View allAll Photos Tagged deepspace

NGC 6063 A non- periodic Coment discovered by the Mount Lemmon Survey in images obtained on 3rd January 2025

Messier 101 (M101), also known as the Pinwheel Galaxy, is a spiral galaxy located in the constellation Ursa Major, the Great Bear. The Pinwheel Galaxy lies at a distance of 20.9 million light-years from Earth. It has the designation NGC 5457 in the New General Catalogue. Technical Info:

15 x 300 sec. Badder UV/IR Cut filter

Gain 200, Offset 50, Binning 1x1

Total 1.25 hours

Explore Scientific 102mm f/7 APO Refractor

Sensor cooled to -25°C on ZWO ASI294MC Pro (Color)

Calibration frames: Bias, Darks, and Flats.

Plate Solve ASTAP via N.I.N.A. 1.11

Image processing Pixinsight 1.8.8 and finished in Photoshop CC 2021

Cygnus Wall.

.....................

Cygnus Wall is the most visible and interesting part of the well-known North America nebula, located 1500 light-years from us, in the constellation Cygnus. The "wall" is actually an area of stellar dust combined with hydrogen ionized by the radiation of young stars and stretches over a length of about 20 light-years, thus being one of the largest and best known stellar "nurseries".

Equipment and settings:

Mount: Skywatcher Eq6r pro

Telescope: Explore Scientific 102ED triplet + 0.75 APM reducer

Camera: ASI 533MM pro

Filter: Astrodon SHO

Total integration: 6h36' ( Ha 43x3min, Sii 40x3min, Oiii 47x3min )

Edit in Pixinsight.

Location: my Bortle 6+ backyard.

Summer Sunset at the Owens Valley Radio Observatory.

Ou4 the Giant Squid Nebula in Ti-colour with 10 hours of added SII and OIII

 

A mysterious, squid-like apparition cataloged as Ou4 ( OIII to blue), and Sh2-129 also known as the Flying Bat Nebula ( Ha to red) located in the constellation Cepheus

  

Imaging telescope: Vixen VSD 100 f/3

Imaging camera: 9.2mp Sony SX814

Mount: Software Bisque Paramount MX

Guiding telescope or lens: Vixen VSD 100 f/3

Filters: Chroma OIII 3nm, Chroma Ha 3nm and Chroma SII 3nm

Dates: Nov.. 3, 2016

Frames: 44x1800" at F3

Integration: 42.0 hours

Avg. Moon age: 1.81 days

Avg. Moon phase: 3.67%

Locations: Home observatory, Valencia, Spain

Photo showing Seven Experiments in Procedural Animation, a work by Karl Sims, in the Ars Electronica Center's Deep Space 8K .

Second image in my short Moon series...

 

This is January's full moon, captured on the evening of the 13th, 2025. I used my 200-500mm Nikkor lens and shot it handheld at 1/125th of a second.

 

For added artistic flare and to give the image more depth, I overlayed a Deep Space filter/layer.

 

Now reach up and touch the moon, traveling into the stars above!

The Spaghetti Nebula is located in the constellations of Auriga and Taurus within the Milky Way and is a supernova remnant from an exploding star. These extremely faint and fine filaments of ionised hydrogen, sulphur and oxygen are all that remains from the explosion approximately 40,000 years ago. It's distance from our solar system is estimated to be 3000 light-years.

 

The size of the nebula is extremely large, approximately 3 degrees, and using my small 81mm telescope, the image almost entirely fills a full frame camera sensor. To capture this image I used over 28 hours of images using 3 narrow band filters for each gas.

 

Technical details:

Location:

Gérgal, Almeria, Spain. Bortle class 4.5

 

Filters used:

Ha: 256 @ 120s 512 min

Oiii: 342 @ 120s 684 min

Sii: 251 @ 120s 502 min

 

Total integration: 28.3 hours

 

Equipment:

Telescope: William Optics GT81 with x0.8 Field Flattener f/5.6 385mm

Image Camera: ZWO ASI 6200MM Pro @ -5 C

Pegasus Astro Falcon rotator

Pegasus Astro Focus Cube

ZWO 7 Position filter wheel

ZWO Filters 7nm Sii, Oiii and Ha

Guide scope: William Optics 50mm Uniguide 200mm f/4

Guide camera: ZWO ASI 192 MM Mini

 

Software:

N.I.N.A, PHD2, Sharpcap Pro, PixInsight, Photoshop, Lightroom and Topaz Denoise.

Dusty Subaru?

I don’t see a dusty old hatchback with bumper stickers floating in space, do you?

Of course not, Subaru is what the Japanese call the Pleiades. It means coming together or clustering, which is exactly what this star cluster is all about.

 

And all the left over dust from the formation of the stars is still floating around, being blown about by the stellar winds.

I was pleased to see that even with my crappy star tracker and vintage 300mm lens I could bring out all the dark dirt that is drifting around that open group of stars.

Big thanks to Siril, the astro photography software that I’m still getting to know.

 

Dust, the bane of my mother’s existence! As a fifties house wife she was obsessed with banishing it from our home. I hope she’s resting in peace now, and not floating around with a cosmic Swiffer trying to clean it up. Because as astro photographers we love dust, especially when it is illuminated, right?

 

IOptron Star Tracker Pro

Nikkor 300mm f4.0 at f4.0

Sony A6400

External bulb timer

75 exposures at 60sec each

The obligatory bias, dark and flat frames, 30 frames each

Stacked and processed in Siril, Starnet++

Finished in Photoshop and Lightroom

 

Theme: Cyberpunk, Deepspace, Fantasy, Steampunk Featuring: Accessories, Apparel, Cosmetics, Decor, Hair, Jewelry, Poses, Shoes, Skins, Tattoos Event Opening Date: April 29, 2022 Event Closing Date: May 22, 2022

  

www.seraphimsl.com/?p=208080

SH-2 132 Lion Nebula HOO

 

SH2-132 Lion Nebula has always been an image I wanted to capture and actually look a little like a Lion.

 

Not sure if it made the grade this time but pleased with the colour contrast and details in the Oiii and Ha regions.

 

In this image I made some changes to the editing workflow to leave the colour control and blending to PhotoShop and used PixInsight for the image pre-processing and stacking.

 

A high resolution image with imaging details can be found on my Astrobin page at: astrob.in/4pj3m2/0/

 

Technical summary:

Captured: 8 Nights in August 2024

Location: Turismo Astronómico, Los Coloraos, Gorafe, Spain

Bortle Class: 3

 

Total Integration: 38 hours 20 mins

Filter: Optolong L-Ultimate

Messier 3 (M3 or NGC 5272) is a globular cluster of stars in the northern constellation of Canes Venatici. It was discovered by Charles Messier on May 3, 1764, and resolved into stars by William Herschel around 1784.

 

This cluster is one of the largest and brightest, and is made up of around 500,000 stars. It is estimated to be 8 billion years old. It is located at a distance of about 33,900 light-years away from Earth.

 

A globular cluster is a spherical collection of stars that orbits a galactic core as as satellite. Globular clusters are very tightly bound by gravity, which gives them their spherical shapes and relatively high stellar densities toward their centres.

 

​Details.

M: Mesu 200

T: TMB 152/1200

C: QSI683 Baader LRGB filters

 

30x600s Luminance

30x600s Red

30x600s Green

30x600s Blue

 

Totalling 20 hours.

 

This was all taken as well during the full moon period, as Globular clusters are less affected by moonlight than other Deep Sky objects.

Markarian's Chain is a stretch of galaxies that forms part of the larger Virgo Custer in the constellation of Virgo. The two bright galaxies on the lower section of the chain are M84 and M86 discovered by Charles Messier in 1781. In this field of view approximately 30 identified galaxies are visible making it a spectacular target to image.

 

A combination of 10 nights imaging in January and February 2022 and May 2023 using two different cameras. 2022 images were taken using a mono camera and 4 filters, 2023 images were taken using a colour camera and a single filter.

 

Imaging and processing details can be found on my Astrobin page at: astrob.in/full/zy1fpo/0/

 

Thank you for looking.

 

Technical summary:

Captured: 7,8,29,30,31 Jan 2022, 1,2,3 Feb 2022 and 13,14 May 2023

Imaging Sessions: 10

Location: Gérgal, Andalucía, Spain 2022 and Gorafe, Granada, Spain 2023

Bortle Class: 4 Gergal, 3 Gorafe

 

Total Integration: 23 hours 10 minutes

 

Blue 116x 120s 3hr 52m BIN 1 Gain 100 -5C

Blue 4x 300s 20m BIN 1 Gain 100 -5C

 

Green 123x 120s 4hr 6m BIN 1 Gain 100 -5C

Green 11x 300s 55m BIN 1 Gain 100 -5C

 

Red 149x 120s 4hr 58m BIN 1 Gain 100 -5C

Red 8x 300s 40m BIN 1 Gain 100 -5C

 

UV/IR 142x 120s 4hr 44m BIN 1 Gain 100 -5C

UV/IR 3x 300s 15m BIN1 Gain 100 -5C

 

Moon & Skyglow: 40x 300s 3hr 20m BIN 1 -5C

 

Pixel Scale: 2 arcsec/pixel

 

Telescope: William Optics GT 81 385mm

Imaging Cameras: ZWO ASI6200MM Pro and ZWO ASI2600MC Pro

Guiding: ZWO UniGuide 50mm - ZWO ASI120MM-S

Filters: ZWO R, G, B, UV/IR and Baader Moon & Skyglow

Mount: Skywatcher EQ6-R Pro

Capture Computer: Eagle 4

 

Capture software: NINA, PHD2

Editing software: PixInsight, Adobe Lightroom

 

Intergalactic Crocodile departing for the dusty emission nebula in Auriga.

 

moonrocksastro.com/index.php/2015/12/23/intergalactic-cro...

 

This is a mosaic made up of three panels with an integration of around 35 to 45 hours of exposure.

 

Caldwell 31, a huge, sprawling nebula spanning five light years and surrounding the ‘Flaming Star’, AE Aurigae, the bright star visible in the upper portion of the nebula. AE Aur (mag. +6) is an runaway star that is thought to have been one of three stars ejected from near the Trapezium in Orion 2.7 million years ago. It’s a class-O hydrogen fusing dwarf that is at least 30,000 times more luminous than our Sun. The nebula and the star lie around 1500 light years away.

 

The smaller nebula at the top is IC405, commonly known as the Tadpole Nebula for the small ‘tadpole-like’ structures of dense, cooler gas that are being shaped by the intense radiation from the hot stars of the young open cluster NGC 1893, embedded in the nebulosity. It’s just possible to see the tadpoles to the upper right of the largest dark section at the centre of the nebulosity, with the open cluster just above. IC405 lies 12,000 light years away.

 

Imaging telescopes or lenses: Vixen VSD

Imaging cameras: Starlight Express SXVR-H18

Mounts: Sky-Watcher MX

Guiding telescopes or lenses:Vixen VSD

Guiding cameras: sx loadstar

Software: Sequence Generator Pro, PHD, Photoshop CS5

Filters: Baader Ha, OIII & SII

Accessories: Starlight Xpress USB filter wheel, Baader Planetarium 36mm narrowband filters

  

NGC 2244

Caldwell 49 & 50

========================

OBJECT

Magnitude: +5.50

Distance: 5,500 light years.

Diameter: 128 light years.

Apparent size of object: 80' x 60'

========================

IMAGE

Exposure: 28.7 min.

Sub-frames: 191s x 9.

FOV: 1.57° x 1.06°

Captured: 2021-03-08.

========================

My Flickr Astronomy Album

WR 134 is a variable Wolf-Rayet star located around 6,000 light years away from Earth in the constellation of Cygnus, surrounded by a faint bubble nebula blown by the intense radiation and fast wind from the star. It is just over four times the radius of the sun, but due to a temperature of 63,000 K it is 250,000 times as luminous as the sun. [Wiki]

 

Imaged over 11 nights in July 2024 .

 

A high resolution image with a starless version and full imaging details can be found on my Astrobin page at: astrob.in/0fg4co/0/

Thank you for looking.

 

Technical summary:

Captured: 11 Nights in July 2024

Location: Turismo Astronómico, Los Coloraos, Gorafe, Spain

Bortle Class: 3

 

Total Integration: 46h 50m

Filters: Optolong L-Ultimate Dual Band

Pixel Scale: 1.4 arcsec/pixel

 

Telescope: Skywatcher Esprit 100ED

Image Camera: ZWO ASI2600MC Pro

Mount: Skywatcher EQ 6R Pro

 

Capture software: NINA, PHD2

Editing software: PixInsight, Adobe Lightroom, Adobe Photoshop

IC 405, the Flaming Star Nebula, is an emission and reflection nebula in the constellation Aurig. It is about 1,500 light-years away from Earth.. Technical Info:

15 x 300 sec. Astronomik Ha 12 nm filter

15 x 300 sec. Astronomik OIII 12 nm filter

15 x 300 sec. Astronomik SII 12 nm filter

Gain 200, Offset 50, Binning 1x1

Total Integration 3.8 hours

Explore Scientific 102mm f/7 APO Refractor

Sensor cooled to -25°C on ZWO ASI1600MM Pro (mono)

Calibration frames: Bias, Darks, and Flats.

Plate Solve-Plate Solver 2 via N.I.N.A. 1.11

Image processing Pixinsight 1.8.8, and Photoshop CC 2021

A boney finger of dark nebulas (Barnard 169 to 174) reaches for the light (Ced 199 Sh2-134 and Sh2-135)

 

See on Fluidr

 

OTA: Takahashi FSQ-106 EDX4

GUIDER: Stellarvue F50

MOUNT: Software Bisque Paramount MyT

CAMERA: FLI ML-16070M

GUIDE CAMERA: ZWO ASI 174 Mini M

REDUCER: Takahashi 645 QE .72x f/3.6

SOFTWARE: SGP, PhD2, TheSkyX, Pixinsight, Starnet++, Photoshop

FILTERS: AstrodonLRGB; 5nm Hα, 3nm SII, 3nm OIII

ACCESSORIES: Optec Gemini Focuser/Rotator

LOCATION: SRO

 

To see more of my work and to buy prints visit www.jklovelacephotography.com/pages/space

The Sadr Region (also known as IC 1318 or the Gamma Cygni Nebula) is the diffuse emission nebula surrounding Sadr (γ Cygni) at the center of Cygnus's cross. The Sadr Region is one of the surrounding nebulous regions; others include the Butterfly Nebula and the Crescent Nebula. It contains many dark nebulae in addition to the emission diffuse nebulae.

 

Sadr itself has approximately a magnitude of 2.2. The nebulous regions around the region are also fairly bright.

 

The Crescent Nebula (also known as NGC 6888, Caldwell 27, Sharpless 105) is an emission nebula in the constellation Cygnus, about 5000 light-years away from Earth. It was discovered by William Herschel in 1792. It is formed by the fast stellar wind from the Wolf-Rayet star WR 136 (HD 192163) colliding with and energizing the slower moving wind ejected by the star when it became a red giant around 250,000 to 400,000 years ago. The result of the collision is a shell and two shock waves, one moving outward and one moving inward. The inward moving shock wave heats the stellar wind to X-ray-emitting temperatures.

 

It is a rather faint object located about 2 degrees SW of Sadr. For most telescopes it requires a UHC or OIII filter to see. Under favorable circumstances a telescope as small as 8 cm (with filter) can see its nebulosity. Larger telescopes (20 cm or more) reveal the crescent or a Euro sign shape which makes some to call it the "Euro sign nebula".

 

EQ6R Pro mount

William Optics GT81 iv Scope

Asi2600mc camera cooled to -10c

Optolong L Extreme Filter

ASIAIR Pro

ZWO EAF

ZWO mini guide scope and camera

 

50 x 300 second exposures

30 x darks

30 x dark flats

30 x flats

 

Stacked and processed in Pixinsight

 

Bortle 6 Sky (Kent UK)

This my interpretation of the Hubble Heritage data for

WFC3-Mosaic-of-Carina-Nebula-HH-901-C in narrowband

 

Hope you find this interesting!

 

The original data can be found here if you want to have a go :)

archive.stsci.edu/prepds/carina/

Rho Ophiuchi Cloud Complex

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Located at about 500 light-years from Earth, Rho Ophiuchi is undoubtedly one of the most spectacular and colorful parts of the night sky.

Emission nebulae, reflection nebulae, dark nebulae or star clusters, all can be found in this small part of the sky. There is also a star nursery, practically the closest to Earth, and not to forget Antares (in the yellow area of the attached photo), a giant star, 700 times larger than the Sun, and 10,000 times brighter.

A book could be written about this area, so I will stop here with the description. I hope I will be lucky enough to repeat the experience at the next new moon.

……………………………………………

Equipment and settings:

Mount: Skywatcher Star Adventure GTI

Camera: Nikon D610 – astro modified

Lens : Rokinon 135mm F2

Settings: F 2.8, ISO 1600

Total exposure: 80 minutes (53 exposures x 90 sec)

Calibration frames: 15 darks.

Location: Bortle ¾.

Edit : Pixinsight.

 

Newton 200x1000 sur HEQ5 pro Rowan.

Correcteur Bader MPCC MIII.

Optolong L-Extreme.

Canon 1000Dd.

132 x 3min - ISO 400.

Version HOO.

Ciel Bortle 8

Last night's full moon was very bright with a slight glow around it although it was a case of standing in the cold night air waiting for the clouds to clear long enough to get a hand-held shot but it was worth it.

 

Waning Gibbous Moon

Illumination: 98.9%

Distance to Earth: 362, 205 KM

Time: 23.13

Location: West Wales

 

Taken in black and white hand-held using a Panasonic DMC FZ200

f/2.8

1/1300

108.0 mm

ISO 100

 

Dedicated to CH (ILYWAMHASAM)

 

Newton 200x1000 - HEQ5.

Guidage chercheur + ASI120mc.

123x2min - ISO400.

CANON 1000Dd - Filtre Idas LPS D1 - Correcteur de coma Baader MPCC Mark III.

PixInSight - PS.

Ciel Bortle 8.

Messier 94 is a spiral galaxy in the mid-northern constellation Canes Venatici. Technical Info:

104 x 180 sec. . OPTOLONG L-eNhance filter

97 x 180 sec. ZWO Red filter

93 x 180 sec. ZWO Green filter

86 x 180 sec. Zwo Blue filter

Gain 200, Offset 50, Binning 1x1

Total Integration 19 hours

Explore Scientific 102mm f/7 APO Refractor

Sensor cooled to -15°C on ZWO ASI1600MM Pro (mono)

Calibration frames: Bias, Darks, and Flats.

Plate Solve-PlateSolver 2 via N.I.N.A. 1.11

Image processing Pixinsight 1.8.8-9, and Photoshop CC 2022

On top of Haleakalā - a volcano on the island of Maui - are a handful of deep space telescopes dotting the barren landscape.

The Pleiades also known as the Seven Sisters.

  

Equipment:

Epsilon 130D dual rig

QHY268m + CFW3M

TS2600MP (Touptek IMX571) + ZWO EFW

Astronomik DeepSky RGB

Skywatcher EQ8

 

12x180s red

12x180s green

12x180s blue

84x180s Luminanz

Heart nebula (IC 1805) taken with my mono CMOS astro-camera with narrowband filters and then colored during post-processing with SHO (SII, Ha, OIII) palette. Image data was collected using my ES 102 mm telescope and the field of view (FOV) only covered about 2/3 of the nebula. I am working on new image of this nebula using a mosaic technique to capture the entire nebula. Technical Info:

76 x 300 sec. Astronomik Ha 12 nm filter

82 x 300 sec. Astronomik OIII 12 nm filter

78 x 300 sec Astronomik SII 12 nm filter

81 x 180 sec. OPTOLONG L-eNhance filter

Gain 200, Offset 50, Binning 1x1

Total Integration 26.5 hours

Explore Scientific 102mm f/7 APO Refractor

Sensor cooled to -15°C on ZWO ASI1600MM Pro (mono)

Calibration frames: Bias, Darks, and Flats.

Plate Solve-PlateSolver 2 via N.I.N.A. 1.11

Image processing Deep Sky Stacker 4.2.6, Pixinsight 1.8.8, and Photoshop CC 2021.

Comet C/2022 E3 (ZTF) in the early morning of January 27, 2023.

The comet was discovered in March 2022 at the Zwicky Transient Facility telescope, thus the ZTF name.

  

Equipment:

SkyWatcher EQ6-R

Nikkor 500mm f/4 P AI-S at f/4

Sony a7RIIIa (unmodified)

ZWO 30mm Guide scope

GPCAM2 Mono Camera

 

Acquisition:

Taos, NM: my back yard - Bortle 3

4 x 121" for 8 minutes and 4 seconds of exposure time.

2 dark frames

15 flats frames

15 bias frames

 

Software:

SharpCap

DeepSkyStacker

Photoshop

Lightroom

 

My Sony a7RIII and adapted Nikkor 500mm f/4 P AI-S were mounted on an ADM vixen rail and secured to the SkyWatcher EQ6-R mount. I polar aligned my mount using SharpCap Pro. I struggled with getting guiding going and decided to trust my mount to track accurately. I took 4 121-second exposures and dark, flat, and bias frames. DeepSkyStacker was used to combine all frames, and then I processed the TIFF file in Photoshop. I stretched the 32-bit file using Levels. I then made it a 16-bit file and continued to stretch the file in levels and curves. I used the color sampler tool and levels to do my best to help keep colors accurate. I then used my skillset, including some dodging & burning, and relied on Astronomy Tools Action Set and Topaz Denoise to give the image a polished look. I brought it into Lightroom to do final color corrections and add EXIF data. I did not attempt to account for the comet's movement, and you can see the nucleus is elongated.

I have been waiting for the perfect conditions to take my first deep-space image of the Orion Nebula, and when it happened, the timing overlapped with the Geminid Meteor Shower. The odds of capturing a meteor in the shot are rare, but what was truly shocking was watching a non-geminid meteor (orange streak) that was a brighter fireball and it broke up right on the edge of my shot. Amazing experience to see and capture.

 

I was standing with another skywatcher at the time the brighter one broke into 2 pieces as it burned up in the atmosphere. As soon as it happened he said, "That is where you are shooting!" I just responded with, "I am too scared to see if I actually got it." When I finally got the nerve, I was absolutely stunned.

 

Image taken at Lake Hudson Recreational Area in Lenawee County Michigan. The Geminid Meteor was at 10:40pm on December 13th, the non-Geminid meteor was at 11:29pm. I was shooting the Orion Nebula from about 10:30pm till midnight.

  

(Explore # 129)

 

www.rossellet.com

This star forming region in the constellation Perseus resembles a snail inching its way across the Galaxy.

 

OTA: Takahashi CCA-250

MOUNT: Software Bisque Paramount ME-II w/AOE encoders

CAMERA: FLI PL-16803

REDUCER: Takahashi 645 CA 0.72X (f/3.6)

SOFTWARE: SGP, PhD2, TheSkyX, Pixinsight, Starnet++, Photoshop

FILTERS: Astrodon LRGB; 5nm Hα, SII 3nm, OIII 3nm

ACCESSORIES: FLI CFW 5-7 Filter Wheel

LOCATION: SRO

 

See on Fluidr

 

To see more of my work and to buy prints visit www.jklovelacephotography.com/pages/space

Facebook | Instagram | Moonrocksastro

 

This is the next installment of my 2016 Cygnus exploration. This image has an integration of approximately 25 hours of photography. Featured in this image: SH2-115 an emission nebula. It is approximately 7500 light years away. Also featured are the Planetary Nebula Abell 71 and Weinberger 1-10 in the center left of frame.

An ancient planetary nebula

 

See on Fluidr

 

OTA: PlaneWave CDK20

GUIDER: Astrodon Monster MOAG

MOUNT: PlaneWave L-500

CAMERA: FLI ML-16803

GUIDE CAMERA: QHY 5-III 174 M

REDUCER: N/A

SOFTWARE: SGP, PhD2, PWI 3 & 4, Pixinsight, Starnet++, Photoshop, various plugins

FILTERS: Astrodon NII 3nm, Hα 3nm, OIII 3nm, RGB

ACCESSORIES: Pegasus UPB,

LOCATION: SRO

 

To see more of my work and to buy prints visit www.jklovelacephotography.com/pages/space

NGC 7822

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This is an emission nebula located in the constellation Cepheus, about 3000 light-years from us, being a region where new stars are born. If the strong radiation emitted by the new stars ionizes the surrounding gas and illuminates the entire area, the same radiation erodes those "pillars" of cosmic dust causing, over time, those concentrated areas of dust to disappear and thus destroy the main "material" that forms the new stars.

Equipment and settings:

Mount: Skywatcher Eq6R

Telescope: Explore Scientific 102ED + 0.75 APM reducer

Camera: ASI 533MM

Filter: Astrodon SHO

Total integration: 10 hours ( Ha 38 exposures x 5 min, Sii 44 x 5 min, Oiii 63 x 3 min )

Edit in Pixinsight.

Location: my Bortle 6+ backyard.

Hypothetical exoplanet seen from one of its satellites. The foreground was changed and stars were added to this version.

 

EXOPLANETS

==================================================

Confirmed 3439

Candidates 4696

Solar systems 2569

Earths 348

 

Data from NASA (exoplanets.nasa.gov/)

==================================================

 

"An exoplanet or extrasolar planet is a planet that orbits a star other than the Sun. Starting in 1988, and as of 1 January 2017, there have been 3,557 exoplanets in 2,668 planetary systems and 601 multiple planetary systems confirmed. HARPS (since 2004) has discovered about a hundred exoplanets while the Kepler space telescope (since 2009) has found more than two thousand. Kepler has also detected a few thousand candidate planets, of which about 11% may be false positives. On average, there is at least one planet per star, with a percentage having multiple planets. About 1 in 5 Sun-like stars [a] have an "Earth-sized" [b] planet in the habitable zone. [c] Assuming there are 200 billion stars in the Milky Way, [d] one can hypothesize that there are 11 billion potentially habitable Earth-sized planets in the Milky Way, rising to 40 billion if planets orbiting the numerous red dwarfs are included.

Besides exoplanets, there are also rogue planets, which do not orbit any star and which tend to be considered separately, especially if they are gas giants, in which case they are often counted, like WISE 0855−0714, as sub-brown dwarfs. The rogue planets in the Milky Way possibly number in the billions (or more)." (Text credits: Wikipedia).

A 4 panel mosaic Frames: 120x1800"

Integration: 60.0 hours

 

moonrocksastro.com 

 

This data was acquired with my Takahashi TSA 102. Hope you enjoy it!

 

NGC 2237 Inside the Rosette nebula

 

Imaging telescopes or lenses: Takahashi TSA 102,

Imaging cameras: Starlight Express SXVR-H18

Mounts: Sky-Watcher NEQ6 Pro

Guiding telescopes or lenses: Takahashi TSA 102

Guiding cameras: sx loadstar

Focal reducers: Takahashi TOA/FS Reducer

Software: PHD, Main Sequence Software

Filters: Baader Red 2", Baader SII 8.5nm, Baader B 2", Baader G 2", Baader O III 8.5nm, Baader Ha 8.5nm

Accessories: Starlight Xpress USB filter wheel

M42 & NGC1977 shot with my telephoto lens @ 230mm, F5.6, from my balcony. Bortle class 7-8 area.

Neighbors, but not close neighbours! On a two dimensional image these targets appear in close proximity to one another. In fact they are separated by more than 10,500 light-years.

 

IC 410, the Tadpoles nebula is a faint and dusty emission nebula approximately 12,000 light-years away from Earth in the northern constellation of Auriga.

 

IC 405,also known as the Flaming Star Nebula, is an emission and reflection nebula in the same constellation. IC405 is approximately 1,500 light-years away from Earth.

 

Image captured over 7 nights; 2022-11-19, 22, & 23, and 2023-01-01, 18, 19 & 22

17 hours 10 minutes total integration

Ha subs 23 * 1,200 sec = 7 hours 40 min

OIII subs 10 * 1,200 sec = 3 hours 20 min

SII subs 14 * 1,200 sec = 4 hours 40 min

R subs 15 * 120sec = 30 min

G subs 15 * 120sec = 30 min

B subs 15 * 120sec = 30 min

 

Imaging Equipment:

SharpStar 94EDPH with reducer at 414mm focal length,

Rainbow Astro RST-135,

ZWOASI2600MM Pro camera

SHO 3.0nm filters & RGB filters

About 10,000 years ago, a star exploded and died here. The Helix Nebula, also known as the Helix or NGC 7293, is a large planetary nebula in the constellation Aquarius.

Karl Ludwig Harding, probably discovered it before 1824 and it is one of the closest objects to Earth among the planetary nebulae, about 700 light years from our Earth. Sixteen hours of exposure from El Sauce Observatory in Chile (TelescopeLive) and image processing with my interpretation of 178 raw images in PixInsight and PhotoShop.

www.astrobin.com/2fxjsj/

------------------------------------------------------

 

• Sky-Watcher Quattro 250P

• Sky-Watcher EQ8-R Pro

• ZWO ASI294MM-Pro

 

• ZWO Hα 7nm: 26x600s bin1 gain 200

• ZWO OIII 7nm: 54x600s bin2 gain 200

(total integration 13.3h)

 

• ZWO OAG & ASI290Mini guide cam

• TS GPU coma corrector

• ZWO EFW, ZWO EAF & Pegasus Astro Ultimate Powerbox 2

 

Trevinca, Valding, Spain

Bortle 3, SQM 21.8

 

processed with Pixinsight

Emission Nebula with dark clouds in the Cygnus constellation.

 

Image taken from my backyard in Luxembourg between june 9 and 13.

 

Total exposure about 30 hours.

 

Gear: 203/926mm Newton, ASI1600mmPro camera, Ha/SII/OIII narrowband filters on an EQ8-Pro mount.

M 81 Also known as Bodes Nebula is a spiral galaxy located in Ursa Major. It is a close neighbour to M82 Cigar Galaxy in the same constellation.

M 81 was first discovered by Johann Elert Bode, who found it, along with M 82, in 1774.

M 81 is approximately 12 million light years from our galaxy and spans almost 70,000 light years.

A few hundred million years ago, a close encounter took place between M 81 and M 82, during which M 82 was dramatically deformed.

 

Imaged over 5 nights from my home in Gérgal, Spain.

A higher resolution image with imaging details can be found on my Astrobin page at: astrob.in/full/btwb3x/0/

 

Thank you for looking.

 

Technical summary:

Captured: 21,22,28,30,31-01-2023

Imaging Sessions: 5

Location: Gérgal, Andalucía, Spain

Bortle Class: 4

 

Total Integration: 28h 47m

Filters:

Red 301x 60s 5h 01m BIN 3 Gain 100 -5C SQM 20.6

Green 259x 60s 4h 19m BIN 3 Gain 100 -5C SQM 20.5

Blue 251x 60s 4h 11m BIN 3 Gain 100 -5C SQM 20.7

UV/IR 905x 60s 15h 05m BIN 3 Gain 100 -5C SQM 20.3

Pixel Scale: 0.389 arcsec/pixel

 

Telescope: Celestron C11 Edge HD 2800mm fl

Image Camera: ZWO ASI 6200MM Pro

Guiding: ZWO OAG L with ZWO ASI 192MM Mini

Filters: Astronomik R, G, B, UV/IR

Mount: Skywatcher EQ6R Pro

Computer: Minix NUC

 

Capture software: NINA, PHD2

Processing Software: PixInsight, Adobe Lightroom

Explanation: A bright spiral galaxy of the northern sky, Messier 63 is about 25 million light-years distant in the loyal constellation Canes Venatici. Also cataloged as NGC 5055, the majestic island universe is nearly 100,000 light-years across, about the size of our own Milky Way. Known by the popular moniker, The Sunflower Galaxy, M63 sports a bright yellowish core and sweeping blue spiral arms, streaked with cosmic dust lanes and dotted with pink star forming regions. This deep exposure also reveals an enormous but dim arc extending far into the halo above the brighter galactic plane. A collaboration of professional and amateur astronomers has shown the arc to be consistent with the stellar stream from a smaller satellite galaxy, tidally disrupted as it merged with M63 during the last 5 billion years. Their discovery is part of an increasing body of evidence that the growth of large spirals by cannibalizing smaller galaxies is commonplace in the nearby Universe. (text: apod.nasa.gov/apod/ap100911.html)

 

This picture was photographed during April 2016 in Rozhen observatory, Bulgaria.

 

Equipment: home assembled reflector 10 in., f/3.8

 

Mount WhiteSwan-180 with a control system «Eqdrive Standart», camera QSI-583wsg, Televue Paracorr-2. Off-axis guidecamera QHY5L-II.

 

LRGB filter set Baader Planetarium.

 

L = 54 * 900 seconds , bin.1, RGB = 21* 450-600 seconds, bin.2 each filter. 22 hours total.

 

FWHM source in L filter 1.80"-2.96", sum in L channel - 2.32"

 

The height above the horizon from 56° to 83°, the scale of 1"/ pixel.

 

Processed Pixinsight 1.8 and Photoshop CS6

M 101 A spiral galaxy in the Constellation Ursa Major. Distance from Earth 21 million light years

To be honest this is more my son Matthew's hobby than mine but I must admit the results are quite surprising even though lacking a little in resolution!

I have been waiting and waiting since November to have a clear night with no wind or moonlight on a weekend. Finally, I got my chance in late March, and it was my last shot until next November as Orion will start to fade below the horizon in April.

 

Orion is one of my favorite deep space objects to photograph, but the bright core makes it a challenge to capture well. I really like how this turned out!

 

(Explore # 84)

 

www.rossellet.com

A small section of the nebula known as the Vela Supernova Remnant

 

See on Fluidr

 

OTA: Takahashi FSQ-106

MOUNT: Software Bisque Paramount MX

CAMERA: SBIG STX-16803

GUIDE CAMERA: SBIG STX built in

REDUCER: na

SOFTWARE: SGP, PhD2, TheSkyX, Pixinsight, Starnet++, Photoshop

FILTERS: Astrodon LRGB; Hα 5nm, SII 5nm, OIII 5nm

ACCESSORIES: SBIG FW-7 Filter Wheel

LOCATION: M & K Observatory, NSW Australia

 

To see more of my work and to buy prints visit www.jklovelacephotography.com/pages/space

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