mean solar day oor Portugees
mean solar day
en
the average length of a solar day, used for practical timekeeping
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dia solar médio
dia
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The mean solar second is defined as 1/86,400 of the mean solar day.
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(The days we will use, as Norman Bloom does, are what astronomers call “mean solar days.”)
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To remind you: The duration of the Thalassan Mean Solar Day is 29.4325 hours ET.
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One second of UT is 1/86,400 of a mean solar day.
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A normal 24-hour mean solar day is the period between successive occasions when the Sun is overhead.
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"(The days we will use, as Norman Bloom does, are what astronomers call ""mean solar days."")"
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The second was originally defined as 1/86,400 of the mean solar day.
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The standard of time prior to 1960 was based on the mean solar day.
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Time Before 1967, the standard of time was defined in terms of the average length of a mean solar day.
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Earth's rotation period relative to the Sun—its mean solar day—is 86,400 seconds of mean solar time (86,400.0025 SI seconds).
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The tropical year is equal to 365.2422 mean solar days, whereas the sidereal year is equal to 365.2564 of these days.
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The length of the mean solar day in SI seconds is available from the IERS for the periods 1623–2005 and 1962–2005.
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Earth orbits the Sun at an average distance of about 150 million km (93 million mi) every 365.2564 mean solar days, or one sidereal year.
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There are times when the Hebrews used ‘day and night’ to mean only a portion of a solar day of 24 hours.
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In recent decades, the average length of a solar day on Earth has been about 86 400.002 seconds (24.000 000 6 hours) and there are about 365.2422 solar days in one mean tropical year.
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Earth's rotation period relative to the Sun—its mean solar day—is 86,400 seconds of mean solar time (86,400.0025 SI seconds).
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(a Biblical “time” or year being the mean between a lunar year of 354 days and a solar year of 365 1/4 days)
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Earth orbits the Sun at an average distance of about 150 million kilometers every 365.2564 mean solar days, or one sidereal year.
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This period of rotation is about 4 minutes less than 24 hours (23 hours 56 minutes and 4.1 seconds) and there are about 366.2422 stellar days in one mean tropical year (one stellar day more than the number of solar days).
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Earth orbits the Sun at an average distance of about 150 million kilometres (93,000,000 mi) every 365.2564 mean solar days, or one sidereal year.
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Earth orbits the Sun at an average distance of about 150 million km (93 million mi) every 365.2564 mean solar days, or one sidereal year.
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All values refer to a mean annual solar radiation of 120 W/m2, a shading share of 0,49 and a mean vehicle driving time of 1 hour per day at 750 W electric power requirement.
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Earth's axial tilt (or obliquity) and its relation to the rotation axis and plane of orbit Earth's rotation period relative to the Sun—its mean solar day—is 86,400 seconds of mean solar time (86,400.0025 SI seconds).
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Earth rotation imaged by DSCOVR EPIC on 29 May 2016, a few weeks before the solstice Earth's rotation period relative to the Sun—its mean solar day—is 86,400 seconds of mean solar time (86,400.0025 SI seconds).
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The basic unit of time corresponding to 1/86,400 of the mean solar day, which is the period of rotation about its own axis of an ideal Earth describing a circle round the Sun in one year, at a constant speed and in the plane of the Equator.
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46 sinne gevind in 28 ms. Hulle kom uit baie bronne en word nie nagegaan nie.