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Carina OB1
Carina OB1 is a giant OB association in the Carina Nebula, which is home to some of the most massive and luminous stars in the Milky Way Galaxy. It includes the young star clusters Collinder 228, NGC 3293, NGC 3324, IC 2581, Trumpler 14, Trumpler 15 and Trumpler 16, the last being the home of Eta Carinae. It also includes another massive and luminous star, HD 93129A. It is approximately from Earth. It is one of the largest known stellar associations, along with Sagittarius OB5 and Cygnus OB2. It is much easier to see than that of the other associations since Carina OB1 has relatively little dust extinction in its region. Together with Carina OB2 Carina OB2 is a giant OB association In astronomy, stellar kinematics is the observational study or measurement of the kinematics or motions of stars through space. Stellar kinematics encompasses the measurement of stellar velocities in the Mil ..., they compromise the most massive stellar grouping known in the galaxy. Cari ...
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NGC 3372d
NGC commonly refers to: * New General Catalogue of Nebulae and Clusters of Stars, a catalogue of deep sky objects in astronomy NGC may also refer to: Companies * NGC Corporation, name of US electric company Dynegy, Inc. from 1995 to 1998 * National Gas Company of Trinidad and Tobago, state-owned natural gas company in Trinidad and Tobago * National Grid plc, a former name of National Grid Electricity Transmission plc, the operator of the British electricity transmission system * Northrop Grumman Corporation, aerospace and defense conglomerate formed from the merger of Northrop Corporation and Grumman Corporation in 1994 * Numismatic Guaranty Corporation, coin certification company in the United States Other uses

* National Gallery of Canada, art gallery founded in 1880 in Ottawa, Canada * National Geographic (American TV channel), National Geographic, documentary and reality television channel established in the United States in 2001 formerly called National Geographic Chann ...
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Trumpler 15
Trumpler 15 is an open cluster in the constellation Carina Carina ( ) is a constellation in the southern sky. Its name is Latin for the keel of a ship, and it was the southern foundation of the larger constellation of Argo Navis (the ship ''Argo'') until it was divided into three pieces, the other two b ... that lies on the outskirts of the Carina Nebula. Estimated ages of the stars in Trumpler 15 suggest that the cluster is slightly older than its sibling clusters Trumpler 14 and 16. References External links * Carina Nebula Open clusters Carina (constellation) Trumpler catalog Star-forming regions {{star-cluster-stub ...
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Carina OB2
Carina OB2 is a giant OB association in the constellation Carina Carina may refer to: Places Australia * Carina, Queensland, a suburb in Brisbane * Carina Heights, Queensland, a suburb in Brisbane * Carina, Victoria, a locality in Mildura Serbia * Carina, Osečina, a village in the Kolubara District .... It contains anywhere from 91 to 157 stars, many of which are hot blue stars of spectral types B and O. It is located 3.1 kiloparsecs distant and is around 4 million years old. References Stellar associations Carina (constellation) {{star-cluster-stub ...
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Cygnus OB2
Cygnus OB2 is an OB association that is home to some of the most massive and most luminous stars known, including suspected Luminous blue variable Cyg OB2 #12. It also includes one of the largest known stars, NML Cygni. The region is embedded within a wider one of star formation known as Cygnus X, which is one of the most luminous objects in the sky at radio wavelengths. The region is approximately 1,570 parsecs from Earth in the constellation of Cygnus. The young cluster is one of the largest known and the largest in the northern hemisphere with some authors formerly classifying it as a young globular cluster similar to those in the Large Magellanic Cloud. Today, however, it is considered a massive, low-density stellar association. Although it is over ten times more massive than the Orion Nebula, which is easily seen with the naked eye, Cygnus OB2 is hidden behind a massive dust cloud known as the Cygnus Rift, which obscures many of the stars in it. This means that ...
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Sagittarius OB5
Sagittarius ( ) may refer to: * Sagittarius (constellation) * Sagittarius (astrology), a sign of the Zodiac Ships *'' SuperStar Sagittarius'', a cruise ship * USS ''Sagittarius'' (AKN-2), a World War II US Navy cargo ship Music *Sagittarius (band), an American sunshine pop studio group * Ensemble Sagittarius, an ensemble conducted by Michel Laplénie Fictional characters *Sagittarius (comics), member of Zodiac, an evil group in the Marvel Universe *Sagittarius Aiolos, a character in ''Saint Seiya'' *Sagittarius, a ''Fairy Tail'' character Zoology *''Sagittarius serpentarius'' or secretarybird, a large, mostly terrestrial bird of prey *''Sibynophis sagittarius'', a species of snake found in South Asia Other uses *Sagittarii, Ancient Roman archers *Sagittario or Sagittarius, a Beyblade toy See also *Sagittarius Dwarf Galaxy (other) * * *Sagitta (other) *''Sagittaria ''Sagittaria'' is a genus of about 30
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HD 93129A
HD 93129 is a triple star system in the Carina Nebula, with all three components being hot O class stars amongst the most luminous stars in the Milky Way. It is the dominant member of the Trumpler 14 star cluster, a young star cluster within the Carina OB1 stellar association that harbors other super-luminous stars, like Eta Carinae and WR 25. Location HD 93129 is found at the centre of the massive Trumpler 14 open cluster in the Carina Nebula star forming region. It is too far away for its distance to have been accurately determined using the annual parallax method, but accurate distances for η Carinae and the Homunculus Nebula, modelling of clusters, and astrophysical data about other stars assumed to be within the same region, all lead to a distance around 2,300 parsecs. HD 93129 Aa is the closest O2 supergiant to Earth. That volume of space is home to many other massive and luminous stars. HD 93128, yet another O3.5 main sequence star, is only 24' away within ...
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Eta Carinae
Eta Carinae (η Carinae, abbreviated to η Car), formerly known as Eta Argus, is a stellar system containing at least two stars with a combined luminosity greater than five million times that of the Sun, located around distant in the constellation Carina. Previously a 4th-magnitude star, it brightened in 1837 to become brighter than Rigel, marking the start of its so-called "Great Eruption". It became the second-brightest star in the sky between 11 and 14 March 1843 before fading well below naked eye visibility after 1856. In a smaller eruption, it reached 6th magnitude in 1892 before fading again. It has brightened consistently since about 1940, becoming brighter than magnitude 4.5 by 2014. At declination −59° 41′ 04.26″, Eta Carinae is circumpolar from locations on Earth south of latitude 30°S, (for reference, the latitude of Johannesburg is 26°12′S); and is not visible north of about latitude 30°N, just south of Cairo, which is at a latitude ...
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Trumpler 16
Trumpler 16 (''Tr 16'') is a massive open cluster that is home to some of the most luminous stars in the Milky Way galaxy. It is situated within the Carina Nebula complex in the Carina–Sagittarius Arm, located approximately from Earth. The cluster has one star visible to the naked eye from the tropics southward, Eta Carinae. Description Its most luminous members are and , with both having luminosities several million times that of the Sun, and there are three other extreme stars with O3 spectral classes. Both and are binaries, with the primary stars contributing most of the luminosity, but with companions which are themselves more massive and luminous than most stars. Totalling all wavelengths, is estimated to be the more luminous of the two, 4,600,000 times the Sun's luminosity ( absolute bolometric magnitude -12) compared to at 2,400,000 times the Sun's luminosity (absolute bolometric magnitude -11.2). However, appears by far the brightest object, both because it ...
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Trumpler 14
Trumpler 14 (''Tr 14'') is an open cluster with a diameter of , located within the inner regions of the Carina Nebula, approximately from Earth. Together with the nearby Trumpler 16, they are the main clusters of the Carina OB1 stellar association, which is the largest association in the Carina Nebula, although Trumpler 14 is not as massive or as large as Trumpler 16. About stars have been identified in Trumpler 14 and the total mass of the cluster is estimated to be 4,300 . Age It is one of the youngest known star clusters, estimates range from 300 to 500 thousand years old. For comparison, the massive super star cluster R136 is about 1 to 2 million years old, and the famous Pleiades is about 115 million years old. Members Due to its location within the inner parts of the Carina Nebula, Trumpler 14 is currently undergoing massive star formation. As a result, the star cluster exhibits many stars of late O to early A spectral type, which are very massive (at least 10 solar ...
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Carina (Chandra)
Carina may refer to: Places Australia * Carina, Queensland, a suburb in Brisbane * Carina Heights, Queensland, a suburb in Brisbane * Carina, Victoria, a locality in Mildura Serbia * Carina, Osečina, a village in the Kolubara District People * Carina (name), a given name (including a list of people with the name) * Carina, a pet form of the given name Cara * Carina, a Latinization of Cairenn, said to be the mother of Niall of the Nine Hostages Anatomy * ''Carina'', the scientific name for an anatomical structure resembling a keel, such as the large keel on the breastbone in birds * Carina of trachea, the point at which the trachea branches to form the two mainstem bronchi Astronomy * Carina (Chinese astronomy) * Carina (constellation), a constellation * Carina Dwarf, a dwarf galaxy orbiting the Milky Way * Carina Nebula (NGC 3372) Arts, entertainment, and media * "Carina" (Corrado Lojacono song), a 1958 song covered by Sophia Loren, Dean Martin and Cliff Richard ...
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NGC 3324
NGC 3324 is an open cluster in the southern constellation Carina, located northwest of the Carina Nebula at a distance of from Earth. It is closely associated with the emission nebula , also known as . The two are often confused as a single object, and together have been nicknamed the "Gabriela Mistral Nebula" due to its resemblance to the Chilean poet. was first catalogued by James Dunlop in 1826. The Hubble Space Telescope observed a western section of NGC 3324 in detail, and the same section was one of the first observations of the James Webb Space Telescope, for comparison. Nearby clusters NGC 3324 is associated with the open cluster NGC 3293. Both are fairly young, at around 12 million years old. They show some degree of mass segregation, with more massive stars concentrated near their centers. Neither are dynamically relaxed. Gallery File:Carina Nebula by Harel Boren (151851961).jpg, The Carina Nebula with NGC 3324 at top right File:NGC 3324 Hubble.jpg, Hubbl ...
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