Beta Carinae Observation data Epoch J2000 | Constellation (pronunciation) | Carina | | Right ascension | 09h 13m 12.0s | | Declination | -69° 43' 02" | | Apparent magnitude (V) | 1.67 | | Characteristics | | Spectral type | A2 IV | | U-B color index | 0.03 | | B-V color index | 0.00 | | Variable type | None | | Astrometry | | Radial velocity (Rv) | -5.2 km/s | | Proper motion (μ) | RA: -157.66 mas/yr Dec.: 108.91 mas/yr | | Parallax (π) | 29.34 ± 0.47 mas | | Distance | 111 ± 2 ly (34.1 ± 0.5 pc) | | Absolute magnitude (MV) | -1.00 | | Details | | Mass | 3 M☉ | | Radius | 5.7 R☉ | | Luminosity | 210 L☉ | | Temperature | 9,100 K | | Metallicity | ? | | Rotation | 2.1 days | | Age | 3.5 × 108 years | | Other designations | Miaplacidus, Gl 339.2, HR 3685, CD−69°600, HD 80007, GCTP 2213.00, SAO 250495, FK5 348, CP−69°1023, HIP 45238, GC 12764 | Beta Carinae (β Car / β Carinae) is the second brightest star in the constellation Carina and one of the brightest stars in the nighttime sky, with apparent magnitude 1.68. It is the brightest star in the south polar asterism known as the Diamond Cross, marking the southwestern end of the asterism. Beta Carinae also has the traditional name Miaplacidus, meaning "placid waters". In astronomy, an epoch is a moment in time for which celestial coordinates or orbital elements are specified. ...
This article is about the star grouping. ...
From the dawn of time, poop observed the sky and grouped stars into patterns or constellations. ...
Carina (IPA: , Latin: ) is a southern constellation which forms part of the old constellation of Argo Navis. ...
Equatorial Coordinates Right ascension (abbrev. ...
In astronomy, declination (abbrev. ...
The apparent magnitude (m) of a star, planet or other celestial body is a measure of its apparent brightness as seen by an observer on Earth. ...
In astronomy, stellar classification is a classification of stars based initially on photospheric temperature and its associated spectral characteristics, and subsequently refined in terms of other characteristics. ...
In astronomy, the color index is a simple numerical expression that determines the color of an object, which in the case of a star gives its temperature. ...
In astronomy, the color index is a simple numerical expression that determines the color of an object, which in the case of a star gives its temperature. ...
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Illustration of the use of optical wavelength interferometry to determine precise positions of stars. ...
Radial velocity is the velocity of an object in the direction of the line of sight. ...
kilometre per second is an SI derived unit of both speed (scalar) and velocity (vector), signified by the symbol km/s or km s-1. ...
The proper motion of a star is the motion of the position of the star in the sky (the change in direction in which we see it, as opposed to the radial velocity) after eliminating the improper motions of the stars, which affect their measured coordinates but are not real...
A milliarcsecond (m, mas) , or a thoundsanth of an arcsecond. ...
A year (from Old English gÄr) is the time between two recurrences of an event related to the orbit of the Earth around the Sun. ...
A milliarcsecond (m, mas) , or a thoundsanth of an arcsecond. ...
A year (from Old English gÄr) is the time between two recurrences of an event related to the orbit of the Earth around the Sun. ...
For other uses, see Parallax (disambiguation). ...
A milliarcsecond (m, mas) , or a thoundsanth of an arcsecond. ...
Distance is a numerical description of how far apart objects are at any given moment in time. ...
A light-year or lightyear (symbol: ly) is a unit of measurement of length, specifically the distance light travels in vacuum in one year. ...
A parsec is the distance from the Earth to an astronomical object which has a parallax angle of one arcsecond. ...
In astronomy, absolute magnitude is the apparent magnitude, m, an object would have if it were at a standard luminosity distance away from us, in the absence of interstellar extinction. ...
For other uses, see Mass (disambiguation). ...
In astronomy, the solar mass is a unit of mass used to express the mass of stars and larger objects such as galaxies. ...
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In astronomy, the solar radius is a unit of length used to express the size of stars and larger objects such as galaxies. ...
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The solar luminosity, , is a unit of luminosity (power emitted in the form of photons) conventionally used by astronomers to give the luminosities of stars. ...
For other uses, see Temperature (disambiguation). ...
For other uses, see Kelvin (disambiguation). ...
The globular cluster M80. ...
This illustration shows the oblate appearance of the star Achernar caused by rapid rotation. ...
This article is about the astronomical object. ...
A year (from Old English gÄr) is the time between two recurrences of an event related to the orbit of the Earth around the Sun. ...
A star catalogue, or star catalog, is an astronomical catalog that lists stars. ...
In astronomy, many stars are referred to simply by catalogue numbers. ...
In astronomy, many stars are referred to simply by catalogue numbers. ...
In astronomy, many stars are referred to simply by catalogue numbers. ...
The Henry Draper Catalogue is an astronomy catalogue with astrometric and spectroscopic data about more than 225,000 stars. ...
In astronomy, many stars are referred to simply by catalogue numbers. ...
Smithsonian Astrophysical Observatory Star Catalog contain the 258,996 stars. ...
Fifth Fundamental Catalogue is a glossary of positions of stars. ...
The Hipparcos and Tycho Catalogues (Tycho-1) are the primary products of the European Space Agencys astrometric mission, Hipparcos. ...
This article is about the star grouping. ...
Carina (IPA: , Latin: ) is a southern constellation which forms part of the old constellation of Argo Navis. ...
Bright stars can be bright because they produce more light, because they are closer to us, or both. ...
The apparent magnitude (m) of a star, planet or other celestial body is a measure of its apparent brightness as seen by an observer on Earth. ...
In astronomy, an asterism is a pattern of stars seen in Earths sky which is not an official constellation. ...
The Diamond Cross is an asterism in the south polar constellation Carina. ...
Beta Carinae's traditional name Miaplacidus made its debut on star maps in 1856 when the star atlas Geography of the Heavens, composed by Elijah Hinsdale Burritt, was published. The meaning and lingusitic origin of the name remained an enigma for many decades, until William Higgins, a great scholar and expert on star names, surmised that the name Miaplacidus is apparently a bilingual combination of Arabic مياه miyāh for "waters" and Latin placidus for "placid". Arabic redirects here. ...
For other uses, see Latins and Latin (disambiguation). ...
References
Year 2005 (MMV) was a common year starting on Saturday (link displays full calendar) of the Gregorian calendar. ...
is the 309th day of the year (310th in leap years) in the Gregorian calendar. ...
External links Year 2005 (MMV) was a common year starting on Saturday (link displays full calendar) of the Gregorian calendar. ...
Year 2005 (MMV) was a common year starting on Saturday (link displays full calendar) of the Gregorian calendar. ...
Year 2005 (MMV) was a common year starting on Saturday (link displays full calendar) of the Gregorian calendar. ...
Miaplacidus (placid waters) is one of the brightest stars in Earths night sky, with apparent magnitude 1. ...
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