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ετυμολογία

short-period variation - translation to ρωσικά

PLANET WITH AN ORBITAL PERIOD LESS THAN ONE EARTH DAY

Ultra-short-period planets; Ultra short period planets; Ultra-short period planets

short-period variation

математика

короткопериодная вариация

variation

WIKIMEDIA DISAMBIGUATION PAGE

Variations; Varied; Varying; Variation (disambiguation); Viccitude; Variations (album); Variation (combinatorics); Variations (Combinatorics); Variation (Combinatorics)

[ve(ə)ri'eiʃ(ə)n]

общая лексика

вариация

изменчивость

изменение

вариационный

варьирование

колебание

колебательность

магнитное склонение

неравномерность

отклонение

разновидность

ход зависимости

нефтегазовая промышленность

отклонение (от номинальной величины)

Смотрите также

age variation; autogenous variation; balanced variation; brusque variation; bud variation; chance variation; continuous variation; cryptic variation; determinate variation; directional variation; discontinuous variation; discrete variation; ecological variation; environmental variation; food variations; genetic variation; geographic variation; group variation; homologous variation; host controlled variation; idiotypic variation; individual variation; interspecific variation; intrapopulation variation; intraspecific variation; local variation; phase variation; phenotypic variation; remaining variation; seasonal variation; sex-associated variation; somatic variation; somatogenic variation; stimulus parameter variation; absolute variation; admissible variation; amount of variation; aperiodic variation; batch variation; batch-to-batch variation; boundary variation; bounded variation; coefficient of variation; combined variation; component of variation; constant of variation; constrained variation; controllable variation; daily variation; day-to-day variation; direct variation; domain of variation; dominated variation; downward variation; explained variation; finite variation; first variation; fractional variation; free variation; generalized variation; gross variation; harmonic variation; higher-order variation; infinitesimal variation; intermittent variation; inverse variation; joint variation; law of variation; limited variation; limits of variation; long-period variation; lower variation; measure variation; mixed variation; n-parameter variation; needle-shaped variation; negative variation; net variation; nonlinear variation; nonperiodic variation; normal variation; one-sided variation; overall variation; pitch variation; plane variation; positive variation; quadratic variation; random variation; region of variation; regular variation; relative variation; saltatory variation; sampling variation; second variation; secular variation; short-period variation; significant variation; smooth variation; source of variation; strong variation; systematic variation; time variation; total variation; transient variation; type of variation; unbounded variation; uncontrolled variation; unexplained variation; unfree variation; upper variation; variation diminishing matrix; variation estimation; variation factor; variation interval; variation kernel; variation limiting matrix; variation measure; variation norm; variation of constants; variation of curve; variation of function; variation of functional; variation of parameters; variation of sign; variation range; weak variation; variations from plumb; variation in the magnitude; variation in the sense; variations in the shape; variation with time; variation of the bending moment along the length of the beam; variation of the project; color variations; diurnal variation; magnetic variation; probable variations in dead load during construction; stress variation; temperature variations; variation of reflection amplitude with angle of incidence; variation of reflection amplitude with offset; variation of reflection coefficient with angle of incidence; amplitude variation with offset; layer thickness variation; near-surface velocity variations; penetration rate variation; reliability variation; rock permeability variations; strength variation; weathering variation; weathering velocity variation; weight-on-bit variation

существительное

общая лексика

изменение

перемена

варьирование

колебание

разновидность

вариант

отклонение

изменение, перемена

склонение магнитной стрелки

специальный термин

вариация

физика

магнитное склонение

грамматика

флексия

биология

аберрация

генетическая изменчивость

мутация

variation

WIKIMEDIA DISAMBIGUATION PAGE

Variations; Varied; Varying; Variation (disambiguation); Viccitude; Variations (album); Variation (combinatorics); Variations (Combinatorics); Variation (Combinatorics)

1) склонение (компаса)

2) ход, изменение

- annual variation

- daily variation

- easterly variation

- magnetic variation

- variation of the compass

- westerly variation

Ορισμός

ШОРТ

(Short) Джеймс (1710-68) , английский астроном и оптик. Создал ок. 1400 зеркальных телескопов высокого качества, изобрел высокоточные маятниковые часы.

Εμφάνιση περισσότερων ορισμών

Βικιπαίδεια

Ultra-short period planet

An ultra-short period (USP) planet is a type of exoplanet with orbital period less than one day. At this short distance, tidal interactions lead to relatively rapid orbital and spin evolution. Therefore when there is a USP planet around a mature main-sequence star it is most likely that the planet has a circular orbit and is tidally locked. There are not many USP planets with sizes exceeding 2 Earth radii. About one out of 200 Sun-like stars (G dwarfs) has an ultra-short-period planet. There is a strong dependence of the occurrence rate on the mass of the host star. The occurrence rate falls from (1.1 ± 0.4)% for M dwarfs to (0.15 ± 0.05)% for F dwarfs. Mostly the USP planets seem consistent with an Earth-like composition of 70% rock and 30% iron, but K2-229b has a higher density suggesting a more massive iron core. WASP-47e and 55 Cnc e have a lower density and are compatible with pure rock, or a rocky-iron body surrounded by a layer of water (or other volatiles).

A difference between hot Jupiters and terrestrial USP planets is the proximity of planetary companions. Hot Jupiters are rarely found with other planets within a factor of 2–3 in orbital period or distance. In contrast, terrestrial USP planets almost always have longer-period planetary companions. The period ratio between adjacent planets tends to be larger if one of them is a USP planet suggesting the USP planet has undergone tidal orbital decay which may still be ongoing. USP planets also tend to have higher mutual inclinations with adjacent planets than for pairs of planets in wider orbits, suggesting that USP planets have experienced inclination excitation in addition to orbital decay.

There are several known giant planets with a period shorter than one day. Their occurrence must be lower by at least an order of magnitude than that of terrestrial USP planets.

It had been proposed that USP planets were the rocky cores of evaporated hot Jupiters, however the metallicity of the host stars of USP planets is lower than that of hot Jupiters' stars so it seems more likely that USP planets are the cores of evaporated gas dwarfs.

https://en.wikipedia.org/wiki/Ultra-short period planet

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