List of stars in Orion - 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....

Orion
Orion (constellation)
Orion, often referred to as The Hunter, is a prominent constellation located on the celestial equator and visible throughout the world. It is one of the most conspicuous, and most recognizable constellations in the night sky...

, 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
Rigel Rigel Rigel is the brightest star in the constellation Orion and the sixth brightest star in the sky, with visual magnitude 0.18...	β	19	34085	24436	0.18	−6.69	773	B8Ia	Algebar, Elgebar; 6th brightest star, triple 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... ; α Cyg variable 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...
Betelgeuse Betelgeuse Betelgeuse, also known by its Bayer designation Alpha Orionis , is the eighth brightest star in the night sky and second brightest star in the constellation of Orion, outshining its neighbour Rigel only rarely...	α	58	39801	27989	0.58 var. 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... (0.3 to 1.2)	−5.14	640	M2Ib	Betelgeuze, Betelgeux, Mankib, Al Mankib; 9th brightest star, variable
γ Ori Gamma Orionis Bellatrix, also known by its Bayer designation Gamma Orionis , is the third brightest star in the constellation Orion, the twenty-seventh brightest star in the night sky, and one of the brightest second-magnitude stars....	γ	24	35468	25336	1.64	−2.72	243	B2III	Bellatrix
ε Ori Epsilon Orionis Alnilam is a large blue supergiant star in the constellation of Orion. Its Flamsteed designation is 46 Orionis....	ε	46	37128	26311	1.69	−6.38	1342	B0Ia	Alnilam, Alnihan, Alnitam; α Cyg variable
ζ Ori A	ζ	50	37742	26727	1.74	−5.25	817	O9.5Ib SB	Alnitak, Alnitah
κ Ori Kappa Orionis Kappa Orionis is the sixth-brightest star in the constellation of Orion. It has the traditional name Saiph.Of the four bright stars that compose Orion's main quadrangle, it is the star at the south-eastern corner...	κ	53	38771	27366	2.07	−4.65	721	B0.5Iavar	Saiph
δ Ori A Delta Orionis Delta Orionis , traditionally known as Mintaka , is a star some 900 light years distant in the constellation Orion. Together with Zeta Orionis and Epsilon Orionis , the three stars make up the belt of Orion, known by many names across many ancient cultures...	δ	34	36486	25930	2.25	−4.99	916	O9.5II	Mintaka, Mentaka, Mintika
ι Ori Iota Orionis Iota Orionis is the brightest star in Orion's sword, and is located at the tip of the sword. It has the traditional names Hatsya , or in Arabic, Na’ir al Saif, which means simply "the Bright One of the Sword."+-9*Iota Orionis is a quadruple system dominated by a massive spectroscopic binary with an...	ι	44	37043	26241	2.75	−5.30	1325	O9III	Hatsya, Na'ir al Saif
π³ Ori	π³	1	30652	22449	3.19	3.67	26	F6V	Tabit, Hassaleh; nearby star
η Ori Eta Orionis Eta Orionis is a star in the constellation Orion. Other names are Saiph, Algjebbah, and Ensis ....	η	28	35411	25281	3.35	−3.86	901	B1V + B2	Saif al Jabbar, Algiebba; 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...
λ Ori A Lambda Orionis Lambda Orionis is a star in the constellation Orion. It has the traditional names Meissa or Heka. "Meissa" derives from the Arabic "Al-Maisan" which means "The Shining One". This term was used for Gamma Gemini , but was somehow also mistakenly applied to λ Orionis and the name stuck...	λ	39	36861	26207	3.39	−4.16	1055	O8III	Meissa, Heka
τ Ori Tau Orionis Tau Orionis is a star in the constellation Orion.This star, along with β Eri, λ Eri and ψ Eri were Al Kursiyy al Jauzah, "the Chair of the Central One"...	τ	20	34503	24674	3.59	−2.56	554	B5III	Yuh Tsing
π⁴ Ori Pi4 Orionis Pi4 Orionis is a spectroscopic binary star in the constellation Orion. It is about 1,300 light years away and is one of the most luminous stars known. It is one of a series of stars that share the Bayer designation Pi Orionis....	π⁴	3	30836	22549	3.68	−4.25	1259	B2III SB
π⁵ Ori	π⁵	8	31237	22797	3.71	−4.36	1342	B2III SB
σ Ori A Sigma Orionis Sigma Orionis or Sigma Ori is a five-star system in the constellation Orion. It is approximately 1,150 light years from Earth....	σ	48	37468	26549	3.77	−3.96	1148	O9.5V...	quintuple star system
ο² Ori	ο²	9	31421	22957	4.06	0.48	169	K2III
φ² Ori Phi Orionis The Bayer designation Phi Orionis is shared by two star systems, φ¹ Orionis and φ² Orionis, in the constellation Orion. The two stars are separated by approximately 0.71° in the sky.-φ¹ Orionis:...	φ²	40	37160	26366	4.09	1.33	116	G8III-IV
μ Ori	μ	61	40932	28614	4.12	0.78	152	Am...
29 Ori	e	29	35369	25247	4.13	0.49	174	G8III
32 Ori	A	32	36267	25813	4.20	−0.53	288	B5V
ζ Ori B	ζ	50	37743	26727	4.21	-2.80	817	O9.7Ib
π² Ori	π²	2	30739	22509	4.35	0.48	194	A1Vn
φ¹ Ori Phi Orionis The Bayer designation Phi Orionis is shared by two star systems, φ¹ Orionis and φ² Orionis, in the constellation Orion. The two stars are separated by approximately 0.71° in the sky.-φ¹ Orionis:...	φ¹	37	36822	26176	4.39	−3.01	985	B0IV...
χ¹ Ori	χ¹	54	39587	27913	4.39	4.67	28	G0V	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...
ν Ori	ν	67	41753	29038	4.42	−1.65	534	B3IV
ξ Ori	ξ	70	42560	29426	4.45	−2.00	634	B3IV
ρ Ori	ρ	17	33856	24331	4.46	−0.65	344	K3III...
π⁶ Ori	π⁶	10	31767	23123	4.47	−2.86	953	K2IIvar
ω Ori	ω	47	37490	26594	4.50	−3.98	1622	B3IIIe	γ Cas variable
161 G. Ori			40657	28413	4.53	−1.02	420	K2IIIvar
42 Ori	c	42	37018	26237	4.58	−2.33	786	B2III...
ψ Ori	ψ	30	35715	25473	4.59	−3.60	1417	B2IV	β Cep variable
υ Ori Upsilon Orionis Upsilon Orionis is a star in the constellation Orion. It has the traditional name Thabit ....	υ	36	36512	25923	4.62	−3.76	1545	B0V	Thabit, Tabit
π¹ Ori	π¹	7	31295	22845	4.64	1.80	121	A0V
χ² Ori	χ²	62	41117	28716	4.64	−10.36	32600	B2Iavar	α Cyg variable
11 Ori		11	32549	23607	4.65	−0.79	400	A0p Si	V1032 Ori; α² CVn variable
ο¹ Ori	ο¹	4	30959	22667	4.71	−1.39	542	M3Sv
31 Ori		31	36167	25737	4.71	−1.02	456	K5III	CI Ori
o Ori	o	22	35039	25044	4.72	−3.26	1289	B2IV-V
56 Ori		56	39400	27750	4.76	−2.91	1113	K2IIvar
49 Ori	d	49	37507	26563	4.77	1.41	153	A4V
103 G. Ori			36960	26199	4.78	−4.00	1863	B0.5V
15 Ori 15 Orionis 15 Orionis has the distinction of being the southern pole star of Uranus.It is an early F-type subgiant located 318 ly from the solar system....		15	33276	24010	4.81	−0.14	318	F2IV
25 Ori 25 Orionis 25 Orionis, less commonly known by its Bayer designation Psi1 Orionis is a fifth-magnitude star in the constellation Orion...	ψ¹	25	35439	25302	4.89	−2.77	1109	B1V:pe	V1086 Ori; 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...
51 Ori	b	51	37984	26885	4.90	0.07	302	K1III
185 G. Ori			44131	30093	4.91	−1.05	506	M1III
127 G. Ori			37756	26736	4.95	−4.08	2090	B2IV-V
69 Ori	f¹	69	42545	29434	4.95	−1.93	774	B5Vn
θ¹ Ori A	θ¹	41	37020	26220	4.98			O7	component of the Trapezium Trapezium (astronomy) The Trapezium, or Orion Trapezium Cluster is a tight open cluster of stars in the heart of the Orion Nebula, in the constellation of Orion. It was discovered by Galileo Galilei. On February 4, 1617 he sketched three of the stars , but missed the surrounding nebulosity...
θ² Ori	θ²	43	37041	26235	4.98	−3.84	1895	O9.5Vpe
23 Ori	m	23	35149	25142	4.99	−2.36	962	B1V
74 Ori	k	74	43386	29800	5.04	3.58	64	F5IV-V
27 Ori	p	27	35410	25282	5.07	1.46	172	K0III
θ¹ Ori C	θ¹	41	37022	26221	5.13		1500	O6Vpe	component of the Trapezium
64 Ori		64	41040	28691	5.14	−2.44	1069	B8V
6 Ori	g	6	31283	22833	5.18	0.84	241	A3V
			33554	24197	5.18	0.21	321	K5III
71 Ori		71	43042	29650	5.20	3.58	69	F6V
60 Ori		60	40446	28296	5.21	−0.05	367	A1Vs
45 Ori		45	37077	26268	5.24	−0.04	370	F0III
52 Ori		52	38710	27386	5.26	−0.58	479	A5V
38 Ori	n²	38	36777	26126	5.32	0.20	345	A2V
5 Ori		5	31139	22730	5.33	−1.13	638	M1III
15 G. Ori			31296	22834	5.33	−0.33	441	K1III
14 Ori	i	14	33054	23879	5.33	1.46	194	Am
21 Ori		21	34658	24817	5.34	1.42	198	F5IIvar
91 G. Ori			36591	25980	5.34	−4.14	2567	B1IV
72 Ori	f²	72	43153	29704	5.34	−0.50	479	B7V
			30210	22157	5.35	0.79	266	Am...
VV Ori			36695	26063	5.36	−3.41	1852	B1V	92 G. Orionis.
55 Ori		55	39291	27658	5.36	−3.20	1680	B2IV-V
			30034	22044	5.39	1.97	157	F0V
75 Ori	l	75	43525	29850	5.39	0.93	254	A2V
U Ori U Orionis U Orionis is a Mira-type variable star in the constellation Orion. It is a classical long period variable star that has been well observed from the United Kingdom for over 120 years. It was discovered on 1885 December 13 by J.E...			39816		6.3-12.0	-3.69	2146	M8III	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... , period 368 days
16 Ori	h	16	33254	23983	5.43	1.77	176	A2m
73 Ori		73	43247	29736	5.44	−2.72	1399	B9II-III
33 Ori	n¹	33	36351	25861	5.46	−2.95	1567	B1.5V
51 G. Ori			34043	24450	5.50	−0.82	598	K4III
18 Ori		18	34203	24555	5.52	0.26	368	A0V
73 G. Ori			35536	25329	5.60	−0.85	635	K5III
35 Ori		35	36653	26093	5.60	−0.39	513	B3V
			36881	26215	5.60	−2.66	1462	B9IIIMNp...
λ Ori B Lambda Orionis Lambda Orionis is a star in the constellation Orion. It has the traditional names Meissa or Heka. "Meissa" derives from the Arabic "Al-Maisan" which means "The Shining One". This term was used for Gamma Gemini , but was somehow also mistakenly applied to λ Orionis and the name stuck...	λ	39	36862	26207	5.61	-1.94	1055	B0.5V
178 G. Ori			43318	29716	5.62	2.86	116	F6V
66 Ori		66	41380	28814	5.63	−3.78	2489	G4III
102 G. Ori			36959	26197	5.67	−5.63	5927	B1Vvar
63 Ori		63	41361	28812	5.67	−1.97	1101	G7III:
			44033	30099	5.67	−0.46	548	K3Ib
60 G. Ori			35007	25028	5.68	−1.91	1076	B3V
64 G. Ori			35299	25223	5.69	−1.28	809	B1.5V
			40369	28302	5.70	−1.35	838	K2III...
170 G. Ori			42111	29151	5.70	−0.66	609	A3Vn
182 G. Ori			43587	29860	5.70	4.27	63	G0.5Vb
115 G. Ori			37209	26345	5.71	−3.14	1918	B1V...
68 Ori		68	42509	29433	5.76	−1.61	970	B9.5V
82 G. Ori			36166	25751	5.77	−2.16	1254	B2V
59 G. Ori			34989	25041	5.78	−0.99	736	B1V...
137 G. Ori			38527	27280	5.78	0.96	300	G8III
			31373	22913	5.79	0.23	423	B9V
143 G. Ori			39007	27549	5.79	0.74	334	G8III
79 G. Ori			36134	25708	5.80	0.02	467	K1III...
175 G. Ori			43023	29575	5.83	0.91	315	G8III
			42954	29616	5.86	0.15	452	A6m
116 G. Ori			37320	26487	5.87	−0.29	556	B8III
154 G. Ori			39910	28011	5.87	1.02	304	K2III:
44 G. Ori			33646	24203	5.88	−1.36	916	F5
42 G. Ori			33608	24162	5.89	2.97	125	F5V
			40020	28139	5.89	1.02	307	K2III
59 Ori		59	40372	28271	5.89	0.72	353	A5me del Del	V1004 Ori; 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...
45 G. Ori			33833	24294	5.90	0.22	446	G7III
27 G. Ori			32263	23408	5.91	−0.01	498	K0
			43112	29678	5.91	−2.21	1370	B1V
96 G. Ori			36780	26108	5.92	−1.14	842	K5III
57 Ori		57	39698	27965	5.92	−2.25	1405	B2V
			36162	25790	5.93	0.81	344	A3Vn
128 G. Ori			37788	26762	5.93	2.38	168	F0IV
138 G. Ori HD 38529 HD 38529 is a binary star approximately 128 light-years away in the constellation of Orion.-HD 38529 A:...			38529	27253	5.94	2.80	138	G4V	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... ; has a planet (Ab HD 38529 Ab HD 38529 b is an extrasolar planet approximately 138 light years away in the constellation of Orion. This planet was discovered in 2000. Because of its mass, it is likely that it is a gas giant.... , a 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... (Ac) and an unconfirmed planet (Ad)
148 G. Ori			39421	27713	5.95	0.62	379	A2Vn
120 G. Ori			37481	26535	5.96	−2.45	1567	B1.5IV
144 G. Ori			39051	27560	5.96	0.00	507	K2III
			39286	27747	5.96	−2.16	1370	B9V + G
			37171	26386	5.97	−1.04	821	K4II SB
134 G. Ori			38089	26926	5.97	2.47	163	F3V
142 G. Ori			38858	27435	5.97	5.01	51	G4V
145 G. Ori			39118	27588	5.97	−1.73	1128	G8III+...
155 G. Ori			39985	28110	5.97	−0.68	697	A0IV
17 G. Ori			31331	22840	5.98	−1.38	964	B5V
65 G. Ori			35281	25187	5.99	0.09	493	B8+...
123 G. Ori			37594	26624	5.99	2.91	135	A8Vs
150 G. Ori			39775	27939	5.99	−1.03	827	K0III
			44497	30318	6.00	2.00	205	F0III
117 G. Ori			37303	26427	6.03	−2.07	1358	B1Vvar
4 G. Ori			30545	22354	6.04	−0.64	707	K1III
31 G. Ori			32686	23643	6.04	−3.83	3075	B5IV
V1031 Ori (140 G. Ori)			38735	27341	6.04	−0.47	653	A4V
			42477	29371	6.04	0.44	430	A0Vnn
176 G. Ori			43285	29728	6.07	−0.72	743	B6V
47 G. Ori			33883	24349	6.08	−1.07	879	A5V
135 G. Ori			38309	27118	6.09	2.57	165	F0III:n
			41076	28686	6.09	0.25	480	A0Vs
W Ori			32736	23680	6.10	−0.56	700	N5	32 G. Orionis.
10 G. Ori			30870	22597	6.11	−0.56	704	B5V
40 G. Ori			33419	24041	6.11	1.19	314	K0III
114 G. Ori			37232	26414	6.11	−1.01	867	B2IV-V
			43683	29931	6.12	−0.33	637	A3V
66 G. Ori			35317	25240	6.13	2.31	189	F7V
			39632	27900	6.13	−2.15	1475	G9II
			31764	23161	6.14	−0.43	671	B7V
13 Ori		13	33021	23852	6.15	3.89	92	G1IV
52 G. Ori			34180	24493	6.15	2.84	150	F0IV
90 G. Ori			36558	25976	6.15	−2.16	1495	K5
161 G. Ori			37356	26477	6.16	−1.52	1120	B2IV-V
90 G. Ori			35588	25378	6.18	−2.25	1583	B2.5V
118 G. Ori			35693	25502	6.18	0.43	461	A1IV
CK Ori			36217	25785	6.21	−0.02	574	K2IIIvar	74 G. Orionis.
157 G. Ori			40347	28252	6.21	0.77	400	K0
125 G. Ori			37744	26713	6.22	−2.34	1680	B1.5V
156 G. Ori			40282	28232	6.22	0.21	519	M0III
87 G. Ori			36430	25869	6.23	−2.43	1762	B2V
41 G. Ori			33555	24130	6.24	2.82	158	G8III
75 G. Ori			35640	25401	6.24	−0.31	667	B9.5Vn
93 G. Ori			36779	26106	6.24	−1.66	1240	B2.5V
106 G. Ori			37016	26234	6.24	−1.46	1128	B2.5V
136 G. Ori			38495	27212	6.24	0.96	371	K1III...
183 G. Ori			43821	29982	6.24	1.11	346	K0
20 G. Ori			31623	23041	6.25	1.63	274	F2
99 G. Ori			36840	26149	6.25	−1.63	1230	G5
V1155 Ori			43819	30019	6.27	−0.16	631	B9IIIsp...	α² CVn variable
			39927	28019	6.28	1.32	321	A2III
			30869	22607	6.30	3.19	136	F5
149 G. Ori			39685	27902	6.30	0.16	552	K0
BL Ori			44984	30564	6.30	−1.70	1299	C5II
25 G. Ori			32115	23296	6.31	2.83	162	A8IV
V1197 Ori (133 G. Ori)			38099	26953	6.31	−0.28	679	K4III
1 G. Ori			30321	22189	6.33	1.68	277	A2V
48 G. Ori			33946	24377	6.33	−0.70	832	M0V
56 G. Ori			34748	24847	6.33	−2.45	1863	B1.5Vn
69 G. Ori			35407	25288	6.33	−1.55	1226	B4IVn
85 G. Ori			36285	25786	6.33	−1.53	1216	B2IV-V
21 G. Ori			31739	23092	6.34	0.62	454	A2V
V1649 Ori (63 G. Ori)			35242	25205	6.34	1.96	245	A2V	δ Sct variable
			35909	25638	6.35	1.38	322	A4V
			44867	30517	6.35	0.99	385	G9III
			35775	25505	6.36	0.78	425	K0
			42351	29326	6.37	−3.18	2650	K1II
179 G. Ori			43358	29746	6.37	1.53	303	F5IV:
			36058	25667	6.39	−0.45	762	A0Vn
			43335	29798	6.39	−0.35	728	K5II
58 G. Ori			34880	24925	6.40	−0.19	679	B8III
V1377 Ori (111 G. Ori)			37055	26263	6.40	−3.12	2608	B3IV
76 G. Ori			35656	25453	6.41	1.55	305	A0Vn
78 G. Ori			35912	25582	6.41	−1.35	1160	B2V
130 G. Ori			37904	26820	6.41	1.80	273	A9IV-V
19 G. Ori			31423	22938	6.42	2.57	192	F5
53 G. Ori			34317	24607	6.42	0.07	608	A0V
			34878	24960	6.43	0.91	415	G8IV
V1357 Ori			42807	29525	6.43	5.14	59	G8V
			35575	25368	6.44	−0.49	791	B3V
28 G. Ori			32273	23419	6.45	0.49	508	B8V
			36814	26104	6.45	0.00	637	K0
V1389 Ori (173 G. Ori)			42787	29509	6.45	−0.24	709	M...
129 G. Ori			37808	26728	6.46	0.38	536	B9.5IIIp Si
V1369 Ori			34959	25011	6.49	−1.42	1244	B5Vp	Be star
			36150	25732	6.49	1.09	391	A2
124 G. Ori			37635	26623	6.49	0.29	566	B7V
18 G. Ori			31411	22923	6.50	0.62	489	A0V
σ Ori B Sigma Orionis Sigma Orionis or Sigma Ori is a five-star system in the constellation Orion. It is approximately 1,150 light years from Earth....	σ	48	37479	26549	6.65	-1.08	1149	B2V...	component of the σ Ori system
θ¹ Ori D	θ¹	41	37023	26224	6.71			B0.5Vp...	component of the Trapezium
δ Ori B Delta Orionis Delta Orionis , traditionally known as Mintaka , is a star some 900 light years distant in the constellation Orion. Together with Zeta Orionis and Epsilon Orionis , the three stars make up the belt of Orion, known by many names across many ancient cultures...	δ	34	36485	25930	6.85	-0.39	916	O9.5II + B2V
HD 31253			31253	22826	7.13		175.5	F8	has a planet (b)
23 Ori	m	23	35148	25145	7.17	−0.21	976	B3Vn
HD 34445 HD 34445 HD 34445 is a 7th magnitude G-type star located approximately 152 light years away in the constellation Orion. This star is larger, hotter, brighter, and more massive than our Sun. Also its metal content is 40% greater than the Sun. In 2004, a gas giant planet was found in orbit around the star...			34445	24681	7.31	3.97	152	G0	has a planet (b HD 34445 b HD 34445 b is an extrasolar planet which orbits the G-type star HD 34445, located approximately 152 light years away in the constellation Orion. This planet was discovered in 2004 and finally confirmed in 2009. This planet has a minimum mass two-thirds that of Jupiter and orbits about 2 AU from the... )
θ¹ Ori B	θ¹	41	37021		7.96				component of the Trapezium
HD 38801			38801	27384	8.26	3.47	296	K0IV	has a planet (b)
σ Ori C Sigma Orionis Sigma Orionis or Sigma Ori is a five-star system in the constellation Orion. It is approximately 1,150 light years from Earth....	σ	48		26549	8.68	0.95	1148	A2V	component of the σ Ori system
HD 37605 HD 37605 HD 37605 is an orange dwarf star located approximately 140 light years away in the constellation Orion. In 2004, a planet was found in orbit....			37605	26664	8.69	5.53	140	K0	has a planet (b HD 37605 b HD 37605 b is an extrasolar planet that has nearly three times more mass than Jupiter. It orbits close to the star, taking 54 days to revolve around the parent star HD 37605. Its orbit is highly eccentric, around 74%... )
V2689 Ori Gliese 208 Gliese 208 is an orange dwarf star with an apparent magnitude of 8.9. It is about 0.47 solar masses.Bobylev's calculations from 2010 suggest that this star passed as close as 1.537 parsecs from the Sun about 500,000 years ago.- External links :*Wikisky of HD 245409...			245409	26335	8.9	8.6	37	K7
HD 290327 HD 290327 HD 290327 is a 9th magnitude G-type subgiant star located approximately 179 light years away in the constellation Orion. This star is larger, cooler, fainter, and less massive than our Sun. Also its metal content is seven-ninths as much as the Sun. In 2009, a gas giant planet was found in orbit...			290327	25191	8.96	5.26	179	G5IV	has a planet (b HD 290327 b HD 290327 b is an extrasolar planet which orbits the G-type subgiant star HD 290327, located approximately 179 light years away in the constellation Orion. This planet has at least five halves the mass of Jupiter and takes 6.7 years to orbit the star at a semimajor axis of 3.35 AU... )
Gl 179				22627	11.96	7.41	266	M3.5	has a planet (b Gliese 179 b Gliese 179 b is an extrasolar planet which orbits the M-type main sequence star Gliese 179, located approximately 40 light years away in the constellation Orion. This planet has a minimum mass a little bit less than Jupiter and it orbits at 2.41 AU or 361 Gm from the star with an eccentricity... )

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