Glossary term: 萬有引力
Description: 萬有引力是具有質量的物體之間的相互吸引力。在經典力學中，任何具有質量的物體總會對另一個具有質量的物體產生吸引力，這種吸引力就是我們所知的萬有引力。愛因斯坦的廣義相對論將萬有引力重新解釋為一種時空曲率，而不是一種力。然而，萬有引力的經典近似值在大多數情況下仍然是準確的。物體的質量越大，其萬有引力/時空扭曲就越強，因此對其他物體的牽拉作用也就越大。
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Term and definition status: The original definition of this term in English have been approved by a research astronomer and a teacher The translation of this term and its definition is still awaiting approval
This is an automated transliteration of the simplified Chinese translation of this term
The OAE Multilingual Glossary is a project of the IAU Office of Astronomy for Education (OAE) in collaboration with the IAU Office of Astronomy Outreach (OAO). The terms and definitions were chosen, written and reviewed by a collective effort from the OAE, the OAE Centers and Nodes, the OAE National Astronomy Education Coordinators (NAECs) and other volunteers. You can find a full list of credits here. All glossary terms and their definitions are released under a Creative Commons CC BY-4.0 license and should be credited to "IAU OAE".
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