Saturn’s rings tagged posts

1.Comparison of the images of Saturn’s rings in the 2008 view in the mid-infrared (left) and the visible light (right). The visible light image was taken on March 16, 2008 with the 105-cm Murikabushi telescope at Ishigakijima Astronomical Observatory. The radial brightness contrast of Saturn’s rings is the inverse between the two wavelength ranges. (Credit: NAOJ) 2.Comparison of the mid-infrared images of Saturn’s rings on April 30, 2005 (top) and January 23, 2008 (bottom). Although both of the images were taken in the mid-infrared, the radial contrast of Saturn’s rings is the inverse of each other. (Credit: NAOJ) 3. A three-color composite of the mid-infrared images of Saturn on January 23, 2008 captured with COMICS on the Subaru Telescope...

This image of the debris disk around SDSS1228+1040 made from observations taken over twelve years. The application of Doppler Tomography results in an image of the velocities within the disk, which has an ‘inside-out’ structure, gas closer to the white dwarf appears further. The two dashed circles illustrated 0.64 and 0.2 times the radius of the Sun. Credit: University of Warwick