January 20, 2025

Snow Moon – 10:40pm 2/15/2022 EST

Snow Moon – 10:40pm 2/15/2022 EST

Telescope: 8” Meade Wide Field LX200GPS @ f/6.3 (Native), Baader Mk III MPCC

Camera: ZWO ASI 294MC

Filter: GSO IR Blocking Filter

Exposure: 128×0.001sec, Gain 200, saved as TIFF

Seeing: Fair, 3/5

White Balance: Nebulosity Automatic

Software: SharpCap Pro, Registax, Nebulosity, Photoshop

This image was taken as part of in initial test using a Baader Mk III MPCC with this wide field 8” SCT and the original, uncooled version of the ASI 294MC. I’m configuring this for remote observing, but it is working so well that I’m going to conduct some additional tests to see how well it works for general purpose imaging.

NGC 2392 – The Eskimo Nebula in Gemini

NGC 2392 – The Eskimo Nebula in Gemini

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.

M46 – Open Cluster in Puppis

M46 – Open Cluster in Puppis

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.

First Quarter Moon – 8:30pm 2/8/2022 EST

First Quarter Moon – 8:30pm 2/8/2022 EST

Telescope: 8” Meade Wide Field LX200GPS @ f/6.3 (Native), Altaz mode

Camera: ZWO ASI 294MC

Filter: Orion Imaging Skyglow Filter

Exposure: 128×0.003sec, Gain 200, saved as TIFF

Seeing: Poor, 2/5

White Balance: Nebulosity Automatic

Software: SharpCap Pro, Registax, Nebulosity, Photoshop

This is a quick stack of images that I grabbed of the moon while setting up my gear for an evening of remote observing. This was taken with the original, uncooled version of the ASI 294MC which is a wonderfully simple, lightweight, and effective camera for this type of work.

 

NGC 1535 – Planetary Nebula in Eridanus

NGC 1535 – Planetary Nebula in Eridanus

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: 62x60sec, 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

NGC 1535 is a beautiful bright planetary nebula in Eridanus. It clearly shows a shelled structure very similar to the Eskimo Nebula (NGC 2392). These little planetary nebula make fine visual targets and are among the few deepsky objects that show a beautiful blue color.

NGC 1535 is currently well placed in the south during the early evening.

NGC 869 & 884 – The Double Cluster in Perseus

NGC 869 & 884 – The Double Cluster in Perseus

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: 18.2

Stacking: Mean with a 1-sigma clip.

White Balance: Nebulosity Automatic

Software: Backyard EOS, 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.

I normally crop these images to give a 4:3 aspect ratio, but I left this one as it came out of the camera to show how well the RC8 covers a full frame sensor. The Double Cluster is currently high in the northwest after sunset.

Waxing Gibbous Moon – 6:40pm 2/5/2022 EST

Waxing Gibbous Moon – 6:40pm 2/5/2022 EST

Telescope: 8” Meade Wide Field LX200GPS @ f/6.3 (Native), Altaz mode

Camera: ZWO ASI 294MC

Filter: Orion Imaging Skyglow Filter

Exposure: 64×0.005sec, Gain 200, saved as TIFF

Seeing: Fair, 3/5

White Balance: Nebulosity Automatic

Software: SharpCap Pro, Registax, Nebulosity, Photoshop

This is a quick stack of images that I grabbed of the moon while setting up my gear for an evening of remote observing; my gear outside, me inside. This was taken with the original, uncooled version of the ASI 294MC which is a wonderfully simple, lightweight, and effective camera for this type of work.

NGC 253 – Spiral Galaxy in Sculptor

NGC 253 – Spiral Galaxy in Sculptor

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: 20x120sec, 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: 18.0

Stacking: Mean with a 1-sigma clip.

White Balance: Nebulosity Automatic

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

NGC 253 is a large, beautiful spiral galaxy located in the faint southern constellation of Sculptor. Although it is one of the brightest galaxies in the sky, it is so far south that it is relatively difficult from mid-northern latitudes. From my backyard it never gets much higher than about 25 degrees above the southern horizon where skyglow is always a challenge. On this particular evening the transparency was really bad and I gave this a try just for yucks. I was very surprised that it turned out as well as it did.

NGC 253 is currently low in the southwest at sunset.

M77 – Spiral Galaxy in Cetus

M77 – Spiral Galaxy in Cetus

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: 17x120sec, 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, fair transparency, moonlight

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

M77 is the closest and brightest example of a Seyfert Galaxy. These galaxies are characterized by a bright stellar core and very strong radio emissions. It is now known that these arise from a super massive black hole at the galaxy’s core. At the core of M77 lies a black hole with an estimated mass of 11 million suns. As a radio source M77 is known as Cetus A. M77 lies about 1 degree east of the 4th magnitude star delta Cetus making it fairly easy to locate. Through a telescope the bright core of M77 is easy to spot, but the spiral arms are quite faint.

M77 is currently located in the southern sky during the early evening.

(1) Ceres – Asteroid in Taurus – 11/22/2021, 10:00pm EST

(1) Ceres – Asteroid in Taurus – 11/22/2021, 10:00pm EST

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: 30x60sec, 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, fair transparency, bright moonlight

Lensed Sky Quality Meter: 18.0

Stacking: Mean with a 1-sigma clip.

White Balance: Nebulosity Automatic

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

The short streak in the center of this field shows the apparent motion of (1) Ceres over the period of about 30 minutes on the evening of November 22, 2021, at 10:00pm local time. Ceres was the first asteroid discovered as part of a methodical search for a ‘missing’ planet between the orbits of Mars and Jupiter that began in 1800. Giuseppe Piazzi, from Palermo, Sicily, discovered Ceres on January 1, 1801, and it just happens to be the largest and most massive asteroid in the solar system. Ceres is 590 mile in diameter and was 164 million miles away shining at magnitude 7.1 in Taurus crossing the Hyades star cluster when this image was taken.

Ceres is still in Taurus, but has since moved off to the west and now lies south of the Pleiades star cluster. Although it is currently 203 million miles away it is still relatively bright at magnitude 8.2 and is an easy target for binoculars or small telescope.