November 26, 2024

M1 – LX850 12” f/8 ACF First-Light

M1 – LX850 12” f/8 ACF First-Light

Telescope: Meade 12” LX850 ACF @ f/8, Orion Atlas EQ-G

Camera: ZWO ASI071 MC Pro, -10C, Gain 200

Filter: Orion Imaging Skyglow Filter

Guide scope: Astro-Tech 60mm, ASI290MM Mini, PHD2

Exposure: (38 + 14)x240sec, saved as FITS

Darks: 32x240s, saved as FITS

Flats: 32x1sec, Tee shirt flats taken at dawn

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

Lensed Sky Quality Meter: 18.3-18.5 mag/arc-sec^2

Stacking: Mean with a 2-sigma clip.

White Balance: Nebulosity Automatic

Software: Nebulosity, Deep Sky Stacker, Photoshop

This is the first-light image taken with my new to me Meade 12” f/8 ACF from LX850 production. The sky conditions were pretty rough with poor transparency, poor seeing, and a bit of a breeze, but I wanted to assess how well my Atlas would carry this scope and how well it would guide. The source images were taken over two consecutive evenings; 38 on the 9th and 14 on the 10th. To keep the weight down I removed the Starlock mount from the telescope and mounted a 50mm Orion mini guider under the Losmandy rail. However, the guiding seemed to be struggling a bit, so I replaced the 50mm mini with an Astrotech 60mm guidescope. I found out later that this whacked the balance of the scope in both RA and dec, but it still guided quite well. Follow-on testing with the telescope properly balanced was excellent. Soooo, although it pushes the Atlas to its limits, this combination seems to work quite well.

M1, the Crab Nebula in Taurus, 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.

Waning Crescent Moon – 12/9/2020, 6h30m EST

Waning Crescent Moon – 12/9/2020, 6h30m EST

Telescope: Meade 12” LX850 ACF @ f/8, Orion Atlas EQ-G

Camera: ZWO ASI071 MC Pro, -10C, Gain 200

Filter: Orion Imaging Skyglow Filter

Exposure: 2x(64×0.015sec), saved as FITS

Seeing: poor, 2/5

White Balance: Nebulosity Automatic

Software: Nebulosity, Registax, Photoshop, Panorama Maker

This is a 2-panel mosaic taken of the waning crescent as dawn brought an end to my first night of imaging with this new to me Meade 12” f/8 LX850 ACF.  The seeing conditions were pretty rough and there was a bit of haze, but I am very happy with the result. Merging the two panels of the mosaic showed that this telescope produces a remarkable flat field providing a uniformly sharp field with almost no distortion. This is a large, fairly heavy telescope that pushes the Atlas to the edge, but it performed brilliantly all night long.

NGC 891 – Edge-on Spiral Galaxy in Andromeda

NGC 891 – Edge-on Spiral Galaxy in Andromeda

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

Camera: ZWO ASI071MC Pro, -10C, Gain 200, Baader Mk III MPCC

Filter: Orion Imaging Skyglow Filter

Guide scope: Astro-Tech 60mm, Meade DSI Pro II, PHD

Exposure: (38+21)x240s, saved as FITS

Darks: 32x240s, saved as FITS

Flats: 32×0.2s, sky flats taken at dusk

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

Lensed Sky Quality Meter: 18.4-18.5 mag/arc-sec^2

Stacking: Mean with a 2-sigma clip.

White Balance: Nebulosity Automatic

Software: Nebulosity, Deep Sky Stacker, Photoshop

This is NGC 891, a fairly large edge-on spiral galaxy in Andromeda. This object is difficult to see visually, but knowing what it shows photographically makes it worth the effort. The dark lane cutting across the galaxy is a band of dust and gas that tends to collect in the plane of spiral galaxy arms. The source images for this field were collected on the evenings of November 6th (38) and the 11th (21).

The Solar Corona from Apollo 11

I have been skimming through the Apollo 11 in Real Time Website and it has been fascinating following all of the chatter between the various mission controllers as well as all of the radio transmissions with the crew. Most of what we usually see and hear are just tiny bits and pieces from the key segments of the mission and it doesn’t capture what it was like to fly the mission. One neat episode that I have not heard before occurs at about Mission Elapsed Time of 71h30m. At this point Apollo 11 is about 11,000 miles from the moon and they enter the moon’s shadow for the first time. The temperature of the spacecraft plummets, though the temperature inside the spacecraft remains stable. Through the windows the crew can see the limb of the moon silhouetted solar corona and the face of the moon is lit by Earthshine. They turn the lights off inside the spacecraft to get a good look at the solar corona and light from the Earthlit moon pours in through the windows. Armstrong also describes being able to clearly see the stars for the first time in the mission.

Very cool.

MVAS Celestron C11 Edge

MVAS Celestron C11 Edge

The club’s C11 Edge HD is now mounted on our new CGX-L mount located in the roll-off roof observatory on the grounds of the John Bryan State Park Observatory and is ready for use by our members. Please contact Qualifcations@MVAS.Org for information.

M97 – The Owl Nebula in Ursa Major

M97 – The Owl Nebula in Ursa Major

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

Camera: ZWO ASI071MC Pro, -10C, Gain 200, Baader Mk III MPCC

Filter: Orion Imaging Skyglow Filter

Guide scope: Astro-Tech 60mm, Meade DSI Pro II, PHD

Exposure: (12+16+36+44)x240s, saved as FITS

Darks: 32x240s, saved as FITS

Flats: 32×0.2s, sky flats taken at dusk

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

Lensed Sky Quality Meter: 18.0-18.4 mag/arc-sec^2

Stacking: Mean with a 2-sigma clip.

White Balance: Nebulosity Automatic

Software: Nebulosity, Deep Sky Stacker, Photoshop

M97 is a wonderful little planetary located just below the bowl of the Big Dipper. It is easy to locate, but a challenge to see from my light polluted backyard. I chose this as the last target from a series of all-night imaging runs starting on the evenings of November 6, 7, 9, and 11. The sky conditions on each of these nights were relatively poor and the source images were pretty rough, but combining a total of 119 images gave a pretty nice result.  If you look closely there are tiny galaxies scattered across the field. For example, to the lower left of the nebula is PGC 34279 (Mv 16.0) and above the nebula are PGC 2490291 (Mv 17.6) and 2490640 (Mv 17.3).

M81 – Spiral Galaxy in Ursa Major

M81 – Spiral Galaxy in Ursa Major

M81 – Spiral Galaxy in Ursa Major – Asro-Tech RC8, ASI294MC Pro

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

Camera: ZWO ASI294MC Pro, 0C, Gain 200

Filter: 2” Orion Imaging Skyglow Filter

Guide scope: Astro-Tech 60mm, Meade DSI Pro II, PHD

Exposure: 52x240sec, saved as FITS

Darks: 32x240s, saved as FITS

Flats: 32×0.25sec, sky flats taken at dusk

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

Lensed Sky Quality Meter: 17.9 mag/arc-sec^2

Stacking: Mean with a 2-sigma clip.

White Balance: Nebulosity Automatic

Software: Nebulosity, Deep Sky Stacker, Photoshop

M81 is a beautiful spiral galaxy that is interacting with the nearby M82. The sky conditions for imaging this delicate galaxy were far from optimal, but it is still neat to see the beautiful sweeping arms tinged with blue star forming regions resulting from a close encounter with M82.

Mars – 11/28/2020, 19h14m EST

Mars – 11/28/2020, 19h14m EST

Telescope: Celestron C9.25 @ f/20, Orion Atlas EQ-G

Camera: ZWO ASI294MC, Gain 300

Filter: Highpoint Scientific IR Filter

Exposure: 10min (73,200×0.008sec), saved as SER

Seeing: fair, 3/5

White Balance: Photoshop & Nebulosity Automatic

Software: Sharpcap Pro, Autostakkert, Nebulosity, Registax, Photoshop This is part of a test sequence taken during an initial evaluation of a new to me Celestron C9.25. There’s a bit of image shift and mirror flop that I need to get sorted (not unusual for a used scope) so I checked the focus and collimation on a nearby star. I used a 1.5x drizzle while stacking and combined the stacked images using 5%, 10%, 25%, and 50% of the source images to smooth out some of the pixilation. A gentle median filter in Photoshop cleaned it up nicely. The “Y” shaped near the eastern limb is the Mariner Valley. To the upper left near the sunrise terminator you can glimpse Olympus Mons as a slightly dark patch and to the lower right of Olympus lying along a diagonal line is the Tharsis Plateau with Arsia, Pavonis, and Ascraeus Mons.

M42/43 – Reflection/Emission Nebula in Orion

M42/43 – Reflection/Emission Nebula in Orion

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

Camera: ZWO ASI071MC Pro, 0C, Gain 200, Baader Mk III MPCC

Filter: Orion Imaging Skyglow Filter

Guide scope: Astro-Tech 60mm, Meade DSI Pro II, PHD

Exposure: 95x90s, saved as FITS

Darks: 32x90s, saved as FITS

Flats: 32×0.2s, sky flats taken at dusk

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

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

Stacking: Mean with a 2-sigma clip.

White Balance: Nebulosity Automatic

Software: Nebulosity, Deep Sky Stacker, Photoshop

This is one of several first-light images taken with my shiny new ASI071MC Pro. The 071 uses an APS-c size chip which makes good use of the relatively flat field of the RC8. It’s neat to compare this camera with the D5300a that I have been using for much of the past year.

M42 is the large section of this nebula while M43 is the smaller, comma shaped section above M42. The red regions of the nebula is light from interstellar hydrogen set aglow by newly formed stars, the smoky blue/gray is starlight reflecting off of interstellar dust, and the dark lanes are veils of dust in the foreground. In this particular image I love the fine detail in the smoky gray rift between M42 and M43.

Visually, M42 appears as a delicate puff of gray smoke about midway along the length of a string of stars that form the Sword of Orion. This line of stars point southwards from the three bright stars that form the distinctive Belt of Orion that is rising in the east as twilight deepens this time of year. The Sword and M42 are easily visible in binoculars or a small telescope. Under dark skies The Great Nebula can even be seen without any optical aid. In a modest telescope the nebula shows some wonderful fine structure in its triangular core that often gets lost in processed images like this one. The core hosts a tiny group of 4 young, relatively bright stars called the Trapezium.

M81 & 82 – Spiral Galaxies in Ursa Major

M81 & 82 – Spiral Galaxies in Ursa Major

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

Camera: ZWO ASI071MC Pro, -10C; Gain: 200

Filter: 2” Orion Imaging Skyglow filter

Guide scope: Williams Optics 50mm, Meade DSI Pro II, PHD

Exposure: 16x240sec saved as FITS

Darks: 32x240sec saved as FITS

Flats: 32x10sec using an LED tracing tablet with 3 layers of muslin

Average Light Pollution: Red zone, fair transparency

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

Stacking: Mean with a 2-sigma clip.

White Balance: Nebulosity Automatic

Software: Nebulosity, Deep Sky Stacker, Photoshop

This is M81 (bottom) and M82 (top), two bright spiral galaxies lying about 12 million light years away in Ursa Major. At present, these two galaxies are about 150,000 light years apart, though a few hundred million years ago the two passed very close to each other. The dark dust lane slashing across M82 is one result of this close encounter with M81 as are the blue star formation regions in M81. If you look to the left of M81 you can just barely glimpse the irregular galaxy UGC 5336. This little ghost is approximately 13 million light years away and is only about 9200 light years across.