Deneb
Observation data Epoch J2000 Equinox J2000 | ||
---|---|---|
Constellation | Cygnus | |
Pronunciation
|
/ˈdɛnɛb/, /ˈdɛnəb/[1] | |
Right ascension | 20h 41m 25.9s[2] | |
Declination | +45° 16′ 49″[2] | |
Apparent magnitude (V) | 1.25[3] (1.21–1.29[4]) | |
Characteristics | ||
Spectral type | A2 Ia[5] | |
U−B color index | −0.23[3] | |
B−V color index | +0.09[3] | |
Variable type | Alpha Cygni[4] | |
Absolute magnitude (MV) | −8.38[7] | |
Details Rotational velocity (v sin i)20±2 km/s | | |
HR 7924, SAO 49941 | ||
Database references | ||
SIMBAD | data |
Deneb (/ˈdɛnɛb/) is a first-magnitude star in the constellation of Cygnus. Deneb is one of the vertices of the asterism known as the Summer Triangle and the "head" of the Northern Cross. It is the brightest star in Cygnus and the 19th brightest star in the night sky, with an average apparent magnitude of +1.25. A blue-white supergiant, Deneb rivals Rigel as the most luminous first-magnitude star. However, its distance, and hence luminosity, is poorly known; its luminosity is somewhere between 55,000 and 196,000 times that of the Sun. Its Bayer designation is α Cygni, which is Latinised to Alpha Cygni, abbreviated to Alpha Cyg or α Cyg.
Nomenclature
α Cygni (Latinised to Alpha Cygni) is the star's designation given by Johann Bayer in 1603. The traditional name Deneb is derived from the Arabic word for "tail", from the phrase ذنب الدجاجة Dhanab al-Dajājah, or "tail of the hen".[8] The IAU Working Group on Star Names has recognised the name Deneb for this star, and it is entered in their Catalog of Star Names.[9]
Denebadigege was used in the
An older traditional name is Arided /ˈærɪdɛd/, from the Arabic ar-ridf 'the one sitting behind the rider' (or just 'the follower'), perhaps referring to the other major stars of Cygnus, which were called al-fawāris 'the riders'.[11]
Observation
The 19th
Deneb is located at the tip of the Northern Cross asterism made up of the brightest stars in Cygnus, the others being Albireo (Beta Cygni), Gamma Cygni, Delta Cygni, and Epsilon Cygni.[13] It also lies at one vertex of the prominent and widely spaced asterism called the Summer Triangle, shared with the first-magnitude stars Vega in the constellation Lyra and Altair in Aquila.[14][15] This outline of stars is the approximate shape of a right triangle, with Deneb located at one of the acute angles.
The
Pole star
Due to the
Preceded by | Pole Star
|
Succeeded by |
---|---|---|
Alderamin
|
8700 AD to 11000 AD | Delta Cygni |
Physical characteristics
Deneb's adopted distance from the Earth is around 802 parsecs (2,620 ly).[7] This is derived by a variety of different methods, including spectral luminosity classes, atmospheric modelling, stellar evolution models, assumed membership of the Cygnus OB7 association, and direct measurement of angular diameter. These methods give different distances, and all have significant margins of error. The original derivation of a parallax using measurements from the astrometric satellite Hipparcos gave an uncertain result of 1.01 ± 0.57 mas[21][22] that was consistent with this distance. However, a more recent reanalysis gives the much larger parallax whose distance is barely half the current accepted value.[2] One 2008 calculation using the Hipparcos data puts the most likely distance at 475 parsecs (1,550 ly), with an uncertainty of around 15%.[23] The controversy over whether the direct Hipparcos measurements can be ignored in favour of a wide range of indirect stellar models and interstellar distance scales is similar to the better known situation with the Pleiades.[2]
Deneb's absolute magnitude is estimated as −8.4, placing it among the visually brightest stars known, with an estimated luminosity of nearly 200,000 L☉. This is towards the upper end of values published over the past few decades, which vary between 55,000 L☉ and 196,000 L☉, while the distance based on the Hipparcos parallax corresponds to closer to 40,000 L☉.[24][25][26]
Deneb is the most luminous first magnitude star, that is, stars with a brighter apparent magnitude than 1.5. Deneb is also the most distant of the 30
Deneb is a bluish-white star of
Evolutionary state
Deneb spent much of its early life as an
Stars evolving red-wards for the first time are most likely fusing hydrogen in a shell around a helium core that has not yet grown hot enough to start fusion to carbon and oxygen. Convection has begun dredging up fusion products but these do not reach the surface. Post-red supergiant stars are expected to show those fusion products at the surface due to stronger convection during the red supergiant phase and due to loss of the obscuring outer layers of the star. Deneb is thought to be increasing its temperature after a period as a red supergiant, although current models do not exactly reproduce the surface elements showing in its spectrum.[29]
Variable star
Deneb is the prototype of the Alpha Cygni (α Cygni) variable stars,[31][30] whose small irregular amplitudes and rapid pulsations can cause its magnitude to vary anywhere between 1.21 and 1.29.[32] Its variable velocity discovered by Lee in 1910,[16] but it was not formally placed as a unique class of variable stars until the 1985 4th edition of the General Catalogue of Variable Stars.[33] The cause of the pulsations of Alpha Cygni variable stars are not fully understood, but their irregular nature seems to be due to beating of multiple pulsation periods. Analysis of radial velocities determined 16 different harmonic pulsation modes with periods ranging between 6.9 and 100.8 days.[34] A longer period of about 800 days probably also exists.[30]
Possible spectroscopic companion
Deneb has been reported as a possible single line spectroscopic binary with a period of about 850 days, where the spectral lines from the star suggest cyclical radial velocity changes.[34] Later investigations have found no evidence supporting the existence of a companion.[31]
Etymology and cultural significance
Names similar to Deneb have been given to at least seven different stars, most notably Deneb Kaitos, the brightest star in the constellation of Cetus; Deneb Algedi, the brightest star in Capricornus; and Denebola, the second brightest star in Leo. All these stars are referring to the tail of the animals that their respective constellations represent.
In Chinese, 天津 (Tiān Jīn), meaning
In the Chinese love story of
Namesakes
See also
- List of bright stars
- Deneb Sector
References
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- ^ Bibcode:2002yCat.2237....0D.
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Kunitzsch, Paul (1986). "The Star Catalogue Commonly Appended to the Alfonsine Tables". S2CID 118597258.
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Barlow, N. G. (2008). Mars: An introduction to its interior, surface and atmosphere. ISBN 978-0-521-85226-5.
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van de Kamp, P. (1953). "The Twenty Brightest Stars". doi:10.1086/126523.
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Lamers, H. J. G. L. M.; Stalio, R.; Kondo, Y. (1978). "A study of mass loss from the mid-ultraviolet spectrum of α Cygni (A2 Ia), β Orionis (B8 Ia), and η Leonis (A0 Ib)". doi:10.1086/156252.
- ^ Kaler, James B. (2017). "The 172 Brightest Stars". STARS. Retrieved 2021-09-17.
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