Living next to a ringed planet in a flat solar system in a spiral galaxy may make you think there are a lot of disk-shapes in space. And, indeed, there are. A January 2005 issue of the journal Science contains a special section featuring the roles disks play in the universe.March 7, 2005 / Posted by: Shige Abe
Astrobiology includes the study of ways that astronomical events can influence the evolution of life on Earth. Alex Pavlov of the NAI University of Colorado team reports in two papers how passage of the solar system through dense cool clouds of dust and gas (called molecular clouds by astronomers) could influence the climate, producing extinctions and perhaps triggering the state known as “snowball Earth”. Much of this research was performed while Pavlov was a NAI postdoctoral fellow.March 3, 2005 / Posted by: Shige Abe
The origins of life – the nature of the transition from inanimate to animate chemistry – is one of the major mysteries of astrobiology. The first of the three theme-questions in astrobiology – Where did we come from? – deals in part with origins, whether the process took place on the ancient Earth or elsewhere. One perspective suggests that chemical interactions between water and various minerals might have been important.February 10, 2005 / Posted by: Shige Abe
On January 14 the Huygens Probe, built by the European Space Agency, made a soft landing on the surface of Saturn’s moon Titan. The first data from the atmosphere and surface reveal a remarkable place indeed, as described in a science press conference held in Paris on January 21.January 27, 2005 / Posted by: Shige Abe
At the boundary between the Permian and Triassic periods, 252 million years ago, multi-celled life on planet Earth was nearly terminated. This PT mass extinction represents the greatest dying in the fossil record, with more than 90 percent of species lost. New results from South Africa provide the best-ever picture of the PT extinction on land, suggesting that it was a much more complex process than would be expected for a comet or asteroid impact.January 21, 2005 / Posted by: Shige Abe
Imagine descending through hurricane-like conditions where wind speeds can reach 400 miles per hour and the ground temperatures drop as low as -300 degrees Fahrenheit. A choking haze envelopes everything. If all goes well, on January 14, a tiny capsule will take this plunge in hopes of sending back data and pictures near the surface of the Earth-like moon, Titan.
As part of the Cassini Imaging team studying the atmosphere on Saturn, Anthony Del Genio explained to Astrobiology Magazine his interests in the giant ringed world, Saturn and its strange moons.
As the Huygens probe begins its descent through Titan’s thick haze, few can offer the unique perspective of those who were there in the room when the daring concept for the mission was conceived.
University of Arizona Emeritus Professor, Don Hunten, was present in the beginning more than two decades ago, and this week’s culmination is another milestone in his remarkable career as a planetary scientist. When Hunten received the prestigious Fleming Award from the American Geophysical Union in 1998, he was recognized by his peers for his “original research and technical leadership in geomagnetism, atmospheric electricity, aeronomy ...
The European Space Agency has released the first 3 of several hundred images captured by the Huygens probe during its descent through the atmosphere of Saturn’s giant moon Titan. Although the images have not yet been cleaned up – they were released in their raw form – they reveal a world of diverse landforms, shaped at least in part by fluid erosion. Two of the images are reminiscent of early photographs of Mars.
The left half of the first image, taken from a height of 16 kilometers (10 miles) above Titan’s surface, shows a pattern of branching channels that look ...
Carolyn Porco of the Space Science Institute (Boulder, Colorado) heads Cassini’s imaging science team. She sat down with Astrobiology Magazine’s Chief Editor, Helen Matsos, to give a scientist’s first look at Titan from the European Space Agency’s Darmstadt, Germany mission control room.
Porco, also an University of Arizona adjunct professor of planetary sciences, describes her excitement and surprise when the Mars-like imagery first beamed down to Earth from Titan’s surface. Porco speculates what might elementally comprise those mysteriously smooth boulders in the foreground.
Helen Matsos (HM): What is your reaction to the stunning photos from ...
For nearly a decade, scientists around the world have been waiting patiently for the European Space Agency’s Huygens probe to arrive at its destination: Saturn’s giant moon Titan. Now, as the Huygens science team gathers at ESA’s control center in Darmstadt, Germany, that wait is almost over. In less than 24 hours, Huygens will descend down through Titan’s thick shroud of fog, taking a host of measurements along the way. The data the probe sends back will reveal Titan in far more detail than any previous mission has offered. Results from Hugyens may also provide a ...
On January 14th, four weeks after separation with the Cassini spacecraft, the European Space Agency’s Huygens probe will enter Titan’s atmosphere. Along its several-hour-long journey to the surface, it will collect, along with other data, the sounds of the atmosphere.January 13, 2005 / Posted by: Shige Abe
NAI-funded research on cores recovered through the Joint Oceanographic’s Ocean Drilling Program show that the activity of microbial life beneath the seafloor is far more diverse than expected.January 10, 2005 / Posted by: Shige Abe
NASA has selected eight proposals to provide instrumentation and associated science investigations for the mobile Mars Science Laboratory rover, scheduled for launch in 2009.December 14, 2004 / Posted by: Shige Abe
Is the methane on Mars coming from deep underground? Astrobiologist Mike Mumma discusses some possibilities while explaining how to measure methane on another world.December 6, 2004 / Posted by: Shige Abe
When the Cassini spacecraft flew by Titan on October 26, the RADAR instrument peered through the moon’s smoggy chemical haze. In an interview with Astrobiology Magazine editor Leslie Mullen, Ralph Lorenz from the University of Arizona’s Lunar and Planetary Lab discussed the surprises revealed by Cassini’s RADAR results.
Astrobiology Magazine (AM): Could you describe what the recent RADAR measurements uncovered on Titan?
Ralph Lorenz (RL): Titan is a unique moon in the solar system because it has a thick, mostly nitrogen atmosphere. That atmosphere also carries a little bit of methane and photochemical smog. That smog is ...
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