The Sun is right where it always is; in the center of the Solar System, with the
planets orbiting around it.
From our perspective standing here on the spinning Earth, the Sun APPEARS TO
rise in the East and set in the West, and to move slowly north between December 21
and June 21, and then to move slowly south from June 21 to December 21. But
just
remember that this is a sort of optical illusion; it's the Earth's movements that make
it seem so.
At the northern hemisphere summer solstice, around June 21, the Sun appears to
pass DIRECTLY overhead for locations along the Tropic of Cancer, at 23 degrees 26 minutes
North Latitude (because the Earth "wobbles" a bit, this value changes very slightly
each year), and then slowly spirals south. On the fall Equinox, the Sun passes
directly overhead along the equator, on September 21. (These dates will fluctuate
a day either way depending on the cycle of leap years.) The Sun "moves" south,
reaching its southernmost location over the Tropic of Capricorn (23 degrees, 26 minutes
south) on December 21, the northern hemisphere winter solstice.
After that, the Sun appears to slowly move north, passing over the equator on the
spring equinox, and passing over the Tropic of Cancer again on June 21.
In terms of the sun's celestial (astronomical) coordinates on the map of the stars:
-- March equinox . . . . . Right Ascension 0hours, Declination 0°
-- June solstice . . . . . . Right Ascension 6hours, Declination +23.4394°
-- September equinox . . Right Ascension 12hours, Declination 0°
-- December solstice. . . Right Ascension 18hours, Declination -23.4394°
The solstices occur at the points where the Earth is either closest to, or farthest away from, the Sun. The equinoxes are the mid-points between the solstices - where the day & night are of equal length.
At the equinox day and night are of the same length all over the world because the Sun is in the plane of the Earth's equator, and that happens on March 21 and September 22 each year.
The solstices are determined by the distance the Earth is from the sun in its orbit. Winter is when the sun is farthest away relative to the Earth's tilt. Summer occurs when the opposite is true.
equinoxes
The equinoxes (approximately 21 March & 21 Sept).
The Earth's tilt results in the solstices and euinoxes, depending on where the Earth is in it's orbit around the sun.
Equinoxes are the two points among the stars where the sun's apparent annual path crosses the celestial equator. Solstices are the two points among the stars where the sun's apparent annual path reaches its extremes, north and south of the celestial equator.
Solstices and Equinoxes are points in the orbit of the Earth around the sun, hence directly related to seasons
north and south
These happen because the axis of Earths spin in inclined at an angle from the normal of to the plane in which it orbits the Sun.
These happen because the axis of Earths spin in inclined at an angle from the normal of to the plane in which it orbits the Sun.
Twice; both during the sun's summer and winter solstices.
Solstices and Equinoxes are points in the orbit of the Earth around the sun, hence directly related to seasons
The solstices occur at the points where the Earth is either closest to, or farthest away from, the Sun. The equinoxes are the mid-points between the solstices - where the day & night are of equal length.
A solar calendar follow the phases of the sun which gives us equinoxes and solstices whereas a lunar calendar follows the phases of the moon and it's cycles.
Measure the angle from the true horizon to the midday Sun on the dates of the vernal and atumnal equinoxes and on the dates of the solstices. The angle between the the solstice noon Sun and an equinox midday Sun will be 23,5 degrees.
There is no latitude on earth at which the sun would be directly overhead at noon on the equinox and the solstice.