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Larry Larry

@deepskyvoyager

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Voyager of the deep sky
Nebulae | Galaxies | Cosmic clouds
Turning ancient starlight into images ✨

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The Lagoon

Messier 8 · NGC 6523
Lagoon Nebula
Distance: ~4,100 ly
Constellation: Sagittarius

One of the brightest star-forming regions visible to the naked eye under dark skies. A dark dust lane cuts through the glowing hydrogen, giving the lagoon its name. Inside sits the young cluster NGC 6530; ultraviolet light from its massive stars ionizes the gas and carves the clouds.

📸 @deepskyvoyager by @deepskyvoyager

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5 days ago

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10 days ago

IC 417 (The Spider Nebula)

IC 417, known as the Spider Nebula, is a vast emission nebula located in the constellation Auriga, approximately 7,000–10,000 light-years from Earth. It spans roughly 100 light-years and is composed primarily of glowing hydrogen gas, with interstellar dust woven throughout its complex structure.
At its heart lies Stock 8, a young open star cluster whose hot, massive stars illuminate and sculpt the surrounding clouds, triggering ongoing star formation. The intricate filaments and glowing arcs of IC 417 reveal a region where gas, dust, and newly born stars interact on an enormous cosmic scale.
IC 417 is part of the larger “Spider and the Fly” complex, together with the smaller nebula NGC 1931.
#astronomyphotography #astrophotography #zwoastro #apod_astronomia #deepskyphotography by @deepskyvoyager

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17 days ago

A very atmospheric nightscape combining the rugged texture of the Mediterranean coast with the intricate dust lanes and stellar richness of the Milky Way.
#astronomyphotography #milkyway_nightscapes #astrophotography #nightskyphotography #milkyway by @deepskyvoyager

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24 days ago

#astronomyphotography #milkywaychasers #milkyway_nightscapes #astrophotography #milkywayphotography by @deepskyvoyager

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a month ago

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#astronomyphotography #milkywaychasers #astrophotography #milkyway_nightscapes #milkywaypics by @deepskyvoyager

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a month ago

The Forsaken Nebula

IC 5068 is a faint H II emission region in the constellation Cygnus, located approximately 1,600 light-years from Earth and catalogued as LBN 328. The nebula consists mainly of ionized hydrogen, with prominent Hα emission and contributions from [O III] and [S II].
Its most distinctive feature is the intricate network of dark dust lanes and filaments crossing the glowing hydrogen clouds, creating a remarkably complex and three-dimensional appearance.
Often overshadowed by the nearby North America and Pelican Nebulae, IC 5068 is a faint and challenging target — but one that reveals extraordinary detail when captured with sufficient integration time.
#astrophotography_ #zwoastro #astrobackyard #apod_astronomia #deepskyastrophotography by @deepskyvoyager

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2 months ago

Sh2-132 is a large H II emission region located in the constellation of Cepheus, close to the border with Lacerta, at an estimated distance of approximately 10,000–12,000 light-years from Earth. The complex extends over roughly 250 light-years and lies within the Perseus Arm of the Milky Way.
The nebula is a highly structured mixture of ionized hydrogen, ionized oxygen, molecular gas and interstellar dust. Its complex morphology is shaped by the intense ultraviolet radiation and powerful stellar winds of massive stars, including the Wolf–Rayet systems WR 152 and WR 153ab. WR 153ab is a binary Wolf–Rayet system and is considered the principal stellar source associated with the ionized region.
The prominent Hα emission traces the extensive ionized hydrogen structures, while the much fainter O III emission reveals higher-ionization regions and intricate filamentary structures. Dense molecular clouds and dark dust lanes are embedded within the ionized gas, producing the characteristic contrast and three-dimensional appearance of the region.
This image presents a small section of the Sh2-132 complex, highlighting the interaction between ionized gas, higher-excitation regions and obscuring interstellar dust.

#zwoastro #deepskyastrophotography #apod_astronomia #astrophotography_ #astrobackyard by @deepskyvoyager

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2 months ago

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The Tulip Nebula (Sh2-101) is an emission nebula approximately 6,000 light-years away in the constellation Cygnus. This active star-forming region is energized by intense ultraviolet radiation from massive young stars, causing its hydrogen gas to glow brightly. The nebula is also located near the microquasar Cygnus X-1, one of the first confirmed stellar-mass black hole systems.

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NGC 6995 is the brightest eastern filament of the Veil Nebula, a supernova remnant located approximately 2,400 light-years away in the constellation Cygnus. It consists of shock-heated gas expanding from a stellar explosion that occurred roughly 10,000–20,000 years ago, revealing intricate filaments dominated by ionized oxygen and hydrogen emission.

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Crescent Nebula (NGC 6888) is an emission nebula located about 5,000 light-years away in the constellation Cygnus. Formed by the powerful stellar winds of the Wolf–Rayet star WR 136, it represents the interaction between fast winds from the evolved star and material ejected during earlier stages of its evolution, producing a complex shell rich in ionized hydrogen, oxygen, and sulfur.

#apod_astronomia #darksky #zwoastro #deepskyphotography #deepskyastrophotography by @deepskyvoyager

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3 months ago

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The Trifid Nebula (M20) is one of the Galaxy’s most remarkable stellar nurseries, where glowing hydrogen, blue reflection dust, and dark molecular clouds coexist in a single breathtaking region.

#trifidnebula #zwoastro #deepskyphotography #ngc6514 #deepspace by @deepskyvoyager

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3 months ago

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Far beyond the edge of human memory, the Crescent Nebula drifted through the silent darkness of space And somewhere inside that endless cloud of light, a lone star still watches,waiting for someone to listen

#zwoastro #crescentnebula #cignusconstellation #caldwell27 #ngc6888 by @deepskyvoyager

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5 months ago

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#deepskyphotography #milkywaychasers #milkywayphoto #milkyway_chasers #milkyway_nightscape_ by @deepskyvoyager

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5 months ago