(Astronomy)a star showing a sudden large increase in brightness and then slowly returning to its original state over a few months (天文)新星。 参见 supernova
Novae are believed to occur in binary star systems. Material falling from a companion star to the surface of a white dwarf collects over a long period, increasing in density and temperature, until there is a sudden runaway thermonuclear reaction which blasts much of the accumulated material into space. Novae are often visible in small telescopes, and sometimes to the naked eye
语源
late 19th cent.: from Latin, feminine of novus 'new' (because such stars were thought to be newly formed)