In the days that follow, the direct rays of the sun migrate to the north of the equator and the length of daylight in the Northern Hemisphere will correspondingly appear to increase. At that moment, the sun will appear directly overhead about 50 miles (80 kilometers) south of Gorontalo, a province of Indonesia - often referred to as the "Emerald of the Equator" - on the island of Sulawesi, on the equator in the Gulf of Tomini. This year it will occur on Thursday (March 19) at 11:49:28 p.m. Sun overhead from the Emerald of the EquatorĪstronomers can calculate the moment of the vernal equinox right down to the nearest second. At the latitude of New York, for instance, day and night are roughly equal a few days before the equinox, on St. This can also result in continuous daylight in far northern countries such as Iceland and Norway.The supposed equality of day and night gives us the Latin name "equinox," which means "equal night." But in reality, thanks to our atmosphere, the day is longer than the night at the equinox. During the summer solstice, the Northern Hemisphere of Earth is tilted towards the Sun, resulting in increased sunlight and warmer temperatures. This situation is reversed at the winter solstice.Īt the summer solstice, the Sun reaches its highest point of the year, while at the winter solstice, the noon Sun is the lowest it will be all year. When it is the summer solstice in the Northern Hemisphere, the areas north of the Arctic circle receive sunlight for a full 24 hours, while areas south of the Antarctic circle have a full day of total darkness. The summer solstice, which occurs around the 21 June in the Northern Hemisphere, is the day of the year with the longest period of daylight while the winter solstice, on or around the 21 December in the Northern Hemisphere, is the day with the shortest period of daylight. These occur twice a year and are referred to as the 'summer solstice' and 'winter solstice'. The equilux is when day and night are equal and occurs a few days before the spring equinox, and a few days after the autumn equinox. The Sun, therefore, appears to rise before its centre at the horizon, giving more daylight than you might expect (12 hours 10 minutes on the equinox). As well as this sunlight is refracted by the Earth's atmosphere. This is because the Sun appears as a disk in the sky, and the top half rises above the horizon before the centre. On the equinox, the length of day and night are only nearly equal. Similarly, the autumn equinox marks the start of autumn as the night becomes longer than the day. The spring equinox marks the beginning of spring and from this day forward the day is longer than the night. During the equinox, day and night will be around the same length which is evident in the word's origin derived from the Latin equi (meaning 'equal') and nox (meaning 'night'). They occur between the summer and winter solstices marking the point the Sun crosses the equator's path and becomes positioned exactly above the equator between the Northern and Southern Hemisphere. The Equinox in the Northern Hemisphere occurs twice a year around 20 March (the spring equinox) and around 22 September (the autumn equinox). The equinox and solstice define the transitions between the seasons of the astronomical calendar and are a key part of the Earth's orbit around the Sun.
0 Comments
Leave a Reply. |
AuthorWrite something about yourself. No need to be fancy, just an overview. ArchivesCategories |