The Milky Way from Cassiopeia to Perseus with the Double Cluster NGC 869 and NGC 844 taking centre stage. The Andromeda Galaxy M31 can be seen top left. |
I hope my regular readers have noticed the over time general improvement in my image processing skills. I put this down to ; lots of practice, a masterclass from Olly Penrice and Professor Ian Morison's articles in the Astro-press.
I'm feeling quite pleased with this image as it clearly show cases the differences in the intensity and colour of stars. It also shows the star clouds of the Milky Way without them appearing overly defined and 'crunchy'
The colour of stars is directly related to their temperature and age. Generally, the bluer the star the hotter and younger the star is. When you look up into the night sky and see stars that appear orange or red to the naked eye, these are old stars that have left or are about to leave the main sequence of hydrogen fusing stars. Generally they have commenced fusing helium and are cooling and increasing in diameter. You can see a number of such stars in the above image. One day in the far future this will be the fate of our local star, the Sun. When this happens "the Earth will literally be toast".
The Milky Way stretches across the night sky and is particularly visible from Europe in the autumn months. Sadly light pollution can seriously diminish the visual grandeur of the Milky Way. The above image was taken from a remote site blessed with wonderfully transparent skies.
From Earth's position in an outer arm of our galaxy we see the Milky Way band of light as an amalgam of the milliuons of stars that are located in the flattened disc of the Milky Way spiral galaxy. The darker parts are not areas where there are less or no stars but instead identify volumes of space where gas and dust dims or extinguishes starlight.
Double Cluster NGC 869 and NGC 844 also known as Caldwell 14 taken from our backyard. |
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