cleomedes subsolar kupala 66.56 dōngzhì solstices heliacal 23.44 zodiacal rōmaji 至 makara sosigenes declination equinoxes 943396 midpoints 2001jha 8332 gēs perihelion chí solstitial hibernal ivison 하지 willmann ecliptic constellations estival
when are the solstices and equinoxes each year
Solstice - wikipedia Solstice Jump to : navigation , search For other uses , see Solstice ( disambiguation ) . <Th_colspan="9"> UT date and time of equinoxes and solstices on Earth event <Th_colspan="2"> equinox <Th_colspan="2"> solstice <Th_colspan="2"> equinox <Th_colspan="2"> solstice month <Th_colspan="2"> March <Th_colspan="2"> June <Th_colspan="2"> September <Th_colspan="2"> December year day time day time day time day time 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 : 12 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 2015 20 22 : 45 21 16 : 38 23 08 : 21 22 04 : 48 2016 20 04 : 30 20 22 : 34 22 14 : 21 21 10 : 44 2017 20 10 : 28 21 04 : 24 22 20 : 02 21 16 : 28 2018 20 16 : 15 21 10 : 07 23 01 : 54 21 22 : 23 2019 20 21 : 58 21 15 : 54 23 07 : 50 22 04 : 19 2020 20 03 : 50 20 21 : 44 22 13 : 31 21 10 : 02 This article needs additional citations for verification . Please help improve this article by adding citations to reliable sources . Unsourced material may be challenged and removed . ( June 2013 ) ( Learn how and when to remove this template message ) The solstice occurs twice each year ( around June 21 and December 21 ) as the Sun reaches its most northerly or southerly excursion relative to the celestial equator on the celestial sphere . The seasons of the year are directly connected to both the solstices and the equinoxes . The term solstice can also be used in a broader sense , as the day when this occurs . The day of the solstice has either the most sunlight of the year ( summer solstice ) or the least sunlight of the year ( winter solstice ) for any place other than the equator . Alternative terms , with no ambiguity as to which hemisphere is the context , are June solstice and December solstice , referring to the months of year in which they take place . At latitudes outside the tropics , the summer solstice marks the day when the sun appears highest in the sky . Within the tropics , the sun appears directly overhead ( called the subsolar point ) from days to months before the solstice and again after the solstice , which means the subsolar point occurs twice each year . The word solstice is derived from the Latin sol ( sun ) and sistere ( to stand still ) , because at the solstices , the Sun stands still in declination ; that is , the seasonal movement of the Sun 's path ( as seen from Earth ) comes to a stop before reversing direction . Contents ( hide ) 1 Definitions and frames of reference 2 Relationship to seasons 3 Cultural aspects 3.1 Ancient Greek names and concepts 3.2 English names 3.3 Solstice terms in East Asia 3.4 Solstice celebrations 3.5 Solstice determination 4 In the constellations 5 Solstices on other planets 6 See also 7 References 8 External links Definitions and frames of reference ( edit ) For an observer on the North Pole , the Sun reaches the highest position in the sky once a year in June . The day this occurs is called the June solstice day . Similarly , for an observer on the South Pole , the Sun reaches the highest position on the December solstice day . When it is the summer solstice at one Pole , it is the winter solstice on the other . The Sun 's westerly motion never ceases as Earth is continually in rotation . However , the Sun 's motion in declination comes to a stop at the moment of solstice . In that sense , solstice means `` sun - standing '' . This modern scientific word descends from a Latin scientific word in use in the late Roman Republic of the 1st century BC : solstitium . Pliny uses it a number of times in his Natural History with a similar meaning that it has today . It contains two Latin - language morphemes , sol , `` sun '' , and - stitium , `` stoppage '' . The Romans used `` standing '' to refer to a component of the relative velocity of the Sun as it is observed in the sky . Relative velocity is the motion of an object from the point of view of an observer in a frame of reference . From a fixed position on the ground , the Sun appears to orbit around Earth . To an observer in an inertial frame of reference , planet Earth is seen to rotate about an axis and revolve around the Sun in an elliptical path with the Sun at one focus . Earth 's axis is tilted with respect to the plane of Earth 's orbit and this axis maintains a position that changes little with respect to the background of stars . An observer on Earth therefore sees a solar path that is the result of both rotation and revolution . A solargraph taken from the Atacama Pathfinder Experiment at the Llano de Chajnantor Observatory in the southern hemisphere . This is a long - exposure photograph , with the image exposed for six months in a direction facing east of north , from mid-December 2009 until the southern winter solstice in June 2010 . The sun 's path each day can be seen from right to left in this image across the sky ; the path of the following day runs slightly lower , until the day of the winter solstice , whose path is the lowest one in the image . The component of the Sun 's motion seen by an earthbound observer caused by the revolution of the tilted axis -- which , keeping the same angle in space , is oriented toward or away from the Sun -- is an observed daily increment ( and lateral offset ) of the elevation of the Sun at noon for approximately six months and observed daily decrement for the remaining six months . At maximum or minimum elevation , the relative yearly motion of the Sun perpendicular to the horizon stops and reverses direction . Outside of the tropics , the maximum elevation occurs at the summer solstice and the minimum at the winter solstice . The path of the Sun , or ecliptic , sweeps north and south between the northern and southern hemispheres . The days are longer around the summer solstice and shorter around the winter solstice . When the Sun 's path crosses the equator , the length of the nights at latitudes + L ° and - L ° are of equal length . This is known as an equinox . There are two solstices and two equinoxes in a tropical year . Relationship to seasons ( edit ) Main article : Season The seasons occur because the Earth 's axis of rotation is not perpendicular to its orbital plane ( the `` plane of the ecliptic '' ) but currently makes an angle of about 23.44 ° ( called the `` obliquity of the ecliptic '' ) , and because the axis keeps its orientation with respect to an inertial frame of reference . As a consequence , for half the year the Northern Hemisphere is inclined toward the Sun while for the other half year the Southern Hemisphere has this distinction . The two moments when the inclination of Earth 's rotational axis has maximum effect are the solstices . At the June solstice the subsolar point is further north than any other time : at latitude 23.44 ° north , known as the Tropic of Cancer . Similarly at the December solstice the subsolar point is further south than any other time : at latitude 23.44 ° south , known as the Tropic of Capricorn . The subsolar point will cross every latitude between these two extremes exactly twice per year . Also during the June solstice , places on the Arctic Circle ( latitude 66.56 ° north ) will see the Sun just on the horizon during midnight , and all places north of it will see the Sun above horizon for 24 hours . That is the midnight sun or midsummer - night sun or polar day . On the other hand , places on the Antarctic Circle ( latitude 66.56 ° south ) will see the Sun just on the horizon during midday , and all places south of it will not see the Sun above horizon at any time of the day . That is the polar night . During the December Solstice , the effects on both hemispheres are just the opposite . This also allows the polar sea ice to increase its annual growth and temporary extent at a greater level due to lack of direct sunlight . Illumination of Earth by Sun at the northern solstice . Illumination of Earth by Sun at the southern solstice . Diagram of the Earth 's seasons as seen from the north . Far right : southern solstice Diagram of the Earth 's seasons as seen from the south . Far left : northern solstice Two images showing the amount of reflected sunlight at southern and northern summer solstices , respectively ( watts / m2 ) . Cultural aspects ( edit ) Ancient Greek names and concepts ( edit ) The concept of the solstices was embedded in ancient Greek celestial navigation . As soon as they discovered that the Earth is spherical they devised the concept of the celestial sphere , an imaginary spherical surface rotating with the heavenly bodies ( ouranioi ) fixed in it ( the modern one does not rotate , but the stars in it do ) . As long as no assumptions are made concerning the distances of those bodies from Earth or from each other , the sphere can be accepted as real and is in fact still in use . The Ancient Greeks use the term `` ηλιοστάσιο '' ( heliostāsio ) , meaning stand of the Sun . The stars move across the inner surface of the celestial sphere along the circumferences of circles in parallel planes perpendicular to the Earth 's axis extended indefinitely into the heavens and intersecting the celestial sphere in a celestial pole . The Sun and the planets do not move in these parallel paths but along another circle , the ecliptic , whose plane is at an angle , the obliquity of the ecliptic , to the axis , bringing the Sun and planets across the paths of and in among the stars. * Cleomedes states : The band of the Zodiac ( zōdiakos kuklos , `` zodiacal circle '' ) is at an oblique angle ( loksos ) because it is positioned between the tropical circles and equinoctial circle touching each of the tropical circles at one point ... This Zodiac has a determinable width ( set at 8 ° today ) ... that is why it is described by three circles : the central one is called `` heliacal '' ( hēliakos , `` of the sun '' ) . The term heliacal circle is used for the ecliptic , which is in the center of the zodiacal circle , conceived as a band including the noted constellations named on mythical themes . Other authors use Zodiac to mean ecliptic , which first appears in a gloss of unknown author in a passage of Cleomedes where he is explaining that the Moon is in the zodiacal circle as well and periodically crosses the path of the Sun . As some of these crossings represent eclipses of the Moon , the path of the Sun is given a synonym , the ekleiptikos ( kuklos ) from ekleipsis , `` eclipse '' . English names ( edit ) The two solstices can be distinguished by different pairs of names , depending on which feature one wants to stress . Summer solstice and winter solstice are the most common names , referring to the seasons they are associated with . However , these can be ambiguous since the northern hemisphere 's summer is the southern hemisphere 's winter , and vice versa . The Latinate names estival solstice ( summer ) and hibernal solstice ( winter ) are sometimes used to the same effect , as are midsummer and midwinter . June solstice and December solstice refer to the months of year in which they take place , with no ambiguity as to which hemisphere is the context . They are still not universal , however , as not all cultures use a solar - based calendar where the solstices occur every year in the same month ( as they do not in the Islamic calendar and Hebrew calendar , for example ) . Northern solstice and southern solstice indicate the hemisphere of the Sun 's location . The northern solstice is in June , when the Sun is directly over the Tropic of Cancer in the Northern Hemisphere , and the southern solstice is in December , when the Sun is directly over the Tropic of Capricorn in the Southern Hemisphere . These terms can be used unambiguously for other planets . First point of Cancer and first point of Capricorn refer to the astrological signs that the sun is entering . Due to the precession of the equinoxes , however , the constellations where the solstices are currently located are Taurus and Sagittarius , respectively . Solstice terms in east asia ( edit ) Main articles : Xiazhi and Dongzhi ( solar term ) The traditional East Asian calendars divide a year into 24 solar terms ( 節氣 ) . Xiàzhì ( pīnyīn ) or Geshi ( rōmaji ) ( Chinese and Japanese : 夏至 ; Korean : 하지 ( Haji ) ; Vietnamese : Hạ chí ; literally : `` summer 's extreme '' ) is the 10th solar term , and marks the summer solstice . It begins when the Sun reaches the celestial longitude of 90 ° ( around June 21 ) and ends when the Sun reaches the longitude of 105 ° ( around July 7 ) . Xiàzhì more often refers in particular to the day when the Sun is exactly at the celestial longitude of 90 ° . Dōngzhì ( pīnyīn ) or Tōji ( rōmaji ) ( Chinese and Japanese : 冬至 ; Korean : 동지 ( Dongji ) ; Vietnamese : Đông chí ; literally : `` winter 's extreme '' ) is the 22nd solar term , and marks the winter solstice . It begins when the Sun reaches the celestial longitude of 270 ° ( around December 22 ) and ends when the Sun reaches the longitude of 285 ° ( around January 5 ) . Dōngzhì more often refers in particular to the day when the Sun is exactly at the celestial longitude of 270 ° . The solstices ( as well as the equinoxes ) mark the middle of the seasons in East Asian calendars . Here , the Chinese character 至 means `` extreme '' , so the terms for the solstices directly signify the summits of summer and winter . Solstice celebrations ( edit ) See also : Fête St - Jean - Baptiste , Festival of San Juan , Saint Jonas Day , St John 's Day ( Estonia ) , Ivan Kupala Day , and Golowan This section does not cite any sources . Please help improve this section by adding citations to reliable sources . Unsourced material may be challenged and removed . ( June 2012 ) ( Learn how and when to remove this template message ) 2005 Summer Solstice Sunrise over Stonehenge The term solstice can also be used in a wider sense , as the date ( day ) that such a passage happens . The solstices , together with the equinoxes , are connected with the seasons . In some languages they are considered to start or separate the seasons ; in others they are considered to be centre points ( in England , in the Northern Hemisphere , for example , the period around the northern solstice is known as midsummer , and Midsummer 's Day is June 24 , about three days after the solstice itself ) . Similarly December 25 is the start of the Christmas celebration , and is the day the Sun begins to return to the Northern Hemisphere . Many cultures celebrate various combinations of the winter and summer solstices , the equinoxes , and the midpoints between them , leading to various holidays arising around these events . For the southern solstice , Christmas is the most popular holiday to have arisen . In addition , Yalda , Saturnalia , Karachun , Hanukkah , Kwanzaa and Yule ( see winter solstice for more ) are also celebrated around this time . For the northern solstice , Christian cultures celebrate the feast of St. John from June 23 to 24 ( see St. John 's Eve , Ivan Kupala Day , Midsummer ) , while Neopagans observe Midsummer , also known as Litha . For the vernal ( spring ) equinox , several spring - time festivals are celebrated , such as the Persian Nowruz , the observance in Judaism of Passover and in most Christian churches of Easter . The autumnal equinox has also given rise to various holidays , such as the Jewish holiday of Sukkot . At the midpoints between these four solar events , cross-quarter days are celebrated . In the southern tip of South America , the Mapuche people celebrate We Tripantu ( the New Year ) a few days after the northern solstice , on June 24 . Further north , the Atacama people formerly celebrated this date with a noise festival , to call the Sun back . Further east , the Aymara people celebrate their New Year on June 21 . A celebration occurs at sunrise , when the sun shines directly through the Gate of the Sun in Tiwanaku . Other Aymara New Year feasts occur throughout Bolivia , including at the site of El Fuerte de Samaipata . In many cultures , the solstices and equinoxes traditionally determine the midpoint of the seasons , which can be seen in the celebrations called midsummer and midwinter . In this vein , the Japanese celebrate the start of each season with an occurrence known as Setsubun . The cumulative cooling and warming that result from the tilt of the planet become most pronounced after the solstices , leading to the more recent custom of using them to mark the beginning of summer and winter in most countries of Central and Northern Europe , as well as in Canada , the United States and New Zealand . In the Hindu calendar , two sidereal solstices are named Makara Sankranti which marks the start of Uttarayana and Karka Sankranti which marks the start of Dakshinayana . The former occurs around January 14 each year , while the latter occurs around July 14 each year . These mark the movement of the Sun along a sidereally fixed zodiac ( precession is ignored ) into Makara , the zodiacal sign which corresponds with Capricorn , and into Karkat , the zodiacal sign which corresponds with Cancer , respectively . The Amundsen -- Scott South Pole Station celebrates every year on June 21 a midwinter party , to celebrate that the Sun is at its lowest point and coming back . The Fremont Solstice Parade takes place every summer solstice in Fremont , Seattle , Washington in the United States . Solstice determination ( edit ) Unlike the equinox , the solstice time is not easy to determine . The changes in solar declination become smaller as the sun gets closer to its maximum / minimum declination . The days before and after the solstice , the declination speed is less than 30 arcseconds per day which is less than ⁄ of the angular size of the sun , or the equivalent to just 2 seconds of right ascension . This difference is hardly detectable with indirect viewing based devices like sextant equipped with a vernier , and impossible with more traditional tools like a gnomon or an astrolabe . It is also hard to detect the changes on sunrise / sunset azimuth due to the atmospheric refraction changes . Those accuracy issues render it impossible to determine the solstice day based on observations made within the 3 ( or even 5 ) days surrounding the solstice without the use of more complex tools . Accounts do not survive but Greek astronomers must have used an approximation method based on interpolation , which is still used by some amateurs . This method consists of recording the declination angle at noon during some days before and after the solstice , trying to find two separate days with the same declination . When those two days are found , the halfway time between both noons is estimated solstice time . An interval of 45 days has been postulated as the best one to achieve up to a quarter - day precision , in the solstice determination . In 2012 , the journal DIO found that accuracy of one or two hours with balanced errors can be attained by observing the sun 's equal altitudes about S = twenty degrees ( or d = about 20 days ) before and after the summer solstice because the average of the two times will be early by q arc minutes where q is ( πe cosA ) / 3 times the square of S in degrees ( e = earth orbit eccentricity , A = earth 's perihelion or sun 's apogee ) , and the noise in the result will be about 41 hours divided by d if the eye 's sharpness is taken as one arc minute . Astronomical almanacs define the solstices as the moments when the sun passes through the solstitial colure , i.e. the times when the apparent geocentric longitude of the sun is equal to 90 ° ( summer solstice ) or 270 ° ( winter solstice ) . In the constellations ( edit ) Using the current official IAU constellation boundaries -- and taking into account the variable precession speed and the rotation of the ecliptic -- the solstices shift through the constellations as follows ( expressed in astronomical year numbering in which the year 0 = 1 BC , − 1 = 2 BC , etc . ) : The northern solstice passed from Leo into Cancer in year − 1458 , passed into Gemini in year − 10 , passed into Taurus in December 1989 , and is expected to pass into Aries in year 4609 . The southern solstice passed from Capricornus into Sagittarius in year − 130 , is expected to pass into Ophiuchus in year 2269 , and is expected to pass into Scorpius in year 3597 . Solstices on other planets ( edit ) Due to the 687 - day orbit of Mars around the Sun ( almost twice that of the Earth ) , the planet experiences its summer and winter solstices at approximately 23 month intervals . See also ( edit ) Analemma Geocentric view of the seasons Iranian calendars Perihelion and aphelion Zoroastrian calendar References ( edit ) Jump up ^ United States Naval Observatory ( 21 September 2015 ) . `` Earth 's Seasons : Equinoxes , Solstices , Perihelion , and Aphelion , 2000 - 2025 '' . Retrieved 9 December 2015 . Jump up ^ `` The Summer and Winter Solstices '' . Scholastic. 2017 . Retrieved October 1 , 2017 . Jump up ^ `` solstice '' . The American Heritage Dictionary of the English Language ( Fifth ed . ) . Houghton Mifflin Harcourt. 2015 . Retrieved December 8 , 2015 . Jump up ^ The Principle of relativity was first applied to inertial frames of reference by Albert Einstein . Before then , the concepts of absolute space and time applied by Isaac Newton prevailed . The motion of the Sun across the sky is still called `` apparent motion '' in celestial navigation in deference to the Newtonian view , but the reality of the supposed `` real motion '' has no special laws to commend it , both are visually verifiable and both follow the same laws of physics . Jump up ^ `` A Solargraph taken from APEX at Chajnantor '' . European Southern Observatory . Retrieved December 9 , 2015 . Jump up ^ For an introduction to these topics of astronomy refer to Bowditch , Nathaniel ( 2002 ) . The American Practical Navigator : an Epitome of Navigation ( PDF ) . Bethesda , Maryland : National Geospatial - Intelligence Agency . Chapter 15 Navigational Astronomy ' . Retrieved December 9 , 2015 . Jump up ^ Strabo . The Geography. II. 5.1. sphairikē ... tēs gēs epiphaneia , spherical is the surface of the Earth Jump up ^ Strabo . The Geography . pp. II. 5.2. sphairoeidēs ... ouranos , spherical in appearance ... is heaven Jump up ^ Strabo II. 5.2. , `` aplaneis asteres kata parallēlōn pherontai kuklōn '' , `` the fixed stars are borne in parallel circles '' Jump up ^ Strabo II. 5.2 , `` ho di'autēs ( gē ) aksōn kai tou ouranou mesou tetagmenos '' , `` the axis through it ( the Earth ) extending through the middle of the sky '' Jump up ^ Cleomedes ( 2004 ) . Cleomedes ' Lectures on Astronomy : A Translation of The Heavens . Translated by Alan C. Bowen and Robert B. Todd . Berkeley : University of California Press . p. 41 . ISBN 0 - 520 - 23325 - 5 . This translation cites this passage at the end of Book I Chapter 2 but other arrangements have it at the start of Chapter 3 . In the Greek version of Cleomedes ( 1891 ) . Ziegler , Hermann , ed . Cleomedis De motu circulari corporum caelestium libri duo . B.G. Teubneri . p. 32 . the passage starts Chapter 4 . Jump up ^ Kent , April Elliott ( June 7 , 2011 ) . The Essential Guide to Practical Astrology . Penguin . p. 284 . ISBN 978 - 1 - 61564 - 093 - 5 . Retrieved December 9 , 2015 . Jump up ^ Bass , Charles O. ( 1994 ) . Astronomy Essentials . Research & Education Assoc . p. 35 . ISBN 978 - 0 - 87891 - 965 - 9 . Retrieved December 9 , 2015 . Jump up ^ Kiddle , Henry ( 1877 ) . A new manual of the elements of astronomy , descriptive and mathematical : comprising the latest discoveries and theoretic views : with directions for the use of the globes , and for studying the constellations . Ivison , Blakeman , Taylor , & Company . p. 82 . Retrieved June 2 , 2011 . Jump up ^ Jain , R.K. ICSE Geography . Ratna Sagar . p. 25 . ISBN 978 - 81 - 8332 - 579 - 0 . Retrieved December 9 , 2015 . Jump up ^ Stewart , Alexander ( 1869 ) . A Compendium of ModernGeography . Edinburgh : Oliver & Boyd . p. 383 . Retrieved December 9 , 2015 . Jump up ^ http://www.southpolestation.com/news/news.html , South Pole News Jump up ^ Mollerup , Asger ( January 12 , 2008 ) . `` Solstice Determination based on Observations '' . Archived from the original on February 11 , 2009 . Retrieved September 27 , 2010 . Jump up ^ Exton , Harold ( 1992 ) . `` A Fresh Analysis of Some Recent Data on Atmospheric Refraction Near the Horizon with Implications in Archaeoastronomy '' . Journal of History of Astronomy , Archaeoastronomy Supplement. 23 : S57 . Bibcode : 1992JHAS ... 23 ... 57E . Jump up ^ Hugh , Thurston ( 2001 ) . `` Early Greek Solstices and Equinoxes '' . Journal for the History of Astronomy . 32 , Part 2 ( 107 ) : 154 -- 156 . Bibcode : 2001JHA ... 32 ... 154T . ISSN 0021 - 8286 . Jump up ^ Meeus , Jean ( 1998 ) . Astronomical Algorithms ( Second English ed . ) . Richmond : Willmann - Bell , Inc . pp. 177 -- 182 . ISBN 0 - 943396 - 61 - 1 . Jump up ^ Meeus , Jean ( 1997 ) . Mathematical astronomy morsels ( 1st English ed . ) . Richmond : Willmann - Bell , Inc . ISBN 0 - 943396 - 51 - 4 . Jump up ^ Planetary Society . `` Mars Calendar '' . Retrieved December 9 , 2015 . External links ( edit ) Look up solstice in Wiktionary , the free dictionary . Wikimedia Commons has media related to Solstice . Equinoxes and Solstices Calculator ( 1600 to 2400 ) `` Earth 's Seasons : Equinoxes , Solstices , Perihelion , and Aphelion ( 2000 -- 2025 ) '' . United States Naval Observatory , Astronomical Applications Department . Retrieved December 9 , 2015 . Weisstein , Eric ( 1996 -- 2007 ) . `` Summer Solstice '' . Eric Weisstein 's World of Astronomy . Retrieved October 24 , 2008 . The above plots show how the date of the summer solstice shifts through the Gregorian calendar according to the insertion of leap years . <Th_colspan="2"> Time measurement and standards <Td_colspan="2"> Chronometry Orders of magnitude Metrology International standards Coordinated Universal Time offset UT ΔT DUT1 International Earth Rotation and Reference Systems Service ISO 31 - 1 ISO 8601 International Atomic Time 6 - hour clock 12 - hour clock 24 - hour clock Barycentric Coordinate Time Barycentric Dynamical Time Civil time Daylight saving time Geocentric Coordinate Time International Date Line Leap second Solar time Terrestrial Time Time zone 180th meridian Obsolete standards Ephemeris time Greenwich Mean Time Prime meridian Time in physics Absolute time and space Spacetime Chronon Continuous signal Coordinate time Cosmological decade Discrete time and continuous time Planck time Proper time Theory of relativity Time dilation Gravitational time dilation Time domain Time translation symmetry T - symmetry Horology Clock Astrarium Atomic clock Complication History of timekeeping devices Hourglass Marine chronometer Marine sandglass Radio clock Watch Water clock Sundial Dialing scales Equation of time History of sundials Sundial markup schema Calendar Astronomical Dominical letter Epact Equinox Gregorian Hebrew Hindu Intercalation Islamic Julian Leap year Lunar Lunisolar Solar Solstice Tropical year Weekday determination Weekday names Archaeology and geology Chronological dating Geologic time scale International Commission on Stratigraphy Astronomical chronology Galactic year Nuclear timescale Precession Sidereal time Units of time Century Day Decade Fortnight Hour Jiffy Lustrum Millennium Minute Moment Month Paksha Saeculum Second Shake Week Year Related topics Chronology Duration music Mental chronometry Metric time System time Time value of money Timekeeper <Th_colspan="2"> Ancient Greek astronomy Astronomers Aglaonice Agrippa Anaximander Andronicus Apollonius Aratus Aristarchus Aristyllus Attalus Autolycus Bion Callippus Cleomedes Cleostratus Conon Eratosthenes Euctemon Eudoxus Geminus Heraclides Hicetas Hipparchus Hippocrates of Chios Hypsicles Menelaus Meton Oenopides Philip of Opus Philolaus Posidonius Ptolemy Pytheas Seleucus Sosigenes of Alexandria Sosigenes the Peripatetic Strabo Thales Theodosius Theon of Alexandria Theon of Smyrna Timocharis Works Almagest ( Ptolemy ) On Sizes and Distances ( Hipparchus ) On the Sizes and Distances ( Aristarchus ) On the Heavens ( Aristotle ) Instruments Antikythera mechanism Armillary sphere Astrolabe Dioptra Equatorial ring Gnomon Mural instrument Triquetrum Concepts Callippic cycle Celestial spheres Circle of latitude Counter-Earth Deferent and epicycle Equant Geocentrism Heliocentrism Hipparchic cycle Metonic cycle Octaeteris Solstice Spherical Earth Sublunary sphere Zodiac Influences Babylonian astronomy Egyptian astronomy Influenced Medieval European science Indian astronomy Medieval Islamic astronomy GND : 4369408 - 1 Retrieved from `` https://en.wikipedia.org/w/index.php?title=Solstice&oldid=806641999 '' Categories : Astronomical events of the Solar System Calendars Movable December observances Dynamics of the Solar System Movable June observances Summer holidays Technical factors of astrology Time in astronomy Winter holidays Hidden categories : Use mdy dates from October 2017 Articles needing additional references from June 2013 All articles needing additional references Articles containing Korean - language text Articles containing Vietnamese - language text Articles needing additional references from June 2012 Wikipedia articles with GND identifiers Talk Contents About Wikipedia Afrikaans Ænglisc Asturianu Azərbaycanca Беларуская Български Boarisch Català Čeština ChiShona Cymraeg Dansk Deutsch Eesti Ελληνικά Español Esperanto Euskara فارسی Français Frysk Gaeilge Galego 한국어 हिन्दी Hrvatski Ido Bahasa Indonesia Íslenska Italiano עברית Kreyòl ayisyen Kurdî Latina Latviešu Lëtzebuergesch Lietuvių Magyar Македонски മലയാളം Bahasa Melayu Nederlands Nedersaksies 日本 語 Norsk Norsk nynorsk Occitan ଓଡ଼ିଆ ਪੰਜਾਬੀ Polski Português Română Русский Саха тыла Shqip Simple English Slovenčina Slovenščina کوردی Српски / srpski Srpskohrvatski / српскохрватски Suomi Svenska Tagalog தமிழ் ไทย Türkçe Українська Tiếng Việt Winaray 吴语 粵語 Žemaitėška 中文 Edit links This page was last edited on 23 October 2017 , at 08 : 38 . 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