Alpha Ursae Majoris A/B/C Observation data Epoch J2000 | | Constellation | Ursa Major | | Right ascension | 11h 03m 43.7s | | Declination | +61° 45′ 03″ | | Apparent magnitude (V) | 1.79 (1.87/4.81/7.12) | | Characteristics | | Spectral type | K0 III / F0 V / F8 | | U-B color index | 0.92 | | B-V color index | 1.07 | | Variable type | Pulsating | | Astrometry | | Radial velocity (Rv) | −9 km/s | | Proper motion (μ) | RA: −136.46 mas/yr Dec.: −35.25 mas/yr | | Parallax (π) | 26.38 ± 0.53 mas | | Distance | 124 ± 2 ly (37.9 ± 0.8 pc) | | Absolute magnitude (MV) | −1.09/1.83/4.22 | | Visual binary orbit | | Companion | α UMa B | | Period (P) | 44.4 yr | | Semimajor axis (a) | 0.603" | | Eccentricity (e) | 0.4 | | Inclination (i) | 152° | | Longitude of the node (Ω) | 2000° | | Periastron epoch (T) | 1956.8 | | Details | | Mass | 4/1.7 M☉ | | Radius | 16/1.3 R☉ | | Luminosity | 300 L☉ | | Temperature | 4,500/7,400 K | | Metallicity | ? | | Rotation | <17 km/s. | | Age | ? years | | Other designations | Dubhe, Dubb, Ak, 50 UMa, HR 4301, BD +62°1161, HD 95689, SAO 15384, FK5 417, GC 15185, ADS 8035, CCDM 11037+6145, HIP 54061. | | Database references | | SIMBAD | data | Alpha Ursae Majoris (α UMa / α Ursae Majoris) is the second-brightest star in the constellation of Ursa Major (despite its Bayer designation of "alpha"). It also has the traditional name Dubhe. In astronomy, an epoch is a moment in time for which celestial coordinates or orbital elements are specified. ...
This article or section does not adequately cite its references or sources. ...
Ursa Major (IPA: ) is a constellation visible throughout the year in most of the northern hemisphere. ...
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. ...
Most stars are of almost constant luminosity. ...
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. ...
This does not adequately cite its references or sources. ...
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. ...
Artists impression of a binary system consisting of a black hole, with an accretion disc around it, and a main sequence star. ...
The orbital period is the time it takes a planet (or another object) to make one full orbit. ...
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. ...
In geometry, the semi-major axis (also semimajor axis) a applies to ellipses and hyperbolas. ...
In astrodynamics, under standard assumptions any orbit must be of conic section shape. ...
Inclination in general is the angle between a reference plane and another plane or axis of direction. ...
It has been suggested that this article or section be merged into Orbital node. ...
This article is about several astronomical terms (apogee & perigee, aphelion & perihelion, generic equivalents based on apsis, and related but rarer terms. ...
In astronomy, an epoch is a moment in time for which celestial coordinates or orbital elements are specified. ...
This article or section is in need of attention from an expert on the subject. ...
In astronomy, the solar mass is a unit of mass used to express the mass of stars and larger objects such as galaxies. ...
Remote Authentication Dial In User Service (RADIUS) is an AAA (authentication, authorization and accounting) protocol for applications such as network access or IP mobility. ...
In astronomy, the solar radius is a unit of length used to express the size of stars and larger objects such as galaxies. ...
Luminosity has different meanings in several different fields of science. ...
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. ...
This article includes a list of works cited or a list of external links, but its sources remain unclear because it lacks in-text citations. ...
The kelvin (symbol: K) is a unit increment of temperature and is one of the seven SI base units. ...
The globular cluster M80. ...
This illustration shows the oblate appearance of the star Achernar caused by rapid rotation. ...
STAR is an acronym for: Organizations Society of Ticket Agents and Retailers], the self-regulatory body for the entertainment ticket industry in the UK. Society for Telescopy, Astronomy, and Radio, a non-profit New Jersey astronomy club. ...
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. ...
The Henry Draper Catalogue is an astronomy catalogue with astrometric and spectroscopic data about more than 225,000 stars. ...
Smithsonian Astrophysical Observatory Star Catalog contain the 258,996 stars. ...
The Hipparcos and Tycho Catalogues (Tycho-1) are the primary products of the European Space Agencys astrometric mission, Hipparcos. ...
SIMBAD (the Set of Identifications, Measurements, and Bibliography for Astronomical Data) is a database of astronomical information about objects within the Milky Way. ...
STAR is an acronym for: Organizations Society of Ticket Agents and Retailers], the self-regulatory body for the entertainment ticket industry in the UK. Society for Telescopy, Astronomy, and Radio, a non-profit New Jersey astronomy club. ...
This article or section does not adequately cite its references or sources. ...
Ursa Major (IPA: ) is a constellation visible throughout the year in most of the northern hemisphere. ...
This article or section is not written in the formal tone expected of an encyclopedia article. ...
It forms part of the Big Dipper (also known as the Plough), and is the northern of the pointers, the two stars of Ursa Major which point towards Polaris. However, it is not part of the Ursa Major moving group. Instead, it is an evolved helium-burning star, about 124 light years away. It is a multiple star, orbited by a main sequence companion, Dubhe B, at a distance of about 23 astronomical units (AU), as well as a close pair, Dubhe C, at a distance of about 8000 AU. Big Dipper map A group of the brightest stars of the constellation Ursa Major, the Great Bear, form a well-known asterism that has been recognized as a distinct grouping in many cultures from time immemorial. ...
Polaris (α UMi / α Ursae Minoris / Alpha Ursae Minoris), more commonly known as The North Star or simply North Star, is the brightest star in the constellation Ursa Minor. ...
The Ursa Major Moving Group is the closest moving group to Earth, with its core being located roughly 80 light years away. ...
General Name, Symbol, Number helium, He, 2 Chemical series noble gases Group, Period, Block 18, 1, s Appearance colorless Standard atomic weight 4. ...
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 multiple star consists of three or more stars which appear from the Earth to be close to one another. ...
Hertzsprung-Russell diagram The main sequence of the Hertzsprung-Russell diagram is the curve where the majority of stars are located in this diagram. ...
The astronomical unit (AU or au or a. ...
Artists impression of a binary system consisting of a black hole, with an accretion disc around it, and a main sequence star. ...
The traditional name comes from the Arabic for "bear", dubb, from the phrase ظهر الدب الاكبر żahr ad-dubb al-akbar "the back of the Greater Bear". It is known as 北斗一 (the First Star of the Northern Dipper) or 天樞 (the Celestial Pivot) in Chinese. |