Understanding Sunsets and Sunrises on the Equinox: A Comprehensive Guide
The earth rotates at approximately 1000 miles per hour, and while the sun doesn't move due to the stationary nature of the celestial body, the tilt of the Earth's axis results in fascinating variations in the timing of sunrises and sunsets. This article explores these phenomena as they occur on the equinoxes, along with the effects of atmospheric refraction and geographical longitude and latitude.
Equinox Definition
The equinox occurs around March 21st and September 23rd, when the Earth's equator passes directly beneath the Sun. At these times, both the Northern and Southern Hemispheres receive roughly equal amounts of sunlight, leading to nearly equal day and night lengths across most of the planet.
Sunrise and Sunset Timing
During the equinoxes, the sun rises due east and sets due west for most locations. However, the exact time of sunrise and sunset can vary based on your geographic location, specifically your latitude and longitude. This is due to the axial tilt of the Earth and atmospheric effects, which will be discussed in detail below.
Atmospheric Refraction
The Earth's atmosphere bends or refracts light, causing the sun to appear to rise earlier and set later than it would in a vacuum. This effect can result in slight variations in the perceived times of sunrise and sunset. For instance, this is why the sun may appear to rise before the exact time calculated.
Longitude Effects
Due to the rotation of the Earth, local times vary with longitude. Even though the sun sets at the same moment globally in terms of celestial mechanics, the clock time of sunset will differ depending on your location. This is why your local time on an equinox might not exactly match the time at which the sun sets in another part of the world.
Latitude Effects
Locations at different latitudes may also experience different lengths of twilight, the period between sunrise and sunset when the sky is still lit by the sun's light. This extended twilight can affect how long you perceive the sun to be visible after it has technically set.
Global Variations on the Equinox
While the sun rises and sets at nearly the same time across the globe on the equinoxes, local variations due to atmospheric effects, longitude, and latitude can lead to differences in the exact timing experienced by observers. This means that while the celestial mechanics of the sun’s position provide a uniform standard, the practical experience on the ground can differ.
Key Takeaways
The equinox occurs twice a year around March 21 and September 23, when the Earth’s equator passes directly under the sun. At the equinox, the sun rises due east and sets due west for most locations, but local variations can affect the exact times. Atmospheric refraction and longitude and latitude can cause slight delays or precisions in the perceived times of sunrise and sunset.In conclusion, while the Earth rotates and the sun doesn’t move relative to its position in space, the tilt of the Earth and its atmospheric effects result in interesting local variations in the timing of sunrises and sunsets during the equinoxes.