Main

January 10, 2010

SALMON AO Amendment 4: Release of a Solicitation for ExoMars Trace Gas Orbiter Instruments Investigations

Release Date: January 15, 2010
Notice of Intent to propose Due: February 12, 2010
Proposals Due: April 15, 2010

With this amendment, the National Aeronautics and Space Administration (NASA) Science Mission Directorate (SMD) Announcement of Opportunity (AO) NNH08ZDA009O, "Stand Alone Missions of Opportunity Notice (SALMON)," is amended to establish a new Program Element Appendix (PEA) as Appendix H6, ExoMars Trace Gas Orbiter Instruments Investigations. This PEA solicits Principal Investigator (PI)-led instrument science investigations for the ExoMars 2016 Orbiter mission. The ExoMars 2016 Orbiter mission is a joint ESA-NASA mission. Together, NASA and ESA expect to select sufficient instrument science investigations to address the ExoMars Trace Gas Orbiter mission science objectives. All proposed investigations must describe a science investigation with goals and objectives that address the ExoMars Trace Gas Orbiter mission science objectives. Further information on the ExoMars 2016 Orbiter mission is available at http://salmon.larc.nasa.gov/SALMONreflib.html#ExoMars.

Continue reading "SALMON AO Amendment 4: Release of a Solicitation for ExoMars Trace Gas Orbiter Instruments Investigations" »

January 7, 2010

Salt Ponds Could Be Clue to Life on Mars

Rocco Mancinelli, PI of NAI's Emeritus Team at the SETI Institute, will use a zeppelin airship to observe red salt ponds turn green while the environment is changed from near-Martian conditions into wetlands. Work will begin next year on a decades-long project to restore thousands of acres of industrial salt-harvesting ponds in San Francisco Bay into native wetland habitat. The ponds are colored red because of the color of microbes that flourish in the extremely salty conditions. Green microbes will replace red ones as the wetlands are restored.

For more information: http://www.sfexaminer.com/local/Salt-ponds-could-be-clue-to-life-on-Mars-79280337.html [Source NAI Newsletter]

September 22, 2009

Student Travel Grants - Workshop on Methane on Mars

November 25-27, 2009 in Frascati, Italy - The NASA Mars Program Office has announced that travel funding will be made available for as many as 5 students who are U.S. citizens or legal residents, with Mars-related interests, to attend the Workshop on Methane on Mars: Current Observations, Interpretation and Future Plans, November 25-27, 2009 in Frascati, Italy. An application must be submitted by September 28, 2009, to be considered for this funding. NASA Headquarters will make the selections and students will be notified no later than October 15, 2009. Reimbursable costs include registration fees, transportation (airfare, mileage to/from airport, parking, rental car) and lodging/per diem. In most cases, actual expenses will exceed the funding provided.

Continue reading "Student Travel Grants - Workshop on Methane on Mars" »

February 11, 2009

A Case for Ancient Springs in Arabia Terra, Mars

Based on new image data from the High Resolution Imaging Science Experiment (HiRISE) on Mars Reconnaissance Orbiter (MRO), a case can be made that several structures in Vernal Crater, Arabia Terra are ancient springs. This interpretation is based on comprehensive geomorphologic analysis coupled with assessment of multiple hypotheses.

Continue reading "A Case for Ancient Springs in Arabia Terra, Mars" »

Short- and Long-Term Olivine Weathering in Svalbard: Implications for Mars

Liquid water is essential to life as we know it on Earth; therefore, the search for water on Mars is a critical component of the search for life. Olivine, a mineral identified as present on Mars, has been proposed as an indicator of the duration and characteristics of water because it dissolves quickly, particularly under low-pH conditions. The duration of olivine persistence relative to glass under conditions of aqueous alteration reflects the pH and temperature of the reacting fluids.

Continue reading "Short- and Long-Term Olivine Weathering in Svalbard: Implications for Mars" »

January 9, 2009

The MARTE VNIR Imaging Spectrometer Experiment: Design and Analysis

Astrobiology. October 2008, 8(5): 1001-1011.
http://www.liebertonline.com/doi/pdfplus/10.1089/ast.2007.0142

We report on the design, operation, and data analysis methods employed on the VNIR imaging spectrometer instrument that was part of the Mars Astrobiology Research and Technology Experiment (MARTE). The imaging spectrometer is a hyperspectral scanning pushbroom device sensitive to VNIR wavelengths from 400-1000 nm. During the MARTE project, the spectrometer was deployed to the Rio Tinto region of Spain. We analyzed subsets of three cores from Rio Tinto using a new band modeling technique. We found most of the MARTE drill cores to contain predominantly goethite, though spatially coherent areas of hematite were identified in Core 23. We also distinguished non Fe-bearing minerals that were subsequently analyzed by X-ray diffraction (XRD) and found to be primarily muscovite. We present drill core maps that include spectra of goethite, hematite, and non Fe-bearing minerals. Astrobiology 8, 1001-1011.

The Subsurface Geology of Rio Tinto: Material Examined During a Simulated Mars Drilling Mission for the Mars Astrobiology Research and Technology Experiment (MARTE)

Astrobiology. October 2008, 8(5): 1013-1021.
http://www.liebertonline.com/doi/pdfplus/10.1089/ast.2006.0107

The 2005 Mars Astrobiology Research and Technology Experiment (MARTE) project conducted a simulated 1-month Mars drilling mission in the Rio Tinto district, Spain. Dry robotic drilling, core sampling, and biological and geological analytical technologies were collectively tested for the first time for potential use on Mars. Drilling and subsurface sampling and analytical technologies are being explored for Mars because the subsurface is the most likely place to find life on Mars. The objectives of this work are to describe drilling, sampling, and analytical procedures; present the geological analysis of core and borehole material; and examine lessons learned from the drilling simulation.

Continue reading "The Subsurface Geology of Rio Tinto: Material Examined During a Simulated Mars Drilling Mission for the Mars Astrobiology Research and Technology Experiment (MARTE)" »

Visible-Near Infrared Point Spectrometry of Drill Core Samples from Rio Tinto, Spain: Results from the 2005 Mars Astrobiology Research and Technology Experiment (MARTE) Drilling Exercise

Astrobiology. October 2008, 8(5): 1049-1060.
http://www.liebertonline.com/doi/pdfplus/10.1089/ast.2007.0146


Sampling of subsurface rock may be required to detect evidence of past biological activity on Mars. The Mars Astrobiology Research and Technology Experiment (MARTE) utilized the Rio Tinto region, Spain, as a Mars analog site to test dry drilling technologies specific to Mars that retrieve subsurface rock for biological analysis. This work examines the usefulness of visible-near infrared (VNIR) (450-1000 nm) point spectrometry to characterize ferric iron minerals in core material retrieved during a simulated Mars drilling mission. VNIR spectrometry can indicate the presence of aqueously precipitated ferric iron minerals and, thus, determine whether biological analysis of retrieved rock is warranted. Core spectra obtained during the mission with T1 (893-897 nm) and T2 (644-652 nm) features indicate goethite-dominated samples, while relatively lower wavelength T1 (832-880 nm) features indicate hematite. Hematite/goethite molar ratios varied from 0 to 1.4, and within the 880-898 nm range, T1 features were used to estimate hematite/goethite molar ratios. Post-mission X-ray analysis detected phyllosilicates, which indicates that examining beyond the VNIR (e.g., shortwave infrared, 1000-2500 nm) will enhance the detection of other minerals formed by aqueous processes.

Continue reading "Visible-Near Infrared Point Spectrometry of Drill Core Samples from Rio Tinto, Spain: Results from the 2005 Mars Astrobiology Research and Technology Experiment (MARTE) Drilling Exercise" »

Underground Habitats in the Rio Tinto Basin: A Model for Subsurface Life Habitats on Mars

Astrobiology. October 2008, 8(5): 1023-1047.
http://www.liebertonline.com/doi/pdfplus/10.1089/ast.2006.0104

A search for evidence of cryptic life in the subsurface region of a fractured Paleozoic volcanosedimentary deposit near the source waters of the Rio Tinto River (Iberian pyrite belt, southwest Spain) was carried out by Mars Astrobiology Research and Technology Experiment (MARTE) project investigators in 2003 and 2004. This conventional deep-drilling experiment is referred to as the MARTE ground truth drilling project. Boreholes were drilled at three sites, and samples from extracted cores were analyzed with light microscopy, scanning electron microscopy-energy dispersive spectroscopy (SEM-EDS), X-ray diffraction (XRD), and Fourier transform infrared spectroscopy. Core leachates were analyzed with ion chromatography, and borehole fluids were analyzed with ion and gas chromatography. Key variables of the groundwater system (e.g., pO2, pH, and salinity) exhibit huge ranges probably due to surficial oxygenation of overall reducing waters, physical mixing of waters, and biologically mediated water-rock interactions.

Continue reading "Underground Habitats in the Rio Tinto Basin: A Model for Subsurface Life Habitats on Mars" »

January 5, 2009

NASA Graduate Student Researchers Program: Planetary Science - Mars

This research focuses on the general circulation and climate system of Mars. There have been 7 successful spacecraft missions to Mars in the past 10 years returning valuable new data about the thermal structure of the atmosphere, the seasonal cycles of dust, water, and carbon dioxide, and the nature of the surface and subsurface. Our group interprets these data using a Mars General Circulation Model. We use the model to simulate the observations and determine what physical and dynamical processes are responsible for them. The model includes a full surface heat budget, a cloud microphysics package, a two-stream radiation code for gases and aerosols, a level-2 boundary layer scheme, mass conserving tracer transport algorithms, and CO2 condensation/sublimation physics. Topics we are currently studying include coupling between the present day dust, water, and CO2 cycles, the effect of orbital changes on past climates, and the nature of the early Martian atmosphere when surface pressures were thought to be higher than they are today. The goal of this work is to understand how the Martian atmosphere and climate system have evolved through time. Deadline: Feb 1, 2009 http://fellowships.hq.nasa.gov/gsrp/research/detail.cfm?oppID=33

December 19, 2008

ROSES-08 Amendment 32: Final text for Moon and Mars Analog Mission Activities (MMAMA)

This amendment replaces the draft text in Appendix C.24 entitled "Moon and Mars Analog Mission Activities" with the final text. NASA Moon and Mars Analog Mission Activities (MMAMA) research addresses the need for integrated interdisciplinary field experiments as an integral part of preparation for planned human and robotic missions to the Moon and Mars. The focus of this program is on providing high-fidelity scientific investigations, scientific input, and science operations constraints in the context of planetary field campaigns. Funding provided in this program element is intended to enable researchers to conduct scientific investigations and integrate their instruments, projects, and/or protocols into field activities designed to help NASA plan for future exploration of the Moon, Mars, and other planetary bodies with both robots and humans.

Continue reading "ROSES-08 Amendment 32: Final text for Moon and Mars Analog Mission Activities (MMAMA)" »

September 4, 2008

Silicate Mineralogy on Mars Indicates Wet Past

Using data from the CRISM instrument on NASA's Mars Reconnaissance Orbiter, astrobiologists from NAI's SETI Institute and Marine Biological Laboratory teams present findings of silicate mineralogy indicating a wide range of past aqueous activity in the Mawrth Vallis on Mars. This work, published in the August 8 issue of Science, suggests that abundant water was once present on Mars and that hydrothermal activity may have occurred. The Mawrith Vallis could be a landing site for future rover missions to Mars. [Source: NAI Newsletter]

August 27, 2008

Silicate Mineralogy on Mars Indicates Wet Past

Using data from the CRISM instrument on NASA's Mars Reconnaissance Orbiter, astrobiologists from NAI's SETI Institute and Marine Biological Laboratory teams present findings of silicate mineralogy indicating a wide range of past aqueous activity in the Mawrth Vallis on Mars. This work, published in the August 8 issue of Science, suggests that abundant water was once present on Mars and that hydrothermal activity may have occurred. The Mawrith Vallis could be a landing site for future rover missions to Mars.

June 26, 2008

Erosion on Earth and Mars: Mere Seepage or Megaflood?

Researchers from NAI's University of California, Berkeley Team have a new study in Science focused on Box Canyon in Idaho. Incised into a basaltic plain with no drainage network upstream, and approximately 10 cubic meters per second of seepage emanating from its vertical headwall, the canyon is a veritable poster child of groundwater seepage erosion. But this new study posits evidence that the canyon?s formation was caused rather by catastrophic megaflood 45,000 years ago. Their results imply that flooding of this kind may have caused similar features on Mars. [Source: NAI Newsletter]

February 18, 2008

2/25 Director's Seminar: "Can Rocks from Mars Yield Definitive Evidence of Past Life?"

Presenter: J. William Schopf
Date/Time: 2/25/2008 11:00 AM PST

Throughout recorded Earth history, microbial life has been ubiquitous, abundant, metabolically diverse, and, for the Precambrian four billion years of geologic time, biotically predominant. In the search for life elsewhere in the Cosmos, the prokaryote-dominated world of the Precambrian is the best analogue we know. Though evidence of microbe-level life will thus be sought in rocks returned from Mars, for the first such missions only minimal samples will be available. This raises important questions: What amount of rock is needed to detect past life? What evidence is required to establish biogenicity? How can true fossils be distinguished from contaminants?

Continue reading "2/25 Director's Seminar: "Can Rocks from Mars Yield Definitive Evidence of Past Life?"" »

January 2, 2008

Hydrogeologic Controls on Episodic H2 Release from Precambrian Fractured Rocks--Energy for Deep Subsurface Life on Earth and Mars

Astrobiology December 2007, 7(6): 971-986

http://www.liebertonline.com/doi/pdfplus/10.1089/ast.2006.0096

Dissolved H2 concentrations up to the mM range and H2 levels up to 9-58% by volume in the free gas phase are reported for groundwaters at sites in the Precambrian shields of Canada and Finland. Along with previously reported dissolved H2 concentrations up to 7.4 mM for groundwaters from the Witwatersrand Basin, South Africa, these findings indicate that deep Precambrian Shield fracture waters contain some of the highest levels of dissolved H2 ever reported and represent a potentially important energy-rich environment for subsurface microbial life. The

Continue reading "Hydrogeologic Controls on Episodic H2 Release from Precambrian Fractured Rocks--Energy for Deep Subsurface Life on Earth and Mars" »

October 1, 2007

Martian Ice Ages

Norbert Schorghofer of NAI's University of Hawai'i Team has a new paper in Nature describing a climate model he developed which accounts for the advance and retreat of the subsurface martian ice layers. The model reveals forty major ice ages over the past five million years, and explains the present distribution of subsurface ice on Mars. His findings outline expectations of ice stratigraphy at the NASA Mars Phoenix Mission's landing site.

Source: NAI Newsletter

July 10, 2007

Evidence for Ancient Ocean on Mars

Scientists from NAI's University of California, Berkeley Team have a new paper out in Nature outlining evidence for the presence of an ancient ocean on Mars. The study points to a large body of liquid water at the pole which could have shifted Mars' spin axis. This shift would have in turn deformed the shoreline of this ocean relative to the rest of the surface topography, in accordance with observations. [Source: NAI Newsletter]

Methane in the Martian Atmosphere

Scientists from NAI's IPTAI Team have a paper out in Geophysical Research Letters detailing a new mechanism for recent methane release on Mars. Their results show that increasing salinity can cause destabilization of subsurface methane hydrates, and that active thermal or pressure fluctuations are not required to account for the presence of methane in the atmosphere. [Source: NAI Newsletter]

June 21, 2007

Mars Special Regions Meeting at COSPAR

Jennifer Heldmann has been invited to participate in a special COSPAR Colloquium on Mars Special Regions. This meeting is an essential step in developing an international consensus on the definition of "special" regions on Mars, which will in-turn determine the application of planetary protection requirements for future Mars lander missions. This 3-day meeting will take place in Rome, Italy on 18-20 September 2007. For more on COSPAR Colloquia visit: http://cosparhq.cnes.fr/Meetings/Colloq.htm

October 19, 2006

The Habitability of Mars: Past and Present

Tom McCollum of the University of Colorado, Boulder team has recently contributed a chapter titled "The Habitability of Mars: Past and Present" that appears in the book "Solar System Update", published this summer by Praxis Publishing. The chapter summarizes current thinking about current and past conditions on Mars that might allow life to exist there.

Continue reading "The Habitability of Mars: Past and Present" »

July 25, 2006

Follow The Water

NASA Mars Picture of the Day: Gullied Recesses

"This image shows gullies on the wall of a martian south mid-latitude impact crater. The channels in each gully head beneath an eroding overhang of layered rock, providing support for the hypothesis that some—if not all—martian gullies result from release of groundwater to the surface."

July 23, 2006

Green ice, Ravens, Ice Caves and the Movie ‘Contact’

Towards the end of our summer expedition while flying back to Eureka from our camp on Axel Heiberg, I spotted a lake with what appeared to be green ice on it.

Continue reading "Green ice, Ravens, Ice Caves and the Movie ‘Contact’" »

May 28, 2006

MARS Journal open for submissions

The MARS Journal, a new online peer reviewed open access journal, is now open for submission of manuscripts. The MARS Journal will publish scholarly papers in three general categories:

Mars Science: Observations, data, theory, models, and reviews of scientific literature Mars Technology: Instruments, spacecraft, missions, tools and techniques, and software Mars Policy: Exploration strategy, economics, planetary protection, history, and commentary Be among the first to publish (for free) in The MARS Journal.

See: http://marsjournal.org

May 26, 2006

NRC Report on Next Decade Mars Architecture

"Review of the Next Decade Mars Architecture" is tentatively scheduled for release during June. However, release dates of National Academies reports depend on successful completion of the review process and on printing schedules.

This report evaluates NASA's Mars exploration program for the next 10 years, and looks at whether it optimizes scientific returns, given the agency's current funding limitations. The report also discusses whether the program incorporates findings from current missions and follows guidelines outlined in a previous report from the Research Council.

Continue reading "NRC Report on Next Decade Mars Architecture" »

February 14, 2005

NRC Report: Safe on Mars

Safe on Mars, Astrobiology Magazine

"The National Research Council was tasked with evaluating the risks of landing humans safely to work on Mars. Their report highlights a number of unique aspects in transit to the red planet, as well as once humans step out onto the surface."

Copyright © 2010 SpaceRef Interactive Inc. All rights reserved. Privacy Policy.

Links