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long-period stability - translation to russian
DESCRIPTION FOR CERTAIN COOL LUMINOUS PULSATING VARIABLE STARS
Long-Period Variable Star; Long-period variables; Long period variable; Long period variables; Long-period variable stars; Long period variable star; Long period variable stars; Long-period-variable stars; Long-period-variable star; Long-period-variable; Long-period-variables; LPV star; LPV stars; Long-period variable; OGLE small amplitude red giant
![Light curves of four [[Mira variable]]s in the [[galaxy]] [[Centaurus A]]](https://commons.wikimedia.org/wiki/Special:FilePath/Eso0315i.jpg?width=200 "Light curves of four [[Mira variable]]s in the [[galaxy]] [[Centaurus A]]")
long-period stability
общая лексика
устойчивость в длиннопериодическом
initial stability
RESISTANCE OF A BOAT TO SMALL CHANGES IN THE DIFFERENCE BETWEEN THE VERTICAL FORCES APPLIED ON ITS TWO SIDES
Primary stability
общая лексика
начальная остойчивость
initial stability
RESISTANCE OF A BOAT TO SMALL CHANGES IN THE DIFFERENCE BETWEEN THE VERTICAL FORCES APPLIED ON ITS TWO SIDES
Primary stability
начальная остойчивость
Definition
synodic period
¦ noun Astronomy the time between successive conjunctions of a planet with the sun.
Wikipedia
Long-period variable star
The descriptive term long-period variable star refers to various groups of cool luminous pulsating variable stars. It is frequently abbreviated to LPV.
