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Puanga
), signalling the Māori new year., litcolor=, observedby=New Zealanders, nickname=, official_name=, alt=, image=M45 Pleiades Pbkwee (cropped to core 9 stars).jpg, relatedto=, date2022=24 June, date2023=14 July In Māori culture, Matariki is the name of the Pleiades star cluster and the celebration of its first rising in late June or early July. This marks the beginning of the new year in the Māori lunar calendar. Historically Matariki was usually celebrated for a period of days during the last quarter of the moon of the lunar month Pipiri (around June). The ceremony involved viewing the individual stars for forecasts of the year to come, mourning the deceased of the past year, and making an offering of food to replenish the stars. Some Māori use the rise of Puanga (Rigel) or other stars to mark the new year. Celebration of Matariki declined during the 20th century, but beginning in the early 1990s it underwent a revival. Matariki was first celebrated as an official public ...
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Rigel
Rigel is a blue supergiant star in the constellation of Orion. It has the Bayer designation β Orionis, which is Latinized to Beta Orionis and abbreviated Beta Ori or β Ori. Rigel is the brightest and most massive componentand the eponymof a star system of at least four stars that appear as a single blue-white point of light to the naked eye. This system is located at a distance of approximately from the Sun. A star of spectral type B8Ia, Rigel is calculated to be anywhere from 61,500 to 363,000 times as luminous as the Sun, and 18 to 24 times as massive, depending on the method and assumptions used. Its radius is more than seventy times that of the Sun, and its surface temperature is . Due to its stellar wind, Rigel's mass-loss is estimated to be ten million times that of the Sun. With an estimated age of seven to nine million years, Rigel has exhausted its core hydrogen fuel, expanded, and cooled to become a supergiant. It is expected to end its life a ...
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New Zealanders
New Zealanders ( mi, Tāngata Aotearoa), colloquially known as Kiwis (), are people associated with New Zealand, sharing a common history, culture, and language (New Zealand English). People of various ethnicities and national origins are citizens of New Zealand, governed by its nationality law. Originally composed solely of the indigenous Māori, the ethnic makeup of the population has been dominated since the 19th century by New Zealanders of European descent, mainly of English, Scottish, Welsh and Irish ancestry, with smaller percentages of other European and Middle Eastern ancestries such as Greek, Turkish, Italian, Lebanese and other Arab, German, Dutch, Scandinavian, South Slavic and Jewish, with Western European groups predominating. Today, the ethnic makeup of the New Zealand population is undergoing a process of change, with new waves of immigration, higher birth rates and increasing interracial marriage resulting in the New Zealand population of Māori, Asian, ...
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Makahiki
The Makahiki season is the ancient Hawaiian New Year festival, in honor of the god Lono of the Hawaiian religion. It is a holiday covering four consecutive lunar months, approximately from October or November through February or March. The focus of this season was a time for men, women and chiefs to rest, strengthen the body, and have great feasts of commemoration (''ʻahaʻaina hoʻomanaʻo''). During Makahiki season labor was prohibited and there were days for resting and feasting. The Hawaiians gave thanks to the god Lonoikamakahiki for his care. He brought life, blessings, peace and victory to the land. They also prayed to the gods for the death of their enemies. ''Makaʻainana'' (commoners) prayed that lands of their ''aliʻi'' (chief) may be increased, and that their own physical health along with the health of their chiefs be at the fullest. In antiquity, many religious ceremonies occurred during this period. Commoners stopped work, made offerings to the chief or ''alii ...
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Māori King Movement
The Māori King Movement, called the in Māori, is a movement that arose among some of the Māori (tribes) of New Zealand in the central North Island in the 1850s, to establish a role similar in status to that of the monarch of the British colonists, as a way of halting the alienation of Māori land. The Māori monarch technically operates in a non-constitutional capacity with no legal or judicial power within the New Zealand government, but nonetheless, is a major political and cultural figure in the country for many of its 5 million people, wielding significant lobbying power and . Reigning monarchs retain the position of paramount chief of several and wield some power over these, especially within Tainui. The current Māori monarch, Tūheitia Paki, was elected in 2006 and his official residence is Tūrongo House at Tūrangawaewae marae in the town of Ngāruawāhia. Tūheitia is the seventh monarch since the position was created and is the continuation of a dynasty that re ...
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Sterope (star)
The Sterope or Asterope system is a double star in the zodiac constellation of Taurus. Its components have the Flamsteed designations 21 Tauri and 22 Tauri, and are sometimes known as Sterope I and Sterope II, respectively. The International Astronomical Union applies the name ''Asterope'' specifically to 21 Tauri. The two stars are thus * 21 Tauri (or Sterope I, formally Asterope) * 22 Tauri (or Sterope II) The two stars are separated by 0.047° on the sky, which is equal to 2.82 arc-minutes and thus closer than the usual naked-eye resolution limit of 4 arc-min, giving an elongated appearance of the two together. Both are members of the Pleiades open star cluster ( M45) and approximately 440 light-years from the Sun. Nomenclature Asterope was one of the Pleiades sisters in Greek mythology. In 2016, the International Astronomical Union organized a Working Group on Star Names (WGSN) to catalogue and standardize proper names for stars. The WGSN decided to attribute ...
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Celaeno (star)
Celaeno , designated 16 Tauri, is a star in the constellation of Taurus and a member of the Pleiades open star cluster ( M45) of stars. Properties 16 Tauri is a blue-white B-type subgiant with an apparent magnitude of +5.45. It is approximately 430 light years from the Sun; about the same distance as the Pleiades. The interstellar extinction of this star is fairly small at 0.05 magnitudes. The projected rotational velocity of the equator is 185 km/s. Vizier table J/ApJ/573/359. It is over four times the radius of the Sun and has a surface temperature of 12,800 K. Nomenclature ''16 Tauri'' is the star's Flamsteed designation. It bore the traditional named ''Celaeno'' (or ''Celeno'') and was called the "Lost Pleiad" by Theon the Younger. Celaeno was one of the Pleiades sisters in Greek mythology. In 2016, the International Astronomical Union organized a Working Group on Star Names (WGSN) to catalogue and standardize proper names for stars. The WGSN approved ...
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Merope (star)
Merope , designated 23 Tauri (abbreviated 23 Tau), is a star in the constellation of Taurus and a member of the Pleiades star cluster. It is approximately away. Distance Despite being one of the closest star clusters to Earth, the distance to the Pleiades and its member stars is still in dispute. The parallax of Merope itself is not known precisely enough to give an accurate distance. Its Hipparcos parallax has a statistical margin of error of about 5% and gave a distance 116 parsecs. This, and an overall distance to the Pleiades calculated from Hipparcos parallaxes of 120 parsecs, are inconsistent with other parallax measurements such as from Gaia. Merope is too bright for Gaia to have a reliable parallax for it, but calculations of the overall distance to the Pleiades cluster using Hipparcos, Gaia, Hubble Space Telescope, and other methods repeatedly show that the Hipparcos parallaxes suffered from some kind of systemic error, and the distance to the Pleia ...
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Electra (star)
Electra , designated 17 Tauri, is a blue-white giant star in the constellation of Taurus (constellation), Taurus. It is the third-brightest star in the Pleiades Open cluster, open star cluster (Messier object, M45); the most visible stars in this group are named for the Pleiades (Greek mythology), Seven Sisters of Greek mythology. Properties The star has an apparent brightness of 3.72, the third-brightest of the stars in the group. Electra belongs to the spectral class B6 IIIe and is approximately 400 light-years from the Sun. The Pleiades cluster is thought to be 444 light-years away. The stellar rotation, projected rotational velocity of this star is 181 km/s, making it a fast rotator. This is the velocity component of the star's equatorial rotation along the line of sight to the Earth. The estimated inclination of the star's pole is , giving it a true equatorial rotational velocity of . The rapid rotation rate of this star flattens the poles and stretch the equa ...
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19 Tauri
19 Tauri is a double star in the constellation of Taurus and a member of the Pleiades open star cluster ( M45). It consists of a binary pair designated 19 Tauri A together with a single star visual companion, 19 Tauri B. 'A's' two components are themselves designated 19 Tauri Aa (officially named Taygeta , the traditional name for the entire system) and Ab. Based on parallax measurements obtained during the Hipparcos mission, 19 Tauri A is approximately 440 light-years from the Sun. Nomenclature ''19 Tauri'' is the system's Flamsteed designation. It also bears the little-used Bayer designation ''q Tauri''. The designations of the two constituents as ''19 Tauri A'' and ''B'', and those of ''A's'' components - ''19 Tauri Aa'' and ''Ab'' - derive from the convention used by the Washington Multiplicity Catalog (WMC) for multiple star systems, and adopted by the International Astronomical Union (IAU). The system bore the traditional name ''Taygeta'' (or ''Taygete''). ...
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Maia (star)
Maia , designated 20 Tauri (abbreviated 20 Tau), is a star in the constellation of Taurus. It is a blue giant of spectral type B8 III, a chemically peculiar star, and the prototype of the Maia variable class of variable star. Maia is the fourth-brightest star in the Pleiades open star cluster (Messier 45), after Alcyone, Atlas and Electra. It is surrounded by one of the brighter reflection nebulae within the Pleiades, designated NGC 1432 and sometimes called the Maia Nebula. Nomenclature The name ''Maia'' originates with the el, Μαῖα and la, Maia. Maia is one of the seven daughters of Atlas and Pleione in Greek mythology—stars which are also included in the Pleiades star cluster. In 2016, the International Astronomical Union organized a Working Group on Star Names (WGSN) to catalog and standardize proper names for stars. The WGSN's first bulletin of July 2016 included a table of the first two batches of names approved by the WGSN; which includ ...
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Alcyone (star)
Alcyone , designated η Tauri (Eta Tauri, abbreviated Eta Tau, η Tau), is a star in the constellation of Taurus. Approximately 440 light-years from the Sun, it is the brightest star in the Pleiades open cluster, which is a young cluster, around 100 million years old. There are a number of fainter stars very close to Alcyone, some of which are members of the same cluster. Nomenclature ''Eta Tauri'' is the star's Bayer designation. The name ''Alcyone'' originates in Greek mythology; she is one of the seven daughters of Atlas and Pleione known as the Pleiades. In 2016, the International Astronomical Union (IAU) organized a Working Group on Star Names (WGSN) to catalog and standardize proper names for stars. The WGSN's first bulletin of July 2016 included a table of the first two batches of names approved by the WGSN; which included ''Alcyone'' for this star. It is now so entered in the IAU Catalog of Star Names. In Chinese, (), meaning '' Hairy Head'', refers to a ...
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Pleione (star)
PleionePronounced or is a binary star and the seventh-brightest star in the Pleiades star cluster (Messier 45). It has the variable star designation BU Tauri (BU Tau) and the Flamsteed designation 28 Tauri (28 Tau). The star is located approximately from the Sun, appearing in the constellation of Taurus. Pleione is located close on the sky to the brighter star Atlas, so is difficult for stargazers to distinguish with the naked eye despite being a fifth magnitude star. The brighter star of the Pleione binary pair, component A, is a hot type B star 184 times more luminous than the Sun. It is classified as Be star with certain distinguishing traits: periodic phase changes and a complex circumstellar environment composed of two gaseous disks at different angles to each other. The primary star rotates rapidly, close to its breakup velocity, even faster than Achernar. Although some research on the companion star has been performed, stellar characteristics of the orbiti ...
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