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Comments by NAS Space Studies Board Chair Lennard Fisk, NAS
"There is consternation these days between the National Aeronautics and Space Administration (NASA) and its external science community. In August, three senior science advisors were dismissed from the NASA Advisory Council (NAC). In the aftermath, the Administrator of NASA, Mike Griffin, through correspondence with the NAC and its science subcommittees and through a major speech at the Goddard Space Flight Center, clarified how NASA will manage its science program, and the role of the science community."
- A Review of NASA's 2006 Draft Science Plan: Letter Report, NAS
- Science and NASA - Speech by NASA Administrator Michael Griffin
- 21 August 2006 Email from Mike Griffin to NASA Advisory Council Members
- Memo From NASA Advisory Council Chair Schmitt Regarding 3 NAC Resignations
- What Mike Griffin *Really* Thinks About NRC's Space Station Report
"I've read the report, and there is not much good in it for us. Not surprising, however, coming from Len Fisk ... The kind of criticism we're receiving in connection with the ISS, in the report Trish references, needs to be addressed for ISS, and needs to be "headed off at the pass" for the Moon."
Director's Corner - Message from NASA Astrobiology Institute Director Carl Pilcher, NAI
"The clearest expression that astrobiology doesn't "measure up" comes from the Administrator of NASA himself, Mike Griffin. Mike has testified before Congress that he does not see astrobiology as having the same importance as other components of the NASA science portfolio. He's also been quoted as saying that it has less intrinsic subject matter, is less advanced, and that its questions are more vague. Shortly before I left NASA Headquarters I had the opportunity to have an "elevator conversation" with Mike about some of his perceptions about astrobiology."
Join us for the next University of Washington Astrobiology Seminar! George Shaw of Union College will be speaking on the topic "A (not so) Brief History of Carbon on Earth." Date/Time: Tuesday, October 24, 2:30PM PDT (11:30am HT/3:30pm MDT/4:30pm CDT/5:30pm EDT)
Abstract: A (not so) Brief History of Carbon on Earth
It is widely agreed that carbon first arrived on Earth in a reduced form, as found in almost all meteorites, and was abiotic in origin. For more than thirty years, the prevailing view has been that the carbon in Earth's early atmosphere (and near surface environment) was virtually all in the form of carbon dioxide, the oxidized chemical state found in volcanic gases that are thought to be the source of atmospheric carbon compounds resulting from degassing of Earth's interior.
For about the same period of time there has also been broad agreement that a large fraction of the near-surface volatiles, including both water and carbon compounds, were degassed very early in Earth's history, implying a carbon dioxide rich early atmosphere. This has been thought by many to be a suitable explanation of the necessary enhanced greenhouse effect required to compensate for the early faint sun.
On the other hand there are several lines of evidence strongly at odds with this model for the early atmosphere:
1) Very early, Rubey pointed out the drastic geochemical and sedimentological consequences of a large CO2-rich atmosphere, including both severe weathering effects and consequent massive deposition of carbonate rocks, for which there is little or no evidence in the early Archean.
2) The delay in oxygenation of the atmosphere following the advent of oxygenic photosynthesis in cyanobacteria, as early as 2.8 BYBP (perhaps even earlier) is a long recognized (if often ignored) problem. Analysis of various sinks and nutrient constraints does not eliminate this problem.
3) The record of carbon isotopes in sediments points to a longstanding (at least since ca. 3.5 BYBP) balance between carbonate carbon and biogenic (fixed organic) carbon at a ratio of about 4 to 1. This implies substantial (and very early) fixation of large amounts of biogenic carbon and release of proportional amounts of free oxygen, which is inconsistent with geologic and isotopic evidence for an anoxic surface environment until ca. 2.1-2.3 BYBP.
These problems could be solved if one could identify a reservoir to hold the degassed carbon and release it into the biosphere on a geologic time scale. The lack of residual early Archean carbonate sediments (or metasediments) from such a hypothetical reservoir speaks against carbonate as the reservoir substance. The likelihood of early degassing precludes a deeper (e.g. upper mantle) reservoir. The only remaining choice is a reduced carbon reservoir at or near the surface. This reservoir cannot be atmospheric methane (or other gaseous hydrocarbon) because photochemical reactions rapidly remove such compounds from the atmosphere.
An early ocean with a high concentration of photochemically (and electrically) produced complex organic compounds solves all of these problems, with the added attraction that it is a favorable environment for the emergence of life. The oxidation of subducted organic rich sediments during upper mantle magmagenesis slowly provides CO2 to the surface environment, on a time scale consistent with the time scale for oxygenation of the surface environment by photosynthetic cyanobacteria, with the record of carbon isotopes in sedimentary rocks, and with the record of carbonate sedimentation.
An early reduced carbon reservoir at/near Earth's surface follows directly from early degassing, under reducing conditions, of the original (and/or hydrogenated) meteoritic carbon compounds. The largely methane atmosphere so produced is short lived, but the photochemical products accumulate in the ocean and are continuously recycled into the atmosphere as methane by low temperature hydrothermal activity. This model provides a suitable source of the early (methane) enhanced greenhouse effect.
For connection information and more, please visit http://nai.arc.nasa.gov/seminars/seminar_detail.cfm?ID=93 [Source: NAI Newsletter]
Andrey Bekker of the Geophysical Laboratory, and the NAI - Carnegie Institution of Washington Team and Ganqing Jiang from the Department of Geoscience, University of Nevada Las Vegas have organized a session at the upcoming Geological Society of America meeting in Philadelphia, October 22 - 25, 2006.
The NAI is sponsoring travel expenses for student and early career speakers at this special session, T139, entitled, "Changes in ocean and atmospheric redox state and the evolution of life".
For more information: http://gsa.confex.com/gsa/2006AM/finalprogram/session_18029.htm and http://gsa.confex.com/gsa/2006AM/finalprogram/session_18361.htm [Source: NAI Newsletter]
With this amendment to ROSES-2006, NASA establishes a new program element in Appendix A.24 entitled "International Polar Year (IPY) Education and Public Outreach."
This new program element solicits proposals to engage, inform, and inspire diverse public audiences by sharing our knowledge about polar science and its global connections during IPY and by communicating NASA's unique contributions to recent advances in Arctic and Antarctic research and climate science. A secondary objective is to extend the spirit of polar exploration and discovery to the poles of the Moon, Mars, and other planets of our solar system and to help attract and educate the next generation of scientists and engineers. This solicitation primarily seeks activities leveraging capabilities from existing projects or dissemination networks at zero or incremental cost for greater impact. Notices of Intent to propose are not requested, and proposals are due January 8, 2007.
On or about October 10, 2006, Amendment No. 16 to the NASA Research Announcement "Research Opportunities in Space and Earth Sciences (ROSES) 2006" (NNH06ZDA001N) will be posted on the NASA research opportunity homepage at http://nspires.nasaprs.com/ (select "Solicitations" then "Open Solicitations" then "NNH06ZDA001N").
Questions may be addressed to Dr. Ming-Ying Wei, Earth Science Division, Science Mission Directorate, NASA Headquarters, Washington, DC 20546-0001; Telephone: (202) 358-0771; Email: Ming-Ying.Wei-1@nasa.gov. [Source: NAI Newsletter]
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.
For more information: http://www.praxis-publishing.co.uk/view.asp?id=230&search=home [Source: NAI Newsletter]
The NASA Astrobiology Institute (NAI) and the National Science Foundation (NSF) are providing matching support towards the study of the ancient rock record of the early Earth, between 2.0 and 2.5 billion years ago. This period represents one of the critical transitions in the Earth's history as it reflects the emergence of the modern aerobic, or oxygen-rich Earth system.
Various lines of evidence continue to indicate that this period witnessed the rise of oxygen in the atmosphere of the Earth, reflecting major changes in the evolution of life on the planet. This project with acquire fresh, i.e., not weathered by surface exposure, drill-core material from deep within the Russian Arctic.
The NAI and NSF support will contribute to major funding from the International Continental Drilling Program, which will be led by investigators at the NAI Penn State University Team. [Source: NAI Newsletter]
"On Tuesday, October 17, the SETI Institute will unveil a new center to study life in the universe and a fund-raising strategy to counter NASA's proposed budget cuts for astrobiology research. From 10 to 11 a.m. at the SETI Institute in Mountain View, a distinguished panel of institute trustees and staff will announce the formation of the Carl Sagan Center for the Study of Life in the Universe. The center's activities will focus on astrobiology and be dedicated to the memory of planetary scientist and astronomer Carl Sagan. The panel will explain a new emphasis on fundraising from private sources to offset a proposed 50 percent budget cut by NASA for astrobiology research."
Exploration, Science, and Art: A Book Review of Terra Antarctica and Driving to Mars, SpaceRef
"When it comes to exploration, there's nothing like being there. Yet at some point, all explorers need to tell others what they have seen - as well as find a way to understand and recall the experience themselves. Exploration is pointless if it is not shared.
It is the process whereby explorers put new vistas and experiences into a context they can internalize - and then how these impressions are shared with others that fascinates author William Fox. In his two most recent books "Terra Antarctica" and "Driving to Mars" Fox recounts his own experiences - and those of others - at Earth's two poles."
This summer Miles Ecclestone of Trent University, returned to our camp next to Colour Lake to continue making improvements to the McGill Arctic Research Station (M.A.R.S.) as part of an infrastructure upgrade. During this time, I asked Miles to download the images from our Campbell Scientific met station’s camera which is pointed across part of the airstrip and part of Colour Lake. We now have daily images (most taken at 9am and again at 1pm) from 17 April 2006 to 17 August 2006. The video contains the stream of images at about 1 second each. My previous blog provides more details of the station and the camera we use.