View allAll Photos Tagged deepspace
NGC7380 or Sh2-142 - The Wizard nebula - is approximately 8000 light years away in the constellation of Cepheus.
This is a reprocess of some old data as I was never happy with the original
Details
M: Avalon Linear Fast reverse
T: Takahashi FSQ85 0.73x
C: Atik 460EXM with 3nm narrowband filters
24x1800s Ha
15x1800s OIII
15x1800s SII
Total integration time - 27 hours
The Veil Nebula is a cloud of heated and ionized gas and dust in the constellation Cygnus, at about 2400 light years from us.
It constitutes the visible portions of the Cygnus Loop,a supernova remnant, many portions of which have acquired their own individual names and catalogue identifiers. In modern usage, the names Veil Nebula, Cirrus Nebula, and Filamentary Nebula generally refer to all the visible structure of the remnant, or even to the entire loop itself. The structure is so large that several NGC numbers were assigned to various arcs of the nebula. There are three main visual components: 1. The Western Veil (also known as Caldwell 34), consisting of NGC 6960 (the "Witch's Broom", Lacework Nebula, "Filamentary Nebula"; 2. The Eastern Veil (also known as Caldwell 33), whose brightest area is NGC 6992, trailing off farther south into NGC 6995 (together with NGC 6992 also known as "Network Nebula"; 3. Pickering's Triangle (or Pickering's Triangular Wisp), brightest at the north central edge of the loop, but visible in photographs continuing toward the central area of the loop.
The source supernova was a star 20 times more massive than the Sun which exploded between 10,000 and 20,000 years ago. At the time of the explosion, the supernova would have appeared brighter than Venus in the sky, and visible in the daytime. The remnants have since expanded to cover an area of the sky roughly 36 times the area of the full Moon.
Equipment and settings:
Mount: Skywatcher EQ6 R pro
Lens: Rokinon 135mm F2
Camera: ASI 533MM Pro
Filters: Astrodon SHO
Total integration: 10h30 ( Ha 49 exposures x 5 min, Sii 30 x 5 min, Oiii 77 x 3 min )
Edit in Pixinsight.
Location: my Bortle 6+ backyard.
In honor of tonight's full moon, here's an image from last month's full moon which I photographed about an hour after it rose.
The moon itself here is my capture, and I have used a deep space filter layered behind it, giving a three dimensional element and experience.
Hit the Enlarge button and enjoy your galactic journey floating into space as you view it :)
Discovered in 1786 by William Herschel, the North
America Nebula shows its characteristic shape only in wide field astrophotographs.
The North America Nebula is separated from the Pelican Nebula by a dark dust cloud catalogued in 1962 as L935.
It took until 2004 for astronomers to identify the star that ionizes both the North America and the Pelican Nebula. The light of the inconspicuous star, named J205551.3+435225, is almost entirely blocked by the dark cloud L935. As J205551.3+435225 lies just off the “Florida coast” of the North America Nebula, it has been more conveniently nicknamed the Bajamar Star ("Islas de Bajamar," meaning "low-tide islands" in Spanish, was the original name of the Bahamas).
Equipment:
Telescope: William Optics Megrez 88
Camera: ZWO ASI 1600MM Pro
ZWO EFW with Baader HaRGB filters
ZWO EAF autofocus
ZWO ASI 385MC autoguider
Equatorially mounted Skywatcher AZ-GTI
Controlled with ASIair Plus
9-panel panorama, each 3x60s with RGB @ 5x 180s Ha, total exposure time: 3h36min
The cluster and nebula lie at a distance of 5,000 light-years from Earth and measure roughly 130 light years in diameter. The radiation from the young stars excites the atoms in the nebula, causing them to emit radiation themselves producing the emission nebula we see.
(wikipedia)
The Rosette Nebula is relatively easy to find, it is located about a third of the way between the star Betelgeuse in Orion and the star Procyon in Canis Minor.
IOptron Star Tracker
Nikkor 300mm f.45 vintage optics
135 60 sec exposures
Integration time: 95 minutes
calibration frames: flat, darks, bias
bulb timer
Processed in Siril
Finished in Lightroom and Photoshop
You are looking at a galaxy edge-on that is located 30 million light years away in the constellation Andromeda.
Consider our own Milky Way galaxy which is a huge disk of stars measuring 100,000 light years in diameter but only 1000 light years thick. So galaxies are quite thin relatively speaking.
A so-called edge-on view of a galaxy is like looking at the edge of a dinner plate and trying to see to the other side through the most dense portion. In the case of a galaxy this is mostly interstellar dust which is the dark linear region you see here. NGC 891, also referred to as the “silver sliver” galaxy, is very similar to our own Milky Way in size and luminosity.
The next time you see the Milky Way in a dark sky remember you are actually looking at it edge on also but this time you are on the inside looking out!
Image info:
Location: SkyPi Remote Observatory, Pie Town, NM US
Telescope: Officina Stellare RiDK 400
Mount: Paramount MEII
Camera: QHY600 M
Data: LRGB 3,5,4,4 hours respectively
Processing: Pixinsight
The Iris Nebula (NGC7023) is a reflection nebula approximately 1300 light years away, located in the constellation of Cepheus. On the right hand of the image is VdB 141 (The ghost nebula) so called because of it's shape. This is also a reflection nebula and is about 1500 light years away.
Details:
M: Avalon Linear fast reverse
T: Takahashi FSQ 85
C: QSI690ws-g with Lum filter and Starlight Express Trius SX25C OSC for the colour.
Luminance - 2 pane mosaic 54x600s in total
Colour - 100x600s
Totalling 25 hours and 40 minutes
Distance: ca.23 Mio. Lj
Equipment:
TS 10" f/4 ONTC Newton
1000mm f4
ZWO ASI 1600mmc
Astrodon LRGB
Skywatcher EQ8
Guding:
Lodestar on TS Optics - ultra short 9mm Off Axis Guider
PHD2
total exposure time: 6:15 hours
80x180 luminanz
15x180 red
15x180 green
15x180 blue
April 2018
Processing: PixInsight
Lunette triplet APO 80x480 + réducteur x0.79 + filtre Idas LPS D1.
HEQ5 et guidage chercheur + ASI120mc.
Canon 1000D défiltré partiel.
28 x 180s ; ISO400.
Ciel mag 21.12.
Siril, Pixinsight, Photoshop
The first color image to feature Sivan 5 and Sivan 6?
I believe this is the first successful color image of the nebulae Sivan 5 and Sivan 6. Siv 5 is the larger mass at the top. Siv 6 lies beneath it and includes Sh2-287, the bright section bottom center. The swooping red wisp that stretches from left to right and looks like a ship’s hull isn’t officially part of either nebula.
Astronomer J.P. Sivan identified these forgotten nebulae in 1974 from an Hα survey of the Milky Way in which they appeared as a couple of tiny, irregular blots. Apparently, no one has bothered with them since.
Sivan nebulae are large and exceedingly faint: this image spans over 5° of the constellation Monoceros; and total exposure time is 74 hours with narrowband filters. This area has been photographed before, but always with far less exposure time. Thus, they scarcely reveal these Sivan objects at all, not that anyone was looking for them. In fact, even the small, brighter Sharpless objects in this image barely appear in most other widefield images. If you find any that clearly show these Sivan nebulae, please let me know and I will update this page.
...Speaking of blots, in the cosmic Rorschach ink blot test that is interstellar space, to me this looks like a dog (or seal) sitting in a boat with a single sail. So, I call this the Seadog Nebula.
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: Astrodon LRGB
ACCESSORIES: Optec Gemini Focuser/Rotator
LOCATION: SRO
COPYRIGHT: 2021 JKLOVELACE
Data Acquisition from 2020-10-17 until 2021-01-13
DSO Color Mapping: SH-HO-O with RGB stars
Original Image (Pix) Scale: 4.00
For More Technical Information: www.astrobin.com/1dnvcy/0/
To see more of my work and to buy prints visit www.jklovelacephotography.com/pages/space
This is the 2nd brightest globular clusters after Omega Centauri and one of the most massive in our galaxy. The cluster has a very dense core where the light falls off to a point vs reaching a flatter profile near the center as in a typical globular cluster. It has been proposed a massive black hole may reside near the center. In the night sky this object is about the size of the full moon.
Takahashi TAO-150B
FLI 16200 (scale 1.1")
AP 1600GTO Abs Encoders
Data from Deepskywest El Sauce Observatory (Rio Hurtado, Chile)
L (23x120s) and (7x300s)
R (16x300s)
G (12x300s)
B (11x300s
Total Integration = 4.6hrs
Pixinsight
BPP
Lum HDRComb/DC/HDRMT/MMT
RGB MMT/ASSx2/HT/CT/LComb
Photoshop
Crop/Levels/Curves
Sharpen Stars w/ Mask
Vibrance
Images taken on March 2, 2021
Mars reflects the sun's light and is ~22 light minutes from Earth. The Pleiades is an open star cluster that is ~ 442 light years away from us. While these two are so different, both of them are prominent and easy to spot in the night sky. It’s very cool to witness the two so close to each other. I knew this was happening, but my life and job have been so busy lately it slipped my mind until it was basically happening already.
Step outside tonight and take a lookup. You can find this event just ahead of the constellation Orion. The next time these two will be near each other in our night sky again in 2038!
Equipment:
Celestron CGEM Mount
Canon FD 300mm f/4 L at f/5.6
Sony a7RIII (unmodified)
Altair 60mm Guide scope
GPCAM2 Mono Camera
Acquisition:
Taos, NM: my backyard - Bortle 3
10 x 121" for 20 min and 10 sec of exposure time.
10 dark frames
15 flats frames
15 bais frames
Guided
Software:
SharpCap
PHD2
DeepSkyStacker
Photoshop
My mount was polar aligned with SharpCap (what an amazing system for aligning). I'm not comfortable using my SCT as my lens yet. My solution is to piggyback my Sony a7RIII and adapted Canon FD 300mm f/4 L on a ADM dovetail rail on the top of my optical tube. I used DeepSkyStacker to combine all frames and then processed the TIFF file in Photoshop. I stretched the 32 bit file and used Gradient XT on the image. I then made it a 16 bit file and stretched in level, then curves. I used the color sampler tool and levels to do my best to keep the background space black. I then using my skillset and relied on Astronomy Tools Action Set, and dodging and burning a bit to give the image the finishing touches.
Wisps of charged gases continue to expand after a supernova explosion over 30,000 years ago
See on Fluidr
OTA: Takahashi FSQ-106 EDX4
GUIDER: None
MOUNT: Software Bisque Paramount MyT
CAMERA: FLI ML-16070M
GUIDE CAMERA: None
REDUCER: Takahashi 645 QE .72x f/3.6
SOFTWARE: SGP, PhD2, TheSkyX, Pixinsight, Starnet++, Photoshop
FILTERS: Astrodon LRGB; 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
After listening to another lecture on quantum physics, I realized that I hadn't spent much time in this area... We will make up for it ! ;)
This nebula also called the Lambda Centauri Nebula is found in the constellation Centaurus.
H: 22x30m
O: 24x30m
S: 25x30m
Total Integration = 35.5hrs
Telescope: PW17
Camera: FLI ML16803
Remote Data from Deepskywest El Sauce Observatory, Chile.
Designation: M15, NGC 7078
Constellation: Pegasus
Visual magnitude: +6.2
Apparent size: 18′
Diameter: 178 light years.
Distance: 34,000 light years.
21 minute exposure.
2019-10-24
A faint emission nebula located in Cygnus. There is no information about the distance of this nebula.
This is a 2 pane mosaic so that all of the delicate dust is captured as well, using an Ha and OIII filter to create a bi colour image.
Details:
M: Avalon Linear Fast reverse
T: Takahashi FSQ85 0.73x
C: QSI690ws-g with 3nm Ha and OIII filter
Pane 1 - 11x1800s Ha, 10x1800s OIII
Pane 2 - 10x1800s, 9x1800s OIII
Totalling 20 hours of exposure time.
English below
Abell 85 o LBN576, nota come Nebulosa Testa d'Aglio, è un resto di supernova nella costellazione di Cassiopea distante circa 9780 anni luce e di diametro di circa 98 anni luce.
11 ore e 20 minuti in pose guidate da 600 secondi con filtro dualband Antlia ALP-T 5nm, per le stelle un'ora in pose guidate da 60 secondi con filtro broadband SV260. Telescopio newton 150/600 con correttore Tecnosky 0.95x, camera Tecnosky Vision 571C, montatura Eq6-R Pro, elaborazione in Pixinsight.
Abell 85 or LBN576, known as the Garlic Nebula, is a supernova remnant in the constellation Cassiopeia, approximately 9,780 light-years away and approximately 98 light-years in diameter.
11 hours and 20 minutes in 600-second guided exposures with an Antlia ALP-T 5nm dual-band filter, and one hour for stars in 60-second guided exposures with an SV260 broadband filter. 150/600 Newtonian telescope with a Tecnosky 0.95x corrector, Tecnosky Vision 571C camera, EQ6-R Pro mount, and Pixinsight processing.
Brief Description:
A dynamic looking region of the constellation Auriga where spherical nebulas appear hurled to crash into each other. This image features the nebulas Sh2-232, Sh2-235, Sh2-231, Sh2-234 and LBN 796, and the open star clusters M38 and M36.
In-depth Description:
This is a dynamic looking region of the constellation Auriga where spherical nebulas appear hurled to crash into each other. This image includes the nebulae Sh2-232, Sh2-235, Sh2-231, Sh2-234 and LBN 796, among others, and the open star clusters M38 and M36.
The eyeball looking nebula (Sh2-232) has been mistaken for a planetary nebula, but none of the round or semispherical objects in this image are actually classified as PNs (per Galaxymap and SIMBAD). In fact, the big fuzzy ball in the lower left center (right above cluster M36) does not seem to have any designation at all and is merely a part of the greater nebula LBN 796. A 2012 study suggests that these unusual forms are all part of an expanding shell, the result of an ancient supernova.
These nebulae are all features of a larger molecular cloud located 1800 pc from us. By comparison the two clusters are much closer: M36 (bottom center) is 1330 pc distant, and M38 (center right) lies only 1066 pc away.
To see more of my work and to buy prints visit www.jklovelacephotography.com/pages/space
Complex reflection dust nebulae in the constellation of Cepheus the circumpolar region. The popular name - "The dance of demons".
This picture was photographed durin November 2015 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 = 20 * 900 seconds , bin.1, RGB = 15 * 300-450 seconds, bin.2 each filter. About 9 hours.
FWHM source in L filter 2.03"-2.92", sum in L channel - 2.50"
The height above the horizon from 52° to 46°, the scale of 1"/ pixel.
Processed Pixinsight 1.8 and Photoshop CS6
------------------------------------------------------
• Sky-Watcher Quattro 250P
• Sky-Watcher EQ8-R Pro
• ZWO ASI294MM-Pro
• Astronomik L: 27x300s bin1 gain 0
• Astronomik RGB: 30x300s bin2 gain 125
• ZWO Hα 7nm: 41x600s bin1 gain 200
• ZWO Hα 7nm: 13x300s bin1 gain 200
• ZWO OIII 7nm: 4x600s bin2 gain 200
• ZWO OIII 7nm: 36x300s bin2 gain 200
(total integration 16.3h)
• 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
Handheld and captured with my D500 and 18-200mm lens... This has a deep space vibe to it and I rather like it.
NGC 7635 a.k.a. Bubble Nebula
……………………………................
Space is full of things / situations / events that intrigue us, NGC7635 being one of those. In short and for everyone to understand, a massive star is caught in a "bubble". This star is almost 50 times larger than the Sun and the emitted radiation is about 1 million times stronger than it, producing a stellar wind that exceeds 5 million km per hour, wind that pushes dust and gas outward creating thus a shell or a bubble, a situation that obviously led to the popular name of this nebula.
As general information, the Bubble Nebula is an emission nebula with a diameter of about 7 light-years, located in the constellation Cassiopeia, at a distance of over 7000 light-years from Earth and it was discovered in 1787 by the British astronomer, William Herschel.
Specialists believe that in a short time ( meaning in the next 10-20 million years), the "guilty" star will consume its energy resources, and will explode, forming a supernova.
Equipment and settings:
Mount: SW EQ6R
Telescope: SW 150/750 PDS
Camera: ASI 533MM Pro
Filters: SHO Astrodon 5nm
Integration: 15h45’
Edit in Pixinsight.
Location: my Bortle 6+ backyard
The beautiful Rosette Nebula.
Emission nebula lit by bright ultraviolet light from stars at the center. NGC 2237.
fine detail present.
Captured 12/2020
Telescope
ASA 500N, F-3.8
CAMERA FLI PL16803
50 cm Newtonian telescope
Chile
Telescope Live
2 hours total exposure, SHO false color.
Pixinsight and photoshop, Topaz sharpen ai.
Nebula is 100 ly wide, and located at a distance of 5000 ly.
M33 is a large, bright galaxy in the constellation Triangulum. Part of the Local Group of Galaxies, which also includes the Milky Way and Andromeda Galaxies, it lies at a distance of "only" 2.7 million light years.
Telescope: Tele Vue 76mm Refractor with 0.8x Focal Reducer (383mm focal length)
Camera: QSI 683wsg
Mount: iOptron iEQ45 Pro
Integration: 75 minutes each of RGB (15 x 5mins)
Software: PixInsight 1.8.8
Every time you change the space around you, it's worth remembering that this can lead to global changes! And our most insignificant actions can lead to very significant changes! Sometimes even a glance at a spider web in the forest can lead to changes all over the planet ;)
Less than a week since our last image, and the tail of Comet C/2025 A6 Lemmon is stealing the show! Stretching longer and more vibrant, this comet is a stunning sight as it blazes through its orbit. ✨
Captured on October 22, 2025—just one day after its closest approach to Earth at about 0.60 AU (90 million km)—this latest view highlights the comet’s growing tail.
C/2025 A6 Lemmon is a long-period comet on an elliptical, retrograde orbit inclined at 143.7° to the ecliptic, taking it on a journey of roughly 1,350 years around the Sun. Currently, it’s hurtling toward perihelion on November 8 at a mere 0.53 AU from the Sun (closer than Venus!), where solar heat will vaporize its icy nucleus and fuel even more dramatic displays. This passage will shorten its orbital period to around 1,150 years—a true cosmic wanderer! 🌌
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.
NGC 4565 a.k.a. Needle Galaxy
.....................................................
NGC 4565, better known as the Needle Galaxy, is a spiral galaxy located in the constellation Coma Berenice, at about 40 million light-years from Earth. This galaxy is larger than the Milky Way, with a diameter of 130-150000 light-years, and appears to be brighter than Andromeda. Due to its shape, in addition to Needle, NGC4565 is also known as Flying Saucer Galaxy or Berenice's Hair Clip. Very well known and popular in astrophotography, Needle Galaxy can be imaged with a small telescope, but a longer focal length would lead to a more detailed result.
Equipment and settings:
Mount: SW EQ6R
Telescope: SW 150 PDS
Camera: ASI 533 MC Pro.
Filter: Baader UV/IR cut
Total exposure: 6h26' ( 193 frames x 2 min )
Stacked with Deep Sky Stacker.
Edit in Pixinsight.
Location: my Bortle 6+ backyard.
CTB 1 is a supernova remnant (SNR) in the constellation Cassiopeia and a source of optical, radio, and X-ray emissions. A recent study reports that a pulsar was born from the supernova that produced CTB 1 and ejected into the galaxy.
CTB 1 is approximately 9784 light years away and physically spans another 98 light years in diameter while it is dated to be approximately 10,000 years old.
Image captured over 5 nights; 2021-11-06, 07, 08, 10, & 11
20.5 hours total integration
Ha subs 18 * 1,800 sec = 9 hours
OIII subs 12 * 1,800 sec = 6 hours
SII subs 11 * 1,800 sec = 5 hours 30 min
Imaging Equipment:
SharpStar 140PH Triplet 910mm focal length
Mesu 200 MKII mount,
ZWOASI2600MM Pro camera
SHO 3.0nm filters
Theme: Cyberpunk, Deepspace, Fantasy, Steampunk Featuring: Accessories, Apparel, Cosmetics, Decor, Hair, Jewelry, Poses, Shoes, Skins, Tattoos Event Opening Date: May 29, 2022 Event Closing Date: June 22, 2022
An LRGB image of NGC2403
The image comprises of:
Luminance - 10 hours.
Red - 4 hours.
Green- 4 hours.
Blue - 4 hours.
Total - 22 hours
10 and 15 minute subs.
Acquisition - Planewave 12.5" CDK, PME, QSI 583 8WSG CCD, Lodestar auto guider, TSX, Maxim DL. Astrodon LRGB filters.
Processing Pixinsight 1.8 - I have had this data set around for a while and have never been happy with my processing results.
Prospetticamente attorno ad una delle più luminose stelle del cielo, la stella multipla e variabile Gamma Cassiopeiae (γ Cas), chiamata Tsih o Navi, si trova la regione di H II (idrogeno ionizzato) conosciuta con la sigla Sh2-185, e al cui interno spiccano due nebulose catalogate con le sigle IC59 e IC63.
Pensavo che riuscire a fotografare questa regione fosse una cosa più semplice invece devo ammettere che la nebulosità più debole di Sh2-185 è veramente molto evanescente e la presenza di gradienti causati da Inquinamento luminoso ha complicato le cose; quindi sono stato costretto mio malgrado ad utilizzare con decisione i tool di denoise per ridurre il rumore.
Ma ciò che ha reso più difficile elaborare questa immagine è stata la presenza della luminosa Gamma Cassiopeiae il cui riverbero abbagliava una parte dell'immagine e attorno alla quale c'era un antiestetico alone penso causato da riflessioni all'interno del riduttore 0.6X.
Ciò malgrado penso di aver raggiunto un discreto risultato.
________
Perspectively surrounding one of the brightest stars in the sky, the multiple variable star Gamma Cassiopeiae (γ Cas), called Tsih or Navi, lies the H II (ionized hydrogen) region known by the acronym Sh2-185, within which stand out two nebulae cataloged as IC59 and IC63.
I thought photographing this region would be easier, but I have to admit that the faintest nebulosity of Sh2-185 is truly very evanescent, and the presence of gradients caused by light pollution complicated matters; so, against my will, I was forced to vigorously use denoising tools to reduce the noise.
But what made processing this image more difficult was the presence of the bright Gamma Cassiopeiae, whose glare dazzled part of the image and which had an unsightly halo around it, I think caused by reflections within the 0.6X reducer.
Even so, I think I achieved a decent result.
____________
Optic: APO Refractor Askar 103APO + 0.6X
Camera: ZWO ASI533MC-Pro
Mount: Sky Watcher HEQ5 Synscan
Seeing: 4 (scala Antoniadi)
Filter: Narrowband Optolong L-eNhance 2" + SVbony UV-IR cut
-199x180s 250gain/ 23dark /27flat /80 bias
-64x300s 250gain/ 35dark /27flat /80 bias
t° sensor: -5°C
Date: 2025-10-25, 27 + 2025-11-12,13
Integration: 15h 17m
Temperature: 16°C (media)
location for : Biancavilla -Catania-(Italy) 515m slm (Bortle 5-6) flic.kr/p/8AWHek
Acquisition: NINA, PHDGuiding
Processing: DSS, SIRIL 1.4, PS, GraXpert
The colorful Rho Ophichui cloud complex is one the closest star forming regions in our Milky Way and a favorite target for astrophotography. Highlighted by the bright star Antares, the region provides an impressive spectacle of colorful glowing gases, juxtaposed with converging dark rivers of thick dust.
IC 4604 (Rho Ophiuchi Nebula) is a large diffuse nebula of 5th magnitude located in the southwestern corner of the constellation Ophiuchus (Serpent Bearer), surrounding the bright multiple star system ρ (Rho) Ophiuchi. Several regions of bright and dark nebulosity surround the area, which takes its name from ρ Oph.
At the mid-northern lattitudes, I normally work from, it plays a bit hard to get, as it always rides close to the horizon and is only visible for a few hours during nights from spring to mid summer.
During my Namibia trip in 2023, I had the pleasure to shoot this wonderful area riding high in the unspoiled southern hemisphere sky.
EXIF
Canon EOS-Ra
Canon 70-200mm f/2.8 L IS USM ll @ 135mm
Equatoriallly mounted Skywatcher AZ-GTI
IDAS 12 filter
30x 90s @ ISO1600, unfiltered & 10x 180s @ ISO6400, filtered
The Whirlpool Galaxy is an interacting spiral galaxy in the constellation Canes Venatici
at distance of 23 Mio. Lj
Equipment:
TS 10" f/4 ONTC Newton
1000mm f4
GPU Aplanatic Koma Korrector
ZWO ASI585mc
Skywatcher EQ8
Guding:
Lodestar on TS Optics - ultra short 9mm Off Axis Guider
PHD2
312x30s
total exposure time: 2,6 hours
Processing: PixInsight
Also known as the “Ghost of Cassiopeia”, these brightly outlined flowing shapes look ghostly on a cosmic scale. A telescopic view toward the constellation Cassiopeia, the colorful skyscape features clouds IC 59 (top border left of center) and IC 63.
The New General Catalogue of Nebulae and Clusters of Stars (abbreviated NGC) is an astronomical catalogue of deep-sky objects compiled by John Louis Emil Dreyer in 1888. The NGC contains 7,840 objects, including galaxies, star clusters and emission nebulae. Dreyer published two supplements to the NGC in 1895 and 1908, known as the Index Catalogues (abbreviated IC), describing a further 5,386 astronomical objects.
The clouds of IC 63 shown in the image, about 600 light-years distant, aren't actually ghosts. They are slowly disappearing though, under the influence of energetic radiation from hot, luminous bluish star gamma Cas to the upper right.
Gamma Cas is physically located only 3 to 4 light-years from the nebulae. Slightly closer to gamma Cas, IC 63 is dominated by red H-alpha light emitted as hydrogen atoms ionized by the hot star's ultraviolet radiation recombine with electrons. Farther from the star on the top border, IC 59 shows less H-alpha emission but more of the characteristic blue tint of dust reflected star light. (courtesy APOD 10/26/2024)
Capture info:
Location: SkyPi Remote Observatory, Pie Town NM US
Dates: 11/8- 12/8/2024
Telescope: Orion Optics UK AG14 (F3.8)
Mount: 10Micron GM3000
Camera: QHY268M
Data: HaRGB 12, 5.5, 5, 5.5hrs respectively
Processing: Pixinsight
M16 Eagle Nebula NGC 6611, is a young open cluster of stars in the constellation Serpens. M16 contains an area made famous as the "Pillars of Creation" imaged by the Hubble Space Telescope Technical Info:
30 x 180 sec. Badder UV/IR Cut filter
74 x 300 sec. Astronomik Ha 12 nm filter
45 x 300 sec. Astronomik OIII 12 nm filter
Gain 200, Offset 50, Binning 1x1
Total Integration 7.5 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-ASTAP via N.I.N.A. 1.11
Image processing Pixinsight 1.8.8 and finished in Photoshop CC 2021.
Some kind of deep space microscopic sea creature or the inside of Riley's old coat and some blade rotation.
Wherever it takes you I suppose.
Single long exposure powered by Ted Baker and Lightpainting Brushes.
50mm Wide field of the Rho Ophiuchi region, with Mars and Saturn. To the bottom right is the Milky Way core, with the Cat's Paw nebula visible.
Mars is the biggest / brightest yellow object to the top left, Saturn is the smaller bright object bottom right.
Image details:
52 Minutes: 13x 240 second exposures
Camera: Canon 60Da
Lens: Canon 24-70mm LII F/2,8. Shot at 50mm F/3,2
Mount: SkyWatcher Star Adventurer
The skies were not really dark enough as our imaging location was only 1,5hrs drive out of town. I think to achieve more red in Antares' region I'll need to take separate Ha exposures and blend them to this.
Location:
Magalies mountain Sanctuary - Gauteng, South Africa
Date: #EveryNewMoon 6 May 2016
Check out PhotographingSpace.com for more tips and tutorials on #Astrophotography.
Or visit my website Astrotanja.com for other related stuff and more on the #EveryNewMoon project.
The Butterfly nebula (IC1318) is located in the constellation of Cygnus. The whole region is huge... Here you can only see IC1318b (upper area of nebulosity) and IC1318c (the lower area). IC1318b and c constitute a single giant HII cloud bisected by a thick obscuring dust lane known as LDN 889 which is shown in the middle of the frame.
The bright star to the top right is a class F8 star known as Sadr or Gamma Cygni. Its true location is only 750 light years away and not related to the nebulosity which is much more distant at 5000 light years.
This is a 6 pane mono mosaic. It has been stitched together using Astro Pixel Processor, whch created a seamless mosaic.
Details
M: Mesu 200
T: TMB 152/1200
C: QSI683 with 3nm Astrodon Ha filter
16x1800s in EACH pane, totalling 48 hours of exposure time.