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Encyclopedia > Zeta Orionis
Zeta Orionis Aa/Ab/B
Observation data
Epoch J2000
Constellation Orion
Right ascension 05h 40m 45.5s
Declination -01° 56′ 34″
Apparent magnitude (V) 1.74/~4/4.2
Characteristics
Spectral type O9.7 Ibe/O/B2 IV
B-V color index -0.21
U-B color index -1.07
Variable type  ?
Astrometry
Radial velocity (Rv) 18 km/s
Proper motion (μ) RA: 3.99 mas/yr
Dec.: 2.54 mas/yr
Parallax (π) 3.99 ± 0.79 mas
Distance 817 ly (251 pc)
Absolute magnitude (MV) -5.25/-3/-2.8
Visual binary orbit
Companion Zeta Orionis B
Period (P) 1,500 years
Semimajor axis (a) 2.728"
Eccentricity (e) 0.07
Inclination (i) 72.0°
Node (Ω) 155.5°
Periastron epoch (T) 2070.6
Details
Mass 28/23/? M
Radius 20/? R
Luminosity 100,000/1,300/? L
Temperature 31,000/? K
Metallicity  ?
Rotation 140 km/sec./?
Age  ? years
Other designations
Alnitak, Al Nitak, 50 Ori, HR 1948/9, BD -02°1338, HD 37742, SAO 132444, HIP 26727.

Zeta Orionis is a star in the constellation Orion. It also has the traditional name Alnitak. The name is taken from the Arabic an-nitaq, “the belt”. In astronomy, an epoch is a moment in time for which celestial coordinates or orbital elements are specified. ... Orion is a remarkable constellation, visible from most places on the globe (but not always the whole year long). ... Orion is a proper name used in many different ways: Orion the hunter, from Greek mythology Orion the constellation Orion the spiral arm in the Milky Way Orion Nebula also known as M42 Orion, a commune in the Pyrénées-Atlantiques département in France Orion, a municipality in... Right ascension (RA; symbol α: Greek letter alpha; celestial longitude) is the astronomical term for one of the two coordinates of a point on the celestial sphere when using the equatorial coordinate system. ... In astronomy, declination (dec) is one of the two coordinates of the equatorial coordinate system, the other being either right ascension or hour angle. ... The apparent magnitude (m) of a star, planet or other heavenly body is a measure of its apparent brightness; that is, the amount of light received from the object. ... 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. ... Shanil Davendra Singh rules 4 life! ... Shanil Davendra Singh rules 4 life! ... Most stars are of nearly constant luminosity. ... Astrometry is a part of astronomy and deals with the positions of stars and other celestial bodies, their distances and movements. ... 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 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 is the time between two recurrences of an event related to the orbit of the Earth around the Sun. ... Parallax (Greek: παραλλαγή (parallagé) = alteration) is the change of angular position of two stationary points relative to each other as seen by an observer, due to the motion of said observer. ... A milliarcsecond (m, mas) , or a thoundsanth of an arcsecond. ... Proximity (2001) is also a movie with Rob Lowe, Fred Ward and James Coburn. ... A light year, abbreviated ly, is the distance light travels in one year: roughly 9. ... The parsec (symbol pc) is a unit of length used in astronomy. ... In astronomy, absolute magnitude is the apparent magnitude, m, an object would have if it were at a standardized distance away. ... A binary star system consists of two stars both orbiting around their barycenter. ... The orbital period is the time it takes a planet (or another object) to make one full orbit. ... 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 is one of the six orbital parameters describing the shape and orientation of a celestial orbit and is the angular distance of the orbital plane from the plane of the reference (usually planets equator or the ecliptic), stated in degrees. ... An orbital node is one of the two points where an inclined orbit crosses a plane of reference (e. ... 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. ... Mass is a property of physical objects that, roughly speaking, measures the amount of matter they contain. ... In astronomy, the solar mass is a unit of mass used to express the mass of stars and larger objects such as galaxies. ... In classical geometry, a radius of a circle or sphere is any line segment with one endpoint on the circle (i. ... 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. ... Temperature is the physical property of a system which underlies the common notions of hot and cold; the material with the higher temperature is said to be hotter. ... The kelvin (symbol: K) is the SI unit of temperature, and is one of the seven SI base units. ... In astronomy, the metallicity of an object is the proportion of its matter made up of chemical elements other than hydrogen and helium. ... Rotation of a planar figure around a point Rotation of a planar body is the movement when points of the body travel in circular trajectories around a fixed point called the center of rotation. ... The Pleiades star cluster A star is a massive body of plasma in outer space that is currently producing or has produced energy through nuclear fusion. ... A year is the time between two recurrences of an event related to the orbit of the Earth around the Sun. ... 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. ... The Smithsonian Astrophysical Observatory (SAO) is a research institute of the Smithsonian Institution headquartered in Cambridge, Massachusetts, where it is joined with the Harvard College Observatory (HCO) to form the Harvard-Smithsonian Center for Astrophysics (CfA). ... In astronomy, many stars are referred to simply by catalogue numbers. ... The Pleiades star cluster A star is a massive body of plasma in outer space that is currently producing or has produced energy through nuclear fusion. ... Orion is a remarkable constellation, visible from most places on the globe (but not always the whole year long). ... Orion, a constellation often referred to as The Hunter, is a prominent constellation, perhaps the best-known in the sky. ...


Alnitak is a triple star system at the eastern end of Orion's belt. The primary is a blue supergiant that is also a close binary. The Alnitak system is bathed in the nebulosity of IC 434. A triple star system consists of three gravitationally bound stars. ... Orion, a constellation often referred to as The Hunter, is a prominent constellation, perhaps the best-known in the sky. ... Supergiants are the most massive stars. ... IC 434, the Horsehead Nebula. ...


References

  • C. A. Hummel et al, "ζ Orionis A is a Double Star", The Astrophysical Journal, volume 540, 2, 2000.

External links


  Results from FactBites:
 
Zeta Orionis - Wikipedia, the free encyclopedia (148 words)
Zeta Orionis is a star in the constellation Orion.
The Alnitak system is bathed in the nebulosity of IC 434.
Hummel et al, "ζ Orionis A is a Double Star", The Astrophysical Journal, volume 540, 2, 2000.
  More results at FactBites »


 

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