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Framed Pictures, Canvas Prints
Posters & Jigsaws since 2004

Star Death Gallery

Available as Prints and Gift Items

Choose from 127 pictures in our Star Death collection for your Wall Art or Photo Gift. All professionally made for Quick Shipping.


Crab nebula (M1)
Crab nebula (M1)
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Supernova explosion, artwork
Supernova explosion, artwork
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Art of Betelgeuse as supernova
Art of Betelgeuse as supernova
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Light echoes from exploding star
Light echoes from exploding star
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Crab nebula, composite image
Crab nebula, composite image
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Planetary nebula
Planetary nebula
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Supernova in galaxy
Supernova in galaxy
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Helix nebula, HST image
Helix nebula, HST image
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Helix nebula, infrared Spitzer image
Helix nebula, infrared Spitzer image
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Einstein ring caused by gravitational lensing
Einstein ring caused by gravitational lensing
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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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Helix nebula, infrared Spitzer image Featured Print

Helix nebula, infrared Spitzer image

Helix nebula (NGC 7293), infrared Spitzer Space Telescope image. This is a planetary nebula, a series of shells of gas cast off by a dying star. The ejection of the star's outer layers exposes its hot core, whose radiation ionises the shells, causing them to glow. This image was taken at wavelengths of varying energy: high (blue), medium (green) and low (red). The gas in the central regions has been ionised more than the outer gas, which is shielded from the stellar core. The most highly ionised areas (cometary heads) are round the edge of the central void. Foreground and background stars are blue. The Helix nebula is 650 light years from Earth, in the constellation of Aquarius. Image data obtained by the IRAC sensor in October 2004

© NASA/JPL-CALTECH/J. HORA (HARVARD-SMITHSONIAN CfA)/SCIENCE PHOTO LIBRARY

Catands Eye nebula
Catands Eye nebula
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Planets around a black hole
Planets around a black hole
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Black hole
Black hole
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Gamma ray burst eruption
Gamma ray burst eruption
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Planetary nebula NGC 6826
Planetary nebula NGC 6826
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Supernova remnant IC 443, composite image
Supernova remnant IC 443, composite image
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The Cat eye Nebula seen from the Hubble Telescope
The Cat eye Nebula seen from the Hubble Telescope
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Infinity symbol and black hole
Infinity symbol and black hole
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Artwork depicting an accretion disc of a black hol
Artwork depicting an accretion disc of a black hol
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Artwork of an AM Herculis binary star
Artwork of an AM Herculis binary star
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Artwork of a gamma-ray burster
Artwork of a gamma-ray burster
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Evolution of supernova 1993J, 1993-2000
Evolution of supernova 1993J, 1993-2000
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Artwork of an AM Herculis binary star Featured Print

Artwork of an AM Herculis binary star

Polar binary star. Artwork of a binary star system known as a polar. Polars are short period variable stars which emit X-rays. They consist of a normal star (left) in mutual orbit with a white dwarf (right). Their periods of variation are typically around 2 hours, and correlate with the orbital period of the white dwarf. Their light is strongly polarised. The gravitational field of the white dwarf pulls material off the larger star, and the dwarf's strong magnetic field channels it towards its poles, as seen at lower right. This material emits X-rays as it nears the white dwarf. Polars are also known as AM Her stars, after the first such star to be discovered, AM Herculis

© MARK GARLICK/SCIENCE PHOTO LIBRARY

Discovery of supernova 1993J
Discovery of supernova 1993J
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Alien patterns on a neutron star, artwork
Alien patterns on a neutron star, artwork
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UFO in a black hole
UFO in a black hole
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White hole
White hole
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Supernova explosion, computer artwork
Supernova explosion, computer artwork
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Red giant seen from a planet, artwork
Red giant seen from a planet, artwork
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Computer artwork of a black holes gravity well
Computer artwork of a black holes gravity well
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Spirograph planetary nebula IC418
Spirograph planetary nebula IC418
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Artwork of double star system SS 433
Artwork of double star system SS 433
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Wolf-Rayet nebula
Wolf-Rayet nebula
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HST image of gas ring around supernova 1987a
HST image of gas ring around supernova 1987a
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Colour HST image of part of Cygnus Loop SNR
Colour HST image of part of Cygnus Loop SNR
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Wolf-Rayet nebula Featured Print

Wolf-Rayet nebula

Wolf-Rayet nebula. Optical image of the Wolf-Rayet nebula NGC 2359. Wolf-Rayet (WR) nebulae comprise gas ejected by a very hot central star (not seen), glowing as it is ionised by the star's radiation. The ejection of this gas, primarily hydrogen, exposes the inner parts of the star, composed of the products of the nuclear reactions which power it. The two main types of WR star contain helium and nitrogen (WN stars, such as this) or helium, carbon and oxygen (WC stars). WR stars may be a million times more luminous than the Sun, and lose mass 100 times faster than comparably luminous stars. NGC 2359 lies around 40, 000 light years from Earth in the constellation Canis Major

© CELESTIAL IMAGE CO./SCIENCE PHOTO LIBRARY

Ant planetary nebula
Ant planetary nebula
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Brown dwarf, computer artwork
Brown dwarf, computer artwork
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Black hole & red giant star
Black hole & red giant star
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Artwork showing a mechanism for gamma-ray bursts
Artwork showing a mechanism for gamma-ray bursts
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X-ray binary, artwork
X-ray binary, artwork
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Artwork of a brown dwarf star
Artwork of a brown dwarf star
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Planetary nebula NGC 7009
Planetary nebula NGC 7009
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Supernova remnant LMC N 49
Supernova remnant LMC N 49
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Supernova remnant IC 443
Supernova remnant IC 443
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Artists impression of brown dwarf star
Artists impression of brown dwarf star
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Supernova remnant Cassiopeia A, X-ray
Supernova remnant Cassiopeia A, X-ray
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SNR Vela Supernova remnant
SNR Vela Supernova remnant
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