This is a photograph of Saturn's icy moon Mimas, perched in front of the ringed planet. Mimas is only 397 kilometers (247 miles) across, so it's absolutely dwarfed by Saturn in the background. NASA's Cassini spacecraft took this photograph on January 20, when it was approximately 1.4 million kilometers (900,000 miles) from Mimas.

University of Arizona researchers have developed an "optical vortex mask" that will block the starlight from a bright star, so that dim objects nearby the star can be observed. This mask could theoretically be attached to a powerful observatory, to completely mask the light from the star, and allow astronomers to see planets 10 billion times less bright. Future space missions, like the Terrestrial Planet Finder might use a similar technique as well.

Officials at the European Space Agency have approved a plan to build and launch a replacement spacecraft for destroyed CryoSat satellite. CryoSat 1 was lost when its Rockot launcher malfunctioned on October 8, 2005. CryoSat-2 will have the same mission objectives as its predecessor, to monitor the thickness of land and sea ice, and to help scientists predict future climates as this ice melts and the planet warms up. It will probably be launched in March, 2009.

If you could strip away all the gas from Jupiter and Saturn, what would you find inside? Inside gas giant planets, the pressures and temperatures are enormous, and not much can survive those conditions. Researchers at the University of Minnesota have calculated that crystals would dissolve, and would actually work like metals, facilitating the flow of electrons. This could help to explain the tremendous magnetic fields detected around gas giant planets.

NASA's Far Ultraviolet Spectroscopic Explorer (FUSE) astronomy satellite has returned to service after being offline for about 10 months. 3 of the spacecraft's 4 reaction wheels had failed; these allow it to point at precise locations in the sky. Even though it only has a single reaction wheel, engineers were able to create a technique which allows it to orient itself. FUSE has already had its original 3-year mission extended twice, so any further science it can gather is a bonus.

A pair of stars with about the same mass will evolve in about the same manner. But if one of the pair is more massive than the other, the more massive star will use its nuclear fuel faster, enter the red giant stage sooner and become a white dwarf earlier while its partner is still red and bloated. This scenario is actually quite common throughout the universe and leads to spectacular results.

Greetings, fellow SkyWatchers! Start your week out "hot" as we take a look at AE Aurigae - The Flaming Star. If you still carry a torch for an old "Flame" then come along as we have a look at NGC 2024. We'll round up the horses, head out for Abell 426, lasso some wild star clusters and ride off into the moonrise as the week ends. All you have to do is turn an eye to the sky, because...

Here's what's up!

NASA's Mars Reconnaissance Orbiter has nearly reached its destination, but its work is just about to begin. On March 10, the spacecraft will turn on its thrusters, allowing it to be captured by Mars' gravity. Over the course of the next six months, it will continue adjusting its orbit through a process called aerobraking, where the spacecraft skims through the Martian atmosphere, slowing it down a little bit each time. In addition to the high resolution images and scientific data it will capture, the spacecraft will help the rovers and future landers communicate back to Earth.

NASA's Swift satellite is continuing to send back surprising information about gamma ray bursts. On February 18, 2006, it discovered something completely unique; a burst that originated 440 million light-years away and lasted about 30 minutes. This event is very similar to the more common bursts that have been seen in the past; however, it was about 25 times closer, and lasted 100 times longer than a typical burst.

These images, of the Ausonia Mensa massif, were taken by ESA's Mars Express spacecraft. This region is a large remnant mountain, 3,700 metres (12,100 feet) high. It's covered by several large impact craters, some of which are partially filled with sediment, and in various stages of erosion.

In late January, astronomers celebrated the creation of an artificial star in the nighttime sky. The star was created 90 km up in the atmosphere by a powerful laser projected out of the ESO's fourth 8.2m Unit Telescope of the Very Large Telescope at Cerro Paranal in Chile. This artificial star allows the telescope's adaptive optics system to compensate against the fluctuations of the Earth's atmosphere, and produce images as crisp and clear as if they were taken from space.

If our Milky Way looked in the mirror, this is what it would probably see. This is a photograph of galaxy Messier 100, located about 60 million light-years away. It presents an intricate structure with a bright core, two large arms, and a pair of fainter spiral arms. Japanese amateur astronomer Shoji Suzuki and Italian astronomer Marco Migliardi recently discovered a Type-Ia supernova in M100 on February 4, 2006.

Boston University astronomers announced today that they've found evidence that solar flares change the upper Martian atmosphere. The researchers found that when X-ray bursts from the Sun reach Mars, they cause the planet's ionosphere to produce additional ions and electrons - exactly the same situation was recorded simultaneously by satellites here on Earth. The measurements were made by NASA's Mars Global Surveyor as it transmitted data back to Earth.