We usually speak of the sun setting in the west, but technically it only sets due west at the spring and autumn equinoxes. For the rest of the year, the direction of sunset pivots about this westerly point, moving northerly in winter, and towards the south in summer.
The Sun's path changes with its declination during the year. The intersections of the curves with the horizontal axis show azimuths in degrees from North where the Sun rises and sets. The Sun appears to move northward during the northern spring, crossing the celestial equator on the March equinox.
The position of the Sun in the sky is a function of both the time and the geographic location of observation on Earth 's surface. As Earth orbits the Sun over the course of a year, the Sun appears to move with respect to the fixed stars on the celestial sphere, along a circular path called the ecliptic .
This marks the path of the Sun during summer solstice and the place where this circle cuts the horizons will mark the place where the Sun will rise and set on the day of summer solstice. A similar circle which is separated from the first circle by 23.5 degrees at zenith towards south will mark the path of the Sun on winter solstice.
As Earth orbits the Sun over the course of a year, the Sun appears to move with respect to the fixed stars on the celestial sphere, along a circular path called the ecliptic.
The ecliptic is the apparent path of the Sun throughout the course of a year. Because Earth takes one year to orbit the Sun, the apparent position of the Sun takes one year to make a complete circuit of the ecliptic. With slightly more than 365 days in one year, the Sun moves a little less than 1° eastward every day.
Because the position of the sun in relationship to the Celestial Equator changes over the year, so does its declination and rising and setting point on the horizon. At spring and fall equinox the sun has a declination of 0 and rises due East and sets due West.
How and why do the sun's celestial coordinates change over the course of each year? Because it is from how we perceive it from the Earth. Since the Earth revolves around the Sun it's position appears to change. This would not happen if the Earth did not have a tilt in its axis.
After the March equinox, the sun's path gradually drifts northward. By the June solstice (usually June 21), the sun rises considerably north of due east and sets considerably north of due west. For mid-northern observers, the noon sun is still toward the south, but much higher in the sky than at the equinoxes.
Earth rotates on a tilted axis and orbits the Sun in a slightly oval-shaped, or elliptical, path. These two motions affect the Sun's changing position in the sky and the times of daily sunrises and sunsets over a year.
The Earth's axis of rotation tilts about 23.5 degrees, relative to the plane of Earth's orbit around the Sun. As the Earth orbits the Sun, this creates the 47° declination difference between the solstice sun paths, as well as the hemisphere-specific difference between summer and winter.
the combination of Earth's rotation and Earth's orbital motion. How does the position of the Sun on the celestial sphere change over the course of a year? Its celestial coordinates remain fixed. Its right ascension remains constant and its declination changes.
The first major contributor to the Sun's apparent motion is the fact that Earth orbits the Sun while tilted on its axis. The Earth's axial tilt of approximately 23.5° ensures that observers at different locations will see the Sun reach higher-or-lower positions above the horizon throughout the year.
On the celestial sphere, lines of right ascension and declination are similar to longitude and latitude lines on Earth. When a telescope's right-ascension axis is lined up with the Earth's axis, as shown here, the telescope can turn on it to follow the rotating sky.
Earth's tilted axis causes the seasons. Throughout the year, different parts of Earth receive the Sun's most direct rays. So, when the North Pole tilts toward the Sun, it's summer in the Northern Hemisphere. And when the South Pole tilts toward the Sun, it's winter in the Northern Hemisphere.
The Sun appears higher in the sky during the northern hemisphere summer, moving lower as we move into winter. The larger loop shows how the Sun's position changes rapidly between measurements. At that time of year the Earth is closer to the Sun and therefore travels faster around it.
This non-circularity of the orbit and the tilt of the Earth's axis of rotation both contribute to the uneven changes in the times of sunrise and sunset. For example, as you noticed, the Sun rises only a little earlier each day in January, but sets noticeably later each day.
The sun appears to rise on the eastern horizon and sets on the western horizon. How much does the location of the sun rising and setting change throughout the year and depending upon where your viewpoint is, i.e., true East, true West, etc. Irrespective of where you are on the globe, the Sun will always rise exactly East ...
Thus, the Sun will rise north of true East and set north of true West during summer whereas during winter, the Sun will rise south of true East and set south of true West. The exact location where the Sun will rise and set will vary widely depending on the place.
This circle marks the path of the Sun from dawn to dusk on the two equinoxes. Now, draw a circle which is exactly parallel to the first circle, but which are separated from the first circle by 23.5 degrees at the zenith towards Polaris.
Irrespective of where you are on the globe, the Sun will always rise exactly East and set exactly West on two days: March 21 and September 21 which are the two equinoxes. As to the second part, it is a little complicated:
Jagadheep built a new receiver for the Arecibo radio telescope that works between 6 and 8 GHz. He studies 6.7 GHz methanol masers in our Galaxy. These masers occur at sites where massive stars are being born. He got his Ph.D from Cornell in January 2007 and was a postdoctoral fellow at the Max Planck Insitute for Radio Astronomy in Germany. After that, he worked at the Institute for Astronomy at the University of Hawaii as the Submillimeter Postdoctoral Fellow. Jagadheep is currently at the Indian Institute of Space Scence and Technology.
This circle marks the path of the Sun from dawn to dusk on the two equinoxes. Now, draw a circle which is exactly parallel to the first circle, but which are separated from the first circle by 23.5 degrees at the zenith towards Polaris.
Jagadheep built a new receiver for the Arecibo radio telescope that works between 6 and 8 GHz. He studies 6.7 GHz methanol masers in our Galaxy. These masers occur at sites where massive stars are being born. He got his Ph.D from Cornell in January 2007 and was a postdoctoral fellow at the Max Planck Insitute for Radio Astronomy in Germany. After that, he worked at the Institute for Astronomy at the University of Hawaii as the Submillimeter Postdoctoral Fellow. Jagadheep is currently at the Indian Institute of Space Scence and Technology.
The first plane is that of the “celestial equator”, which is parallel to the plane of the Earth’s equator. This is the plane in which the sun appears to make its daily journey about Earth, from sunrise to sunset and on through the night until sunrise again. Today, following pioneers such as Nicolas Copernicus, we can imagine this more easily, ...
The equinoxes and the directions of sunset show why. The equinoxes occur when the sun sets due west, and the days and nights are (virtually) of equal length everywhere on Earth. At the equator, however, the days and nights are always 12 hours ...
The circle’s age is unknown, but it could be as old as 11,000 years, and researchers – including former Monash academic Duane Hamacher – think it's likely that the circle includes deliberate markers of the direction of sunset at the solstices and equinoxes. We’ll never know just why, or even if, the builders of Wurdi Youang, Stonehenge, ...
Among many other things Ptolemy was interested in was the fact that the symmetry in the arc of sunset directions is reflected in the symmetry between the sun’s midday altitude at the summer and winter solstices. The sunset direction reaches its northerly and southerly extremes at the solstices, while the noon altitudes are also at their extremes ...
At the equinoxes – when the direction of the sunset is halfway between the most northerly and southerly sunset points – the sun is at the point of intersection of the ecliptic and the celestial equator, as I mentioned. So the angle between these two intersecting planes must be half the difference between the summer and winter solstice solar ...
The sunset direction reaches its northerly and southerly extremes at the solstices, while the noon altitudes are also at their extremes (highest and lowest) at the solstices. The midpoints in both cases occur at the equinoxes.
So, in its yearly journey along the ecliptic, there are only two days when the sun crosses the equator.
The Celestial Sphere explanation at Galactic Sky Charts; Celestial Sphere showing relationship between longitude, latitude, and right ascension and declination; The celestial sphere is an imaginary sphere that we use to help visualize the motion of celestial bodies in the entire sky.
If we extend the North and South poles of the Earth outward until they intersected the sphere, the intersection points are defined as the North Celestial Pole and the South Celestial Pole. These always point back to the North and South poles on the Earth.
Thus if you were standing at the North Pole and looked straight up, you would be looking at the North Celestial Pole in the sky. If you were at the South Pole, you would see the South Celestial Pole directly overhead.
(2) Point with your left arm to Polaris. Make a right angle to your left arm with your right arm. Your right arm is now pointing to somewhere on the celestial equator.
Remember that the Sun appears to be in different constellations of the zodiac at different times of the year because the Earth is orbiting the Sun. In Figure 1.10 of the celestial sphere, this would correspond to the Sun moving along the ecliptic, making a complete circuit once a year.
The star Polaris is located very close to the North Celestial Pole. As a result, as the Earth rotates about its axis in its diurnal cycle, all the stars appear to rotate about us in the sky except for Polaris which stays fixed in its position near the North Celestial Pole.
That is, the APPARENT motion of the stars is moving east to west. The ACTUAL motion is that the Earth is spinning on its axis. The stars are fixed (at least on the time scale of the Earth's 24 hour daily spin). For the next couple of sessions we will be concerned about the APPARENT motion of the Sun, stars and Moon to an observer standing on Earth.