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Framed Pictures, Canvas Prints
Posters & Jigsaws since 2004

Stellar Gallery

Available as Prints and Gift Items

Choose from 975 pictures in our Stellar collection for your Wall Art or Photo Gift. All professionally made for Quick Shipping.


Orions Belt
Orions Belt
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The Plough asterism in Ursa Major
The Plough asterism in Ursa Major
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Orion nebula
Orion nebula
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Optical photograph of the constellation of Orion
Optical photograph of the constellation of Orion
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Orion constellation
Orion constellation
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Cassiopeia constellation
Cassiopeia constellation
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The constellation of the Southern Cross
The constellation of the Southern Cross
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Crab nebula (M1)
Crab nebula (M1)
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M16, The Eagle Nebula in Serpens
M16, The Eagle Nebula in Serpens
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Optical image of the constellation of Lyra
Optical image of the constellation of Lyra
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Supernova explosion, artwork
Supernova explosion, artwork
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The majestic Sombrero Galaxy (Messier 104)
The majestic Sombrero Galaxy (Messier 104)
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Orion nebula Featured Image

Orion nebula

Orion nebula. Coloured composite infrared and visible light image of the Orion nebula M42. This emission nebula, a cloud of gas and dust in which starbirth takes place, is found in the constellation Orion, some 1500 light years from Earth. Glowing clouds of ionised hydrogen and sulphur gases are green, and cool clouds of polycyclic aromatic hydrocarbons are orange and red. The gases are ionised by radiation from the four young Trapezium stars at the core (centre left). The small orange dots are embryonic stars, growing as they accumulate dust and gas. M42's neighbour, the M43 nebula, can also be seen (pale blue, top left). Infrared data from the Spitzer Space Telescope, visible light data from the Hubble Space Telescope

© NASA/JPL-CALTECH/STSCI/SCIENCE PHOTO LIBRARY

Supernova in galaxy
Supernova in galaxy
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Gas pillar in the Eagle nebula
Gas pillar in the Eagle nebula
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The constellation of Orion
The constellation of Orion
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Constellation of Orion with halo effect
Constellation of Orion with halo effect
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Diagram showing the spectral class and luminosity of stars
Diagram showing the spectral class and luminosity of stars
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Art of Betelgeuse as supernova
Art of Betelgeuse as supernova
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Planetary nebula
Planetary nebula
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Andromeda Galaxy, UV image
Andromeda Galaxy, UV image
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Crab nebula, composite image
Crab nebula, composite image
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Constellation Canis Major with halo effect
Constellation Canis Major with halo effect
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18th century world map
18th century world map
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Optical image of the star Sirius
Optical image of the star Sirius
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Diagram showing the spectral class and luminosity of stars Featured Image

Diagram showing the spectral class and luminosity of stars

Diagram showing the spectral class and luminosity of stars. The diagram was named The Hertzsprung-Russell Diagram, or the H-R diagram for short. At the beginning of the 20th century two astronomers found that if stars were plotted on a diagram with their luminosity (brightness) on one axis, and their spectral class on the other, that stars formed three distinct groups. The largest group, the Main Sequence Stars, is where 90% of the stars are found. These stars are fusing hydrogen into helium in their cores. This group propagates diagonally from the upper left corner, down to the right corner. The group below the main sequence is the White Dwarfs, which is a group of small, earth-sized stellar remnants. The third group, which is found above the main sequence is that of the giants.
Stars appear on a specific place on the main sequence depending on their mass and age. The mass determines when it will leave the main sequence.The H-R diagram is a significant tool for astronomers, when it comes to understanding stellar evolution

© Fahad Sulehria/Stocktrek Images

Merope star and nebulosity
Merope star and nebulosity
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Scorpius constellation
Scorpius constellation
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Light echoes from exploding star
Light echoes from exploding star
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Helix nebula, HST image
Helix nebula, HST image
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Pleiades star cluster
Pleiades star cluster
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Scorpius constellation
Scorpius constellation
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Red dwarf star
Red dwarf star
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Helix nebula, planetary nebula
Helix nebula, planetary nebula
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Einstein ring caused by gravitational lensing
Einstein ring caused by gravitational lensing
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Snowflake
Snowflake
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Core of Omega Centauri globular cluster
Core of Omega Centauri globular cluster
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Aurora borealis and Milky Way above Fish Lake, Yukon, Canada
Aurora borealis and Milky Way above Fish Lake, Yukon, Canada
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Core of Omega Centauri globular cluster Featured Image

Core of Omega Centauri globular cluster

Core of Omega Centauri globular cluster (NGC 5139), Hubble Space Telescope image. Globular clusters are spherical clusters of very old stars, about 12 billion years old, that are tightly bound by gravity and orbit a dense central core. This cluster is the largest globular star cluster found orbiting the Milky Way. This image shows an area 50 light years across and containing around 2 million stars. The entire cluster is 150 light years across and contains some 10 million stars. Omega Centauri is around 18, 000 light years from Earth, in the constellation Centaurus. This image, based on optical and infrared light, was obtained in June 2002 with the Advanced Camera for Surveys

© Nasa/Esa/Hubble Heritage Team (stsci/Aura)/Science Photo Library

A spacial phenomenon in the cosmos
A spacial phenomenon in the cosmos
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Optical image of the stars of Orions belt
Optical image of the stars of Orions belt
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Antares/Rho Ophiuchi region
Antares/Rho Ophiuchi region
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Cygnus and Lyra constellations
Cygnus and Lyra constellations
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Optical photo of the star Sirius using star filter
Optical photo of the star Sirius using star filter
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Cygnus constellation
Cygnus constellation
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Planets around a black hole
Planets around a black hole
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The Plough in Ursa Major, optical image
The Plough in Ursa Major, optical image
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Catands Eye nebula
Catands Eye nebula
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A galactic light show in spiral galaxy NGC 4258
A galactic light show in spiral galaxy NGC 4258
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Star formation in the Tarantula Nebula
Star formation in the Tarantula Nebula
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Star Vega in the constellation of Lyra
Star Vega in the constellation of Lyra
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