论文标题
行星结构和科幻小说的动态。星际的科学分析与审查[UCM学士学位论文，2015年]
Planetary Structure & Dynamic in Science Fiction. Scientific Analysis & Review of Interstellar [UCM Bachelor Thesis, 2015]
论文作者
论文摘要
克里斯托弗·诺兰（Christopher Nolan）的最新大片《星际》（Interstellar）不仅从摄影上的角度来看，而且在当前观众与科学之间的关系中都认为革命。该报告的目的是分析星际中提出的某些功能。基本的牛顿物理学表明，绕行超级质量黑洞（如Gargantua）的行星如何以0.25的光速行驶，以便在稳定的轨道上行驶。因此，该轨道离黑洞太远，无法解释在米勒的行星中观察到的时间扩张，而可以解释这种时间扩张的轨道要比Roche的极限要小得多。此外，我解释了通过研究Gargantua产生的潮汐电势，获得200公里高的潮汐势可以出现巨大的波浪，但通过考虑米勒星球中的一系列海啸来获得更好的结果。最后，我对曼星冰覆盖的景观介绍了一个解释，其中雪球理论起着基本作用。为了使研究的理解更加容易，不会使用困难的一般相对性公式。 主管：M。L. Osete和J. Gorgas
Christopher Nolan's latest blockbuster, Interstellar, has supposed a revolution not only from a cinematographically viewpoint, but also in the relation between current spectators and science. The aim of this report is to analyze some features presented in Interstellar. Basic Newtonian Physics shows how a planet orbiting a supermassive black hole like Gargantua must travel at 0.25 the speed of light in order to be in a stable orbit. Thus, this orbit is too far from the black hole to explain the time dilatation observed in Miller's Planet and an the orbit that could explain such a time dilatation is much more smaller that Roche's limit. Furthermore, I explain how enormous waves as Miller's Planet ones could appear by studying the tidal potential created by Gargantua, obtaining a wave of 200 kilometers high, but better results are obtained by considering a series of tsunamis in Miller's Planet. Finally, I present an explanation to Mann's Planet ice-covered landscape in which Snowball Earth Theory plays a fundamental role. No difficult General Relativity formulas will be used in order to make easier the comprehension of the research. Supervisors: M. L. Osete & J. Gorgas
