Raph's Girl
08-01-2008, 06:49 AM
2 Water discovery stories in one sitting!
First up...the Phoenix lander has apperantly "tasted" water!
http://news.yahoo.com/s/nm/20080731/sc_nm/space_mars_dc_2
NASA scientists said on Thursday they had definitive proof that water exists on Mars after further tests on ice found on the planet in June by the Phoenix Mars Lander.
"We have water," said William Boynton, lead scientist for the Thermal and Evolved-Gas Analyzer instrument on Phoenix.
"We've seen evidence for this water ice before in observations by the Mars Odyssey orbiter and in disappearing chunks observed by Phoenix last month, but this is the first time Martian water has been touched and tasted," he said, referring to the craft's instruments.
NASA on Thursday also extended the mission of the Phoenix Mars Lander by five weeks, saying its work was moving beyond the search for water to exploring whether the red planet was ever capable of sustaining life.
"We are extending the mission through September 30," Michael Meyer, chief scientist for NASA's Mars exploration program, told a televised news conference.
The extension will add about $2 million to the $420 million cost of landing Phoenix on May 25 for what was a scheduled three-month mission, Meyer said.
Phoenix is the latest NASA bid to discover whether water -- a crucial ingredient for life -- ever flowed on Mars and whether life, even in the form of mere microbes, exists or ever existed there.
Phoenix touched down in May on an ice sheet and samples of the ice were seen melting away in photographs taken by the lander's instruments in June.
Boynton said that water was positively identified after the lander's robotic arm delivered a soil sample on Wednesday to an instrument that identifies vapors produced by heating.
Mission scientists said the extension would give time for more analysis of Martian samples. They plan to dig two additional trenches -- dubbed "cupboard" and "neverland" -- using the robotic arm on the Phoenix craft.
"We hope to be able to answer the question of whether this was a habitable zone on Mars. It will be for future missions to find if anyone is home on this environment," Phoenix principal investigator Peter Smith told the news conference.
Mission scientists said in June that Martian soil was more alkaline than expected and had traces of magnesium, sodium, potassium and other elements. They described the findings as a "huge step forward."
Meyer said the scientific proof of the existence of water meant that Phoenix could "move from looking for water to seeing whether there were habitats for life.
"We are moving towards understanding whether there were or could be places on Mars that are habitable," Meyer said.
2nd up...a giant lake has been confirmed on Saturn's moon Titan that they've dubbed Ontario Lacus (cuz it's bigger than Lake Ontario).
http://news.yahoo.com/s/space/20080730/sc_space/giantlakeconfirmedonsaturnsmoontitan
A giant, glassy lake larger than North America's Lake Ontario graces the south pole of Saturn's largest moon Titan, new research confirms.
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"This is the first observation that really pins down that Titan has a surface lake filled with liquid," said lead researcher Robert Brown of the University of Arizona's Lunar and Planetary Laboratory in Tucson.
Called Ontario Lacus, the lake extends 150 miles (235 kilometers) and covers an area of about 7,800 square miles (20,000 square kilometers). The lake structure is filled mostly with methane and ethane, hydrocarbons that are gases on Earth but liquid on the bone-chilling surface of Titan.
Wet ideas
The finding, detailed in the July 31 issue of the journal Nature, is just another gold star for Titan, which has become one of the most fascinating bodies in the solar system for exploring environments that may give rise to life. Boasting a size that's one-and-a-half times that of Earth's moon and bigger than Mercury, Titan is the only solar system moon known to support a planet-like atmosphere.
The idea of liquid features on Titan is not new. Before the Cassini mission to Saturn, astronomers thought Titan was covered in a global ocean, though the spacecraft's flybys of the moon sucked the life out of that wet notion. Even still, evidence for features similar to Earth's lakes and seas, along with telltale signs of erosion from flowing water, have since come to light.
Possible evidence for lake-like features came from radar images, but this method can't distinguish between liquid and very fine gravel or other tiny solids, Brown explained.
"Detection of liquid ethane in Ontario Lacus confirms a long-held idea that lakes and seas filled with methane and ethane exist on Titan," said researcher Larry Soderblom of the U.S. Geological Survey in Flagstaff, Ariz.
Titan lake
Soderblom, Brown and their colleagues used the infrared abilities of Cassini's visual and infrared mapping spectrometer, or VIMS, to peer through Titan's cotton-ball-like veil of hydrocarbons that extends more than 620 miles (1,000 km) above the moon's surface.
The measurements showed three features of the lake structure: the shoreline, or the outer edge of the lake; the so-called beach just inside the shoreline, which could be a sort of "bathtub ring" of material left behind as the ethane mixture evaporated; and the lake's interior, which appears dark, the researchers say.
"It seems to have partially evaporated, and that makes sense because the south pole has just gone through summer," Brown told SPACE.com. "The maximum evaporation will have already occurred or is in the process of occurring."
He added, "There's still a lot of liquid left in that lake, and we don't think it's going to evaporate much further."
Plus, the lake feature could be replenished by Titan's dreary drizzle of methane, which when hit by sunlight breaks down into ethane.
As for how the liquid lake feature would feel if one were to step in, "Liquid ethane-methane mix would be less viscous than water," Brown said. "If riffling your fingers through it you wouldn't feel as much resistance."
The Cassini mission is an international cooperative effort of NASA, the European Space Agency (ESA), Italian Space Agency (ASI) and several separate European academic and industrial contributors.
First up...the Phoenix lander has apperantly "tasted" water!
http://news.yahoo.com/s/nm/20080731/sc_nm/space_mars_dc_2
NASA scientists said on Thursday they had definitive proof that water exists on Mars after further tests on ice found on the planet in June by the Phoenix Mars Lander.
"We have water," said William Boynton, lead scientist for the Thermal and Evolved-Gas Analyzer instrument on Phoenix.
"We've seen evidence for this water ice before in observations by the Mars Odyssey orbiter and in disappearing chunks observed by Phoenix last month, but this is the first time Martian water has been touched and tasted," he said, referring to the craft's instruments.
NASA on Thursday also extended the mission of the Phoenix Mars Lander by five weeks, saying its work was moving beyond the search for water to exploring whether the red planet was ever capable of sustaining life.
"We are extending the mission through September 30," Michael Meyer, chief scientist for NASA's Mars exploration program, told a televised news conference.
The extension will add about $2 million to the $420 million cost of landing Phoenix on May 25 for what was a scheduled three-month mission, Meyer said.
Phoenix is the latest NASA bid to discover whether water -- a crucial ingredient for life -- ever flowed on Mars and whether life, even in the form of mere microbes, exists or ever existed there.
Phoenix touched down in May on an ice sheet and samples of the ice were seen melting away in photographs taken by the lander's instruments in June.
Boynton said that water was positively identified after the lander's robotic arm delivered a soil sample on Wednesday to an instrument that identifies vapors produced by heating.
Mission scientists said the extension would give time for more analysis of Martian samples. They plan to dig two additional trenches -- dubbed "cupboard" and "neverland" -- using the robotic arm on the Phoenix craft.
"We hope to be able to answer the question of whether this was a habitable zone on Mars. It will be for future missions to find if anyone is home on this environment," Phoenix principal investigator Peter Smith told the news conference.
Mission scientists said in June that Martian soil was more alkaline than expected and had traces of magnesium, sodium, potassium and other elements. They described the findings as a "huge step forward."
Meyer said the scientific proof of the existence of water meant that Phoenix could "move from looking for water to seeing whether there were habitats for life.
"We are moving towards understanding whether there were or could be places on Mars that are habitable," Meyer said.
2nd up...a giant lake has been confirmed on Saturn's moon Titan that they've dubbed Ontario Lacus (cuz it's bigger than Lake Ontario).
http://news.yahoo.com/s/space/20080730/sc_space/giantlakeconfirmedonsaturnsmoontitan
A giant, glassy lake larger than North America's Lake Ontario graces the south pole of Saturn's largest moon Titan, new research confirms.
ADVERTISEMENT
"This is the first observation that really pins down that Titan has a surface lake filled with liquid," said lead researcher Robert Brown of the University of Arizona's Lunar and Planetary Laboratory in Tucson.
Called Ontario Lacus, the lake extends 150 miles (235 kilometers) and covers an area of about 7,800 square miles (20,000 square kilometers). The lake structure is filled mostly with methane and ethane, hydrocarbons that are gases on Earth but liquid on the bone-chilling surface of Titan.
Wet ideas
The finding, detailed in the July 31 issue of the journal Nature, is just another gold star for Titan, which has become one of the most fascinating bodies in the solar system for exploring environments that may give rise to life. Boasting a size that's one-and-a-half times that of Earth's moon and bigger than Mercury, Titan is the only solar system moon known to support a planet-like atmosphere.
The idea of liquid features on Titan is not new. Before the Cassini mission to Saturn, astronomers thought Titan was covered in a global ocean, though the spacecraft's flybys of the moon sucked the life out of that wet notion. Even still, evidence for features similar to Earth's lakes and seas, along with telltale signs of erosion from flowing water, have since come to light.
Possible evidence for lake-like features came from radar images, but this method can't distinguish between liquid and very fine gravel or other tiny solids, Brown explained.
"Detection of liquid ethane in Ontario Lacus confirms a long-held idea that lakes and seas filled with methane and ethane exist on Titan," said researcher Larry Soderblom of the U.S. Geological Survey in Flagstaff, Ariz.
Titan lake
Soderblom, Brown and their colleagues used the infrared abilities of Cassini's visual and infrared mapping spectrometer, or VIMS, to peer through Titan's cotton-ball-like veil of hydrocarbons that extends more than 620 miles (1,000 km) above the moon's surface.
The measurements showed three features of the lake structure: the shoreline, or the outer edge of the lake; the so-called beach just inside the shoreline, which could be a sort of "bathtub ring" of material left behind as the ethane mixture evaporated; and the lake's interior, which appears dark, the researchers say.
"It seems to have partially evaporated, and that makes sense because the south pole has just gone through summer," Brown told SPACE.com. "The maximum evaporation will have already occurred or is in the process of occurring."
He added, "There's still a lot of liquid left in that lake, and we don't think it's going to evaporate much further."
Plus, the lake feature could be replenished by Titan's dreary drizzle of methane, which when hit by sunlight breaks down into ethane.
As for how the liquid lake feature would feel if one were to step in, "Liquid ethane-methane mix would be less viscous than water," Brown said. "If riffling your fingers through it you wouldn't feel as much resistance."
The Cassini mission is an international cooperative effort of NASA, the European Space Agency (ESA), Italian Space Agency (ASI) and several separate European academic and industrial contributors.