Astrophoto Lab
--- your online source for astronomical & satellite images ---

Clear New View of a Classic Spiral
Home
Welcome!
General Information
Special Galleries
AstroIndex
EarthIndex
Deep Space
Galaxies
Nebulae
Stars, Supernovae
Solar System
Earth from Space
NASA Space Programs
Other Astro Images
Posters
Space Image Gallery
Useful Links
Credits & Useage
Feedback
Signup
Name: Messier 83
Description: Spiral Galaxy
Position: RA 13hr 37m 0.95s Dec -29° 51' 57.07"
Constellation: Hydra
Distance: 15 million light years
Field of view: 13.03 x 13.03 arc-minutes
Orientation:
North is 0.0° left of vertical
Image Credit: ESO/M. Gieles, Ack: Mischa Schirmer
Release Date: May 19, 2010




More M83: G0525  G0825  G0917  G0929  G1020  G1404  G1404(closeup)
Click the image to buy a print
+
—————————————————————————————————————————————————

ABOUT THIS IMAGE:

ESO is releasing a beautiful image of the nearby galaxy Messier 83 taken by the HAWK-I instrument on ESO's Very Large Telescope (VLT) at the Paranal Observatory in Chile. The picture shows the galaxy in infrared light and demonstrates the impressive power of the camera to create one of the sharpest and most detailed pictures of Messier 83 ever taken from the ground.

The galaxy Messier 83 is located about 15 million light-years away in the constellation of Hydra (the Sea Serpent). It spans over 40 000 light-years, only 40 percent the size of the Milky Way, but in many ways is quite similar to our home galaxy, both in its spiral shape and the presence of a bar of stars across its center. Messier 83 is famous among astronomers for its many supernovae: vast explosions that end the lives of some stars. Over the last century, six supernovae have been observed in Messier 83 - a record number that is matched by only one other galaxy. Even without supernovae, Messier 83 is one of the brightest nearby galaxies, visible using just binoculars.

Messier 83 has been observed in the infrared part of the spectrum using HAWK-I [1], a powerful camera on ESO's Very Large Telescope (VLT). When viewed in infrared light most of the obscuring dust that hides much of Messier 83 becomes transparent. The brightly lit gas around hot young stars in the spiral arms is also less prominent in infrared pictures. As a result much more of the structure of the galaxy and the vast hordes of its constituent stars can be seen. This clear view is important for astronomers looking for clusters of young stars, especially those hidden in dusty regions of the galaxy. Studying such star clusters was one of the main scientific goals of these observations. When compared to earlier images, the acute vision of HAWK-I reveals far more stars within the galaxy.

The combination of the huge mirror of the VLT, the large field of view and great sensitivity of the camera, and the superb observing conditions at ESO's Paranal Observatory makes HAWK-I one of the most powerful near-infrared imagers in the world. Astronomers are eagerly queuing up for the chance to use the camera, which began operation in 2007, and to get some of the best ground-based infrared images ever of the night sky.

Notes:
[1] HAWK-I stands for High-Acuity Wide-field K-band Imager.