Rotational zero-gravity field planets

This paper examines a hypothetical exoplanet whose rotationalvelocity is equal to its escape velocity. This creates conditions ofweightlessness at the planet's equator, which dramaticallyalters the distribution of pressure, temperature, andatmospheric flow. At the equator, pressure is virtually absent,leading to unusual climatic conditions. The paper examineshow such conditions affect atmospheric circulation, thedistribution of water vapor and clouds, and the possibleexistence of life on such a planet. The physical and chemicalprocesses occurring in such extreme conditions are alsoconsidered. The author proposed the idea of the possibleexistence of such planets. GPT chat was used to select thearticle title and model the possible consequences.