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Framed Pictures, Canvas Prints
Posters & Jigsaws since 2004

Astrophysics Gallery

Available as Prints and Gift Items

Choose from 922 pictures in our Astrophysics collection for your Wall Art or Photo Gift. All professionally made for Quick Shipping.


Orbit of Sputnik 1, Soviet 1957 diagram
Orbit of Sputnik 1, Soviet 1957 diagram
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Andromeda galaxy (M31) and Earths moon
Andromeda galaxy (M31) and Earths moon
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Planetary conjunction, optical image
Planetary conjunction, optical image
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Ring Nebula M57, Hubble image
Ring Nebula M57, Hubble image
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Underside of Arecibo radio telescope
Underside of Arecibo radio telescope
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Interacting galaxies NGC 5257 and 5258
Interacting galaxies NGC 5257 and 5258
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Supernova explosion, artwork
Supernova explosion, artwork
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Star birth in the early universe
Star birth in the early universe
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Quasar
Quasar
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Spiral galaxy M81, Hubble image
Spiral galaxy M81, Hubble image
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Nebula in M17
Nebula in M17
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Dark matter gravitational lensing
Dark matter gravitational lensing
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Spiral galaxy M81, Hubble image Featured Print

Spiral galaxy M81, Hubble image

Spiral galaxy M81, Hubble Space Telescope image.This was the sharpest image ever taken of M81 whenit was released in May 2007. The data werecollected between 2004 and 2006 by the AdvancedCamera for Surveys (ACS) on Hubble. Despite lying11.6 million light years away, individual starscan be identified, and numerous open starclusters, globular clusters and nebulae can beseen. M81 is the largest member of the M81 Group, one of the nearest groups of galaxies to our ownLocal Group (which includes our Milky Way and theAndromeda Galaxy). M81 is located in theconstellation Ursa Major. * The 70Mb hi-res file isa resized version of the original, which is 1Gb insize. Please contact SPL if you would like thefull size image *

© Nasa/Esa/Stsci/Science Photo Library

Diagram showing the spectral class and luminosity of stars
Diagram showing the spectral class and luminosity of stars
Stocktrek Images

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Edwin Hubble, US astronomer
Edwin Hubble, US astronomer
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Interacting galaxies
Interacting galaxies
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Cigar galaxy (M82), composite image
Cigar galaxy (M82), composite image
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Milky Way
Milky Way
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Dark matter distribution
Dark matter distribution
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Orion nebula (M42 and M43)
Orion nebula (M42 and M43)
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Aurora borealis and Moon
Aurora borealis and Moon
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Halleys Comet, 1910
Halleys Comet, 1910
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Whirlpool galaxy (M51)
Whirlpool galaxy (M51)
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Hubble Telescope
Hubble Telescope
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Rainbow over the dishes of the VLA radio telescope
Rainbow over the dishes of the VLA radio telescope
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Diagram showing the spectral class and luminosity of stars Featured Print

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

Bullet cluster (1E 0657-56)
Bullet cluster (1E 0657-56)
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Cartwheel galaxy, multi-wavelength image
Cartwheel galaxy, multi-wavelength image
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Core of Omega Centauri globular cluster
Core of Omega Centauri globular cluster
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Solar prominence
Solar prominence
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Open star cluster NGC 3603, HST image
Open star cluster NGC 3603, HST image
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Time warp, conceptual image
Time warp, conceptual image
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Antares/Rho Ophiuchi region
Antares/Rho Ophiuchi region
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Lovell Radio Telescope dish at Jodrell Bank
Lovell Radio Telescope dish at Jodrell Bank
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Red dwarf star
Red dwarf star
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Planetary nebula
Planetary nebula
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Albert Einstein, artwork
Albert Einstein, artwork
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Lovell radio telescope
Lovell radio telescope
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Antares/Rho Ophiuchi region Featured Print

Antares/Rho Ophiuchi region

Antares/Rho Ophiuchi region, optical image. Thiscolourful region lies in the constellationsScorpius and Ophiuchus. The blue area at upperright is the triplet star Rho Ophiuchi, embeddedin the reflection nebula IC 4604. This nebula doesnot emit light of its own, but reflects light fromthe star and appears blue due to blue light beingscattered more than red light. The large orb atlower left is the supergiant star Antares (AlphaScorpii), next to the yellow emission nebula IC4606. This nebula emits light due to its gas anddust clouds being ionised by radiation from thestars. At right is the star Sigma Scorpii with itspink emission nebula Ced 130, and at lower rightis the dense globular star cluster M4 (NGC 6121)

© Adam Block/Science Photo Library

Mauna Kea telescopes and Milky Way
Mauna Kea telescopes and Milky Way
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Helix nebula, planetary nebula
Helix nebula, planetary nebula
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Halo stars in Andromeda Galaxy
Halo stars in Andromeda Galaxy
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Trifid Nebula
Trifid Nebula
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Orion nebula
Orion nebula
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Comet with aurora
Comet with aurora
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Solar coronal loops, TRACE image
Solar coronal loops, TRACE image
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Mars, composite satellite images
Mars, composite satellite images
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Milky way galaxy, artwork
Milky way galaxy, artwork
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Kepler Mission space telescope, artwork
Kepler Mission space telescope, artwork
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Edge-on galaxy NGC 4565
Edge-on galaxy NGC 4565
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Catands Eye nebula
Catands Eye nebula
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