Satellites Can Track Epidemics
Mars Orbiter Survives Its Journey to the Red Planet
Next Solar Max Will Be a Big One
Fly Through of a Martian Canyon
Super Earths Might Be Common
Pluto and Its Moons Were Born Together
What's Up This Week - March 13 - March 19, 2006
Astrophoto: The Vela Supernova Remnant by Loke Kun Tan
The NASA Science Missions Getting Cut
Book Review: Chasing Hubble's Shadows
NASA Orbiter Arrives at Mars
GIOVE A Transmits Loud and Clear
Merging White Dwarfs Create Helium Stars
Cometary Globule CG4
SOHO Can See Right Through the Sun
Liquid Water Might Be On Enceladus
Gigantic Eruptions Helped in the Dinosaur's Demise
Say Goodbye to the Polar Ice Sheets
Enceladus in Front of Saturn
Iapetus' Terminator
Saturn's G Ring
Furthest Gamma Ray Burst Seen
What's Up 2006 - Printed Version Available
The Early Universe Was Unkind to Life's Building Blocks
The Part-Time Pulsar
Antarctica is Melting Faster
Jupiter's Next Great Red Spot
Towering Cliffs at the Edge of Olympus Mons
Saturn's Northern Lights Can Go Backwards
Scientists are Starting to Understand Solar Cycles
Galactic Chimneys Rising Above NGC 2841
Book Review: Parallel Worlds
What's Up This Week - March 6 - March 12, 2006
Astrophoto: Comet Pojmanski by R. Jay GaBany
Researchers mimic high-pressure form of ice found in giant icy moons
Andromeda's Origin is Similar to That of the Milky Way
Shock Wave in Stephan's Quintet Galaxy
Magnetic Fields Confine a Dying Star's Jets
The Source of Titan's Methane
Cepheids Live in Cocoons
Hubble Portrait of the Pinwheel Galaxy
Pulsar Blasts Through a Ring of Gas
Mimas and Saturn
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.
Continue reading
Block Starlight to See Planets
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.
Continue reading
CryoSat-2 Will be Constructed
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.
Continue reading
What's Inside a Gas Giant?
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.
Continue reading
FUSE Satellite is Working Again
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.
Continue reading
Astrophoto: A New Star in Ophiucus by John Chumack
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.
Continue reading
What's Up This Week - February 27 - March 5, 2006
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!
Continue reading
Here's what's up!
Universe Today