Lista mgławic planetarnych
Lista mgławic planetarnych o jasności do 13m spośród około 3000 znanych obecnie w Drodze Mlecznej.
Dane obserwacyjne
Tabela zestawiona według rosnącej rektascensji.
Numer katalogu NGC/IC | Powszechna nazwa | RA (J2000) | Dec (J2000) | Współrzędne galaktyczne | Wielkość gwiazdowa Mgł. Gw. | Rozmiar kątowy | Odległość (w ly) [1] [2] [3] | Gwiazdozbiór |
---|---|---|---|---|---|---|---|---|
NGC 40 | 00h 13,0m | +72° 31’ | 120,0° +9,9° | 10,5m 11,6m | 36” | – 4600 – | Cefeusz | |
NGC 246 | 00h 47,1m | –11° 52’ | 118,9° –74,7° | 8,5m 12,0m | 225” | – – 1600 | Wieloryb | |
NGC 650/1 | Małe Hantle (M76) | 01h 42,3m | +51° 35’ | 130,9° –10,5° | 11,0m 16,3m | 120” | – 2100 – | Perseusz |
IC 289 | 03h 10,3m | +61° 19’ | 138,8° +2,8° | 13,0m 15,9m | 40” | – – – | Kasjopeja | |
NGC 1360 | 03h 33,2m | –25° 52’ | 220,4° –53,9° | 9,5m 11,4m | 380” | 1700 – – | Piec | |
IC 351 | 03h 47,5m | +35° 03’ | 159,1° –15,2° | 12,0m 15,8m | 7” | 39100 14700 – | Perseusz | |
IC 2003 | 03h 56,4m | +33° 53’ | 161,3° –14,9° | 12,0m 15,0m | 8” | – 11700 31800 | Perseusz | |
NGC 1501 | 04h 07,0m | +60° 55’ | 144,6° +6,6° | 12,5m 14,4m | 52” | – – – | Żyrafa | |
NGC 1514 | 04h 09,3m | +30° 47’ | 165,5° –15,3° | 10,5m 9,4m | 120” | – – – | Byk | |
NGC 1535 | 04h 14,3m | –12° 44’ | 206,5° –40,6° | 9,5m 12,2m | 18” | 4900 4200 – | Erydan | |
IC 418 | Mgławica Spirograf | 05h 27,5m | –12° 42’ | 215,2° –24,3° | 10,0m 10,2m | 12” | 5200 3900 – | Zając |
NGC 2022 | 05h 42,1m | +09° 05’ | 196,7° –10,9° | 11,5m 15,0m | 20” | – 10400 – | Orion | |
IC 2149 | 05h 56,4m | +46° 06’ | 166,2° +10,5° | 11,0m 11,6m | 9” | 4600 7200 – | Woźnica | |
IC 2165 | 06h 21,7m | –12° 59’ | 221,3° –12,4° | 12,0m 17,9m | 8” | 8200 14000 – | Wielki Pies | |
NGC 2346 | 07h 09,4m | –00° 48’ | 215,7° +3,6° | 10,5m 11,5m | 55” | – – 3000 | Jednorożec | |
NGC 2371/2 | 07h 25,6m | +29° 29’ | 189,2° +19,9° | 11,5m 14,9m | 50” | – 8500 – | Bliźnięta | |
NGC 2392 | Mgławica Eskimos | 07h 29,1m | +20° 55’ | 197,9° +17,4° | 9,5m 10,5m | 45” | 1800 3000 3800 | Bliźnięta |
NGC 2438 | 07h 41,8m | –14° 44’ | 231,8° +4,1° | 10,5m 17,7m | 70” | – 3200 – | Rufa | |
NGC 2440 | 07h 41,9m | –18° 13’ | 234,8° +2,4° | 10,5m 17,7m | 30” | 8500 3200 5700 | Rufa | |
NGC 2452 | 07h 47,4m | –27° 20’ | 243,4° –1,0° | 12,5m 17,7m | 19” | – 15700 10500 | Rufa | |
IC 2448 | 09h 07,1m | –69° 57’ | 285,8° –15,0° | 11,0m 14,2m | 9” | 10100 9100 – | Kil | |
NGC 2792 | 09h 12,4m | –42° 26’ | 265,8° +4,1° | 12,5m 13,8m | 25” | 10100 11400 8200 | Żagiel | |
NGC 2818 | 09h 16,0m | –36° 38 | 262,0° +8,6° | 12,5m 19,4m | 40” | – 8500 – | Kompas | |
NGC 2867 | 09h 21,4m | –58° 19’ | 278,2° –5,9° | 9,5m 16,6m | 15” | – 12400 6200 | Kil | |
NGC 2899 | 09h 27,1m | –56° 06’ | 277,2° –3,8° | 12,0m 15,9m | 90” | – 6500 – | Żagiel | |
IC 2501 | 09h 38,8m | –60° 06’ | 281,0° –5,7° | 11,0m 14,5m | 2” | 19200 – – | Kil | |
NGC 3132 | Mgł. Pierścień Poł. | 10h 07,0m | –40° 26’ | 272,1° +12,4° | 8,5m 10,1m | 45” | – 2200 2100 | Żagiel |
IC 2553 | 10h 09,3m | –62° 37’ | 285,5° –5,4° | 11,5m 15,5m | 9” | 1700 13400 – | Kil | |
NGC 3195 | 10h 09,3m | –80° 52’ | 296,6° –20,0° | 11,5m 15,3m | 40” | – – – | Kameleona | |
NGC 3211 | 10h 17,8m | –62° 40’ | 286,3° –4,9° | 11,5m 18,0m | 16” | 12100 5900 9200 | Kil | |
NGC 3242 | Duch Jowisza | 10h 24,8m | –18° 39’ | 261,1° +32,1° | 9,5m 12,3m | 40” | 3600 3900 2900 | Hydra |
IC 2621 | 11h 00,3m | –65° 15’ | 291,6° –4,8° | 11,5m 15,4m | 5” | 15300 8200 15500 | Kil | |
NGC 3587 | Mgł. Sowa (M97) | 11h 14,8m | +55° 01’ | 148,5° +57,1° | 11,0m 16,0m | 190” | – 2200 – | Wielka Niedźwiedzica |
NGC 3699 | 11h 28,0m | –59° 57’ | 292,7° +1,3° | 11,0m ? | 45” | – – – | Centaur | |
NGC 3918 | Niebieska mgł. planet. | 11h 50,3m | –57° 11’ | 294,7° +4,7° | 8,0m ? | 16” | 4900 6800 5000 | Centaur |
NGC 4361 | 12h 24,5m | –18° 47’ | 294,1° +43,6° | 10,5m 13,2m | 100” | 4900 5200 4700 | Kruk | |
IC 3568 | 12h 33,1m | +82° 34’ | 123,7° +34,5° | 11,5m 13,5m | 15” | 8200 11400 – | Żyrafa | |
IC 4191 | 13h 08,8m | –67° 39’ | 304,6° –4,8° | 11,5m 16,4m | 14” | 10800 14400 – | Mucha | |
NGC 5189 | 13h 33,5m | –65° 58’ | 307,2° –3,4° | 10,0m 14,9m | 140” | – 4900 4100 | Mucha | |
NGC 5307 | 13h 51,1m | –51° 12’ | 312,4° +10,6° | 11,5m 14,7m | 13” | 8500 7200 8100 | Centaur | |
NGC 5315 | 13h 54,0m | –66° 31’ | 309,1° –4,4° | 11,5m 14,4m | 6” | – 13700 8400 | Cyrkiel | |
IC 4406 | Mgł. Siatkówka | 14h 22,4m | –44° 09’ | 319,7° +15,7° | 10,5m 17,0m | 30” | – 3000 – | Wilk |
NGC 5873 | 15h 12,8m | –38° 08’ | 331,3° +16,8° | 12,0m 15,5m | 6” | 24500 19900 30000 | Wilk | |
NGC 5882 | 15h 16,8m | –45° 39’ | 327,8° +10,1° | 10,0m 13,4m | 14” | 6200 8800 – | Wilk | |
NGC 5979 | 15h 47,7m | –61° 13’ | 322,6° –5,3° | 12,0m 15,3m | 8” | – – – | Trójkąt Poł. | |
Shapley 1 | Fine Ring Nebula | 15h 51,7m | –51° 31’ | 329,1° +2,0° | 13,0m 14,0m | 72” | – – 4700 | Węgielnica |
NGC 6058 | 16h 04,4m | +40° 41’ | 64,7° +48,3° | 13,0m 13,9m | 26” | – 9100 – | Herkules | |
IC 4593 | Białooki Groszek | 16h 11,7m | +12° 04’ | 25,3° +40,8° | 11,0m 11,2m | 12” | – 6800 – | Herkules |
NGC 6153 | 16h 31,5m | –40° 15’ | 341,9° +5,4° | 11,0m 16,1m | 24” | 5900 6500 5400 | Skorpion | |
NGC 6210 | 16h 44,5m | +23° 48’ | 43,1° +37,8° | 9,0m 12,7m | 16” | 6200 10100 5300 | Herkules | |
IC 4634 | 17h 01,6m | –21° 50’ | 0,4° +12,2° | 11,0m 13,9m | 7” | 14400 16000 16000 | Wężownik | |
NGC 6302 | Mgławica Robak | 17h 13,7m | –37° 06’ | 349,5° +1,1° | 12,0m ? | 45” | 330 1800 – | Skorpion |
NGC 6309 | Mgł. Skrzynka | 17h 14,1m | –12° 55’ | 9,7° +14,8° | 11,0m 14,4m | 14” | 12700 10800 – | Wężownik |
NGC 6326 | 17h 20,8m | –51° 45’ | 338,2° –8,4° | 11,5m 13,5m | 12” | 12700 15700 – | Ołtarz | |
NGC 6337 | 17h 22,3m | –38° 29’ | 349,4° –1,1° | 12,0m 14,9m | 48” | 4900 – – | Skorpion | |
NGC 6369 | Mgł. Mały Duch | 17h 29,3m | –23° 45’ | 2,4° +5,9° | 11,5m 15,9m | 28” | 3000 5500 4900 | Wężownik |
Henize 3-1475 | Zraszacz ogrodowy | 17h 45m 14,19s | -17° 56′ 46,9″ | 18 000 | Strzelec | |||
IC 4663 | 17h 45,5m | –44° 54’ | 346,3° –8,2° | 12,5m 15,2m | 14” | 6500 – – | Skorpion | |
NGC 6445 | 17h 49,3m | –20° 01’ | 8,1° +3,9° | 12,0m 19,0m | 33" | – 3300 7300 | Strzelec | |
NGC 6543 | Mgł. Kocie Oko | 17h 58,6m | +66° 38’ | 96,5° +29,9° | 8,5m 11,1m | 20” | – 5900 – | Smok |
IC 4673 | 18h 03,3m | –27° 06’ | 3,6° –2,4° | 13,0m 17,6m | 16” | 11700 13400 – | Strzelec | |
NGC 6537 | Czerwony Pająk | 18h 05,2m | –19° 51’ | 10,1° +0,7° | 12,0m 18,8m | 6” | – 4200 6900 | Strzelec |
NGC 6565 | 18h 11,9m | –28° 11’ | 3,5° –4,6° | 12,5m 18,5m | 10” | 6200 5900 – | Strzelec | |
NGC 6563 | 18h 12,0m | –33° 52’ | 358,5° –7,3° | 12,5m 18,0m | 45” | 9500 3100 – | Strzelec | |
NGC 6572 | 18h 12,1m | +06° 52’ | 34,6° +11,9° | 8,5m 13,6m | 14” | 9500 7800 – | Wężownik | |
NGC 6567 | 18h 13,8m | –19° 05’ | 11,7° –0,7° | 11,5m 14,4m | 9” | – 9100 4200 | Strzelec | |
IC 4699 | 18h 18,5m | –45° 59’ | 348,0° –13,9° | 12,5m 15,1m | 7” | 20500 – – | Luneta | |
NGC 6629 | 18h 25,7m | –23° 12’ | 9,4° –5,1° | 11,5m 12,9m | 15” | 5900 5500 6400 | Strzelec | |
NGC 6644 | 18h 32,6m | –25° 08’ | 8,4° –7,3° | 11,5m 15,6m | 3” | 10400 21200 9800 | Strzelec | |
IC 4776 | 18h 45,8m | –33° 21’ | 2,1° –13,4° | 11,5m 14,1m | 7” | 20500 – 24000 | Strzelec | |
NGC 6720 | Mgł. Pierścień (M57) | 18h 53,6m | +33° 02’ | 63,2° +14,0° | 9,0m 15,3m | 70” | 1500 1500 – | Lutnia |
NGC 6741 | Phantom Streak | 19h 02,6m | –00° 27’ | 33,8° –2,7° | 11,0m 14,7m | 8” | 2350 16300 4800 | Orzeł |
NGC 6751 | 19h 05,9m | –06° 00’ | 29,2° –5,9° | 12,0m 15,5m | 21” | – 8200 6400 | Orzeł | |
IC 4846 | 19h 16,5m | –09° 03’ | 27,6° –9,7° | 12,5m 15,2m | 3” | 31300 24800 – | Orzeł | |
IC 1297 | 19h 17,4m | –39° 37’ | 358,3° –21,6° | 10,5m 14,2m | 7” | – 7800 – | Korona Poł | |
NGC 6781 | 19h 18,5m | +06° 32’ | 41,8° –3,0° | 12,0m 16,8m | 120” | – 950 5100 | Orzeł | |
NGC 6790 | 19h 22,9m | +01° 31’ | 37,9° –6,3° | 10,5m 13,5m | 5” | 18600 – – | Orzeł | |
NGC 6803 | 19h 31,3m | +10° 03’ | 46,4° –4,1° | 11,5m 15,2m | 6” | – – 5700 | Orzeł | |
NGC 6804 | 19h 31,6m | +09° 14’ | 45,8° –4,6° | 12,0m 14,4m | 35” | – 4900 5000 | Orzeł | |
NGC 6818 | Mgł. Mały Klejnot | 19h 44,0m | –14° 09’ | 25,9° –17,9° | 10,0m 16,9m | 18” | – 8200 7300 | Strzelec |
NGC 6826 | Mgł. Mrugająca | 19h 44,8m | +50° 32’ | 83,6° +12,8° | 9,5m 10,4m | 25” | 3900 5200 – | Łabędź |
NGC 6842 | 19h 55,0m | +29° 17’ | 65,9° +0,6° | 13,0m 16,0m | 48” | – – – | Lisek | |
NGC 6853 | Mgł. Hantle (M27) | 19h 59,6m | +22° 43’ | 60,8° –3,7° | 7,5m 13,9m | 330” | 910 1100 – | Lisek |
NGC 6852 | 20h 00,7m | +01° 44’ | 42,6° –14,5° | 13,0m 17,9m | 28” | – – – | Orzeł | |
NGC 6884 | NGC 6766 | 20h 10,4m | +46° 28’ | 82,1° +7,1° | 12,5m 15,6m | 6” | 17600 12700 – | Łabędź |
NGC 6879 | 20h 10,4m | +16° 55’ | 57,2° –8,9° | 13,0m 14,8m | 5” | – 20500 – | Strzała | |
NGC 6886 | 20h 12,7m | +19° 59’ | 60,1° –7,7° | 12,0m 15,7m | 8” | 23500 22200 – | Strzała | |
NGC 6891 | 20h 15,1m | +12° 42’ | 54,2° –12,1° | 11,0m 12,4m | 12” | 8500 8500 – | Delfin | |
IC 4997 | 20h 20,1m | +16° 44’ | 58,3° –11,0° | 11,5m 14,4m | 2” | 23500 24500 – | Strzała | |
NGC 6905 | Mgł. Niebieski Błysk | 20h 22,4m | +20° 06’ | 61,5° –9,6° | 11,5m 15,7m | 45” | – – – | Delfin |
NGC 7008 | 21h 00,5m | +54° 33’ | 93,4° +5,5° | 12,0m 13,2m | 85” | – – 2900 | Łabędź | |
NGC 7009 | Mgławica Saturn | 21h 04,2m | –11° 22’ | 37,8° –34,6° | 8,0m 12,8m | 28” | 3100 5200 3500 | Wodnik |
NGC 7026 | 21h 06,3m | +47° 51’ | 89,0° +0,4° | 12,0m 14,2m | 12” | – 7200 – | Łabędź | |
NGC 7027 | 21h 07,0m | +42° 14’ | 84,9° –3,5° | 9,0m 16,3m | 14” | – 3200 3400 | Łabędź | |
NGC 7048 | 21h 14,3m | +46° 17’ | 88,8° –1,7° | 11,5m 19,1m | 60” | – – 5600 | Łabędź | |
IC 5117 | 21h 32,5m | +44° 36’ | 89,9° –5,1° | 12,5m 16,7m | 2” | – 19200 – | Łabędź | |
IC 5148/50 | 21h 59,6m | –39° 23’ | 2,7° –52,4° | 12,0m 16,5m | 120” | – – – | Żuraw | |
IC 5217 | 22h 23,9m | +50° 58’ | 100,6° –5,4° | 12,0m 15,5m | 7” | 19600 14700 – | Jaszczurka | |
NGC 7293 | Mgławica Ślimak | 22h 29,6m | –20° 50’ | 36,2° –57,1° | 7,0m 13,5m | 900” | 520 590 700 | Wodnik |
NGC 7354 | 22h 40,3m | +61° 17’ | 107,8° +2,3° | 12,5m 16,2m | 20” | 6800 – – | Cefeusz | |
NGC 7662 | Mgł. Niebieska Kula Śnieżna | 23h 25,9m | +42° 32’ | 106,6° –17,6° | 9,0m 13,2m | 20” | 5200 5500 – | Andromeda |
- [1] Zhang C, (1995), A statistical distance scale for galactic planetary nebulae, Astrophys J Suppl, 98, 659.
- [2] Mal'kov Yu.F, (1997), Distances and physical parameters of Pne, Astron. Zh. 74, 853.
- [3] Bensby T, Lundström I, (2001), The Distance Scale of Planetary Nebulae, Astron and Astrophys, 374, 599.
Zobacz też
Bibliografia
- Richard Powell: Mgławice planetarne. [w:] Atlas Wszechświata [on-line]. [dostęp 2008-11-13]. [zarchiwizowane z tego adresu (2012-08-18)].
Media użyte na tej stronie
This is a mosaic image, one of the largest ever taken by NASA's Hubble Space Telescope, of the Crab Nebula, a six-light-year-wide expanding remnant of a star's supernova explosion. Japanese and Chinese astronomers recorded this violent event in 1054 CE, as did, almost certainly, Native Americans.
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 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.
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 more detailed appearance that yields clues into the spectacular demise of a star, 6,500 light-years away.
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 nebula represents neutral oxygen, green is singly-ionized sulfur, and red indicates doubly-ionized oxygen.