Light from the Large Magellanic Cloud takes nearly 200,000 years to travel to Earth. And it’s worth the wait. In this image from the NASA/ESA Hubble Space Telescope, a dragon roars out of the cloud, or maybe you see a rearing horse.
Explore the bright pockets of color, dark lanes of dark dust and blazing new stars in this image of LHA 120-N 11, or just simply N11, from the NASA/ESA Hubble Space Telescope.
This region of the Large Magellanic cloud is ablaze with star formation. It is the brightest and most prolific stellar nursery known to scientists. Explore the regions of colorful gas and dark fingers of fine dust. Hydrogen gas glows its characteristic pinkish-red throughout the image providing plenty of fuel for new stars. Massive stars, born from the cloud itself, blast the surrounding nebula with stellar winds and ultraviolet radiation that ionizes the hydrogen gas causing it to glow. Bright pockets of star formation, NGC 1769, in the center, and NGC 1763, to the right in the image, dominate this scene.
Alot of Hubble’s time is spent peering at the star clouds of the Large Magellanic Cloud. The LMC, an irregular dwarf galaxy, is close astronomically speaking. This proximity – less than one-tenth the distance to the Andromeda Galaxy (M31), the closest large spiral galaxy – allows astronomers to study star formation as well as galaxy evolution in detail. It is also relatively clear of the Milky Way’s busy and dusty plane offering a clear view uncluttered by bright foreground stars. LMC shares some features with spiral galaxies, such as a single arm and a clearly visible central bar. Some research indicates that the small galaxy is just passing by, distorted by the gravitational tug of the much larger Milky Way Galaxy.
View more of Hubble’s Hidden Treasures.