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  2. Tropical year - Wikipedia

    en.wikipedia.org/wiki/Tropical_year

    When viewed over a one-year period, the mean longitude is very nearly a linear function of Terrestrial Time. To find the length of the tropical year, the mean longitude is differentiated, to give the angular speed of the Sun as a function of Terrestrial Time, and this angular speed is used to compute how long it would take for the Sun to move ...

  3. Sidereal time - Wikipedia

    en.wikipedia.org/wiki/Sidereal_time

    Sidereal time was defined such that the March equinox would transit the meridian of the observatory at 0 hours local sidereal time. [7] Beginning during the 1970s, the radio astronomy methods very-long-baseline interferometry (VLBI) and pulsar timing overtook optical instruments for the most precise astrometry.

  4. Hipparchic cycle - Wikipedia

    en.wikipedia.org/wiki/Hipparchic_cycle

    Indeed, from the values of the tropical year (365.2421896698 days) and the synodic month (29.530588853) cited in the respective articles of Wikipedia, it follows that the length of 228=12×19 tropical years is about 83,275.22 days, shorter than the length of 12×235 synodic months—namely about 83,276.26 days—by one day plus about one hour.

  5. Dynamical time scale - Wikipedia

    en.wikipedia.org/wiki/Dynamical_time_scale

    Using data from Newcomb's Tables of the Sun (based on the theory of the apparent motion of the Sun by Simon Newcomb, 1895, as retrospectively used in the definition of ephemeris time), the SI second was defined in 1960 as: the fraction 1/31,556,925.9747 of the tropical year for 1900 January 0 at 12 hours ephemeris time.

  6. Timekeeping on Mars - Wikipedia

    en.wikipedia.org/wiki/Timekeeping_on_Mars

    (The two Mars Exploration Rovers happen to be approximately 12 hours and one minute apart.) Since the late 1990s and arrival of Mars Global Surveyor at Mars, the most widely used system for specifying locations on Mars has been planetocentric coordinates , which measure longitude 0°–360° East and latitude angles from the center of Mars. [ 11 ]

  7. Solar time - Wikipedia

    en.wikipedia.org/wiki/Solar_time

    On a prograde planet like the Earth, the sidereal day is shorter than the solar day. At time 1, the Sun and a certain distant star are both overhead. At time 2, the planet has rotated 360° and the distant star is overhead again (1→2 = one sidereal day). But it is not until a little later, at time 3, that the Sun is overhead again (1→3 = one solar day). More simply, 1→2 is a complete ...

  8. Florida on long-range alert for upcoming Gulf tropical threat

    www.aol.com/weather/florida-long-range-alert...

    The Gulf of Mexico remains the zone to watch for tropical development and impacts to the United States in the days ahead, and this time Florida may be the prime target for any budding system next ...

  9. Metonic cycle - Wikipedia

    en.wikipedia.org/wiki/Metonic_cycle

    Thus, every 2 to 3 years there is a discrepancy of 22 to 33 days, or a full synodic month. For example, if the winter solstice and the new moon coincide, it takes 19 tropical years for the coincidence to recur. The mathematical logic is this: A tropical year lasts 365.2422 days. [21] a span of 19 tropical years (365.2422 × 19) lasts 6,939.602 days