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Searching For Water On Mars Home

Searching for Water on Mars. Working under NASA's principle of "Follow the Water". The objectives of this investigation are to measure the electromagnetic properties of Mars analog materials under Mars ambient conditions. A number of different devices were used to measure magnetic susceptibility over a large range of low frequencies (. In addition to the frequency measurements, some of the Martian analog samples have been characterized. Details about the characterizations can be found here.

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Searching For Water On Mars Home | mars.mines.edu Reviews
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Searching for Water on Mars. Working under NASA's principle of Follow the Water. The objectives of this investigation are to measure the electromagnetic properties of Mars analog materials under Mars ambient conditions. A number of different devices were used to measure magnetic susceptibility over a large range of low frequencies (. In addition to the frequency measurements, some of the Martian analog samples have been characterized. Details about the characterizations can be found here.
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1 magnetic susceptibility
2 radar properties
3 characterization
4 please contact us
5 space dust research
6 measurements
7 equipment
8 samples
9 publications
10 links
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magnetic susceptibility,radar properties,characterization,please contact us,space dust research,measurements,equipment,samples,publications,links,people,beau winters,david stillman,brianne douthit,andy kass
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Searching For Water On Mars Home | mars.mines.edu Reviews

https://mars.mines.edu

Searching for Water on Mars. Working under NASA's principle of "Follow the Water". The objectives of this investigation are to measure the electromagnetic properties of Mars analog materials under Mars ambient conditions. A number of different devices were used to measure magnetic susceptibility over a large range of low frequencies (. In addition to the frequency measurements, some of the Martian analog samples have been characterized. Details about the characterizations can be found here.

INTERNAL PAGES

mars.mines.edu mars.mines.edu
1

Space Dust

http://mars.mines.edu/dev2/index.htm

Working under NASA, the purpose of this investigation are to measure the electrostatic properties of Mars and Moon dusts. For more information, please contact Gary Olhoeft - golhoeft@mines.edu. Site Created by Matthew Hergert. This site is best viewed in Internet Explorer with a resolution of 800x600.

2

Samples

http://mars.mines.edu/samples.htm

42 Martian Analog samples that have been acquired. CSM Geology Museum Samples - Hematite. 138 hematite rock samples. CSM Geology Museum Samples - Magnetite. 92 magnetite rock samples. For more information, please contact Gary Olhoeft - golhoeft@mines.edu. Site Created by Matthew Hergert. NASA Grant 20119458 NAG5-12754. This site is best viewed in Internet Explorer with a resolution of 800x600.

3

Magnetic Susceptibility

http://mars.mines.edu/magsus.htm

CSM Geology Museum measurements. The magnetic susceptibilities of 230 hematite and magnetite rock samples from the CSM Geology Museum were measured using a Sapphire Instruments system at 600 Hz. The magnetic susceptibilities of 32 Martian analog soil samples was measured using a Bartington Instruments system at 465 Hz and 4,650 Hz. The magnetic susceptibilities of 32 Martian analog soil samples was measured using a Sapphire Instruments system at 600 Hz and 6,000 Hz. Comparison of MS measurements.

4

Measurements

http://mars.mines.edu/measure.htm

Of Martian Analog samples were measured at low frequencies (. Complex dielectric permittivity and complex magnetic permeability) of Martian Analog samples were measured at RADAR frequencies and from a temperature range of 303K to 180K. For more information, please contact Gary Olhoeft - golhoeft@mines.edu. Site Created by Matthew Hergert. NASA Grant 20119458 NAG5-12754. This site is best viewed in Internet Explorer with a resolution of 800x600.

5

Equipment

http://mars.mines.edu/equip/equip.htm

HP Vector Network Analyzer 8753D. Complex dielectric permittivity and complex magnetic permeability measurements were made in the frequency domain using an HP 8754D vector network analyzer (VNA) controlled by an external computer. The frequency range of the VNA is from 30 kHz - 3 GHz. HP 4284 Precision LCR Meter. So-Low Ultra-Low freezer, Model #C85-5. Is used to get down to Martian like temperatures. YSI 44006 Epoxy-Encapsulated Thermistors. Used to measure temperature inside the freezer. Used to measur...

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Searching for Water on Mars. Working under NASA's principle of "Follow the Water". The objectives of this investigation are to measure the electromagnetic properties of Mars analog materials under Mars ambient conditions. A number of different devices were used to measure magnetic susceptibility over a large range of low frequencies (. In addition to the frequency measurements, some of the Martian analog samples have been characterized. Details about the characterizations can be found here.

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