Callisto Voyager / Galileo Image Mosaic Globe

Global Mosaic | Globe

The images used for the base of this globe were chosen from the best image quality and moderate resolution coverage supplied by Galileo SSI and Voyager 1 and 2 (Batson, 1987; Becker

Europa Voyager / Galileo Image Mosaic Globe

Globe

The images used for the base of this globe were chosen from coverage supplied by the Galileo solid-state imaging (SSI) camera and Voyager 1 and 2 spacecraft. The individual images were radiometrically

Ganymede Voyager Galileo Image Mosaic Globe

Global Mosaic | Globe

The images used for the base of this globe were chosen from coverage supplied by the Galileo solid-state imaging (SSI) camera and Voyager 1 and 2 spacecraft. The monochrome and color data

Io Voyager / Galileo Image Mosaic Globe

Global Mosaic | Globe

A global monochrome mosaic of the best resolution images from both Galileo and Voyager 1 was created that includes 51 Voyager 1 images with spatial resolutions sometimes exceeding the 1 km/pixel scale

Mars Global Surveyor MOLA Globe

Globe | Topographic Map

The color shaded relief image used as the base for this globe has a resolution of 32 pixels per degree (approximately 1850 m/pixel), and was produced and supplied by the MOLA Science

Mars Mini Globes

Globe

Project sheet with instructions for creating the Viking and Global Surveyor Mars globes using tennis balls.

Mars Viking Globe

Globe

The photomosaic that forms the base for this globe was created by merging two global digital image models (DIM's) of Mars, a medium-resolution monochrome mosaic processed to emphasize topographic features, and a

Moon Clementine Topographic Globe

Globe | Topographic Map

The photomosaic that forms the base for this globe combines a gray-shaded relief airbrush image with color-coded topographic data. The shaded relief data provide interpretations of lunar morphology based on lunar images

Venus Magellan Globe

Globe

The images used for the base of this globe show the northern and southern hemispheres of Venus as revealed by more than a decade of radar investigations culminating in the 1990-1994 Magellan