Glossary term: Cor
Description: A cor de um objeto astronômico pode conter informações importantes sobre suas propriedades físicas. Mesmo a olho nu, uma estrela azulada que você vê no céu, como Alkaid no final da "alça" da Ursa Maior, será consideravelmente mais quente do que uma estrela avermelhada, como Betelgeuse no ombro de Orion. Para quantificar a cor, os astrônomos normalmente determinam o brilho de uma estrela quando vista através de um dos vários filtros azuis especializados possíveis e comparam com o brilho através de um filtro vermelho. Várias definições de cores distintas desse tipo, comparando o brilho em diferentes filtros específicos, estão em uso. Os resultados podem ser usados em análises estatísticas. Um exemplo são os diagramas de cor-magnitude, que representam a cor do objeto em relação ao brilho do objeto.
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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
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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