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Encyclopedia > Delta Velorum
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δ Velorum
Epoch J2000.0
Constellation Vela
Right ascension 08h 44m 42.2s
Declination −54° 42' 30"
Distance 79.7 ± 0.7 ly (24.4 ± 0.2 pc)
Spectral type A1V
Apparent magnitude +1.93
Other designations
Gl 321.3, HR 3485,
HD 74956, CP-54 1788,
HIP 42913, SAO 236232,
GC 12069, CCDM 08448-5442

Delta Velorum (δ Vel / δ Velorum) is a star system in the constellation Vela. It is approximately 79.7 light years from Earth. In astronomy, an epoch is a moment in time for which celestial coordinates or orbital elements are specified. ... Jump to: navigation, search The J2000. ... Jump to: navigation, search Orion is a remarkable constellation, visible from most places on the globe (but not always the whole year long). ... Categories: Astronomy stubs | Modern constellations | Constellations | Vela constellation | Argo Navis constellation ... 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. ... A light year, abbreviated ly, is the distance light travels in one year: roughly 9. ... Jump to: navigation, search The parsec (symbol pc) is a unit of length used in astronomy. ... In astronomy, stellar classification is a classification of stars based initially on photospheric temperature and its associated spectral characteristics, and subsequenly refined in terms of other characteristics. ... 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, 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. ... In astronomy, many stars are referred to simply by catalogue numbers. ... In astronomy, many stars are referred to simply by catalogue numbers. ... A star system or stellar system is a group of stars (and possibly smaller bodies such as planets or asteroids) that orbit one another (systems with planetary bodies orbiting stars, are referred to as solar systems or planetary systems). ... Jump to: navigation, search Orion is a remarkable constellation, visible from most places on the globe (but not always the whole year long). ... Categories: Astronomy stubs | Modern constellations | Constellations | Vela constellation | Argo Navis constellation ... A light year, abbreviated ly, is the distance light travels in one year: roughly 9. ... Jump to: navigation, search Earth, also known as the Earth, Terra, and (mostly in the 19th century) Tellus, is the third-closest planet to the Sun. ...


The system is composed of two binary stars. The brightest of the four stars, δ Velorum A, is a white A-type main sequence dwarf with an apparent magnitude of +2.02. Its binary companion, δ Velorum B, has a magnitude of +5.1 and is separated from the A component by 2.6 arcseconds. A binary star system consists of two stars both orbiting around their barycenter. ... In astronomy, stellar classification is a classification of stars based initially on photospheric temperature and its associated spectral characteristics, and subsequenly refined in terms of other characteristics. ... 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 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. ... A second of arc or arcsecond is a unit of angular measurement which comprises one-sixtieth of an arcminute, or 1/3600 of a degree of arc or 1/1296000 ≈ 7. ...


The second binary system is 69 arcseconds away. It is composed of the 11th magnitude δ Velorum C and the 13th magnitude δ Velorum D, which are 6 arcseconds apart. A second of arc or arcsecond is a unit of angular measurement which comprises one-sixtieth of an arcminute, or 1/3600 of a degree of arc or 1/1296000 ≈ 7. ... A second of arc or arcsecond is a unit of angular measurement which comprises one-sixtieth of an arcminute, or 1/3600 of a degree of arc or 1/1296000 ≈ 7. ...


This star was recently discovered to be variable by the Galileo spaceprobe at Jupiter.[1] It fluctuates by about 30% every 45 days. Curiously, being one of the brighter stars in the sky, this had not been noticed previously. Galileo is prepared for mating with the IUS booster Galileo being deployed after being launched by the Space Shuttle Atlantis on the STS-34 mission Galileo was an unmanned spacecraft sent by NASA to study the planet Jupiter and its moons. ... Jump to: navigation, search Adjective Jovian Atmospheric characteristics Atmospheric pressure 70 kPa Hydrogen ~86% Helium ~14% Methane 0. ...


Because of precession, δ Velorum will be the South Polar Star around 9000 AD. Jump to: navigation, search There are two types of precession, torque-free and torque-induced, the latter being discussed here in more detail. ...


  Results from FactBites:
 
Delta Scuti star (237 words)
Delta Scuti stars are Population I objects of spectral type A0 to F5 and lie in the lower part of the instability strip, either on the main sequence or among the subgiants and giants.
The prototype of the class, Delta Scuti itself, is a widespread triple system at a distance of 187 light-years.
Delta Scuti A (spectral class F2, visual magnitude 4.71, luminosity 33 times that of the Sun, mass 2.3 solar masses) has two main periods of 4.65 and 4.48 hours with others of 2.79, 2.28, 2.89, and 20.11 hours; its overall change in luminosity is only 0.2 magnitudes.
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