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Encyclopedia > Beta Pictoris
Beta Pictoris
Observation data
Epoch J2000
Constellation Pictor
Right ascension 05h 47m 17.1s
Declination -51° 03′ 59″
Apparent magnitude (V) 3.86
Characteristics
Spectral type A5 V
B-V color index 0.17
U-B color index 0.09
Variable type None
Astrometry
Radial velocity (Rv) +20 km/s
Proper motion (μ) RA: 4.65 mas/yr
Dec.: 81.96 mas/yr
Parallax (π) 51.87 ± 0.51 mas
Distance 62.9 ly (19.3 pc)
Absolute magnitude (MV) 2.44
Details
Mass 1.7 M
Radius 1.4 R
Luminosity 8.6 L
Temperature 8,250 K
Metallicity 100%
Rotation 13 hours (130 km/s.)
Age 8-20 × 106 years
Other designations
GJ 219.0, HR 2020, CD -51°1620, HD 39060, GCTP 1339.00, SAO 234134, HIP 27321.

Beta Pictoris (β Pic / β Pictoris) is the second brightest star in the constellation Pictor. 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 at one time or another during the year. ... Pictor, being Latin for easel, is one of the minor southern (declination -50 to -60) constellations. ... Right ascension (RA; symbol α: Greek letter alpha) 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. ... // Headline text HEY!! HOW ARE YOU ALL?? Its nice of you to come read this page. ... 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 almost constant luminosity. ... This article does not cite its references or sources. ... 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 an observer. ... A milliarcsecond (m, mas) , or a thoundsanth of an arcsecond. ... The distance between two points is the length of a straight line segment between them. ... 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 standard luminosity distance away from us. ... Mass is a property of a physical object that quantifies the amount of matter and energy it contains. ... 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 from its center to its boundary. ... 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 also the name of a song by Sean Paul. ... 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 plane, seen as the rotation of the terrain relative to the plane (exposure time 1. ... 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. ... 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. ... 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 at one time or another during the year. ... Pictor, being Latin for easel, is one of the minor southern (declination -50 to -60) constellations. ...


The star β Pictoris shows an excess of infrared emission compared to normal stars of its type. This excess comes from dust near the star. Detailed observations reveal a large disk of dust and gas orbiting the star, considered to be a type of protoplanetary disk called a debris disk. The β Pic system is very young, only 8-20 million years old. [1] New studies using a NASA ultraviolet space telescope called FUSE have discovered that this disk contains a surprising overabundance of carbon gas. Currently, the two suggested explanations for this are 1) β Pic might be in the process of forming exotic carbon-rich worlds, in contrast to the oxygen-rich Earth, or 2) it is passing through an unknown phase that might also have occurred early in the development of our solar system. [2] A protoplanetary disc (also protoplanetary disk, proplyd) is an accretion disc surrounding a T Tauri star. ... A year is the time between two recurrences of an event related to the orbit of the Earth around the Sun. ... This article or section does not cite its references or sources. ... Look up Fuse on Wiktionary, the free dictionary The word fuse has several meanings: To fuse is to combine in a process of fusion. ... General Name, Symbol, Number carbon, C, 6 Chemical series nonmetals Group, Period, Block 14, 2, p Appearance black (graphite) colorless (diamond) Atomic mass 12. ... General Name, Symbol, Number carbon, C, 6 Chemical series nonmetals Group, Period, Block 14, 2, p Appearance black (graphite) colorless (diamond) Atomic mass 12. ... General Name, Symbol, Number oxygen, O, 8 Chemical series Nonmetals, chalcogens Group, Period, Block 16, 2, p Appearance colorless Atomic mass 15. ... Earth (often referred to as The Earth) is the third planet in the solar system in terms of distance from the Sun, and the fifth in order of size. ... The solar system comprises the Earths Sun and the retinue of celestial objects gravitationally bound to it. ...


The star-system's disk extends more than 500 AUs away from β Pictoris, and shows a warp-like shape in the inner region. This suggests the presence of a massive object, perhaps a brown dwarf or a gas giant planet, orbiting the star and causing the disk's odd shape; however, the existence of this object has not yet been confirmed. [3] The astronomical unit (AU or au or a. ... This brown dwarf (smaller object) orbits the star Gliese 229, which is located in the constellation Lepus about 19 light years from Earth. ... A planet is generally considered to be a relatively large mass of accreted matter in orbit around a star. ...


External links


  Results from FactBites:
 
Beta Pictoris - Wikipedia, the free encyclopedia (276 words)
Beta Pictoris (β Pic / β Pictoris) is the second brightest star in the constellation Pictor.
Currently, the two suggested explanations for this are 1) β Pic might be in the process of forming exotic carbon-rich worlds, in contrast to the oxygen-rich Earth, or 2) it is passing through an unknown phase that might also have occurred early in the development of our solar system.
This suggests the presence of a massive object, perhaps a brown dwarf or a gas giant planet, orbiting the star and causing the disk's odd shape; however, the existence of this object has not yet been confirmed.
Beta Pictoris (469 words)
However, this is almost certainly not the case since Beta Pictoris is a main sequence star with an age of approximately 100 million years.
The dust presently in its disk has a life-time of the order of 100 thousand years, and therefore must undergo continuous replenishment (see regenerated disk).
This might be due to a brown dwarf in a wide orbit around Beta Pictoris or the nearby passage of another star.
  More results at FactBites »


 

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