List of stars in Cygnus - AbsoluteAstronomy.com

This is the list of notable star

Star

A star is a massive, luminous sphere of plasma held together by gravity. At the end of its lifetime, a star can also contain a proportion of degenerate matter. The nearest star to Earth is the Sun, which is the source of most of the energy on Earth...

s in the constellation

Constellation

In modern astronomy, a constellation is an internationally defined area of the celestial sphere. These areas are grouped around asterisms, patterns formed by prominent stars within apparent proximity to one another on Earth's night sky....

Cygnus
Cygnus (constellation)
Cygnus is a northern constellation lying on the plane of the Milky Way. Its name is the Latinized Hellenic word for swan. One of the most recognizable constellations of the northern summer and autumn, it features a prominent asterism known as the Northern Cross...

, sorted by decreasing brightness.

Name	B Bayer designation A Bayer designation is a stellar designation in which a specific star is identified by a Greek letter, followed by the genitive form of its parent constellation's Latin name...	F Flamsteed designation Flamsteed designations for stars are similar to Bayer designations, except that they use numbers instead of Greek letters. Each star is assigned a number and the Latin genitive of the constellation it lies in...	HD Henry Draper Catalogue The Henry Draper Catalogue is an astronomical star catalogue published between 1918 and 1924, giving spectroscopic classifications for 225,300 stars; it was later expanded by the Henry Draper Extension , published between 1925 and 1936, which gave classifications for 46,850 more stars, and by the...	HIP	vis. mag. Apparent magnitude The apparent magnitude of a celestial body is a measure of its brightness as seen by an observer on Earth, adjusted to the value it would have in the absence of the atmosphere...	abs. mag. Absolute magnitude Absolute magnitude is the measure of a celestial object's intrinsic brightness. it is also the apparent magnitude a star would have if it were 32.6 light years away from Earth...	Dist. (ly)	Sp. class Stellar classification In astronomy, stellar classification is a classification of stars based on their spectral characteristics. The spectral class of a star is a designated class of a star describing the ionization of its chromosphere, what atomic excitations are most prominent in the light, giving an objective measure...	Notes
Deneb Deneb Deneb 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...	α	50	197345	102098	1.25	−8.73	3228	A2Ia	Deneb el Adige, Deneb Cygni, Arided, Aridif, Arrioph, Gallina; prototype of α Cyg variables Alpha Cygni variable Alpha Cygni variables are variable stars which exhibit non-radial pulsations, meaning that some portions of the stellar surface are contracting at the same time others parts expand. They are supergiant stars of spectral types B or A...
γ Cyg Gamma Cygni Gamma Cygni is a star in the constellation Cygnus. It has the traditional name Sadr ....	γ	37	194093	100453	2.23	−6.12	1523	F8Ib	Sadr, Sador, Sadir, Sadr al Dedjadjet, Pectus Gallinæ; variable Variable star A star is classified as variable if its apparent magnitude as seen from Earth changes over time, whether the changes are due to variations in the star's actual luminosity, or to variations in the amount of the star's light that is blocked from reaching Earth...
ε Cyg Epsilon Cygni Epsilon Cygni is a star in the constellation Cygnus . It is also called Gienah, a traditional name it shares with Gamma Corvi...	ε	53	197989	102488	2.48	0.76	72	K0III	Gienah, Gienah Cygni
δ Cyg Delta Cygni Delta Cygni is the third-magnitude star in the constellation Cygnus. It has the traditional name Rukh. It will be the "North Star" for at least four centuries around 11,250....	δ	18	186882	97165	2.86	−0.74	171	B9.5III	Ruc, Rukh, Urakhga, Al Fawaris; triple star Star system A star system or stellar system is a small number of stars which orbit each other, bound by gravitational attraction. A large number of stars bound by gravitation is generally called a star cluster or galaxy, although, broadly speaking, they are also star systems.-Binary star systems:A stellar...
Albireo A Albireo Albireo is the fifth brightest star in the constellation Cygnus. Although it has the Bayer designation beta, it is fainter than Gamma Cygni, Delta Cygni, and Epsilon Cygni. Albireo appears to the naked eye to be a single star of magnitude 3 but through a telescope, even low magnification views...	β¹	6	183912	95947	3.05	−2.31	385	K3II+...	Al Minhar al Dajajah, Menchir al Dedjadjet Rostrum Gallinæ; prominent visual binary star Binary star A binary star is a star system consisting of two stars orbiting around their common center of mass. The brighter star is called the primary and the other is its companion star, comes, or secondary... with Albireo B; spectroscopic binary
ζ Cyg Zeta Cygni Zeta Cygni and CCDM J21129+3014B form a binary star system in the constellation Cygnus, approximately 151 light-years away from Earth....	ζ	64	202109	104732	3.21	−0.12	151	G8II SB	multiple star Star system A star system or stellar system is a small number of stars which orbit each other, bound by gravitational attraction. A large number of stars bound by gravitation is generally called a star cluster or galaxy, although, broadly speaking, they are also star systems.-Binary star systems:A stellar...
ξ Cyg	ξ	62	200905	104060	3.72	−4.07	1177	K5Ibv SB
τ Cyg Tau Cygni Tau Cygni is a binary star system in the constellation Cygnus, approximately 69 light years away from Earth. The main star, 4th magnitude GJ 822.1 A, is a yellowish white subgiant star of the spectral type F2IV. It therefore has a surface temperature of 6,000 to 7,500 kelvins and is larger,...	τ	65	202444	104887	3.74	2.14	68	F1IV	multiple star; δ Sct variable Delta Scuti variable A Delta Scuti variable is a variable star which exhibits variations in its luminosity due to both radial and non-radial pulsations of the star's surface. Typical brightness fluctuations are from 0.003 to 0.9 magnitudes in V over a period of a few hours, although the amplitude and period of the...
ι Cyg	ι	10	184006	95853	3.76	0.89	122	A5Vn
κ Cyg	κ	1	181276	94779	3.80	0.91	123	K0III	variable
ο¹ Cyg	ο¹	31	192577	99675	3.80	−4.29	1353	K2II+...	V695 Cyg; Algol variable Algol variable Algol variables or Algol-type binaries are a class of eclipsing binary stars where the orbital plane of the stars are coincident with the line of sight from Earth. When the cooler component passes in front of the hotter one, part of the latter's light is blocked, and the total brightness of the...
η Cyg Eta Cygni Eta Cygni is a star in theconstellation Cygnus. It is located about 137 light years from the Sun and is categorized as an orange giant star of spectral class K0III....	η	21	188947	98110	3.89	0.74	139	K0IIIvar	multiple star
ν Cyg	ν	58	199629	103413	3.94	−1.25	356	A1Vn
ο² Cyg	ο²	32	192909	99848	3.96	−3.70	1109	K3Ib-II comp	V1488 Cyg; Algol variable
ρ Cyg	ρ	73	205435	106481	3.98	1.07	124	G8III	variable
41 Cyg		41	195295	101076	4.01	−2.82	758	F5II	variable
52 Cyg		52	197912	102453	4.22	0.22	206	K0III	double star Double star In observational astronomy, a double star is a pair of stars that appear close to each other in the sky as seen from Earth when viewed through an optical telescope. This can happen either because the pair forms a binary star, i.e...
σ Cyg	σ	67	202850	105102	4.22	−6.49	4528	B9Iab
π² Cyg Pi2 Cygni Pi² Cygni is a fourth-magnitude star in the constellation Cygnus. It has the traditional name Pennae Caudalis, which is Latin for "Tail Feathers"...	π²	81	207330	107533	4.23	−3.52	1156	B3III	Pennae Caudalis, Sama al Azrak; spectroscopic binary
33 Cyg		33	192696	99655	4.28	0.93	152	A3IV-Vn	variable
υ Cyg	υ	66	202904	105138	4.41	−2.80	901	B2Vne	emission-line star; γ Cas variable
39 Cyg 39 Cygni 39 Cygni is a star in the constellation Cygnus, approximately 260 light years away from Earth. It is an orange star of the spectral type K3III, meaning it has a surface temperature of 3,500 to 5,000 kelvins. It is cooler, but much larger and brighter, than our Sun....		39	194317	100587	4.43	−0.04	255	K3III
θ Cyg Theta Cygni Theta Cygni is a white main sequence star, spectral class F3 V, forming a wide binary system with a dim red dwarf star, of spectral type M3. The primary component of binary is suspected to host an extrasolar planet.-Planetary companion?:...	θ	13	185395	96441	4.49	3.14	61	F4V	triple star
λ Cyg	λ	54	198183	102589	4.53	−2.62	879	B6IV	Be star Be star A Be star is a B-type star with prominent emission lines of hydrogen in its spectrum. The designation is combined by the spectral class, B, and the lowercase e denoting emission in the spectral classification system. Line emission from other atomic ions might be present as well, but is typically...
63 Cyg	f²	63	201251	104194	4.56	−2.83	982	K4II	double star
47 Cyg A		47	196093	101474	4.61	−2.66	929	K2Ib comp	V2125 Cyg; double star; pulsating variable Variable star A star is classified as variable if its apparent magnitude as seen from Earth changes over time, whether the changes are due to variations in the star's actual luminosity, or to variations in the amount of the star's light that is blocked from reaching Earth...
φ Cyg	φ	12	185734	96683	4.68	0.25	251	G8III-IV...	spectroscopic binary
π¹ Cyg Pi1 Cygni Pi1 Cygni is a star in the constellation Cygnus. It has the traditional name Azelfafage.In Chinese, , meaning Flying Serpent, refers to an asterism consisting of π1 Cygni, α Lacertae, 4 Lacertae, π2 Cygni, HD 206267, ε Cephei, β Lacertae, σ Cassiopeiae, ρ Cassiopeiae, τ Cassiopeiae, AR...	π¹	80	206672	107136	4.69	−3.87	1680	B3IV	Azelfafage; spectroscopic binary
μ¹ Cyg	μ¹	78	206826	107310	4.69	2.94	73	F6V	multiple star
8 Cyg 8 Cygni 8 Cygni is a 5th magnitude star in the constellation Cygnus, approximately 630 light years away from Earth. It is a bluish white subgiant star of the spectral type B3IV. Its surface temperature is 11,000 to 25,000 kelvins. Its surface is therefore at least twice as hot as that of our Sun, and it is...		8	184171	96052	4.74	−1.68	627	B3IV
59 Cyg	f¹	59	200120	103632	4.74	−2.95	1124	B1ne	V832 Cyg; irregular variable Irregular variable An irregular variable is a type of variable star in which variations in brightness show no regular periodicity. There are two main sub-types of irregular variable: eruptive and pulsating.Eruptive irregular variables are divided into three categories:...
P Cyg P Cygni P Cygni is a variable star in the constellation Cygnus. The designation "P" was originally assigned by Johann Bayer in Uranometria as a nova....	P	34	193237	100044	4.77	−6.65	6269	B2pe	Revenante of the Swan, Nova Cygni 1600; hypergiant Hypergiant A hypergiant is a star with a tremendous mass and luminosity, showing signs of a very high rate of mass loss.-Characteristics:... ; prototype of P Cyg variables
30 Cyg		30	192514	99639	4.80	−1.91	716	A5IIIn	variable
57 Cyg		57	199081	103089	4.80	−1.13	501	B5V	spectroscopic binary
55 Cyg		55	198478	102724	4.81	−4.38	2248	B3Ia	V1661 Cyg; α Cyg variables; emission-line star
72 Cyg		72	205512	106551	4.87	0.40	255	K1III
15 Cyg		15	186675	97118	4.89	0.23	279	G8III
ψ Cyg Psi Cygni Psi Cygni is a star in the constellation called Cygnus. It is located 288 lightyears from Earth....	ψ	24	189037	98055	4.91	0.18	288	A4Vn	multiple star
28 Cyg	b²	28	191610	99303	4.93	−2.18	860	B2.5V	V1624 Cyg; Be star; emission-line star
29 Cyg	b³	29	192640	99770	4.93	1.86	134	A2V	V1644 Cyg; variable
T Cyg			198134	102571	4.93	−0.51	399	K3IIIvar	triple star; variable
ω¹ Cyg	ω¹	45	195556	101138	4.94	−2.19	869	B2.5IV	Ruchba; V2014 Cyg; β Cep variable
22 Cyg		22	188892	98068	4.95	−2.89	1203	B5IV	Mokhtarzada
			189276	98073	4.98	−2.27	918	K5II-III
2 Cyg		2	182568	95372	4.99	−1.89	774	B3IV	double star
17 Cyg		17	187013	97295	5.00	3.40	68	F5
20 Cyg	d	20	188056	97635	5.03	1.18	192	K3IIIvar	variable
68 Cyg	A	68	203064	105186	5.04	−11.29	60257	O8e	V1809 Cyg; rotating ellipsoidal variable Rotating ellipsoidal variable Rotating ellipsoidal variables are a class of variable star. They are close binary systems whose components are ellipsoidal. They are not eclipsing, but fluctuations in apparent magnitude occur due to changes in the amount of light emitting area visible to the observer...
74 Cyg		74	205835	106711	5.04	1.03	206	A5V
			186155	96825	5.06	1.62	159	F5II	variable
26 Cyg	e	26	190147	98571	5.06	−0.54	429	K1II-III	multiple star
56 Cyg		56	198639	102843	5.06	1.93	138	A4me...	double star
75 Cyg		75	206330	106999	5.09	−0.38	404	M1IIIvar	triple star; variable
Albireo B Albireo Albireo is the fifth brightest star in the constellation Cygnus. Although it has the Bayer designation beta, it is fainter than Gamma Cygni, Delta Cygni, and Epsilon Cygni. Albireo appears to the naked eye to be a single star of magnitude 3 but through a telescope, even low magnification views...	β²	6	183914	95951	5.12	−0.19	376	B8V	component of the Albireo system; emission-line star
23 Cyg		23	188665	97870	5.14	−1.32	638	B5V
35 Cyg		35	193370	100122	5.14	−3.80	2000	F5Ib	spectroscopic binary
25 Cyg		25	189687	98425	5.15	−3.27	1575	B3IV	V1746 Cyg; γ Cas variable & β Cep variable Beta Cephei variable Beta Cephei variables are variable stars which exhibit variations in their brightness due to pulsations of the stars' surfaces. The point of maximum brightness roughly corresponds to the maximum contraction of the star. Typically, Beta Cephei variables change in brightness by 0.01 to 0.3... ; emission-line star
4 Cyg		4	183056	95556	5.17	−1.34	653	B9sp...	V1741 Cyg; spectroscopic binary
			185351	96459	5.17	2.13	132	K0III
19 Cyg		19	187849	97630	5.18	−1.29	642	M2IIIa	V1509 Cyg; variable
61 Cyg A 61 Cygni 61 Cygni,Not to be confused with 16 Cygni, a more distant system containing two G-type stars harboring the gas giant planet 16 Cygni Bb. sometimes called Bessel's Star or Piazzi's Flying Star, is a binary star system in the constellation Cygnus...		61	201091	104214	5.20	7.49	11	K5V	V1803 Cyg; BY Draconis variable BY Draconis variable BY Draconis variables are main sequence variable stars of late spectral types, usually K or M. The name comes from the archetype for this category of variable star system, BY Draconis. They exhibit variations in their luminosity due to rotation of the star coupled with star spots, and other... ; 14th nearest star system
71 Cyg	g	71	204771	106093	5.22	1.04	224	K0III
			193092	99968	5.27	−2.16	1000	K5II	variable
			204411	105898	5.29	−0.10	389	A6pe...	α²CVn variable Alpha2 Canum Venaticorum variable An Alpha2 Canum Venaticorum variable is a type of variable star. These stars are chemically peculiar main sequence stars of spectral class B8p to A7p. They have strong magnetic fields and strong silicon, strontium, or chromium spectral lines...
70 Cyg		70	204403	105942	5.30	−3.38	1772	B3V
			184875	96288	5.34	−0.64	512	A2V
27 Cyg	b¹	27	191026	99031	5.38	3.46	79	K0IV	V2008 Cyg; RS CVn variable RS Canum Venaticorum variable RS Canum Venaticorum variables are a type of variable star. They are close binary stars having active chromospheres which can cause large stellar spots. These spots are believed to cause variations in their observed luminosity...
60 Cyg		60	200310	103732	5.38	−2.73	1364	B1V	V1931 Cyg; eclipsing binary
9 Cyg		9	184759	96302	5.39	−0.70	538	A0V+...	spectroscopic binary
14 Cyg		14	185872	96693	5.41	−1.20	685	B9III
51 Cyg		51	197511	102177	5.41	−1.85	924	B2V	multiple star
ω² Cyg	ω²	46	195774	101243	5.44	−0.03	404	M2III	Ruchba, Rukbat al Dajajah, Al Rukbah al Dajajah; double star
			189178	98194	5.46	−2.90	1531	B5V	double star
			199101	103145	5.47	−0.89	609	K5III
			199098	103094	5.48	−1.31	744	K0II
			189395	98325	5.51	−0.60	544	B9Vn
49 Cyg		49	197178	102066	5.51	−1.45	805	G8IIb
			206749	107235	5.51	−0.77	587	M2III
49 Cyg		49	197177	102066	5.53	−1.43	805	G8IIb
			184293	96014	5.55	−0.22	465	K1III
			199870	103519	5.55	1.00	265	G8III
V1942 Cyg			209515	108845	5.57	−0.48	529	A0IV	α² CVn variable
36 Cyg		36	193369	100108	5.58	1.70	195	A2V
			194152	100437	5.58	0.06	415	K0IIIvar
			199955	103530	5.59	−2.35	1264	B5Vn
			204153	105769	5.59	2.91	112	F0V
			188209	97757	5.60	−7.69	14818	O9.5Ia
			198345	102635	5.60	−0.49	538	K5III
V389 Cyg			201433	104371	5.60	−0.07	444	B9V	multiple; variable
V1768 Cyg			190603	98863	5.62	−7.48	13583	B1.5Ia comp	α Cyg variables
40 Cyg		40	195050	100907	5.63	1.04	270	A3V
V380 Cyg			187879	97634	5.68	−3.80	2567	B1III	Algol variable
			196852	101899	5.68	0.31	386	K2III
			197392	102155	5.68	−1.84	1042	B8II-III
V2140 Cyg			199478	103312	5.68	−6.60	9314	B8Ia	α Cyg variables
			203644	105497	5.68	0.66	328	K0III
79 Cyg		79	206774	107253	5.69	1.08	272	A0V
			192787	99841	5.70	0.88	300	K0III
			184960	96258	5.71	3.67	83	F7V
7 Cyg		7	183534	95656	5.73	0.51	361	A1V
Gl 777 Gliese 777 Gliese 777, often abbreviated as Gl 777 or GJ 777, is a yellow subgiant approximately 52 light-years away in the constellation of Cygnus. The system is also a binary star system made up of two stars and possibly a third...			190360	98767	5.73	4.72	52	G6IV+...	binary star; has two planets Extrasolar planet An extrasolar planet, or exoplanet, is a planet outside the Solar System. A total of such planets have been identified as of . It is now known that a substantial fraction of stars have planets, including perhaps half of all Sun-like stars... (b Gliese 777 b Gliese 777 b, also known as Gliese 777 Ab or HD 190360 b, is an extrasolar planet approximately 52 light-years away in the constellation of Cygnus. The planet was discovered orbiting the primary star of the Gliese 777 system in June 2002 using the radial velocity method... & c Gliese 777 c Gliese 777 c, often catalogued as Gliese 777 Ac or simply HD 190360 c, is an extrasolar planet approximately 52 light-years away in the constellation of Cygnus. The planet was discovered orbiting the primary star of the Gliese 777 system in June 2005 using the radial velocity method... )
43 Cyg		43	195068	100859	5.73	2.85	123	F0V:	V2121 Cyg; γ Dor variable Gamma Doradus variable Gamma Doradus variables are variable stars which display variations in luminosity due to non-radial pulsations of their surface. The stars are typically young, early F or late A type main sequence stars, and typical brightness fluctuations are 0.1 magnitudes with periods on the order of one day...
77 Cyg		77	206644	107162	5.73	0.44	372	A0V
			201834	104516	5.75	0.15	431	B9III
			203245	105282	5.75	−0.33	536	B6V
			204485	106003	5.75	2.50	145	F0V
			193592	100097	5.76	1.01	291	A2Vs
DT Cyg			201078	104185	5.77	−3.05	1895	F7.5Ib-IIv	Cepheid variable Cepheid variable A Cepheid is a member of a class of very luminous variable stars. The strong direct relationship between a Cepheid variable's luminosity and pulsation period, secures for Cepheids their status as important standard candles for establishing the Galactic and extragalactic distance scales.Cepheid...
			205314	106393	5.77	−0.05	475	A0V
V2015 Cyg			196178	101475	5.78	−0.06	481	B9sp...	α² CVn variable
			188650	97985	5.79	−2.58	1538	Fp
			209419	108758	5.79	−1.77	1058	B5III
			191195	99026	5.81	3.00	119	F5V
			187235	97376	5.83	−0.05	489	B8Vn
			193322	100069	5.83	−2.56	1552	O9V
			199611	103359	5.83	2.20	174	F0III
			179957	94336	5.85	3.87	81	G4V+...
			186619	97081	5.86	−0.57	631	M0III
			192985	99889	5.87	3.18	113	F5V:
V2119 Cyg			194335	100574	5.87	−1.32	893	B2Vne	Be star
V1762 Cyg			179094	94013	5.88	1.65	229	K1IV	RS CVn variable
V1143 Cyg			185912	96620	5.89	2.89	130	F6Vasv	Algol variable
			195554	101084	5.89	−1.30	896	B9Vn
V1334 Cyg			203156	105269	5.89	−4.27	3505	F2Ib	δ Cep variable
42 Cyg		42	195324	101067	5.90	−2.67	1689	A1Ib
			188252	97774	5.91	−3.49	2470	B2III
			189684	98383	5.92	0.12	472	A5III
			199612	103360	5.92	−2.04	1273	G8II-III
			186377	96977	5.93	−3.26	2248	A5III
			200817	103956	5.93	0.46	405	K0III
69 Cyg		69	204172	105811	5.93	−3.71	2763	B0Ib
			194193	100501	5.95	−1.15	856	M0III
			199579	103371	5.96	−4.44	3928	O6...
W Cyg			205730	106642	5.96	−0.43	617	M4IIIe-M6e	semiregular variable
			197139	101986	5.97	0.17	470	K2III
V460 Cyg			206570	107129	5.98	−2.96	2000	C6.3	carbon star Carbon star A carbon star is a late-type star similar to a red giant whose atmosphere contains more carbon than oxygen; the two elements combine in the upper layers of the star, forming carbon monoxide, which consumes all the oxygen in the atmosphere, leaving carbon atoms free to form other carbon compounds,... ; variable
16 Cyg A 16 Cygni 16 Cygni or 16 Cyg is a triple star system approximately 70 light-years away from Earth in the constellation of Cygnus. It consists of two Sun-like yellow dwarf stars, 16 Cygni A and 16 Cygni B, together with a red dwarf, 16 Cygni C...	c	16	186408	96895	5.99	4.32	70	G2V	triple star system
V1743 Cyg			184786	96198	6.00	−2.26	1462	M4.5III
			192439	99579	6.01	0.50	412	K1III:
			200253	103734	6.01	−0.51	657	G5III
			204428	105891	6.01	0.35	442	B6V
			181096	94755	6.02	2.88	138	F6IV:
			197120	102033	6.02	1.45	267	A2V
			204965	106171	6.02	0.18	479	A3V
11 Cyg		11	185037	96387	6.03	−0.74	738	B8Vn
			189066	98143	6.03	−1.64	1113	B5IV
			186568	97087	6.04	−1.17	901	B8III
61 Cyg B 61 Cygni 61 Cygni,Not to be confused with 16 Cygni, a more distant system containing two G-type stars harboring the gas giant planet 16 Cygni Bb. sometimes called Bessel's Star or Piazzi's Flying Star, is a binary star system in the constellation Cygnus...		61	201092	104217	6.05	8.33	11	K7V	component of the 61 Cyg system
			203439	105432	6.05	−0.29	605	A1V
			188793	97892	6.06	0.97	339	A3V
V2130 Cyg			197018	101949	6.07	−1.13	898	B6IIIp Mn	SX Ari variable SX Arietis variable SX Arietis variables are a class of variable stars. They are high-temperature analogues of Alpha2 Canum Venaticorum variables and exhibit strong magnetic fields and intense He I and Si III spectral lines. They have brightness fluctuations of approximately 0.1 magnitudes with periods of...
			202240	104765	6.07	−2.62	1781	F0III
			203630	105558	6.07	0.77	374	K1III
76 Cyg		76	206538	107097	6.07	0.34	455	A2V
			186440	97028	6.08	1.01	337	A1V
			194097	100486	6.09	−0.26	607	K2
			185837	96724	6.10	0.29	474	A3IV
			189127	98044	6.10	0.34	462	G9III
			200577	103894	6.10	−0.41	655	G8III
			206731	107186	6.10	−1.03	869	G8II
			207516	107664	6.10	0.20	493	B8V
V1339 Cyg			206632	107140	6.11	−0.47	676	M4.5
			187638	97538	6.12	−0.53	697	G6III
			191243	99145	6.12	−2.83	2012	B5Ib
			202923	105064	6.12	0.67	401	A1V
μ² Cyg	μ²	78	206827		6.12			G2V
V2093 Cyg			187880	97651	6.13	−3.96	3396	M3III
			188149	97789	6.13	−0.65	739	K4III
			192535	99685	6.13	−0.64	738	K4III
			186927	97242	6.14	0.57	424	A2V+...
			187372	97372	6.14	−1.74	1230	M2III
V2100 Cyg			189775	98379	6.14	−0.72	769	B5III	α²CVn variable
			190964	98915	6.14	−0.64	741	M1IIIa
			195964	101285	6.14	−0.87	821	K5III
			203096	105229	6.15	−2.43	1698	A5IV
			189296	98111	6.16	1.50	279	A4Vn
			190781	98858	6.16	−0.09	579	A2IV
			206040	106771	6.16	−0.33	647	K1III
			206509	107041	6.16	−0.51	703	K0III
			186121	96805	6.17	−1.99	1399	M2III
			199892	103532	6.17	0.40	465	B7III
			202862	105101	6.17	−1.57	1152	B7Vn
			205114	106267	6.17	−1.56	1148	G2Ib+...
			205551	106518	6.17	−2.32	1630	B9III
			187038	97307	6.18	0.92	367	K2
			190771	98921	6.18	4.80	62	G5IV
			200527	103828	6.18	−1.71	1235	M3Ib-II:
			202314	104822	6.18	−3.18	2433	G2Ib
			191096	98946	6.19	2.60	170	F4V
			196379	101556	6.19	−5.54	7244	A9II
CP Cyg			205939	106752	6.19	−0.35	661	A7III	variable
			194220	100515	6.20	1.17	331	K0IIIvar
			195820	101245	6.20	1.06	348	K0III
V1619 Cyg			207857	107856	6.20	−1.39	1072	B9p HgMn	α²CVn variable
44 Cyg		44	195593	101214	6.21	−2.22	1583	F5Iab
			196642	101756	6.21	1.19	328	K0III
			186307	96907	6.22	1.62	272	A6V
			188074	97700	6.22	2.12	215	F2V
			193702	100268	6.22	1.03	355	A1V
			181960	94974	6.23	0.53	450	A1V
			189942	98563	6.23	−1.21	1003	K0III
			193944	100295	6.23	−2.26	1630	K5
			202720	105034	6.23	−0.89	865	K2
			185955	96706	6.25	0.79	402	K0III
16 Cyg 16 Cygni 16 Cygni or 16 Cyg is a triple star system approximately 70 light-years away from Earth in the constellation of Cygnus. It consists of two Sun-like yellow dwarf stars, 16 Cygni A and 16 Cygni B, together with a red dwarf, 16 Cygni C...	c	16	186427	96901	6.25	4.60	70	G5V	component of the 16 Cyg system; has a planet Extrasolar planet An extrasolar planet, or exoplanet, is a planet outside the Solar System. A total of such planets have been identified as of . It is now known that a substantial fraction of stars have planets, including perhaps half of all Sun-like stars... (b 16 Cygni Bb 16 Cygni Bb or 16 Cyg Bb is an extrasolar planet approximately 70 light-years away in the constellation of Cygnus. The planet was discovered orbiting the sun-like star 16 Cygni B, one of two solar-mass components of the triple star system 16 Cygni... )
			207446	107637	6.25	−0.41	701	K5
			183986	95953	6.26	−0.57	758	B9.5III
			198513	102712	6.26	−0.67	791	B8np
			180756	94623	6.27	1.16	342	G8III
			205349	106420	6.27	−2.05	1502	K1Ibvar
			186815	97070	6.28	1.83	253	K2III
			192934	99893	6.28	0.78	410	A1V
			186760	97033	6.29	3.02	147	G0V
			198387	102642	6.29	3.18	137	K0V:
V819 Cyg			188439	97845	6.30	−3.53	3019	B0.5IIIn	β Cep variable
			198151	102530	6.30	0.79	413	A3V
			181597	94890	6.32	0.81	413	K1III
			193217	100016	6.32	−2.49	1884	K4II:
48 Cyg		48	196606	101765	6.32	−0.58	784	B8IIIn
			200753	103949	6.32	1.79	263	F0IVn
			189432	98320	6.33	−2.33	1762	B5IV
V2136 Cyg			198625	102827	6.33	−0.92	918	B4V
			198181	102499	6.34	0.72	434	K0
			200723	103963	6.34	1.31	330	F3IV
			193469	100155	6.35	−2.98	2397	K5Ib
			186776	97151	6.36	−0.86	906	M3III
			192983	99870	6.36	1.18	355	A2Vn
			198976	103079	6.36	0.78	427	K2
			202710	105017	6.36	−2.00	1531	K0III+...
			205688	106661	6.36	1.16	357	G8III-IV
V1817 Cyg			184398	96003	6.37	−1.17	1052	K2II-IIIcomp	RS CVn variable
			186506	97029	6.37	−1.86	1442	K0
			200740	103929	6.37	0.99	388	K0
			186901	97228	6.38	−2.43	1884	B9.5V
			194069	100434	6.38	−2.01	1552	G5II+...
			195066	100808	6.38	0.26	547	B9V
			185114	96316	6.39	1.14	365	K0
V2090 Cyg			186702	97142	6.39	−0.64	830	M1III
			190227	98701	6.39	−1.31	1128	K1III
			194951	100866	6.39	−3.01	2470	F1II
			203454	105406	6.39	4.27	87	F8V
			207119	107398	6.40	−3.20	2717	K5Ib
			198237	102585	6.41	−1.61	1309	K3III
V2173 Cyg			208727	108348	6.42		985	B8V
V1351 Cyg			186532	96919	6.42	−0.44	767	M5IIIa
V1765 Cyg			187459	97485	6.42	−2.74	2218	B0.5Ibvar	β Lyr variable Beta Lyrae variable Beta Lyrae variables are a class of close binary stars. Their total brightness is variable because the two component stars orbit each other, and in this orbit one component periodically passes in front of the other one, thereby blocking its light. The two component stars of Beta Lyrae systems are...
			198820	102993	6.42	−2.47	1952	B3III
			185268	96503	6.43	−0.71	874	B5V
			195506	101133	6.43	0.91	415	K2+...
			185435	96546	6.44	−2.11	1672	K5
			189377	98253	6.44	−1.51	1268	A3V
			194882	100714	6.44	−0.88	948	A3III
			207088	107445	6.44	0.51	499	G8III
			197101	101900	6.45	0.88	424	F2Vn
			202654	104962	6.45	−1.94	1552	B4IV
			203358	105390	6.45	2.13	239	G8IV
			189253	98146	6.46	1.30	350	A1V
V1773 Cyg			193536	100142	6.46	−3.09	2650	B2V
			201836	104537	6.46	−1.86	1502	B6IV
HD 203857 HD 203857 HD 203857 is a late type K giant star in the constellation Cygnus, located nearly 920 light years away from Sun. The star is thought to form a visual binary system with the F-type bright giant BDS 10966 A, though it's likely they are actually not gravitationally bound...			203857	105637	6.46	−0.79	921	K5	has a possible planet
			185264	96396	6.47	0.11	609	G9III
			185657	96572	6.47	0.53	503	G6V
			192538	99719	6.47	−0.98	1009	A0V
			192987	99929	6.47	−1.25	1140	B6III
			195690	101268	6.47	3.20	147	F2
			200030	103596	6.47	−0.39	767	B9
X Cyg			197572	102276	6.48	−2.68	2218	G8Ib	Cepheid variable
			207673	107749	6.48	−5.62	8579	A2Ib
V1276 Cyg			186357	96988	6.49		266	F1III	δ Sct variable
			191892	99294	6.49	−1.41	1240	K0
V1584 Cyg			193722	100250	6.49	−1.38	1221	B9p Si	α²CVn variable
			194668	100651	6.49	−1.77	1462	B9.5III
			196134	101467	6.50	1.56	317	K0III-IV
			198624	102804	6.50	−1.32	1194	F7V: comp
			200465	103822	6.50	−1.68	1411	A1V comp
			200595	103871	6.50	−1.59	1353	B3Vn
HD 185269 HD 185269 HD 185269 is a seventh magnitude star approximately 153 light-years away in the constellation Cygnus. It is easily visible to binoculars, but not the naked eye....			185269	96507	6.67	3.29	155	G0IV	has a planet (b HD 185269 b HD 185269 b is a hot Jupiter extrasolar planet approximately 153 light years away in the constellation of Cygnus. The minimum mass is slightly less than Jupiter and the orbital period is about one week... )
WR 136 WR 136 WR 136, a Wolf–Rayet star.-References:* http://jumk.de/astronomie/big-stars/wr-136.shtml* http://www.springerlink.com/content/04205412121836v4/* http://chandra.harvard.edu/photo/2003/ngc6888/* http://www.giga-parsec.de/WRspectra.html...			192163	99546	7.48	−3.57	5279	WN6	Wolf–Rayet Star
HD 187123 HD 187123 HD 187123 is an 8th magnitude G-type main sequence star located approximately 156 light-years away in the constellation of Cygnus. Like our Sun, it is a yellow dwarf . Being at a distance of about 160 light-years it is not visible to the unaided eye...			187123	97336	7.86	4.46	163	G5	has two planets (b HD 187123 b HD 187123 b is a typical "hot Jupiter" located approximately 156 light-years away in the constellation of Cygnus, orbiting the star HD 187123. It has a mass about half that of Jupiter and it orbits in a very tight, round orbit around the star every three days... & c HD 187123 c HD 187123 c is an extrasolar planet located approximately 156 light-years away in the constellation of Cygnus, orbiting the star HD 187123. This planet was discovered in 1998 and published in 2006. The radius of the planet's orbit is 4.80 AU, 113 times more distant from the star than first... )
χ Cyg Chi Cygni Chi Cygni is a variable star of the Mira type in the constellation Cygnus.Chi Cygni shows one of the largest variations in magnitude known. Typically it brightens and fades from 5th to 13th magnitude. The average period of this brightness fluctuation is 407 days. Observed extremes were 3.3 and...	χ		187796	97629	7.91	2.78	346	S7,1e:	Mira variable Mira variable Mira variables , named after the star Mira, are a class of pulsating variable stars characterized by very red colors, pulsation periods longer than 100 days, and light amplitudes greater than one magnitude in infrared and 2.5 magnitude in visual... ; V_max = 3.62^m, V_min = 15.00^m
R Cyg			185456		8.15			S...	Mira variable
RT Cyg			186686	97068	8.45	−1.85	3749	M3e	Mira variable
U Cyg			193680	100219	8.77	−1.00	2938	R....	Mira variable
Cygnus X-1 Cygnus X-1 Cygnus X-1 is a well-known galactic X-ray source in the constellation Cygnus. It was discovered in 1964 during a rocket flight and is one of the strongest X-ray sources seen from Earth, producing a peak X-ray flux density of 2.3 Wm−2Hz−1...			185456	98298	8.95	−2.23	>6000	O9.7Iab	V1357 Cyg; X-ray binary X-ray binary X-ray binaries are a class of binary stars that are luminous in X-rays.The X-rays are produced by matter falling from one component, called the donor to the other component, called the accretor, which is compact: a white dwarf, neutron star, or black hole.The infalling matter releases... one component being a black hole Black hole A black hole is a region of spacetime from which nothing, not even light, can escape. The theory of general relativity predicts that a sufficiently compact mass will deform spacetime to form a black hole. Around a black hole there is a mathematically defined surface called an event horizon that...
47 Cyg B		47	196094		9.40			K2Ib+...	component of 47 Cyg system
HAT-P-11 HAT-P-11 HAT-P-11, also designated GSC 03561-02092, is an orange dwarf metal rich star about 123 light-years away in the constellation Cygnus. This star is notable for its relatively large rate of proper motion. The magnitude of this star is about 9, which means it is not visible to the naked eye but can be...					9.59	6.69	123	K4	has a transiting planet (b HAT-P-11b HAT-P-11b is an extrasolar planet orbiting the star HAT-P-11. This planet was discovered by the transit method and submitted for publication on January 2, 2009.... )
Campbell's star			184738	96295	10.45			WC...	V1966 Cyg
HAT-P-7 HAT-P-7 HAT-P-7 is a yellow white dwarf star located about 1044 light-years away in the constellation Cygnus. The apparent magnitude of this star is 10.5, which means it is not visible to the naked eye but can be seen with a small telescope on a clear dark night.-Planetary system:This star has one known...					10.5		1044	F8	has a transiting Astronomical transit The term transit or astronomical transit has three meanings in astronomy:* A transit is the astronomical event that occurs when one celestial body appears to move across the face of another celestial body, hiding a small part of it, as seen by an observer at some particular vantage point... planet (b HAT-P-7b HAT-P-7b is an extrasolar planet discovered in 2008. It orbits very close to its parent star GSC 03547-01402, and is both larger and more massive than Jupiter. Due to the extreme heat it receives from its star, the dayside temperature is predicted to be 2730 K... )
HAT-P-17 HAT-P-17 HAT-P-17 is a K type star about 90 ± 3 pc away. It has a mass of about 0.857 ± 0.039 M☉. It is the host of two planets, HAT-P-17b and HAT-P-17c, both discovered in 2010.- References :*...					10.54		293.5	G0	has two planets (b & c)
WASP-48					11.06				has a transiting planet (b)
Kepler-6 Kepler-6 Kepler-6 is a yellow giant situated in the constellation Cygnus. The star lies within the field of view of the Kepler Mission, which discovered it as part of a NASA-led mission to discover Earth-like planets...					13.8	4.4	2522	G4	has a transiting planet (b Kepler-6b Kepler-6b is an extrasolar planet in the orbit of the unusually metal-rich Kepler-6, a star in the field of view of the NASA-operated Kepler spacecraft, which searches for planets that cross directly in front of, or transit, their host stars. It was the third planet to be discovered by Kepler.... )
Kepler-5 Kepler-5 Kepler-5 is a star located in the constellation Cygnus in the field of view of the Kepler Mission, a NASA project aimed at detecting planets in transit of, or passing in front of, their host stars as seen from Earth. One closely orbiting, Jupiter-like planet, named Kepler-5b, has been detected...					13.9	3.3	4167	F8	has a transiting planet (b Kepler-5b Kepler-5b is one of the first five planets discovered by NASA's Kepler spacecraft. It is a Hot Jupiter that orbits a subgiant star that is more massive, larger, and more diffuse than the Sun is... )
Kepler-11 Kepler-11 Kepler-11 is a sun-like star slightly larger than the Sun in the constellation Cygnus, located some 2,000 light years from Earth. It is located within the field of vision of the Kepler spacecraft, the satellite that NASA's Kepler Mission uses to detect planets that may be transiting their stars...					14.2		1999	G	has six transiting planets (b Kepler-11b Kepler-11b is an exoplanet discovered in the orbit of the star Kepler-11 by the Kepler spacecraft, a NASA-led mission to discover Earth-like planets. Kepler-11b is four times more massive and twice as large as Earth, but it has a lighter density estimated at a little over half Earth's, and is... , c Kepler-11c Kepler-11c is an exoplanet discovered in the orbit of the sun-like star Kepler-11 by the Kepler spacecraft, a NASA telescope aiming to discover Earth-like planets. It is the second planet from its parent star, and is most likely a water planet with a thin hydrogen–helium atmosphere. Kepler-11c... , d Kepler-11d Kepler-11d is an exoplanet discovered in the orbit of the sun-like star Kepler-11. It is named for the telescope that discovered it, a NASA spacecraft named Kepler that is designed to detect Earth-like planets by measuring small dips in the brightness of their host stars as the planets cross in front... , e Kepler-11e Kepler-11e is an exoplanet discovered in the orbit of the sunlike star Kepler-11. It is the fourth of six planets around Kepler-11 discovered by NASA's Kepler spacecraft. Kepler-11e was found by using the transit method, in which a the dimming effect that a planet causes as it crosses in front of... , f Kepler-11f Kepler-11f is an exoplanet discovered in the orbit of the sunlike star Kepler-11 by NASA's Kepler spacecraft, which searches for planets that transit their host stars. Kepler-11f is the sixth planet from its star, orbiting one fourth of the distance of the Earth from the Sun every 47 days... & g)
V1500 Cyg V1500 Cygni V1500 Cygni or Nova Cygni 1975 was a bright nova occurring in 1975 in the constellation Cygnus.V1500 Cygni was discovered on August 29 and reached magnitude 1.7 on the next day. It remained visible to the naked eye for about a week...					17.1				Nova Nova A nova is a cataclysmic nuclear explosion in a star caused by the accretion of hydrogen on to the surface of a white dwarf star, which ignites and starts nuclear fusion in a runaway manner... Cygni 1975; V_max = 2.0^m
V476 Cyg V476 Cygni V476 Cygni or Nova Cygni 1920 was a nova which occurred in the constellation Cygnus in 1920. It reached a brightness of 2.0 mag. Nowadays its brightness is 17.09 mag.Coordinates :Right ascension: 19h 58m 24,6sDeclination: +53° 37’ 07"...							~200		Nova Cygni 1920; V_max = 2.0^m
V1668 Cyg V1668 Cygni V1668 Cygni was a nova that appeared in the constellation Cygnus in 1978 with a maximum brightness of 6th apparent magnitude....									Nova Cygni 1978; V_max = 6.0^m
AFGL 2591 AFGL 2591 \|- style="vertical-align: top;"\| Distance \| 3261.6 LyAFGL 2591 is a young, massive star in the constellation Cygnus. It is more than 3,000 light-years from Earth, at least 10 times the size of the Sun, and over 20,000 times as bright...							3261.6		associated Rfn Nebula
V1974 Cyg V1974 Cygni V1974 Cygni or Nova Cygni 1992 was a relatively bright nova in the constellation Cygnus.It was discovered on February 19, 1992 by Peter Collins. At that time it was magnitude 6, the maximum magnitude reached was 4.4. The hydrogen burning on the white dwarf ended two years later, in 1994. This nova...									Nova Cygni 1992; V_max = 4.5^m

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