List of stars in Aquila - 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....

Aquila
Aquila (constellation)
Aquila is a stellar constellation. Its name is Latin for 'eagle' and it is commonly represented as such. In mythology, Aquila was owned by the Roman god Jupiter and performed many tasks for him....

, 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
Altair	α	53	187642	97649	0.76	2.20	17	A7IV-V	Atair, Al Nesr Al Tair, Vulture Volans; 12th brightest star; nearby; has two optical components 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... ; 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...
γ Aql	γ	50	186791	97278	2.72	−3.03	460	K3II	Tarazed, Tarazad, Reda, Menkib al Nesr, Humerus Vulturis; 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... ; suspected variable
ζ Aql Zeta Aquilae Zeta Aquilae is a triple star system in the constellation Aquila. It has the traditional names Deneb el Okab, from an Arabic term ذنب العقاب ðanab al-cuqāb meaning "the tail of the falcon", and the Mandarin names Woo and Yuë, derived from and represent the state Wu , an old state was located at...	ζ	17	177724	93747	2.99	0.96	83	A0Vn	Deneb el Okab, Denebokab Australis, Woo, Yuë (吳越), Dzeneb al Tair, Cauda (Vulturis) Volantis; triple star
θ Aql Theta Aquilae Theta Aquilae is a binary star in the constellation Aquila. It is approximately 287 light years from Earth. It has the traditional name Tseen Foo, which is derived from the Mandarin 天桴 tiānfú meaning "the heavenly raft"; it may also mean drumsticks, with Altair, Beta Aquilae and Gamma Aquilae...	θ	65	191692	99473	3.24	−1.48	287	B9.5III	Tseen Foo, Thanih Ras al Akab, Secunda Capitis Vulturis; spectroscopic binary; suspected variable
δ Aql Delta Aquilae Delta Aquilae is a triple star system in the constellation Aquila. It is approximately 50.1 light years from Earth.Sometimes, this star is called by the name Denebokab, meaning the tail of eagle in Arabic...	δ	30	182640	95501	3.36	2.43	50	F0IV	Denebokab, Song, Sung, Djenubi Menkib al Nesr, Australior Humerus Vulturis; 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... ; suspected variable
λ Aql	λ	16	177756	93805	3.43	0.51	125	B9Vn	Al Thalimain
β Aql	β	60	188512	98036	3.71	3.03	45	G8IVvar	Alshain, Alschain, Alschairn, Unuk al Ghyrab, Collum Corvi; 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... ; suspected variable; triple star; suspected variable
η Aql Eta Aquilae Eta Aquilae is a star in the constellation Aquila. It was also part of the former constellation Antinous. It is a Cepheid variable star, varying from apparent magnitude 3.5 to 4.4 with a period of 7.176641 days...	η	55	187929	97804	3.87	−3.91	1173	F6Ib-G4Ib	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... ,
ε Aql	ε	13	176411	93244	4.02	0.65	154	K2III	Deneb el Okab, Denebokab Borealis, Woo, Yuë (吳越); triple star
12 Aql	i	12	176678	93429	4.02	0.73	149	K1IIIvar	suspected variable
71 Aql	l	71	196574	101847	4.31	−1.04	384	G8III SB	spectroscopic binary
ι Aql	ι	41	184930	96468	4.36	−0.51	307	B5III	Al Thalimain; double star
μ Aql	μ	38	184406	96229	4.45	1.80	111	K3III	multiple star; suspected variable
ν Aql Nu Aquilae Nu Aquilae is a star in the constellation Aquila.Nu Aquilae is a yellow-white F-type supergiant with an apparent magnitude of +4.64. It is at least 3000 light years from Earth and lies close to the celestial equator.-References:...	ν	32	182835	95585	4.64	−8.12	11643	F2Ib	double star; suspected variable
ξ Aql Xi Aquilae - External links :* * *...	ξ	59	188310	97938	4.722	5.769	204	G9IIIb	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 Xi Aquilae b Xi Aquilae b is an extrasolar planet approximately 200 light-years away in the constellation of Aquila. The planet was discovered orbiting the yellow giant star Xi Aquilae in 2008. The planet has a minimum mass of 2.8 Jupiter and a period of 137 days.... )
69 Aql 69 Aquilae 69 Aquilae is a star in the constellation Aquila. Its apparent magnitude is 4.91....		69	195135	101101	4.91	1.07	191	K2III
70 Aql 70 Aquilae 70 Aquilae is a star in the constellation Aquila. Its apparent magnitude is 4.91....		70	196321	101692	4.91	−4.24	2203	K5II
κ Aql Kappa Aquilae Kappa Aquilae is a star in the constellation Aquila.Kappa Aquilae is a blue-white B-type giant with an apparent magnitude of +4.93. It is approximately 1460 light years from Earth.-References:* * *...	κ	39	184915	96483	4.93	−3.32	1455	B0.5III
26 Aql	f	26	181391	95066	4.98	1.61	154	G8III-IV...	spectroscopic binary
4 Aql 4 Aquilae 4 Aquilae is a star in the constellation Aquila. Its apparent magnitude is 5.02....		4	173370	91975	5.02	−0.78	472	B9V
36 Aql 36 Aquilae 36 Aquilae or e Aquilae is a star in the constellation Aquila. Its apparent magnitude is 5.03.-References:* *...	e	36	183630	95937	5.03	−0.91	502	M1IIIvar	suspected variable
18 Aql 18 Aquilae 18 Aquilae or Y Aquilae is a star in the constellation Aquila. Its apparent magnitude is 5.07.-Components:-References:* *...		18	178125	93867	5.07	−0.89	507	B8III	Y Aql; double star; eclipsing binary
23 Aql		23	180972	94885	5.10	−0.24	381	K2II-IIIvar	triple star
37 Aql 37 Aquilae 37 Aquilae is a G-type giant star in the constellation of Aquila. It has an apparent visual magnitude of approximately 5.137....		37	184492	96327	5.12	−0.55	444	G8III
ο Aql	ο	54	187691	97675	5.12	3.68	63	F8V	multiple star system
21 Aql 21 Aquilae 21 Aquilae or V1288 Aquilae is a star in the constellation Aquila. Its apparent magnitude is 5.14.-Components:-References:* * * *...		21	179761	94477	5.14	−1.33	640	B8II-IIIp(Hg:)	V1288 Aql; double star; α² CVn 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... ,
31 Aql	b	31	182572	95447	5.17	4.27	49	G8IVvar	triple star; suspected variable
σ Aql Sigma Aquilae Sigma Aquilae is a binary star in the constellation Aquila. It is approximately 680 light years from Earth.Sigma Aquilae is an eclipsing spectroscopic binary. Both components are detached blue-white B-type main sequence dwarfs which do not fill their Roche lobes. The mean apparent magnitude of...	σ	44	185507	96665	5.18	−1.42	682	B3V + B3V	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... ,
19 Aql 19 Aquilae 19 Aquilae is a star in the constellation Aquila. Its apparent magnitude is 5.23.-Alternate designations:HR 7266HD 178596SAO 124318BD +5 4040*FK5: 3530...		19	178596	94068	5.23	2.03	142	F0III-IV
11 Aql 11 Aquilae 11 Aquilae is a binary star in the constellation Aquila. The stars making up the pair are apparent magnitudes 5.7 and 9.2. There is a noticeable color difference between the two components. They are approximately 155 light years away.-References:*...		11	176303	93203	5.27	1.88	155	F8V	triple star; suspected variable
ω¹ Aql Omega¹ Aquilae Omega1 Aquilae is an F-type subgiant star in the constellation of Aquila. It has an apparent visual magnitude of approximately 5.300 and is approximately 420 light-years from the Earth.-External links:* *...	ω¹	25	180868	94834	5.28	−0.28	422	F0IV
χ Aql A Chi Aquilae Chi Aquilae is a double star in the constellation Aquila. It is approximately 750 light-years from Earth.The more luminous component is a yellow G-type giant with an apparent magnitude of +5.6. It has a white A-type main sequence dwarf companion with an apparent magnitude of +6.8...	χ	47	186203	96957	5.28	−1.53	751	F3V:+...	multiple star system 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...
φ Aql Phi Aquilae Phi Aquilae is a binary star in the constellation Aquila.Phi Aquilae is a spectroscopic binary which is classified as a white A-type subgiant with an apparent magnitude of +5.28. The binary has an orbital period of 3.32 days and is approximately 206 light years from Earth.-References:* * *...	φ	61	188728	98103	5.28	1.28	206	A1IV	spectroscopic binary; suspected variable
132 G. Aql			194013	100541	5.30	0.91	246	G8III-IV
FF Aql FF Aquilae FF Aquilae is a classical cepheid variable .-External links:* * *...			176155	93124	5.33	−4.07	2470	F5Ia-F8Ia	double star; Cepheid variable,
20 Aql 20 Aquilae 20 Aquilae is a star in the constellation Aquila. Its apparent magnitude is 5.35.Other designations:BD -08 4887,GC 26461,HD 179406,SAO 143134,HIP 94385....		20	179406	94385	5.35	−2.51	1216	B3V
51 Aql 51 Aquilae 51 Aquilae is a star in the constellation Aquila. Its apparent magnitude is 5.38.-Components:-References:* * *...		51	187532	97650	5.38	3.27	86	F0V	binary star
14 Aql 14 Aquilae 14 Aquilae or is a star in the constellation Aquila. Its apparent magnitude is 5.40.-References:* * *...	g	14	176984	93526	5.40	−0.53	499	A1V	double star
15 Aql 15 Aquilae 15 Aquilae is a double star in the constellation Aquila. Its apparent magnitude is 5.40. It's composed of a magnitude 5 yellow star and a magnitude 7 star, resolvable in a small telescope.-Components:-References:*...	h	15	177463	93717	5.40	0.41	325	K1III	double star; suspected variable
66 Aql 66 Aquilae 66 Aquilae is a star in the constellation Aquila. Its apparent magnitude is 5.44....		66	192107	99631	5.44	−1.74	888	K5III
42 Aql 42 Aquilae 42 Aquilae is a star in the constellation Aquila. Its apparent magnitude is 5.45....		42	185124	96556	5.45	2.92	105	F3IV
27 Aql 27 Aquilae 27 Aquilae is a B-type giant star in the constellation of Aquila. It has an apparent visual magnitude of approximately 5.460....	d	27	181440	95073	5.46	−0.51	509	B9III
τ Aql Tau Aquilae Tau Aquilae is a star in the constellation Aquila.Tau Aquilae is an orange K-type giant with an apparent magnitude of +5.51. It is approximately 527 light years from Earth.-References:* *...	τ	63	190327	98823	5.51	−0.53	527	K0III
28 Aql 28 Aquilae 28 Aquilae or V1208 Aquilae is a star in the constellation Aquila. Its apparent magnitude is 5.53. The primary has an FO spectrum. It has a 9.0 magnitude companion at 59.7".-References:* * *...	A	28	181333	94982	5.53	0.39	347	F0III	V1208 Aql; triple star; δ Sct variable,
			183492	95822	5.57	0.85	286	K0III
62 Ser 62 Serpentis 62 Serpentis is a variable star. Despite its name, the star can be found in the constellation Aquila.-External links:**...		62	175515	92872	5.58	0.81	293	G9III	suspected variable
			180262	94624	5.58	−0.79	613	G8II-III	double star
22 Aql 22 Aquilae 22 Aquilae is a star in the constellation Aquila. Its apparent magnitude is 5.59.Other designations:22 Aql, AG +04 2489, BD +04 4045, GC 26567, 2MASS J19163102+0450052, HD 180482, HIP 94727....		22	180482	94727	5.59	−0.53	546	A3IV
58 Aql 58 Aquilae 58 Aquilae is a star in the constellation Aquila. Its apparent magnitude is 5.60.It is a constellation in the Northern Hemisphere and the Milky Way near Aquarius and Serpens Cauda....		58	188350	97980	5.60	0.48	345	A0III
V1291 Aql V1291 Aquilae V1291 Aquilae is variable star.-References:* *... (90 G. Aql)			188041	97871	5.63	0.99	277	A5p(Sr-Cr-Eu)	α² CVn variable,
45 Aql 45 Aquilae 45 Aquilae or IDS 19356-0051 A is star in double system.-References:* * *...		45	185762	96807	5.64	0.93	285	A3IV	double star
			180555	94720	5.65	0.36	372	B9.5V	binary star
62 Aql 62 Aquilae 62 Aquilae is a star in the constellation Aquila. Its apparent magnitude is 5.67....		62	190299	98844	5.67	−0.59	582	K4III
π Aql B Pi Aquilae Pi Aquilae or 52 Aquilae is a triple star in the constellation Aquila. It is approximately 570 light years from Earth....	π	52	187260		5.70				component of the π Aql system
57 Aql A 57 Aquilae 57 Aquilae or IDS 19492-0829 A is a double star in the constellation Aquila. Its apparent magnitude is 5.28. The magnitude 6 components can already be resolved using a weak telescope.-References:* * * -Components:...		57	188293	97966	5.70	0.64	335	B7Vn	double star
14 Sge 14 Sagittae 14 Sagittae or HD 190229 is a star, in the Aquila constellation.-References:* *...		14	190229	98754	5.73	−0.72	637	B9MNp...
π Aql Pi Aquilae Pi Aquilae or 52 Aquilae is a triple star in the constellation Aquila. It is approximately 570 light years from Earth....	π	52	187259	97473	5.75	−0.46	570	F2V:+...	component of the π Aql system
			182900	95572	5.76	2.03	182	F6III
56 Aql 56 Aquilae 56 Aquilae is a star in the constellation Aquila. Its apparent magnitude is 5.76, meaning it would be barely visible to the naked eye, under ideal conditions.It was discovered by nineteenth Century Astronomer John Herschel....		56	188154	97928	5.76	0.35	394	K5III	double star
35 Aql 35 Aquilae 35 Aquilae or V1431 Aquilae, c Aquilae is a star in the constellation Aquila. Its apparent magnitude is 5.79.-References:* *...	c	35	183324	95793	5.79	1.94	192	A0V	V1431 Aql; rapidly oscillating α² CVn variable,
42 G. Aql			181907	95222	5.81	0.58	363	G8III:
13 G. Aql			177178	93580	5.82	2.11	180	A4V
49 G. Aql			183227	95732	5.84	−1.65	1025	B6III
100 G. Aql			189340	98416	5.87	3.92	80	F8V
5 Aql		5	173654	92117	5.89	1.40	258	A2m	binary star
υ Aql Upsilon Aquilae Upsilon Aquilae is a star in the constellation Aquila.Upsilon Aquilae is a white A-type subgiant with an apparent magnitude of +5.89. It is approximately 176 light years from Earth.-References:* *...	υ	49	186689	97229	5.89	2.22	176	A3IV
103 G. Aql			189695	98526	5.90	−1.30	898	K5III
10 Aql		10	176232	93179	5.91	1.55	242	A4p(Eu-Cr-Sr)	V1286 Aql; α² CVn variable,
64 Aql 64 Aquilae 64 Aquilae is a star in the constellation Aquila. Its apparent magnitude is 5.97....		64	191067	99171	5.97	2.57	156	K1IV
			185018	96481	5.98	−1.74	1140	G0Ib	multiple star
QS Aql QS Aquilae \|- bgcolor="#FFFAFA"\| duration of the eclipse \|\| 17 % of period the duration of the light constancy phase at minimum light is equal to zeroQS Aquilae is eclipsing binary of Algol type.-References:* * *...			185936	96840	5.98	−2.54	1646	B5V	double star; 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... ,
80 G. Aql			187195	97499	6.00	1.29	285	K5III
ω² Aql Omega² Aquilae Omega2 Aquilae is an A-type main sequence star in the constellation of Aquila. It has an apparent visual magnitude of approximately 6.023 and is approximately 280 light years from the Earth.-External links:* *...	ω²	29	181383	95002	6.03	1.37	278	A2V
131 G. Aql			193329	100232	6.05	0.58	405	K0
8 Aql 8 Aquilae 8 Aquilae is a star in the constellation Aquila. Its apparent magnitude is 6.08.-References:* *...		8	174589	92524	6.08	1.44	276	F2III	Delta Scuti 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...
53 G. Aql			183589	95898	6.08	−2.46	1663	K5Ib	multiple star; suspected variable
R Aql R Aquilae R Aquilae is a variable star in the constellation Aquila.-References:* *...			177940	93820	7.61	8.75	700	M7IIIev	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... ,
V923 Aql V923 Aquilae V923 Aquilae is a Be star.-References:* *... (55 G. Aql)			183656	95929	6.09	−1.26	962	B5.5IIIpe-B8V	γ Cas variable,
137 G. Aql			194454	100758	6.10	−0.60	713	K1III:
85 G. Aql			187660	97687	6.12	−0.09	570	K5III
68 Aql 68 Aquilae 68 Aquilae is a star in the constellation Aquila. Its apparent magnitude is 6.12.-References:* * -Components:...		68	194939	100977	6.12	−0.04	557	B9V	double star
96 G. Aql			188385	97970	6.14	1.60	263	A2V	double star
135 G. Aql			194244	100664	6.14	−0.92	840	B9V	triple star; suspected variable
			187923	97767	6.16	3.95	90	G0V	double star; suspected variable
101 G. Aql			189322	98385	6.17	−0.69	769	G8III
34 G. Aql			180782	94833	6.19	1.56	275	A1Vn
6 G. Aql			175640	92963	6.20	0.17	525	B9III
145 G. Aql			196426	101746	6.21	−0.26	643	B8IIIp
7 G. Aql			176095	93138	6.22	2.45	185	F5IV
4 G. Aql			174240	92386	6.24	0.01	575	A1V
12 G. Aql			176981	93488	6.25	−0.83	849	K2III
52 G. Aql			183387	95812	6.25	−0.08	603	K2
ψ Aql Psi Aquilae Psi Aquilae is a star in the constellation Aquila.Psi Aquilae is a blue-white B-type giant with an apparent magnitude of +6.25. It is approximately 810 light years from Earth.-References:* *...	ψ	48	186547	97139	6.25	−0.72	809	B9III-IV
88 G. Aql			187753	97697	6.25	0.92	380	A1m
120 G. Aql			191984	99585	6.25	−0.08	603	A0	double star
37 G. Aql			181122	94916	6.31	0.31	517	G9III
43 G. Aql			182038	95281	6.31	0.41	493	K0
			183144	95664	6.31	−0.73	834	B4III	suspected variable
71 G. Aql			185966	96917	6.31	1.26	334	K2
60 G. Aql			184573	96356	6.32	1.13	355	K0
46 Aql 46 Aquilae 46 Aquilae is a seventh magnitude star in the constellation Aquila. It is approximately 700 light years from Earth....		46	186122	96931	6.33	−0.39	720	B9III
25 G. Aql			178744	94149	6.34	−0.80	874	B5Vn
44 G. Aql			182101	95253	6.34	3.58	116	F6V
			191263	99234	6.34	−2.42	1842	B3IV
V450 Aql V450 Aquilae V450 Aquilae is semi-regular pulsating star.-References:* * *...			184313	96204	6.35	−0.75	858	M5III-M8III	semiregular variable,
67 G. Aql			185423	96630	6.36			B3III
			174569	92475	6.37	−2.41	1863	K5III+...	double star
U Aql U Aquilae U Aquilae or ADS 12503 A is classical Cepheid variable .-Components:-References:*...			183344	95820	6.37	−2.07	1590	F5-G1I-II	Cepheid variable,
61 G. Aql			184663	96351	6.37	3.25	137	F6IV
			184944	96428	6.37	1.19	354	K0II-III
V1472 Aql V1472 Aquilae V1472 Aquilae is a semi-regular pulsating star.-References:* * *...			190658	98954	6.37	−0.44	749	M2 comp	eclipsing variable,
V1401 Aql V1401 Aquilae V1401 Aquilae is semi-regular pulsating star.-References:* *... (108 G. Aql)			190390	98910	6.38	−1.58	1273	F1III	semiregular variable,
24 Aql 24 Aquilae 24 Aquilae is a star in the constellation Aquila. Its apparent magnitude is 6.40.-References:* * -Components:...		24	181053	94913	6.40	0.52	488	K0II-III:..	multiple star
136 G. Aql			194263	100672	6.41	−0.71	865	K5
75 G. Aql			186535	97144	6.43	1.00	398	K0
114 G. Aql			191104	99158	6.43	3.25	141	F3V	double star
			187203	97454	6.44	−2.22	1762	F8Ib-II
128 G. Aql HD 192699 HD 192699 is a yellow subgiant star located approximately 220 light-years away in the constellation of Aquila. It has the apparent magnitude of 6.45. Based on its mass of 1.68 solar, it was an A-type star when it was a main-sequence...			192699	99894	6.44	2.30	220	G8IV	has a planet (b HD 192699 b HD 192699 b is an exoplanet located approximately 220 light-years away in the constellation of Aquila, orbiting the star HD 192699. This planet was discovered in April 2007, massing at least 2.5 times the mass of Jupiter... )
30 G. Aql			179791	94478	6.47	0.15	598	A3V	suspected variable
77 G. Aql			186660	97244	6.47	−1.14	1087	B3III
87 G. Aql			187734	97709	6.47			K0...	double star
110 G. Aql			190664	99024	6.47	1.37	341	K0
122 G. Aql			192086	99624	6.47	−1.94	1567	K5
142 G. Aql			195617	101339	6.47	−1.23	1132	K2
V Aql V Aquilae V Aquilae is a carbon star in the constellation Aquila. This is a type of star with a spectrum that is dominated by strong absorption lines of the molecules C2 and CN. The enhanced levels of carbon in the atmosphere may have been contributed by recently nucleosyntesized material that has been...			177336	93666	6.48	−1.36	1207	C5,4 - C6,4(N6)	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,... ; semiregular variable,
V1339 Aql V1339 Aquilae V1339 Aquilae is a Be star. Binary star nature discovered by speckle interferometry.-References:* *... (84 G. Aql)			187567	97607	6.49	−1.90	1552	B2.5IVe	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... ; γ Cas variable,
57 Aql B 57 Aquilae 57 Aquilae or IDS 19492-0829 A is a double star in the constellation Aquila. Its apparent magnitude is 5.28. The magnitude 6 components can already be resolved using a weak telescope.-References:* * * -Components:...		57	188294	97967	6.49	1.27	361	B8V	component of the 57 Aql system
97 G. Aql			188405	98038	6.49	1.83	279	F2V	double star
V1691 Aql (45 G. Aql)			182475	95453	6.50	1.48	329	A9V	δ Sct variable
TT Aql TT Aquilae TT Aquilae is a classical Cepheid variable .- References :* * * *...			178359	93990	7.10	−4.84	7951	F6-G5	Cepheid variable,
HD 183263 HD 183263 HD 183263 is an 8th magnitude subgiant star located approximately 172 light-years away in the constellation Aquila. This star is about to or already ran out of hydrogen fuel and eventually becomes a red giant and then dies as a white dwarf...			183263	95740	7.86	4.25	172	G2IV	has two planets (b HD 183263 b HD 183263 b is an extrasolar planet orbiting the star HD 183263. This planet has a minimum mass of 3.69 times more than Jupiter and takes 1.7364 years to orbit the star... & c HD 183263 c HD 183263 c is an exoplanet orbiting approximately 4.25 AU from the parent star HD 183263. This planet was announced by Wright et al. on December 8, 2008 using multiple observations in Lick and Keck Observatories earlier in that year. This planet was calculated to have minimum mass of 3.82 times... )
V1703 Aql			192263	99711	8.10	6.61	65	K2V	double star; has a planet (b HD 192263 b HD 192263 b is a gas giant planet with a mass about three quarters that of Jupiter mass. It orbits the star in a circular orbit completing one revolution in 24 days or so.... )
V603 Aql V603 Aquilae V603 Aquilae was a bright nova occurring in Aquila in 1918.It reached a magnitude of −1.4, and was the brightest nova of modern times.-References:* -External links:* * *...			174107	92316	11.64	4.76	776	pec(NOVA) - e+cont	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... Aquilae 1918;
V500 Aql V500 Aquilae V500 Aquilae or Nova Aquilae 1943 was a nova which appaeared in the constellation Aquila in 1943 and reached a brightness of 6.1 mag. Its brightness decreased in 30 days around 3 mag.-External links:* * * * * *...					6.1			pec(NOVA) - e+cont	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... Aquilae
V1494 Aql V1494 Aquilae V1494 Aquilae or NOVA Aquilae 1999 b was a nova which occurred in 1999 in the constellation Aquila and which reached a brightness of 4.0 mag.-References:* -External links:* * * * * * *...					8.8			pec(NOVA) - e+cont	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... Aquilae
V604 Aql V604 Aquilae V604 Aquilae or Nova Aquilae 1905 was a nova, which occurred in the constellation Aquila in 1905 with a maximum brightness of 7.6 mag.-External links:* * * *...					7.6			pec(NOVA) - e+cont	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... Aquilae
HD 179079 HD 179079 HD 179079 is a G-type subgiant star in the constellation of Aquila. It has an apparent visual magnitude of approximately 7.96. It is larger than our Sun as it has a radius of approximately 1.48 solar radii. An exoplanet, HD 179079 b, was announced in August 2009 to be orbiting this star...			179079	94256	7.96	3.94	208	G5IV	has a planet (b HD 179079 b HD 179079 b is an extrasolar planet which orbits the G-type subgiant star HD 179079, located approximately 208 light years away in the constellation Aquila. This planet has mass only 1/12 that of Jupiter or 1.5 times Neptune. The planet orbits very close to the star, at a distance of 0.11 AU. This... )
V606 Aql V606 Aquilae V606 Aquilae was a nova, which lit up in the constellation Aquila in 1899. It reached 5.5 magnitude.- External links :* * * * * * * * *...								pec(NOVA) - e+cont	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... Aquilae
W50 (nebula) W50 (nebula) W50 or SNR G039.7-02.0 is a Supernova remnant located in the Aquila constellation, about 18,000 light years away. In its centre lies the micro-quasar SS 433, whose jets are distorting the remnant's shell. Most likely W50 and SS443 are related objects, remnants from a supernova which occurred about...							16000		Supernova remnant
χ Aql B Chi Aquilae Chi Aquilae is a double star in the constellation Aquila. It is approximately 750 light-years from Earth.The more luminous component is a yellow G-type giant with an apparent magnitude of +5.6. It has a white A-type main sequence dwarf companion with an apparent magnitude of +6.8...	χ	47	186204		12.30		800	G0:+A3V	component of the χ Aql system
COROT-2 COROT-2 COROT-2 is a yellow dwarf main sequence star a little cooler than the Sun. This star is located approximately 930 light-years away in the constellation of Aquila...					12.57		930	G7V	has a transiting planet (b)
COROT-3 COROT-3 COROT-3 is a white-yellow dwarf main sequence star hotter than our Sun. This star is located approximately 2200 light-years away in the constellation of Aquila...					13.3		2200	F3V	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... brown dwarf Brown dwarf Brown dwarfs are sub-stellar objects which are too low in mass to sustain hydrogen-1 fusion reactions in their cores, which is characteristic of stars on the main sequence. Brown dwarfs have fully convective surfaces and interiors, with no chemical differentiation by depth... (b)
COROT-8					14.80	6.89	~1250	K1V	text-align:left; > has a transiting planet (b)
COROT-10					15.22	7.53	~1130	K1V	text-align:left; > has a transiting planet (b)
VB 10 VB 10 VB 10, also referred to as Van Biesbroeck's star, is a very small and very dim M-type red dwarf star located in the constellation Aquila...					17.30	18.47	19	M8V	has a planet (b)

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