Monitoring M2-9
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.
Monitoring M2-9
Knowledge Talks, Wisdom Listens. 
