M2-9

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Planetary nebula

title: "M2-9" type: doc version: 1 created: 2026-02-28 author: "Wikipedia contributors" status: active scope: public tags: ["planetary-nebulae", "ophiuchus", "articles-containing-video-clips"] description: "Planetary nebula" topic_path: "general/planetary-nebulae" source: "https://en.wikipedia.org/wiki/M2-9" license: "CC BY-SA 4.0" wikipedia_page_id: 0 wikipedia_revision_id: 0

::summary Planetary nebula ::

| image = [[File:The Twin Jet Nebula.jpg|300px]] | caption = M2-9 as taken by the Hubble Space Telescope | name = Minkowski 2-9 (M2-9) | type = Planetary | epoch = J2000 | ra = | dec = | dist_ly = 2,100 ly (650 pc) | appmag_v = 14.7 | size_v = 115 × 18 | constellation = Ophiuchus | radius_ly = 0.7 ly (0.2 pc)Radius = distance × sin(angular size / 2) = 2.1 kly * sin(115 / 2) = 0.6 ly | notes = Bipolar outflow, Bipolar nebula | names = Twin Jet Nebula,

Butterfly Nebula,

PNG 010.8+18.0

PK 010+18.2

Minkowski 2-9, abbreviated M2-9 (also known as Minkowski's Butterfly, Twin Jet Nebula, the Wings of a Butterfly Nebula, or just Butterfly Nebula) is a planetary nebula that was discovered by Rudolph Minkowski in 1947. It is located about 2,100 light-years away from Earth in the direction of the constellation Ophiuchus. This bipolar nebula takes the peculiar form of twin lobes of material that emanate from a central star. Astronomers have dubbed this object as the Twin Jet Nebula because of the jets believed to cause the shape of the lobes. Its form also resembles the wings of a butterfly. The nebula was imaged by the Hubble Space Telescope in the 1990s.

The primary component of the central binary is the hot core of a star that reached the end of its main-sequence life cycle, ejected most of its outer layers and became a red giant, and is now contracting into a white dwarf. It is believed to have been a sun-like star early in its life. The second, smaller star of the binary orbits very closely and may even have been engulfed by the other's expanding stellar atmosphere with the resulting interaction creating the nebula. Astronomers theorize that the gravity of one star pulls some of the gas from the surface of the other and flings it into a thin, dense disk extending into space. As the central binary orbits with a period of about 86 to 120 years, the wind emitting from the binary changes direction with it.

The nebula has inflated dramatically due to a fast stellar wind, blowing out into the surrounding disk and inflating the large, wispy hourglass-shaped wings perpendicular to the disk. These wings produce the butterfly appearance when seen in projection. The outer shell is estimated to be about 1,200 years old .

Notes

References

  • {{Cite APOD | title = M2-9: Wings of a Butterfly Nebula | date = June 12, 2005 | access-date = }}
  • {{Cite APOD | title = Monitoring M2-9 | date = June 18, 2007 | access-date = }}
  • {{Citation | last1 = Hora | first1 = Joseph L. | last2 = Latter | first2 = William B. | title = The near-infrared structure and spectra of the bipolar nebulae M2-9 and AFGL 2688: The role of ultraviolet pumping and shocks in molecular hydrogen excitation | journal = The Astrophysical Journal | date = 1994 | volume = 437 | issue = 1 | pages = 281–295 | doi=10.1086/174995 | bibcode=1994ApJ...437..281H |arxiv = astro-ph/9408011 | s2cid = 119525312 }}
  • {{Citation | last1 = Livio | first1 = Mario | last2 = Soker | first2 = Noam | title = The "Twin Jet" Planetary Nebula M2-9 | journal = The Astrophysical Journal | date = 2001 | volume = 552 | issue = 2 | pages = 685–691 | authorlink = Mario Livio | url = http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2001ApJ...552..685L | arxiv = astro-ph/0010241 |bibcode = 2001ApJ...552..685L |doi = 10.1086/320567 | s2cid = 16212439 }}
  • {{Citation | last = Savage | first = Don | title = Hubble Witnesses the Final Blaze of Glory of Sun-Like Stars | journal = Space Telescope Science Institute | date = December 17, 1997 | url = http://hubblesite.org/newscenter/newsdesk/archive/releases/1997/38/text/
  • {{Citation | last1 = Schwarz | first1 = H. E. | last2 = Aspin | first2 = C. | last3 = Corradi | first3 = R. L. M. | last4 = Reipurth | first4 = B. | title = M 2-9: moving dust in a fast bipolar outflow | journal = Astronomy and Astrophysics | date = 1997 | volume = 319 | pages = 267–273 | url = http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=1997A%26A...319..267S |bibcode = 1997A&A...319..267S }}
  • {{Citation | last = SIMBAD | title = Results for PN M 2-9 | authorlink = SIMBAD | date = December 22, 2006 | publisher = SIMBAD, Centre de Données Astronomiques de Strasbourg | url = http://simbad.u-strasbg.fr/simbad/sim-id?protocol=html&Ident=PN+M2-9

References

  1. {{Harv. SIMBAD. 2006
  2. {{Harv. Schwarz. Aspin. Corradi. Reipurth. 1997
  3. (3 Feb 2011). "A disc inside the bipolar planetary nebula M2-9". EDP Sciences.
  4. (2022). "The symbiotic and bipolar nebula M 2-9: Morphological variability of the collimated ionized wind arising from the core". Publications of the Astronomical Society of Japan.
  5. {{Harv. Nemiroff. Bonnell. 2007

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