How do stars orbit the core in an elliptical galaxy structure?
Answer
In somewhat random, three-dimensional paths
A key structural distinction between elliptical galaxies and spiral galaxies lies in the orbital dynamics of their stellar components. Unlike the organized, flat disk and defined spiral arms where stars orbit in relatively coherent, planar paths around the center, the stars within an elliptical galaxy move in complex, non-uniform trajectories. These orbits are generally described as random and three-dimensional, radiating outward from the core in various directions. This randomized motion, rather than a collective rotation, is what contributes significantly to the smooth, structureless appearance that characterizes these ellipsoidal systems.
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