```text Perspective: The Pivotal Role of Rotation in Shaping Celestial Bodies ```

**Title**: Perspective: The Pivotal Role of Rotation in Shaping Celestial Bodies **Description**:This Perspective article explores the critical role of self-rotation in shaping the morphologies of planets, dwarf planets, and large moons, challenging the traditional view that gravitational hydrostatic equilibrium alone drives their spheroidal forms. By analyzing rapidly rotating bodies like Haumea (3.9-hour period, triaxial ellipsoid) against slowly rotating ones like Pluto (6.4-day period, near-spherical), we demonstrate how rotation induces viscous or plastic flow to redistribute mass in celestial bodies exceeding ~10^22 kg. The proposed framework integrates recent planetary science insights, addresses observational and computational challenges, and accounts for confounding factors such as tidal interactions and material composition. We propose testable predictions leveraging upcoming surveys like the Legacy Survey of Space and Time (LSST) and discuss implications for exoplanet morphology and habitability studies. This work offers a novel lens on planetary diversity, with applications to future missions like JWST, ARIEL, and Juno. **Keywords**: Planetary Morphology, Self-Rotation, Hydrostatic Equilibrium, Centrifugal Effects, Planetary Dynamics **License**: CC-BY 4.0 **Files Included**:- main.tex: LaTeX source file of the manuscript- references.bib: BibTeX file with cited references- main.pdf: Compiled PDF of the manuscript- README.txt: Compilation instructions **Compilation Instructions**:1. Run `pdflatex main.tex`2. Run `bibtex main`3. Run `pdflatex main.tex` twiceRequires: pdflatex, bibtex **Author**: Your Full Name, Your Affiliation (e.g., Department of Astronomy, University of XYZ, City, Country), ORCID: 0000-1234-5678-9012 **DOI**: (To be assigned upon publication, e.g., 10.5281/zenodo.16888691) **Community**: Planetary Science **Funding**: (If applicable, add funding details here, e.g., "This work was supported by [Funding Agency, Grant Number].")标题：专题评述：自转在天体形态塑造中的核心作用 描述：本评述性文章探讨了自转在行星、矮行星及大型卫星形态塑造中的关键作用，对仅靠引力流体静力学平衡造就其类球形态的传统观点提出了挑战。通过对比分析快速自转天体（如自转周期3.9小时、呈三轴椭球体形态的妊神星（Haumea））与慢速自转天体（如自转周期6.4天、近似球形的冥王星（Pluto）），本文阐明了在质量约10^22千克以上的天体中，自转如何通过黏滞或塑性流动实现物质再分布。本文提出的研究框架整合了近期行星科学领域的前沿认知，回应了观测与计算层面的挑战，并纳入了潮汐相互作用、物质组成等干扰因素的影响。我们依托时空遗产巡天（Legacy Survey of Space and Time, LSST）等即将开展的巡天项目提出了可验证的预测，并探讨了该研究对系外行星形态与宜居性研究的启示。本研究为行星多样性研究提供了全新视角，其成果可应用于詹姆斯·韦布空间望远镜（James Webb Space Telescope, JWST）、系外行星大气红外遥感大巡天卫星（Atmospheric Remote-Sensing Infrared Exoplanet Large-survey, ARIEL）以及朱诺号探测器（Juno）等未来航天任务。 关键词：行星形态学（Planetary Morphology）、自转（Self-Rotation）、流体静力学平衡（Hydrostatic Equilibrium）、离心效应（Centrifugal Effects）、行星动力学（Planetary Dynamics） 授权协议：CC-BY 4.0 包含文件： - main.tex：稿件的LaTeX源文件 - references.bib：参考文献BibTeX文件 - main.pdf：编译完成的稿件PDF文件 - README.txt：编译说明文件 编译说明： 1. 运行`pdflatex main.tex` 2. 运行`bibtex main` 3. 运行`pdflatex main.tex`两次 所需环境：pdflatex、bibtex 作者：您的全名，您的所属机构（例如：XYZ大学天文系，城市，国家），ORCID：0000-1234-5678-9012 DOI：（出版后分配，例如：10.5281/zenodo.16888691） 所属领域：行星科学 资助信息：（如有，请添加资助详情，例如："本研究得到[资助机构，项目编号]资助。"）