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Giant Cycones at Saturn's Poles Create a Swirl of Mystery 10/15/2008

New images yield clues to seasons of Uranus 10/15/2008

NASA Supercomputer Shows How Dust Rings Point to Exo-Earths 10/14/2008

Astronomers get best view yet of infant stars at feeding time 10/13/2008

Phoenix Lander Digs And Analyzes Soil As Darkness Gathers 10/13/2008

Venus Express searching for life - on Earth 10/12/2008

South Pole Telescope team uses new method to discover clusters of galaxies far, far away 10/12/2008

Cosmic eye sheds light on early galaxy formation 10/11/2008

Stars stop forming when big galaxies collide 10/11/2008

CoRoT discovery challenges the definition of extra-solar planets 10/10/2008

Born from the Wind - Unique Multi-wavelength Portrait of Star Birth 10/9/2008

NASA spacecraft ready to explore outer solar system 10/8/2008

Cassini flyby of Saturn moon offers insight into solar system history 10/8/2008

Researchers and students to develop small CubeSat satellites 10/7/2008

Meteorites From Inner Solar System Match Up To Earth's Platinum Standard 10/7/2008

Highest Resolution View Ever From Mars Comes From Phoenix Lander (6/8/2008)

Tags:
planets, mars, phoenix, landers

The color composite image on the right was acquired by the Optical Microscope, a part of the Microscopy, Electrochemistry, and Conductivity Analyzer (MECA) instrument suite on NASA's Phoenix Mars Lander. The image was taken on the ninth Martian day of the mission, or Sol 9 (June 3, 2008). Comparison with a black-and-white image (left) acquired during Phoenix's flight from Earth to Mars, identifies new particles deposited during the landing event. The particles are presumably samples from the Martian surface, although contamination from the lander itself cannot be ruled out. Most particles are the typical reddish-brown of the Martian surface, but some are translucent. The particles are on a silcone substrate target 3 millimeters (0.12 inch) in diameter, which provides a sticky surface for holding the particles while the microscope images them. Blow-ups of four of the larger particles are shown in the center. These particles range in size from about 30 microns to 150 microns (from about one one-thousandth of an inch to six one-thousandths of an inch).
The color composite image on the right was acquired by the Optical Microscope, a part of the Microscopy, Electrochemistry, and Conductivity Analyzer (MECA) instrument suite on NASA's Phoenix Mars Lander.

The image was taken on the ninth Martian day of the mission, or Sol 9 (June 3, 2008). Comparison with a black-and-white image (left) acquired during Phoenix's flight from Earth to Mars, identifies new particles deposited during the landing event. The particles are presumably samples from the Martian surface, although contamination from the lander itself cannot be ruled out. Most particles are the typical reddish-brown of the Martian surface, but some are translucent.

The particles are on a silcone substrate target 3 millimeters (0.12 inch) in diameter, which provides a sticky surface for holding the particles while the microscope images them. Blow-ups of four of the larger particles are shown in the center. These particles range in size from about 30 microns to 150 microns (from about one one-thousandth of an inch to six one-thousandths of an inch).
A microscope on NASA's Mars Phoenix Lander has taken images of dust and sand particles with the greatest resolution ever returned from another planet.

The mission's optical microscope observed particles that had fallen onto an exposed surface, revealing grains as small as one-tenth the diameter of a human hair.

"We have images showing the diversity of mineralogy on Mars at a scale that is unprecedented in planetary exploration," said Michael Hecht of NASA's Jet Propulsion Laboratory, located in Pasadena, Calif. He is the lead scientist for Phoenix's Microscopy, Electrochemistry and Conductivity Analyzer, or MECA, instrument suite.

The Phoenix mission is led by Peter Smith at The University of Arizona with project management at JPL and development partnership at Lockheed Martin, located in Denver.

Phoenix received commands Thursday to collect its first soil sample to be delivered to a laboratory instrument on the lander deck. Commands for that same activity sent on Wednesday did not reach Phoenix because the orbiter intended for relaying the transmission, NASA's Mars Odyssey, had put itself into a safe standby mode shortly before the commands would have reached Odyssey.

On Wednesday, the lander completed a backup plan of activities that had been sent previously, reported JPL's Chris Lewicki, mission manager for Phoenix surface operations on the lander's 11th Martian day. That plan included weather monitoring and additional imaging for a high-resolution color panorama of the site.

The optical microscope images, taken Tuesday, were of particles that had collected on a sticky surface exposed during the Phoenix landing and for five days after landing. "It's a first quick look," Hecht said. "This experiment was partly an insurance policy for something to observe with the microscope before getting a soil sample delivered by the arm, and partly a characterization of the optical microscope. All the tools are working well."

Some of the particles might have come from inside the spacecraft during the forceful events of landing, but many match expectations for Martian particles. "We will be using future observations of soil samples delivered by the robotic arm to confirm whether the types of particles in this dustfall sample are also seen in samples we can be certain are Martian in origin," Hecht said.

The particles show a range of shapes and colors.

"You can see the amount of variety there is in what appears otherwise to be just reddish-brown soil," said Tom Pike, Phoenix science team member from Imperial College London. He noted that one translucent particle resembles a grain of salt, but that it is too early to say for sure.

Thursday's commands were relayed to Phoenix via NASA's Mars Reconnaissance Orbiter. The relay radio on that orbiter has been working well in recent days, after intermittently turning itself off last week. Phoenix will continue to do relays via the Mars Reconnaissance Orbiter until Odyssey is fully functioning again, and then Phoenix will use both orbiters.

"We are currently bringing the Odyssey spacecraft back into nominal operations, and we will resume relay service with Odyssey in the next day or two," said JPL's Chad Edwards, chief telecommunications engineer for the JPL Mars Exploration Program.

"We think Odyssey went into safe mode because of a single event that affected computer memory," Edwards said. "Yesterday's safe mode event appears to be very similar to events that have caused Odyssey to go into safe mode two or three times earlier during its long operation around Mars." Odyssey has been orbiting Mars since 2001.

International contributions to the Phoenix Mars mission come from the Canadian Space Agency; the University of Neuchatel, Switzerland; the universities of Copenhagen and Aarhus, Denmark; Max Planck Institute, Germany; and the Finnish Meteorological Institute.

Note: This story has been adapted from a news release issued by the University of Arizona

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