low mass stars翻译
low mass stars的基本解释
读音: 美: 英:
低质量恒星:指质量较小的恒星,通常质量小于太阳质量的一半。这类恒星的演化过程较慢,寿命较长。
例句
Through almost 30 years observation and study, astronomers come to a relatively clear agreement that low mass stars form by collapse, accretion and outflow.近30多年的观测研究使得天文学家对小质量恒星的形成有了相对明确的认识:小质量恒星通过坍缩、吸积和外向流的路标而形成。Even at this smaller mass, however, many astronomers would still classify it as a low mass star rather than a planet, since the circumstances of birth for stars and planets differ.即使在这样较小的质量下,鉴于恒星和行星诞生的环境的不同,许多天文学家依然会将它划分为小质量恒星而不是行星。
For decades, astronomers have been confident that relatively low-mass stars such as our sun form by the gradual accretion, or buildup, of mass from a disk of gas and dust.几十年来,天文学家已经确信质量相对较小的星体,如我们的太阳,是逐渐积累或建立自碟状气体或尘埃而形成的。
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