1100:"}},"text\/plain":{"en":{"":"checksum"}}},"{\"value\":\"70fd7d0343e373fa0ac4735eeaf1fe26fe26e548\",\"type\":\"string\"}":{"text\/html":{"en":{"P4092":"70fd7d0343e373fa0ac4735eeaf1fe26fe26e548"}},"text\/plain":{"en":{"P4092":"70fd7d0343e373fa0ac4735eeaf1fe26fe26e548"}}},"{\"value\":{\"entity-type\":\"property\",\"numeric-id\":459,\"id\":\"P459\"},\"type\":\"wikibase-entityid\"}":{"text\/html":{"en":{"":"
327:الخيوط البرتقالية الظاهرة في الصورة هي أشلاء وشظايا متبقّية من النجم الذي انفجر (وكوّن السديم) وهي تتركب بشكل رئيسي من الهيدروجين. النجم النيوتروني سريع "الدوران المحوري" المتواري في وسط السديم يَعمل كمولد طاقة يُسبب البريق المُزرقّ الغريب المُشع من وسط السديم. وهذا الضوء الأزرق قادم من إلكترونات تدور بما يُقارب سرعة الضوء حول الحقل المغناطيسي للنجم النيوتروني. النجم النيوتروني, مثل المنارة, يُطلق شعاعين من الضوء في اتجاهين مختلفين يَجعلناه يبدو كأنه ينبض 30 مرة في الثانية نتيجة لدورانه المحوري السريع (النجوم النيوترونية تُتم بضعة دورات حول نفسها في الثانية على الأقل). والنجم النيوتروني هو نواة مسحوقة شديدة الكثافة لنجم انفجر.
980:"}},"text\/plain":{"en":{"":"inception"}}},"{\"value\":{\"time\":\"+2005-12-01T00:00:00Z\",\"timezone\":0,\"before\":0,\"after\":0,\"precision\":11,\"calendarmodel\":\"http:\\\/\\\/www.wikidata.org\\\/entity\\\/Q1985727\"},\"type\":\"time\"}":{"text\/html":{"en":{"P571":"1 December 2005"}},"text\/plain":{"en":{"P571":"1 December 2005"}}}}": -->
494:
138:
1096:
524:
535:
196:
148:
43:
707:
688:
669:
650:
631:
612:
593:
574:
442:
226:
103:
768:
681:
677:
310:
bleue provient des électrons tourbillonnant presque à la vitesse de la lumière autour de lignes du champ magnétique de l'étoile à neutrons. L'étoile à neutrons, comme un phare, émet des faisceaux de rayonnements jumeaux qui semblent battre 30 fois par seconde en raison de la rotation de l'étoile à neutrons. Une étoile à neutrons est le noyau écrasé ultra-dense de l'étoile qui a explosé.
1056:"}},"text\/plain":{"en":{"":"Commons quality assessment"}}},"{\"value\":{\"entity-type\":\"item\",\"numeric-id\":63348049,\"id\":\"Q63348049\"},\"type\":\"wikibase-entityid\"}":{"text\/html":{"en":{"P6731":"
1104:"}},"text\/plain":{"en":{"":"determination method"}}},"{\"value\":{\"entity-type\":\"item\",\"numeric-id\":13414952,\"id\":\"Q13414952\"},\"type\":\"wikibase-entityid\"}":{"text\/html":{"en":{"P459":"
1167:"}},"text\/plain":{"en":{"":"data size"}}},"{\"value\":{\"amount\":\"+14508851\",\"unit\":\"http:\\\/\\\/www.wikidata.org\\\/entity\\\/Q8799\"},\"type\":\"quantity\"}":{"text\/html":{"en":{"P3575":"14,508,851
1018:"}},"text\/plain":{"en":{"":"media type"}}},"{\"value\":\"image\\\/jpeg\",\"type\":\"string\"}":{"text\/html":{"en":{"P1163":"image\/jpeg"}},"text\/plain":{"en":{"P1163":"image\/jpeg"}}}}": -->
916:"}},"text\/plain":{"en":{"P180":"Crab Nebula"}}},"{\"value\":{\"entity-type\":\"item\",\"numeric-id\":1044623,\"id\":\"Q1044623\"},\"type\":\"wikibase-entityid\"}":{"text\/html":{"en":{"P180":"
1212:"}},"text\/plain":{"en":{"":"height"}}},"{\"value\":{\"amount\":\"+3864\",\"unit\":\"http:\\\/\\\/www.wikidata.org\\\/entity\\\/Q355198\"},\"type\":\"quantity\"}":{"text\/html":{"en":{"P2048":"3,864
1257:"}},"text\/plain":{"en":{"":"width"}}},"{\"value\":{\"amount\":\"+3864\",\"unit\":\"http:\\\/\\\/www.wikidata.org\\\/entity\\\/Q355198\"},\"type\":\"quantity\"}":{"text\/html":{"en":{"P2049":"3,864
912:"}},"text\/plain":{"en":{"":"depicts"}}},"{\"value\":{\"entity-type\":\"item\",\"numeric-id\":10934,\"id\":\"Q10934\"},\"type\":\"wikibase-entityid\"}":{"text\/html":{"en":{"P180":"
1253:
287:
The newly composed image was assembled from 24 individual Wide Field and
Planetary Camera 2 exposures taken in October 1999, January 2000, and December 2000. The colors in the image indicate the different elements that were expelled during the explosion. Blue in the filaments in the outer part of the
1430:
1400:
1370:
586:
387:
Material credited to STScI on this site was created, authored, and/or prepared for NASA under
Contract NAS5-26555. Unless otherwise specifically stated, no claim to copyright is being asserted by STScI and it may be freely used as in the public domain in accordance with NASA's contract. However, it
280:
The orange filaments are the tattered remains of the star and consist mostly of hydrogen. The rapidly spinning neutron star embedded in the center of the nebula is the dynamo powering the nebula's eerie interior bluish glow. The blue light comes from electrons whirling at nearly the speed of light
284:
The Crab Nebula derived its name from its appearance in a drawing made by Irish astronomer Lord Rosse in 1844, using a 36-inch telescope. When viewed by Hubble, as well as by large ground-based telescopes such as the
European Southern Observatory's Very Large Telescope, the Crab Nebula takes on a
309:
Les filaments oranges sont les restes en lambeaux de l'étoile et se composent principalement d'hydrogène. L'étoile à neutrons qui tourne rapidement sur elle-même, intégrée dans le centre de la nébuleuse, est la dynamo alimentant l'intérieur de la nébuleuse de l'étrange lueur bleuâtre. La lumière
312:
L'image est formée de l'assemblage de 24 prises individuelles de la Wide Field and
Planetary Camera 2 datant d'octobre 1999, janvier 2000 et décembre 2000. Les couleurs de l'image indiquent les différents éléments qui ont été expulsé lors de l'explosion. Le bleu dans les filaments de la partie
306:
de la NASA, est en réalité une mosaïque de plusieurs clichés. La nébuleuse s'étend sur une distance de six années-lumière et est composée des restes de l'explosion d'une supernova. Les astronomes chinois et japonais ont observé cette violente explosion il y a environ un millénaire, en 1054.
662:
1340:
281:
around magnetic field lines from the neutron star. The neutron star, like a lighthouse, ejects twin beams of radiation that appear to pulse 30 times a second due to the neutron star's rotation. A neutron star is the crushed ultra-dense core of the exploded star.
1477:
Image: A New View of the Helix Nebula Source: http://hubblesite.org/gallery/album/entire_collection/pr2004032d/ Copyright Notice: Material credited to STScI on this site was created, authored, and/or prepared for NASA under
Contract NAS5-26555. Unless
388:
is requested that in any subsequent use of this work NASA and STScI be given appropriate acknowledgement. STScI further requests voluntary reporting of all use, derivative creation, and other alteration of this work. Such reporting should be sent to
658:
462:. NASA Hubble material (and ESA Hubble material prior to 2009) is copyright-free and may be freely used as in the public domain without fee, on the condition that only NASA, STScI, and/or ESA is credited as the source of the material.
325:, وهو بقايا مستعر أعظم تمتد على مساحة قطرها 6 سنوات ضوئية. قام الفلكيون القدماء العرب والصينيون بتسجيل هذا الحدث قبل 1,000 عام في سنة 1054م, كما فعل ذلك البحارة الأمريكيون (بالرغم من أنه ليس من المؤكد تماماً أن ما سجلوه هو هذا).
137:
2261:
2196:
719:
582:
605:
1105:
1057:
643:
917:
846:
The Crab Nebula as seen by the Hubble Space
Telescope (HST). The Nebula is a Supernova Nebula — One formed from a supernova which left a millisecond pulsar at its center.
913:
169:
it as one of the finest images on the
English Knowledge, adding significantly to its accompanying article. If you have a different image of similar quality, be sure to
164:
1254:
1209:
1164:
1097:
1053:
1015:
1101:
977:
909:
557:
467:
The material was created for NASA by Space
Telescope Science Institute under Contract NAS5-26555, or for ESA by the Hubble European Space Agency Information Centre.
624:
700:
2216:
2251:
1350:
2226:
278:, a six-light-year-wide expanding remnant of a star's supernova explosion. Japanese and Chinese astronomers recorded this violent event in 1054 CE.
2256:
2211:
1410:
212:
715:
775:
2483:
322:
1998:
1489:
380:
2271:
2488:
313:
extérieure de la nébuleuse représente l'oxygène neutre, le vert est le souffre ionisé I, et le rouge indique l'oxygène ionisé II.
1149:
1083:
2151:
963:
182:
158:
2301:
This file contains additional information, probably added from the digital camera or scanner used to create or digitize it.
1060:"}},"text\/plain":{"en":{"P6731":"Wikimedia Commons featured picture"}}}}": -->
389:
743:
946:
472:
2290:
1268:
1223:
1178:
1115:
1067:
1025:
1901:
2181:
2141:
1142:
987:
930:
639:
464:
This license does not apply if ESA material created after 2008 or source material from other organizations is in use.
1981:
601:
234:
178:
2281:
696:
69:
65:
174:
61:
57:
53:
47:
2304:
If the file has been modified from its original state, some details may not fully reflect the modified file.
1781:
1488:
More than 100 pages use this file. The following list shows the first 100 pages that use this file only. A
203:
114:
2206:
2176:
1459:
1454:
1429:
1424:
1399:
1394:
1369:
1364:
288:
nebula represents neutral oxygen, green is singly-ionized sulfur, and red indicates doubly-ionized oxygen.
285:
more detailed appearance that yields clues into the spectacular demise of a star, 6,500 light-years away.
2403:
1931:
1831:
1171:"}},"text\/plain":{"en":{"P3575":"14,508,851 byte"}}}}": -->
154:
82:
2478:
1801:
553:
1261:"}},"text\/plain":{"en":{"P2049":"3,864 pixel"}}}}": -->
1216:"}},"text\/plain":{"en":{"P2048":"3,864 pixel"}}}}": -->
353:
2276:
2241:
2236:
2221:
2191:
920:"}},"text\/plain":{"en":{"P180":"Crab Pulsar"}}}}": -->
1976:
1941:
1916:
1611:
620:
298:
739:
122:
1886:
1841:
1736:
1496:
479:
459:
274:
This is a mosaic image, one of the largest ever taken by NASA's Hubble Space
Telescope, of the
1108:"}},"text\/plain":{"en":{"P459":"SHA-1"}}}}": -->
147:
1771:
1631:
1811:
1741:
1666:
483:
195:
8:
1946:
1796:
1766:
1616:
1571:
1470:
493:
403:
2231:
2021:
1936:
1921:
1601:
1501:
731:
2036:
1671:
1866:
1661:
208:
109:
2031:
2026:
1380:
1966:
1826:
1816:
1776:
1636:
349:
1986:
1821:
1731:
1521:
1339:
1334:
735:
399:
73:
42:
2056:
321:هذه الصورة المركبة, هي واحدة من أكبر الصور على الإطلاق التي التقطها تلسكوب هبل ل
1956:
1926:
1906:
1876:
1786:
1726:
1706:
1701:
1596:
1561:
1541:
450:
170:
2051:
2472:
1961:
1951:
1911:
1891:
1806:
225:
825:
2266:
1896:
1646:
1440:
275:
239:
2101:
2086:
2418:
1871:
1851:
1846:
1721:
1716:
1711:
1556:
1278:
1233:
1188:
1125:
1077:
1035:
997:
957:
940:
1971:
1761:
1746:
1681:
2076:
796:
730:
If you have an image of similar quality that can be published under a
2201:
2161:
1991:
1861:
1856:
1751:
1691:
1656:
1651:
1591:
1586:
1526:
1506:
2126:
1686:
1676:
1641:
1621:
1581:
1307:
Click on a date/time to view the file as it appeared at that time.
468:
2111:
1566:
1551:
718:) and is considered one of the finest images. See its nomination
699:) and is considered one of the finest images. See its nomination
680:) and is considered one of the finest images. See its nomination
661:) and is considered one of the finest images. See its nomination
642:) and is considered one of the finest images. See its nomination
623:) and is considered one of the finest images. See its nomination
604:) and is considered one of the finest images. See its nomination
585:) and is considered one of the finest images. See its nomination
556:) and is considered one of the finest images. See its nomination
2091:
2246:
2186:
2171:
2166:
1881:
1696:
1576:
1546:
1536:
1516:
2071:
1791:
1756:
1626:
1531:
455:
364:
1836:
1606:
1511:
368:
2066:
762:
2116:
2096:
338:
97:
87:(3,864 × 3,864 pixels, file size: 13.84 MB, MIME type:
2081:
2041:
2131:
1486:
404:
https://www.flickr.com/photos/nasahubble/27747556420/
2106:
2007:
1305:
121:
Commons is a freely licensed media file repository.
508:
482:on the spacetelescope.org site since 2009, use the
2061:
820:
371:, J. Hester and A. Loll (Arizona State University)
2046:
2016:
817:
2470:
509:
823:
473:2008 copyright statement at spacetelescope.org
400:https://www.flickr.com/photos/gsfc/4398655649/
102:
814:
811:
808:
805:
375:
334:
261:
436:
395:
360:
344:
14:
1258:
1213:
1168:
804:
2022:Knowledge:Uitgesoekte herdenkings/22 April
2037:Knowledge:Uitgesoekte herdenkings/4 Julie
2009:The following other wikis use this file:
534:
1131:70fd7d0343e373fa0ac4735eeaf1fe26fe26e548
523:
296:Cette image, une des plus grandes de la
133:
2032:Knowledge:Uitgesoekte herdenkings/April
2027:Knowledge:Uitgesoekte herdenkings/Julie
886:A Rák-köd a Hubble Űrtávcső felvételén.
302:jamais prises par le télescope spatial
2471:
469:Copyright statement at hubblesite.org
441:
250:
784:
220:
190:
142:
2057:Knowledge:Voorbladbeeld week 2 2012
1298:
714:on the Chinese language Knowledge (
695:on the Turkish language Knowledge (
657:on the Persian language Knowledge (
638:on the Spanish language Knowledge (
619:on the English language Knowledge (
13:
2484:Knowledge Picture of the day files
2299:
1902:Hypothetical types of biochemistry
1084:Wikimedia Commons featured picture
1058:Wikimedia Commons featured picture
907:
901:
893:
885:
877:
869:
861:
853:
845:
773:
600:on the German language Knowledge (
581:on the Arabic language Knowledge (
492:
315:
290:
268:
251:
134:
80:
2500:
2306:
2052:Knowledge:Beeld van die week/2012
906:
676:on the Tamil language Knowledge (
539:
135:
1982:Talk:Cosmic microwave background
836:
766:
705:
686:
667:
648:
629:
610:
591:
572:
538:
533:
522:
440:
224:
194:
146:
136:
101:
31:
21:
2452:Date metadata was last modified
2262:بوابة:الفيزياء/بوابات ذات علاقة
833:
797:View the annotations at Commons
269:
2489:Stars portal selected pictures
2004:
1302:
832:
316:
291:
181:it to a relevant article, and
26:
1:
2087:Portaal:Sterrekunde/Inleiding
854:Krebsnebel im Sternbild Stier
504:
36:
2197:بوابة:علم الفلك/مقالة مختارة
1782:Classical Kuiper belt object
1483:
926:Items portrayed in this file
478:For material created by the
412:
7:
2444:Date and time of digitizing
2404:Adobe Photoshop CS2 Windows
2296:
2148:Usage on anp.wikipedia.org
2123:Usage on als.wikipedia.org
1932:Wuxing (Chinese philosophy)
1832:Cosmic microwave background
902:Messier 1(Yengeç Bulutsusu)
774:This image was selected as
201:This image was selected as
10:
2505:
2158:Usage on ar.wikipedia.org
2138:Usage on am.wikipedia.org
2013:Usage on af.wikipedia.org
1068:Commons quality assessment
1054:Commons quality assessment
732:suitable copyright license
513:
454:because it was created by
258:
253:
2410:File change date and time
2077:Lys van Messier-voorwerpe
1299:
794:This image is annotated:
566:
531:
520:
232:This image featured as a
16:
2102:Lys van planetêre newels
1942:Talk:Anthropic principle
1917:Minute and second of arc
1612:Aquarius (constellation)
835:
778:on Vietnamese Knowledge.
159:members of the community
108:This is a file from the
41:
2455:06:37, 28 November 2005
2447:06:37, 28 November 2005
2413:11:37, 28 November 2005
1476:
1446:
1416:
1386:
1356:
1335:14:56, 25 November 2012
337:
112:. Information from its
2127:Vorlage:Houptsyte/4.07
1887:Double-slit experiment
1842:Cygnus (constellation)
1802:Comet Shoemaker–Levy 9
1737:Carina (constellation)
1497:Aberration (astronomy)
1455:00:35, 16 January 2006
552:on Wikimedia Commons (
497:
115:description page there
46:Size of this preview:
2376:Horizontal resolution
2227:فيلا (أقمار اصطناعية)
2217:علم الفلك خارج المجري
1772:Charge-coupled device
1632:Aries (constellation)
1357:Lossless optimization
678:இன்றைய சிறப்புப் படம்
496:
480:European Space Agency
2368:Number of components
2252:نظرية الحالة الثابتة
2112:Supernova-oorblyfsel
1977:Talk:Comet Hale–Bopp
1812:Copernican principle
1742:Carl Friedrich Gauss
1667:Background radiation
1143:determination method
1102:determination method
448:This file is in the
173:it using the proper
74:3,864 × 3,864 pixels
70:2,048 × 2,048 pixels
66:1,024 × 1,024 pixels
2384:Vertical resolution
2092:Portaal:Sterrekunde
1947:Talk:Apollo program
1767:Chandrasekhar limit
1672:Barnard's Star
1617:Ara (constellation)
1572:Anthropic principle
1425:21:26, 9 March 2006
1395:09:31, 20 June 2009
640:Recursos destacados
157:, which means that
52:Other resolutions:
2344:Compression scheme
2326:Bits per component
2272:اقتران (علم الفلك)
2257:توهج القمر الصناعي
2212:جمعية منسا الدولية
1937:Talk:3753 Cruithne
1922:Physical cosmology
1602:Apparent magnitude
1502:Absolute magnitude
1417:Higher resolution.
1365:10:13, 17 May 2012
894:კირჩხიბის ნისლეული
776:picture of the day
498:
299:Nébuleuse du Crabe
204:picture of the day
2479:Featured pictures
2467:
2466:
2352:Pixel composition
2291:more global usage
2072:Veranderlike ster
2005:Global file usage
1867:Diatomic molecule
1662:Astronomical unit
1481:
1260:
1215:
1170:
900:
892:
884:
878:صورة سديم السرطان
876:
868:
860:
852:
844:
803:
802:
783:
782:
760:
759:
756:
755:
752:
751:
727:
726:
659:نگارههای برگزیده
621:Featured pictures
602:Exzellente Bilder
554:Featured pictures
502:
501:
489:
435:
434:
409:
408:
384:
381:Reusing this file
247:
246:
219:
218:
213:December 25, 2006
209:English Knowledge
189:
188:
130:
129:
110:Wikimedia Commons
32:Global file usage
2496:
2392:Data arrangement
2307:
1967:Talk:Capricornus
1827:Cosmic inflation
1817:Corona Australis
1777:Chemical formula
1637:Arthur Eddington
1467:
1437:
1407:
1377:
1347:
1309:
1287:
1242:
1197:
1152:
1147:
898:
890:
882:
874:
866:
858:
850:
842:
785:
770:
769:
763:
712:featured picture
710: This is a
709:
708:
693:featured picture
691: This is a
690:
689:
674:featured picture
672: This is a
671:
670:
655:featured picture
653: This is a
652:
651:
636:featured picture
634: This is a
633:
632:
617:featured picture
615: This is a
614:
613:
598:featured picture
596: This is a
595:
594:
579:featured picture
577: This is a
576:
575:
564:
563:
550:featured picture
542:
541:
537:
536:
526:
525:
518:
517:
514:
510:
486:
477:
444:
443:
437:
431:
428:
425:
422:
417:
416:
378:
340:
320:
295:
293:Français :
273:
265:
259:
228:
221:
198:
191:
175:free license tag
155:featured picture
150:
143:
140:
126:
105:
104:
98:
92:
90:
77:
62:768 × 768 pixels
58:480 × 480 pixels
54:240 × 240 pixels
48:600 × 600 pixels
2504:
2503:
2499:
2498:
2497:
2495:
2494:
2493:
2469:
2468:
2295:
2003:
1987:Talk:Cosmic ray
1822:Corona Borealis
1797:Comet Hale–Bopp
1732:Carbon monoxide
1522:Albert Einstein
1482:
1473:
1465:
1443:
1435:
1413:
1405:
1383:
1375:
1353:
1345:
1301:
1300:
1297:
1296:
1295:
1294:
1293:
1292:
1291:
1290:
1288:
1285:
1275:
1274:
1273:
1271:
1252:
1251:
1250:
1249:
1248:
1247:
1246:
1245:
1243:
1240:
1230:
1229:
1228:
1226:
1207:
1206:
1205:
1204:
1203:
1202:
1201:
1200:
1198:
1195:
1185:
1184:
1183:
1181:
1162:
1161:
1160:
1159:
1158:
1157:
1156:
1155:
1154:
1153:
1148:
1145:
1136:
1135:
1134:
1132:
1122:
1121:
1120:
1118:
1095:
1094:
1093:
1092:
1091:
1090:
1089:
1088:
1086:
1074:
1073:
1072:
1070:
1051:
1050:
1049:
1048:
1047:
1046:
1045:
1044:
1042:
1032:
1031:
1030:
1028:
1013:
1012:
1011:
1010:
1009:
1008:
1007:
1006:
1004:
1003:1 December 2005
994:
993:
992:
990:
975:
974:
973:
972:
971:
970:
969:
968:
966:
955:
954:
953:
952:
951:
949:
937:
936:
935:
933:
905:
904:
903:
896:
895:
888:
887:
880:
879:
872:
871:
864:
863:
856:
855:
848:
847:
830:
829:
822:
819:
816:
813:
810:
807:
791:
779:
767:
761:
706:
697:Seçkin resimler
687:
668:
649:
630:
611:
592:
573:
507:
484:
429:
426:
423:
420:
415:
410:
339:1 December 2005
330:
314:
289:
264:Crab Nebula.jpg
263:
256:
249:
248:
243:
141:
132:
131:
120:
119:
118:is shown below.
94:
88:
86:
79:
78:
51:
12:
11:
5:
2502:
2492:
2491:
2486:
2481:
2465:
2464:
2461:
2457:
2456:
2453:
2449:
2448:
2445:
2441:
2440:
2437:
2433:
2432:
2429:
2425:
2424:
2421:
2415:
2414:
2411:
2407:
2406:
2401:
2397:
2396:
2393:
2389:
2388:
2385:
2381:
2380:
2377:
2373:
2372:
2369:
2365:
2364:
2361:
2357:
2356:
2353:
2349:
2348:
2345:
2341:
2340:
2339:
2338:
2335:
2332:
2327:
2323:
2322:
2319:
2315:
2314:
2311:
2298:
2293:of this file.
2287:
2286:
2285:
2284:
2279:
2274:
2269:
2264:
2259:
2254:
2249:
2244:
2239:
2234:
2229:
2224:
2219:
2214:
2209:
2204:
2199:
2194:
2189:
2184:
2179:
2174:
2169:
2164:
2156:
2155:
2154:
2146:
2145:
2144:
2136:
2135:
2134:
2129:
2121:
2120:
2119:
2114:
2109:
2104:
2099:
2094:
2089:
2084:
2079:
2074:
2069:
2064:
2059:
2054:
2049:
2044:
2039:
2034:
2029:
2024:
2019:
2006:
2001:to this file.
1995:
1994:
1989:
1984:
1979:
1974:
1969:
1964:
1959:
1957:Talk:Astrology
1954:
1949:
1944:
1939:
1934:
1929:
1927:Stellar corona
1924:
1919:
1914:
1909:
1907:Ibn al-Haytham
1904:
1899:
1894:
1889:
1884:
1879:
1877:Doppler effect
1874:
1869:
1864:
1859:
1854:
1849:
1844:
1839:
1834:
1829:
1824:
1819:
1814:
1809:
1804:
1799:
1794:
1789:
1787:Clyde Tombaugh
1784:
1779:
1774:
1769:
1764:
1759:
1754:
1749:
1744:
1739:
1734:
1729:
1727:Carbon dioxide
1724:
1719:
1714:
1709:
1707:Canes Venatici
1704:
1702:Camelopardalis
1699:
1694:
1689:
1684:
1679:
1674:
1669:
1664:
1659:
1654:
1649:
1644:
1639:
1634:
1629:
1624:
1619:
1614:
1609:
1604:
1599:
1597:Apollo program
1594:
1589:
1584:
1579:
1574:
1569:
1564:
1562:Anders Celsius
1559:
1554:
1549:
1544:
1542:Alpha Centauri
1539:
1534:
1529:
1524:
1519:
1514:
1509:
1504:
1499:
1492:is available.
1485:
1480:
1479:
1475:
1472:DragonFire1024
1471:
1468:
1462:
1457:
1452:
1449:
1448:
1447:larger version
1445:
1441:
1438:
1434:2,224 × 2,212
1432:
1427:
1422:
1419:
1418:
1415:
1411:
1408:
1404:3,864 × 3,864
1402:
1397:
1392:
1389:
1388:
1387:Higher quality
1385:
1381:
1378:
1374:3,864 × 3,864
1372:
1367:
1362:
1359:
1358:
1355:
1351:
1348:
1344:3,864 × 3,864
1342:
1337:
1332:
1328:
1327:
1324:
1321:
1318:
1315:
1312:
1304:
1289:
1283:
1281:
1280:
1279:
1277:
1276:
1272:
1267:
1265:
1264:
1263:
1262:
1256:
1244:
1238:
1236:
1235:
1234:
1232:
1231:
1227:
1222:
1220:
1219:
1218:
1217:
1211:
1199:
1193:
1191:
1190:
1189:
1187:
1186:
1182:
1177:
1175:
1174:
1173:
1172:
1166:
1141:
1140:
1139:
1138:
1137:
1133:
1130:
1128:
1127:
1126:
1124:
1123:
1119:
1114:
1112:
1111:
1110:
1109:
1107:
1103:
1099:
1087:
1082:
1080:
1079:
1078:
1076:
1075:
1071:
1066:
1064:
1063:
1062:
1061:
1059:
1055:
1043:
1040:
1038:
1037:
1036:
1034:
1033:
1029:
1024:
1022:
1021:
1020:
1019:
1017:
1005:
1002:
1000:
999:
998:
996:
995:
991:
986:
984:
983:
982:
981:
979:
967:
962:
960:
959:
958:
956:
950:
945:
943:
942:
941:
939:
938:
934:
929:
927:
924:
923:
922:
921:
919:
915:
911:
897:
889:
881:
873:
870:Krabí mlhovina
865:
857:
849:
841:
840:
837:
834:
801:
800:
792:
789:
781:
780:
771:
758:
757:
754:
753:
750:
749:
725:
724:
569:
568:
545:
544:
530:
528:
506:
503:
500:
499:
490:
485:{{ESA-Hubble}}
445:
433:
432:
414:
411:
407:
406:
397:
396:Other versions
393:
392:
385:
373:
372:
362:
358:
357:
346:
342:
341:
336:
332:
331:
266:
257:
255:
252:
245:
244:
235:selected image
231:
229:
217:
216:
199:
187:
186:
151:
128:
127:
106:
96:
95:
45:
40:
39:
34:
29:
24:
19:
9:
6:
4:
3:
2:
2501:
2490:
2487:
2485:
2482:
2480:
2477:
2476:
2474:
2462:
2459:
2458:
2454:
2451:
2450:
2446:
2443:
2442:
2438:
2435:
2434:
2430:
2427:
2426:
2422:
2420:
2417:
2416:
2412:
2409:
2408:
2405:
2402:
2400:Software used
2399:
2398:
2395:chunky format
2394:
2391:
2390:
2386:
2383:
2382:
2378:
2375:
2374:
2370:
2367:
2366:
2362:
2359:
2358:
2354:
2351:
2350:
2346:
2343:
2342:
2336:
2333:
2330:
2329:
2328:
2325:
2324:
2320:
2317:
2316:
2312:
2309:
2308:
2305:
2302:
2294:
2292:
2283:
2280:
2278:
2275:
2273:
2270:
2268:
2265:
2263:
2260:
2258:
2255:
2253:
2250:
2248:
2245:
2243:
2240:
2238:
2235:
2233:
2230:
2228:
2225:
2223:
2220:
2218:
2215:
2213:
2210:
2208:
2205:
2203:
2200:
2198:
2195:
2193:
2190:
2188:
2185:
2183:
2182:ثلاثي الكربون
2180:
2178:
2175:
2173:
2170:
2168:
2165:
2163:
2160:
2159:
2157:
2153:
2150:
2149:
2147:
2143:
2140:
2139:
2137:
2133:
2130:
2128:
2125:
2124:
2122:
2118:
2115:
2113:
2110:
2108:
2105:
2103:
2100:
2098:
2095:
2093:
2090:
2088:
2085:
2083:
2080:
2078:
2075:
2073:
2070:
2068:
2067:Kompakte ster
2065:
2063:
2060:
2058:
2055:
2053:
2050:
2048:
2045:
2043:
2040:
2038:
2035:
2033:
2030:
2028:
2025:
2023:
2020:
2018:
2015:
2014:
2012:
2011:
2010:
2002:
2000:
1993:
1990:
1988:
1985:
1983:
1980:
1978:
1975:
1973:
1970:
1968:
1965:
1963:
1962:Talk:Big bang
1960:
1958:
1955:
1953:
1952:Talk:Asteroid
1950:
1948:
1945:
1943:
1940:
1938:
1935:
1933:
1930:
1928:
1925:
1923:
1920:
1918:
1915:
1913:
1912:Impact crater
1910:
1908:
1905:
1903:
1900:
1898:
1895:
1893:
1892:Double planet
1890:
1888:
1885:
1883:
1880:
1878:
1875:
1873:
1870:
1868:
1865:
1863:
1860:
1858:
1855:
1853:
1850:
1848:
1845:
1843:
1840:
1838:
1835:
1833:
1830:
1828:
1825:
1823:
1820:
1818:
1815:
1813:
1810:
1808:
1807:Constellation
1805:
1803:
1800:
1798:
1795:
1793:
1790:
1788:
1785:
1783:
1780:
1778:
1775:
1773:
1770:
1768:
1765:
1763:
1760:
1758:
1755:
1753:
1750:
1748:
1745:
1743:
1740:
1738:
1735:
1733:
1730:
1728:
1725:
1723:
1720:
1718:
1715:
1713:
1710:
1708:
1705:
1703:
1700:
1698:
1695:
1693:
1690:
1688:
1685:
1683:
1680:
1678:
1675:
1673:
1670:
1668:
1665:
1663:
1660:
1658:
1655:
1653:
1650:
1648:
1645:
1643:
1640:
1638:
1635:
1633:
1630:
1628:
1625:
1623:
1620:
1618:
1615:
1613:
1610:
1608:
1605:
1603:
1600:
1598:
1595:
1593:
1590:
1588:
1585:
1583:
1580:
1578:
1575:
1573:
1570:
1568:
1565:
1563:
1560:
1558:
1555:
1553:
1550:
1548:
1545:
1543:
1540:
1538:
1535:
1533:
1530:
1528:
1525:
1523:
1520:
1518:
1515:
1513:
1510:
1508:
1505:
1503:
1500:
1498:
1495:
1494:
1493:
1491:
1474:
1469:
1463:
1461:
1458:
1456:
1453:
1451:
1450:
1444:
1439:
1433:
1431:
1428:
1426:
1423:
1421:
1420:
1414:
1409:
1403:
1401:
1398:
1396:
1393:
1391:
1390:
1384:
1379:
1373:
1371:
1368:
1366:
1363:
1361:
1360:
1354:
1349:
1343:
1341:
1338:
1336:
1333:
1330:
1329:
1325:
1322:
1319:
1316:
1313:
1311:
1310:
1308:
1282:
1270:
1266:
1237:
1225:
1221:
1192:
1180:
1176:
1151:
1144:
1129:
1117:
1113:
1085:
1081:
1069:
1065:
1039:
1027:
1023:
1001:
989:
985:
965:
961:
948:
944:
932:
928:
925:
862:ערפילית הסרטן
838:
831:
828:
827:
799:
798:
793:
787:
786:
777:
772:
765:
764:
748:
747:
745:
741:
737:
734:, be sure to
733:
728:
723:
721:
717:
713:
704:
702:
698:
694:
685:
683:
679:
675:
666:
664:
660:
656:
647:
645:
641:
637:
628:
626:
622:
618:
609:
607:
603:
599:
590:
588:
584:
580:
571:
570:
565:
562:
561:
559:
555:
551:
547:
546:
543:
529:
527:
519:
516:
515:
512:
511:
495:
491:
487:
481:
476:
474:
470:
466:
465:
461:
457:
453:
452:
451:public domain
446:
439:
438:
424:Public domain
421:Public domain
419:
418:
405:
401:
398:
394:
390:
386:
382:
377:
374:
370:
366:
363:
359:
355:
351:
347:
343:
333:
328:
324:
319:
311:
305:
301:
300:
294:
286:
282:
277:
272:
267:
260:
241:
237:
236:
230:
227:
223:
222:
214:
210:
206:
205:
200:
197:
193:
192:
184:
180:
176:
172:
168:
167:
166:
160:
156:
152:
149:
145:
144:
139:
124:
117:
116:
111:
107:
100:
99:
93:
84:
83:Original file
75:
71:
67:
63:
59:
55:
49:
44:
38:
35:
33:
30:
28:
25:
23:
20:
18:
15:
2436:Image height
2423:Uncalibrated
2303:
2300:
2288:
2282:مقراب راديوي
2117:Sterevolusie
2097:Hemelliggaam
2008:
1996:
1897:Dyson sphere
1647:Astrobiology
1487:
1352:Hawky.diddiz
1306:
1303:File history
824:
795:
729:
711:
692:
673:
654:
635:
616:
597:
578:
549:
532:
521:
463:
449:
447:
348:HubbleSite:
326:
323:سديم السرطان
317:
308:
303:
297:
292:
283:
279:
270:
233:
202:
163:
162:
123:You can help
113:
81:
22:File history
2460:IIM version
2428:Image width
2419:Color space
2360:Orientation
2207:مطلع مستقيم
2177:تطور النجوم
1872:Diffraction
1852:Declination
1847:Dark matter
1722:Capricornus
1717:Canis Minor
1712:Canis Major
1557:Anaximander
1194:14,508,851
964:Crab Pulsar
947:Crab Nebula
918:Crab Pulsar
914:Crab Nebula
826:Crab Pulsar
788:Annotations
744:nominate it
276:Crab Nebula
262:Description
240:star portal
183:nominate it
2473:Categories
2277:علم الهيئة
2242:راية الأرض
2237:خرزات بيلي
2222:عنقود نجمي
2192:مستعر أعظم
1999:more links
1972:Talk:Comet
1762:Chamaeleon
1747:Carl Sagan
1682:Black hole
1484:File usage
1464:400 × 400
1376:(14.61 MB)
1346:(13.84 MB)
1320:Dimensions
1041:image/jpeg
1026:media type
1016:media type
583:صور مختارة
567:Knowledge
548:This is a
505:Assessment
376:Permission
165:identified
153:This is a
89:image/jpeg
27:File usage
2152:अधिनवतारा
2142:ሠማያዊ አካላት
2082:Krapnewel
2042:Supernova
1992:Talk:Crux
1862:Deuterium
1857:Delphinus
1752:Centaurus
1692:CNO cycle
1657:Astronaut
1652:Astrology
1592:Apollo 13
1587:Apollo 11
1527:Aldebaran
1507:Acetylene
1490:full list
1436:(3.08 MB)
1406:(6.18 MB)
1382:Metrónomo
1317:Thumbnail
1314:Date/Time
1179:data size
1165:data size
988:inception
978:inception
883:Hungarian
790:InfoField
413:Licensing
318:العربية:
271:English:
2439:3,864 px
2431:3,864 px
2321:3,864 px
2313:3,864 px
2297:Metadata
1677:Big Bang
1642:Asteroid
1622:Arcturus
1582:Apollo 1
1116:checksum
1098:checksum
891:Georgian
839:Captions
742:it, and
37:Metadata
2387:300 dpi
2379:300 dpi
2232:الشلياق
2132:4. Juli
2107:SN 1054
1567:Antares
1552:Ammonia
1466:(23 KB)
1442:Stianbh
1412:Tryphon
1331:current
1326:Comment
931:depicts
910:depicts
899:Turkish
843:English
354:release
350:gallery
254:Summary
238:on the
207:on the
85:
2363:Normal
2318:Height
1882:Dorado
1697:Caelum
1687:Boötes
1577:Antlia
1547:Altair
1537:Alioth
1517:Albedo
1284:3,864
1239:3,864
1224:height
1210:height
875:Arabic
859:Hebrew
851:German
736:upload
361:Author
345:Source
304:Hubble
171:upload
2310:Width
2289:View
2267:الظهر
2062:Newel
1997:View
1792:Comet
1757:Cetus
1627:Argon
1532:Algol
1286:pixel
1269:width
1259:pixel
1255:width
1241:pixel
1214:pixel
1150:SHA-1
1106:SHA-1
867:Czech
430:false
427:false
161:have
2202:شهاب
2162:مجرة
2047:Ster
2017:1054
1837:Crux
1607:Apus
1512:Aeon
1323:User
1196:byte
1169:byte
821:3864
818:3864
809:1926
806:1996
738:it,
720:here
716:特色图片
701:here
682:here
663:here
644:here
625:here
606:here
587:here
558:here
488:tag.
458:and
456:NASA
402:and
365:NASA
335:Date
211:for
17:File
2355:RGB
2347:LZW
2247:سمت
2187:فجر
2172:سنة
2167:نجم
740:tag
471:or
460:ESA
369:ESA
179:add
2475::
1146::
815:64
812:52
367:,
352:,
177:,
72:|
68:|
64:|
60:|
56:|
50:.
2463:2
2371:3
2337:8
2334:8
2331:8
746:.
722:.
703:.
684:.
665:.
646:.
627:.
608:.
589:.
560:.
475:.
391:.
383:)
379:(
356:.
242:.
215:.
185:.
125:.
91:)
76:.
Text is available under the Creative Commons Attribution-ShareAlike License. Additional terms may apply.
