Small Magellanic Cloud (click for larger image)
In this high-resolution color image you can see a lot of detail that you cannot see with your eye.
How This Image Was Created
These types of deep sky astro images are not taken with a regular camera but with a highly specialized astro camera directly attached to a powerful telescope. The telescope is located in SE Australia in a remote observatory and is set up to be fully remotely operated from anywhere in the world.
Here are all the technical details for astro buffs:
Telescope: Takahashi FSQ-105ED 106mm F3.6 APO refractor
Camera: QHY-600MThe photographic technique used is called Narrowband Imaging with the Hydrogen Alpha, Sulfur II, and Oxygen III bands, which are wavelengths of light not visible to the naked eye. Therefore they do not correspond to any colors perceived by humans. So the image is false color with an arbitrary mapping chosen for clarity and aesthetic considerations.
The mapping used in the above image is: Halpha -> Green, SII -> Blue, OIII -> Red
A total of 300 separate frames (100 frames for each channel) were combined to create the final image. The total exposure time was over 50 hours!
A total of 300 separate frames (100 frames for each channel) were combined to create the final image. The total exposure time was over 50 hours!
SMC Facts
It has "Cloud" in the name but it's actually a galaxy. SMC is a dwarf irregular galaxy located about 200,000 light-years from
Earth, visible in the southern celestial hemisphere. It’s a satellite galaxy of
the Milky Way, gravitationally bound to it, and spans roughly 7,000 light-years
in diameter. The SMC contains approximately 3 billion stars, significantly fewer
than the Milky Way’s 200-400 billion, and is rich in gas and dust, fostering
active star formation. It’s part of the Local Group of Galaxies, which includes the Milky
Way, the Large Magellanic Cloud (LMC), and the Andromeda Galaxy.


