- (astronomy) main sequence
Generated definitions (experimental)
- 主序带 refers to the main sequence in astronomy.
It signifies a continuous and distinctive band of stars in the Hertzsprung-Russell diagram, where stars spend the majority of their lifespan fusing hydrogen into helium.
Most stars are located in the main sequence.
Stars in the main sequence are typically in the early stages of stellar formation.
Generated collocations (experimental)
zhǔ主xù序dài带xīng星main sequence starzhǔ xù dài主序带yǎn huà演化main sequence evolutionzhǔ xù dài主序带mó xíng模型main sequence modelzhǔ xù dài主序带xíng xīng行星main sequence planetzhǔ xù dài主序带zhōu wéi周围around the main sequencezhǔ xù dài主序带suǒ所zhàn占qū yù区域area occupied by the main sequencezhǔ xù dài主序带héng xīng恒星main sequence starszhǔ主xù序dài带guāng光pǔ谱main sequence spectrumzhǔ xù dài主序带tè zhēng特征characteristics of the main sequencezhǔ主xù序dài带tiān天wén xué文学main sequence astronomy