evection वाक्य
उदाहरण वाक्य
मोबाइल
- The effect can be explained by so-called " evection resonance ".
- Ptolemy described lunar motion by using a well-defined geometric model of epicycles and evection.
- During the live show Miguel was chosen by Secret Story ( A Voz / La Voix ) to choose between Fanny and Daniela S . to go up for evection.
- The evection can be considered as opposing the Moon's equation of the center at the new and full moons, and augmenting the equation of the center at the Moon's quarters.
- In astronomy, "'evection "'( Latin for " carrying away " ) is the largest Bullialdus in connection with his own ( unsuccessful ) theory of the Moon's motion .)
- :In week seven only female housemates could nominate . During the live show Fanny was chosen as the leader of the women and had to choose between Jo�o M . and Marco to go up for evection.
- Their combination also continually changes its shape as the annual argument changes, and also as the evection shows itself in libratory changes in the eccentricity, and in the direction, of the long axis of the eccentric ellipse.
- This can be seen from the combination of the principal term of the equation of the center with the evection : + 22639.55 " \ sin ( l ) + 4586.45 " \ sin ( 2D-l ).
- Pedro and Marco were nominated by Secret Story ( A Voz / La Voix ) for disrespecting the rules . During the live show Daniela S . was chosen as the leader of the women and had to choose between Jo�o J . and Paulo to go up for evection.
- At the quarters, D = 90?or 270? 2D is effectively 180?in either case, changing the sign of the expression for the evection, so that the combined expression then reduces to + ( 22639.55 + 4586.45 ) " \ sin ( l ).
- This figure is much smaller than evection : the difference is accounted for by the fact that the ancient measurements were taken at times of eclipses, and the effect of the evection ( which subtracts under those conditions from the equation of the center ) was at that time unknown and overlooked . " For further information see also separate article Evection ."
- This figure is much smaller than evection : the difference is accounted for by the fact that the ancient measurements were taken at times of eclipses, and the effect of the evection ( which subtracts under those conditions from the equation of the center ) was at that time unknown and overlooked . " For further information see also separate article Evection ."
- This figure is much smaller than evection : the difference is accounted for by the fact that the ancient measurements were taken at times of eclipses, and the effect of the evection ( which subtracts under those conditions from the equation of the center ) was at that time unknown and overlooked . " For further information see also separate article Evection ."
- The Variation is the second-largest solar perturbation of the Moon's orbit after the Evection, and the third-largest inequality in the motion of the Moon altogether; ( the first and largest of the lunar inequalities is the equation of the centre, a result of the eccentricity & ndash; which is not an effect of solar perturbation ).
- The main visible effect ( in longitude ) of the variation of the Moon is that during the course of every month, at the octants of the Moon's phase that follow the syzygies ( i . e . halfway between the new or the full moon and the next-following quarter ), the Moon is about two thirds of a degree farther ahead than would be expected on the basis of its mean motion ( as modified by the equation of the centre and by the evection ).
- Evection causes the Moon's ecliptic longitude to vary by approximately & plusmn; 1.274?( degrees ), with a period of about 31.8 days . The evection in longitude is given by the expression + 4586.45 " \ sin ( 2D-l ), where D is the ( mean ) elongation, i . e . mean angular distance of the Moon from the Sun, and l is the moon's mean anomaly, i . e . mean angular distance of the moon from its perigee.
- Evection causes the Moon's ecliptic longitude to vary by approximately & plusmn; 1.274?( degrees ), with a period of about 31.8 days . The evection in longitude is given by the expression + 4586.45 " \ sin ( 2D-l ), where D is the ( mean ) elongation, i . e . mean angular distance of the Moon from the Sun, and l is the moon's mean anomaly, i . e . mean angular distance of the moon from its perigee.
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