Kapteyn's Star Observation data Epoch J2000 | Constellation (pronunciation) | Pictor | | Right ascension | 05h 11m 40.6s | | Declination | -45° 01' 06" | | Apparent magnitude (V) | 8.85 | | Characteristics | | Spectral type | sdM1 V | | U-B color index | 1.15 | | B-V color index | 1.56 | | Variable type | Unknown | | Astrometry | | Radial velocity (Rv) | +245.5 km/s | | Proper motion (μ) | RA: 6506.05 mas/yr Dec.: -5731.39 mas/yr | | Parallax (π) | 255.27 ± 0.86 mas | | Distance | 12.78 ± 0.04 ly (3.92 ± 0.01 pc) | | Absolute magnitude (MV) | 10.88 | | Details | | Mass | 0.38 M☉ | | Radius | 0.24 R☉ | | Luminosity | 0.004 L☉ | | Temperature | 3,800 K | | Metallicity | 32% | | Age | ? years | | Other designations | VZ Pictoris, GJ 191, HD 33793, CD-45°1841, CP(D)-44°612, SAO 217223, LHS 29, LTT 2200, LFT 395, CD GCTP 1181, UGPMF 628, HIP 24186. | Kapteyn's Star (also known as GJ 191, HD 33793 or CD -45 1841) is a class M0 subdwarf discovered by Jacobus Kapteyn in 1897. It is 12.79 light years from Earth's Solar System, and is distinctive in a number of regards; it has a high radial velocity, orbits the Milky Way retrograde, and is the nearest halo star to the Sun. 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. ...
Pictor (IPA: , Latin: ) is one of the minor southern (declination -50° to -60°) constellations. ...
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. ...
This article or section contains a plot summary that is overly long or excessively detailed. ...
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. ...
This article is about an authentication, authorization, and accounting protocol. ...
In astronomy, the solar radius is a unit of length used to express the size of stars and larger objects such as galaxies. ...
This article does not cite any references or sources. ...
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 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. ...
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. ...
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. ...
In astronomy, many stars are referred to simply by catalogue numbers. ...
In astronomy, many stars are referred to simply by catalogue numbers. ...
The Hipparcos and Tycho Catalogues (Tycho-1) are the primary products of the European Space Agencys astrometric mission, Hipparcos. ...
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. ...
A subdwarf star, sometimes denoted by sd, is luminosity class VI under the Yerkes spectral classification system. ...
Jacobus Cornelius Kapteyn, (January 19, 1851 â June 18, 1922) was a Dutch astronomer, best known for his extensive studies of the Milky Way and as the first discoverer of evidence for galactic rotation. ...
1897 (MDCCCXCVII) was a common year starting on Friday (see link for calendar). ...
A light-year or lightyear (symbol: ly) is a unit of measurement of length, specifically the distance light travels in vacuum in one year. ...
This article is about Earth as a planet. ...
This article is about the Solar System. ...
For other uses, see Milky Way (disambiguation). ...
This article is about retrograde motion. ...
The galactic halo is a region of space surrounding spiral galaxies, including our galaxy, the Milky Way. ...
When discovered, it had the highest proper motion of any star known, dethroning Groombridge 1830. Later it dropped to second place after the discovery of Barnard's Star. 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...
Groombridge 1830 is a star. ...
Barnards Star is a very low-mass star in the constellation Ophiuchus which was discovered by the astronomer E. E. Barnard in 1916. ...
See also
The planetary systems of stars other than the Sun and its Solar System are a staple element in much science fiction. ...
This list of the nearest stars to Earth is ordered by increasing distance out to a maximum of 5 parsecs (16. ...
External links - SolStation.com: Kapteyn's Star
Discovery announced - "Stern mit grösster bislang bekannter Eigenbewegung", AN 145 (1898) 159/160 (in German)
|