Caption
The California Nebula is seen in its entirety in this image from NASA’s WISE mission, covering over 25 square degrees of sky. In this infrared view, the dust clouds underlying the nebula glimmer in greens and reds. Also known as NGC 1499, it derives its common name from its similarity to the dramatic coastline of the U.S. state of California.
The California Nebula extends 100 light years through space, and it is illuminated by one of the hottest stars visible in the night sky, known as Menkib. Its surface temperature is about 37,000 degrees, and its total energy output is over 300,000 times more than that of our own Sun. It belongs to an association of very hot stars that were born from the California Nebula only a few million years ago.
The stellar winds blowing out from the fast-moving Menkib pile up as they impact interstellar gas and dust to create a shock wave. Known a “bow shock,” as an analogy to the waves that pile up at the bow of a sailing ship, it heats up the ambient dust clouds through which it is passing, seen here in red.
This image uses data from the original cryogenic phase of the WISE mission. Infrared wavelengths of 3.4 & 4.6 microns are displayed in blue and cyan, respectively, and are dominated by the glow of stars. Light with a wavelength of 12 microns is displayed in green and traces the presence of carbon-rich dust known as polycyclic aromatic hydrocarbons (PAHs). The 22 micron light is rendered in red and is dominated by the thermal glow of warm dust.