Telescope: Meade SN10 at f/4, Orion Atlas EQ-G

Camera: Canon EOS Ra

Filter: GSO IR Blocking Filter

Guide scope: Williams Optics 50mm, ASI290MM mini, PHD

Exposure: 115x20sec, ISO 800, saved as RAW

Darks: Internal (Long Exposure Noise Reduction On)

Flats: 32×1/60sec, tee shirt flats taken at dusk

Average Light Pollution: Red zone, poor transparency, bright moonlight

Lensed Sky Quality Meter: 17.7 mag/arc-sec^2

Stacking: Mean with a 1-sigma clip.

White Balance: Nebulosity Automatic

Software: Backyard EOS, Nebulosity, Deep Sky Stacker, Photoshop

M3 is a beautiful example of a globular cluster in a relatively lonely stretch of sky. The cluster is a member of the galactic halo and spends much of its time orbiting well outside the plane of the galaxy. It is presently 33,000 light years away from us, 40,000 light years from the galactic core, and 33,000 light years ‘above’ the galactic plane. Home to about 500,000 stars, M3 is relatively young as globular clusters go with an estimated age of 8 billion years.

M3 currently rises in the northeast during the late evening.

Telescope: Meade SN10 at f/4, Orion Atlas EQ-G

Camera: Canon EOS Ra

Filter: GSO IR Blocking Filter

Guide scope: Williams Optics 50mm, ASI290MM mini, PHD

Exposure: 145x20sec, ISO 800, saved as RAW

Darks: Internal (Long Exposure Noise Reduction On)

Flats: 32×1/60sec, tee shirt flats taken at dusk

Average Light Pollution: Red zone, poor transparency, bright moonlight

Lensed Sky Quality Meter: 18.1 mag/arc-sec^2

Stacking: Mean with a 1-sigma clip.

White Balance: Nebulosity Automatic

Software: Backyard EOS, Nebulosity, Deep Sky Stacker, Photoshop

M51 is a beautiful face-on spiral galaxy in Canes Venatici, just south of Alkaid, the bright star that lies at the eastern end of the Big Dipper. The spiral arm that appears to connect M51 to the nearby companion (NGC 5195) is a bit of an illusion. The companion actually lies behind M51, and if you look closely you can see that the spiral arm is silhouetted against the background galaxy. Modern observations and computer modeling suggest that the companion has made at least two passes through the main disk of M51. During the first, it approached M51 from behind, passed through the face of the galaxy, swung around in an orbit that took it in front, and then back through the disk where it lies now behind M51. These passes set off bursts of star formation that gives the arms of M51 their beautiful blue color.

Under dark skies the spiral structure of M51 shows quite well, but from my light polluted backyard all I can see are the cores of the two galaxies. On this particular evening the conditions were so bad with poor transparency and bright moonlight I ordinarily would not have attempted to image a galaxy, but I needed to get some sleep so I picked a target that I would let me catch a nap. I was surprised at how well it turned out. It’ll be neat to see how well this works when it is actually clear!

M51 currently rises in the northeast during the late evening.

Telescope: GSO 8” f/12 Classical Cassegrain @ f/12, Orion Atlas EQ-G

Camera: Canon EOS Ra, Baader Mk III MPCC

Filter: GSO IR Blocking Filter

Guide scope: Williams Optics 50mm, ASI290MM mini, PHD

Exposure: 22x60sec, ISO 800, saved as RAW

Darks: Internal (Long Exposure Noise Reduction On)

Flats: 32×1/25sec, Tee shirt flats taken at dusk

Average Light Pollution: Red zone, Bortle 8, poor transparency

Lensed Sky Quality Meter: 17.8 mag/arc-sec^2

Stacking: Mean with a 1-sigma clip.

White Balance: Nebulosity Automatic

Software: Backyard EOS, Deep Sky Stacker, Nebulosity, Photoshop

NGC 7662 is a remarkable little planetary nebula in Andromeda. Visually, it appears as a beautiful blue spot, easily visible even in my little ETX-60 as an out of focus star. Photographically, it shows a sharply defined shell with a ring circling the central star. The shell also shows hints of fine detail. The central star itself is rather unusual for a planetary in that it is a variable star that ranges from Mv 12 to 16.

This is the first in a series of images taken to test the performance of the CC8 at f/12 with a full-frame camera. This shows some interesting possibilities as a high-resolution imaging system.

The Blue Snowball is presently in the northwest as the sky darkens.

Telescope: Meade SN10 at f/4, Orion Atlas EQ-G

Camera: Canon EOS Ra

Filter: GSO IR Blocking Filter

Guide scope: Williams Optics 50mm, ASI290MM mini, PHD

Exposure: 58x10sec, ISO 800, saved as RAW

Darks: Internal (Long Exposure Noise Reduction On)

Flats: 32×1/60sec, tee shirt flats taken at dusk

Average Light Pollution: Red zone, poor transparency

Lensed Sky Quality Meter: 18.2 mag/arc-sec^2

Stacking: Mean with a 1-sigma clip.

White Balance: Nebulosity Automatic

Software: Backyard EOS, Nebulosity, Deep Sky Stacker, Photoshop

This field shows the Great Nebula bracketed by NGC 1977 to the north and NGC 1980 to the south, forming the Sword of Orion. This is a wonderful region to explore with binoculars or a small telescope. Visually the nebula shows a soft gray and displays a wealth of fine detail. This is also a very rewarding region to photograph and even short exposures show a range of beautiful colors. The red of the Great Nebula is the emission of hydrogen set aglow by hot young stars within the nebula while the smoky blue/gray of M42 and the soft blue of NGC 1977 is starlight reflecting off of interstellar dust. The dark lanes are veils of dust in the foreground.

This is the first in a series of images taken to evaluate how the SN10 performs with a full-frame camera. It’s not perfect, but not bad either. I forgot how fast the SN10 is, on this particular evening reaching my local skyglow limit in only 20 second and anything longer than 10 seconds saturated the core of M42. Wonderful!

The Sword of Orion is currently well placed in the south as the sky darkens.

Telescope: Astro-Tech 8” f/8 Ritchey-Chretien, Orion Atlas EQ-G

Camera: Canon EOS Ra, Baader Mk III MPCC

Filter: GSO IR blocking filter

Guide scope: Astro-Tech 60mm, Starlight Xpress Super Star, PHD2

Exposure: 32x60sec, ISO 800, saved as RAW

Darks: Internal (Long Exposure Noise Reduction On)

Flats: 32×1/2sec, Tee shirt flats taken at dusk

Average Light Pollution: Red zone, Bortle 8, poor transparency

Lensed Sky Quality Meter: 18.3

Stacking: Mean with a 1-sigma clip.

White Balance: Nebulosity Automatic

Software: Backyard EOS, Deep Sky Stacker, Nebulosity, Photoshop

NGC 1245 is a relatively faint but rich open cluster in central Perseus. It may be a tad faint for small telescopes, but blossoms into a fine patch of stardust in larger telescopes.

NGC 1245 is currently well placed in the evening sky and is high overhead in the as the sky darkens.

Telescope: Astro-Tech 8” f/8 Ritchey-Chretien, Orion Atlas EQ-G

Camera: Canon EOS Ra, Baader Mk III MPCC

Filter: GSO IR blocking filter

Guide scope: Astro-Tech 60mm, Starlight Xpress Super Star, PHD2

Exposure: 28x60sec, ISO 800, saved as RAW

Darks: Internal (Long Exposure Noise Reduction On)

Flats: 32×1/2sec, Tee shirt flats taken at dusk

Average Light Pollution: Red zone, Bortle 8, poor transparency

Lensed Sky Quality Meter: 18.4

Stacking: Mean with a 1-sigma clip.

White Balance: Nebulosity Automatic

Software: Backyard EOS, Deep Sky Stacker, Nebulosity, Photoshop

NGC 2392, Eskimo Nebula, is a wonderful little planetary nebula Gemini. Visually this nebula looks much like its nickname, even in a small telescope. Planetary nebula are formed when a star sheds its outer shell as it nears the end of its life. The core collapses into a fiercely bright white dwarf whose intense radiation sets the expanding shell of gas aglow, often with a beautiful blue/green color. The structure of NGC 2392 shows that it experienced several shedding events.

The Eskimo Nebula is currently well placed in the east during the early evening and a fairly easy target for small telescopes.

Telescope: Astro-Tech 8” f/8 Ritchey-Chretien, Orion Atlas EQ-G

Camera: Canon EOS Ra, Baader Mk III MPCC

Filter: Orion Imaging Skyglow Filter

Guide scope: Astro-Tech 60mm, Starlight Xpress Super Star, PHD2

Exposure: 30x120sec, ISO 800, saved as RAW

Darks: Internal (Long Exposure Noise Reduction On)

Flats: 32×1/125sec, Tee shirt flats taken at dusk

Average Light Pollution: Red zone, Bortle 8, poor transparency

Lensed Sky Quality Meter: 18.4

Stacking: Mean with a 1-sigma clip.

White Balance: Nebulosity Automatic

Software: Backyard EOS, Deep Sky Stacker, Nebulosity, Photoshop

M46 is one of several relatively bright open clusters that grace the evening sky in winter. This cluster also sports a beautiful little planetary nebula (NGC 2438) in the foreground. This little nebula looks quite stunning in a modest size telescope with the rich open cluster in the background. I first found M46 with my homemade 10” f/6.7 Newtonian during a Messier Marathon at JB in 1978. I’ll never forget seeing the little planetary nebula in the foreground, it was so neat!

M46 is currently rising in the east at sunset.