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NML Cygni
CygOB2 med.jpg
H-Alpha light image of Cygnus OB2, the stellar association in which NML Cygni is located
Observation data
Epoch J2000      Equinox J2000
Constellation Cygnus
Right ascension 20h 46m 25.6s
Declination +40° 06′ 59.4″
Apparent magnitude (V) 16.60
Characteristics
Spectral type M6I[1]
B−V color index 2.0
Variable type Semiregular
Astrometry
Proper motion (μ) RA: −1.55[2] mas/yr
Dec.: −4.59[2] mas/yr
Parallax (π) 0.620[2] ± 0.047[2] mas
Distance 1.61k[2] pc
Details
Mass 25–40[2] M
Radius 1,642–2,775[2] R
Luminosity 270,000[2] L
Other designations
V* V1489 Cyg, RAFGL 2650, IRC +40448
Database references
SIMBAD data

NML Cygni or V1489 Cygni is a red hypergiant[2] and one of the largest stars currently known with a radius about 1,650 times the Sun's,[3] equal to 15.3 astronomical units. Its distance from Earth is estimated to be around 1.6 kpc, about 5,300 light-years.[3]

NML Cygni is a part of the Cygnus OB2 association, one of the closest massive associations to the Sun, spanning nearly 2° on the sky or ∼30 pc in radius at the distance of 1.74 ± 0.2 kpc.[4]

Observational history[edit]

NML Cygni was discovered in 1965 by Neugebauer, Martz, and Leighton who described two extremely red luminous stars, their colour being described as consistent with a black body temperature of 1,000 K.[5] The name NML comes from the names of these three discoverers.[6] The second star was briefly referred to as NML Tauri[7] but is now known as IK Tauri,[8] an M9 Mira variable. NML Cygni has since also been given the designation V1489 Cygni on account of the small semi-regular brightness variations,[9] but is still most commonly referred to as NML Cygni. Its composition began to be revealed with the discovery of OH masers (1612 MHz) in 1968.[10] Molecules like H
2
O
, SiO, CO, HCN, CS, SO, SO
2
, and H
2
S
have also been detected.[11]

Characteristics[edit]

The diameter of NML Cygni, at 1,650 times that of the Sun, is about 2,295,000,000 kilometres (1.426×109 mi). If placed at the center of the Solar System, its surface would extend beyond the orbit of Jupiter, filling over half the gap between Jupiter and Saturn's orbit. It contains a volume approximately 4.5 billion times that of the Sun. The bolometric luminosity (Lbol) for NML Cygni is near 3 × 105 L. Its bolometric magnitude (Mbol) is around −9.0. It is one of the most luminous cool hypergiants.[4] It is also a semiregular variable star with a period of around 940 days.[4]

NML Cygni is evolved and a number of heavy elements and molecules have been detected in its atmosphere, particularly oxygen, hydroxyl, and water. It is surrounded by dusty material[2][4] and it exhibits a bean-shaped asymmetric nebula that is coincident with the distribution of its H2O vapor masers.[12]

Relative sizes of the planets in the Solar System and several stars, including NML Cygni
1. Mercury < Mars < Venus < Earth
2. Earth < Neptune < Uranus < Saturn < Jupiter
3. Jupiter < Proxima Centauri < Sun < Sirius
4. Sirius < Pollux < Arcturus < Aldebaran
5. Aldebaran < Rigel < Antares < Betelgeuse
6. Betelgeuse < VY Canis Majoris < NML Cygni < UY Scuti.

NML Cygni has an estimated mass loss rate of 2×10−4 M per year,[11][13] one of the highest known for any star. The annual parallax of NML Cygni is measured to be around 0.62 milli-arc-seconds.[2] From the observations, it is estimated that NML Cygni has two discrete optically thick envelopes of dust and molecules. The optical depth of the inner shell is found to be 1.9, while that of the outer one is 0.33.[14] These dust envelopes are formed due to the strong post-main-sequence wind, which has a velocity 23 km/s.[citation needed]

Because of its position on the outskirts of the massive Cygnus OB2 association, the detectable effects of NML Cygni's radiation on the surrounding dust and gas are limited to the region away from the central hot stars of the association.[4]

See also[edit]

References[edit]

  1. ^ Monnier, J. D.; Millan‐Gabet, R.; Tuthill, P. G.; Traub, W. A.; Carleton, N. P.; Coude Du Foresto, V.; Danchi, W. C.; Lacasse, M. G.; Morel, S.; Perrin, G.; Porro, I. L.; Schloerb, F. P.; Townes, C. H. (2004). "High‐Resolution Imaging of Dust Shells by Using Keck Aperture Masking and the IOTA Interferometer". The Astrophysical Journal 605: 436. arXiv:astro-ph/0401363. Bibcode:2004ApJ...605..436M. doi:10.1086/382218.  edit
  2. ^ a b c d e f g h i j k Zhang, B.; Reid, M. J.; Menten, K. M.; Zheng, X. W.; Brunthaler, A. (2012). "The distance and size of the red hypergiant NML Cygni from VLBA and VLA astrometry". Astronomy & Astrophysics 544: A42. arXiv:1207.1850. Bibcode:2012A&A...544A..42Z. doi:10.1051/0004-6361/201219587.  edit
  3. ^ a b Schuster, Michael Thomas (2007). Investigating the Circumstellar Environments of the Cool Hypergiants. ProQuest. p. 57. ISBN 978-0-549-32782-0. Retrieved 27 August 2012. 
  4. ^ a b c d e Schuster, M. T.; Marengo, M.; Hora, J. L.; Fazio, G. G.; Humphreys, R. M.; Gehrz, R. D.; Hinz, P. M.; Kenworthy, M. A.; Hoffmann, W. F. (2009). "Imaging the Cool Hypergiant NML Cygni's Dusty Circumstellar Envelope with Adaptive Optics". The Astrophysical Journal 699 (2): 1423. arXiv:0904.4690. Bibcode:2009ApJ...699.1423S. doi:10.1088/0004-637X/699/2/1423.  edit
  5. ^ Neugebauer, G.; Martz, D. E.; Leighton, R. B. (July 1965). "Observations of Extremely Cool Stars". Astrophysical Journal 142: 399–401. Bibcode:1965ApJ...142..399N. doi:10.1086/148300. 
  6. ^ Hearnshaw, J. B. (2 May 1996). "New infrared sources and their interpretation". The Measurement of Starlight: Two Centuries of Astronomical Photometry. Cambridge University Press. p. 278. ISBN 978-0-521-40393-1. Retrieved 23 August 2012. 
  7. ^ Pesch, P. (1967). "Objective-Prism Spectra of Some Very Red Stars". The Astrophysical Journal 147: 381. doi:10.1086/149015.  edit
  8. ^ Kukarkin, B. V.; Efremov, Yu. N.; Frolov, M. S.; Medvedeva, G. I. et al. (8 November 1968). "Identification List of the New Variable Stars Nominated in 1968". Information Bulletin on Variable Stars 311 (1). Bibcode:1968IBVS..311....1K. 
  9. ^ Kukarkin, B. V.; Kholopov, P. N.; Kukarkina, N. P. (27 November 1975). "61st Name-List of Variable Stars". Information Bulletin on Variable Stars 1068 (1). Bibcode:1975IBVS.1068....1K. 
  10. ^ Cohen, R. J.; Downs, G.; Emerson, R.; Grimm, M. et al. (1 April 1987). "Narrow polarized components in the OH 1612-MHz maser emission from supergiant OH-IR sources". Monthly Notices of the Royal Astronomical Society 225: 491–498. Bibcode:1987MNRAS.225..491C. doi:10.1093/mnras/225.3.491. 
  11. ^ a b Kevin Marvel (19 December 1996). "NML Cygni". The Circumstellar Environment of Evolved Stars As Revealed by Studies of Circumstellar Water Masers. Universal-Publishers. pp. 182–212. ISBN 978-1-58112-061-5. Retrieved 23 August 2012. 
  12. ^ Schuster, M. T.; Humphreys, R. M.; Marengo, M. (2006). "The Circumstellar Environments of NML Cygni and the Cool Hypergiants". The Astronomical Journal 131: 603. arXiv:astro-ph/0510010. Bibcode:2006AJ....131..603S. doi:10.1086/498395.  edit
  13. ^ "Combined Array for Research in Millimeter-wave Astronomy" (PDF). Retrieved August 27, 2012. 
  14. ^ DanchiI, W. C.; Green, W. H.; Hale, D. D. S.; McEleroy, K. et al. (July 2001). "Proper Motions of Dust Shells Surrounding NML Cygni". The Astrophysical Journal 555: 405. Bibcode:2001ApJ...555..405D. doi:10.1086/322237. 
Preceded by
VY Canis Majoris
Largest known star
2012–2013
Succeeded by
Westerlund 1 BKS AS

Original courtesy of Wikipedia: http://en.wikipedia.org/wiki/NML_Cygni — Please support Wikipedia.
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The Epoch Times

The Epoch Times
Wed, 21 Aug 2013 16:42:13 -0700

The largest star documented to date, named NML Cygni, is 165,000 times larger than the sun, making it large enough to contain within it 165 billion planet Earths. Not only is the star massive enough to reach from Earth to Jupiter's orbital track in our ...
 
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Fri, 02 Nov 2012 08:02:32 -0700

The largest known star, the red supergiant NML Cygni, is approximately 1650 times the diameter of our sun, or over 1.4 billion miles across! Placed where our sun is, this star would swallow up all the planets closer to the sun than Saturn—and Saturn ...
 
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Fri, 21 Dec 2012 21:30:53 -0800

NML Cygni is the largest known star, where the radius is reasonably certain. There are other known stars That may very well be larger, however it is not well established that they actually are, and they may in fact be Smaller. Rather than choosing one ...

Irish Times

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Tue, 01 Apr 2014 17:19:03 -0700

Let us consider the very large. In the whole visible universe, or at least the bits of it that our Earthly telescopes have swept, the biggest single thing we've yet found is a star called NML Cygni. It is a red hyper-giant, a star so unbelievably ...

EarthSky

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Mon, 27 Aug 2012 07:42:02 -0700

How big can stars get? And how do these monster stars get so big? When speaking of bigness among stars, you have to define your terms. The heaviest star is thought to be R136a1. It's 265 times more massive than our sun – nearly twice as massive as what ...
 
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Wed, 13 Nov 2013 19:39:29 -0800

It was a landmark year for science. NML Cygni became the star with the largest volume. Higgs boson was discovered at CERN (confirmed to 99.999% certainty). Photonic Molecules were discovered at MIT. The Beach Boys embarked on a 2012 world concert ...
 
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Mon, 26 Jan 2015 10:26:39 -0800

co powiecie na to ze gwiazda Canis Majoris jest tak ogromna ze okrazenie jej samolotem z predkoscia 900 km/h zajelo by ponad 1100 lat?a pare lat temu odkryto najwieksza jak dotad gwiazde NML Cygni,jest tak ogromna ze zajelaby nasz caly Uklad ...
 
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Fri, 03 Dec 2010 19:07:55 -0800

Naufal Renardi 1 month ago. UY Scuti And NML Cygni Is More Bigger -,-. Read more Show less. Reply · 1. ▽ Report spam or abuse. Fk 1 year ago. "There is only one place in the universe that generates that much gravity" ofc it is, we all know they ...
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