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Courtesy of NASA's National Space Science Data Center
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The spacecraft comprises a octagonal base supported on three landing legs. Two octagonal solar panel wings extend from the base to provide power. Communication will be primarity through UHF relay via the Mars 2001 Odyssey orbiter, but Mars Reconnaissance Orbiter, and Mars Express can also be used as relays, and Phoenix has a steerable medium gain X-band antenna to provide communications directly with Earth.
The science experiments and a robotic arm are mounted on the base. The experiments are: the Microscopy, Electrochemistry, and Conductivity Analyzer (MECA), the Robotic Arm Camera (RAC), the Surface Stereo Imager (SSI), the Thermal and Evolved Gas Analyzer (TEGA), the Mars Descent Imager (MARDI), and the meteorological station (MET). Total science payload mass is 55 kg.
Phoenix launched on 4 August 2007 at 9:26:34 UT (5:26 a.m. EDT) on a Delta II 7925 from Cape Canaveral Air Force Station. The 681 million km heliocentric cruise to Mars will take approximately 10 months, with landing on Mars on 25 May of 2008. A powered descent and soft-landing will be achieved using a pulsed propulsion system with 8 thrusters. The landing site will be in the north polar region between 65 and 72 degrees N. Surface temperatures in this region range between about 190 and 260 K and the landing altitude will be about 3.5 km below the planetary reference. Mars will be 275 million km from Earth at the time of touchdown. The solar panels will be deployed after allowing time for the dust to settle, and all instruments will be deployed in the first two days after landing.
Cost of the mission is estimated at $417 million.
Phoenix Lander on Mars
NASA's Phoenix Mars Lander monitors the atmosphere overhead and reaches
out to the soil below in this artist's depiction of the spacecraft fully
deployed on the surface of Mars.
Phoenix has been assembled and tested for launch in August 2007 from Cape Canaveral Air Force Station, Fla., and for landing in May or June 2008 on an arctic plain of far-northern Mars. The mission responds to evidence returned from NASA's Mars Odyssey orbiter in 2002 indicating that most high-latitude areas on Mars have frozen water mixed with soil within arm's reach of the surface.
Phoenix will use a robotic arm to dig down to the expected icy layer. It will analyze scooped-up samples of the soil and ice for factors that will help scientists evaluate whether the subsurface environment at the site ever was, or may still be, a favorable habitat for microbial life. The instruments on Phoenix will also gather information to advance understanding about the history of the water in the icy layer. A weather station on the lander will conduct the first study Martian arctic weather from ground level.
The vertical green line in this illustration shows how the weather station
on Phoenix will use a laser beam from a lidar instrument to monitor dust
and clouds in the atmosphere. The dark "wings" to either side of the
lander's main body are solar panels for providing electric power.
(Courtesy NASA/JPL/UA/Lockheed Martin)
Launch of the Mars Phoenix Lander
The Delta II 7925 rocket carrying NASA's Phoenix Mars lander thunders to life at 5:26 a.m. EDT at Pad 17A on Cape Canaveral Air Force Station. Phoenix will land in icy soils near the north polar, permanent ice cap of Mars and explore the history of the water in these soils and any associated rocks, while monitoring polar climate. Landing on Mars is planned in May 2008 on arctic ground where a mission currently in orbit, Mars Odyssey, has detected high concentrations of ice just beneath the top layer of soil.
(Courtesy NASA)
Launch of the Mars Phoenix Lander
NASA's Phoenix Mars lander illuminates Launch Pad 17A as it lifts off aboard a Delta II 7925 rocket at 5:26 a.m. EDT from Cape Canaveral Air Force Station. Phoenix will land in icy soils near the north polar, permanent ice cap of Mars and explore the history of the water in these soils and any associated rocks, while monitoring polar climate. Landing on Mars is planned in May 2008 on arctic ground where a mission currently in orbit, Mars Odyssey, has detected high concentrations of ice just beneath the top layer of soil.
(Courtesy NASA)
Phoenix Twilight (Artist Concept)
In this artist's concept illustration, NASA's Phoenix Mars Lander begins
to shut down operations as winter sets in. The far-northern latitudes on
Mars experience no sunlight during winter. This will mark the end of the
mission because the solar panels can no longer charge the batteries on the
lander. Frost covering the region as the atmosphere cools will bury the
lander in ice.
(Courtesy NASA/JPL-Calech/University of Arizona)
Powered Landing of Phoenix (Artist Concept)
This artist's concept depicts NASA's Phoenix Mars Lander a moment before
its 2008 touchdown on the arctic plains of Mars. Pulsed rocket engines
control the spacecraft's speed during the final seconds of descent.
(Courtesy NASA/JPL-Calech/University of Arizona)
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