List of stars in Pisces - 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....

Pisces
Pisces (constellation)
Pisces is a constellation of the zodiac. Its name is the Latin plural for fish, and its symbol is . It lies between Aquarius to the west and Aries to the east...

, 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
η Psc Eta Piscium Eta Piscium is the brightest star in the constellation Pisces. Eta Piscium is located at a distance of about 294 light years from Earth and shines at magnitude +3.62. It is of Spectral type G7 III...	η	99	9270	7097	3.62	−1.16	294	G8III	Alpherg, Kullat-Nunu; 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...
γ Psc Gamma Piscium Gamma Piscium is a star approximately 138 light years away from Earth, in the constellation Pisces. It is a yellow star with a spectral type of G9III, meaning it has a surface temperature of 5,000 to 6,000 degrees and is a normal giant star. It is slightly cooler than our Sun, yet it is 11 solar...	γ	6	219615	114971	3.70	0.68	131	G7III	Simmah
α Psc A Alpha Piscium Alpha Piscium is a star in the constellation Pisces. It has the traditional name Alrescha , from the Arabic الرشآء al-rišā’ "the well rope". Less common names are Kaitain and Okda, the latter from the Arabic عقدة ‘uqdah "knot".The distance to α Psc is about 139 light years...	α	113	12446	9487	3.82	0.67	139	A2	Alrescha, Al Rescha, Alrischa, Alrisha, Rescha, El Rischa, Al Richa, Kaitain, Okda; α² CVn variable
ω Psc Omega Piscium Omega Piscium is a star approximately 106 light years away from Earth, in the constellation Pisces. It has a spectral type of F4IV, meaning it is a subgiant/dwarf star, and it has a temperature of 6,600 kelvins. It may or may not be a close binary star system...	ω	28	224617	118268	4.03	1.47	106	F4IV	Vernalis
ι Psc Iota Piscium Iota Piscium is a star 45 light years away from Earth, in the constellation Pisces. The star is a yellowish dwarf star of spectral type F7V, which is somewhat larger and brighter than our sun, but still within the range considered to have the potential for Earth-like planets. It has a surface...	ι	17	222368	116771	4.13	3.43	45	F7V
ο Psc Omicron Piscium Omicron Piscium is a star in the constellation Pisces, located about 142 light years from Earth.It has an apparent magnitude of +4.26 and belongs to spectral type G8. The star has the traditional name Torcularis septentrionalis, from the Latin torculāris septentriōnālis "of the northern press"....	ο	110	10761	8198	4.26	−0.23	258	K0III	Torcularis Septentrionalis
ε Psc Epsilon Piscium Epsilon Piscium is a star approximately 182 light years away from the Earth, in the constellation Pisces. It is a yellow-orange star of the G9III or K0III spectral type, meaning it has a surface temperature around 5,000 kelvins. It is a normal giant star, slightly cooler in surface temperature,...	ε	71	6186	4906	4.27	0.44	190	K0III	Kaht
θ Psc Theta Piscium Theta Piscium is a star approximately 159 light years away from Earth in the constellation Pisces. It is an orange-red star of the spectral type K1III, meaning it is a normal giant star with a surface temperature of 3,500 to 5,000 kelvins, and is brighter yet cooler than our sun....	θ	10	220954	115830	4.27	0.83	159	K1III
α Psc B Alpha Piscium Alpha Piscium is a star in the constellation Pisces. It has the traditional name Alrescha , from the Arabic الرشآء al-rišā’ "the well rope". Less common names are Kaitain and Okda, the latter from the Arabic عقدة ‘uqdah "knot".The distance to α Psc is about 139 light years...	α	113	12447		4.33
30 Psc		30	224935	154	4.37	−1.15	415	M3III	YY Psc
δ Psc Delta Piscium Delta Piscium is a binary star in the constellation Pisces.-In fiction:Linteum is the most notable star the moon will be closest to on the solstice of December 21, 2012. Some works of fiction mention Linteum combining myths about the Maya calendar and Revelation 13:5...	δ	63	4656	3786	4.44	−0.42	305	K5III	Linteum
ν Psc Nu Piscium Nu Piscium is a star approximately 368 light years away from Earth, in the constellation Pisces. It is an orange star of the spectral type K3IIIb, meaning it possesses a surface temperature between 3,500 and 5,000 kelvins. It is a giant star, cooler in surface temperature than our Sun, yet larger...	ν	106	10380	7884	4.45	−0.81	368	K3III
β Psc Beta Piscium Beta Piscium is a star in the constellation Pisces. It has the traditional name Fum al Samakah, from the Arabic فم السمكة fum al-samakah "mouth of the fish" ....	β	4	217891	113889	4.48	−1.42	492	B6Ve	Fum al Samakah, Samaka
λ Psc Lambda Piscium Lambda Piscium is a star approximately 101 light years away from Earth in the constellation Pisces. It is a bluish-white star of A7V spectral classification, meaning it has a surface temperature of 7,500 to 11,000 kelvins. It is much brighter and hotter in surface temperature than our sun, yet is...	λ	18	222603	116928	4.49	2.04	101	A7V
τ Psc	τ	83	7106	5586	4.51	1.03	162	K0III-IV...	Anunitum
33 Psc		33	28	443	4.61	1.63	128	K1III	BC Psc; 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...
ξ Psc	ξ	111	11559	8833	4.61	0.78	191	K0III SB
χ Psc	χ	84	7087	5571	4.66	−0.99	439	K0III
φ Psc Phi Piscium Phi Piscium is a binary star system approximately 380 light years away in the constellation Pisces. It consists of Phi Piscium A, with a spectral type of K0III, and Phi Piscium B. Phi Piscium A possesses a surface temperature of 3,500 to 5,000 kelvins...	φ	85	7318	5742	4.67	−0.65	377	K0III...
υ Psc Upsilon Piscium Upsilon Piscium is a star approximately 310 light years away from Earth, in the constellation Pisces. It is bluish-white star of the spectral type A3V. It has a surface temperature of 7,500 to 11,000 kelvins, and is approximately the same size as our Sun, yet is much hotter and brighter. It has a...	υ	90	7964	6193	4.74	−0.16	311	A3V
μ Psc Mu Piscium Mu Piscium is a multiple star with three components approximately 360 light years away from Earth, in the constellation Pisces. Its nearest multiple is approximately 5.6 degrees dimmer in apparent magnitude....	μ	98	9138	7007	4.84	−0.38	360	K4III
27 Psc		27	224533	118209	4.88	0.70	224	G9III
κ Psc Kappa Piscium Kappa Piscium is a multiple star approximately 162 light years away from Earth, in the constellation Pisces. Appearing as a single point in the sky, it is easily split when viewed with a pair of binoculars, and consists of three components...	κ	8	220825	115738	4.95	1.47	162	A0p	α² CVn variable
19 Psc 19 Piscium TX Piscium is a variable carbon star in the constellation Pisces. It is amongst the reddest stars known, with a significant reddish hue when seen in binoculars....		19	223075	117245	4.95	−1.89	760	C5II	TX Psc; 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,...
47 Psc		47	2411	2219	5.01	−0.88	490	M3IIIvar	TV Psc; semiregular variable Semiregular variable star Semiregular variable stars are giants or supergiants of intermediate and late spectral type showing considerable periodicity in their light changes, accompanied or sometimes interrupted by various irregularities. Periods lie in the range from 20 to more than 2000 days, while the shapes of the light...
7 Psc	b	7	220009	115227	5.05	−0.05	341	K2III
64 Psc		64	4676	3810	5.07	3.18	78	F8V...
29 Psc		29	224926	145	5.13	−0.36	409	B7III-IV
89 Psc	f	89	7804	6061	5.13	0.99	220	A3V
82 Psc	g	82	7034	5544	5.15	−1.03	560	F0V
ζ Psc A	ζ	86	7344	5737	5.21	1.93	148	A7IV	Revati Revati (nakshatra) Revati is the twenty-seventh nakshatra in Hindu astrology, corresponding to ζ Piscium.It is ruled by Puṣan,one of the 12 Ādityas... of Vedic astrology
91 Psc	l	91	8126	6315	5.23	0.12	344	K5III
107 Psc		107	10476	7981	5.24	5.87	24	K1V	nearby
ψ¹ Psc	ψ¹	74	6456	5131	5.33	1.01	238	A1Vn
ρ Psc	ρ	93	8723	6706	5.35	3.27	85	F2V:var
55 Psc		55	3690	3138	5.36	−0.14	411	F3V...
57 Psc		57	4408	3632	5.36	−0.92	587	M4III	EL Psc
41 Psc	d	41	1635	1645	5.38	−0.04	395	K3III
52 Psc		52	2910	2568	5.38	0.90	257	K0III
5 Psc	A	5	218527	114273	5.42	0.75	280	G8IV
2 Psc		2	217264	113521	5.43	0.76	280	K1III:
68 Psc	h	68	5575	4510	5.44	−1.23	704	G6III
20 Psc		20	223252	117375	5.49	0.73	291	G8III
σ Psc	σ	69	6118	4889	5.50	−0.02	414	B9.5V
94 Psc		94	8763	6732	5.50	0.63	307	K1III
58 Psc		58	4482	3675	5.51	0.99	262	G8II
80 Psc	e	80	6763	5346	5.51	2.73	117	F0III-IV
34 Psc		34	560	813	5.54	0.55	325	B9V
π Psc Pi Piscium Pi Piscium is a star approximately 110 light years away from Earth, in the constellation Pisces. It is a yellowish white star of the spectral type F0V, meaning it possesses a surface temperature of 6,000 to 7,500 kelvins, and is approximately the same size as our Sun, yet brighter and hotter in...	π	102	9919	7535	5.54	2.89	110	F0V
ψ¹ Psc	ψ¹	74	6457	5132	5.55	1.38	222	A0Vn
ψ² Psc	ψ²	79	6695	5310	5.56	2.09	161	A3V
ψ³ Psc	ψ³	81	6903	5454	5.57	0.11	403	G0III
22 Psc		22	223719	117683	5.59	−2.21	1181	K4II
72 Psc		72	6397	5081	5.64	1.95	178	F4II-III
16 Psc		16	221950	116495	5.68	3.22	101	F6Vbwvar
51 Psc		51	2913	2548	5.69	1.15	264	B9.5V
32 Psc	c	32	225003	194	5.70	2.82	123	F0V
96 G. Psc HD 4628 HD 4628 is a main sequence dwarf star star in the constellation Pisces. It has a spectral classification of K2, giving it an orange-red hue and a slightly smaller mass and girth than our Sun. It lies at a distance of approximately 24 light years from us and has a relatively high proper motion...			4628	3765	5.74	6.38	24	K2V	nearby
44 Psc		44	2114	2006	5.77	−0.53	593	G5III
21 Psc		21	223438	117491	5.77	1.20	267	A5m
XZ Psc (52 G. Psc)			224062	117887	5.78	−0.69	643	M5IIb
66 Psc		66	5267	4267	5.80	0.54	367	A1Vn
			6953	5494	5.81	0.60	360	K5III
67 G. Psc			587	840	5.84	2.14	179	K1III
11 G. Psc			217459	113622	5.85	−0.27	547	K4III
54 Psc 54 Piscium 54 Piscium is an orange dwarf star approximately 36 light-years away in the constellation of Pisces. In 2002, an extrasolar planet was confirmed to be orbiting the star, and in 2006, a brown dwarf was also discovered orbiting it....		54	3651	3093	5.88	5.65	36	K0V	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 54 Piscium b 54 Piscium b , occasionally catalogued as 54 Piscium Ab in order to differentiate from the brown dwarf in the system, is an extrasolar planet approximately 36 light-years away in the constellation of Pisces. The planet was discovered orbiting the orange dwarf star 54 Piscium... )
53 Psc		53	3379	2903	5.89	−1.21	856	B2.5IV	AG Psc; 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...
112 Psc		112	12235	9353	5.89	3.43	101	G2IV
40 G. Psc			222602	116918	5.89	0.81	338	A3Vn
			9640	7359	5.90	−0.41	597	M2III
131 G. Psc			11037	8404	5.91	0.90	328	G9III
14 Psc		14	221675	116323	5.91	1.67	230	A2m
62 Psc		62	4627	3760	5.92	−0.62	661	G8III
24 Psc		24	223825	117761	5.93	0.00	499	G9III
			9780	7447	5.95	2.07	195	F0IV
87 Psc		87	7374	5778	5.97	0.04	500	B8III
			8388	6492	5.97	−1.05	827	K5
60 Psc		60	4526	3697	5.98	0.25	455	G8III
105 Psc		105	10164	7740	5.98	0.26	454	K2III
97 Psc		97	9100	6981	6.01	0.69	379	A4IV	VX Psc; 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...
35 Psc 35 Piscium 35 Piscium is a binary star system in the constellation Pisces. According to Cester , the system has a period of 0.841658 days, zero eccentricity, and an inclination of 19 degrees...		35	1061	1196	6.02	1.50	261	F0IV	UU Psc; 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...
73 Psc		73	6386	5074	6.03	−0.69	721	K5III
88 Psc		88	7446	5824	6.04	0.29	461	G6III:
			7578	5936	6.04	1.12	315	K1III
48 Psc		48	2436	2224	6.05	−1.62	1113	K5III
88 G. Psc			2454	2235	6.05	3.25	119	F6Vawvar
			1419	1465	6.07	0.38	448	K0III
			6966	5483	6.07	−0.09	557	M0III
84 G. Psc			2023	1939	6.08	−0.02	541	K1III
67 Psc	k	67	5382	4366	6.08	1.47	273	A5IV
59 Psc		59	4490	3685	6.11	0.96	349	F0Vn	XX Psc; δ Sct variable
1 Psc		1	216701	113167	6.11	1.24	307	A7III
36 Psc		36	1227	1319	6.12	0.46	442	G8II-III
WW Psc (100 G. Psc)			5820	4655	6.14	−1.42	1062	M2III
75 Psc		75	6557	5204	6.14	0.89	366	G8III
6 G. Psc HD 217107 HD 217107 is a yellow subgiant star approximately 65 light-years away from Earth in the constellation of Pisces . Its mass is very similar to the Sun's, although it is considerably older...			217107	113421	6.17	4.70	64	G8IV	has two planets (b HD 217107 b HD 217107 b is an extrasolar planet approximately 64 light-years away from Earth in the constellation of Pisces . The planet was discovered orbiting the star HD 217107 approximately every seven days, classifying the planet as a hot Jupiter... & c HD 217107 c HD 217107 c is an extrasolar planet approximately 64 light-years away from Earth in the constellation of Pisces . The planet was the second planet to be discovered orbiting the star HD 217107... )
5 Cet		5	352	664	6.18	−1.26	1003	K2III	AP Psc; 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...
			8634	6669	6.18	1.75	251	F5III
76 G. Psc			1367	1421	6.19	1.17	330	K0II
			5316	4317	6.19	−0.05	578	M4III
			6301	5034	6.20	3.08	137	F7IV-V
			10308	7874	6.20	2.46	183	F2III
118 G. Psc			8949	6868	6.22	0.96	367	K1IIIvar	variable
3 Psc		3	217428	113610	6.22	−0.24	639	G4III
26 Psc		26	224103	117927	6.22	0.76	403	B9V
78 Psc		78	6680	5319	6.23	3.12	137	F5IV
101 Psc 101 Piscium 101 Piscium is a star in the constellation Pisces. The 6.23m blue-white giant is variable in brightness. 101 Piscium a distant star, located over 2000 light-years away.-References:*...		101	9766	7436	6.23	−3.01	2296	B9.5III
			7229	5679	6.24	1.15	340	G1V...
42 Psc		42	1796	1772	6.25	0.13	545	K3III
9 Psc		9	220858	115768	6.26	0.78	407	G7III
109 Psc 109 Piscium 109 Piscium is a yellow subgiant star located about 106 light years away in the constellation Pisces. It has a similar mass to our Sun, and has a higher abundance of iron.-Planetary system:In 1999 an extrasolar planet was detected around this star....		109	10697	8159	6.27	3.71	106	G5IV	has a planet (b 109 Piscium b 109 Piscium b is a long-period extrasolar planet discovered in orbit around 109 Piscium. It is at least 6.38 times the mass of Jupiter and is likely to be a gas giant... )
WZ Psc (140 G. Psc)			12872	9809	6.27	−0.88	879	M4
76 Psc		76	6476	5175	6.28	0.02	582	K0
5 G. Psc			217019	113360	6.28	0.53	460	K1III
25 Psc		25	223855	117774	6.29	0.53	462	A1V
			5612	4520	6.30	0.28	522	G8III
121 G. Psc			9496	7243	6.31	0.04	584	K0
62 G. Psc			6	417	6.32	0.53	469	G9III:
			3268	2832	6.32	3.44	123	F7V
31 Psc		31	224995	186	6.33	0.72	432	A6V
DT Psc			7351	5772	6.33	−1.14	1016	M2S SB	semiregular variable
24 G. Psc			220406	115476	6.33	−1.89	1436	K2
124 G. Psc			10262	7819	6.34	2.62	181	F2
77 Psc A		77	6479	5141	6.35	3.05	149	F3V	binary star
8 G. Psc			217186	113465	6.35	1.44	313	A1V
30 G. Psc			221147	115945	6.35	−0.91	924	K0
			7724	6025	6.36	1.72	277	K0
7 G. Psc			217131	113433	6.38	1.44	317	F0V
			3166	2734	6.39	0.95	400	K0
98 G. Psc			4928	3992	6.39	0.70	448	K0III
CY Psc (123 G. Psc)			9889	7505	6.39	−0.83	906	M0
16 G. Psc			218103	114005	6.39	0.90	409	G9III
13 Psc		13	221409	116146	6.39	−0.56	801	K1III
46 Psc		46	2410	2213	6.40	0.33	533	K0
15 G. Psc			217926	113904	6.42	1.82	271	F2V
4 Cet		4	315	635	6.43	0.56	487	B8IIIsp...	variable
92 G. Psc			3457	2954	6.43	0.19	577	K4III
			2358	2178	6.44	0.87	423	A5
ζ Psc B	ζ	86	7345	5743	6.44	2.55	195	F7V
			8733	6714	6.44	1.59	304	K0
138 G. Psc			12730	9706	6.44	0.60	479	K0
13 G. Psc			217590	113705	6.44	0.22	571	G5
			5418	4382	6.46	0.53	501	G8II
			5641	4558	6.47	0.88	428	A2V
15 Psc		15	221833	116422	6.47	1.58	310	K0
45 G. Psc			223346	117445	6.47	2.76	180	F5III-IV
			2035	1948	6.48	0.40	535	K0
112 G. Psc			7107	5575	6.49	0.98	412	G5
61 Psc		61	4568	3730	6.51	2.71	187	F8V
3 Ari 3 Arietis 3 Arietis is a variable star of δ Scuti type. Despite its Flamsteed designation, the star is actually located in the constellation Pisces near the border of Aries. Its apparent magnitude is 6.55. The star also has the variable star designation VY Piscium....		3	10845	8271	6.55	−0.13	707	A9III	VY Psc; δ Sct variable
40 Psc		40	1563	1595	6.60	0.45	553	K0
38 Psc		38	1317	1392	6.66	2.58	213	F5
104 Psc		104	10135	7710	6.74	1.07	444	K0
45 Psc		45	2140	2025	6.77	−0.62	979	K0
95 Psc		95	8875	6815	7.01	2.75	232	G0V
65 Psc	i	65	4757	3885	7.0	0.42	347	F4III	forms a binary with HD 4758
65 Psc	i	65	4758	3885	7.1			F5III	forms a binary with HD 4757
HD 8574 HD 8574 HD 8574 is a yellow-white star in the constellation Pisces. It has an apparent magnitude of +7.12 and absolute magnitude of +3.90. The stellar distance is 44.15 parsecs or 144 light years from our solar system....			8574	6643	7.11	3.89	144	F8	has a planet (b HD 8574 b HD 8574 b is an extrasolar planet discovered in 2001 by a team of European astronomers using Doppler spectroscopy as part of the ELODIE Planet Search Survey, and was published in a paper with five other planets. HD 8574 b is in the orbit of host star HD 8574... )
77 Psc B		77	6480	5144	7.26	4.04	144	F6V	component of the 77 Psc system
100 Psc		100	9656	7364	7.28	2.68	272	A3V
HD 4203 HD 4203 HD 4203 is a 9th magnitude star located approximately 253 light years away in the constellation Pisces. The star is yellow with spectral type G5. The star has evolved for 9.41 billion years. The star has a gas giant planet orbiting around a high metallicity star....			4203	3479	7.79	5.22	107	G7V	has a planet (b HD 4203 b HD 4203 b is an exoplanet more massive than Jupiter. It orbits two times further from the star than Earth to the Sun. The planet takes 1.1824 year to orbit the star very eccentrically from 1.00 AU to 3.14 AU. The planet was discovered by Steve Vogt using the Keck telescope.... )
HD 217786			217786	113834	7.80		179	F8V	has a planet (b)
HD 4313			4313	3574	7.82	2.23	429	G5D	has a planet (b HD 4313 b HD 4313 b is an extrasolar planet orbiting the G-type star HD 4313 approximately 447 lightyears away in the constellation Pisces.-See also:* HD 95089 b* HD 181342 b* HD 206610 b* HD 180902 b* HD 136418 b* HD 212771 b... )
HD 218566			218566	114322	8.63		98	K3V	has a planet (b)
WASP-32					11.3			G	has a transiting planet (b)
WASP-28					12.0	4.4	1090	F8-G0	has a transiting planet (b)
Van Maanen's star Van Maanen's star Van Maanen's star is a white dwarf star. Out of the white dwarfs known, it is the third closest to the Sun, after Sirius B and Procyon B, in that order, and the closest known solitary white dwarf...				3829	12.36	14.14	14	DG...	31st closest star system; the nearest single 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...

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