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UTC date and time of solstices and equinoxes[1]
year Equinox
Mar
Solstice
June
Equinox
Sept
Solstice
Dec
day time day time day time day time
2002 20 19:16 21 13:24 23 04:55 22 01:14
2003 21 01:00 21 19:10 23 10:47 22 07:04
2004 20 06:49 21 00:57 22 16:30 21 12:42
2005 20 12:33 21 06:46 22 22:23 21 18:35
2006 20 18:26 21 12:26 23 04:03 22 00:22
2007 21 00:07 21 18:06 23 09:51 22 06:08
2008 20 05:48 20 23:59 22 15:44 21 12:04
2009 20 11:44 21 05:45 22 21:18 21 17:47
2010 20 17:32 21 11:28 23 03:09 21 23:38
2011 20 23:21 21 17:16 23 09:04 22 05:30
2012 20 05:14 20 23:09 22 14:49 21 11:11
2013 20 11:02 21 05:04 22 20:44 21 17:11
2014 20 16:57 21 10:51 23 02:29 21 23:03

In astronomy, equinox can have two meanings:

An equinox in astronomy is that moment in time (not a whole day) when the centre of the Sun can be observed to be directly above the Earth's equator, occurring around March 20 and September 23 each year. Astronomy (from the Greek words astron (ἄστρον "star" and nomos (νόμος "law" is the scientific study The Sun (Sol is the Star at the center of the Solar System. EARTH was a short-lived Japanese vocal trio which released 6 singles and 1 album between 2000 and 2001 The equator (sometimes referred to colloquially as "the Line") is the intersection of the Earth 's surface with the plane perpendicular to the Events 1600 - The Linköping Bloodbath takes place on Maundy Thursday in Linköping, Sweden. Events 1122 - Concordat of Worms. 1459 - Battle of Blore Heath, the first major battle of the English

More technically, at an equinox, the Sun is at one of two opposite points on the celestial sphere where the celestial equator (i. In Astronomy and Navigation, the celestial sphere is an imaginary rotating Sphere of "gigantic Radius " The celestial equator is a Great circle on the imaginary Celestial sphere, in the same plane as the Earth 's Equator. e. declination 0) and ecliptic intersect. The ecliptic is the apparent path that the Sun traces out in the sky during the year These points of intersection are called equinoctial points—the vernal point and the autumnal point. By extension, the term equinox may be used to denote an equinoctial point.

There is either an equinox (autumn and spring) or a solstice (summer and winter) on approximately the 21st day of the last month of every quarter of the calendar year. Solstices occur twice a year when the tilt of the Earth's axis is most oriented toward or away from the Sun, causing the Sun to reach its northernmost and southernmost extremes On a day which has an equinox, the centre of the Sun will spend a nearly equal amount of time above and below the horizon at every location on Earth and night and day will be of nearly the same length. The word equinox derives from the Latin words aequus (equal) and nox (night). In reality, the day is longer than the night at an equinox. Commonly the day is defined as the period that sunlight reaches the ground in the absence of local obstacles. A day (symbol d is a unit of Time equivalent to 24 Hours and the duration of a single Rotation of planet Earth with respect to the From Earth, the Sun appears as a disc and not a single point of light; so, when the centre of the Sun is below the horizon, the upper edge is visible. Furthermore, the atmosphere refracts light; so, even when the upper limb of the Sun is below the horizon, its rays reach over the horizon to the ground. In sunrise/sunset tables, the assumed semidiameter (apparent radius) of the sun is 16 minutes of arc and the atmospheric refraction is assumed to be 34 minutes of arc. Sunrise is the instant at which the upper edge of the Sun appears above the Horizon in the East. Sunset, also called sundown in some American English Dialects is the instant when the trailing edge of the Sun 's disk disappears below Remote Authentication Dial In User Service ( RADIUS) is a networking protocol that provides centralized access authorization and accounting management for people or computers A minute of arc, arcminute, or MOA is a unit of angular measurement, equal to one sixtieth (1/60 of one degree. Atmospheric Refraction is the deviation of Light or other Electromagnetic wave from a straight line as it passes through the atmosphere due to the Their combination means that when the upper limb of Sun is on the visible horizon its centre is 50 minutes of arc below the geometric horizon, which is the intersection with the celestial sphere of a horizontal plane through the eye of the observer. These effects together make the day about 14 minutes longer than the night at the equator, and longer still at sites toward the poles. The real equality of day and night only happens at places far enough from the equator to have at least a seasonal difference in daylength of 7 minutes, and occurs a few days towards the winter side of each equinox.

Illumination of the Earth by the Sun on the day of equinox, (ignoring twilight).
Illumination of the Earth by the Sun on the day of equinox, (ignoring twilight).
The Earth in its orbit around the Sun causes the Sun to appear on the celestial sphere moving over the ecliptic (red), which is tilted on the equator (blue).
The Earth in its orbit around the Sun causes the Sun to appear on the celestial sphere moving over the ecliptic (red), which is tilted on the equator (blue).
Diagram of the Earth's seasons as seen from the north. Far right: December solstice
Diagram of the Earth's seasons as seen from the north. Far right: December solstice
Diagram of the Earth's seasons as seen from the south. Far left: June solstice
Diagram of the Earth's seasons as seen from the south. Far left: June solstice
Day arc at 0° latitude, equator
Day arc at 0° latitude, equator
Day arc at 20° latitude
Day arc at 20° latitude
Day arc at 50° latitude
Day arc at 50° latitude
Day arc at 70° latitude
Day arc at 70° latitude
Day arc at 90° latitude, pole
Day arc at 90° latitude, pole

Contents

Names

Heliocentric view of the seasons

The Earth's seasons are caused by the rotation axis of the Earth not being perpendicular to its orbital plane. A season is one of the major divisions of the Year, generally based on yearly periodic changes in Weather. The Earth's axis is tilted at an angle of approximately 23. 44° from the orbital plane. This tilt is called the axial tilt. In Astronomy, axial tilt is the Inclination angle of a planet's rotational axis in relation to its orbital plane. As a consequence, for half a year (from around 20 March to around 22 September) the northern hemisphere tips toward the Sun, with the maximum around 21 June, while for the other half year the southern hemisphere has this honour, with the maximum around 21 December. Events 1600 - The Linköping Bloodbath takes place on Maundy Thursday in Linköping, Sweden. Events 66 - Emperor Nero creates the Legion I Italica. 1236 - The Lithuanians Events 524 - Godomar, King of the Burgundians defeats the Franks at the Battle of Vézeronce. Events 69 - The end of the Year of the four emperors: Following Galba, Otho and Vitellius, Vespasian The two instances when the Sun is directly overhead at the equator are the equinoxes. The equator (sometimes referred to colloquially as "the Line") is the intersection of the Earth 's surface with the plane perpendicular to the Also at that moment both the north pole and south pole of the Earth are just on the terminator, and day and night are divided equally between the hemispheres. The terminator is a fictive line that delimits the illuminated day side and dark Night side of a planetary body (also known as the "grey line" or

The table above gives the dates and times of equinoxes and solstices over several years. Solstices occur twice a year when the tilt of the Earth's axis is most oriented toward or away from the Sun, causing the Sun to reach its northernmost and southernmost extremes A few remarks can be made about the equinoxes:

Geocentric view of the seasons

The explanation given in the previous section would be useful for an observer in outer space. As seen by an observer on Earth, it may appear to the casual observer that the Sun revolves around the Earth once a year. As such, in the half year centred around June it rises and sets more towards the north, which means longer days and shorter nights for the northern hemisphere and shorter days and longer nights for the southern hemisphere. In the half year centred around December the Sun rises and sets more towards the south, and the day and night durations are reversed.

Also on the equinox day, the Sun rises, for every place on Earth (except at the poles), at 6:00 in the morning and sets at 18:00 in the evening local time. But these times are not exact for several reasons.

Day arcs of the Sun

Some of the above statements can be made clearer when picturing the day arc: the path the Sun tracks along the celestial dome in its diurnal movement. Diurnal motion is an astronomical term referring to the apparent daily motion of Stars around the Earth, or more precisely around the two The pictures show this for every hour on equinox day. In addition, also some 'ghost' suns are indicated below the horizon, up to 18° down. The Sun in this area still causes twilight. Twilight is the time before Sunrise, called Dawn, and the time after Sunset, called Dusk. The pictures can be used for both the northern and the southern hemisphere. The observer is supposed to sit near the tree on the island in the middle of the ocean. The green arrows give the cardinal directions.

The following special cases are depicted.

Celestial coordinate systems

The vernal point (vernal equinox)—the one the Sun passes in March on its way from south to north—is used as the origin of some celestial coordinate systems:

Because of the precession of the Earth's axis, the position of the vernal point changes over time and as a consequence both the equatorial and the ecliptic coordinate systems change over time. In Astronomy, Precession refers to the movement of the rotational axis of a body such as a planet with respect to Inertial space. Therefore, when specifying celestial coordinates for an object, one have to specify at what time the vernal point (and also the celestial equatorial) are taken. That reference time is also called equinox. In Astronomy, equinox is a moment in time at which the vernal point Celestial equator, and other such elements are taken to be used in the definition of a

The autumnal equinox is at ecliptic longitude 180° and at right ascension 12h.

The upper culmination of the vernal point is considered the start of the sidereal day for the observer. In astronomy the culmination, at a given point of a Planet, Star, Constellation, etc Sidereal time is a measure of the position of the Earth in its rotation around its axis or time measured by the apparent Diurnal motion of the Vernal equinox The hour angle of the vernal point is, by definition, the observer's sidereal time. In Astronomy, the hour angle is one of the coordinates used in the Equatorial coordinate system for describing the position of a point on the Celestial sphere Sidereal time is a measure of the position of the Earth in its rotation around its axis or time measured by the apparent Diurnal motion of the Vernal equinox

For Western tropical astrology, the same thing holds true; the vernal equinox is the first point (i. Western astrology is the system of Astrology most popular in Western countries e. the start) of the sign of Aries. Aries, the ram, is the first Astrological sign in the Zodiac. In this system, it is of no significance that the fixed stars and equinox shift compared to each other due to the precession of the equinoxes. In Astronomy, Precession refers to the movement of the rotational axis of a body such as a planet with respect to Inertial space.

In Jyotiṣa on the other hand, their 'vernal equinox' was fixed to the stars about 17 centuries ago, and has been drifting away from the seasons since then, now amounting to 22 days. Jyotiṣa ( Sanskrit jyotiṣa, from jyótis- "light heavenly body" also spelled Jyotish and Jyotisha in English

Cultural aspects

In the list below the terms March and September equinoxes are used when the celebration is fixed in time, while the terms spring and autumn equinoxes refer to those which are different in the two hemispheres.

Myths, fables and facts

References

  1. ^ United States Naval Observatory (01/28/07). Earth's Seasons: Equinoxes, Solstices, Perihelion, and Aphelion, 2000-2020.
  2. ^ Anthony Aveni, "Spring Equinox: Watching the Serpent Descend," The Book of the Year: A Brief History of Our Seasonal Holidays (Oxford: Oxford University Press, 2004), 47-61.
  3. ^ Baha'i calendar
  4. ^ The Ismaili: Navroz. Retrieved on 2008-03-26. 2008 ( MMVIII) is the current year in accordance with the Gregorian calendar, a Leap year that started on Tuesday of the Common Events 1026 - Pope John XIX crowns Conrad II as Holy Roman Emperor.
  5. ^ Infernal Egguinox
  6. ^ Standing an egg on end on the Spring Equinox
  7. ^ Equinox Means Balanced Light, Not Balanced Eggs
  8. ^ http://www.de-fact-o.com/fact_read.php?id=99 De-Fact-o article on the egg equinox myth

External links

Dictionary

equinox

-noun

  1. The intersection of the ecliptic (apparent path of the sun) with the celestial equator. Vernal Equinox is the intersection that the sun crosses about March 20; autumnal equinox denotes the crossing point about September 23.
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