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31 December 2009
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Deneb Yıldızı
Deneb, Kuğu Takımyıldızı'nda yer alan en parlak yıldız.
Deneb'in kütlesi, Güneş'in kütlesinin 25 katı ve çapı Güneş'in çapının 200 katıdır. Güneş'ten 265.000 kat parlak olan Deneb, son derece parlak, beyaz renkte bir dev yıldızdır.
Deneb, 1.25 görünür büyüklüğüyle gökyüzünün en parlak 19. yıldızıdır. Aynı zamanda, Samanyolu'daki en parlak yıldızlardan biridir. Kuğu Takımyıldızı'nda yer alan Deneb, Lir Takımyıldızı'ndaki Vega ve Kartal Takımyıldızı'ndaki Altair'le birlikte yaz üçgeninin köşelerini oluşturan yıldızlardan biridir. Adı Arapça "kuyruk" anlamına gelen Deneb, Kuğu'nun kuyruğunda yer almaktadır. En iyi görüldüğü zamanlar, Kuğu Takımyıldızı'nın Eylül ayı başlarında akşam göğünde en yüksek konumu aldığı günlerdir.
Deneb, Samanyolu'nun en büyük yıldızlarından biridir; eğer Güneş'in yerinde olsaydı, yıldızın yuvarlağı Dünya'nın yörüngesini içine alırdı. Deneb'in kütlesi, Güneş'in kütlesinin 25 katı ve çapı Güneş'in çapının 200 katıdır. Güneş'ten 265.000 kat parlak olan Deneb, son derece parlak, beyaz renkte bir dev yıldızdır. Spektrum türü A olan beyaz yıldızlar, evrendeki yıldızların yaklaşık %1'ini oluştururlar. Deneb benzeri dev yıldızların parlaklıkları, Güneş'ten ortalama 10.000 kat, kütleleri 10 ile 100 kat, çapları ise 20 ile 1.000 daha fazladır. Bunlar, hemen her spektrum türünde olabilen genç yıldızlardır (Rigel, Betelgeuse, Canopus, Antares gibi).
Deneb'in bizden çok uzakta olmasından ötürü, yıldızın gerçek parlaklığı ve evrimsel durumu kesin olarak bilinmemektedir. Ancak, önümüzdeki birkaç milyon yl içinde patlayacağı neredeyse kesindir.
Deneb (α Cyg / α Cygni / Alpha Cygni) is the brightest star in the constellation Cygnus and one of the vertices of the Summer Triangle. It is the 19th brightest star in the night sky, with an apparent magnitude of 1.25. A blue-white supergiant, Deneb is also one of the most luminous nearby stars. It is, or has been, known by a number of other traditional names, including Arided and Aridif, but today these have fallen out of use.
Distance and physical characteristics
Deneb's absolute magnitude is about −7, placing it among the most luminous stars known, with an estimated luminosity 60,000 times that of our Sun.[2]
Deneb's exact distance from the Earth is uncertain, which makes determining many of Deneb's other properties similarly imprecise. However, the uncertainty has been dramatically reduced upon analysis of the New Hipparcos Data Reduction in 2007. One 2008 study puts the most likely distance at approximately 1,550 light-years, and the reduced parallax uncertainties do not rule out a distance as close as 1,340 light-years or as far as 1,840 light-years [3] It is the farthest first-magnitude star from Earth.
Based on its temperature and luminosity and also on direct measurements of its tiny angular diameter (a mere 0.002 second of arc), Deneb appears to have a diameter about 200 times that of the Sun; if placed at the center of our Solar System, Deneb would extend to the orbit of the Earth.[4] It is one of the largest white stars known.
Deneb is a blue-white colored star of spectral type A2Ia, with a surface temperature of 8,400 Kelvin. It is the prototype of a class of variable stars known as Alpha Cygni variables. Its surface undergoes non-radial fluctuations which cause its brightness and spectral type to change slightly.
Deneb's mass is estimated at 20 solar masses.[5][4] As a blue-white supergiant, its high mass and temperature mean that the star will have a short lifespan and will probably go supernova within a few million years. It has already stopped fusing hydrogen in its core. The star was probably an O class star during its main sequence lifetime and is now likely expanding into a red supergiant like Mu Cephei. As it expands, it will go through the F, G, K and M spectral types.
Deneb's solar wind causes it to lose mass at a rate of 0.8 millionth of a solar mass per year, a hundred thousand times the flow rate from the Sun.[4]
[edit] Etymology and cultural significance
The name Deneb is derived from dhaneb, the Arabic for "tail", from the phrase ذنب الدجاجة Dhanab ad-Dajājah, or "tail of the hen".[6] Similar names were given to at least seven different stars, most notably Deneb Kaitos, the brightest star in the constellation Cetus, and Denebola, the second brightest star in Leo.
Less contracted names include Deneb Adige, Denebadigege, and Denebedigege. Arided was used in the Alfonsine Tables, this latter name derived from Al Ridhādh, a name for the constellation. Johann Bayer called it Arrioph, derived from Aridf and Al Ridf, 'the hindmost' or Gallina. Caesius termed it Os rosae, or Rosemund in German, or Uropygium – the parson's nose.[6]
It is known as 天津四 (the Fourth Star of the Celestial Ford) in Chinese. In the Chinese love story of Qi Xi, Deneb marks the magpie bridge across the Milky Way which allows the separated lovers Niu Lang (Altair) and Zhi Nü (Vega) to be reunited on one special night of the year in late summer. In other versions of the story Deneb is a fairy who acts as chaperone when the lovers meet.
References
1. ^ Hipparcos star catalog entry
2. ^ Spacewatch Friday: Summer Triangle: Easy-to-Find Guide to the Milky Way
3. ^ Apellániz, J. Maíz; E. J Alfaro, A. Sota (2008-04-16). "Accurate distances to nearby massive stars with the new reduction of the Hipparcos raw data". 0804.2553.http://arxiv.org/abs/0804.2553. Retrieved 2009-08-18.
4. ^ a b c Deneb by Jim Kaler at astro.uiuc.edu
5. ^ Deneb at domeofthesky.com
6. ^ a b Richard Hinckley Allen, Star Names: Their Lore and Meaning (1963), p. 195.
Deneb, Samanyolu'nun en büyük yıldızlarından biridir; eğer Güneş'in yerinde olsaydı, yıldızın yuvarlağı Dünya'nın yörüngesini içine alırdı. Deneb'in kütlesi, Güneş'in kütlesinin 25 katı ve çapı Güneş'in çapının 200 katıdır. Güneş'ten 265.000 kat parlak olan Deneb, son derece parlak, beyaz renkte bir dev yıldızdır. Spektrum türü A olan beyaz yıldızlar, evrendeki yıldızların yaklaşık %1'ini oluştururlar. Deneb benzeri dev yıldızların parlaklıkları, Güneş'ten ortalama 10.000 kat, kütleleri 10 ile 100 kat, çapları ise 20 ile 1.000 daha fazladır. Bunlar, hemen her spektrum türünde olabilen genç yıldızlardır (Rigel, Betelgeuse, Canopus, Antares gibi).
Deneb'in bizden çok uzakta olmasından ötürü, yıldızın gerçek parlaklığı ve evrimsel durumu kesin olarak bilinmemektedir. Ancak, önümüzdeki birkaç milyon yl içinde patlayacağı neredeyse kesindir.
Deneb (α Cyg / α Cygni / Alpha Cygni) is the brightest star in the constellation Cygnus and one of the vertices of the Summer Triangle. It is the 19th brightest star in the night sky, with an apparent magnitude of 1.25. A blue-white supergiant, Deneb is also one of the most luminous nearby stars. It is, or has been, known by a number of other traditional names, including Arided and Aridif, but today these have fallen out of use.
Distance and physical characteristics
Deneb's absolute magnitude is about −7, placing it among the most luminous stars known, with an estimated luminosity 60,000 times that of our Sun.[2]
Deneb's exact distance from the Earth is uncertain, which makes determining many of Deneb's other properties similarly imprecise. However, the uncertainty has been dramatically reduced upon analysis of the New Hipparcos Data Reduction in 2007. One 2008 study puts the most likely distance at approximately 1,550 light-years, and the reduced parallax uncertainties do not rule out a distance as close as 1,340 light-years or as far as 1,840 light-years [3] It is the farthest first-magnitude star from Earth.
Based on its temperature and luminosity and also on direct measurements of its tiny angular diameter (a mere 0.002 second of arc), Deneb appears to have a diameter about 200 times that of the Sun; if placed at the center of our Solar System, Deneb would extend to the orbit of the Earth.[4] It is one of the largest white stars known.
Deneb is a blue-white colored star of spectral type A2Ia, with a surface temperature of 8,400 Kelvin. It is the prototype of a class of variable stars known as Alpha Cygni variables. Its surface undergoes non-radial fluctuations which cause its brightness and spectral type to change slightly.
Deneb's mass is estimated at 20 solar masses.[5][4] As a blue-white supergiant, its high mass and temperature mean that the star will have a short lifespan and will probably go supernova within a few million years. It has already stopped fusing hydrogen in its core. The star was probably an O class star during its main sequence lifetime and is now likely expanding into a red supergiant like Mu Cephei. As it expands, it will go through the F, G, K and M spectral types.
Deneb's solar wind causes it to lose mass at a rate of 0.8 millionth of a solar mass per year, a hundred thousand times the flow rate from the Sun.[4]
[edit] Etymology and cultural significance
The name Deneb is derived from dhaneb, the Arabic for "tail", from the phrase ذنب الدجاجة Dhanab ad-Dajājah, or "tail of the hen".[6] Similar names were given to at least seven different stars, most notably Deneb Kaitos, the brightest star in the constellation Cetus, and Denebola, the second brightest star in Leo.
Less contracted names include Deneb Adige, Denebadigege, and Denebedigege. Arided was used in the Alfonsine Tables, this latter name derived from Al Ridhādh, a name for the constellation. Johann Bayer called it Arrioph, derived from Aridf and Al Ridf, 'the hindmost' or Gallina. Caesius termed it Os rosae, or Rosemund in German, or Uropygium – the parson's nose.[6]
It is known as 天津四 (the Fourth Star of the Celestial Ford) in Chinese. In the Chinese love story of Qi Xi, Deneb marks the magpie bridge across the Milky Way which allows the separated lovers Niu Lang (Altair) and Zhi Nü (Vega) to be reunited on one special night of the year in late summer. In other versions of the story Deneb is a fairy who acts as chaperone when the lovers meet.
References
1. ^ Hipparcos star catalog entry
2. ^ Spacewatch Friday: Summer Triangle: Easy-to-Find Guide to the Milky Way
3. ^ Apellániz, J. Maíz; E. J Alfaro, A. Sota (2008-04-16). "Accurate distances to nearby massive stars with the new reduction of the Hipparcos raw data". 0804.2553.http://arxiv.org/abs/0804.2553. Retrieved 2009-08-18.
4. ^ a b c Deneb by Jim Kaler at astro.uiuc.edu
5. ^ Deneb at domeofthesky.com
6. ^ a b Richard Hinckley Allen, Star Names: Their Lore and Meaning (1963), p. 195.
