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Astrophysical Gallery

Available as Prints and Gift Items

Choose from 773 pictures in our Astrophysical collection for your Wall Art or Photo Gift. All professionally made for Quick Shipping.


Pale Blue Dot, Voyager 1
Pale Blue Dot, Voyager 1
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Hubble Ultra Deep Field 2012
Hubble Ultra Deep Field 2012
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MAP microwave background
MAP microwave background
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1919 solar eclipse
1919 solar eclipse
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1919 solar eclipse
1919 solar eclipse
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Orion nebula
Orion nebula
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Pillars of Creation
Pillars of Creation
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Nebula Sh 2-106, HST image
Nebula Sh 2-106, HST image
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Gas pillars in the Eagle Nebula
Gas pillars in the Eagle Nebula
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Hubble Ultra Deep Field galaxies
Hubble Ultra Deep Field galaxies
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Cosmic microwave background
Cosmic microwave background
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Orions belt
Orions belt
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Pale Blue Dot, Voyager 1 Featured Image

Pale Blue Dot, Voyager 1

This unique narrow-angle color image is of the Earth, dubbed Pale Blue Dot, is a part of the first ever portrait of the solar system taken by Voyager 1. The spacecraft acquired a total of 60 frames for a mosaic of the solar system from a distance of more than 4 billion miles from Earth and about 32 degrees above the ecliptic. From Voyager's great distance Earth is a mere point of light, less than the size of a picture element even in the narrow-angle camera. Earth was a crescent only 0.12 pixel in size. Coincidentally, Earth lies right in the center of one of the scattered light rays resulting from taking the image so close to the sun. This blown-up image of the Earth was taken through three color filters -- violet, blue and green -- and recombined to produce the color image. The background features in the image are artifacts resulting from the magnification

© NASA/SCIENCE PHOTO LIBRARY

Sombrero galaxy (M104), HST image
Sombrero galaxy (M104), HST image
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Milky Way
Milky Way
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Antennae colliding galaxies, Hubble image
Antennae colliding galaxies, Hubble image
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Crab nebula (M1)
Crab nebula (M1)
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Orion nebula (M42)
Orion nebula (M42)
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Crab nebula, composite image
Crab nebula, composite image
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Moon rising over Earths horizon
Moon rising over Earths horizon
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Light echoes from exploding star
Light echoes from exploding star
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Supernova explosion, artwork
Supernova explosion, artwork
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Aurora over Antarctica, satellite image
Aurora over Antarctica, satellite image
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Saturn, Cassini image
Saturn, Cassini image
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Solar System, artwork
Solar System, artwork
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Aurora over Antarctica, satellite image Featured Image

Aurora over Antarctica, satellite image

Aurora over Antarctica, ultraviolet satellite image. Australia is at upper left. This is the aurora australis (green ring), the southern lights display. It is caused by interactions between charged particles from the Sun (the solar wind) and gas atoms and molecules about 100 kilometres above the Earth. On reaching Earth, the charged particles are drawn by Earth's magnetic field to the poles, where they collide with gas atoms and molecules, causing them to emit light. This display, on 11 September 2005, was caused by a large solar flare. The aurora image was obtained by NASA's IMAGE satellite, which carried out a five year study of Earth's magnetic field

© NASA/SCIENCE PHOTO LIBRARY

Interacting galaxies NGC 5257 and 5258
Interacting galaxies NGC 5257 and 5258
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Helix nebula, infrared Spitzer image
Helix nebula, infrared Spitzer image
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Mars, composite satellite images
Mars, composite satellite images
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Spiral galaxy M81, composite image
Spiral galaxy M81, composite image
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Kepler Mission space telescope, artwork
Kepler Mission space telescope, artwork
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Orbit of Sputnik 1, Soviet 1957 diagram
Orbit of Sputnik 1, Soviet 1957 diagram
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Interacting galaxies Arp 147, HST image
Interacting galaxies Arp 147, HST image
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Io and Jupiter, Cassini image
Io and Jupiter, Cassini image
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Ring Nebula M57, Hubble image C017/3725
Ring Nebula M57, Hubble image C017/3725
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Edwin Hubble, US astronomer C008/8831
Edwin Hubble, US astronomer C008/8831
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Cigar galaxy (M82), composite image
Cigar galaxy (M82), composite image
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Dark matter distribution
Dark matter distribution
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Dark matter distribution Featured Image

Dark matter distribution

Dark matter distribution. Image 3 of 4. Supercomputer simulation, known as the Millennium Run, showing the distribution of dark matter in the local universe. The frame is 63 megaparsecs (206 million light years) in distance across. Dark matter is a form of matter that cannot be detected by telescopes as it emits no radiation. It is thought that cold dark matter first formed after the Big Bang. This matter then collapsed under its own weight to form vast halos (bright yellow) which sucked in normal matter to form visible matter, such as galaxies. This simulation was created in 2005 by the Virgo Consortium of international scientists using supercomputers at the Max Planck Society, Germany. For complete sequence, see images R980/209 - R980/212

© VOLKER SPRINGEL/MAX PLANCK INSTITUTE FOR ASTROPHYSICS/SCIENCE PHOTO LIBRARY

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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Mauna Kea telescopes and Milky Way
Mauna Kea telescopes and Milky Way
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Halleys Comet, 1910
Halleys Comet, 1910
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Observing the Universe, conceptual image
Observing the Universe, conceptual image
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Helix nebula, HST image
Helix nebula, HST image
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Transit of Venus, 8th June 2004
Transit of Venus, 8th June 2004
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Alexander Friedman, Soviet cosmologist
Alexander Friedman, Soviet cosmologist
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Open star cluster NGC 3603, HST image
Open star cluster NGC 3603, HST image
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Milky way galaxy, artwork
Milky way galaxy, artwork
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Kitt Peak Observatory and Milky Way
Kitt Peak Observatory and Milky Way
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Time warp, conceptual image
Time warp, conceptual image
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