The cosmic butterfly pictured in this NASA/ESA Hubble Space Telescope image goes by many names. It is called the Twin Jet Nebula as well as answering to the slightly less poetic name of PN M2-9.
The M in this name refers to Rudolph Minkowski, a German-American astronomer who discovered the nebula in 1947. The PN, meanwhile, refers to the fact that M2-9 is a planetary nebula. The glowing and expanding shells of gas clearly visible in this image represent the final stages of life for an old star of low to intermediate mass. The star has not only ejected its outer layers, but the exposed remnant core is now illuminating these layers, resulting in a spectacular light show like the one seen here. However, the Twin Jet Nebula is not just any planetary nebula; it is a bipolar nebula.
The characteristic shape of the wings of the Twin Jet Nebula is most likely caused by the motion of the two central stars around each other. It is believed that a white dwarf orbits its partner star, and thus the ejected gas from the dying star is pulled into two lobes rather than expanding as a uniform sphere. However, astronomers are still debating whether all bipolar nebulae are created by binary stars. Meanwhile the nebula’s wings are still growing, and by measuring their expansion, astronomers have calculated that the nebula was created only 1,200 years ago.
Within the wings, starting from the star system and extending horizontally outward like veins are two faint blue patches. Although these may seem subtle in comparison to the nebula’s rainbow colors, these are actually violent twin jets streaming out into space at speeds in excess of 621,000 mph (1 million km/h). This is a phenomenon that is another consequence of the binary system at the heart of the nebula. These jets slowly change their orientation, precessing across the lobes as they are pulled by the wayward gravity of the binary system.
The two stars at the heart of the nebula circle one another roughly every 100 years. This rotation not only creates the wings of the butterfly and the two jets, but also allows the white dwarf to strip gas from its larger companion, which then forms a large disk of material around the stars, extending out as far as 15 times the orbit of Pluto. Even though this disk is of incredible size, it is much too small to be seen on the image taken by Hubble.