digplanet beta 1: Athena
Share digplanet:

Agriculture

Applied sciences

Arts

Belief

Business

Chronology

Culture

Education

Environment

Geography

Health

History

Humanities

Language

Law

Life

Mathematics

Nature

People

Politics

Science

Society

Technology

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 7.67 astronomical units. Its distance from Earth is estimated to be around 1.6 kpc, or 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]

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 has a dusty environment surrounding it,[2][4] and it exhibits a bean-shaped asymmetric nebula that is coincident with the distribution of its H2O vapor masers.[5]

NML Cygni has an estimated mass loss rate of 2×10−4 M per year,[6][7] 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.[8] These dust envelopes are formed due to the strong post-main sequence wind velocity, 23 km/s, and the high mass loss.

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]

Observational history[edit]

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 was discovered in 1965, by Neugebauer, Martz, and Leighton which described two extremely red luminous stars, their colour being described as consistent with a black body temperature of 1,000K.[9] The name NML comes from the names of these three discoverers.[10] The second star was briefly referred to as NML Tauri[11] but is now known as IK Tauri,[12] an M9 Mira variable. NML Cygni has since also been given the designation V1489 Cygni on account of the small semi-regular brightness variations,[13] 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.[14] The presence of molecules like H
2
O
, SiO, CO, HCN, CS, SO, SO
2
, and H
2
S
was also revealed in the later years.[6]

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. ^ 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
  6. ^ 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. 
  7. ^ "Combined Array for Research in Millimeter-wave Astronomy". Retrieved August 27, 2012. 
  8. ^ DanchiI, W. C.; Green, W. H.; Hale, D. D. S.; McEleroy, K.; Monnier, J. D.; Tuthill, P. G.; Townes, C. H. (July 2001). "Proper Motions of Dust Shells Surrounding NML Cygni". The Astrophysical Journal 555: 405. Bibcode:2001ApJ...555..405D. doi:10.1086/322237. 
  9. ^ 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. 
  10. ^ 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. 
  11. ^ Pesch, P. (1967). "Objective-Prism Spectra of Some Very Red Stars". The Astrophysical Journal 147: 381. doi:10.1086/149015.  edit
  12. ^ Kukarkin, B. V.; Efremov, Yu. N.; Frolov, M. S.; Medvedeva, G. I.; Kholopov, P. N.; Kurochkin, N. E.; Kukarkina, N. P.; Perova, N. B.; Fedorovich, V. P. (8 November 1968). "Identification List of the New Variable Stars Nominated in 1968". Information Bulletin on Variable Stars 311 (1). Bibcode:1968IBVS..311....1K. 
  13. ^ 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. 
  14. ^ Cohen, R. J.; Downs, G.; Emerson, R.; Grimm, M.; Gulkis, S.; Stevens, G.; Tarter, J. (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. 
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.
This page uses Creative Commons Licensed content from Wikipedia. A portion of the proceeds from advertising on Digplanet goes to supporting Wikipedia.
558 videos foundNext > 

Nml Cygni X Vy Canis Majoris

A estrela Vy Canis Majoris era a maior estrela do universo, mas pouco tempo se passou e ja descobriu-se uma estrela maior, a Nml Cygni. Isso significa que po...

The Largest Known Star in the Universe

VY Canis Majoris is no longer the biggest star. NML Cygni is !

Ultimate Size Comparison of the Entire Universe (In 1080p)

From the subatomic to the cosmic scale, the ultimate size comparison of the entire universe will show you how large things really are! This is an update vers...

Estrellas a escala - NML Cygni vs Sol

Este video fue hecho para que admiren las maravillas del universo, al igual como yo lo he admirado, me llamo Gabriel Spinelli y espero que lo hayan disfrutad...

nml cygni, la estrella mas grande descubierta

en este sencillo video te muestro la estrella mas grande hasta ahora descubierta.

LAS ESTRELLAS MAS GRANDES NML CYGNI

UNA REPRESENTACION DE LAS ESTRELLAS MAS GRANDES EN COMPARACION CON NUESTRO SOL.

Nml Cygni

Vy canis majoris deixou de ser a maior estrela do universo quando descobriram a nml cygni.

10 Largest Stars Known HD

Hey guys, as you can see Vy Canis Majoris is not the biggest star at all, after some better research scientist have found that his size was not very well mea...

Star size comparison

This is my own star size comparison video, starting with proxima centauri and ending at the largest known star, NML cygni. After that has finished comes some...

Bilinen En Büyük Yıldız Nml Cygni

Bu yıldız resimde de gördüğünüz gibi devasa bişey Güneş'ten 1650 kat daha büyük ve çok daha parlaktır. http://arulphi.com/index.php?topic=167.0.

558 videos foundNext > 

73 news items

 
KQED QUEST (blog)
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 ...

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 ...
 
YouTube
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 ...
 
Cricket Country
Wed, 13 Nov 2013 19:39:29 -0800

When we look back at the career of Sachin Tendulkar, the enormous longevity often boggles the mind. We are struck by the way he has remained an almost eternal constant across global changes that have metamorphosed the world beyond recognition.
 
YouTube
Mon, 13 May 2013 08:43:10 -0700

LISTEN UY SCUTI IS A MISTAKE NML CYGNI IS STILL THE LARGEST SO U KNOW WESTURLUND 1-26 Q3BARAIDION AND UY SCUTI ALL ARE NOT LARGER THAN NML CYGNI IT IS STILL THE LARGEST!!!!!!!!!!!!!!!!. Read moreShow less. Reply.
 
YouTube
Fri, 03 Dec 2010 19:07:55 -0800

We'll nml cygni can be confirmed as the star that will kill us all. Read moreShow less. Reply. ·. View 1 reply. Show moreLoading... Loading... Advertisement. 56:45. Play next; Play now. The Ultimate Guide to Black Holes by Izabella Willett 130,789 ...

HDblog (Blog)

HDblog (Blog)
Fri, 14 Mar 2014 10:29:16 -0700

warrior44aa14 Mar 2014 @ 07:06. Da Wikipedia. 1- UY Scuti 1708 2- NML Cygni 1650 3- WOH G64 1540. Quella la mettono come 1056 - 1575. Gabrix9314 Mar 2014 @ 07:03. 12K anni luce......ah ah ah sta bene li. Giacomo Consonni14 Mar 2014 @ 06:36.
 
Day.Az
Fri, 16 May 2014 01:41:55 -0700

Этот клип показывает, насколько мала Земля по сравнению с самой большой известной звездой NML Cygni. А так выглядит яйцо под водой без скорлупы. Вот что происходит, когда вы выливаете кипящую воду на 40 градусный мороз.
Loading

Oops, we seem to be having trouble contacting Twitter

Support Wikipedia

A portion of the proceeds from advertising on Digplanet goes to supporting Wikipedia. Please add your support for Wikipedia!

Searchlight Group

Digplanet also receives support from Searchlight Group. Visit Searchlight