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

Camera: QHY 268c, Mode 0, Gain 30, Offset 30, -10C

Filter: 2” Radian Triad Ultra Hb, OIII, Ha, SII filter

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

Exposure: 41x300sec, saved as RAW16/FITS

Darks: 32×300 sec

Flats: 64×2 sec, tee shirt flats taken at dusk

Average Light Pollution: Red zone, fair transparency

Lensed Sky Quality Meter: 18.6 mag/arc-sec^2

Stacking: Mean with a 1-sigma clip.

White Balance: Nebulosity Automatic

Software: SharpCap Pro, Nebulosity, Deep Sky Stacker, Photoshop

This is M1, the Crab Nebula in Taurus (the Bull). M1 is a supernova remnant; the remains of a star that ended its life in one of the most violent events in nature. This particular supernova erupted in 1054 and the star became so bright that it was visible in broad daylight for 23 days. The resulting nebula is expanding so fast that the motion can be detected in images taken a few years apart. At the heart of the nebula is a pulsar; a neutron star spinning at over 30 revolutions per second!

M1 currently rises in the northeast around 7:30 and is high overhead during the early morning.

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

Camera: QHY 268c, Mode 0, Gain 30, Offset 30, -10C

Filter: 2” Radian Triad Ultra Hb, OIII, Ha, SII filter

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

Exposure: 32x300sec, saved as RAW16/FITS

Darks: 40×300 sec

Flats: 64×2 sec, tee shirt flats taken at dusk

Average Light Pollution: Red zone, fair transparency, moonlight

Lensed Sky Quality Meter: 18.4 mag/arc-sec^2

Stacking: Mean with a 1-sigma clip.

White Balance: Nebulosity Automatic

Software: SharpCap Pro, Nebulosity, Deep Sky Stacker, Photoshop

This is the iconic Horsehead Nebula in Orion. The Horsehead itself is the dark nebula, Barnard 33, silhouetted against the red emission nebula, IC 434. To the left is the blue reflection nebula NGC 2023. To the lower right is the beautiful Sigma Orionis multiple star system. It is interesting to note how the right side of this image shows an abundance of faint background stars while the left does not. This is due to an expanse of interstellar dust forming a veil blocking the light from the distant stars on the left side of this field. This is another excellent example of how well the Radian Triad Ultra cuts through challenging sky conditions. I have never seen the horsehead nebula visually from my backyard even with my 16.5” and I have only glimpsed it from our dark sky site.

IC 434 is located just south of the bright star Alnitak, the easternmost star in Orion’s belt, and rises due east around 11pm and is high in the south during the early morning.

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

Camera: QHY 268c, Mode 0, Gain 30, Offset 30, -10C

Filter: 2” Radian Triad Ultra Hb, OIII, Ha, SII filter

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

Exposure: 19x300sec, saved as RAW16/FITS

Darks: 32×300 sec

Flats: 64×2 sec, tee shirt flats taken at dusk

Average Light Pollution: Red zone, fair transparency

Lensed Sky Quality Meter: 18.3 mag/arc-sec^2

Stacking: Mean with a 1-sigma clip.

White Balance: Nebulosity Automatic

Software: SharpCap Pro, Nebulosity, Deep Sky Stacker, Photoshop

NGC 7293 is one of those wonderful objects that hides in plain sight. It is so large (about half the size of the full moon) that its light is spread out over a large area, making it very difficult to see and all but invisible from my red-zone backyard. This is a good example of how a modern multiband narrowband filter can punch through challenging sky conditions. The Helix appears so large as it is one of the closest planetary nebula with a distant of only 650 light years. It spans a diameter of about 2.5 light years and is relatively young with an age estimated to be about 10,600 years.

NGC 7293 is currently rising in the southwest at dusk.

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

Camera: QHY 268c, Mode 0, Gain 30, Offset 30, -10C

Filter: 2” Radian Triad Ultra Hb, OIII, Ha, SII filter

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

Exposure: 32x300sec, saved as RAW16/FITS

Darks: 32×300 sec

Flats: 64×2 sec, tee shirt flats taken at dusk

Average Light Pollution: Red zone, fair transparency, moonlight

Lensed Sky Quality Meter: 18.5 mag/arc-sec^2

Stacking: Mean with a 1-sigma clip.

White Balance: Nebulosity Automatic

Software: SharpCap Pro, Nebulosity, Deep Sky Stacker, Photoshop

This image shows the giant spiral galaxy M33 as viewed through a Triad Ultra narrowband filter. This filter suppresses the light from broadband sources like stars and reflection nebula while passing the light from narrowband sources such as planetary and emission nebula. In this image the stars of M33 are dimmed while the soft glow of emission nebula are highlighted. These are principally star formation regions sprinkled along the spiral arms. Several of the larger and brighter regions can be seen visually and even have their own NGC and IC numbers such as NGC 604 to the upper left. It’s sooo neat observing deepsky objects within a nearby galaxy!

M33 is currently rising in the southeast at dusk. (Photo credit: John Graham, 10-4-2022)

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

Camera: QHY 268c, Mode 0, Gain 30, Offset 30, -10C

Filter: 2” Radian Triad Ultra Hb, OIII, Ha, SII filter

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

Exposure: 16x300sec, saved as RAW16/FITS

Darks: 32×300 sec

Flats: 64×2 sec, tee shirt flats taken at dusk

Average Light Pollution: Red zone, fair transparency, moonlight

Lensed Sky Quality Meter: 18.4 mag/arc-sec^2

Stacking: Mean with a 1-sigma clip.

White Balance: Nebulosity Automatic

Software: SharpCap Pro, Nebulosity, Deep Sky Stacker, Photoshop

This is NGC 7635, the Bubble Nebula in Cassiopeia, with just a bit of the open cluster M52 in the upper left corner. The Bubble is almost the inverse of a planetary nebula; rather than an expanding shell of gas shed from a dying star, the Bubble is formed from the intense radiation of a hot blue star pushing out a sphere in the surrounding gas, making an empty bubble and setting the hydrogen aglow with a beautiful red color.

NGC 7635 is currently high in the southeast at dusk.

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

Camera: QHY 268c, Mode 0, Gain 30, Offset 30, -10C

Filter: GSO IR Blocking Filter

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

Exposure: 16x180sec, saved as FITS

Darks: 32×180 sec

Flats: 64×1 sec, tee shirt flats taken at dusk

Average Light Pollution: Red zone, good transparency

Lensed Sky Quality Meter: 18.7 mag/arc-sec^2

Stacking: Mean with a 1-sigma clip.

White Balance: Nebulosity Automatic

Software: SharpCap Pro, Nebulosity, Deep Sky Stacker, Photoshop

NGC 7006 is one of two small of two globular clusters in Delphinus, the other being NGC 6934. Although relatively small and faint (Mv 10.6), NGC 7006 is very dense as a class 1 globular. This is one of the farthest globular clusters within easy reach of amateur telescopes; 135,000 light years from us and 127,000 light years from the galactic center. Visually, I’m not sure that I’ve ever resolved this cluster much more than a gray ghost, so it was very rewarding to see it nicely resolved in this image.

NGC 7006 was featured in the October 2015 issue of Sky & Telescope in Ken Hewitt-White’s Going Deep article ‘Small Globular, Tiny Galaxies.’ Many of the galaxies described in this article can be found in this image. Kinda cool.

NGC 7006 is currently high in the southeast at dusk.