January 19, 2025

NGC 7293 – The Helix Nebula in Aquarius

NGC 7293 – The Helix Nebula in Aquarius

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.

M33 – Spiral Galaxy in Triangulum Narrowband

M33 – Spiral Galaxy in Triangulum Narrowband

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)

NGC 7635 – The Bubble Nebula in Cassiopeia

NGC 7635 – The Bubble Nebula in Cassiopeia

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.

NGC 7006 – Globular Cluster in Delphinus

NGC 7006 – Globular Cluster in Delphinus

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.

NGC 869 & 884 – The Double Cluster in Perseus

NGC 869 & 884 – The Double Cluster in Perseus

Telescope: Meade 10” LX850 ACF @ f/8, Orion Atlas EQ-G

Camera: QHY 367c Pro, GSO IR Blocking Filter

Guide scope: Astro-Tech 60mm, ASI120MM Mini, PHD2

Exposure: 76x60sec, gain 2800, offset 50, -10C, saved as Raw16/FITS

Darks: 32x180sec, gain 2800, offset 50, -10C, saved as Raw16/FITS

Flats: 64×0.250sec, tee shirt flats taken at dusk

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

Lensed Sky Quality Meter: 17.9

Stacking: Mean with a 1-sigma clip.

White Balance: Nebulosity Automatic

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

For a long time there was some debate as to whether the two clusters that make up the Double Cluster are actually associated with each other or just happened to appear in the same line of sight with one lying behind the other. It now appears that they are indeed lying next to each other, each about 7,000 light years away and about 100 light years apart. However, there is some evidence that the two clusters are of different ages, so while they may have formed separately from each other, they are now traveling companions.

The Double Cluster is currently rising in the northeast after sunset.

M15 – Globular Cluster in Pegasus

M15 – Globular Cluster in Pegasus

Telescope: Meade 10” LX850 ACF @ f/8, Orion Atlas EQ-G

Camera: QHY 367c Pro, GSO IR Blocking Filter

Guide scope: Astro-Tech 60mm, ASI120MM Mini, PHD2

Exposure: 28x180sec, gain 2800, offset 50, -10C, saved as Raw16/FITS

Darks: 32x180sec, gain 2800, offset 50, -10C, saved as Raw16/FITS

Flats: 64×0.250sec, tee shirt flats taken at dusk

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

Lensed Sky Quality Meter: 18.2

Stacking: Mean with a 1-sigma clip.

White Balance: Nebulosity Automatic

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

M15, a bright, condensed globular cluster in a relatively lonely stretch of sky in Pegasus. It is one of the oldest known globular clusters with an estimated age of 13.2 billion years and the first globular cluster found to have a planetary nebula (Pease 1), one of only four planetary nebula associated with a globular cluster. M15 is also one of the most condensed globular cluster and at some point in the distant past it experienced a core collapse that may have heralded the formation of a black hole in its nucleus.

M15 is currently well placed in the southeast as the sky darkens.

M2 – Globular Cluster in Aquarius

M2 – Globular Cluster in Aquarius

Telescope: Meade 10” LX850 ACF @ f/8, Orion Atlas EQ-G

Camera: QHY 367c Pro, GSO IR Blocking Filter

Guide scope: Astro-Tech 60mm, ASI120MM Mini, PHD2

Exposure: 26x180sec, gain 2800, offset 50, -10C, saved as Raw16/FITS

Darks: 32x180sec, gain 2800, offset 50, -10C, saved as Raw16/FITS

Flats: 64×0.250sec, tee shirt flats taken at dusk

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

Lensed Sky Quality Meter: 18.0

Stacking: Mean with a 1-sigma clip.

White Balance: Nebulosity Automatic

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

M2 is a big, beautiful globular cluster that is well placed in the eastern sky in late summer and early fall. It is an easy target for a small telescope. Under dark skies it can even be glimpsed without a telescope or even binoculars. M2 is about 37,500 light years away and lies beyond the galactic center. Like most globular clusters M2 is an ancient relic of the early universe with an estimated age of about 13 billion years.

M2 is currently well placed in the eastern sky during the early evening.

Jupiter & Io – 9/8/2022 02h30m EDT

Jupiter & Io – 9/8/2022 02h30m EDT

Telescope: Celestron C11 @ f/25, Orion Atlas EQ-G

Camera: ZWO ASI462MC, 2.5x Powermate

Filter: Highpoint Scientific IR Blocking Filter

Seeing: fair, 3/5

Exposure: 5% of 5x(3min @ 2msec), gain 400, saved as RAW8, SER

Histogram: 70%

White Balance: Nebulosity Automatic

Software: SharpCap Pro, AutoStakkert, Registax, Nebulosity, WinJUPOS, Photoshop

This image of Jupiter was taken at 2:30am on the morning of September 8th shortly after Io completed a transit of the planet. I thought that it was neat that this image shows a hint of detail on Io as well as its beautiful color. I still have some data sets sitting on my hard drive that were taken during the transit that I will process as soon as I get a chance.

Jupiter rises in the northeast during the early evening and is high in the south after midnight.

Jupiter – 9/9/2022 01h56m EDT

Jupiter – 9/9/2022 01h56m EDT

Telescope: Celestron C11 @ f/25, Orion Atlas EQ-G

Camera: ZWO ASI462MC, 2.5x Powermate

Filter: Highpoint Scientific IR Filter

Seeing: fair, 3/5

Exposure: 5% of 10x(5min @ 2msec), gain 400, saved as RAW8, SER

Histogram: 70%

White Balance: Nebulosity Automatic

Software: SharpCap Pro, AutoStakkert, Registax, Nebulosity, WinJUPOs, Photoshop

This image of Jupiter was taken shortly before 2am on the morning of September 9th shortly after the Great Red Spot crossed Jupiter’s central meridian. The Great Red Spot continues to slowly shrink and fade, but still makes quite an impression on the southern equatorial belt.

Jupiter rises in the northeast during the early evening and is high in the south after midnight.

Saturn – 9/9/2022 23h15m EDT

Saturn – 9/9/2022 23h15m EDT

Telescope: Celestron C11 @ f/25, Orion Atlas EQ-G

Camera: ZWO ASI462MC, 2.5x Powermate

Filter: Highpoint Scientific IR Filter

Seeing: poor to fair, 2-3/5

Exposure: 5% of 5min @ 15msec, gain 400, saved as RAW8, SER

Histogram: 75%

White Balance: Nebulosity Automatic

Software: SharpCap Pro, AutoStakkert, Registax, Nebulosity, WinJUPOs, Photoshop

It has been quite a while since I have done any extensive planetary imaging, but I’m starting to get the hang of it. I wasn’t planning on imaging Saturn as the seeing wasn’t forecast to be very good, but it was better than I had expected. I wanted to test some camera settings and processing work flow that I am working on and I’m pretty happy with the results. A big part of this is getting comfortable with this fairly old (1994) C11 that I have been working with and it seems to be settling in nicely.

Saturn is well placed in the evening sky rising in the east as the sun set and high in the south by midnight.