List of stars in Vulpecula - 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....

Vulpecula, 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
α Vul Alpha Vulpeculae Alpha Vulpeculae is the brightest star in the constellation Vulpecula. It has a traditional name, variously represented as Lukida, Lucida Anseris, or Anser, a tradition kept from when the constellation had the name Vulpecula et Anser 'the fox and the goose'.Alpha Vulpeculae is a red giant of...	α	6	183439	95771	4.44	−0.35	296	M0 comp	Anser
23 Vul 23 Vulpeculae 23 Vulpeculae is a star in a double star system in the constellation Vulpecula.-References:*...		23	192806	99874	4.50	−0.51	328	K3III
31 Vul 31 Vulpeculae 31 Vulpeculae is a variable star in the constellation Vulpecula.-References:*...	(r) Map of constellations Lyra, Cygnus, Lacerta, Vulpec, Anser, and Sagitta. - Flamsteed, John. 1729. Atlas coelestis: Linda Hall Library.	31	198809	103004	4.56	0.45	216	G8III
13 Vul 13 Vulpeculae 13 Vulpeculae is a star in the constellation Vulpecula.-References:*...		13	188260	97886	4.57	−0.64	359	B9.5III
15 Vul 15 Vulpeculae 15 Vulpeculae is a star in the constellation Vulpecula....		15	189849	98543	4.66	0.49	222	A4III	NT Vul; α² CVn variable
1 Vul 1 Vulpeculae 1 Vulpeculae is a star in the constellation Vulpecula....		1	180554	94703	4.76	−2.47	911	B4IV
QR Vul HD 192685 HD 192685, also known as QR Vul or HR 7739, is a star 1,199 ly away in the Vulpecula constellation. It is a Be star and is slightly variable....			192685	99824	4.79	−3.04	1199	B3V	slightly variable
29 Vul 29 Vulpeculae 29 Vulpeculae is a star in the constellation Vulpecula....		29	196724	101867	4.81	0.73	213	A0V
12 Vul 12 Vulpeculae 12 Vulpeculae is a star in the constellation Vulpecula....		12	187811	97679	4.90	−1.49	619	B2.5V	V395 Vul; 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...
30 Vul 30 Vulpeculae 30 Vulpeculae is a star in the constellation Vulpecula....		30	197752	102388	4.92	−0.32	365	K2III
9 Vul 9 Vulpeculae 9 Vulpeculae is a star in the constellation Vulpecula. Its apparent magnitude is 5.0...		9	184606	96275	5.00	−1.35	608	B8IIIn
32 Vul 32 Vulpeculae 32 Vulpeculae is a star in the constellation Vulpecula....	(q)	32	199169	103200	5.03	−1.75	739	K4III
28 Vul 28 Vulpeculae 28 Vulpeculae is a star in the constellation Vulpecula....		28	196740	101868	5.06	−0.84	493	B5IV
17 Vul 17 Vulpeculae 17 Vulpeculae is a star in the constellation Vulpecula....		17	190993	99080	5.08	−0.80	488	B3V
4 Vul 4 Vulpeculae 4 Vulpeculae is a star 236.7 ly away in the constellation Vulpecula....		4	182762	95498	5.14	0.84	237	K0III
22 Vul 22 Vulpeculae 22 Vulpeculae is a star 4,348.7 ly away in the constellation Vulpecula....		22	192713	99853	5.18	−5.44	4347	G2Ib SB	QS Vul; 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...
21 Vul 21 Vulpeculae 21 Vulpeculae is a star 327.1 ly away from Earth in the Vulpecula constellation....		21	192518	99738	5.19	0.18	327	A7IVn	NU Vul; 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...
3 Vul 3 Vulpeculae 3 Vulpeculae is a star 402.7 ly away in the constellation Vulpecula....		3	182255	95260	5.22	−0.24	402	B6III	V377 Vul
16 Vul 16 Vulpeculae 16 Vulpeculae is a star 211.4ly away in the constellation Vulpecula....		16	190004	98636	5.23	1.17	211	F2III
24 Vul 24 Vulpeculae 24 Vulpeculae is a star 472 ly away in the Vulpecula constellation....		24	192944	99951	5.30	−0.50	472	G8III
33 Vul 33 Vulpeculae 33 Vulpeculae is a star 397.3 ly away in the constellation Vulpecula....		33	199697	103511	5.30	−0.13	397	K4III
35 Vul 35 Vulpeculae 35 Vulpeculae is a star 181.6 ly away in the Vulpecula constellation....		35	204414	105966	5.39	1.66	182	A1V
2 Vul 2 Vulpeculae 2 Vulpeculae is a star 1,918.6 ly away in the constellation Vulpecula....		2	180968	94827	5.46	−3.39	1918	B0.5IV	ES Vul; 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...
10 Vul 10 Vulpeculae 10 Vulpeculae is a star 356.5 ly away in the constellation Vulpecula....		10	186486	97077	5.50	0.31	356	G8III
25 Vul 25 Vulpeculae 25 Vulpeculae is a star 1,802 ly away in the constellation Vulpecula....		25	193911	100435	5.50	−3.21	1801	B8IIIn
18 Vul 18 Vulpeculae 18 Vulpeculae is a star 419.8 ly away in the constellation Vulpecula....		18	191747	99404	5.51	−0.04	420	A3III
19 Vul		19	192004	99518	5.51	−2.96	1614	K3II-III
			187982	97765	5.54	−3.15	1781	A1Iab
			188485	97961	5.56	−0.25	472	A0III
27 Vul		27	196504	101716	5.59	0.73	305	B9V
5 Vul		5	182919	95560	5.60	1.47	218	A0V
T Vul			198726	102949	5.66	−2.89	1672	F5Ib	δ Cep variable
			203925	105703	5.67	1.53	220	A8III
14 Vul		14	189410	98375	5.68	2.26	158	F0
			194577	100754	5.68	−0.43	543	G6III
			203803	105652	5.70	1.98	181	F1IV
			178187	93845	5.78	0.74	332	A4III
8 Vul		8	183491	95785	5.82	−0.04	484	K0III
			182955	95582	5.84	0.12	455	M0III
			189944	98609	5.88	−0.69	672	B4V
			184010	96016	5.89	2.03	193	K0III-IV
20 Vul		20	192044	99531	5.91	−1.81	1140	B7Ve...
			196753	101870	5.91	−3.00	1976	K0II-III+..
			187193	97402	6.00	0.56	400	K0II-III
			179648	94382	6.02	−1.43	1006	A2Vn
			196821	101919	6.08	−1.19	926	A0III
			201051	104172	6.13	0.99	348	K0II-III
			182807	95492	6.19	3.97	90	F7V
			203858	105660	6.20	−0.17	612	A2V
			178476	93975	6.22	3.01	143	F3V
			191877	99479	6.24	−8.55	29636	B1Ib
			193094	100018	6.24	0.98	367	G9III
PS Vul			186518	97091	6.27	−4.35	4347	B7V + G1:III
V387 Vul			176541	93270	6.28	−0.55	756	M4III
			203206	105344	6.29	0.20	539	B6IV
			182761	95487	6.31	0.87	400	A0V
			184961	96417	6.33	0.11	571	B9sp...
7 Vul		7	183537	95818	6.34	−0.50	760	B5Vn
			203886	105689	6.35	0.39	508	K0III
			195692	101300	6.37	1.82	264	Am
			182422	95340	6.40	−1.30	1132	B9.5V
26 Vul		26	196362	101641	6.40	−0.26	701	A5III
			186021	96856	6.43	−1.80	1442	K0Iab:
			176971	93443	6.44	0.92	414	A4V
V379 Vul			187640	97572	6.45	−2.13	1698	B5V
			190322	98772	6.45	0.46	513	K2
			187614	97573	6.46	0.64	475	G8III
			189671	98458	6.49	−1.79	1475	G8II
			196035	101505	6.49	−1.79	1475	B3IV
			185436	96601	6.50	0.28	572	K0III
			190066	98661	6.50	−3.75	3663	B1Iab
BW Vul			199140	103191	6.55	−2.13	1772	B2IIIvar	variable star
HD 190228 HD 190228 HD 190228 is a star located in the constellation Vulpecula. Its apparent magnitude is 7.31 and the absolute magnitude is 3.34. The distance is 204 light years from Earth...			190228	98714	7.31	3.34	203	G5IV	has a planet (b)
HD 189733 HD 189733 HD 189733, also catalogued as V452 Vulpeculae, is a binary star system approximately 63 light-years away in the constellation of Vulpecula . The primary star is suspected to be an orange dwarf star, while the secondary star is a red dwarf star...			189733	98505	7.68	6.26	62.9	K1-K2	planetary transit variable, has a transiting planet (b HD 189733 b HD 189733 b is an extrasolar planet approximately 63 light-years away in the constellation of Vulpecula . The planet was discovered orbiting the star HD 189733 on October 5, 2005, when astronomers in France observed the planet transiting across the face of the star. The planet is classified as a... )
HD 188015 HD 188015 HD 188015 is an 8th magnitude star about 172 light-years away in the constellation of Vulpecula. It is a yellow subgiant, a Sun-like star that has ceased or is about to stop hydrogen fusion in its core. However, it is only slightly brighter than the Sun, but probably much older.The star is almost...			188015	97769	8.22	4.61	172	G5IV	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 HD 188015 b HD 188015 b is an extrasolar planet announced by the California and Carnegie Planet Search team in 2005. Like majority of known planets, it was discovered using the radial velocity method.The planet has a minimum mass about quarter greater than Jupiter... )
PY Vul PY Vulpeculae PY Vulpeculae a variable star in the constellation Vulpecula.-References:*...					12.97			DA	variable star, white dwarf White dwarf A white dwarf, also called a degenerate dwarf, is a small star composed mostly of electron-degenerate matter. They are very dense; a white dwarf's mass is comparable to that of the Sun and its volume is comparable to that of the Earth. Its faint luminosity comes from the emission of stored...
CK Vul		11						ea	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... Vulpeculae 1670; Magnitude 2.7 (max)
PSR B1919+21							2283		first pulsar Pulsar A pulsar is a highly magnetized, rotating neutron star that emits a beam of electromagnetic radiation. The radiation can only be observed when the beam of emission is pointing towards the Earth. This is called the lighthouse effect and gives rise to the pulsed nature that gives pulsars their name... discovered
PSR J2007+2722 PSR J2007+2722 PSR J2007+2722 is a 40.8-hertz isolated pulsar in the Vulpecula constellation, 5.3 kpc distant in the plane of the Galaxy, and is most likely a Disrupted Recycled Pulsar ....							17200		pulsar Pulsar A pulsar is a highly magnetized, rotating neutron star that emits a beam of electromagnetic radiation. The radiation can only be observed when the beam of emission is pointing towards the Earth. This is called the lighthouse effect and gives rise to the pulsed nature that gives pulsars their name... discovered by Einstein@home Einstein@Home Einstein@Home is a volunteer distributed computing project hosted by the University of Wisconsin–Milwaukee and the Max Planck Institute for Gravitational Physics . The project is directed by Bruce Allen...

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