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Symmetry in a star refers to the uniform distribution of its mass and energy, which contributes to its overall shape and stability. Most stars, including our Sun, exhibit spherical symmetry due to the gravitational forces pulling matter evenly towards the center. This symmetry helps maintain hydrostatic equilibrium, balancing the inward pull of gravity with the outward pressure from nuclear fusion in the core. Deviations from perfect symmetry, such as in pulsating or binary stars, can lead to variations in brightness and structure.

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4mo ago

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A 10-point star has 10 lines of symmetry. Each line of symmetry passes through one point of the star and the midpoint of the opposite side, allowing for mirror symmetry across each line. Additionally, the star can be rotated in increments that align with its points, further supporting the symmetry.


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The order of symmetry for a star depends on its specific type. For example, a regular five-pointed star has rotational symmetry of order 5, meaning it can be rotated by multiples of 72 degrees and still look the same. Similarly, other star shapes may have different orders of symmetry based on their number of points and overall design. In general, the order of symmetry can be determined by the number of identical sections or angles in the star's structure.