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 nazwaRA (J2000)Dec (J2000)Współrzędne
galaktyczne
Wielkość gwiazdowa
Mgł. Gw.
Rozmiar kątowyOdległość
(w ly)
[1] [2] [3]
Gwiazdozbiór
NGC 4000h 13,0m+72° 31’120,0° +9,9°10,5m 11,6m36”– 4600 –Cefeusz
NGC 24600h 47,1m–11° 52’118,9° –74,7°8,5m 12,0m225”– – 1600Wieloryb
NGC 650/1Małe Hantle (M76)01h 42,3m+51° 35’130,9° –10,5°11,0m 16,3m120”– 2100 –Perseusz
IC 28903h 10,3m+61° 19’138,8° +2,8°13,0m 15,9m40”– – –Kasjopeja
NGC 136003h 33,2m–25° 52’220,4° –53,9°9,5m 11,4m380”1700 – –Piec
IC 35103h 47,5m+35° 03’159,1° –15,2°12,0m 15,8m7”39100 14700 –Perseusz
IC 200303h 56,4m+33° 53’161,3° –14,9°12,0m 15,0m8”– 11700 31800Perseusz
NGC 150104h 07,0m+60° 55’144,6° +6,6°12,5m 14,4m52”– – –Żyrafa
NGC 151404h 09,3m+30° 47’165,5° –15,3°10,5m 9,4m120”– – –Byk
NGC 153504h 14,3m–12° 44’206,5° –40,6°9,5m 12,2m18”4900 4200 –Erydan
IC 418Mgławica Spirograf05h 27,5m–12° 42’215,2° –24,3°10,0m 10,2m12”5200 3900 –Zając
NGC 202205h 42,1m+09° 05’196,7° –10,9°11,5m 15,0m20”– 10400 –Orion
IC 214905h 56,4m+46° 06’166,2° +10,5°11,0m 11,6m9”4600 7200 –Woźnica
IC 216506h 21,7m–12° 59’221,3° –12,4°12,0m 17,9m8”8200 14000 –Wielki Pies
NGC 234607h 09,4m–00° 48’215,7° +3,6°10,5m 11,5m55”– – 3000Jednorożec
NGC 2371/207h 25,6m+29° 29’189,2° +19,9°11,5m 14,9m50”– 8500 –Bliźnięta
NGC 2392Mgławica Eskimos07h 29,1m+20° 55’197,9° +17,4°9,5m 10,5m45”1800 3000 3800Bliźnięta
NGC 243807h 41,8m–14° 44’231,8° +4,1°10,5m 17,7m70”– 3200 –Rufa
NGC 244007h 41,9m–18° 13’234,8° +2,4°10,5m 17,7m30”8500 3200 5700Rufa
NGC 245207h 47,4m–27° 20’243,4° –1,0°12,5m 17,7m19”– 15700 10500Rufa
IC 244809h 07,1m–69° 57’285,8° –15,0°11,0m 14,2m9”10100 9100 –Kil
NGC 279209h 12,4m–42° 26’265,8° +4,1°12,5m 13,8m25”10100 11400 8200Żagiel
NGC 281809h 16,0m–36° 38262,0° +8,6°12,5m 19,4m40”– 8500 –Kompas
NGC 286709h 21,4m–58° 19’278,2° –5,9°9,5m 16,6m15”– 12400 6200Kil
NGC 289909h 27,1m–56° 06’277,2° –3,8°12,0m 15,9m90”– 6500 –Żagiel
IC 250109h 38,8m–60° 06’281,0° –5,7°11,0m 14,5m2”19200 – –Kil
NGC 3132Mgł. Pierścień Poł.10h 07,0m–40° 26’272,1° +12,4°8,5m 10,1m45”– 2200 2100Żagiel
IC 255310h 09,3m–62° 37’285,5° –5,4°11,5m 15,5m9”1700 13400 –Kil
NGC 319510h 09,3m–80° 52’296,6° –20,0°11,5m 15,3m40”– – –Kameleona
NGC 321110h 17,8m–62° 40’286,3° –4,9°11,5m 18,0m16”12100 5900 9200Kil
NGC 3242Duch Jowisza10h 24,8m–18° 39’261,1° +32,1°9,5m 12,3m40”3600 3900 2900Hydra
IC 262111h 00,3m–65° 15’291,6° –4,8°11,5m 15,4m5”15300 8200 15500Kil
NGC 3587Mgł. Sowa (M97)11h 14,8m+55° 01’148,5° +57,1°11,0m 16,0m190”– 2200 –Wielka Niedźwiedzica
NGC 369911h 28,0m–59° 57’292,7° +1,3°11,0m  ?45”– – –Centaur
NGC 3918Niebieska mgł. planet.11h 50,3m–57° 11’294,7° +4,7°8,0m  ?16”4900 6800 5000Centaur
NGC 436112h 24,5m–18° 47’294,1° +43,6°10,5m 13,2m100”4900 5200 4700Kruk
IC 356812h 33,1m+82° 34’123,7° +34,5°11,5m 13,5m15”8200 11400 –Żyrafa
IC 419113h 08,8m–67° 39’304,6° –4,8°11,5m 16,4m14”10800 14400 –Mucha
NGC 518913h 33,5m–65° 58’307,2° –3,4°10,0m 14,9m140”– 4900 4100Mucha
NGC 530713h 51,1m–51° 12’312,4° +10,6°11,5m 14,7m13”8500 7200 8100Centaur
NGC 531513h 54,0m–66° 31’309,1° –4,4°11,5m 14,4m6”– 13700 8400Cyrkiel
IC 4406Mgł. Siatkówka14h 22,4m–44° 09’319,7° +15,7°10,5m 17,0m30”– 3000 –Wilk
NGC 587315h 12,8m–38° 08’331,3° +16,8°12,0m 15,5m6”24500 19900 30000Wilk
NGC 588215h 16,8m–45° 39’327,8° +10,1°10,0m 13,4m14”6200 8800 –Wilk
NGC 597915h 47,7m–61° 13’322,6° –5,3°12,0m 15,3m8”– – –Trójkąt Poł.
Shapley 1Fine Ring Nebula15h 51,7m–51° 31’329,1° +2,0°13,0m 14,0m72”– – 4700Węgielnica
NGC 605816h 04,4m+40° 41’64,7° +48,3°13,0m 13,9m26”– 9100 –Herkules
IC 4593Białooki Groszek16h 11,7m+12° 04’25,3° +40,8°11,0m 11,2m12”– 6800 –Herkules
NGC 615316h 31,5m–40° 15’341,9° +5,4°11,0m 16,1m24”5900 6500 5400Skorpion
NGC 621016h 44,5m+23° 48’43,1° +37,8°9,0m 12,7m16”6200 10100 5300Herkules
IC 463417h 01,6m–21° 50’0,4° +12,2°11,0m 13,9m7”14400 16000 16000Wężownik
NGC 6302Mgławica Robak17h 13,7m–37° 06’349,5° +1,1°12,0m  ?45”330 1800 –Skorpion
NGC 6309Mgł. Skrzynka17h 14,1m–12° 55’9,7° +14,8°11,0m 14,4m14”12700 10800 –Wężownik
NGC 632617h 20,8m–51° 45’338,2° –8,4°11,5m 13,5m12”12700 15700 –Ołtarz
NGC 633717h 22,3m–38° 29’349,4° –1,1°12,0m 14,9m48”4900 – –Skorpion
NGC 6369Mgł. Mały Duch17h 29,3m–23° 45’2,4° +5,9°11,5m 15,9m28”3000 5500 4900Wężownik
Henize 3-1475Zraszacz ogrodowy17h 45m 14,19s-17° 56′ 46,9″18 000Strzelec
IC 466317h 45,5m–44° 54’346,3° –8,2°12,5m 15,2m14”6500 – –Skorpion
NGC 644517h 49,3m–20° 01’8,1° +3,9°12,0m 19,0m33"– 3300 7300Strzelec
NGC 6543Mgł. Kocie Oko17h 58,6m+66° 38’96,5° +29,9°8,5m 11,1m20”– 5900 –Smok
IC 467318h 03,3m–27° 06’3,6° –2,4°13,0m 17,6m16”11700 13400 –Strzelec
NGC 6537Czerwony Pająk18h 05,2m–19° 51’10,1° +0,7°12,0m 18,8m6”– 4200 6900Strzelec
NGC 656518h 11,9m–28° 11’3,5° –4,6°12,5m 18,5m10”6200 5900 –Strzelec
NGC 656318h 12,0m–33° 52’358,5° –7,3°12,5m 18,0m45”9500 3100 –Strzelec
NGC 657218h 12,1m+06° 52’34,6° +11,9°8,5m 13,6m14”9500 7800 –Wężownik
NGC 656718h 13,8m–19° 05’11,7° –0,7°11,5m 14,4m9”– 9100 4200Strzelec
IC 469918h 18,5m–45° 59’348,0° –13,9°12,5m 15,1m7”20500 – –Luneta
NGC 662918h 25,7m–23° 12’9,4° –5,1°11,5m 12,9m15”5900 5500 6400Strzelec
NGC 664418h 32,6m–25° 08’8,4° –7,3°11,5m 15,6m3”10400 21200 9800Strzelec
IC 477618h 45,8m–33° 21’2,1° –13,4°11,5m 14,1m7”20500 – 24000Strzelec
NGC 6720Mgł. Pierścień (M57)18h 53,6m+33° 02’63,2° +14,0°9,0m 15,3m70”1500 1500 –Lutnia
NGC 6741Phantom Streak19h 02,6m–00° 27’33,8° –2,7°11,0m 14,7m8”2350 16300 4800Orzeł
NGC 675119h 05,9m–06° 00’29,2° –5,9°12,0m 15,5m21”– 8200 6400Orzeł
IC 484619h 16,5m–09° 03’27,6° –9,7°12,5m 15,2m3”31300 24800 –Orzeł
IC 129719h 17,4m–39° 37’358,3° –21,6°10,5m 14,2m7”– 7800 –Korona Poł
NGC 678119h 18,5m+06° 32’41,8° –3,0°12,0m 16,8m120”– 950 5100Orzeł
NGC 679019h 22,9m+01° 31’37,9° –6,3°10,5m 13,5m5”18600 – –Orzeł
NGC 680319h 31,3m+10° 03’46,4° –4,1°11,5m 15,2m6”– – 5700Orzeł
NGC 680419h 31,6m+09° 14’45,8° –4,6°12,0m 14,4m35”– 4900 5000Orzeł
NGC 6818Mgł. Mały Klejnot19h 44,0m–14° 09’25,9° –17,9°10,0m 16,9m18”– 8200 7300Strzelec
NGC 6826Mgł. Mrugająca19h 44,8m+50° 32’83,6° +12,8°9,5m 10,4m25”3900 5200 –Łabędź
NGC 684219h 55,0m+29° 17’65,9° +0,6°13,0m 16,0m48”– – –Lisek
NGC 6853Mgł. Hantle (M27)19h 59,6m+22° 43’60,8° –3,7°7,5m 13,9m330”910 1100 –Lisek
NGC 685220h 00,7m+01° 44’42,6° –14,5°13,0m 17,9m28”– – –Orzeł
NGC 6884NGC 676620h 10,4m+46° 28’82,1° +7,1°12,5m 15,6m6”17600 12700 –Łabędź
NGC 687920h 10,4m+16° 55’57,2° –8,9°13,0m 14,8m5”– 20500 –Strzała
NGC 688620h 12,7m+19° 59’60,1° –7,7°12,0m 15,7m8”23500 22200 –Strzała
NGC 689120h 15,1m+12° 42’54,2° –12,1°11,0m 12,4m12”8500 8500 –Delfin
IC 499720h 20,1m+16° 44’58,3° –11,0°11,5m 14,4m2”23500 24500 –Strzała
NGC 6905Mgł. Niebieski Błysk20h 22,4m+20° 06’61,5° –9,6°11,5m 15,7m45”– – –Delfin
NGC 700821h 00,5m+54° 33’93,4° +5,5°12,0m 13,2m85”– – 2900Łabędź
NGC 7009Mgławica Saturn21h 04,2m–11° 22’37,8° –34,6°8,0m 12,8m28”3100 5200 3500Wodnik
NGC 702621h 06,3m+47° 51’89,0° +0,4°12,0m 14,2m12”– 7200 –Łabędź
NGC 702721h 07,0m+42° 14’84,9° –3,5°9,0m 16,3m14”– 3200 3400Łabędź
NGC 704821h 14,3m+46° 17’88,8° –1,7°11,5m 19,1m60”– – 5600Łabędź
IC 511721h 32,5m+44° 36’89,9° –5,1°12,5m 16,7m2”– 19200 –Łabędź
IC 5148/5021h 59,6m–39° 23’2,7° –52,4°12,0m 16,5m120”– – –Żuraw
IC 521722h 23,9m+50° 58’100,6° –5,4°12,0m 15,5m7”19600 14700 –Jaszczurka
NGC 7293Mgławica Ślimak22h 29,6m–20° 50’36,2° –57,1°7,0m 13,5m900”520 590 700Wodnik
NGC 735422h 40,3m+61° 17’107,8° +2,3°12,5m 16,2m20”6800 – –Cefeusz
NGC 7662Mgł. Niebieska Kula Śnieżna23h 25,9m+42° 32’106,6° –17,6°9,0m 13,2m20”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.

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Crab Nebula.jpg
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.