synodic month वाक्य
उदाहरण वाक्य
मोबाइल
- Strictly speaking, the months appearing in a Tibetan almanac, called by us Tibetan calendar months, are not the same as lunar or synodic months ( " tshes zla " ), which can begin and end at any time of day.
- This allows the calculation of 12, 24, 36, 48, 54 and 57 synodic months in the lunar system and of 12, 18, 24, 36, 48, 54 and 57 sun months ( i . e . twelfths of a tropical year ).
- We need to approximate this ratio by common fractions : the numerators and denominators then give the multiples of the two periods draconic and synodic months that ( approximately ) span the same amount of time, representing an eclipse cycle.
- He argued that Naburimannu developed the Babylonian System A of calculating solar system ephemerides, and that later Kidinnu developed the Babylonian System B . A Greco-Roman tradition, mentioned above, attributes to Kidinnu the discovery that 251 synodic months equals 269 anomalistic months.
- The period of the mean synodic month can be approximated as 29 + 26 / 49 days ( a more accurate vulgar fraction is 29 + 451 / 850; the Hebrew calendar uses 29 + 12 hours + 793 / 1080 hours ).
- The Babylonian estimate for the synodic month was adopted for the greater part of two millennia by Hipparchus, Ptolemy and medieval writers ( and it is still in use as part of the basis for the calculated Hebrew ( Jewish ) calendar ).
- As seen from the Earth, the time it takes for the Moon to return to a node, the draconic month, is less than the time it takes for the Moon to return to the same ecliptic longitude as the Sun : the synodic month.
- The Metonic cycle has 19 tropical years and 235 synodic months in 6940 days . The Callippic cycle synchronizes days per orbit and rotations per orbit within the Metonic cycle, noting the difference of one after 4 Metonic cycles, a duration of 76 years.
- Eclipse cycles have a period in which a certain number of synodic months closely equals an integer or half-integer number of draconic months : one such period after an eclipse, a node of the Moon's orbit on the ecliptic, and an eclipse can occur again.
- The Variation has a period of half a synodic month and causes the Moon's ecliptic longitude to vary by nearly two-thirds of a degree, more exactly by + 2370 " sin ( 2D ) where D is the mean elongation of the Moon from the Sun.
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