Images

Emission Photos ❘ lookphotos

Comet C/2022 E3 (ZTF) passing Mars in the constellation of Taurus on the night of Feb 10,2023. Mars appears to be at the tip of a dark lane of interstellar dust in the Taurus Dark Clouds. The comet is showing its whitish dust tail and blue ion tail,as well as its cyan coma from diatomic carbon emission. The star cluster at left is NGC 1746.
13999415 - Comet C/2022 E3 (ZTF) passing Mars in the constellation of Taurus on the night of Feb 10,2023. Mars appears to be at the tip of a dark lane of interstellar dust in the Taurus Dark Clouds. The comet is showing its whitish dust tail and blue ion tail,as well as its cyan coma from diatomic carbon emission. The star cluster at left is NGC 1746.
This is a framing of the rich starfield in northern Sagittarius to southern Serpens that contains the bright Messier 24 star cloud at bottom (aka the Small Sagittarius Starcloud),the emission nebula Messier 17 aka the Swan or Omega Nebula at centre,and Messier 16 or Eagle Nebula at top.
13999237 - This is a framing of the rich starfield in northern Sagittarius to southern Serpens that contains the bright Messier 24 star cloud at bottom (aka the Small Sagittarius Starcloud),the emission nebula Messier 17 aka the Swan or Omega Nebula at centre,and Messier 16 or Eagle Nebula at top.
A rich starfield in the constellation of Vulpecula the Fox,in the Milky Way,with a mix of nebulosity. At bottom is the Coathanger asterism of stars,aka Collinder 399,or Brocchi's Cluster. At top left is the emission nebula NGC 6820. Other dark nebulas from the Lynds Dark Nebula catalogue populate the field. The blue glow above the Coathanger is reflection nebulosity which does not appear to have a catlogue number. A small reflection nebula around the blue stars at right is van den Burgh 126. The small round red emission nebula at lower left is Sharpless 2-82. The yellow star at top right is An
13998813 - A rich starfield in the constellation of Vulpecula the Fox,in the Milky Way,with a mix of nebulosity. At bottom is the Coathanger asterism of stars,aka Collinder 399,or Brocchi's Cluster. At top left is the emission nebula NGC 6820. Other dark nebulas from the Lynds Dark Nebula catalogue populate the field. The blue glow above the Coathanger is reflection nebulosity which does not appear to have a catlogue number. A small reflection nebula around the blue stars at right is van den Burgh 126. The small round red emission nebula at lower left is Sharpless 2-82. The yellow star at top right is An
This is a framing of an array of emission nebulas in Cygnus: the bright North America Nebula (NGC 7000) at right,and to the right of it,the Pelican Nebula (IC 5067/8). Those bright nebulas are set amid a complex of fainter nebulosity,notably the Clamshell Nebula at left,as it has become known recently,and catalogued as Sharpless 2-119. At bottom right is the curving Cygnus Arc,aka IC 5068. The small star cluster NGC 7044 is below the Clamshell.
13998611 - This is a framing of an array of emission nebulas in Cygnus: the bright North America Nebula (NGC 7000) at right,and to the right of it,the Pelican Nebula (IC 5067/8). Those bright nebulas are set amid a complex of fainter nebulosity,notably the Clamshell Nebula at left,as it has become known recently,and catalogued as Sharpless 2-119. At bottom right is the curving Cygnus Arc,aka IC 5068. The small star cluster NGC 7044 is below the Clamshell.
The infamous "Green" Comet C/2022 E3 (ZTF) passing by reddish Mars with both in the constellation of Taurus on the night of Feb 11,2023. The comet was 2° south of Mars this night. Mars was embedded in some of the dark obscuring dust clouds in Taurus,creating the dark patchy appearance to the background sky. The comet's coma glows cyan due to emission from diatomic carbon molecules,a common trait of comets. The dust tail and faint ion tail are just visible.
13998596 - The infamous "Green" Comet C/2022 E3 (ZTF) passing by reddish Mars with both in the constellation of Taurus on the night of Feb 11,2023. The comet was 2° south of Mars this night. Mars was embedded in some of the dark obscuring dust clouds in Taurus,creating the dark patchy appearance to the background sky. The comet's coma glows cyan due to emission from diatomic carbon molecules,a common trait of comets. The dust tail and faint ion tail are just visible.
This is a framing of the rich complex of nebulosity in and around the constellations of northern Cygnus and southern Cepheus, in a blend of "white light" images and images shot through a deep red hydrogen-alpha filter that isolates the red emission line from the gas clouds, bringing them out in much more detail than is otherwise possible.
13900257 - This is a framing of the rich complex of nebulosity in and around the constellations of northern Cygnus and southern Cepheus, in a blend of "white light" images and images shot through a deep red hydrogen-alpha filter that isolates the red emission line from the gas clouds, bringing them out in much more detail than is otherwise possible.
This is a framing of the rich array of nebulas in central Auriga. The complex of star cluster Stock 8 and IC 417 is at upper left. The large nebula at lower centre is IC 410 with the star cluster NGC 1893 embedded in it. The large nebula at right is IC 405, aka the Flaming Star Nebula, with a mix of red emission and blue reflection nebulosity.
13899799 - This is a framing of the rich array of nebulas in central Auriga. The complex of star cluster Stock 8 and IC 417 is at upper left. The large nebula at lower centre is IC 410 with the star cluster NGC 1893 embedded in it. The large nebula at right is IC 405, aka the Flaming Star Nebula, with a mix of red emission and blue reflection nebulosity.
This is a framing of the rich array of nebulas in central Auriga. The complex of star cluster Stock 8 and IC 417 is at upper left. The large nebula at lower centre is IC 410 with the star cluster NGC 1893 embedded in it. The large nebula at right is IC 405, aka the Flaming Star Nebula, with a mix of red emission and blue reflection nebulosity.
13899593 - This is a framing of the rich array of nebulas in central Auriga. The complex of star cluster Stock 8 and IC 417 is at upper left. The large nebula at lower centre is IC 410 with the star cluster NGC 1893 embedded in it. The large nebula at right is IC 405, aka the Flaming Star Nebula, with a mix of red emission and blue reflection nebulosity.
A framing of the major areas of bright and dark nebulosity in Cygnus and Cepheus, showing pink emission nebulas contrasting with dark dusty regions in the Cygnus and into the Perseus arms of the Milky Way. Cepheus is at upper left; northern Cygnus is at right, with the bright Cygnus starcloud right of centre. The reddening (or yellowing) effects of interstellar dust in the spiral arms of the Milky Way is apparent.
13899552 - A framing of the major areas of bright and dark nebulosity in Cygnus and Cepheus, showing pink emission nebulas contrasting with dark dusty regions in the Cygnus and into the Perseus arms of the Milky Way. Cepheus is at upper left; northern Cygnus is at right, with the bright Cygnus starcloud right of centre. The reddening (or yellowing) effects of interstellar dust in the spiral arms of the Milky Way is apparent.
Bush crickets have very small wings, the pronotum resembles a saddle. The atrophied wings of Ephippiger species are unfit to flight and only used for the emission of sounds. This one has some parasitic mites on it
13848185 - Bush crickets have very small wings, the pronotum resembles a saddle. The atrophied wings of Ephippiger species are unfit to flight and only used for the emission of sounds. This one has some parasitic mites on it
Stunning constellation from the emission nebula Orion Nebula M42 in the night sky over Germany in February 2023
71433391 - Stunning constellation from the emission nebula Orion Nebula M42 in the night sky over Germany in February 2023
This is a rich region in the Milky Way in northern Sagittarius. with four Messier objects: The Small Sagittarius Starcloud,aka Messier 24,is at right of centre,flanked by: the pink Messier 17,the Swan or Omega Nebula,above; and the star cluster Messier 25 at lower left. Above M25 at upper left is the star cluster NGC 6645. Below M17 is the small star cluster Messier 18. The small but rich star cluster embedded in the Starcloud is NGC 6603. The nebulosity at bottom is IC 1283,a red emission nebula; and NGC 6589/90 and NGC 6595,both blue reflection nebulas. The dark nebula on the west (right) si
13998256 - This is a rich region in the Milky Way in northern Sagittarius. with four Messier objects: The Small Sagittarius Starcloud,aka Messier 24,is at right of centre,flanked by: the pink Messier 17,the Swan or Omega Nebula,above; and the star cluster Messier 25 at lower left. Above M25 at upper left is the star cluster NGC 6645. Below M17 is the small star cluster Messier 18. The small but rich star cluster embedded in the Starcloud is NGC 6603. The nebulosity at bottom is IC 1283,a red emission nebula; and NGC 6589/90 and NGC 6595,both blue reflection nebulas. The dark nebula on the west (right) si
The small constellation of Sagitta the Arrow, in the Milky Way. The small globular cluster, Messier 71, is between Gamma Sagittae and Delta Sagittae. Below M71 is the very sparse star cluster Harvard 20. The emission nebula Sharpless 2-84 is supposedly at centre but does not show up here except perhaps as a dim blue area of reflection nebulosity, though there is some faint red emission nebulosity at lower right.
13899970 - The small constellation of Sagitta the Arrow, in the Milky Way. The small globular cluster, Messier 71, is between Gamma Sagittae and Delta Sagittae. Below M71 is the very sparse star cluster Harvard 20. The emission nebula Sharpless 2-84 is supposedly at centre but does not show up here except perhaps as a dim blue area of reflection nebulosity, though there is some faint red emission nebulosity at lower right.
The Horsehead Nebula, B33, below the Belt of Orion and the star Alnitak, along with the bright Flame Nebula, NGC 2024, to the left of Alnitak. Many other bright reflection nebulas populate the field, such as NGC 2023 just left of the Horsehead itself. The quintuple star system Sigma Orionis is right of the Horsehead. The dark Horsehead is set against the bright streak of the emission nebula IC 434.
13899384 - The Horsehead Nebula, B33, below the Belt of Orion and the star Alnitak, along with the bright Flame Nebula, NGC 2024, to the left of Alnitak. Many other bright reflection nebulas populate the field, such as NGC 2023 just left of the Horsehead itself. The quintuple star system Sigma Orionis is right of the Horsehead. The dark Horsehead is set against the bright streak of the emission nebula IC 434.
The large emission nebula IC 1805 in Cassiopeia, aka the Heart Nebula. The round nebula at top right is NGC 896. The large loose star cluster at centre is Mel 15; the star cluster at left is NGC 1027. The small cluster below NGC 896 is Tombaugh 4.
13897628 - The large emission nebula IC 1805 in Cassiopeia, aka the Heart Nebula. The round nebula at top right is NGC 896. The large loose star cluster at centre is Mel 15; the star cluster at left is NGC 1027. The small cluster below NGC 896 is Tombaugh 4.
A subtle and pastel aurora borealis (Northern Lights) in the northeast, above a prairie meadow at "Lone Tree Hill". The foreground and sky are lit by a bright waxing gibbous Moon, a day before Full, shining in the south. This was just after midnight on July 11/12, 2022. The auroral curtains exhibit the usual green band and rays, though with shades of green visible, perhaps from hydrogen-beta proton emission as well as oxygen electron emission, but also upper altitude reds and purples and a faint blue tint at the very tops where the aurora is lit by the Sun. The aurora was never bright this nig
13900221 - A subtle and pastel aurora borealis (Northern Lights) in the northeast, above a prairie meadow at "Lone Tree Hill". The foreground and sky are lit by a bright waxing gibbous Moon, a day before Full, shining in the south. This was just after midnight on July 11/12, 2022. The auroral curtains exhibit the usual green band and rays, though with shades of green visible, perhaps from hydrogen-beta proton emission as well as oxygen electron emission, but also upper altitude reds and purples and a faint blue tint at the very tops where the aurora is lit by the Sun. The aurora was never bright this nig
The spectacular field of Messier 8 and 20 emission and reflection nebulas in Sagittarius, with M8, aka the Lagoon Nebula below, and M20, the Trifid Nebula, above, all set in the rich starfields of the Milky Way. The diffuse nebula left of M8 is NGC 6559. Two globular clusters, NGC 6544 and NGC 6553, sit below and to the left (east) of M8. The Messier open cluster, M21, sits above M20.
13899923 - The spectacular field of Messier 8 and 20 emission and reflection nebulas in Sagittarius, with M8, aka the Lagoon Nebula below, and M20, the Trifid Nebula, above, all set in the rich starfields of the Milky Way. The diffuse nebula left of M8 is NGC 6559. Two globular clusters, NGC 6544 and NGC 6553, sit below and to the left (east) of M8. The Messier open cluster, M21, sits above M20.
This is the field in Vulpecula the Fox that contains the famous planetary nebula, the Dumbbell Nebula aka Messier 27, at left, but also the faint emission nebulas NGC 6820 at right and Sharpless 2-88 above it. The small star cluster below centre is NGC 6830. A small star cluster, NGC 6823, lies embedded in NGC 6820. The field is yellowed by the interstellar dust reddening distant objects.
13899801 - This is the field in Vulpecula the Fox that contains the famous planetary nebula, the Dumbbell Nebula aka Messier 27, at left, but also the faint emission nebulas NGC 6820 at right and Sharpless 2-88 above it. The small star cluster below centre is NGC 6830. A small star cluster, NGC 6823, lies embedded in NGC 6820. The field is yellowed by the interstellar dust reddening distant objects.
The wonderful open star clusrter NGC 6124 in Scorpius amid a field of dark nebulas and on the edge of a bright star cloud with red emission nebulosity. I call this the Dark River Cluster.
13899037 - The wonderful open star clusrter NGC 6124 in Scorpius amid a field of dark nebulas and on the edge of a bright star cloud with red emission nebulosity. I call this the Dark River Cluster.
The complex area of clusters and nebulosity in central Auriga, including: M38 the Starfish Cluster and its smaller companion cluster NGC 1907; the emission/reflection nebulas NGC 1931, IC 417, IC 410 and IC 405 (from right to left here). Magenta and cyan (from emission and reflection components) IC 405 at right is the Flaming Star Nebula. Between IC 405 and IC 410 is the asterism known as The Little Fish.
13898788 - The complex area of clusters and nebulosity in central Auriga, including: M38 the Starfish Cluster and its smaller companion cluster NGC 1907; the emission/reflection nebulas NGC 1931, IC 417, IC 410 and IC 405 (from right to left here). Magenta and cyan (from emission and reflection components) IC 405 at right is the Flaming Star Nebula. Between IC 405 and IC 410 is the asterism known as The Little Fish.
A portrait of the infamous STEVE arc of hot flowing gas associated with an active aurora, here showing his distinctive pink colour and the fleeting appearance of the green picket fence fingers that often show up hanging down from the main arc. On this night the green fingers lasted no more than two minutes. STEVE = Strong Thermal Emission Velocity Enhancement, and is a river of hot gas flowing east to west equatorward of the main aurora band. STEVE appeared after the main Kp5-level aurora died down in activity to the north, typical behaviour for STEVE. He was visible for only 35 to 40 minutes,
13898370 - A portrait of the infamous STEVE arc of hot flowing gas associated with an active aurora, here showing his distinctive pink colour and the fleeting appearance of the green picket fence fingers that often show up hanging down from the main arc. On this night the green fingers lasted no more than two minutes. STEVE = Strong Thermal Emission Velocity Enhancement, and is a river of hot gas flowing east to west equatorward of the main aurora band. STEVE appeared after the main Kp5-level aurora died down in activity to the north, typical behaviour for STEVE. He was visible for only 35 to 40 minutes,
The area around the head of Scorpius, including the bright star Antares at lower left of centre and the dark lanes leading to the star Rho Ophiuchi. The area is filled with colourful nebulosity, including yellow and blue reflection nebulas and magenta emission nebulas. To the right of Antares is the globular cluster Messier 4. The field is similar to what binoculars would take in.
13897790 - The area around the head of Scorpius, including the bright star Antares at lower left of centre and the dark lanes leading to the star Rho Ophiuchi. The area is filled with colourful nebulosity, including yellow and blue reflection nebulas and magenta emission nebulas. To the right of Antares is the globular cluster Messier 4. The field is similar to what binoculars would take in.
A bush cricket on a Rosmary plant. The atrophied wings of Ephippiger species are unfit to flight and only used for the emission of sounds. This one has some parasitic mites on it
13846754 - A bush cricket on a Rosmary plant. The atrophied wings of Ephippiger species are unfit to flight and only used for the emission of sounds. This one has some parasitic mites on it
A framing of a field in southwestern Gemini rich in star clusters and nebulas. At top right is the rich star cluster Messier 35 and its small more distant companion cluster NGC 2158. At bottom right is the emission nebula NGC 2174 that is over the border in northern Orion. Above centre is the supernova remnant IC 443 arcing to the east of the orange star Propus or Eta Geminorum. The large diffuse nebula at left is IC 444 above the orange star Tejat Posterior or Mu Geminorum. The large,loose cluster Collinder 89 is embedded in IC 444. That region also has some blue reflection nebulosity,as does
13999418 - A framing of a field in southwestern Gemini rich in star clusters and nebulas. At top right is the rich star cluster Messier 35 and its small more distant companion cluster NGC 2158. At bottom right is the emission nebula NGC 2174 that is over the border in northern Orion. Above centre is the supernova remnant IC 443 arcing to the east of the orange star Propus or Eta Geminorum. The large diffuse nebula at left is IC 444 above the orange star Tejat Posterior or Mu Geminorum. The large,loose cluster Collinder 89 is embedded in IC 444. That region also has some blue reflection nebulosity,as does
This frames the region of northern Cygnus containing the bright emission nebulas,the North America and Pelican Nebulas,at bottom,and the dark nebula called LeGentil 3 or the Funnel Cloud Nebula at top,for its tornado-like shape. The latter is one of the darkest areas of the northern Milky Way,similar to the Coal Sack in the southern sky. The bright star at bottom right is Deneb. The small patch of emission nebulosity to the right of Deneb is Sharpless 2-112. Above it is Sh2-115. The large nebula at bottom left is the Clamshell Nebula or Sharpless 2-119. The curving nebula below the Pelican Neb
13998868 - This frames the region of northern Cygnus containing the bright emission nebulas,the North America and Pelican Nebulas,at bottom,and the dark nebula called LeGentil 3 or the Funnel Cloud Nebula at top,for its tornado-like shape. The latter is one of the darkest areas of the northern Milky Way,similar to the Coal Sack in the southern sky. The bright star at bottom right is Deneb. The small patch of emission nebulosity to the right of Deneb is Sharpless 2-112. Above it is Sh2-115. The large nebula at bottom left is the Clamshell Nebula or Sharpless 2-119. The curving nebula below the Pelican Neb
A panorama of the Kp5-level aurora on May 27, 2022, from home, with the aurora displaying prominent magenta rays, created by the red oxygen emission blending with illumination from blue scattered sunlight at high altitudes, common around the summer solstice when the high atmosphere is lit all night long. As a bonus, a dim STEVE arc is forming at far right, to the south of the main auroral oval where STEVE normally appears. STEVE faded, then returned to become more strong and visible across the sky from east to west as the main aurora to the north faded.
13900512 - A panorama of the Kp5-level aurora on May 27, 2022, from home, with the aurora displaying prominent magenta rays, created by the red oxygen emission blending with illumination from blue scattered sunlight at high altitudes, common around the summer solstice when the high atmosphere is lit all night long. As a bonus, a dim STEVE arc is forming at far right, to the south of the main auroral oval where STEVE normally appears. STEVE faded, then returned to become more strong and visible across the sky from east to west as the main aurora to the north faded.
A portrait of the infamous STEVE arc of hot flowing gas associated with an active aurora, here showing his distinctive pink colour and the fleeting appearance of the green picket fence fingers that often show up hanging down from the main arc. On this night the green fingers lasted no more than two minutes. STEVE = Strong Thermal Emission Velocity Enhancement, and is a river of hot gas flowing east to west equatorward of the main aurora band.
13899294 - A portrait of the infamous STEVE arc of hot flowing gas associated with an active aurora, here showing his distinctive pink colour and the fleeting appearance of the green picket fence fingers that often show up hanging down from the main arc. On this night the green fingers lasted no more than two minutes. STEVE = Strong Thermal Emission Velocity Enhancement, and is a river of hot gas flowing east to west equatorward of the main aurora band.
Emission nebulas in northern and central Cygnus, including the North America Nebula (NGC 7000) at lower left and the Gamma Cygni complex (IC 1318) at upper right. Deneb is the bright star at left, while Gamma Cygni itself is at upper right.
13898156 - Emission nebulas in northern and central Cygnus, including the North America Nebula (NGC 7000) at lower left and the Gamma Cygni complex (IC 1318) at upper right. Deneb is the bright star at left, while Gamma Cygni itself is at upper right.
The Belt of Orion with the Horsehead Nebula at botton, the dark nebula set in the bright emission nebula IC 434. The nebula at left of the Zeta Orionis (aka Alnitak) is the Flame Nebula, NGC 2024. The reflection nebula at upper left is the M78 complex with NGC 2071. The other Belt stars are Alnilan (centre) and Mintaka (upper right). The field contains a wealth of other blue reflection and red emission nebulas.
13897998 - The Belt of Orion with the Horsehead Nebula at botton, the dark nebula set in the bright emission nebula IC 434. The nebula at left of the Zeta Orionis (aka Alnitak) is the Flame Nebula, NGC 2024. The reflection nebula at upper left is the M78 complex with NGC 2071. The other Belt stars are Alnilan (centre) and Mintaka (upper right). The field contains a wealth of other blue reflection and red emission nebulas.
The aptly-named Coathanger Cluster,a more properly an asterism of stars in Vulpecula. A true star cluster,NGC 6802,lies at the left end of the coathanger arm. The field contains diffuse blue reflection nebulosity which appears to not have a catalogue number. The small round emission nebula at bottom is Sharpless 2-82. A very small round red nebula above the right end of the Coathanger is Sh2-83.
13999628 - The aptly-named Coathanger Cluster,a more properly an asterism of stars in Vulpecula. A true star cluster,NGC 6802,lies at the left end of the coathanger arm. The field contains diffuse blue reflection nebulosity which appears to not have a catalogue number. The small round emission nebula at bottom is Sharpless 2-82. A very small round red nebula above the right end of the Coathanger is Sh2-83.
This is a framing of an array of emission nebulas in Cygnus: the bright North America Nebula (NGC 7000) at right,and to the right of it,the Pelican Nebula (IC 5067/8). Those bright nebulas are set amid a complex of fainter nebulosity,notably the Clamshell Nebula at left,as it has become known recently,and catalogued as Sharpless 2-119. At bottom right is the curving Cygnus Arc,aka IC 5068. The small star cluster NGC 7044,yellowed by interstellar dust,is below the Clamshell. The nebulas are marked by lots of structure and radial streaks,perhaps from magnetic fields.
13999304 - This is a framing of an array of emission nebulas in Cygnus: the bright North America Nebula (NGC 7000) at right,and to the right of it,the Pelican Nebula (IC 5067/8). Those bright nebulas are set amid a complex of fainter nebulosity,notably the Clamshell Nebula at left,as it has become known recently,and catalogued as Sharpless 2-119. At bottom right is the curving Cygnus Arc,aka IC 5068. The small star cluster NGC 7044,yellowed by interstellar dust,is below the Clamshell. The nebulas are marked by lots of structure and radial streaks,perhaps from magnetic fields.
The open star cluster NGC 1528,at left,accompanied by the emission nebula NGC 1491,at right,aka the Fossil Footprint Nebula,both in Perseus. The very red star below NGC 1528 is SY Persei. The faint nebula at centre is unidentified – the nebulas Sharpless 2-209 and Sharpless 2-206 are in the area but their positions on the TriAtlas do not coincide with the nebula recorded here. Nor is it marked on any other atlas I was able to check. But the TriAtlas might plot the Sharpless nebulas incorrectly. But photos on-line label this object as Sh2-209. The bright star at bottom right is Lambda Persei.
13999258 - The open star cluster NGC 1528,at left,accompanied by the emission nebula NGC 1491,at right,aka the Fossil Footprint Nebula,both in Perseus. The very red star below NGC 1528 is SY Persei. The faint nebula at centre is unidentified – the nebulas Sharpless 2-209 and Sharpless 2-206 are in the area but their positions on the TriAtlas do not coincide with the nebula recorded here. Nor is it marked on any other atlas I was able to check. But the TriAtlas might plot the Sharpless nebulas incorrectly. But photos on-line label this object as Sh2-209. The bright star at bottom right is Lambda Persei.
This is the California Nebula,aka NGC 1499,in Perseus near the star Menkib,or Xi Persei,at bottom. While this is primarly an emission nebula,there is dust in the periphery forming some faint reflection nebulosity. The main nebula emits strongly in not only the red H-Alpha wavelength but also the blue-green H-Beta wavelength,thus the pink or magenta colour.
13999255 - This is the California Nebula,aka NGC 1499,in Perseus near the star Menkib,or Xi Persei,at bottom. While this is primarly an emission nebula,there is dust in the periphery forming some faint reflection nebulosity. The main nebula emits strongly in not only the red H-Alpha wavelength but also the blue-green H-Beta wavelength,thus the pink or magenta colour.
A widefield view of Orion's Belt and Sword showing the complex of nebulosity in the area. The three Belt stars are at top (L to R): Alnitak,Alnilam and Mintaka,with the dark Horsehead Nebula (B33) below Alnitak. Above Alnitak is the pinkish Flame Nebula,NGC 2024. At bottom are Messiers 42 and 43,making up the Orion Nebula,with the bluish Running Man Nebula above it,aka NGC 1973-5-7. Above it is the star cluster NGC 1981. Messier 78 is just on frame at upper left. Numerous other bits of emission and reflection nebulas populate the field amid a backdrop of faint emission nebulosity. The stars ar
13998672 - A widefield view of Orion's Belt and Sword showing the complex of nebulosity in the area. The three Belt stars are at top (L to R): Alnitak,Alnilam and Mintaka,with the dark Horsehead Nebula (B33) below Alnitak. Above Alnitak is the pinkish Flame Nebula,NGC 2024. At bottom are Messiers 42 and 43,making up the Orion Nebula,with the bluish Running Man Nebula above it,aka NGC 1973-5-7. Above it is the star cluster NGC 1981. Messier 78 is just on frame at upper left. Numerous other bits of emission and reflection nebulas populate the field amid a backdrop of faint emission nebulosity. The stars ar
A framing of the major areas of bright and dark nebulosity in Cygnus, showing pink emission nebulas contrasting with dark dusty regions in the Cygnus arm of the Milky Way. The main area of the bright Cygnus Starcloud is at upper right.
13900307 - A framing of the major areas of bright and dark nebulosity in Cygnus, showing pink emission nebulas contrasting with dark dusty regions in the Cygnus arm of the Milky Way. The main area of the bright Cygnus Starcloud is at upper right.
The False Comet Cluster area of southern Scorpius, which includes the open cluster NGC 6231 and emission nebula IC 4628, and open cluster NGC 6242 at top. This is a superb binocular field.
13900199 - The False Comet Cluster area of southern Scorpius, which includes the open cluster NGC 6231 and emission nebula IC 4628, and open cluster NGC 6242 at top. This is a superb binocular field.
The colourful region around Antares in Scorpius, the yellow star at centre. To the right is the globular cluster Messier 4. Above right of Antares is the smaller globular NGC 6144. Above are the nebulas associated with Rho Ophiuchi. The area is filled with reflection (yellow and blue) and emission nebulas (red and pink). The field simulates a binocular field.
13900192 - The colourful region around Antares in Scorpius, the yellow star at centre. To the right is the globular cluster Messier 4. Above right of Antares is the smaller globular NGC 6144. Above are the nebulas associated with Rho Ophiuchi. The area is filled with reflection (yellow and blue) and emission nebulas (red and pink). The field simulates a binocular field.
This is a framing of the rich complex of nebulosity in and around the constellation of Cygnus, in a blend of "white light" images and images shot through a deep red hydrogen-alpha filter that isolates the red emission line from the gas clouds, bringing them out in much more detail than is otherwise possible.
13899816 - This is a framing of the rich complex of nebulosity in and around the constellation of Cygnus, in a blend of "white light" images and images shot through a deep red hydrogen-alpha filter that isolates the red emission line from the gas clouds, bringing them out in much more detail than is otherwise possible.
The large emission nebula IC 1396 in Cepheus with the orange “Garnet Star” at top, and the Elephant Trunk Nebula, van den Bergh 142, at bottom as a dark lane protruding into the emission nebula.
13899543 - The large emission nebula IC 1396 in Cepheus with the orange “Garnet Star” at top, and the Elephant Trunk Nebula, van den Bergh 142, at bottom as a dark lane protruding into the emission nebula.
This is a portrait of the southern region of Cepheus the King that takes in the red emission nebulas in the constellation. The area is also laced with dark lanes of dust.
13899241 - This is a portrait of the southern region of Cepheus the King that takes in the red emission nebulas in the constellation. The area is also laced with dark lanes of dust.
The Rosette Nebula (aka NGC 2237) in Monoceros, an emission nebula and site of star formation in the Orion Arm of the Milky Way. The star cluster at the centre of the nebula is NGC 2244.
13899200 - The Rosette Nebula (aka NGC 2237) in Monoceros, an emission nebula and site of star formation in the Orion Arm of the Milky Way. The star cluster at the centre of the nebula is NGC 2244.
The Belt and Sword region of Orion, with the Orion Nebula, Messiesr 42 and 43, at bottom. Below the left star of the Belt, Alnitak, is the famous Horsehead Nebula, while above it is NGC 2024, aka the Flame Nebula. At very top left is Messier 78, while part of Barnard’s Loop arc across the field at left. The field is filled with other faint red emission and blue reflection nebulas. The large loose open cluster Collinder 70 surrounds the middle star of the Belt, Alnilam.
13898929 - The Belt and Sword region of Orion, with the Orion Nebula, Messiesr 42 and 43, at bottom. Below the left star of the Belt, Alnitak, is the famous Horsehead Nebula, while above it is NGC 2024, aka the Flame Nebula. At very top left is Messier 78, while part of Barnard’s Loop arc across the field at left. The field is filled with other faint red emission and blue reflection nebulas. The large loose open cluster Collinder 70 surrounds the middle star of the Belt, Alnilam.
The appearance of the infamous STEVE glowing arc south of the main auroral curtains, on May 27-28, 2022 from home in southern Alberta. This was early on about 11:53 pm MDT as STEVE appeared in his classic mauve colour in the east. STEVE = Strong Thermal Emission Velocity Enhancement, created by hot gas flowing east to west south of the main aurora during an active display. It was Kp5 this night. The main aurora has some subtle blue rays within it at left.
13898108 - The appearance of the infamous STEVE glowing arc south of the main auroral curtains, on May 27-28, 2022 from home in southern Alberta. This was early on about 11:53 pm MDT as STEVE appeared in his classic mauve colour in the east. STEVE = Strong Thermal Emission Velocity Enhancement, created by hot gas flowing east to west south of the main aurora during an active display. It was Kp5 this night. The main aurora has some subtle blue rays within it at left.
This is a portrait of Cassiopeia the Queen that takes in the red emission nebulas in the constellation as well as recording some of the larger star clusters. The area is also laced with dark lanes of dust.
13897883 - This is a portrait of Cassiopeia the Queen that takes in the red emission nebulas in the constellation as well as recording some of the larger star clusters. The area is also laced with dark lanes of dust.
A framing of the northern winter sky constellation of Gemini. the Twins The Messier star cluster M35 is at right,along with the emission nebulas IC 443 and NGC 2174. The twin stars of Castor (top) and Pollux are at left,but showing their colour difference here. The Milky Way runs down the right side of the frame making this area much brighter and richer than the sky at left.
13999153 - A framing of the northern winter sky constellation of Gemini. the Twins The Messier star cluster M35 is at right,along with the emission nebulas IC 443 and NGC 2174. The twin stars of Castor (top) and Pollux are at left,but showing their colour difference here. The Milky Way runs down the right side of the frame making this area much brighter and richer than the sky at left.
This is a framing of the main area of central Auriga filled with an array of Messier star clusters and faint IC emission nebulas.
13999053 - This is a framing of the main area of central Auriga filled with an array of Messier star clusters and faint IC emission nebulas.
The Veil Nebula complex in Cygnus,aka the Cygnus Loop or Cirrus Nebula. This is a remnant of a supernova explosion that occured 5000 to 8000 years ago. It features a mix of red hydrogen-alpha and cyan oxygen III emission for a colourful complex of lacy filaments. The components have the catalogue numbers of NGC 6992-5 (eastern component at left) and NGC 6960 (western component at right,through the star 52 Cygni),and NGC 6974 for the middle area at top called Pickering's Triangle.
13998977 - The Veil Nebula complex in Cygnus,aka the Cygnus Loop or Cirrus Nebula. This is a remnant of a supernova explosion that occured 5000 to 8000 years ago. It features a mix of red hydrogen-alpha and cyan oxygen III emission for a colourful complex of lacy filaments. The components have the catalogue numbers of NGC 6992-5 (eastern component at left) and NGC 6960 (western component at right,through the star 52 Cygni),and NGC 6974 for the middle area at top called Pickering's Triangle.
This is the region of the Milky Way that extends from southern Cygnus at top down into Vulpecula and Sagitta at bottom. Below centre is the Coathanger asterism,aka Brocchi's Cluster or Cr399. Above it is the blue reflection nebula Sharpless 2-83. The magenta emission nebula above and to the left is NGC 6820. A small red nebula above it is Sharpless 2-88. The bright star at upper right is Albireo in Cygnus.
13998294 - This is the region of the Milky Way that extends from southern Cygnus at top down into Vulpecula and Sagitta at bottom. Below centre is the Coathanger asterism,aka Brocchi's Cluster or Cr399. Above it is the blue reflection nebula Sharpless 2-83. The magenta emission nebula above and to the left is NGC 6820. A small red nebula above it is Sharpless 2-88. The bright star at upper right is Albireo in Cygnus.
The amazing area of the southern Milky Way in Carina and Crux, the brightest part of the Milky Way after the galactic core region. At right is the Carina Nebula, with the Southern Pleiades cluster, IC 2602, below it. The Football Cluster, NGC 3532, is at upper left of the Carina Nebula. At centre is the region of Lambda Centauri, with the star cluster NGC 3766, the Pearl Cluster, above the emission nebulosity. At left is the Southern Cross, with the dark Coal Sack at bottom left of the Cross, with thin tendrils extending to the right. To the left of Alpha Cruxis at the bottom of the Cross is t
13900602 - The amazing area of the southern Milky Way in Carina and Crux, the brightest part of the Milky Way after the galactic core region. At right is the Carina Nebula, with the Southern Pleiades cluster, IC 2602, below it. The Football Cluster, NGC 3532, is at upper left of the Carina Nebula. At centre is the region of Lambda Centauri, with the star cluster NGC 3766, the Pearl Cluster, above the emission nebulosity. At left is the Southern Cross, with the dark Coal Sack at bottom left of the Cross, with thin tendrils extending to the right. To the left of Alpha Cruxis at the bottom of the Cross is t
The colourful region in and around the Coathanger asterism in Vulpecula the Fox. The grouping is not a star cluster per se, though it is catalogued as one, Collinder 399. It is also known as Brocchi's Cluster. A true star cluster, NGC 6802, is located at the east (left) end of the Coathanger, as the small clump of stars. The area is also rich in faint nebulosity, notably: the Sharpless 2-83 reflection nebula complex above the Coathanger, and the small, round Sharpless 2-82 emission and reflection nebula below the Coathanger. The large area of red emission nebula at bottom right is not catalogu
13899982 - The colourful region in and around the Coathanger asterism in Vulpecula the Fox. The grouping is not a star cluster per se, though it is catalogued as one, Collinder 399. It is also known as Brocchi's Cluster. A true star cluster, NGC 6802, is located at the east (left) end of the Coathanger, as the small clump of stars. The area is also rich in faint nebulosity, notably: the Sharpless 2-83 reflection nebula complex above the Coathanger, and the small, round Sharpless 2-82 emission and reflection nebula below the Coathanger. The large area of red emission nebula at bottom right is not catalogu
The colourful region around yellow Antares (bottom) in Scorpius and blue Rho Ophiuchi (top) in Ophiuchus. The nebulas are largely reflection nebulas, taking on the colour of the stars embedded in the nebulas. However, the field also contains a lot of emission nebulosity, hydrogen gas glowing red and magenta. Plus there are fingers of brown dark dusty nebulosity. It is one of the most colourful regions of the sky.
13899016 - The colourful region around yellow Antares (bottom) in Scorpius and blue Rho Ophiuchi (top) in Ophiuchus. The nebulas are largely reflection nebulas, taking on the colour of the stars embedded in the nebulas. However, the field also contains a lot of emission nebulosity, hydrogen gas glowing red and magenta. Plus there are fingers of brown dark dusty nebulosity. It is one of the most colourful regions of the sky.
Open cluster pair of NGC 2451 (right), a bright loose cluster, and NGC 2477 (left), a fainter but very rich open cluster. The field is also filled with faint emission nebulosity. Taken from Timor Cottage, Coonabarabran, NSW, Australia, December 12, 2010. This is a stack of 5 x 6 minute exposures at ISO 1600 with Canon 5D MkII camera on 105mm Astro-Physics Traveler apo refractor at f/5.8 with 6x7 field flattener.
13898239 - Open cluster pair of NGC 2451 (right), a bright loose cluster, and NGC 2477 (left), a fainter but very rich open cluster. The field is also filled with faint emission nebulosity. Taken from Timor Cottage, Coonabarabran, NSW, Australia, December 12, 2010. This is a stack of 5 x 6 minute exposures at ISO 1600 with Canon 5D MkII camera on 105mm Astro-Physics Traveler apo refractor at f/5.8 with 6x7 field flattener.
A portrait of the infamous STEVE arc of hot flowing gas associated with an active aurora, here showing his distinctive pink colour and the fleeting appearance of the green picket fence fingers that often show up hanging down from the main arc. On this night the green fingers lasted no more than two minutes. STEVE = Strong Thermal Emission Velocity Enhancement, and is a river of hot gas flowing east to west equatorward of the main aurora band. STEVE appeared after the main Kp5-level aurora died down in activity to the north, typical behaviour for STEVE. He was visible for only 35 to 40 minutes,
13897598 - A portrait of the infamous STEVE arc of hot flowing gas associated with an active aurora, here showing his distinctive pink colour and the fleeting appearance of the green picket fence fingers that often show up hanging down from the main arc. On this night the green fingers lasted no more than two minutes. STEVE = Strong Thermal Emission Velocity Enhancement, and is a river of hot gas flowing east to west equatorward of the main aurora band. STEVE appeared after the main Kp5-level aurora died down in activity to the north, typical behaviour for STEVE. He was visible for only 35 to 40 minutes,