rotation period oor Noorse Bokmål
rotation period
en
rotational period
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rotasjonsperiode
en
(of a celestial object) time that it takes to complete one revolution around its axis of rotation relative to the background stars
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Ground-based observations of coma brightness suggested that Halley's rotation period was about 7.4 days.
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He was also able to estimate the rotation period of the planet.
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He surmised the planet must have a much longer rotation period than had previously been thought.
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"Rotation Period and Day Length".
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Pluto's rotation period, its day, is equal to 6.39 Earth days.
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Ida's rotation period is 4.63 hours, making it one of the fastest rotating asteroids yet discovered.
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Its orbital period is around 4.1 Earth days, coincident with its rotational period.
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Its sidereal rotation period (day) is roughly 16.11 hours.
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The rotational period of the interior of Uranus is 17 hours, 14 minutes.
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Its orbital period is 4.84 years, and its rotation period is 4.63 hours.
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By contrast, the reverse is true for the polar regions where the rotation period is 12 hours.
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The planet Venus rotates once every 224.7 days – by far the slowest rotation period of any of the major planets.
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Friedrich Bessel used Schröter's drawings to erroneously estimate the rotation period as 24 hours and an axial tilt of 70°.
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During their observations, they established that most of Mars' surface features were permanent, and more precisely determined the planet's rotation period.
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If the rotation period were substantially longer, the side of the earth facing the sun would bake while the other froze.
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They began by establishing that most of Mars's surface features were permanent and by more precisely determining the planet's rotation period.
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It is spinning extremely rapidly, with a rotation period of only 15.9 hours, which causes it to have a highly oblate shape.
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Viewed from Earth as it orbits the Sun, the apparent rotational period of the Sun at its equator is about 28 days.
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In 1989, speckle interferometry was used to measure a dimension that varied between 498 and 7005548000000000000♠548 km during the rotational period.
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The rotational period and seasonal cycles of Mars are likewise similar to those of Earth, as is the tilt that produces the seasons.
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This also means that the rotation period of each is equal to the time it takes the entire system to rotate around its barycenter.
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In a frame of reference defined by the stars, the rotational period is approximately 25.6 days at the equator and 33.5 days at the poles.
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Many of them, such as Pan and Daphnis, orbit within Saturn's ring system and have orbital periods only slightly longer than the planet's rotation period.
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Radar observations of Venus were first carried out in the 1960s, and provided the first measurements of the rotation period, which were close to the modern value.
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While approaching Saturn in 2004, Cassini found that the radio rotation period of Saturn had increased appreciably, to approximately 10 hr 45 min 45 sec (± 36 sec).
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126 sinne gevind in 19 ms. Hulle kom uit baie bronne en word nie nagegaan nie.