Magnitude +11.2 face-on spiral galaxy NGC 6814 lies in the constellation Aquila, 74.4 million light-years from Earth. Click the image for a full-size view. Image credit: ESA/Hubble & NASA. Acknowledgement: Judy Schmidt.Spiral galaxies together with irregular galaxies make up approximately 60 percent of the galaxies in the local Universe. However, despite their prevalence, each spiral galaxy is unique — like snowflakes, no two are alike. This is demonstrated by the striking face-on spiral galaxy NGC 6814, whose luminous nucleus and spectacular sweeping arms, rippled with an intricate pattern of dark dust, are captured in this NASA/ESA Hubble Space Telescope image.
NGC 6814 has an extremely bright nucleus, a telltale sign that the galaxy is a Seyfert galaxy. These galaxies have very active centres that can emit strong bursts of radiation. The luminous heart of NGC 6814 is a highly variable source of X-ray radiation, causing scientists to suspect that it hosts a supermassive black hole with a mass about 18 million times that of the Sun.
As NGC 6814 is a very active galaxy, many regions of ionised gas are studded along its spiral arms. In these large clouds of gas, a burst of star formation has recently taken place, forging the brilliant blue stars that are visible scattered throughout the galaxy.
The ghostly shells of galaxy ESO 381-12 are captured here in a new image from the NASA/ESA Hubble Space Telescope, set against a backdrop of distant galaxies. Some 270 million light-years from Earth in the constellation of Centaurus, ESO 381-12 is categorised as a lenticular galaxy — a hybrid type that shares properties with both spiral and elliptical galaxies.
The Whirlpool Galaxy, also known as M51, is familiar to legions of amateur astronomers as a relatively faint face-on spiral with a smaller companion galaxy, but the Hubble Space Telescope reveals the Whirlpool in all its splendour, a magnificent spiral studded with countless clusters and dust lanes.
The Hubble Space Telescope has spotted the brightest quasar ever seen in the early universe, an active galactic nucleus shining 11 trillion times brighter than the Sun.
