292:, is so luminous that it is likely what is causing most of the surrounding ring to glow. In fact its powerful stellar winds are what cleared out the surrounding warm dust and created the ring-shaped feature in the first place. The bright greenish-yellow region left of center is similar to the ring, though more dense. The bluish-white stars scattered throughout are stars located both in front of, and behind, the nebula.
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The green ring is made of tiny particles of warm dust whose composition is very similar to smog. The red cloud in the middle is probably made of dust that is more metallic and cooler than the surrounding regions. The bright star in the middle of the red cloud, called
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light. Blue and cyan (blue-green) represent light emitted at wavelengths of 3.4 and 4.6 microns, which is predominantly from stars. Green and red represent light from 12 and 22 microns, respectively, which is mostly emitted by dust.
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Regions similar to this nebula are found near the band of the Milky Way in the night sky. The "wreath" is slightly off this band, near the boundary between the constellations of
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and Taurus, but at a relatively close distance of only about 1,000 light-years, the cloud is a still part of our Milky Way.
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with a radius of about 22 light-years, located about 1,000 light-years away within the
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The colors used in this image represent specific wavelengths of
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complex, near the boundary with the constellation of
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403:National Aeronautics and Space Administration
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51:introducing citations to additional sources
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284:, places where new stars are being born.
41:Relevant discussion may be found on the
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167:+31° 55′ 33″
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7:
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401:from websites or documents of the
355:. You can help Knowledge (XXG) by
14:
351:This nebula-related article is a
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397: This article incorporates
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34:relies largely or entirely on a
23:
16:Nebula in constellation Perseus
1:
133:Barnard 3, the Wreath Nebula.
1985:650 (Little Dumbbell Nebula)
455:Perseus in Chinese astronomy
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2236:UGC 2885 (Godzilla galaxy)
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126:
2000:1499 (California Nebula)
450:List of stars in Perseus
439:Constellation of Perseus
205:Physical characteristics
2352:Perseus (constellation)
270:Perseus molecular cloud
399:public domain material
1756:HAT-P-29 (Muspelheim)
254:IRAS Ring G159.6-18.5
2100:1175 (Peanut Galaxy)
1946:Alpha Persei Cluster
1751:HAT-P-15 (Berehynia)
557:π (Gorgonea Secunda)
47:improve this article
2285:Astronomical events
587:ω (Gorgonea Quarta)
562:ρ (Gorgonea Tertia)
324:Wreath Nebula from
278:Interstellar clouds
116:
1842:WASP-11b/HAT-P-10b
139:Observation data:
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282:stellar nurseries
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2342:Emission nebulae
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1796:NGC 1333 IRAS 4B
1791:NGC 1333 IRAS 4A
1786:NGC 1333 IRAS 2A
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237:Lists of nebulae
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1761:IRAS 04296+3429
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280:like these are
258:emission nebula
248:(also known as
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151:Right ascension
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121:Emission nebula
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62:"Wreath Nebula"
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2026:Wreath Nebula
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246:Wreath Nebula
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194:Constellation
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115:Wreath Nebula
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64: –
63:
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58:Find sources:
52:
48:
44:
38:
37:
36:single source
32:This article
30:
26:
21:
20:
2337:Nebula stubs
2025:
1806:PSR B0355+54
1166:
794:
391:
357:expanding it
350:
328:
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245:
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227:Designations
100:
90:
83:
76:
69:
57:
33:
2347:Perseus Arm
2021:Barnard 203
1781:NGC 1333 13
1766:L1448-IRS2E
262:H II region
176:306.6
163:Declination
2331:Categories
1956:Trumpler 2
1834:Exoplanets
1801:NGC 1624-2
1776:LRLL 54361
547:ξ (Menkib)
482:α (Mirfak)
311:References
235:See also:
156:03 39 55.8
73:newspapers
2293:SN 2006gy
2241:4C +37.11
1731:BD+48 740
1726:BD+31 643
602:Flamsteed
527:κ (Misam)
512:η (Miram)
487:β (Algol)
290:HD 278942
266:Milky Way
250:Barnard 3
230:Barnard 3
103:July 2019
43:talk page
2318:Category
2298:Perseids
2040:Galaxies
1858:clusters
1771:LkHα 101
807:Variable
552:ο (Atik)
331:mission.
304:infrared
218: ly
172:Distance
1970:Nebulae
1880:884 (χ)
1875:869 (h)
1741:G 95-57
1736:G 38-29
1347:918 (k)
297:Perseus
268:in the
199:Perseus
87:scholar
2231:IC 310
1951:IC 348
1167:61 And
1165:V520 (
785:58 (e)
780:57 (m)
760:53 (d)
755:52 (f)
740:48 (c)
735:43 (A)
730:42 (n)
725:40 (o)
710:32 (l)
274:Taurus
256:is an
211:Radius
185:
89:
82:
75:
68:
60:
2224:Other
2014:Other
1939:Other
1746:GD 61
1719:Other
1710:29587
1705:26702
1700:25329
1695:23596
1690:23301
1685:22781
1680:21684
1675:17605
1670:17245
1665:17092
1660:16760
1655:16691
1650:14434
1645:14433
1640:13519
1219:V1024
796:1 Aur
645:9 (i)
625:4 (g)
474:Bayer
465:Stars
144:epoch
141:J2000
94:JSTOR
80:books
2215:1334
2210:1294
2205:1293
2200:1283
2195:1282
2190:1281
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2110:1250
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2065:1058
2060:1023
2055:1003
2005:1579
1995:1491
1990:1333
1930:1624
1925:1545
1920:1528
1915:1513
1910:1444
1905:1342
1900:1285
1895:1220
1890:1039
1856:Star
1816:WR 4
1622:1514
1617:1500
1612:1493
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1422:1001
1214:V718
1209:V621
1204:V576
1199:V575
1194:V573
1189:V572
1184:V551
1179:V545
1174:V521
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1125:V472
1120:V471
1115:V461
1110:V459
1105:V440
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1080:V392
1075:V386
1070:V380
1065:V376
1060:V361
1055:V357
1050:V356
1045:V351
353:stub
329:WISE
326:NASA
260:and
244:The
183:1000
66:news
2048:NGC
1978:NGC
1885:957
1867:NGC
1417:991
1412:986
1407:979
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1397:973
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1267:641
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1247:529
1242:526
1237:470
252:or
181:or
49:by
2333::
1632:HD
1229:HR
1040:LX
1035:KW
1030:KT
1025:KS
1020:KP
1015:IZ
1010:IX
1005:IW
1000:IU
995:IQ
990:IP
985:IK
980:GK
975:FO
970:DY
965:DM
960:BM
955:AX
950:AW
945:AS
940:AR
935:AG
930:AB
925:YZ
920:XZ
915:XY
910:XX
905:VX
900:UY
895:UX
890:UV
885:TZ
880:SV
875:SU
870:ST
865:RY
860:RW
855:RV
850:RT
845:RS
790:59
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405:.
276:.
216:22
187:ly
178:pc
1169:)
840:Z
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830:V
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820:T
815:S
640:8
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620:3
615:2
610:1
592:b
582:ψ
577:φ
572:τ
567:σ
542:ν
537:μ
532:λ
522:ι
517:θ
507:ζ
502:ε
497:δ
492:γ
431:e
424:t
417:v
384:e
377:t
370:v
359:.
105:)
101:(
91:·
84:·
77:·
70:·
53:.
39:.
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