So you have observed the Messier and Caldwell objects and want to know what other wonders are out there, the Herschel 400 would be a good start, but if you are after inspiration why not look at what others are observing by having a browse below.
The latest stunning image of the Veil Nebula by member Neil Webster. Updated with another 3 hours worth of imaging grabbed on the night of the 21st Nov 2022.
Neil said ”I finally managed to get enough data to start to show the incredible subtle details in this object. This was processed from 5 hrs of data amassed over 3 evenings.”
The Veil Nebula is a diffuse nebula located in the northern constellation Cygnus, the Swan. It is the expanding remains of a massive star that exploded about 8,000 years ago.
Called the Veil Nebula, the debris is one of the best-known supernova remnants, deriving its name from its delicate, draped filamentary structures. The entire nebula is 110 light-years across, covering six full moons on the sky as seen from Earth.
It lies a few degrees to the south of the star Epsilon Cygni, also known as Aljanah.
Aljanah is one of the stars of the Northern Cross and marks the right wing of the celestial Swan.
The Veil Nebula is also known as Witch’s Broom Nebula, Bridal Veil Nebula, Cirrus Nebula or Filamentary Nebula. It is located approximately 1,470 light years from Earth.
The Veil Nebula has three main parts: the Eastern Veil, the Western Veil, and Fleming’s Triangle (Pickering’s Triangle). It has the designations NGC 6960, NGC 6992, NGC 6995, NGC 6974 and NGC 6979 in the New General Catalogue. The southernmost part of the Eastern Veil Nebula is assigned the catalogue designation IC 1340.
To see a more detailed view of this image check out Neil’s Flickr page at https://www.flickr.com/photos/137388222@N05/52515415329/
Member Neil Webster has been busy……….
This is the latest stunning deep sky image by Neil of Hydrogen Alpha nebulosity surrounding the star Gamma Cygni (Sadr) taken on the 20th October 2022.
Neil acquired the image using a AA 115mmAPO, EQ6 R, ZWO ASI294MC Pro, Optolong L enhance filter, Orion 50mm Guide Scope and ZWO ASI290MM.
47 x 240s lights, 12 x Darks, 35 x flats/bias.
APT, PHD, Nebulosity & Photoshop.
To see a higher resolution photo of this image check out Neil’s Flickr page at https://www.flickr.com/photos/137388222@N05/52443297014/
Sadr, Gamma Cygni (γ Cyg) is a yellow-white supergiant star located in the constellation Cygnus. Sadr is the constellation’s second brightest star after Deneb with an apparent magnitude of 2.23. It is the star forming the intersection of an asterism of five stars called the Northern Cross an asterism that dominates the summer sky in the northern hemisphere. Sadr lies in a rich field of the Milky Way and is surrounded by the diffuse emission nebula IC1318 also known as the Gamma Cygni Nebula or Sadr Region.
Plus hot off the press today – the latest music video created by Neil titled Pickering’s Triangle. Take a trip round Pickering’s Triangle in Cygnus imaged by Neil to a pulsey soundtrack and seriously wayward piano near the end.
Member Neil Webster has been busy and produced this wonderful image of NGC 6823 & SH-2-86 in the constellation Vulpecula plus a new music video.
SH-2-86 is an H Alpha emitting region (red glow) from the Sharpless Catalogue and NGC 6823 is a small open cluster just above the central dark spike in the image.
Published by Stewart Sharpless in 1959, the SH2 catalogue lists 312 emission nebulae, planetary nebulae and supernova remnants visible in the northern hemisphere. Despite overlapping with deep-sky objects in the Messier and NGC catalogs that are visible to the unaided eye, SH2 is primarily composed of obscure, dim nebulae which can only be revealed through astrophotography.
Neil acquired the image on the 2nd October 2022 using a AA 115mm APO, EQ6-R, ZWO ASI294MC Pro, L EnHance filter, Orion 50mm Guide Scope, ZWO ASI290MM
90 x 140s Lights, 15 x Darks, 30 x Flats/Bias.
Nebulosity, Photoshop (Camera Raw)
To view a higher resolution image visit Neil’s Flickr page at https://www.flickr.com/photos/137388222@N05/
Then sit back and relax and take a tour of the Jellyfish Nebula (IC 443) in the constellation Gemini imaged by Neil whilst listening to a piano based soundtrack. To do so click on the following link The Jellyfish Nebula IC 443 – YouTube where you find Neil’s latest music video.
An absolutely stunning image by member Kevin Langford of The North America Nebula (NGC 7000 or Caldwell 20). The North America Nebula is an emission nebula in the constellation Cygnus, close to the star Deneb.
ES 102ED APO, 0.7x focal reducer corrector, EQ5 Pro
ZWO ASI071, Orion MMAG,L-eNhance filter
1 1/2 Hrs of exposures
To see a higher resolution photo of the image check out Kevin’s Flickr page at www.flickr.com/photos/77708720@N08/52383552499/
An absolutely fantastic widefield image of the Veil Nebula taken by member Kevin Langford on the 12th August 2022 from Bexley, Kent. The image was acquired using an ES 102ED APO, 0.7x focal reducer corrector, EQ5 Pro, ZWO ASI071, Orion MMAG and L-eNhance filter.
The 3 hours of exposure was then processed in photoshop.
To see a higher resolution photo of this image click on the following link to be taken to Kevin’s flickr page https://www.flickr.com/photos/77708720@N08/52321231907/
An awesome capture by Simon Dawes of a Supernova called SN2022hrs in NGC 4647.
NGC 4647 is an intermediate spiral galaxy in the constellation Virgo. Supernova SN2022hrs was discovered in the galaxy NGC4647 on the 16th April 2022 by astronomer Koichi Itagaki. NGC 4647 is 63 million light years away, so, this star exploded 63 million years ago and it took that long for the light of the explosion to reach us.
Messier 60 (NGC 4649), an elliptical galaxy, is also in the image and it is in the centre of the frame and NGC 4647 is slightly down and to the right of it. SN2022hrs looks like a bright star in front of the galaxy but it is actually an exploding star within the galaxy.
Planet Mercury at the bottom & M45 (The Pleiades) above right taken on the 28th April 2022 at 2015 local time MST in Arizona, USA. Richard acquired this splendid image using a Canon 6D, 400mm tele f2.8, ISO 800 and 12 second exp.
Dr. Mike Rushton took advantage of some clear skies recently (25th April 2022) and took these 3 super deepsky images using his eVscope of Messier 13, Messier 51 and the Bow Tie Nebula.
Messier 13 (M13) also designated NGC 6205 and also called the Great Globular Cluster in Hercules and the Hercules Globular Cluster, is a globular cluster of a several hundred thousand stars in the constellation of Hercules.
Messier 51, known as The Whirlpool Galaxy and as Messier 51a, M51a, and NGC 5194, is a spiral galaxy found in the constellation Canes Venatici, M51 was the first galaxy to be classified as a spiral galaxy and is 31 million light-years away from Earth.
The Bow Tie Nebula also designated NGC 40 and Caldwell 2 is a planetary nebula discovered by William Herschel in 1788. It is composed of hot gas around a dying star. The nebula gets its name from the fact it has an intriguing bow-tie shape.
Supernova SN 2022ewj in galaxy NGC 3367 taken by Simon Dawes on the 23 Mar 2022 from Bexleyheath.
Details of how Simon acquired this superb image is on the photo.
NGC 3367 is a barred spiral galaxy located in the constellation Leo. It is located at a distance of around 120 million light years from Earth, which, given its apparent dimensions, means that NGC 3367 is about 85,000 light years across. The galaxy was discovered by William Herschel on March 19, 1784
Mag 15.5, SN 2022ewj was discovered on the 19th March 2022 by Koichi Itagaki and is a type II Supernova. This is the 6th supernova to be observed in NGC3367 over the last 30 odd years.
Not the easiest of objects to image from the London Borough of Bexley!
All images are copyright. Permission must be sought to from the image owner to the use of any of these images.