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

This Isn’t Saturn


uranus_irThis is a near-infrared view of Uranus with its rings and some of its moons. It was made by the 8.2-m VLT ANTU telescope at the ESO Paranal Observatory in Chile. The contrast between the rings and the planet is strongly enhanced at the wavelength at which this picture was made; the incoming sunlight is almost completely absorbed by gaseous methane present in the planetary atmosphere causing Uranus to appear unsually dark, but the icy material in the rings reflects the sunlight and appears relatively bright.

Uranus is unique among the planets of the solar system in having its axis of rotation tilted almost 90°. When Voyager 2 flew by in 1986, the south pole was pointed toward the Earth. In this picture made 16 years later (and about 20 percent of the away around the planet’s orbit), the Uranian ring system were seen at an angle comparable to Saturn’s when its ring system is most open.

Seven moons of Uranus are in the picture Titania and Oberon are the brightest. The much smaller and fainter Puck and Portia have visual magnitude about 21 and are barely visible in the photo.

Image Credit: ESO

Uranus and Ariel


Uranus_ArielUranus’ moon Ariel (white dot) and its shadow (black dot) were caught crossing the face of Uranus in this Hubble Space Telescope image. Note that the cloud bands which are aligned with the planet’s rotation are nearly vertical in the picture. Uranus is the giant planet whose equator is nearly at right angles to its orbit. A collision with an Earth-sized object several billion years ago is the likely cause of Uranus’ tilt. Nearly a twin to Neptune, Uranus has more methane in its mainly hydrogen and helium atmosphere than Jupiter or Saturn. Methane gives Uranus its blue tint.

Image Credit: NASA

Infrared Uranus


infrared_uranusThe Solar System’s third largest planet usually looks quite plain. Uranus typically appears as a featureless small spot in a small telescope or a featureless large orb in a large telescope. Back in the late ’90s, the Hubble Space Telescope photographed Uranus in infrared light. In this image the distant planet’s unusual clouds, rings, and moons are visible. Analysis indicates that clouds seen here in orange appear to circle Uranus at speeds in excess of 500 km/h.

Image Credit: NASA

To Be or Not To Be Among the Fairies


What is Hamlet doing hanging out with Oberon from A Midsummer Night’s Dream?

Since 1919, the International Astronomical Union has been charged with the task of establishing “conventional” nomenclature for planets, satellites, and surface features. Namesakes from Shakespearean works have been chosen for moons and objects around Uranus. Thus, Oberon, king of the fairies, is also Uranus’ most distant and second largest moon, and Hamlet is a tragically large and princely crater on its surface, the large dark crater to the right of center. This picture shows the known surface features of Oberon. It was constructed by the U.S. Geological Survey based on data from NASA’s Voyager 2.

Image Credit: NASA/USGS