Everything about Season totally explained
A
season is one of the major divisions of the
year, generally based on yearly periodic changes in
weather.
Seasons happen due to the yearly revolution of the Earth around the Sun and the tilt of the Earth's axis relative to the plane of revolution. In Temperate and Polar regions, the seasons are marked by changes in the amount of sunlight which may cause animals to go into hibernation or to migrate, and plants to be dormant.
In
temperate and
polar regions generally four seasons are recognized:
spring,
summer,
autumn,
winter.
In some
tropical and
subtropical regions it's more common to speak of the
rainy (or wet, or
monsoon) season versus the
dry season, because the amount of
precipitation may vary more dramatically than the average temperature.
In other tropical areas a three-way division into hot, rainy and cool season is used.
In some parts of the world, special "seasons" are loosely defined based upon important events such as a
hurricane season,
tornado season or a
wildfire season.
Causes and effects
The seasons result from the
Earth's
axis being
tilted to its
orbital plane; it deviates by an angle of approximately 23.5
degrees. Thus, at any given time during summer or winter, one part of the planet is more directly exposed to the rays of the
Sun (see
Fig. 1). This exposure alternates as the Earth revolves in its orbit. At any given time, regardless of season, the
northern and
southern hemispheres experience opposite seasons.
It is easy to observe the effect of the axis tilt from the change in
day length, and
altitude of the Sun at
noon (the
culmination of the Sun), during a
year.
Seasonal weather differences between hemispheres are further caused by the
elliptical orbit of Earth. Earth reaches
perihelion (the point in its orbit closest to the
Sun) in January, and it reaches
aphelion (farthest point from the Sun) in July.
Even though the effect this has on Earth's seasons is minor, it does noticeably soften the northern hemisphere's winters and summers. In the southern hemisphere, the opposite effect is observed.
Seasonal weather fluctuations (changes) also depend on factors such as proximity to
oceans or other large bodies of water,
currents in those oceans,
El Niño/ENSO and other oceanic cycles, and prevailing
winds.
In the temperate and polar regions, seasons are marked by changes in the amount of
sunlight, which in turn often causes
cycles of dormancy in plants and
hibernation in animals. These effects vary with latitude and with proximity to bodies of water. For example, the
South Pole is in the middle of the continent of
Antarctica and therefore a considerable distance from the moderating influence of the southern oceans. The
North Pole is in the
Arctic Ocean, and thus its temperature extremes are buffered by the water. The result is that the South Pole is consistently colder during the southern winter than the North Pole during the northern winter.
The cycle of seasons in the polar and temperate zones of one hemisphere is opposite to that in the other. When it's summer in the
Northern hemisphere, it's winter in the
Southern hemisphere, and vice versa.
In the
tropics, there's no noticeable change in the amount of sunlight. However, many regions (such as the northern
Indian ocean) are subject to
monsoon rain and wind cycles.
A study of temperature records over the past 300 years shows that the climatic seasons, and thus the
seasonal year, are governed by the
anomalistic year rather than the
tropical year.
In meteorological terms, the summer
solstice and winter solstice (or the maximum and minimum
insolation, respectively) don't fall in the middles of summer and winter. The heights of these seasons occur up to a month later because of
seasonal lag. Seasons, though, are not always defined in meteorological terms.
Compared to axial tilt, other factors contribute little to seasonal temperature changes. The seasons are not the result of the variation in
Earth’s distance to the sun because of its
elliptical orbit.
Orbital eccentricity can influence temperatures, but on Earth, this effect is small and is more than counteracted by other factors; research shows that the Earth as a whole is actually slightly warmer when
farther from the sun.
Mars however experiences wide temperature variations and
violent dust storms
every year at perihelion.
Polar day and night
Any point north of the
Arctic Circle or south of the
Antarctic Circle will have one period in the summer when the sun doesn't set, and one period in the winter when the sun doesn't rise. At progressively higher latitudes, the periods of "
midnight sun" (or "midday dark" for the other side of the globe) are progressively longer. For example, at the military and weather station
Alert on the northern tip of
Ellesmere Island,
Canada (about 450
nautical miles or 830
km from the
North Pole), the sun begins to peek above the horizon in mid-February and each day it climbs higher and stays up longer; by
21 March, the sun is up for 12 hours. However, mid-February isn't first light. The sky (as seen from Alert) has
twilight, or at least a pre-dawn glow on the horizon, for increasing hours each day, for more than a month before the sun first appears.
In the weeks surrounding
21 June, the sun is at its highest, and it appears to circle the sky without going below the horizon. Eventually, it does go below the horizon, for progressively longer periods each day until, around the middle of October, it disappears for the last time. For a few more weeks, "day" is marked by decreasing periods of twilight. Eventually, for the weeks surrounding
21 December, it's continuously dark. In later winter, the first faint wash of light briefly touches the horizon (for just minutes per day), and then increases in duration and pre-dawn brightness each day until sunrise in February.
Reckoning
Meteorological
Meteorological seasons are reckoned by temperature, with summer being the hottest quarter of the year and winter the coldest quarter of the year.
Using this reckoning, the
Roman calendar began the year and the spring season on the first of March, with each season occupying three months. This reckoning is also used in
Denmark, the former
USSR, and
Australia. In the modern
United Kingdom there are no hard and fast rules about seasons, and informally many people use this reckoning.
So, in meteorology for the Northern hemisphere: spring begins on
March 1, summer on
June 1, autumn on
September 1, and winter on
December 1. Conversely, for the Southern hemisphere: summer begins on
December 1, autumn on
March 1, winter on
June 1, and spring on
September 1.
Astronomical
In
astronomical reckoning, the seasons begin at the
solstices and
equinoxes. The
cross-quarter days are considered seasonal midpoints. The length of these seasons isn't uniform because of the elliptical orbit of the earth and its
different speeds along that orbit.
In the conventional United States calendar: Winter (89 days) begins on
21 December, the winter solstice; spring (92 days) on
20 March, the vernal equinox; summer (93 days) on
20 June, the summer solstice; and autumn (90 days) on
22 September, the autumnal equinox.
Because of the differences in the Northern and Southern Hemispheres, it's no longer considered appropriate to use the northern-seasonal designations for the astronomical quarter days. The modern convention for them is: March Equinox; June Solstice; September Equinox; and December Solstice
Traditional
Traditional seasons are reckoned by
insolation, with summer being the quarter of the year with the greatest insolation and winter the quarter with the least. These seasons begin about 4 weeks earlier than the meteorological seasons and 7 weeks earlier than the astronomical seasons.
In traditional reckoning, the seasons begin at the
cross-quarter days. The solstices and equinoxes are the
midpoints of these seasons. For example, the days of greatest and least insolation are considered the "midsummer" and "midwinter" respectively.
This reckoning is used by various traditional cultures in the Northern Hemisphere, including
East Asian and Irish cultures.
In
Iran,
Afghanistan and some other parts of middle east the beginning of the astronomical spring is the beginning of the new year which is called
Nowruz.
So, according to traditional reckoning, winter begins between
5 November and
10 November,
Samhain,
立冬 (lìdōng); spring between
2 February and
7 February,
Imbolc,
立春 (lìchūn); summer between
4 May and
10 May,
Beltane,
立夏 (lìxià); and autumn between
3 August and
10 August,
Lughnasadh,
立秋 (lìqiū).
The middle of each season is considered Mid-winter, between
20 December and
23 December,
冬至 (dōngzhì); Mid-spring, between
19 March and
22 March,
春分 (chūnfēn); Mid-summer, between
19 June and
23 June,
夏至 (xiàzhì); and Mid-autumn, between
21 September and
24 September,
秋分 (qiūfēn).
.
Australia
In
Australia, the traditional aboriginal people defined the seasons by what was happening to the plants, animals and weather around them. This led to each separate tribal group have different seasons, some with up to 8 seasons each year. However, most modern
Aboriginal Australians follow the meteorological seasons as do non-Aboriginal Australians.
In art
The (four) seasons have inspired many artists. Below is a list of some notable artwork about this theme:
Further Information
Get more info on 'Season'.
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