Beta Pavonis estimated radius has been calculated as being 4.24 times bigger than the Sun. More Memory Beta, non-canon Star Trek Wiki. [8], Delta Pavonis has been identified by Maggie Turnbull and Jill Tarter of the SETI Institute as the "Best SETI target" among the 100 closest G-type stars. 45, 153 (, J.C. Cooper (Thames & Hudson 1987) An Illustrated Encyclopaedia of Traditional Symbols Paperback, p. 127 (, Ian Ridpath (James Clark & Co. 1988) Star Tales, p. 99 (, "A Photometric Study of the Eclipsing Symbiotic Binary AR Pavonis", Monthly Notices of the Royal Astronomical Society. [8], Monthly Notices of the Royal Astronomical Society, "Kinematic structure of the corona of the Ursa Major flow found using proper motions and radial velocities of single stars", https://en.wikipedia.org/w/index.php?title=Beta_Pavonis&oldid=950949056, Creative Commons Attribution-ShareAlike License, This page was last edited on 14 April 2020, at 18:08. β Pavonis (beta Pavonis) β Pavonis is a giant star in the constellation of Pavo. -0.046 arcsec per year in Right Ascension and 0.012 arcsec per year in Declination and the associated displacement Covering 378 square degrees, it ranks 44th of the 88 modern constellations in size and covers 0.916% of the night sky. G6V white star Based upon an annual parallax shift of 24.14 mas as seen from Earth, it is located 135 light years from the Sun. U.G. However with the 2007 release of updated Hipparcos files, the radius is now calculated at being round 4.16. [13], The Wardaman people of the Northern Territory in Australia saw the stars of Pavo and the neighbouring constellation Ara as flying foxes. Beta Pavonis is a popular song by Michael Garfield | Create your own TikTok videos with the Beta Pavonis song and explore 0 videos made by new and popular creators. Pavo is the radiant of two annual meteor showers: the Delta Pavonids and August Pavonids. The star's Galacto-Centric Distance is 7,371.00 Parsecs or 24,041.50 Light Years. Super-Earth and Neptune-mass Planets in Multiple Planet Systems HD 47186 and HD 181433", "Extrasolar Planets around HD 196050, HD 216437 and HD 160691", "The HARPS Search for Southern Extra-solar Planets XXI. Based on the spectral type (A5IV) of the star, the star's colour is blue - white . It is purely that the distance was recalculated. (ST references: Star Charts, The Worlds of the Federation). image of Delta Pavonis at the NASA Star and Exoplanet Database.) The constellation contains NGC 6752, the third-brightest globular cluster in the sky, and the spiral galaxy NGC 6744, which closely resembles the Milky Way but is twice as large. System Summary. However, Houk (1979) listed a more evolved class of A7 III,[4] suggesting it is already a giant star. [32] The galactic wind bearing NGC 6810 and the interacting NGC 6872/IC 4970 galaxies lie 87 and 212 million light-years away from Earth respectively. Location: Your guide to the Solar System and the night sky. in the constellation of [9], The peacock and the "Argus" nomenclature are also prominent in a different myth, in which Io, a beautiful princess of Argos, was lusted after by Zeus (Jupiter). In TNG video game: Birth of the Federation, the orbital configuration of the game map star systems was randomly generated each time a new game started. XVII. [10], Zorec and Royer (2012) list a stellar classification for this star of A5 IV,[3] indicating it is an evolving subgiant star that has consumed the hydrogen at its core and has begun to expand onto the red giant branch. French explorer and astronomer Nicolas-Louis de Lacaille labelled them Alpha to Omega in 1756, but omitted Psi and Xi, and labelled two pairs of stars close together Mu and Phi Pavonis. Our own Sun is the brightest star and therefore has the lowest of all magnitudes, -26.74. A name is preferred even if its a random made up one by yourself. situated south of the celestial equator, as such, it is more easily visible from the southern emisphere. The brightest star in the constellation is normally given the Alpha designation, there are exceptions such as Pollux which is Beta Geminorum. The Radial Velocity, that is the speed at which the star is moving away/towards the Sun is 3.70000 km/s with an error of about 0.50 km/s . Based on the star's spectral type of A5IV , Beta Pavonis's colour and type is blue - white subgiant star. [24] East of Beta and at the constellation's eastern border with Indus is Gamma Pavonis, a fainter, solar-type star 30 light years from Earth with a magnitude of 4.22 and stellar class F9V. Magnitude, whether it be apparent/visual or absolute magnitude is measured by a number, the smaller the number, the brighter the Star is. Celestial coordinates for the J2000 equinox as well as galactic coordinates of β Pavonis are provided in the following table: The simplified sky map below shows the position of β Pavonis in the sky: Location: Greenwich, United Kingdom [change] BETA PAV (Beta Pavonis). Pavo constellation French explorer and astronomer Nicolas-Louis de Lacaille gave its stars Bayer designations in 1756.
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