Difference between revisions of "Phoenix Mars Mission"

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Analysis of the first soil sample discovered bound water and CO<sub>2</sub> These were released during the highest-temperature, 1,000 °C) heating cycle.<ref>cite web|last=Lakdawalla|first=Emily|title=''Phoenix'' sol 30 update: Alkaline soil, not very salty, "nothing extreme" about it!|website=The Planetary Society |publisher=[[Planetary Society]]|date=2008-06-26|url=http://www.planetary.org/blog/article/00001526/|accessdate=2008-06-26</ref>
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Analysis of the first soil sample discovered bound water and CO<sub>2</sub> These were released during the highest-temperature, 1,000 °C) heating cycle.<ref>http://www.planetary.org/blogs/emily-lakdawalla/2008/1526.html</ref>
  
Chemicals measured in the samples were chloride, bicarbonate, magnesium, sodium, potassium, calcium, and sulfate.<ref name="Kounaves et al 2010 Geophysical Research Letters"/> Further data analysis indicated that the soil contains soluble sulfate (SO<sub>3</sub>) at a minimum of 1.1% and provided a refined formulation of the soil.<ref name="Kounaves et al 2010 Geophysical Research Letters"/>
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Chemicals measured in the samples were chloride, bicarbonate, magnesium, sodium, potassium, calcium, and sulfate.<ref name="Kounaves et al 2010 Geophysical Research Letters"/> Further data analysis indicated that the soil contains soluble sulfate (SO<sub>3</sub>) at a minimum of 1.1% and provided a refined formulation of the soil.<ref>Kounaves, Samuel P; Hecht, Michael H; Kapit, Jason; Quinn, Richard C; Catling, David C; Clark, Benton C; Ming, Douglas W; Gospodinova, Kalina; Hredzak, Patricia; McElhoney, Kyle; Shusterman, Jennifer (2010). "Soluble sulfate in the martian soil at the Phoenix landing site". Geophysical Research Letters. 37 (9): L09201.</ref>
  
  
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==See Also==
 
==See Also==
 +
 
[[The Phoenix Mars Mission (MarsHome.org)]]
 
[[The Phoenix Mars Mission (MarsHome.org)]]
  

Revision as of 12:40, 6 November 2018

The official logo for the Phoenix Mars Mission.

NASA's Phoenix mission was a robotic mission, the first lander in NASA's "Scout class". The lander landed in Mars' north polar region on May 25th 2008, and the scientific package aimed to answer the questions:

  1. Can the Martian arctic support life?
  2. What is the history of water at the landing site?
  3. How is the Martian climate affected by polar dynamics?

The mission name derives from several components built previously for cancelled missions, including 2001's Mars Surveyor lander.

The mission was of considerable interest to planners of human missions to Mars, as many practical mission designs assume the availability of easily-extractable water for fuel production and industrial processes. The polar regions were expected to be the most likely places to find water ice.


Phoenix Lander with instruments labeled


Mission Profile

An artist's impression of the Phoenix lander's "powered landing" on touching down on the Mars surface.


Phoenix lander descending to surface, as imaged by HiRISE

Phoenix was launched on 4th August 2007 on a Delta II 7925 rocket, and the scheduled landing on Mars on 25th May 2008 was successful. The landing site was the ice-capped northern polar region in the Green Valley of Vastitas Borealis.[1]

Although the primary mission was expected to last around 90 sols, the lander was working 152 sols. The last transmission was received on November 2nd, 2008 by the project team.

Wide view from Phoenix lander Solar panels are visible.

Accomplishments

Phoenix has confirmed the presence of water ice in the Martian soil.[2] The soil contains small amounts of salt (perchlorate salt, calcium carbonate). The mildly alkaline soil environment provides good conditions for growing plants.


Analysis of the first soil sample discovered bound water and CO2 These were released during the highest-temperature, 1,000 °C) heating cycle.[3]

Chemicals measured in the samples were chloride, bicarbonate, magnesium, sodium, potassium, calcium, and sulfate.[4] Further data analysis indicated that the soil contains soluble sulfate (SO3) at a minimum of 1.1% and provided a refined formulation of the soil.[5]


View under Phoenix spacecraft Bright regions are probably top of an ice sheet.


View from Phoenix showing polygons on surface

See Also

The Phoenix Mars Mission (MarsHome.org)

References:

  1. https://www.webcitation.org/5W4NeGhno?url=http://phoenix.lpl.arizona.edu/
  2. Smith, P., et al. 2009. H2O at the Phoenix Landing Site. Science: 325, 58-61.
  3. http://www.planetary.org/blogs/emily-lakdawalla/2008/1526.html
  4. Cite error: Invalid <ref> tag; no text was provided for refs named Kounaves et al 2010 Geophysical Research Letters
  5. Kounaves, Samuel P; Hecht, Michael H; Kapit, Jason; Quinn, Richard C; Catling, David C; Clark, Benton C; Ming, Douglas W; Gospodinova, Kalina; Hredzak, Patricia; McElhoney, Kyle; Shusterman, Jennifer (2010). "Soluble sulfate in the martian soil at the Phoenix landing site". Geophysical Research Letters. 37 (9): L09201.

External Links