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In a double star system, the masses of the stars are m, and m₂. They are separated by distance d. The two bodies rotate about their common centre of mass. The ratio of the area swept by the first and second star in equal time interval about their common centre of mass is:

In a double star system, the masses of the stars are m, and m₂. They are separated by distance d. The two bodies rotate about their common centre of mass. The ratio of the area swept by the first and second star in equal time interval about their common centre of mass is:

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In a double star system, the masses of the stars are m, and m₂. They are separated by distance d. The two bodies rotate about Q. their common centre of mass. The ratio of the area swept by the first and second star in equal time interval about their common centre of mass is: m₁ m₂ m₂ m₁ mí 2 m 2
Transcribed Image Text:In a double star system, the masses of the stars are m, and m₂. They are separated by distance d. The two bodies rotate about Q. their common centre of mass. The ratio of the area swept by the first and second star in equal time interval about their common centre of mass is: m₁ m₂ m₂ m₁ mí 2 m 2
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