27 Scorpii

This is the list of notable stars in the constellation Scorpius, sorted by decreasing brightness.

Zdroj:https://en.wikipedia.org?pojem=27_Scorpii
Text je dostupný za podmienok Creative Commons Attribution/Share-Alike License 3.0 Unported; prípadne za ďalších podmienok. Podrobnejšie informácie nájdete na stránke Podmienky použitia.

Navigácia: Veda >

Analytika
Antropológia
Aplikované vedy
Bibliometria
Dejiny vedy
Encyklopédie
Filozofia vedy
Forenzné vedy
Humanitné vedy
Knižničná veda
Kryogenika
Kryptológia
Kulturológia
Literárna veda
Medzidisciplinárne oblasti
Metódy kvantitatívnej analýzy
Metavedy
Metodika

Metodológia vedy
Náboženstvo a veda
Náučná literatúra
Podvody vo vede
Popularizácia vedy
Potravinárstvo
Prírodné vedy
Pseudoveda
Scientometria
Spoločenské vedy
Teórie
Teatrológia
Technické vedy
Technika
Terminológia
Umenie
Výskum

Veda
Veda a technika podľa štátu
Veda a technika podľa kontinentu
Veda a technika podľa roka
Veda v kozme
Vedci
Vedecká literatúra
Vedecké databázy
Vedecké experimenty
Vedecké konferencie
Vedecké metódy
Vedecké ocenenia
Vedecké organizácie
Vedecké parky
Vedeckí spisovatelia
Vzdelávanie
Záhady

Príbuzné výrazy:

Text je dostupný za podmienok Creative Commons Attribution/Share-Alike License 3.0 Unported; prípadne za ďalších podmienok.
Podrobnejšie informácie nájdete na stránke Podmienky použitia.

Name	B	F	Var	HD	HIP	RA	Dec	vis. mag.	abs. mag.	Dist. (ly)	Sp. class	Notes
Antares A	α	21		148478	80763	16^h 29^m 24.47^s	−26° 25′ 55.0″	0.91	−5.24	553	M1.5Iab-b	Cor Scorpii, Qalb al-Aqrab, Vespertilo; 16th brightest star; binary; semiregular variable, V_max = 0.75^m, V_min = 1.21^m, P = 2180 d
λ Sco	λ	35		158926	85927	17^h 33^m 36.53^s	−37° 06′ 13.5″	1.62	−5.05	703	B2IV+DA7.9	Shaula; β Cep and Algol variable, V_max = 1.59^m, V_min = 1.65^m, P = 0.21 d
θ Sco	θ			159532	86228	17^h 37^m 19.13^s	−42° 59′ 52.2″	1.86	−2.75	272	F1II	Sargas; suspected variable, V_max = 1.84^m, V_min = 1.88^m
δ Sco	δ	7		143275	78401	16^h 00^m 20.01^s	−22° 37′ 17.8″	2.29	−3.16	401	B0.2IVe	Dschubba, Al Jabba, Iclarkrau; γ Cas variable, V_max = 1.59^m, V_min = 2.32^m
ε Sco	ε	26		151680	82396	16^h 50^m 10.24^s	−34° 17′ 33.4″	2.29	0.78	65	K2IIIb	Wei, Larawag; suspected variable, V_max = 2.24^m, V_min = 2.35^m
κ Sco	κ			160578	86670	17^h 42^m 29.28^s	−39° 01′ 47.7″	2.39	−3.38	464	B1.5III	Girtab; β Cep variable, V_max = 2.41^m, V_min = 2.42^m, P = 0.20 d
β¹ Sco	β¹	8		144217	78820	16^h 05^m 26.23^s	−19° 48′ 19.4″	2.62	−3.44	530	B0.5V	Acrab, Elacrab, Graffias, Grafias, Grassias; suspected variable, V_max = 2.61^m, V_min = 2.67^m
υ Sco	υ	34		158408	85696	17^h 30^m 45.84^s	−37° 17′ 44.7″	2.70	−3.31	518	B2IV	Lesath, Lesuth
τ Sco	τ	23		149438	81266	16^h 35^m 52.96^s	−28° 12′ 57.5″	2.82	−2.78	430	B0V	Paikauhale,^[1] Alniyat, Al Niyat
π Sco	π	6		143018	78265	15^h 58^m 51.12^s	−26° 06′ 50.6″	2.89	−2.85	459	B1V + B2V	Fang; Nur;^[2] Vrischika, Iclil rotating ellipsoidal variable, V_max = 2.88^m, V_min = 2.91^m, P = 1.57 d
σ Sco	σ	20		147165	80112	16^h 21^m 11.32^s	−25° 35′ 33.9″	2.90	−3.86	734	B1III	Alniyat, Al Niyat, β Cep variable, V_max = 2.86^m, V_min = 2.94^m, P = 0.25 d
ι¹ Sco	ι¹			161471	87073	17^h 47^m 35.08^s	−40° 07′ 37.1″	2.99	−5.71	1791	F3Ia	Apollyon
μ¹ Sco	μ¹			151890	82514	16^h 51^m 52.24^s	−38° 02′ 50.4″	3.00	−4.01	821	B1.5IV + B	Xamidimura, Denebakrab; β Lyr variable, V_max = 2.94^m, V_min = 3.22^m, P = 1.45 d
G Sco	G			161892	87261	17^h 49^m 51.45^s	−37° 02′ 36.1″	3.19	0.24	127	K0/K1III	γ Tel, Fuyue
η Sco	η			155203	84143	17^h 12^m 09.18^s	−43° 14′ 18.6″	3.32	1.61	72	F3p	suspected variable
μ² Sco	μ²			151985	82545	16^h 52^m 20.15^s	−38° 01′ 02.9″	3.56	−2.44	517	B2IV	Pipirima, Shéngōng (神宮),^[3]
ζ² Sco	ζ²			152334	82729	16^h 54^m 35.11^s	−42° 21′ 38.7″	3.62	0.30	150	K4III	suspected variable, V_max = 3.59^m, V_min = 3.65^m
ρ Sco	ρ	5		142669	78104	15^h 56^m 53.09^s	−29° 12′ 50.4″	3.87	−1.62	409	B2IV/V	Iklil, suspected variable
ω¹ Sco	ω¹	9		144470	78933	16^h 06^m 48.43^s	−20° 40′ 08.9″	3.93	−1.64	423	B1V	Jabhat al Akrab
ν Sco	ν	14		145502	79374	16^h 11^m 59.74^s	−19° 27′ 38.3″	4.00	−1.63	436	B2IV	Jabbah, Jabah; quintuple star
H Sco	H			149447	81304	16^h 36^m 22.46^s	−35° 15′ 19.3″	4.18	−0.90	339	K5III	β Nor; suspected variable, V_max = 4.15^m, V_min = 4.18^m
N Sco	N			148703	80911	16^h 31^m 22.94^s	−34° 42′ 15.6″	4.24	−2.56	746	B2III-IV	α Nor
Q Sco	Q			159433	86170	17^h 36^m 32.85^s	−38° 38′ 05.5″	4.26	1.03	144	G8/K0III/IV	suspected variable, V_max = 4.26^m, V_min = 4.29^m
ω² Sco	ω²	10		144608	78990	16^h 07^m 24.30^s	−20° 52′ 07.2″	4.31	−0.24	265	G6/G8III	Jabhat al Akrab
ο Sco	ο	19		147084	80079	16^h 20^m 38.18^s	−24° 10′ 09.4″	4.55	−3.24	1177	A4II/III	suspected variable, V_max = 4.52^m, V_min = 4.58^m
13 Sco	c²	13		145482	79404	16^h 12^m 18.21^s	−27° 55′ 34.7″	4.58	−1.20	468	B2V
2 Sco	A	2		142114	77840	15^h 53^m 36.73^s	−25° 19′ 37.5″	4.59	−1.03	434	B2.5Vn
1 Sco	b	1		141637	77635	15^h 50^m 58.75^s	−25° 45′ 04.4″	4.63	−1.39	522	B1.5Vn
ζ¹ Sco	ζ¹			152236	82671	16^h 53^m 59.73^s	−42° 21′ 43.3″	4.70	−8.5	2,600	B1Iae	in NGC 6231; luminous blue variable, V_max = 4.66^m, V_min = 4.86^m
ξ Sco A	ξ			144070		16^h 04^m 22.10^s	−11° 22′ 23.0″	4.77		92		51 Lib; sextuple star
ι² Sco	ι²			161912	87294	17^h 50^m 11.11^s	−40° 05′ 25.5″	4.78	−5.50	3705	A6Ib	suspected variable
22 Sco	i	22		148605	80815	16^h 30^m 12.48^s	−25° 06′ 54.6″	4.79	−0.61	393	B3V	suspected variable
HD 161840				161840	87220	17^h 49^m 10.47^s	−31° 42′ 11.5″	4.79	−1.56	607	B8Ib/II
HD 146624	d			146624	79881	16^h 18^m 17.92^s	−28° 36′ 49.6″	4.80	1.63	140	A0V:
V1073 Sco	k		V1073	154090	83574	17^h 04^m 49.35^s	−34° 07′ 22.5″	4.83	−4.74	2672	B2Iab	α Cyg variable
HD 163145				163145	87846	17^h 56^m 47.43^s	−44° 20′ 31.9″	4.85	−0.29	347	K2III
HD 163376				163376	87936	17^h 57^m 47.81^s	−41° 42′ 58.5″	4.88	−1.24	547	M0III	suspected variable
β² Sco	β²			144218	78821	16^h 05^m 26.58^s	−19° 48′ 06.6″	4.90	−2.80	530	B2V	component of the β Sco system
ψ Sco	ψ	15		145570	79375	16^h 12^m 00.00^s	−10° 03′ 51.1″	4.93	1.41	165	A3IV
HD 143787				143787	78650	16^h 03^m 20.67^s	−25° 51′ 54.5″	4.96	0.90	212	K3III
HD 153613				153613	83336	17^h 01^m 52.65^s	−32° 08′ 36.2″	5.03	−0.86	491	B8V
HD 154948				154948	84033	17^h 10^m 42.35^s	−44° 33′ 27.2″	5.06	0.24	300	G8/K0III+..
ξ Sco B	ξ			144069	78727	16^h 04^m 22.3^s	−11° 22′ 18″	5.07		92	F5IV	component of the ξ Sco system
HD 145250				145250	79302	16^h 11^m 02.13^s	−29° 24′ 57.6″	5.09	0.62	255	K0III
HD 157243				157243	85162	17^h 24^m 13.09^s	−44° 09′ 45.0″	5.10	−1.73	756	B7III
Antares B	α	21		148479		16^h 29^m 24.2^s	−26° 25′ 51″	5.2	−0.9	553	B2.5V	component of the Antares system
HD 151804			V973	151804	82493	16^h 51^m 33.72^s	−41° 13′ 49.9″	5.23	−6.36	6792	O8Iaf	α Cyg variable, V_max = 5.22^m, V_min = 5.28^m
χ Sco	χ	17		145897	79540	16^h 13^m 50.91^s	−11° 50′ 15.8″	5.24	−0.41	439	K3III
HD 148688			V1058	148688	80945	16^h 31^m 41.77^s	−41° 49′ 01.7″	5.31	−6.79	8579	B1Ia	α Cyg variable
HD 144690				144690	79050	16^h 08^m 07.52^s	−26° 19′ 36.0″	5.35	−0.23	425	M2III	variable star, ΔV = 0.008^m, P = 7.61 d
HD 147513				147513	80337	16^h 24^m 01.24^s	−39° 11′ 34.8″	5.37	4.82	42	G3/G5V	has a planet (b)
HD 142165				142165	77858	15^h 53^m 53.92^s	−24° 31′ 59.1″	5.38	−0.14	414	B5V
HR 5907			V1040	142184	77859	15^h 53^m 55.87^s	−23° 58′ 40.9″	5.41	0.01	393	B2V	Algol variable, V_max = 5.39^m, V_min = 5.43^m, P = 1.02 d
HD 147628				147628	80390	16^h 24^m 31.77^s	−37° 33′ 57.5″	5.42	−0.36	468	B8V	suspected rotating ellipsoidal variable, ΔV = 0.02^m
HD 142990			V913	142990	78246	15^h 58^m 34.87^s	−24° 49′ 53.1″

[1]

[2]

[3]