Image Description and Details :

Exposition:
30x600 '' with Ha filter (1x1 binning).
24x600 '' with SII filter (2x2 binning).
24x600 '' with OIII filter (2x2 binning).

Equipment: QHY9, TS 65 Quadruplet (f / 6.5), EQ6-R and Lunático autoguiding.

Software: Astrophotography Tools, PHD Guiding 2.6.5, PixInsight 1.8.

Place: Nerpio, Albacete (Spain).



Copyright: ASTROMONOS - ANTONIO SANCHEZ DEL MAZO

Pythagoras Crater is at the center of this field of view and is a prominent impact crater located near the northwestern limb of the Moon. It has a diameter of 80 miles and is 16,400 feet deep. The prominent central peak rises just over 4,200 feet and is casting a very long shadow that appears to just be touching the western wall of the crater. The rim is well-preserved and the terraced walls are quite apparent. Captured Jan 26 during a full terminator imaging session at 20:28 during the 97.3 % waxing phase. To the southeast is Babbage and to the northeast is Anaximander.Celestron CPC Deluxe 1100 HDAltair IMX174 MonoZWO Filter Wheel - Green Channel FilterX-Cel 3.0 BarlowPrimalucelab Eagle 2 Pro

Copyright: Gary Varney

Image Description and Details :

RECORDING DATA:Object: NGC 1333Date of recording: November 2020Distance: 1,000 light yearsExposure: 144 x 300 sec. (Total 12 hours)Calibration: Darks / Flats / DarkFlatsMount: Skywatcher EQ6-R PROTelescope: Lacerta Fotonewton 250/1000Corrector: Lacerta GPU coma correctorFilter: Astronomik L2 UV-IR Block 2 ″Camera: QHY268c @ Gain 0 at -15 ° CGuiding: ZWO OAG with ASI 120mm-s and PHD2Software: APP / Photoshop CC



Copyright: Daniel Nimmervoll

Image Description and Details :

Lying within the Large Magellanic Cloud, a satellite galaxy to ours around 158,000 light years away in the constellation of Doradus, this rather chaotic but beautiful nebula complex presents an Ha and O3 rich tapestry of colourful nebulae and star clusters. This is a natural colour palette image (I.e. an LRGB image augmented with Ha and OIII narrow band data) comprising 17 hours of data.

FOV: 39.2 x 26.2 arc-minutes @ 0.59 arc-seconds/pixel.

Telescope: Officina Stellare ProRC 360

Camera: SBIG STXL 11002M, AOX and FW-8G

Mount: Paramount ME

Luminance: 12x15 minutes (binned 1x1)Red: 8x15 minutes (binned 1x1) Green: 8x15 minutes (binned 1x1) Blue: 8x15 minutes (binned 1x1) Ha: 10x30 minutes (binned 1x1)O3: 6x30 minutes



Copyright: Marcus Davies

The complex cloud displays an unusual combination of both red emission and blue reflection areas as well as numerous intricate dark patterns. The nebula is located 9000 light years away in the direction towards the galactic centre. The entire area is sprinkled with thousands of stars and fainter dusty and nebulous areas throughout. A separate prominent dark cloud appears dramatically silhouetted against the starry background to the right.A curious example of gas evaporation can bee seen near the core of the Trifid itself. Here a dense stalk, 8 light years from the centre, is emerging from the edge of the bubble surrounding the central cluster, and in the other direction a powerful stellar jet from a young star, HH 399 embedded in the gas, is shooting out in an upwards direction. The bright young stars in the central cluster emit strong radiation which eats away the surrounding gas and dust. The stalk only appears because a denser region lies at its very tip and protects a thin strip of the cloud from this interstellar erosion. The Hubble Space Telescope has imaged this fascinating area in high resolution: http://imgsrc.hubblesite.org/.../hs-2004-17-a-print.jpg. Throughout the nebula lies countless young T Tauri stars just having emerged from their birthplaces inside the gas and dust. These are typically rather faint and reddish, though they are more easily visible in this image of another stellar nursery near AntaresImage details: Date: May - September 2020Exposure: HaLRGB: 270:916:190:190:195 mins, total 29 hours 21 mins @ -25CTelescope: Homebuilt 12.5" f/4 Serrurier Truss NewtonianCamera: QSI 683wsg with Lodestar guiderFilters: Astrodon LRGB E-Series Gen 2 and 3nm H-AlphaTaken from my observatory in Auckland, New Zealand See Less

Copyright: Rolf Wahl Olsen

Image Description and Details :

This image is a blend of 9 images taken on 9 days from 25.12.2020 to 02.01.2021. This shows how the sunspot AR12794 and AR12795 moves along the solsr disk due to Sun’s rotation. Also noticable is the change in thr apparent size of the sunspots where AR12795 ultimately becomes a faculae. The photo was taken with Nikon D5600, Sigma 150-600c and Thousand Oaks Solar Filter (white light). Post-processed via PIPP, Adobe Camera Raw and Photoshop.



Copyright: Soumyadeep Mukherjee

Image Description and Details :

I'm very proud to present this photo in L-HOO which required a total exposure of 27 hours per 20 minutes per photo, spread over 7 nights of the month of May, not counting the 10 hours of image calibration. At a magnitude of 14.74, it is very little luminous, which makes it difficult to image it.

It is located in the constellation Cepheus at a distance of 980 light-years.
Sh2-174 is one of the oldest planetary nebulae that is more unusual because the white dwarf is not in the center of the nebula. This asymmetry is due to the interaction of the planetary nebula with the surrounding interstellar medium.

Exifs :
Imaging telescopes: Skywatcher 200/1000 Newton
Imaging cameras: ASI 1600MM-Pro
Mounts: Skywatcher AZ EQ-6 GT Pro
Guiding telescopes or lenses: Skywatcher 200/1000 Newton
Guiding cameras: Altair GPCAM2 290C Colour
COMA Corector: Baader MPCC Mark III
Software: Pixinsight - NINA - Lightroom
Filters: ZWO OIII 7nm 36mm · ZWO Hɑ 7nm 36mm
Accessory: ZWO OAG

Dates:May 22, 2020 - Country: Hymont (Vosges )- France
Frames: 80x1200" (40 with Ha filter - 40 with OIII filter)
Integration: 26.7 hours



Copyright Information: Jordan Marlière

Image Description and Details :

Captured over several nights in August 202027.5 hours total using HA – OIII – SII filtersAll are 15min exposures – 440xHa – 36xOiii – 30xSii Skywatcher Esprit 120ED with Apex-L reducer – 546mm fl – f/4.55Starlight Xpress Trius Pro-814Astrodon 5nm Ha – 3nm Oiii – 5nm Sii filtersSkywatcher EQ6R Pro mount guided with Lodestar X2 using OAG on the Midi filter wheelOther gear - Intel Nuc PC, Pegasus UPBv2, Starlight Instruments Posidrive autofocusCaptured with N.I.N.A., PHD2, Polemaster All processing in PixinsightCaptured from my backyard in Birch Bay, WA


Copyright: Justin Katsinis - AstroLayne

This image shows the rising Seagull Nebula soaring high above Mt. Druesberg in central Switzerland.

The Seagull Nebula is an emission nebula on the borders of the constellations of Monoceros and Canis Major. Its location 10 degrees below the celestial equator puts it rather low for northern hemisphere observers, which may be the reason why it is not as famous as other nebula that rise higher during the night.

For deepscapes however, a deep space object needs to hug the horizon, which makes the Seagull Nebula a perfect target.

Despite careful planning, the resulting image contains a big surprise: The Seagull Nebula is not that splendid bird with a bright body and wispy wings and tail you can see in this deep image. I didn't even know that these structures exist. What is known as the Seagull Nebula is just the bright body part that remotely resembles a soaring bird on its own - it is the bird in a much bigger, more detailed bird! How awesome!

EXIF

Canon EOS 6D, astro-modified

ZWO ASI 1600MM Pro

Canon EF 70-200mm f/2.8 @ f/4

Baader Ultra Narrowband H-alpha and Olll filters

Modified Skywatcher AZ-GTI mount, controlled with ASIair

Sky:

Canon EOS 6D @ 200mm:

26 x 60s @ ISO1600 for RGB

ZWO ASI 1600MM Pro @ 96mm (to match the 200mm full frame FOV)

20 x 300s H-alpha @ Gain 200

10 x 300s Olll @ Gain 200

Foreground:

8 x 90s @ ISO1600

Copyright: Ralf Rohner

Image Description and Details :

Sh2 -132 is a large and very weak emission nebula in the constellation of Cepheus .
The stars responsible for the ionization of its gases are very hot and massive; in particular, two Wolf-Rayet stars were identified , known with the initials HD 211564 and HD 211853.

Processed by Santiago Rodríguez

Combination:

Image captured with Halfa and OIII filters of 5 nm. by Carlos Uriarte.
R:Halfa
G: 20%Halfa/80% OIII
B:OIII
Halfa astrodon 5nm filter (900 "x 91): 22.75h BIN 1
OIII astrodon 5nm filter (900"x50):12.5h
Total: 35.25h
CCD: Atik 460exmono
Telescope: Takahashi FSQ106ED
Ager, LLeida, Spain



Copyright: SantiRoHe

Image Description and Details :

Another bright planetary nebula to capture during a full moon.
NGC 1501 is a complex planetary nebula in the constellation Camelopardalis.
It's progenitor star is a pulsating star, meaning that its brightness varies regularly and periodically. In the case of NGC 1501’s progenitor star, this is incredibly fast, with the star’s brightness changing significantly in just half an hour.

Image captured on my dual rig in Spain.Scopes: APM TMB LZOS 152 RefractorsCameras: QSI6120wsg8Mount: 10Micron GM2000 HPSA total of 7 hours image capture.


Copyright: Peter Goodhew

This portion of the Milky Way in the southern hemisphere is very rich in nebulae and some star clusters, my favorite constellation "The southern cross" with its beautiful stars (Acrux, Mimosa, Gacrux and Imai) are the 4 main stars that they form this constellation which serves to find the south cardinal point by moving the central axis of the "cross" 3 and a half times.

We can also see the nebula of the keel or eta carina and below the cross the sack of coal or head of the "Choique" as the Mapuches knew it.

While taking these photos I was able to observe the passage of the International Space Station next to some Russian polar orbit satellites in the province of Rio Negro.

Nikon D 850 camera, 3x 25 ". Iso 6400 nikon 24-120 f4 lens

Copyright: Ariel Maderna

Coronado Solarmax 3 Double Stack

Asi Zwo 178 MM

Copyright: Claudio Ciceri

This is a beautiful region of nebulosity known as NGC 2327. It is part of a larger nebula commonly called The Seagull. It is on the border between Monoceros and Canis Major. This is 30 hours of Ha and LRGB data.

Copyright: Albert Barr

Abell 370 is known for its gravitational lensing effect.

RECORDING DATA:Object: Abell 370Date of recording: November 2020 Distance: 6 billion light yearsExposure: 240 x 180 sec. (Total 12 hours)

Calibration: Darks / Flats / DarkFlats

Mount: Skywatcher EQ6-R PRO

Telescope: Lacerta Fotonewton 250/1000

Corrector: Lacerta GPU coma corrector

Filter: Astronomik L2 UV-IR Block 2 ″Camera: QHY268c @ Gain 0 at -15 °

CGuiding: ZWO OAG with ASI 120mm-s and

PHD2Resolution: 0.77 arcseconds / pixel

Software: APP / Photoshop CC

Copyright: Daniel Nimmervoll

Image Description and Details :

Just below the teapot of Sagittarius in Corona Australis lies a strikingly-beautiful region containing several objects of widely differing ages and distances. Exquisite blue reflection nebulae (NGC 6726/27), lit by the embedded bright stars TY CrA and HD 176386, and IC 4812 (HD 176269 and 176270) appear to be connected by wispy blue filaments that span the dust lane SL-41. Nearly 200 lys closer than those stars, the wing-shaped nebula (NGC 6729) below those filaments is energized by the 310 ly distant R CrA. Closer still is the bright blue eclipsing binary star at the upper right, epsilon CrA, at 102 lys, which along with the far more distant globular cluster NGC 6723 span the "depth" of this 53-arcmin x 53-arcmin scene. The image was made using ten minute guided exposures taken through red, green and blue filters by an unbinned FLI ProLine 16803 camera mounted on Chilescope’s 0.5-m Telescope 2, which were stacked for 1-hr; north is left, and east is down.


Copyright Information: Hal Heaton

Image Description and Details :

The Iris Nebula is a reflection nebula in the constellation Cepheus, which is actually a patch of interstellar dust illuminated by a blue star. In the 2-panel-mosaic wide-field image, you can see that this area of the sky is actually filled with interstellar dust, but the other dust is not illuminated by nearby stars like the Iris Nebula. Image Telescope/Lens: SharpStar 150 2.8 HNTImage Camera: QHYCCD QHY268CMount: iOptron CEM 70Frames :301 * 300sIntegration: 25.1 hoursLocation: Milky Way Observatory, Kangbao County, Zhangjiakou, Hebei Province, China.

Copyright Information: Steed Yu

Image Description and Details : This is an image of M78. Actually, M78 is the brightest reflection nebula (blue nebula near the center) of a nebula complex that includes NGC 2064 (the red nebula on the left of the image), NGC 2067 (the reflection nebula just on the other side of the dark nebula from M78) and NGC 2071 (the reflection nebula in the lower right of the image). This nebula complex is about 1,300 light years away in the constellation Orion, slightly above Alnitak, the leftmost star in Orion’s belt.Telescope: Planewave CDK-17 Camera: FLI PL16803 Mount: Paramount ME Luminance: 27x20 minutes (binned 1x1)Red: 16x15 minutes (binned 1x1) Green: 16x15 minutes (binned 1x1) Blue: 16x15 minutes (binned 1x1)



Copyright: Bernard Miller

Image Description and Details :

NGC 2835 is an intermediate barred spiral galaxy with a massive black hole at its center. It is located in the constellation Hydra, at a distance of approximately 35 to 40 million light years from Earth, and is about 65,000 light years across. Seen face on with its tightly woven arms it has a sea shell like appearance.Imaged in LRGB on our Officina Stellare RiDK 700 at Obstech,Chile.OTA RiDK 700 FL 4900 mm, Mount OS Polar Fork, Camera PL 16803, Filters ChromaLuminance 15 hours 900sRGB 6 hours per channel 900s bin 2



Copyright: Mike Selby

Image Description and Details :

Located in the direction of the Orion constellation about 1600 light-years, its apparent size is slightly larger than the full moon.the monkey's head nebula or simply NGC 2175 is an emission nebula that emits in different wavelengths mainly in HA but also in Sii and Oiii.In the center is the star catalogued HD 42088 which emits a strong ultraviolet radiation that ionizes the gases in the vicinity.In addition to ultraviolet radiation, this star emits powerful stellar winds that shape the nebula's gas cluster, helping to create several pillars (visible in the image) that form a star nursery.Technical data:- Takahashi fsq 85 F/D 3.8- iOptron cem60 ec mount- Zwo asi 1600 mm cooled pro- 130x300s HA : 10h50min- 145x600s OIII : 24h10min- 30x3x60s RGB : 1h30 min- Total integration: 36 hours 30 minutes- DOF: 27x101x35- Date: January 2021- Location: Ben Slimane MAO Observatory, Morocco.

Copyright: Aziz Kaeouach