Pluto Gallery
Available as Framed Prints, Photos, Wall Art and Gift Items
Choose from 72 pictures in our Pluto collection for your Wall Art or Photo Gift. Popular choices include Framed Prints, Canvas Prints, Posters and Jigsaw Puzzles. All professionally made for quick delivery.
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Featured Pluto Print
Jupiter and Io, New Horizons image
Jupiter and Io. Montage of images of Jupiter (left) and its moon Io (right), obtained by the New Horizons spacecraft in February and March 2007 as it passed Jupiter on its way to Pluto. The image of Jupiter was obtained with its infrared spectrometer (LEISA). The different colours show high-altitude clouds (blue), and deeper clouds (red). The Great Red Spot (lower left) is blue and white. The Io image was obtained in approximate true colour with a long-range camera (LORRI) and a multispectral camera (MVIC). The red dot on the nightside of Io is an eruption of the Tvashtar volcano. The volcanic plume (blue) seen above the eruption is 330 kilometres high. Jupiter is the solar system's largest planet
© NASA/JHU/APL/SCIENCE PHOTO LIBRARY
Featured Pluto Print
Planets internal structures
Planets internal structures, and Pluto, computer artwork. Mercury, Mars and Venus consist of a large iron core (spherical), surrounded by a thick silicate mantle (yellow) covered in a surface crust. Earth consists of an inner core of solid iron and nickel (yellow) and a molten outer core (orange), surrounded by a mantle of highly viscous liquid (brown) covered by a surface crust. Jupiter and Saturn consist of a core of rock (spherical) surrounded by ice (mat grey). This is surrounded by a layer of liquid metallic hydrogen (grey) and liquid normal hydrogen (blue). Uranus and Neptune have a core of rock (spherical) surrounded by ice and liquid hydrogen (blue). Pluto has a dense rocky core (grey) surrounded by ice (black)
© CHRISTIAN DARKIN/SCIENCE PHOTO LIBRARY
Featured Pluto Print
Outer solar system formation
Outer solar system formation. Artwork showing the formation of the unusual orbits of bodies in the outer solar system. The inset shows three stages in the formation of the solar system. Early on (top) it is a disc of small bodies (planetesimals), which collide and accrete into gradually larger bodies. These accrete smaller ones until their orbital paths are nearly clear of debris (middle), but some large bodies do remain, and collisions (orange) still occur. Some smaller bodies are thrown out of the solar system by the gravity of larger bodies (lower right of middle stage). The result (bottom) is that some bodies, such as the dwarf planet Pluto, have highly eccentric orbits (yellow lines)
© HENNING DALHOFF / SCIENCE PHOTO LIBRARY
