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首页> 外文期刊>Journal for the History of Astronomy >Twentieth-Century Longitude: When Greenwich Moved
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Twentieth-Century Longitude: When Greenwich Moved

机译:二十世纪经度:格林威治时

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摘要

By the beginning of the twentieth century, the meridian passing though the Royal Observatory at Greenwich had become a near-universal reference for place and time. It was the zero of longitude. But our current standard of zero longitude is about 100 metres away from the original. That mobility needs historical context: Greenwich began to move in the years after the First World War, when wireless techniques for the astronomical determination of longitude and the standardisation of time were developed, and has carried on moving ever since. In this article, I describe how twentieth-century techniques for the determination of longitude not only brought improved precision but also led to fundamental changes in our long-standing conventions of longitude. And I show how - despite its mobility - our current standard of zero longitude continues to respect the original.
机译:到20世纪初,经过格林威治皇家天文台的子午线已成为几乎普遍的时空参考。它是经度的零。但是我们目前的零经度标准距离原始标准约100米。移动性需要历史背景:第一次世界大战后的几年,格林威治开始发展,当时用于天文确定经度和时间标准化的无线技术得到了发展,并且一直在发展。在本文中,我描述了二十世纪确定经度的技术如何不仅提高了精度,而且还导致了我们长期以来的经度惯例发生了根本性的变化。而且,我将展示尽管其具有灵活性,但我们目前的零经度标准仍将继续遵循原始标准。

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