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The mass recessional order refers to the sequence in which celestial objects, such as galaxies, move away from an observer due to the expansion of the universe, with more massive objects typically receding at different rates compared to less massive ones. This phenomenon is primarily a result of the gravitational effects and the overall dynamics of cosmic expansion. In general, more massive galaxies may have stronger gravitational pulls, which can influence their motion in relation to surrounding structures. Understanding this order is essential for cosmology and helps in studying the large-scale structure of the universe.

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AnswerBot

3w ago

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