<img class=”wp-image-3551 size-large” src=”https://i0.wp.com/www.davelaneastrophotography.com/wp-content/uploads/2018/02/M78-HH-Barnard-Final-1-1-flat.jpg?resize=1024%2C674″ alt=”Horse Head Nebula M78 Barnard’s Loop” width=”1024″ height=”674″ data-wp-pid=”3551″ srcset=”https://i0.wp.com/www.davelaneastrophotography.com/wp-content/uploads/2018/02/M78-HH-Barnard-Final-1-1-flat.jpg?resize=1024%2C674 1024w, https://i0.wp.com/www.davelaneastrophotography.com/wp-content/uploads/2018/02/M78-HH-Barnard-Final-1-1-flat.jpg?resize=300%2C197 300w, https://i0.wp.com/www.davelaneastrophotography.com/wp-content/uploads/2018/02/M78-HH-Barnard-Final-1-1-flat.jpg?resize=768%2C505 768w, https://i0.wp.com/www.davelaneastrophotography.com/wp-content/uploads/2018/02/M78-HH-Barnard-Final-1-1-flat.jpg?resize=1080%2C711 1080w, https://i0.wp.com/www.davelaneastrophotography.com/wp-content/uploads/2018/02/M78-HH-Barnard-Final-1-1-flat.jpg?resize=610%2C401 610w, https://i0.wp.com/www.davelaneastrophotography.com/wp-content/uploads/2018/02/M78-HH-Barnard-Final-1-1-flat.jpg?resize=510%2C336 510w, https://i0.wp.com/www.davelaneastrophotography.com/wp-content/uploads/2018/02/M78-HH-Barnard-Final-1-1-flat.jpg?resize=800%2C527 800w, https://i0.wp.com/www.davelaneastrophotography.com/wp-content/uploads/2018/02/M78-HH-Barnard-Final-1-1-flat.jpg?w=2160 2160w, https://i0.wp.com/www.davelaneastrophotography.com/wp-content/uploads/2018/02/M78-HH-Barnard-Final-1-1-flat.jpg?w=3240 3240w” sizes=”(max-width: 1024px) 100vw, 1024px” data-recalc-dims=”1″ />
Horse Head nebula M78 Barnards Loop
Whats better than Orion in the Winter sky? Nothing that’s what!
Saturday here in Kansas we had a rare clear night with the temperature above 5 degrees F, wind below 40 mph and just a tiny sliver of moon. It was a perfect night to go out and hunt Orion the Hunter!
In this shot, I managed to bag the Horsehead Nebula (right), M78 or Messier 78 (center left blue), and a piece of the large area around Orion called Barnard’s Loop.
There are so many fantastic areas of Hydrogen Alpha Emissions (called Ha) and super bright Nebulas in this region. These are that areas you see as pink in the image. The HA emission is 656 nanometers which a bit above the color red on the light spectrum. Here a bit from Wikipedia on H-Alpha emissions.
H-alpha (Hα) is a specific deep-red visible spectral line in the Balmer series with a wavelength of 656.28 nm; it occurs when a hydrogen electron falls from its third to second lowest energy level. H-alpha light is important to astronomers as it is emitted by many emission nebulae and can be used to observe features in the Sun‘s atmosphere, including solar prominences and the chromosphere.
H-Alpha emissions are typically emitted by dense nebulas which are the star-forming regions of galaxies. Trillions of tons of dust and remnants of supernova explosions gather together like a snowball rolling downhill slowly gathering more and more material until gravity compresses the material to the point it heats to ignition. Then in a massive explosion that jets out leftover material and creates a Herbig-Haro object that is a protostar.
All the pink areas and dark dust areas are stars in evolution, from a clump of dust to the largest star. All represented in a single picture.
Enjoy! Plus check out the cool way to focus at night I created too!
EXIF: 300mm f4.0 122 x 70secs, ISO 4000