1 has m₁ = 3.4 solar masses, Star 2 has m₂ = 1.4 solar masses, and the total separation of the two (R) is 52 AU. (One AU is Earth's average distance from the Sun.) (a)What is the distance, d₁, (in AU) from Star 1 to the center of mass? _AU (b) What is the distance, d2, (in AU) from Star 2 to the center of mass? _AU
Using the center-of-mass equations or the Center of Mass Calculator (under Binary-Star Basics, above), you will investigate a specific binary-star system. Assume that Star 1 has m₁ = 3.4 solar masses, Star 2 has m₂ = 1.4 solar masses, and the total separation of the two (R) is 52 AU. (One AU is Earth's average distance from the Sun.) (a)What is the distance, d₁, (in AU) from Star 1 to the center of mass? _AU (b) What is the distance, d2, (in AU) from Star 2 to the center of mass? _AU
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Transcribed Image Text:Using the center-of-mass equations or the Center of Mass Calculator (under
Binary-Star Basics, above), you will investigate a specific binary-star system.
Assume that Star 1 has
m₁ = 3.4 solar masses, Star 2 has m₂ = 1.4 solar masses, and the total
separation of the two (R) is 52 AU. (One AU is Earth's average distance from the
Sun.)
(a)What is the distance, d₁, (in AU) from Star 1 to the center of mass?
AU
(b)What is the distance, d2, (in AU) from Star 2 to the center of mass?
AU
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