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Дата изменения: Mon Jun 18 17:06:52 2007
Дата индексирования: Sat Dec 29 11:37:07 2007
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Monitoring M2-9
Astronomy Picture of the Day
    


Monitoring M2-9
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Monitoring M2-9
Credit: R. Corradi, M. Santander-Garcia (Isaac Newton Group, IAC), Bruce Balick (U. Washington)
Explanation: Exploring the myriad shapes found in the cosmic zoo of planetary nebulae, some astronomers have focused on the intriguing example of M2-9. About 2,100 light-years away and over one light-year across, M2-9 is known as a twin jet or butterfly nebula in reference to its striking bipolar symmetry. Monitoring M2-9 over many years from ground based telescopes has revealed the dramatic west to east (left to right) progression of features illustrated in this collage. The apparent motion could well be caused by an energetic rotating beam sweeping across the nebular material. Astronomers argue that the beam is collimated by interacting stellar winds in a double star system at the center of M2-9. The binary system of a giant star and hot white dwarf star orbit each other about once every 120 years. Click on the image to watch an animated gif of M2-9.

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Authors & editors: Robert Nemiroff (MTU) & Jerry Bonnell (USRA)
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Based on Astronomy Picture Of the Day

Publications with keywords: butterfly nebula - planetary nebula - binary star
Publications with words: butterfly nebula - planetary nebula - binary star
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