January 19, 2025

Saturn – 9/6/2022 22h40m EDT

Saturn – 9/6/2022 22h40m EDT

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

Camera: ZWO ASI462MC, 2.5x Powermate

Filter: Highpoint Scientific IR Filter

Seeing: poor, 2/5

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

Histogram: 70%

White Balance: Nebulosity Automatic

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

This is my first image from the opening of the 2022 planetary imaging season. I still have lots to learn, but I’m off to a good start!

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

Pluto – 8/26 & 8/27/2022 21h 30m EDT

Pluto – 8/26 & 8/27/2022 21h 30m EDT

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

Camera: Canon EOS Ra

Filter: GSO IR Blocking Filter

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

Exposure: 20x120sec, ISO 800, saved as Raw

Darks: Internal (Long Exposure Noise Reduction On)

Flats: 32×1/50sec, Tee shirt flats taken at dusk

Average Light Pollution: Red zone, Bortle 8, fair transparency, light haze

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

This is my annual pilgrimage to the frozen outlands beyond the orbit of Neptune and my homage to Clyde Tombaugh who discovered Pluto on photographic plates taken at the Lowell Observatory in 1930. These two images were taken almost exactly 24 hours apart showing Pluto’s apparent motion against the background stars (marked by red ‘V’ symbols). I say ‘apparent’ as this motion has more to do with the Earth than Pluto. The true motion of the outer planets is from west to east, but in these images Pluto appears to move from east to west (retrograde). This results from our changing perspective as the Earth sweeps past Pluto in its orbit around the sun. Pluto will remain in retrograde motion until October 6th.

When these images were taken Pluto was 3.14 billion miles away shining at Mv 14.4. The sun’s illumination took a little over 4-1/2 hours to reach Pluto and the feeble reflected sunlight took another 4-1/2 hours to make the journey back to the Earth.

Pluto is currently well placed in the southern sky at dusk.

M27 – Planetary Nebula in Vulpecula

M27 – Planetary Nebula in Vulpecula

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

Camera: Canon EOS Ra

Filter: GSO IR Blocking Filter

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

Exposure: 24x120sec, ISO 800, saved as Raw

Darks: Internal (Long Exposure Noise Reduction On)

Flats: 32×1/50sec, Tee shirt flats taken at dusk

Average Light Pollution: Red zone, Bortle 8, fair transparency, light haze

Lensed Sky Quality Meter: 18.7

Stacking: Mean with a 1-sigma clip.

White Balance: Nebulosity Automatic

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

M27, the Dumbbell nebula, is an expanding shell of gas that was ejected from a sun-like star as it exhausted its hydrogen fuel. Swollen into a red giant, the star shed its outer shell while its core collapsed into a white dwarf. Fierce UV radiation from the collapsed core sets the surrounds gas aglow with the blue/green light of doubly ionized oxygen. The diameter of the nebula is about 1 light-year with an estimated age of 9,800 years. Located between Sagitta and Cygnus, M27 is fairly easy to find with a small telescope. Visually, it shows two lobes connected by a neck of nebulosity, giving the nebula its characteristic dumbbell shape.

M27 is currently high in the east after sunset.

M15 – Globular Cluster in Pegasus

M15 – Globular Cluster in Pegasus

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

Camera: Canon EOS Ra

Filter: GSO IR Blocking Filter

Guide scope: Orion 50mm, ASI120MM Mini, PHD2

Exposure: 52x60sec, ISO 800, saved as Raw

Darks: Internal (Long Exposure Noise Reduction On)

Flats: 32x1sec, Tee shirt flats taken at dusk

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

Lensed Sky Quality Meter: 18.6

Stacking: Mean with a 1-sigma clip.

White Balance: Nebulosity Automatic

Software: Backyard EOS, 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. This is supported by the fact the M15 is an x-ray source.

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

M11 – Open Cluster in Scutum

M11 – Open Cluster in Scutum

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

Camera: Canon EOS Ra

Filter: GSO IR Blocking Filter

Guide scope: Orion 50mm, ASI120MM Mini, PHD2

Exposure: 59x30sec, ISO 1600, saved as Raw

Darks: Internal (Long Exposure Noise Reduction On)

Flats: 32x1sec, Tee shirt flats taken at dusk

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

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

M11 is a bright and wonderfully rich open cluster just off the tail of Aquila. It is an easy binocular object that just gets keeps getting better in large telescopes. The cluster lies approximately 6000 light years away and contains an estimated 2900 stars in a volume of space about 20 light years across. The average distance between the stars in the cluster is about 1 light year, making this a very crowded neighborhood!

M11 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: Canon EOS Ra, GSO IR Blocking Filter

Guide scope: Orion 50mm, ASI120MM Mini, PHD2

Exposure: 26x60sec, ISO 800, saved as Raw

Darks: Internal (Long Exposure Noise Reduction On)

Flats: 32x1sec, tee shirt flats taken at dusk

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

Lensed Sky Quality Meter: 18.1

Stacking: Mean with a 1-sigma clip.

White Balance: Nebulosity Automatic

Software: Backyard EOS, 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.

M22 – Meade 10” LX850 ACF First-light, EOS Ra

M22 – Meade 10” LX850 ACF First-light, EOS Ra

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

Camera: Canon EOS Ra, GSO IR Blocking Filter

Guide scope: Orion 50mm, ASI120MM Mini, PHD2

Exposure: 46x30sec, ISO 800, saved as Raw

Darks: Internal (Long Exposure Noise Reduction On)

Flats: 32x1sec, tee shirt flats taken at dusk

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

Lensed Sky Quality Meter: 18.1

Stacking: Mean with a 1-sigma clip.

White Balance: Nebulosity Automatic

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

M22 is one of several gorgeous globular clusters in and near Sagittarius and is one of the gems of the summer sky in the northern hemisphere. With an estimated distance of 10,600 light years it is one of the closer globulars in our galaxy. In many ways M22 should outshine M13, but it can get a bit lost among the stars near the Sagittarius star clouds and its light is dimmed by dust along the galactic plane. Still, it is large, bright, and easily resolves into this beautiful glow of stardust even in a modest telescope. In a large telescope it blossoms into a glorious sight.

M22 is currently well placed in the southern sky during the early evening.

NGC 5694 – Globular Cluster in Hydra

NGC 5694 – Globular Cluster in Hydra

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

Camera: Full Spectrum Modified Nikon D810, Baader Mk III MPCC

Filter: GSO IR Blocking Filter

Guide scope: Astro-Tech 60mm, ZWO ASI120MM mini, PHD2

Exposure: 11x120sec, ISO 200, 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, low altitude

Lensed Sky Quality Meter: 18.0

Stacking: Mean with a 1-sigma clip.

White Balance: Nebulosity Automatic

Software: Backyard Nikon, Nebulosity, Photoshop

NGC 5694 is a tiny globular cluster on the border between Hydra and Libra and it never gets very high above the southern horizon from mid northern latitudes. This little globular is an interesting target for a couple of reasons. First, it is quite distant; 113,000 light years from the sun and 95,000 light years from the galactic center. Second, it is traveling and an amazing speed; 170 miles/second relative to the galactic core. At this speed the cluster is not gravitationally bound to the Milky Way and is on a hyperbolic path that will take it out into intergalactic space. Also, the chemical composition of its stars suggest that it did not originate in the galactic halo, marking NGC 5694 as an intergalactic wanderer making its one and only pass through the Milky Way.

NGC 5694 is currently low in the southwest at dusk.

NGC 7635 – The Bubble Nebula in Cassiopeia

NGC 7635 – The Bubble Nebula in Cassiopeia

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

Camera: QHY 367c Pro, 0C, Baader Mk III MPCC

Filter: GSO IR Blocking Filter

Guide scope: Astro-Tech 60mm, ZWO ASI120MM mini, PHD2

Exposure: 33x300sec, gain 2800, offset 50, saved as FITS, dithered every 2 images

Darks: 32, 0C, gain 2800, offset 50, saved as FITS

Flats: 64x500ms, Tee shirt flats taken at dusk

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

Lensed Sky Quality Meter: 18.6

Stacking: Average, 1 sigma clip

White Balance: Nebulosity Automatic

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

This is NGC 7635 is almost the inverse of a planetary nebula. Planetaries are expanding shells of gas shed from a dying star. The Bubble is formed from the intense radiation a hot blue star pushing out a spherical void in the surrounding gas and setting the hydrogen aglow with a beautiful red color. The Bubble looks like a delicate Christmas ornament on an unimaginable scale.

NGC 7635 rises in the northeast in the early evening and is high overhead at dawn.

M27 – Planetary Nebula in Vulpecula

M27 – Planetary Nebula in Vulpecula

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

Camera: QHY 367c Pro, 0C, Baader Mk III MPCC

Filter: GSO IR Blocking Filter

Guide scope: Astro-Tech 60mm, ZWO ASI120MM mini, PHD2

Exposure: 21x300sec, gain 2800, offset 50, saved as FITS, dithered every 2 images

Darks: 32, 0C, gain 2800, offset 50, saved as FITS

Flats: 64x500ms, Tee shirt flats taken at dusk

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

Lensed Sky Quality Meter: 18.6

Stacking: Average, 1 sigma clip

White Balance: Nebulosity Automatic

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

M27, the Dumbbell nebula, is an expanding shell of gas that was ejected from a sun-like star as it exhausted its hydrogen fuel. Swollen into a red giant, the star shed its outer shell while its core collapsed into a white dwarf. Fierce UV radiation from the collapsed core sets the surrounds gas aglow with the blue/green light of doubly ionized oxygen. The diameter of the nebula is about 1 light-year with an estimated age of 9,800 years. Located between Sagitta and Cygnus, M27 is fairly easy to find with a small telescope. Visually, it shows two lobes connected by a neck of nebulosity, giving the nebula its characteristic dumbbell shape.

It took a couple of nights to get this new camera settled in, but I think that I’m close. There’s a little bit of tweaking to do yet, bit I’m starting to get the results that I was hoping for.

M27 is currently well placed in the northeast in the early evening and is high in the south after midnight.