View allAll Photos Tagged Cepheus

From left to right you can see the constellations: Cepheus, Lacerta, Cygnus, Lyra, Sagitta and Aquila.

Next to the top-center, the star Vega stands out. On the other side of the Milky Way, in the center to the right, Altair is clearly visible.

This is the faint emission nebula designated as IC 1396 in the constellation Cepheus. This region is energized by the bright, bluish central multiple star HD 206267. You can see the Elephant’s Trunk Nebula, IC 1396A, on the lower edge of this image. From NASA APOD, “Stars could still be forming inside the dark shapes by gravitational collapse. But as the denser clouds are eroded away by powerful stellar winds and radiation, any forming stars will ultimately be cutoff from the reservoir of star stuff.”

 

Tech Specs: William Optics REDCAT 51 Telescope, ZWO ASI071MC camera running at 0F and Optolong L-eXtreme 2” Filter, 5 Hours and 35 Minutes using 5-minute subs, Sky-Watcher EQ6R-Pro mount, ZWO EAF (ProAstroGear Black-CAT) and ASIAir Pro, guided using a ZWO 30mm f/4 mini guide scope and ZWO 120 mini, processed in PixInsight. Image Date: August 3, 2025. Location: The Dark Side Observatory (W59), Weatherly, PA, USA (Bortle Class 4).

September 2019

Telescope:Explore Scientific 102 FCD100

Image Camera:ZWO ASI1600mmPro-Cool

Mount:Sky Watcher EQ6R-Pro

LRGB, 2 min exposures approx 100 images per filter

2 Panel Mosaic processed with PixInsight

About 13 hours gathering data, Another 20 hours to process into a finished image.

  

M31 aka The Andromeda Galaxy. Andromeda was the daughter of king Cepheus and his wife Cassiopeia. Cassiopeia would boast that Andromeda was more beautiful than the Nereids (the nymph daughters of the sea god Nereus). This angered Poseidon. Poseidon then send the sea monster Cetus to ravage Andromeda as divine punishment. King Cepheus then chains Andromeda to a rock as sacrifice to sate the sea monster. Along comes Perseus to save Andromeda and slay the sea monster. Ahhh so romantic.

William Optics FLT132 refractor, ZWO ASI2600MC camera, imaged at Tellin, Belgium.

Rad og række, Uge 19, Cepheus Park, Randers

 

In 1898, Randers Sportsklub Freja was founded, and was in 1970 for the first time in the top of Danish football.

In 1985 and 1987, Randers Freja was in the best row (1st division), but had difficulty in meeting the requirements for paid football.

The 1990s were a low point for Randers Freja, as at one point there was a risk of moving down in the Danish series.

in 2003, the current Randers FC was formed by a merger of 5 local football clubs.

vdB 149 and vdB 150 are a reflection nebulae visible in the constellation Cepheus. It seems that they're part of the great dark nebula LDN 1235 and their estimated distance from the earth is about 1019 a.l.

 

Camera: Moravian G2 8300

Filters: 31mm unmounted Optolong

Optic: Triplet Apo Tecnosky 80mm f/4.8

Mount: Ioptron CEM60 HP

Autoguider: camera Magzero 5m, SW 70/500, Phd guiding

Frames: L: 14X600sec - RGB: 4X600 sec each bin1

Processing: Pixinsight, Photoshop

ROG Livery Class 37, No. 37884 "Cepheus"

Seen outside Loram at Derby RTC

Europhoenix/ROG 37884 "Cepheus" burbles away on the DRL where it is booked to stop for 73 minutes, working 5W78 12.17 Gresty Green Through Sidings - Landore T.M.D. conveying off lease Transport for Wales 2car Coradia units 175006 & 175007 between barrier vehicles 6330 & 6344 with 37608 "Andromeda" bringing up the rear.

NGC 7822 in Cepheus

 

Ikharos 10" RC telescope

QSI 683wsg CCD camera

Paramount MX mount.

 

Image taken remotely from AstroCamp, Nerpio, Spain 2014.

 

Narrowband Hubble palette.

Ha: 103 x 600s

OIII: 38 x 600s

SII: 33 x 600s

 

New process with Astro Pixel Processor, PixInsight, Affinity Photo

 

Image: Nik Szymanek & Ian King.

 

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THANKS TO EVERYONE FOR ONE MILLION + VIEWS!!!👍👍

 

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www.astrobin.com/413187

 

Iris Nebula is dramatic reflection nebula in the constellation Cepheus.

With plenty of dark interstellar dust is illuminated by a central hot star named SAO 19158 which is 10 times the mass of our sun.

 

It lies 1,300 light-years away and is six light-years across.

 

It was integrated only 15 hours, 50% best frames of the total valid frames taken between May and June of 2019.

 

PD: I am glad to check my improvements when I compare to this other capture from three years ago. :D

www.astrobin.com/263914

 

Technical card

Imaging telescope or lens:Altair Astro RC250-TT 10" RC Truss Tube

 

Imaging camera:ZWO ASI1600MM-Cool

 

Mount:Astro-Physics Mach-1 GTO CP4

 

Guiding telescope or lens:Celestron OAG Deluxe

 

Guiding camera:QHYCCD QHY5III174

 

Focal reducer:Riccardi Reducer/Flattener 0.75x

 

Software:Main Sequence Software Seqence Generator Pro, Astro-Physics AAPC, Pleiades Astrophoto PixInsight

 

Filters:Astrodon L Gen.2 E-series 36mm, Astrodon B Gen.2 E-series 36mm, Astrodon G Gen.2 E-series 36mm, Astrodon R Gen.2 E-series 36mm

 

Accessories:ZWO EFW, MoonLite NiteCrawler WR30

 

Resolution: 2318x1665

 

Dates:June 1, 2019

 

Frames:

Astrodon B Gen.2 E-series 36mm: 41x180" (gain: 75.00) -20C bin 1x1

Astrodon G Gen.2 E-series 36mm: 40x180" (gain: 75.00) -20C bin 1x1

Astrodon L Gen.2 E-series 36mm: 177x180" (gain: 75.00) -20C bin 1x1

Astrodon R Gen.2 E-series 36mm: 42x180" (gain: 75.00) -20C bin 1x1

 

Integration: 15.0 hours

 

Avg. Moon age: 27.55 days

 

Avg. Moon phase: 4.36%

 

Astrometry.net job: 2777189

 

RA center: 315.429 degrees

 

DEC center: 68.162 degrees

 

Pixel scale: 1.007 arcsec/pixel

 

Orientation: 270.122 degrees

 

Field radius: 0.399 degrees

 

Locations: AAS Montsec, Àger, Lleida, Spain

 

Data source: Own remote observatory

 

Remote source: Non-commercial independent facility

  

I am really happy with my latest image of the Elephant trunk nebula (IC 1396). The Elephant's Trunk Nebula is a concentration of interstellar gas and dust within the much larger ionized gas region IC 1396 located in the constellation Cepheus about 2,400 light years away from Earth.

 

The Elephant's Trunk Nebula is now thought to be a site of star formation, containing several very young (less than 100,000 yr) stars that were discovered in infrared images in 2003. Two older (but still young, a couple of million years, by the standards of stars, which live for billions of years) stars are present in a small, circular cavity in the head of the globule. Winds from these young stars may have emptied the cavity. The combined action of the light from the massive star ionizing and compressing the rim of the cloud, and the wind from the young stars shifting gas from the center outward lead to very high compression in the Elephant's Trunk Nebula. This pressure has triggered the current generation of protostars.

 

Equipment:

Telescope - William Optics Redcat 51

Imaging Camera- Qhy268m

Mount - Sky-watcher EQ6-R Pro

 

Software:

Sequence Generator Pro

Pixinsight

Lightroom

Photoshop

 

Lights:

R-50x30sec

G-50x30sec

B-50x30sec

Sii-40x300sec

Ha-40x300sec

Oiii-40x300sec

 

35 Darks

100 Bias

Total integration 12.5 hours

This is a 140° panorama of the northernmost section of the Milky Way, from Auriga at left to Aquila at right. Perseus, Cassiopeia, Cepheus and Cygnus are across the centre.

 

This northern section of the Milky Way stretches high across the sky on autumn nights as seen from the northern hemisphere, as it was this night, October 30, 2021.

 

The Milky Way is laced with many dark lanes of interstellar dust which extend off the main band of the Milky Way, as at centre. The dust colours the Milky Way and sky with a yellow-brown tint. Punctuating the Milky Way are red and magenta emission nebulas, the most prominent being the North America Nebula in Cygnus (right of centre) and the California Nebula (at far left) in Perseus.

 

At right are the three stars of the Summer Triangle (R to L: Altair, Vega and Deneb); at left is Capella in Auriga. At centre is the W of stars of Cassiopeia.

 

This is a stitch of 4 segments, each a stack of 8 x 4-minute expsures at ISO 800 with the Canon Ra and with the RF 28-70mm lens at 28mm and f/2.8. It was on the Star Adventurer Mini tracker. Another panorama of 4 segments taken through a Kase StarGlow filter and layered in added the glows on the bright stars.

 

All stacking, stitching and alignment was in Photoshop. Taken from home on a very clear night October 30, 2021. A bright Kp 6 to 7 aurora was forecast for this night but never materialized. Bands of reddish airglow drifted through the fields during the exposures but the stacking and averaging helped smooth out the discolouration.

This is the faint emission nebula designated as IC 1396 in the constellation Cepheus. This region is energized by the bright, bluish central multiple star HD 206267. You can see the Elephant’s Trunk Nebula, IC 1396A, on the lower edge of this image. From NASA APOD, “Stars could still be forming inside the dark shapes by gravitational collapse. But as the denser clouds are eroded away by powerful stellar winds and radiation, any forming stars will ultimately be cutoff from the reservoir of star stuff.”

 

Tech Specs: Williams Optics REDCAT51, ZWO ASI071mc-Pro running at 0C, Sky-Watcher EQ6R-Pro mount, Optolong L-eNhance filter (2”), 32 x 300 seconds (2hr40min), guided using a ZWO 30mm f/4 mini guide scope and ZWO 120 Mini, controlled with a ZWO ASIAir Pro running v1.5 software, stacked in DSS and processed using PixInsight and Adobe Lightroom. Image date: September 19th and 20th, 2020. Location: The Dark Side Observatory, Weatherly, PA, USA.

NGC 7023 or Iris Nebula is a wonderful example of an open star cluster associated with a reflection nebula. It is located in Cepheus, about 3.5 degrees southwest of β Cep (Alfirk).

 

Visually, NGC 7023 is a fairly bright, irregularly-shaped reflection nebula surrounding a 7th magnitude star (HD 200775) . NGC 7023 lies in a region of the Milky Way darkened by dust, within which the nebula is embedded.

 

NGC 7023 is about 6 light-years across, and 1,300 light-years away. Within the Iris, dusty nebular material surrounds a massive, hot, young star in its formative years.

 

Imaged in December 2024 over three nights at the Turismo Astronómico complex in Los Coloraos, Gorafe, Spain using the Esprit 100ED telescope and ASI 2600 MC Pro camera through a UV/IR cut filter.

 

Full details and a high resolution image you can download here or at: astrob.in/wi2br0/0/

Target: SH2-159 Lobster Claw Nebula

This nebula lies between the constellations of Cassiopeia and Cepheus. In the upper right is the beginnings of the Bubble Nebula that I recently imaged. I used a dual narrowband filter (Ha and Oiii) and processed this as a HOO pallet with the reds indicating Hydrogen and blues Oxygen.

  

Gear:

Mount: ZWO AM5

Main Cam: ZWO ASI294MC Pro @ gain 121 and 8F

Guide Cam: ZWO ASI120MM Mini with ZWO 30mm f/4 scope

Telescope: Askar 103APO w/ 0.8x reducer/flattener - 420mm f/4

Filter: Antlia ALP-T Dual Narrowband 5nm Ha and Oiii

 

Acquisition:

Light frames: 91 5min subs for 7hr 35Min integration

Sessions: 09-Oct-2024

Moon: 8 days old 35% 111deg from target

Location: Houston Backyard ~ Bortle 8/9

 

Processing

• Pixinsight Auto DBE, BTX, STX

• Pixinsight split starless channels, NXT

• Pixinsight Create HOO channels

• Ha = R • Oiii = .5*B+.5*G

• Pixinsight Statistical stretch

• Pixinsight Create HOO image

• R = Ha

• G = ((Oiii*Ha)^~(Oiii*Ha))*Ha + ~((Oiii*Ha)^~(Oiii*Ha))*Oiii

• B = Oiii

• Pixinsight Narrowband Normalization HOO, Lightness Ha, Blend Mode 1 Amount 0

• Pixinsight HT black point and balance channels, Curves for saturation

• Pixinsight Stretch Stars using - Star Stretch

• Pixinsight HT black point color balance, Saturation Curves

• Photoshop ACR contrast, black point, clarity, de haze

• Photoshop Selective Colors, ACR, channel D&B to balance colors

• Photoshop Screen stars, duplicate layer/black mask/reveal select stars

• Photoshop Final curves, watermark

37884 'Cepheus' 5Q70 13.00 Stewarts Lane T&RSMD - Wolverton Centre Sdgs.

Taking 455814 to works.

 

28/07/18

 

37884 "Cepheus" passes Wingfield Park while working Transport for Britain "The Buxton Spa Express" 1Z86 1710 Buxton - Lichfield City returning charter which has 57312 and 37608 on the rear on 18th July 21.....having chased from Buxton in Sunday traffic, this was just a point and press from the car door having run out of time

PM1-333 is a small (70 arc seconds) planetary nebula in the constellation Cepheus. It was discovered by Andrea Preite-Martinez in 1988. I believe this to be the deepest, and highest resolution colour image of this target. The tiny blue progenitor star can just be made out dead centre of the image.

It lies within IC1396 where it appears as a small dot at the bottom left hand corner in J-P Metsavainio's excellent image 1.bp.blogspot.com/-JEMi-QvpB0Q/XicHMRDQXbI/AAAAAAAARug/EC...

Image captured on my remote dual rig at Fregenal de la Sierra in Spain between 20-30 September 2021.

Scopes: APM TMB LZOS 152 Refractors

Cameras: QSI6120wsg8

Mount: 10Micron GM2000 HPS

A total of 54 hours image capture (HaOIIILRGB)

More details at: www.imagingdeepspace.com/pm1-333.html

The Elephant's Trunk nebula and it's surroundings (IC 1396) form a large emission nebula complex located in the Cepheus constellation and about 2,400 light years away from earth.

 

Image taken with a TS Star71/347mm flatfield apo & ATIK 383l+ CCD Camera. (h-alpha & OIII data)

NGC6946 is a face-on intermediate spiral galaxy with a small bright nucleus, located on the boundary between the constellations of Cepheus and Cygnus. Its distance from Earth is about 22.5 million light-years. Discovered by William Herschel on 9 September 1798, this well-studied galaxy has a diameter of approximately 40.000 light-years, about one-third of the Milky Way’s size, and it contains roughly half the number of stars as the Milky Way. Due to its prodigious star formation it has been classified as an active starburst galaxy. In the past century, eight supernovas have been observed to explode in the arms of this galaxy, attaching weight to its nickname of the “Fireworks Galaxy.” The galaxy is heavily obscured by interstellar matter as it lies quite close to the galactic plane of our Milky Way.

 

Appearing in the same field, just 40′ northwest of NGC6946 you find NGC6939, a dim open star cluster. The cluster lies approximately 4.000 light years away and it is over a billion years old.

 

Telescope: 16″ f3.75 Dream Scope

Camera: FLI ML16803

Mount: ASA DDM85

Exposure: 8 hours (60x300s L + 3x10x300s RGB)

Acquisition: May 2018 – Processing: May 2021

Location: Southern Alps, France

 

more on delsaert.com/

37884"Cepheus" +769421 pass Lower Moor on 03/Jan/25 with 5Q42 10.47 Long Marston to Crewe.

The Elephant's Trunk nebula is a concentration of interstellar gas and dust within the much larger ionized gas region IC 1396 located in the constellation Cepheus about 2,400 light years away from Earth. The piece of the nebula shown here is the dark, dense globule IC 1396A; it is commonly called the Elephant's Trunk nebula because of its appearance at visible light wavelengths, where there is a dark patch with a bright, sinuous rim. (Wikipedia)

 

Narrowband image: 19-20-21/4/15

Oxfordshire, UK

4.3 Hours Total Exposure

Bin 1x1: 7x1200s Ha

Bin 2x2: 6x600s SII, 6x600s OIII

 

Equipment:

T: Takahashi FSQ106ED

C: QSI683ws Mono CCD, Astronomik Filters (6nm Ha)

M: Celestron Advanced Vx

G: QHY5-II

 

Acquisition and Processing:

PHD2, Sequence Generator Pro, CCDStack2, Photoshop CS6

This is a dark nebula in Cepheus. I imaged this with the Takahashi Epsilon 180 and the ZWO ASI 2400 MC PRO.

 

ROG operated Class 37/8 No.37884 ‘Cepheus‘ hauling 317511 at Milton Malsor with 5Q58 09:01 Kilmarnock Bonnyton Depot - Ilford E.M.U.D.

 

Nikon D5100 + Zenithstar 73

SVBony CLS filter

ZWO ASI224MC + WO Uniguide 120mm

 

November 6th & 8th, 2021

140 x 2min

 

AstroM1

(r2xb.2)

  

Here is my recent image of the Elephant trunk nebula (IC 1396) with my big telescope the Celestron 9.2 5Edge HD. The Elephant's Trunk Nebula is a concentration of interstellar gas and dust within the much larger ionized gas region IC 1396 located in the constellation Cepheus about 2,400 light years away from Earth.

 

The Elephant's Trunk Nebula is now thought to be a site of star formation, containing several very young (less than 100,000 yr) stars that were discovered in infrared images in 2003. Two older (but still young, a couple of million years, by the standards of stars, which live for billions of years) stars are present in a small, circular cavity in the head of the globule. Winds from these young stars may have emptied the cavity. The combined action of the light from the massive star ionizing and compressing the rim of the cloud, and the wind from the young stars shifting gas from the center outward lead to very high compression in the Elephant's Trunk Nebula. This pressure has triggered the current generation of protostars.

 

Equipment:

Telescope - Celestron 9.25 Edge HD

Imaging Camera- Qhy268m

Mount - Sky-watcher EQ6-R Pro

 

Software:

Sequence Generator Pro

Pixinsight

Lightroom

Photoshop

 

Lights:

R-30x60sec

G-30x60sec

B-30x60sec

Sii-50x300sec

Ha-50x300sec

Oiii-50x300sec

 

35 Darks

100 Bias

Total integration 14 hours

Rail Operations Group 37884 "Cepheus" stands at the signal on the DRL hauling scrap yard bound former Strathclyde EMU 314206 working 5Q76 22.26 Shields T.M.D. [E] - Newport Docks [Simsgroup]

This nebula is rightly named the Dark Shark nebula. This was my third try at capturing this one, with the first two not worth completing the processing. The nebula is both a dark and reflection nebula in the constellation Cepheus approximately 650 light-years away. The shark spans approximately 15 light-years head-to-tail.

 

Gear:

Mount: ZWO AM5

Main Cam: ZWO ASI294MC Pro @ gain 121 and 8F

Guide Cam: ZWO ASI120MM Mini with ZWO 30mm f/4 scope

Telescope: Askar 103APO w/ 0.8x reducer/flattener - 560mm f/5.4

Filter: Baader Moon and Sky glow Broadband light pollution

 

Acquisition:

Light frames: 142 180 second subs for 7hr 6min integration

Sessions: 02-Oct-2024

Moon: 0 days old 0%

Location: Houston Astronomical Society Dark Site ~ Bortle 4

 

Processing

• Pixinsight Auto DBE, SPCC ,BTX, STX

• Pixinsight Stretch Starless using script - statistical stretch

• Pixinsight Stretch Stars using - GHS Arcsinh stretch

• Pixinsight Histogram stretch to set better black point color balance, Saturation Curves

• Photoshop ACR contrast, black point, clarity, de-haze

• Photoshop Selective Colors to balance colors

• Photoshop Screen stars, duplicate layer/black mask/reveal select stars

• Photoshop Final curves, watermark

Spooky shapes seem to haunt this starry expanse, drifting through the night in the royal constellation Cepheus. Of course, the shapes are cosmic dust clouds faintly visible in dimly reflected starlight. Far from your own neighborhood on planet Earth, they lurk at the edge of the Cepheus Flare molecular cloud complex some 1,200 light-years away. Over 2 light-years across the ghostly nebula known as vdB 141 or Sh2-136 is near the center of the field. The core of the dark cloud on the right is collapsing and is likely a binary star system in the early stages of formation.

(Text from apod.nasa.gov/apod/ap101030.html)

This picture was photographed on July 6-8, 2011 in the Crimea during the festival of amateur astronomy, "Southern Nights 2011" (height of 600 m above. sea level)

  

Equipment: reflector S&D 254 mm. f/4.7 (New carbon tube!), Mount WhiteSwan-180, camera QSI-583wsg, Tevevue Paracorr. Off-axis guidecamera Orion SSAG.

RGB filter set Baader Planetarium.

L: 20x600 sec., RGB: 10x600 sec. each filter, all unbinned.

North up.

Processed Pixinsight and Photoshop CS5.

 

Prints, cards and more are available via the website: shiny.photo/photo/Sh2-132-The-Lion-Nebula--Cepheus-20c162...

 

Sh2-132, also known as the "Lion Nebula", is an emission nebula located in the constellation Cepheus. Part of the Sharpless catalog, a list ofH II regions - clouds of glowing gas where star formation occurs.

 

About 10,000ly distant and 250ly across, Sh2-132 is situated in the Perseus arm of the Milky Way.

 

The most prominent sources of ionization in Sh2-132 are two Wolf-Rayet stars, which are extremely hot and massive stars nearing the end of their lives. These stars emit intense stellar winds shaping the surrounding gas into intricate structures.

 

Another of those occasions where one tries to match the DSS image of the Ha emission pattern resembling a lion with how the data looks. Make the OIII too bright a blue and it becomes a cut-'n'-shut with the front and rear ends too separate... It's also about the fine veins and blobs of dark nebulae - lanes of dust in the foreground.

 

4hr35min total integration with the IDAS NBZ dual-narrowband (Ha + OIII) filter, from which I extracted the Ha & OIII data separately using APP and recombined in PI.

The Cave Nebula is a diffuse nebula in the constellation Cepheus. Sh2-155 is an ionized Hydrogen Alpha region with ongoing star formation activity, at an estimated distance of 2400 light-years from Earth.

Image captured from Grasslands National Park, SK under Bortle 1 skies. 2020-08-14, 2020-08-15 & 2020-08-16.

Image capture details: (5h 40m)

Ha-7x1,200sec (2h20m)

OIII-5x1,200sec((1h 40m)

SII-5x1,200sec(1h 40m)

Imaging Equipment:

SharpStar 140PH Triplet

Celestron CGEM II mount (hypertuned),

ZWOASI1600MM Pro camera

ROG Class 37 37884 "Cepheus" passes Woodacre near Garstang on 0s08 Dertby RTC - Kilmarnock Civil Engineer's Sidings on 26/06/2022

Was the name of a 1954 book by Aldous Huxley. This Is IC 1396 an area of star formation in the constellation of Cepheus containing the well known Elephants trunk Nebula which can be seen at about 12 o'clock in the Nebula. This is a stack of 8 HSO one click observations taken with the Telescope live Facility in Spain telescope.live/

My travel on the LDN catalogue of dark nebulae is still in progress.

 

Now I visited the nice west area of the Cepheus Pilars (NGC7822), integrating more than 80 hours of data to create this picture.

 

NGC 7822 is a young star forming complex in the constellation of Cepheus.

 

The complex encompasses the emission region designated Sharpless 171, and the young cluster of stars named Berkeley 59.

The complex is believed to be some 3,000 light years, with the younger components aged no more than a few million years. (credits Wikipedia)

 

Technical card

Imaging telescopes or lenses:Teleskop Service TS Photoline 107mm f/6.5 Super-Apo , Altair Astro RC250-TT 10" RC Truss Tube

 

Imaging cameras:ZWO ASI183MM-Cool , ZWO ASI1600MM-Cool

 

Mounts:Skywatcher EQ6R Pro , Mesu 200 Mk2

 

Guiding telescopes or lenses:Celestron OAG Deluxe , Teleskop Service TSOAG9 Off-Axis Guider

 

Guiding cameras:ZWO ASI290 Mini , ZWO ASI174 Mini

 

Focal reducers:Riccardi Reducer/Flattener 0.75x , Telescope-Service TS 2" Flattener

 

Software:Pleiades Astrophoto PixInsight , Seqence Generator Pro

 

Filters:Astrodon O-III 36mm - 5nm , Astrodon S-II 36mm - 5nm , Astrodon R Gen.2 E-series 36mm , Astrodon G Gen.2 E-series 36mm , Astrodon B Gen.2 E-series 36mm , Astrodon HA 36mm - 5nm , Astrodon L Gen.2 E-series 36mm

 

Accessory:ZWO EFW , MoonLite NiteCrawler WR30 , TALON6 R.O.R , MoonLite CSL 2.5" Focuser with High Res Stepper Motor

 

Dates:Sept. 11, 2020 , Sept. 12, 2020 , Sept. 13, 2020 , Sept. 14, 2020

 

Frames:

Astrodon B Gen.2 E-series 36mm: 100x30" (gain: 75.00) -20C bin 1x1

Astrodon G Gen.2 E-series 36mm: 100x30" (gain: 75.00) -20C bin 1x1

Astrodon HA 36mm - 5nm: 231x600" (gain: 200.00) -20C bin 1x1

Astrodon O-III 36mm - 5nm: 130x600" (gain: 183.00) -15C bin 1x1

Astrodon R Gen.2 E-series 36mm: 100x30" (gain: 75.00) -20C bin 1x1

Astrodon S-II 36mm - 5nm: 121x600" (gain: 183.00) -15C bin 1x1

 

Integration: 82.8 hours

 

Avg. Moon age: 24.69 days

 

Avg. Moon phase: 24.99%

 

Basic astrometry details

Astrometry.net job: 3890533

 

Resolution: 2328x1760

 

Locations: AAS Montsec, Àger, Lleida, Spain

 

Data source: Own remote observatory

 

Remote source: Non-commercial independent facility

Avenue Victor Hugo, Paris. October 18th 2014.

Van den Berg (VdB) 152 is an elongated molecular cloud 1,400 light years distant in the constellation of Cepheus. It is sufficiently dense in localized areas to block all light from stars from reaching us. In other areas, some stars shine through. Its reddish color is largely due to light scattering off dust particles within the cloud. This preferentially scatters light of shorter wavelengths and lets redder light through. The tip of the cloud near the center of the image is reflecting blue light from a nearly embedded star.

 

Telescope: 16″ f3.75 Dream Scope

Camera: FLI ML16803

Mount: ASA DDM85

Exposure: 56x5min L + 18x5min each for RGB

Acquisition: April – May 2017 – Processing: April 2021

Location: Southern Alps, France

 

more on delsaert.com/

SAC SH 2 - 132 named as the Lion Nebula is a very faint nebula in Cepheus, emission Nebula.

Hubble palette image

rear

NEQ6R PRO

W/O FLT 98mm APO

SXV 694 COOLED CCD MONO ( minus 10 deg)

LOADSTAR GUIDE CCD

ASTRODON 5nm NARROWBAND FILTERS

 

3 HRS TOTAL IN HA , o3 s2 ( 900 SEC SUBS)

MAXIM

PHOTOSHOP CC

The Lion Nebula SH2-132

 

Found in the constellation of Cepheus and is 10000 light years from Earth. Captured using narrowband filters to create a colour image.

 

Equipment Used;

FRA 600 telescope

CGX Mount

QHY268M camera

Astronomik narrowband filters

  

Capture details;

48 x 300 ha

48 x 300 oiii

100 x bias (super bias in Pixinsight)

  

Software Used;

PHD2, SGP, Pixinsight & Photoshop

Sharpless 155, is a diffuse nebula in the constellation of Cepheus within a larger nebula complex containing emission, reflection, and dark nebulosity. It is widely known as the Cave Nebula, though that name was applied earlier to Ced 201, a different nebula in Cepheus. Sh-155 is an ionized H II region with ongoing star formation activity and lies at an estimated distance of 2400 light-years. Imaged over 2 nights the 17th and 25th of August 2019.

HEQ5 PRO

ED100mm DS-PRO

QHY294C Gain 2900 Offset 20 -20C

STC Duo narrowband filter

15 x 720sec subs

12 x 900sec subs

Processed using Pixinsight and Photoshop.

LDN 1251, in Lynd's Catalog of Dark Nebulae, is a dense star forming region located in the constellation Cepheus. Together it and other objects combine to form the Cepheus Flare, a large molecular cloud above the Milky Way. Many objects are visible in this image including the dust of LDN 1251, LDN 1243, and a few galaxies including PGC166755 and PGC69472.

 

This image is a 2-panel mosaic taken over 10 nights, with approximately 19 hours of exposure time per panel.

 

- Location: Remote Observatory (Bortle 1, SQM 21.99) near Fort Davis, TX

- Total Exposure Time: 38.75 Hours

 

Equipment:

- Scope: Esprit 100ED w/ 1x Flattener

- Imaging Camera: QHY 268M

- Filters: Chroma LRGB (36mm)

- Mount: Astro Physics Mach1GTO

- Guidescope: SVBony 50mm Guidescope

- Guide camera: ASI 120mm mini

- Focuser: Moonlite Nitecrawler WR35

- Accessories: Pegasus Ultimate Powerbox v2, QHY Polemaster, Optec Alnitak Flip Flat

 

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Software:

- N.I.N.A for image acquisition, platesolving, and framing

- PHD2 for guiding

- PixInsight for processing

 

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Acquisition (Total between both panels):

- L: 380 x 3m

- R: 132 x 3m

- G: 131 x 3m

- B: 132 x 3m

- All images at Gain 56, Offset 25 (Readout mode 1) and -5C sensor temperature

- 20 flats per filter

- Master Dark, Flat & Bias from Library

- Nights: 6/23-6/27, 6/30, 7/1-7/3/22

 

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Processing:

 

- BatchPreprocessing for all calibration

- ImageIntegration with PSFSignalWeights for integration of all masters

 

Combining panels for each master:

- DynamicCrop on each panel

- DynamicBackgroundExtraction on each panel

- ImageSolver to platesolve panels

- MosaicByCoordinates script to create mosaic templates

- PhotometricMosaic script to create 2-panel LRGB masters

 

RGB Processing (apply to each master):

- FastRotation 90 degrees

- DynamicCrop

- DynamicBackgroundExtraction

- NoiseXterminator for linear NR

- StarAlign B and G to R

- ChannelCombination to combine into linear RGB image

- DynamicBackgroundExtraction to remove color gradients

- STF for stretch to non-linear

- CurvesTransformation to balance color

 

Luminance Processing:

- FastRotation 90 degrees

- DynamicCrop

- DynamicBackgroundExtraction

- NoiseXterminator for linear NR

- GeneralizedHyperbolicStretch for initial stretch

- HistogramTransformation x2 for further stretch

- CurvesTransformation on starless copy to increase nebulosity

- PixelMath to combine pushed starless and original via: (1- (1-$T) * (1-star)*F)+($T*~F) where F=0.3

- CurvesTransformation for contrast

 

Combine RGB and Luminance:

- StarAlign RGB to Luminance

- LRGBCombination with RGB channel weights set to 0.9, chrominance NR enabled, and saturation boost

- SCNR green @ 0.2

 

Further Processing:

- CurvesTransformation for contrast

- NoiseXterminator for slight nonlinear NR @ 0.2

- Starnet2 to create starmask

- MorphologicalTransformation for slight star reduction

- ColorSaturation to saturate brown dust

- CurvesTransformation for contrast

- DynamicCrop to remove edges

 

Created Annotated Version:

- Duplicate final image and StarAlign to initial linear Luminance

- ImageSolver script on luminance

- Transfer FITSHeader from solved luminance to staraligned final image

- AnnotateImage script to label objects

- DynamicCrop to remove edges

- IntegerResample to downsample 2x

- Save as PNG

Skywatcher ed 80, f/7.5

Atik 314L+ mono

Filter : Baader Ha 7nm

Total exposure 140min

Constellation: Cepheus

IC 405 in Auriga . a Narrow band image of Halpha, O111 and synthetic Green.

The Fireworks Galaxy on the Cygnus Cepheus border. Reprocess of data captured through Esprit150/ASI1600mm in 2018 and Esprit150/S46 in 2021

The Elephant's Trunk Nebula is a concentration of interstellar gas and dust within the much larger ionised gas region IC 1396. It is located in the constellation of Cepheus and lies around 2,400 light years distant. The piece of the nebula shown here is the dark, dense globule IC 1396A.

Processed using data collected using my TSAPO130Q/QHY163M and 150mm Esprit/QHY163M set ups.

SHO data:

NEQ6 PRO

TSAPO130Q

QHY163M Gain200 Offset 70 -20C

Baader SHO narrowband filter set

Ha 18 x 300sec

OIII 23 x 300sec

SII 25 x 300sec subs

Ha data:

EQ6-R-PRO

QHY163M Gain 200 Offset -20C

8 x 600sec subs

Total acquisition time 6hrs50mins

Processed using Straton star removal, RegiStar, Pixinsight and Photoshop.

150mm Esprit

 

The dark nebulae Barnard 169, 170 and 171 are in the constellation of Cepheus seen against the background stars of the milky way. Dark nebulae are interstellar clouds that contain a very high concentration of dust. This allows them to scatter and absorb all incident optical light, making them completely opaque at visible wavelengths. They are most obvious when located in front of a bright emission nebula or a dense background of stars like in this example. The average temperature inside a dark nebula ranges from about 10 to 100 Kelvin, allowing hydrogen molecules to form and star formation to take place. Large dark nebulae can contain over a million solar masses.

 

Telescope: 16″ f3.75 Dream Scope

Camera: FLI ML16803

Mount: ASA DDM85

Exposure: 7.5 hours (44x300s L + 3x15x300s RGB)

Acquisition: May – June 2021

Location: Southern Alps, France

 

more on delsaert.com/

Rail Operations Group 37884 'Cepheus' passes Acton Wells working 5Q94, 10.31 Wimbledon CSD - Long Marsden with South Western Railways 456024/007/014 on 11/2/22.

Rail Operations Group 37608 'Andromeda' top & tailed with 37884 'Cepheus' pass Pinxton with 5M58 15.08 Worksop Up reception - Derby RTC barrier move on 23rd February 2023.

Sh2-132 is an emission nebula complex located in the top south of Cepheus constellation. Is around 10.500 light years far from Earth. We can see extensive clouds of ionized gas which responsible stars are very hot and massive. Two of these stars has been identified as Wolf-Rayett. It is probable that, in the past, a chained star formation processes took place in the nebula. it seems that this processes are now suspended, as there is no activity evidences. There is also quite information in the net referring to the possible connection between embedded and open clusters, being the Sh2-132 complex the canvas of some of these investigations.

 

The colors of this image (a modded SHO palette mapped as RGB) shows us the different ionized elements that conforms the nebula gas: Sulfur II, Oxygen III and H-alpha.

  

Technical data:

 

Remote Observatory "FarLightTeam"

Team: Jesús M. Vargas, Bittor Zabalegui,José Esteban, Marc Valero.

Telescope: Takahashi FSQ106 ED 530mm f/5

CCDs: QSI683 wsg8

Filters: Baader Planetarium - Halpha-OIII

Mount: 10Micron GM1000 HPS

Imaging Software: Voyager

Processing Software: PixInsight

 

Captured on E-eye Remote Observatory facilities (Fregenal de la Sierra ) Badajoz, Spain.

 

Processing: Marc Valero

 

Resolution: 2,09 arc”/pix

  

Ha: 101x1200”

SII: 106x1200”

OIII: 112x1200”

RGB: 30x300” (each)

 

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