Sirius: Difference between revisions
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'''Sirius''' (α Canis Majoris) is the brightest star visible from Earth other than the Sun (Sol). Sirius (Right Ascension 6h 45m 8.7s, declination -16°43’03”) is sometimes called the "Dog Star" because it is located in the southern constellation [[Canis Major]] (Larger Dog). As is true of almost all stars Sirius is not visible during all seasons. In the Northern Hemisphere it is most easily viewed in the winter in early evening.<ref name="Comins">{{Cite book | |||
'''Sirius''' (α Canis Majoris) is the brightest star visible from Earth other than the Sun (Sol). Sirius is sometimes called the "Dog Star" because it is located in the southern constellation Canis Major | |||
| publisher = W. H. Freeman | | publisher = W. H. Freeman | ||
| isbn = 9781429217972 | | isbn = 9781429217972 | ||
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Sirius is the seventh nearest star to Earth at a distance of 8. | Sirius is the seventh nearest star to Earth at a distance of 8.61 light years, according to the latest measurements of the Hipparcos satellite. Sirius is a binary star system consisting of Sirius A (spectral class A1 V, absolute visual magnitude +1.47) and Sirius B (spectral class B0wd, absolute visual magnitude +8.44). This means Sirius has a much brighter absolute visual magnitude than the Sun (absolute visual magnitude +4.85). In fact Sirius is approximately 23.2 times more luminous than the Sun. Luminosity, which is mathematically related to absolute visual magnitude, is the actual amount of light put out by an object. Both Sirius's luminosity and its nearness to Earth contribute to it being the brightest star in the night sky.<ref name="Comins" /> | ||
Other than its brightness and location, Sirius is noteworthy as the first discovered instance of a “white dwarf” star (Sirius B), an extremely hot, small and dense stellar remnant. Although an orbiting companion of Sirius | |||
Other than its brightness and location, Sirius is noteworthy as the first discovered instance of a “white dwarf” star (Sirius B), an extremely hot, small and dense stellar remnant. Although German astronomer Friedrich Bessel suspected an orbiting companion of Sirius as early as 1844, due to a slight, gravitationally induced and very regular “wobble” in Sirius’ proper motion the the presence of Sirius B was not confirmed until 1862. While conducting star-tests of the 18.5-inch Dearborn refracting telescope on January 31, 1862, American telescope maker Alvan Graham Clark noted a very small star close to Sirius that had not been previously noted. Further observations confirmed Sirius B’s binary nature in an orbit with a period of about 50 years and at a distance from Sirius A of about 20 astronomical units which are equivalent to 3 billion kilometers.<ref>{{Citation | |||
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| first =Gary, L. | | first =Gary, L. | ||
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==References== | ==References== | ||
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Latest revision as of 03:24, 7 October 2013
Sirius (α Canis Majoris) is the brightest star visible from Earth other than the Sun (Sol). Sirius (Right Ascension 6h 45m 8.7s, declination -16°43’03”) is sometimes called the "Dog Star" because it is located in the southern constellation Canis Major (Larger Dog). As is true of almost all stars Sirius is not visible during all seasons. In the Northern Hemisphere it is most easily viewed in the winter in early evening.[1]
Sirius is the seventh nearest star to Earth at a distance of 8.61 light years, according to the latest measurements of the Hipparcos satellite. Sirius is a binary star system consisting of Sirius A (spectral class A1 V, absolute visual magnitude +1.47) and Sirius B (spectral class B0wd, absolute visual magnitude +8.44). This means Sirius has a much brighter absolute visual magnitude than the Sun (absolute visual magnitude +4.85). In fact Sirius is approximately 23.2 times more luminous than the Sun. Luminosity, which is mathematically related to absolute visual magnitude, is the actual amount of light put out by an object. Both Sirius's luminosity and its nearness to Earth contribute to it being the brightest star in the night sky.[1]
Other than its brightness and location, Sirius is noteworthy as the first discovered instance of a “white dwarf” star (Sirius B), an extremely hot, small and dense stellar remnant. Although German astronomer Friedrich Bessel suspected an orbiting companion of Sirius as early as 1844, due to a slight, gravitationally induced and very regular “wobble” in Sirius’ proper motion the the presence of Sirius B was not confirmed until 1862. While conducting star-tests of the 18.5-inch Dearborn refracting telescope on January 31, 1862, American telescope maker Alvan Graham Clark noted a very small star close to Sirius that had not been previously noted. Further observations confirmed Sirius B’s binary nature in an orbit with a period of about 50 years and at a distance from Sirius A of about 20 astronomical units which are equivalent to 3 billion kilometers.[2]
References
- ↑ 1.0 1.1 Comins, Neil F. (2008-12-15). Discovering the Essential Universe. W. H. Freeman. ISBN 9781429217972.
- ↑ Cameron, Gary, L. (2007), "Clark Family", in Hockey, Thomas et al, The biographical encyclopedia of astronomers, vol. 1, A-L, New York: Springer Science+Business Media, LLC