Internet Astronomy: Uranus and Moons

This video of Uranus and some of its moons was taken in infrared light using the ESO’s Very Large Telescope during the planet’s 2008 equinox. Every 42 years, the ring (and satellites) plane of Uranus crosses the Sun, giving observers on Earth the opportunity to observe the rings edge on. Ring plane crossing also allow us to observe the rings from their dark side (that is, while the Sun is illuminating them from the opposite side), aiding the search for faint satellites, faint rings, or faint ring structures. A ring plane crossing is also an opportunity to observe mutual interactions between satellites such as eclipses or occultation phenomena.

The movie shows the Uranus system of satellites over a two hour period. It’s easy to see the impact of fluctuating seeing conditions on the image quality. Under good seeing, the small satellites Puck and Portia become clearly visible, but the images start to blur when the seeing degrades.

Video Credit: ESO/C. Dumas, B. Sicardy, and J.-E. Arlot

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