Similarities between Alpha Cephei and Beta Cephei
Alpha Cephei and Beta Cephei have 31 things in common (in Unionpedia): Apparent magnitude, Arabic, Astronomische Gesellschaft Katalog, Bayer designation, Bright Star Catalogue, Catalog of Components of Double and Multiple Stars, Catalogues of Fundamental Stars, Celestial sphere, Centre de données astronomiques de Strasbourg, Cepheus (constellation), Circumpolar star, Constellation, Durchmusterung, Eta Cephei, Europe, Flamsteed designation, Henry Draper Catalogue, Hipparcos, IAU Working Group on Star Names, International Astronomical Union, Iota Cephei, Latinisation of names, Light pollution, Main sequence, North Pole, Polaris, Pole star, Precession, Smithsonian Astrophysical Observatory Star Catalog, Ulugh Beg, ..., VizieR. Expand index (1 more) »
Apparent magnitude
The apparent magnitude of a celestial object is a number that is a measure of its brightness as seen by an observer on Earth.
Alpha Cephei and Apparent magnitude · Apparent magnitude and Beta Cephei ·
Arabic
Arabic (العَرَبِيَّة) or (عَرَبِيّ) or) is a Central Semitic language that first emerged in Iron Age northwestern Arabia and is now the lingua franca of the Arab world. It is named after the Arabs, a term initially used to describe peoples living from Mesopotamia in the east to the Anti-Lebanon mountains in the west, in northwestern Arabia, and in the Sinai peninsula. Arabic is classified as a macrolanguage comprising 30 modern varieties, including its standard form, Modern Standard Arabic, which is derived from Classical Arabic. As the modern written language, Modern Standard Arabic is widely taught in schools and universities, and is used to varying degrees in workplaces, government, and the media. The two formal varieties are grouped together as Literary Arabic (fuṣḥā), which is the official language of 26 states and the liturgical language of Islam. Modern Standard Arabic largely follows the grammatical standards of Classical Arabic and uses much of the same vocabulary. However, it has discarded some grammatical constructions and vocabulary that no longer have any counterpart in the spoken varieties, and has adopted certain new constructions and vocabulary from the spoken varieties. Much of the new vocabulary is used to denote concepts that have arisen in the post-classical era, especially in modern times. During the Middle Ages, Literary Arabic was a major vehicle of culture in Europe, especially in science, mathematics and philosophy. As a result, many European languages have also borrowed many words from it. Arabic influence, mainly in vocabulary, is seen in European languages, mainly Spanish and to a lesser extent Portuguese, Valencian and Catalan, owing to both the proximity of Christian European and Muslim Arab civilizations and 800 years of Arabic culture and language in the Iberian Peninsula, referred to in Arabic as al-Andalus. Sicilian has about 500 Arabic words as result of Sicily being progressively conquered by Arabs from North Africa, from the mid 9th to mid 10th centuries. Many of these words relate to agriculture and related activities (Hull and Ruffino). Balkan languages, including Greek and Bulgarian, have also acquired a significant number of Arabic words through contact with Ottoman Turkish. Arabic has influenced many languages around the globe throughout its history. Some of the most influenced languages are Persian, Turkish, Spanish, Urdu, Kashmiri, Kurdish, Bosnian, Kazakh, Bengali, Hindi, Malay, Maldivian, Indonesian, Pashto, Punjabi, Tagalog, Sindhi, and Hausa, and some languages in parts of Africa. Conversely, Arabic has borrowed words from other languages, including Greek and Persian in medieval times, and contemporary European languages such as English and French in modern times. Classical Arabic is the liturgical language of 1.8 billion Muslims and Modern Standard Arabic is one of six official languages of the United Nations. All varieties of Arabic combined are spoken by perhaps as many as 422 million speakers (native and non-native) in the Arab world, making it the fifth most spoken language in the world. Arabic is written with the Arabic alphabet, which is an abjad script and is written from right to left, although the spoken varieties are sometimes written in ASCII Latin from left to right with no standardized orthography.
Alpha Cephei and Arabic · Arabic and Beta Cephei ·
Astronomische Gesellschaft Katalog
The Astronomische Gesellschaft Katalog (AGK) is an astrometric star catalogue.
Alpha Cephei and Astronomische Gesellschaft Katalog · Astronomische Gesellschaft Katalog and Beta Cephei ·
Bayer designation
A Bayer designation is a stellar designation in which a specific star is identified by a Greek letter, followed by the genitive form of its parent constellation's Latin name.
Alpha Cephei and Bayer designation · Bayer designation and Beta Cephei ·
Bright Star Catalogue
The Bright Star Catalogue, also known as the Yale Catalogue of Bright Stars or Yale Bright Star Catalogue, is a star catalogue that lists all stars of stellar magnitude 6.5 or brighter, which is roughly every star visible to the naked eye from Earth.
Alpha Cephei and Bright Star Catalogue · Beta Cephei and Bright Star Catalogue ·
Catalog of Components of Double and Multiple Stars
The Catalog of Components of Double and Multiple Stars, or CCDM, is an astrometric star catalogue of double and multiple stars.
Alpha Cephei and Catalog of Components of Double and Multiple Stars · Beta Cephei and Catalog of Components of Double and Multiple Stars ·
Catalogues of Fundamental Stars
The Catalogue of Fundamental Stars is a series of six astrometric catalogues of high precision positional data for a small selection of stars to define a celestial reference frame, which is a standard coordinate system for measuring positions of stars.
Alpha Cephei and Catalogues of Fundamental Stars · Beta Cephei and Catalogues of Fundamental Stars ·
Celestial sphere
In astronomy and navigation, the celestial sphere is an abstract sphere with an arbitrarily large radius concentric to Earth.
Alpha Cephei and Celestial sphere · Beta Cephei and Celestial sphere ·
Centre de données astronomiques de Strasbourg
The Centre de Données astronomiques de Strasbourg (CDS; English translation: Strasbourg Astronomical Data Center) is a data hub which collects and distributes astronomical information.
Alpha Cephei and Centre de données astronomiques de Strasbourg · Beta Cephei and Centre de données astronomiques de Strasbourg ·
Cepheus (constellation)
Cepheus is a constellation in the northern sky, which is named after Cepheus (a King in the Greek mythology).
Alpha Cephei and Cepheus (constellation) · Beta Cephei and Cepheus (constellation) ·
Circumpolar star
A circumpolar star is a star, as viewed from a given latitude on Earth, that never sets below the horizon due to its apparent proximity to one of the celestial poles.
Alpha Cephei and Circumpolar star · Beta Cephei and Circumpolar star ·
Constellation
A constellation is a group of stars that are considered to form imaginary outlines or meaningful patterns on the celestial sphere, typically representing animals, mythological people or gods, mythological creatures, or manufactured devices.
Alpha Cephei and Constellation · Beta Cephei and Constellation ·
Durchmusterung
In astronomy, Durchmusterung or Bonner Durchmusterung (BD), is the comprehensive astrometric star catalogue of the whole sky, compiled by the Bonn Observatory (Germany) from 1859 to 1903.
Alpha Cephei and Durchmusterung · Beta Cephei and Durchmusterung ·
Eta Cephei
Eta Cephei (η Cep, η Cephei) is a star in the northern circumpolar constellation of Cepheus.
Alpha Cephei and Eta Cephei · Beta Cephei and Eta Cephei ·
Europe
Europe is a continent located entirely in the Northern Hemisphere and mostly in the Eastern Hemisphere.
Alpha Cephei and Europe · Beta Cephei and Europe ·
Flamsteed designation
A Flamsteed designation is a combination of a number and constellation name that uniquely identifies most naked eye stars in the modern constellations visible from southern England.
Alpha Cephei and Flamsteed designation · Beta Cephei and Flamsteed designation ·
Henry Draper Catalogue
The Henry Draper Catalogue (HD) is an astronomical star catalogue published between 1918 and 1924, giving spectroscopic classifications for 225,300 stars; it was later expanded by the Henry Draper Extension (HDE), published between 1925 and 1936, which gave classifications for 46,850 more stars, and by the Henry Draper Extension Charts (HDEC), published from 1937 to 1949 in the form of charts, which gave classifications for 86,933 more stars.
Alpha Cephei and Henry Draper Catalogue · Beta Cephei and Henry Draper Catalogue ·
Hipparcos
Hipparcos was a scientific satellite of the European Space Agency (ESA), launched in 1989 and operated until 1993.
Alpha Cephei and Hipparcos · Beta Cephei and Hipparcos ·
IAU Working Group on Star Names
The International Astronomical Union (IAU) established a Working Group on Star Names (WGSN) in May 2016 to catalog and standardize proper names for stars for the international astronomical community.
Alpha Cephei and IAU Working Group on Star Names · Beta Cephei and IAU Working Group on Star Names ·
International Astronomical Union
The International Astronomical Union (IAU; Union astronomique internationale, UAI) is an international association of professional astronomers, at the PhD level and beyond, active in professional research and education in astronomy.
Alpha Cephei and International Astronomical Union · Beta Cephei and International Astronomical Union ·
Iota Cephei
Iota Cephei (ι Cephei, ι Cep) is a solitary star in the northern constellation Cepheus.
Alpha Cephei and Iota Cephei · Beta Cephei and Iota Cephei ·
Latinisation of names
Latinisation or Latinization is the practice of rendering a non-Latin name (or word) in a Latin style.
Alpha Cephei and Latinisation of names · Beta Cephei and Latinisation of names ·
Light pollution
Light pollution, also known as photopollution, is the presence of anthropogenic light in the night environment.
Alpha Cephei and Light pollution · Beta Cephei and Light pollution ·
Main sequence
In astronomy, the main sequence is a continuous and distinctive band of stars that appear on plots of stellar color versus brightness.
Alpha Cephei and Main sequence · Beta Cephei and Main sequence ·
North Pole
The North Pole, also known as the Geographic North Pole or Terrestrial North Pole, is (subject to the caveats explained below) defined as the point in the Northern Hemisphere where the Earth's axis of rotation meets its surface.
Alpha Cephei and North Pole · Beta Cephei and North Pole ·
Polaris
Polaris, designated Alpha Ursae Minoris (Ursae Minoris, abbreviated Alpha UMi, UMi), commonly the North Star or Pole Star, is the brightest star in the constellation of Ursa Minor.
Alpha Cephei and Polaris · Beta Cephei and Polaris ·
Pole star
Pole star or polar star refers to a star, preferably bright, closely aligned to the axis of rotation of an astronomical object.
Alpha Cephei and Pole star · Beta Cephei and Pole star ·
Precession
Precession is a change in the orientation of the rotational axis of a rotating body.
Alpha Cephei and Precession · Beta Cephei and Precession ·
Smithsonian Astrophysical Observatory Star Catalog
The Smithsonian Astrophysical Observatory Star Catalog is an astrometric star catalogue.
Alpha Cephei and Smithsonian Astrophysical Observatory Star Catalog · Beta Cephei and Smithsonian Astrophysical Observatory Star Catalog ·
Ulugh Beg
Mīrzā Muhammad Tāraghay bin Shāhrukh (میرزا محمد طارق بن شاہ رخ, میرزا محمد تراغای بن شاہ رخ), better known as Ulugh Beg (March 22, 1394 in Sultaniyeh, Persia – October 27, 1449, Samarkand), was a Timurid ruler as well as an astronomer, mathematician and sultan.
Alpha Cephei and Ulugh Beg · Beta Cephei and Ulugh Beg ·
VizieR
The VizieR Catalogue Service is an astronomical catalog service provided by Centre de données astronomiques de Strasbourg.
The list above answers the following questions
- What Alpha Cephei and Beta Cephei have in common
- What are the similarities between Alpha Cephei and Beta Cephei
Alpha Cephei and Beta Cephei Comparison
Alpha Cephei has 58 relations, while Beta Cephei has 58. As they have in common 31, the Jaccard index is 26.72% = 31 / (58 + 58).
References
This article shows the relationship between Alpha Cephei and Beta Cephei. To access each article from which the information was extracted, please visit: