Solstice

A solstice, also called solstitium (Latin for "solar standstill"), occurs twice in the course of the year. On this date, the highest or lowest midday position of the sun is reached in geographical latitudes outside the tropics between the tropics:

• At the summer solstice, the Sun has its greatest noon altitude above the horizon - in the northern hemisphere of the Earth on June 20, 21 or 22; in 2020, the summer point was passed on June 20 at 23:44 CEST, in 2021 it was on June 21 at 05:32 CEST.

• At the winter solstice, the Sun has the lowest noon altitude above the horizon - in the northern hemisphere of the Earth on December 21 or 22; in 2019, the winter point was passed on December 22 at 05:19 CET, in 2020 on December 21 at 11:02 CET.

In the southern hemisphere the situation is reversed: during the northern winter it is summer in the southern hemisphere, and vice versa. Over places on the equator the apparent path of the sun at the equinoxes passes exactly through the zenith; but during the northern summer it passes somewhat more northerly, and during the southern summer somewhat more southerly, in both cases therefore not quite as high as the zenith.

Twice in the course of a tropical year, the Sun takes up positions of greatest angular separation in its apparent motion along the ecliptic north or south of the celestial equator. The two reversal points are also called solstices and, depending on the hemisphere, are referred to as the summer or winter solstice. After passing these points of extreme declination - at the summer and winter points, respectively - their position approaches the celestial equator again, which is reached at the vernal and autumnal points. Together with these two equinoxes (equinoxes), the two solstices terminate the astronomical seasons.

Astronomical basics

Definition

The exact definition is: The solstices are the times when the apparent geocentric ecliptical longitude of the sun is 90° or 270°.

• Apparent means: taking aberration and nutation into account.
• Geocentric means: seen from a fictitious observer at the center of the earth. The definition is therefore independent of the location of a real observer; the solstices therefore occur worldwide at the same time (which, however, corresponds to different times depending on the local time zone).

A simple planetary geometric definition is: Solstice: The angle sun center-earth center-earth pole is extreme. Two cases: Extreme angle minimum -> summer solstice; extreme angle maximum -> winter solstice; so the two Earth hemispheres have both cases simultaneously, alternating. (Equinox: The angle sun-center-earth-center-earth-pole is a right one).

The two times coincide, except for a few minutes, with those times when the Sun reaches its greatest northern or southern declination - about 23° 26′ 20″ - and thus its northernmost or southernmost position on the celestial sphere. The small time difference results from the fact that it is actually the barycenter of the Earth/Moon system that moves uniformly around the Sun in the Earth's orbital plane (ecliptic), while the Earth itself orbits this common center of gravity and is usually slightly above or below this plane. Seen from the geocenter, the Sun therefore does not run exactly on the ecliptic (it has a non-zero ecliptic latitude). Therefore, on the one hand, it does not pass exactly the northernmost or southernmost point of the ecliptic, and on the other hand, its variable ecliptic latitude means that the maximum declination is not usually assumed to be exactly at the solstice points.

Conclusions

The solstices mark the beginning of the astronomical summer or winter. When the Sun reaches its greatest northern or southern declination of 23.4°, it is perpendicular to the so-called tropics of the Earth (namely the parallels of latitude at 23.4° north or south). So it stands

• on 21 or 20 June above the Tropic of Cancer (summer solstice in the northern hemisphere, winter solstice in the southern hemisphere),
• on 21 or 22 December over the Tropic of Capricorn (winter solstice in the northern hemisphere, summer solstice in the southern hemisphere).

The following applies to both hemispheres: At the winter solstice the sun reaches its lowest point in the course of the year in relation to the meridian passage. At this time there is the shortest day and the longest night, because the greater part of the daily solar orbit lies below the horizon. Conversely, the sun reaches its highest position at the summer solstice. At this time there is the longest day and the shortest night, because the greater part of the daily solar orbit lies above the horizon.

Near the polar circles there is a day without sunrise at the winter solstice and a day without sunset at the summer solstice (midnight sun, "white nights"). Further to the pole, there is a polar day for weeks or months, or a polar night at the other pole. During these periods without twilight, the daily path of the sun lies completely above or below the horizon.

Between the solstices, the sun crosses the celestial equator and then stands vertically above the earth's equator. These times are the equinoxes or equinoxes. Equinoxes and solstices represent the beginning of the respective astronomical seasons.

Although the day of the winter solstice is the shortest day, the earliest sunset in the northern hemisphere occurs about ten days earlier and the latest sunrise about ten days later. The reason for this is the equation of time. At the summer solstice in the northern hemisphere, this effect is analogous to about four days.

Date

Because the solar year is almost six hours longer than the calendar common year with exactly 365 days, the time of the solstices shifts in each year by almost six hours to a later time. Since in leap years such as 2016, 2020 and 2024 (highlighted in bold in the table) a leap day is inserted in February, the date given in the calendar is then one day earlier than that of the previous year.

In the Central European Time Zone, the summer solstice currently falls on June 21. In the 20th century, it could also occur on June 22. In the 21st century, starting in 2020, it will sometimes be on June 20 because the leap rule (365.2425 days) can only approximate the actual length of the year (365.2422 days). Without the Gregorian calendar reform, its date would shift by seven to eight days per millennium. This shortening took place by the fact that - deviating from the leap rule of the Julian calendar - the secular years (that are years, whose number is divisible by 100) receive no more leap day, unless the year number is divisible by 400.

Year	Summer Solstice		Winter Solstice
2015	June 21	18:38 CEST	December 22	05:48 CET
2016	June 21	00:34 CEST	December 21	11:44 CET
2017	June 21	06:24 CEST	December 21	17:28 CET
2018	June 21	12:07 CEST	December 21	23:23 CET
2019	June 21	17:54 CEST	December 22	05:19 CET
2020	June 20	23:44 CEST	December 21	11:02 CET
2021	June 21	05:32 CEST	December 21	16:59 CET
2022	June 21	11:14 CEST	December 21	22:48 CET
2023	June 21	16:58 CEST	December 22	04:27 CET
2024	June 20	22:51 CEST	December 21	10:20 CET
2025	June 21	04:42 CEST	December 21	16:03 CET
2026	June 21	10:24 CEST	December 21	21:50 CET
2027	June 21	16:11 CEST	December 22	03:42 CET

For more details, see the article Season.

Winter point and summer point

At the moment of the winter solstice, the Sun is located in comparison to the background stars in the so-called winter point - one of the two points of the ecliptic that are exactly 90° away from the vernal point (right ascension = 18h). It is currently located in the constellation Sagittarius (lat.: sagittarius); the galactic center is also located approximately in this direction.

Similarly, at the moment of the summer solstice, the Sun is in the so-called summer point (right ascension = 6h) in the constellation of Taurus.

Due to the precession of the Earth's axis, the winter point and the summer point move once through the entire zodiac in the course of 25,780 years (cycle of precession). Thus, in ancient times, the winter point was still in the constellation of Capricorn (hence "Tropic of Capricorn") and will move to the constellation of the Serpent Bearer in about 300 years.

In early antiquity, the summer equinox was located in the constellation Cancer (hence "Tropic of Cancer"), and its migration is shown in the following table over an entire cycle of precession. If we take the modern boundaries of the constellations as a basis, then it is located in the following constellations:

Constellation	Sector	Transit time	Admission	Middle	Exit
Shooter	33,3°	2380 years	13030 BC	11840 B.C.	10650 BC
Serpent Bearer	18,6°	1340 years	10650 BC	9980 BC	9310 BC
Scorpio	6,7°	480 years	9310 BC	9070 BC	8830 BC
Libra	23,0°	1650 years	8830 BC	8005 BC	7180 BC
Virgin	44,1°	3160 years	7180 BC	5600 BC	4020 BC
Lion	35,7°	2570 years	4020 BC	2735 BC.	1450 BC
Cancer	20,1°	1440 years	1450 BC	740 BC	10 BC
Twins	27,9°	2000 years	10 BC	990 A.D.	1989 AD. (20 Oct. 1989)
Taurus	36,7°	2620 years	1990 A.D. (near Orion)	3300 AD	4610 A.D.
Aries	24,7°	1770 years	4610 A.D.	5495 A.D.	6380 A.D.
Fish	37,2°	2670 years	6380 A.D.	7715 A.D.	9050 AD
Aquarius	24,0°	1710 years	9050 AD	9905 A.D.	10760 A.D.
Capricorn	28,0°	2010 years	10760 A.D.	11765 A.D.	12770 AD
Shooter	33,3°	2380 years	12770 AD	13960 A.D.	15150 AD

At an angle of 90° to the summer point and winter point lie the vernal point (right ascension = 0h) and the autumn point (right ascension = 12h), where the sun is located at the equinox.

Solstice line

The line connecting the positions of the earth at the time of the summer solstice and the winter solstice is called the solstice line. So this line passes through the middle of the sun, its extension outside the earth's orbit through the summer point and the winter point. It is perpendicular to the equinoctial line.

The Earth's orbit with equinoctial (green) and solstital (red) lines, as well as the elliptical major axis (turquoise) with aphelion and perihelion.


The dawn in Europe on a June 21


Annual cycle of the earth around the sun. Far left: Summer in the northern hemisphere. Far right: winter in the northern hemisphere.