We're all made of Stardust...

Lantern Saturn
Credit: VIMS Team, U. Arizona, ESA, NASA

Explanation: Known for its bright ring system and many moons, gas giant Saturn looks strange and unfamiliar in this false-color view from the Cassini spacecraft. In fact, in this Visual and Infrared Mapping Spectrometer (VIMS) mosaic the famous rings are almost invisible, seen edge-on cutting across picture center. The most striking contrast in the image is along the terminator or boundary between night and day. To the right (day side) blue-green hues are visible sunlight reflected from Saturn’s cloud tops. But on the left (night side) in the absence of sunlight, the lantern-like glow of infrared radiation from the planet’s warm interior silhouettes features at Saturn’s deeper cloud levels. The infrared glow also shines from the broad shadows of Saturn’s rings sweeping across the planet’s upper hemisphere.

Serene Scene

Even in a peaceful looking scene such as this one of Saturn and its moon Tethys, the Cassini spacecraft reveals clues about how Saturn is ever-changing. Saturn’s northern hemisphere still shows the scars of the huge storm that raged through much of 2011 (see PIA14905). And, day by day, the shadows cast by the rings on the planet’s southern hemisphere are growing wider as the seasons progress toward northern summer. See PIA11667 and PIA09793 to learn about the changing seasons and the shadows cast by the rings.

Tethys (660 miles, or 1,062 kilometers across) appears above the rings to the left of the center of the image.

The image was taken with the Cassini spacecraft wide-angle camera on Jan. 10, 2012 using a spectral filter sensitive to wavelengths of near-infrared light centered at 752 nanometers. The view was obtained at a distance of approximately 1.4 million miles (2.3 million kilometers) from Saturn and at a Sun-Saturn-spacecraft, or phase, angle of 39 degrees. Image scale on Saturn is 84 miles (136 kilometers) per pixel.

Image Credit: NASA/JPL-Caltech/Space Science Institute

A Close Pass of Saturn’s Moon Dione
Image Credit: Cassini Imaging Team, ISS, JPL, ESA, NASA

Explanation: What’s that past Dione? When making its closest pass yet of Saturn’s moon Dione late last year, the robotic Cassini spacecraft snapped this far-ranging picture featuring Dione, Saturn’s rings, and the two small moons Epimetheus and Prometheus. The above image captures part of the heavily cratered snow-white surface of the 1,100 kilometer wide Dione, the thinness of Saturn’s rings, and the comparative darkness of the smaller moon Epimetheus. The image was taken when Cassini was only about 100,000 kilometers from the large icy moon. Future events in Cassini’s continuing exploration of Saturn and its moons include tomorrow’s flyby of Titan and imaging the distant Earth passing behind Saturn in June.

Saturn, taken last night with my phone through one of the larger telescopes at the YAS observatory. Very happy with it, it’s a great improvement from what I took last week. :D

Another example of why you don’t need to own expensive equipment to take pictures of space. :)

Took these photos last night using my phone, held up to various telescopes at the YAS observatory. Just goes to show you don’t need to have expensive equipment to take photos of space. :)

Top left: Venus as a pretty little crescent. :)

Top right: Mars, not a brilliant photo but it was the only one I took of it and wanted to post it anyway.

Bottom: Saturn, a lot better than my previous attempts so I’m pretty proud of this one. :D

Saturn’s Moon Helene in Color
Image Credit: NASA/JPL/SSI; Color Composite: Daniel Machácek

Explanation: Although its colors may be subtle, Saturn’s moon Helene is an enigma in any light. The moon was imaged in unprecedented detail last June as the robotic Cassini spacecraft orbiting Saturn swooped to within a single Earth diameter of the diminutive moon. Although conventional craters and hills appear, the above image also shows terrain that appears unusually smooth and streaked. Planetary astronomers are inspecting these detailed images of Helene to glean clues about the origin and evolution of the 30-km across floating iceberg. Helene is also unusual because it circles Saturn just ahead of the large moon Dione, making it one of only four known Saturnian moons to occupy a gravitational well known as a stable Lagrange point.