06 January 2009

SpaceViz's New Video on Planetary Defense


Alternate Streaming site:
http://www.spaceviz.com/documentaries/planetarydefense/planetarydefense.html
Who will save Earth?Scientists and the military have only recently awakened to the notion that impacts with Earth do happen. "Planetary Defense" meets with both the scientific and military communities to study our options to mitigate an impact from asteroids and comets, collectively known as NEO's (Near Earth Objects). “Civilization is ill prepared for the inevitable. It's not if an impact will happen with the Earth, it's when!”

Looks to contain an all star cast, including David Morrison, Dr. Simon "Pete" Worden, Duncan Steel, Michael Belton,

National Academies Takes Up Planetary Defense

http://www7.nationalacademies.org/ssb/NEO_surveys_mitigation.html#P16_19

Request for InformationTo: Members of the Space Science and Technology Community From: Irwin Shapiro, Chair, and Faith Vilas and Michael A’Hearn, Vice ChairsNRC Committee to Review Near-Earth Object Surveys and Hazard Mitigation StrategiesDate: December 17, 2008The Space Studies Board, in coordination with the Aeronautics and Space Engineering Board of the National Research Council (NRC), is beginning a two-part study to address issues concerning the detection, tracking, and characterization of potentially hazardous Near-Earth Objects (NEOs), and approaches to mitigating identified hazards. Both tasks will include an assessment of the costs of various alternatives, using independent cost estimating. More information about the committee can be found at: http://www7.nationalacademies.org/ssb/NEO_surveys_mitigation.html#P16_19To obtain the greatest possible input of ideas from the community about issues in surveying, detecting, and characterizing NEOs, as well as potential mission concepts for deflection/mitigation, we are soliciting information in these areas. Submitters may draw upon the use of different facilities (ground- or space-based), and/or involve international cooperation, in their proposed solutions.We invite you to write a program or mission concept for detecting, characterizing, or mitigating the hazards of NEOs, due by March 20, 2009. For logistical reasons, we ask that you first submit a Letter of Intent (LOI) by January 30, 2009. LOIs should be no longer than 1 page and include the authoring organization’s name and a short (no more than 200 words) description of the proposed solution.The NRC’s Committee to Review Near-Earth Object Surveys and Hazard Mitigation Strategies may select several proposed solutions for further study and invite the author of each to make a formal presentation at a future committee meeting. Identification of promising solutions by the committee does not imply future study funding by NASA or any other entity.Solutions should be devoted to detecting, characterizing, or mitigating NEOs; authors wishing to address two or more tasks should submit separate solutions for each. Authors may also submit as many separate solutions as they wish.The committee will use the following general criteria in evaluating submissions:1-The relative technical feasibility of the solutions; 2-The cost range into which each solution is likely to fall; and3-The relative merits of solutions and whether they outweigh their inherent challenges.More specific aspects of criterion 3 for the different types of proposed solutions are:i. Detecting and surveying NEOs: Does the proposal realistically address the requirements set by Congress for NASA to detect 90% of NEOs with perihelion distances of less than 1.3 astronomical units that are 140 meters in diameter or larger by 2020?ii. Characterizing NEOs: Does the proposal focus on any or all of the various key characteristics of any target, such as its size, density, composition, and inclination and speed of approach?iii. Hazard mitigation: Does the proposed solution offer a technically feasible method of deflecting an asteroid impact? Have the merits of the proposal been adequately compared to its disadvantages (if any), including the possibility of reduced costs over alternative courses of action? How much technical development is required for implementation? All responses will be considered non-proprietary public information for distribution with attribution. Those submitting responses must also fill out the relevant (i.e., government or non-government) NRC copyright form provided on the committee’s website.The proposed solutions should be no longer than ten pages in length (12-point font) and involve the following items (by numbered sections):
1. A summary of the proposal;
2. Preliminary cost estimates*; and
3. A summary of the advantages and disadvantages of your proposed method for detecting, characterizing, or mitigating the hazards of Near Earth Objects.
Please submit your LOI to the NRC by January 30, 2009 via email to neorfi@nas.edu.Please submit your proposed solution(s) to the NRC by March 20, 2009 via email to neorfi@nas.edu.Questions about the RFI may be directed to the study director, Dwayne A. Day (dday@nas.edu), or to us: (ishapiro@cfa.harvard.edu); (fvilas@mmto.org); (ma@astro.umd.edu).You can also contact Dr. Day by telephone at 202-334-3477, or by fax at 202-334-3701.* We recognize the lack of accuracy of cost estimates for space missions in the early conceptual stages of development. You may consider using the NASA Advanced Missions Cost Model located at http://cost.jsc.nasa.gov/AMCM.html to determine approximate costs.

Statement of Task
The National Research Council Space Studies Board, in cooperation with the Aeronautics and Space Engineering Board, shall conduct a two-part study to address issues in the detection of potentially hazardous NEOs and approaches to mitigating identified hazards. Both tasks should include an assessment of the costs of various alternatives, using independent cost estimating. Options that blend the use of different facilities (ground- or space-based), or involve international cooperation, may be considered. Each study phase will result in a report to be delivered on the schedule provided in the contract. Key questions to be addressed during each phase of the study are the following:Task 1: NEO Surveys What is the optimal approach to completing the NEO census called for in the George E. Brown, Jr. Near-Earth Object Survey section of the 2005 NASA Authorization Act to detect, track, catalogue and characterize the physical characteristics of at least 90% of potentially hazardous NEOs larger than 140 meters in diameter by the end of year 2020? Specific issues to be considered include, but are not limited to, the following:
• What observational, data-reduction, and data-analysis resources are necessary to achieve the Congressional mandate of detecting, tracking, and cataloguing the NEO population of interest?
• What physical characteristics of individual objects above and beyond the determination of accurate orbits should be obtained during the survey to support mitigation efforts?
• What role could be played by the National Science Foundation's Arecibo Observatory in characterizing these objects?
• What are possible roles of other ground- and space-based facilities in addressing survey goals, e.g., potential contributions of the Large Synoptic Survey Telescope (LSST) and the Panoramic Survey Telescope and Rapid Response System (Pan STARRS)?
Task 2: NEO Hazard Mitigation What is the optimal approach to developing a deflection capability, including options with a significant international component? Issues to be considered include, but are not limited to, the following:
• What mitigation strategy should be followed if a potentially hazardous NEO is identified?
• What are the relative merits and costs of various deflection scenarios that have been proposed?

21 December 2008

Head-Sized Meterorite Part Found.


Several more fragments have been found from the 10-ton asteroid that exploded over western Canada on November 20, including a head-sized piece weighing 13-kilograms (28 lbs). Imagine that landing on your house or car (or head!). University of Calgary professor Alan Hildebrand, who is leading the search estimates there could be 2,000 fragments per hectare (about 2.5 acres) in the area near where fragments were initially found. The asteroid is becoming known as the Buzzard Coulee fireball, named after the picturesque, but luckily uninhabited valley where the first pieces were located. Check out the website of Bruce McCurdy of Edmonton Space & Science Foundation and the Royal Astronomical Society of Canada, who has joined in the search for more meteorite images.
More than two dozen pieces of the asteroid have been found by researchers or members of the public. The search is focused on a 24-square-kilometer section of agricultural land along the Battle River where the scientists calculated the debris would be located.

Obama Transition team considering SSP



DynaSoar writes "President-elect Obama's transition team has published for public comment a white paper entitled Space Solar Power (SSP) — A Solution for Energy Independence & Climate Change. The paper was prepared and submitted by the Space Frontier Foundation and other citizen space advocates, and calls for the new Administration to make development of Space Solar Power a national priority. The SSP white paper was among the first ten released by the Obama transition team. It is the first and only space-related white paper released by the team to date. With 145 comments thus far, it is already among the top five most-discussed of the 20-some white papers on Change.gov."


Check out the direct link:

25 November 2008

Giant Camera Tracks Asteroids



Giant Camera Tracks Asteroids
The camera will offer sharper, broader views of the sky.
By Robert Lemos

The first of four new asteroid-tracking telescopes will come online next month in Hawaii, promising to quickly scan large swaths of the sky--thanks to the world's largest digital camera.

The project, known as the Panoramic Survey Telescope and Rapid Response System (Pan-STARRS), aims to scan the entire sky visible from the summit of Mount Haleakala in Maui Island, Hawaii, three times a month, searching for asteroids and near-Earth objects (NEOs) as small as 300 meters in diameter. At the heart of each telescope is a 1.4-billion-pixel digital camera that can photograph broad swaths of the night sky in sharp detail.

The first prototype telescope using the camera will go online in December. This telescope will scan the night sky, searching for asteroids and comets that could pose a threat to Earth. Pan-STARRS is designed to have at least three times the collecting power of current NEO telescopes.

The Pan-STARRS's cameras, each consisting of a 40-centimeter-square array of charge-coupled devices (CCDs), bring new technology to the optics used in astronomy. Perhaps the most innovative aspect is the ability of each CCD cell to electronically shift an image to counteract atmospheric blur and deliver clearer astrophotography, says Barry Burke, a senior staff member at MIT's Lincoln Laboratory, which makes the cameras.

"The atmosphere is the limit to the quality of the image, but there is a special feature of these chips that allows them to remove some of the blur due to atmospheric effects," Burke says. "It allows the image to be shifted in any direction in the chip in a way that matches the motion of the stars and that takes out a significant part of the blur."

Known as orthogonal transfer CCD (OTCCD), the technology uses electronics to adjust the image rather than mechanically tilting a camera's lens or mirror, a more common technique used in consumer cameras that have optical image stabilization. Because the process is electronic, the technology can be distributed to each cell of the CCD array, allowing for much more granular adjustments to localized atmospheric turbulence. The result is an image that is sharper than what a ground-based observatory could produce.

The mosaic structure of the CCD camera also leads to a more reliable system and less expensive manufacturing costs, Burke says. "The chip could not possibly be made to that size, so we are forced to break the camera down into tiles," he says.

Each Pan-STARRS camera consists of an eight-by-eight array of devices, each containing an eight-by-eight array of CCD cells. The size of each cell--about six millimeters on a side--is determined by a sweet spot...

Space experts call for asteroid action plan

From: http://www.msnbc.msn.com/id/27910044/
Space experts call for asteroid action plan
Time needed to deflect asteroids, evacuate people living in impact zone
updated 11:55 a.m. ET, Tues., Nov. 25, 2008
VIENNA, Austria - Space experts are urging the United Nations to devise a plan that allows for quick action against asteroids. Rusty Schweickart, a former U.S. astronaut, says such a plan would save the time needed to deflect asteroids or evacuate people living in a possible impact zone. He says researchers will increasingly be able to predict collisions and that, for the first time in history, technical capabilities exist to prevent them. Schweickart and other experts spoke to reporters Tuesday after presenting a report on the matter to U.N. officials in Vienna.

24 November 2008

All-Sky Camera Network



One method by which meteors can be observed & tracked.

Did Asteroid Cause Ancient N.Y. Tsunami?




Long before New York City was the Big Apple, or even New Amsterdam, a giant tsunami crashed ashore.
It was 2,300 years ago. The Palisades that frame the Hudson River were whisper-quiet, the sandy beaches of Long Island and New Jersey empty, and Manhattan was still just an unbroken sylvan carpet.
Then came the mammoth wave, roaring into the serenity. No one knows for sure what caused it, but new clues found in the Hudson's silt suggest an asteroid 100 meters (330 feet) in diameter slammed into the Atlantic Ocean nearby.
While sifting through samples, Katherine Cagen of Harvard University and a team of researchers found carbon spherules -- perfectly round particles that form in the extreme pressures of an impact.
"But the main thing that closes the deal is that we looked in the spherules and found nano-diamonds," said Dallas Abbott of Columbia University, a co-author on the work. "These have only been found in impact ejecta or in meteorites."
The team found grains of several shocked minerals in the sediments as well, but the discovery remains controversial.
"To get a wave 2.5 meters high that far up the Hudson, you need a wave 20 meters high at Manhattan," said Steven Ward of the University of California, Santa Cruz. "It would've gone several hundred meters inland on Long Island; you should see evidence of this thing all over the place."
Bunch of terrific Asteroid/Tidal Wave Sims here: http://es.ucsc.edu/~ward/

$10,000 to anyone who can locate and give him the first one-kilogram chunk


This meteor was thought to generate only about 1/3 KT (from 10% luminous efficiency based on measured irradiance), which would make it significantly smaller (less than half) than 2008TC3 which impacted the atmosphere over Sudan (see earlier posts). The Canadians are apparently feverishly working to estimate the fall area and recover fragments before the first snow.



This particular meteor was thought to weigh about one to seven tonnes before it entered the Earth's atmosphere, and was five times as bright as a full moon.

He said the people with the best chance of finding pieces are the ones who heard the sonic boom made by the falling meteorite chunks.
"If you hear that, then you're probably within 30 kilometres of it."

22 November 2008

Amazing Video of Meteor over Canada

http://www.youtube.com/watch?v=e_2aX-784sw&NR=1
http://www.youtube.com/watch?v=PSL3b6bCR7s&NR=1
http://www.youtube.com/watch?v=e_2aX-784sw
About 1730 yesterday, in Edmonton, Canada:
From: http://www.google.com/hostednews/canadianpress/article/ALeqM5jU4E6gEY14ICcUMiwnqPkveUsF3w
"I just happened to look outside facing east," he said. "All of a sudden I saw this big flash coming down and I thought somebody was playing tricks on me, like fireworks behind the house or something.
"Just before that I heard a boom. I didn't know if it was a tree against the house. It was green and blue and it was coming down pretty fast."
Gobeil said the light display eventually turned orange, yellow and red and lasted 10 seconds.
"I was waiting for it to explode," he said. "It looked similar to when we watch (news reports) in Afghanistan. When I didn't see that, I said, 'well, that's something from outer space.' I'm sure it landed way out in Winnipeg or something."
"It's exciting - both scary and really nice."

10 November 2008

Future Channel Posts new video on Space Solar Power

A new video for math and science classrooms:

http://www.thefutureschannel.com/dockets/realworld/space_based_solar_power/
To consider the space solar power concept requires an understanding of science, technology, engineering, math, energy, policy, environmental factors, and more. Space solar power is an engineering project on a scale that rivals the greatest in history. Students need to be informed and able to participate in the conversation.

Image of TC3 in Sky


A month after asteroid 2008 TC3 hit the Earth's atmosphere, the first ground-based image of the event has surfaced on the Internet. Admittedly, it's not the fireball everyone has been waiting to see, but it is visual evidence that something hit us above Sudan on October 7th. The image above was taken from a frame of video that was being recorded by Mr. Mohamed Elhassan Abdelatif Mahir in the dawn following the asteroid impact with the atmosphere. The smoky feature is the remnant of the fireball as the 3 meter-wide asteroid blasted through the upper atmosphere, eventually exploding. The long-lasting persistent train is seen hanging in the air, high altitude winds causing it to twist in the morning sunlight.
We may not have a dazzling fireball re-entry video of 2008 TC3, but this striking image provides the first ground-based evidence of the direct hit, and may help refine the search for any meteorites from the disintegrated asteroid…

27 October 2008

Energy Biz: Japan has high hopes for Space Solar Power




From: http://energycentral.fileburst.com/EnergyBizOnline/2008-5-sep-oct/Tech_Frontier_Solar_Space.pdf
Japan is working hard toadvance its laser and microwave research so that solar power generated in space can be beamed to Earth in two decades, Scientific American reported this summer. By 2030, the Japanese hope to generate 1,000 megawatts at an orbiting solar generator and transport it to Earth. To learn more about the effort, EnergyBiz e-mailed questions to Hiroaki Suzuki with the Japan Aerospace Exploration Agency, also known as JAXA. He is one of 180 Japanese scientists working on the program, according to Scientific American. It also reported that the ultimate cost of such a project could climb to tens of billions of dollars, but the Japanese are intent on mastering the technology first, and then driving down the cost to levels that are competitive.
We have investigated two types of space solar panel systems, laser and microwave.With laser-based systems, Earth-orbiting solar condenser mirrors concentrate solar energy and divert it to laser amplifiers. A direct solar pumping solid-state laser diode uses the concentrated solar energy to amplify a low-power seed laser beam. The amplified laser beam is transmitted to Earth. Thus, this type of system uses no solar cell panels. Radiators dissipate the laser generator’s waste heat into space. A ground-based photovoltaic device converts the transmitted laser beam into electricity. This system can also be used to produce hydrogen with photocatalytic hydrogen generation or water electrolysis.With microwave-based systems, primary mirrors collect solar energy that solar panels convert to electricity that powers semiconductordevices to generate a microwave beam. A ground-based rectifying antenna array collects the transmitted microwave beam and converts it into electricity that is supplied to commercial power grids.
In the elemental technology development study, a laser amplifier with a direct solar pumping solid-state laser diode made of yttrium aluminum garnet ceramic doped with neodymium and chromium is being studied. The atmospheric transmittal propertiesof a high-energy laser beam and beam-pointing technology are studied for their applications in a laser-based system. For the microwave-based system, a large-scale phased array antenna, microwave amplifier, retro-directive beam control, and rectifying antenna are being studied. For both systems, a large-scale, ultra-light reflective mirror is also studied.
In the ground energy transmission demonstration, a kilowatt-class experiment for laser and microwave system is planned and is expected to be conducted within five years.System concepts and architectures of commercial-grade microwave- and laser-based space solar panel systems have been studied for years. System concepts and architectures have been developed and associated key technologieshave been identified.
Although a preliminarycost estimate has been conducted, it includes a lot of ambiguities. We are not ready to show you our cost analysis. We expect space solar panel systems will be competitive with the existing power plants in 20 to 30 years, if the space transportation cost is considerably reduced. It should be noted that solar systems do not emit CO2, nor do they create nuclear waste.
We are proposing a roadmap that consists of a stepped approach to achieve 1-gigawatt-class commercial space solar panel systems in 20 to 30 years. That means 2030 would see the very beginning of commercial systems. We expect the ultimate percentage of electricity derived from space will be more than several tens of percent. By the way, Japanese total electricity generation was about 275 gigawatts or 990,000 gigawatt-hours in 2005.

26 October 2008

NSS PositionPaper on Space Solar Power

Exerpts From: http://www.nss.org/legislative/positions/NSS-SSP-PositionPaper.pdf
Space Solar Power: An Investment for Today – An Energy Solution for Tomorrow
October 2007
The United States and the rest of the world need to find alternative sources of energy besides fossil fuels. The National Space Society believes that one of the most important long-term solutions for meeting those energy needs is Space Solar Power (SSP), which gathers energy from sunlight in space and sends it to Earth. We believe that SSP can solve our energy and greenhouse gas emissions problems. Not just help, not just take a step in the right direction; solve. SSP can provide large quantities of energy to each and every person on Earth with very little environmental impact. The NSS recommends that SSP be considered along with ground-based solar collectors and wind turbines as a safe, renewable, and clean energy option.
Solar energy is routinely used on spacecraft today, and the solar energy available in space is literally billions of times greater than we use today. The lifetime of the sun is an estimated 4 to 5 billion years, making SSP a truly long-term energy solution. Space solar power can have an extremely small environmental footprint, perhaps competitive with ground-solar and wind, because with sufficient investments in space infrastructure, the SSP can be built from materials from space with zero terrestrial environmental impact. Only energy receivers need be built on Earth. As Earth receives only one part in 2.3 billion of the sun's output, SSP is by far the largest
potential energy source available, dwarfing all others combined. Development cost and time, of course, are considerable. This makes SSP a long-term solution rather than a short-term stop-gap, although there are some intriguing near-term possibilities.... While all viable energy options should be pursued with vigor, SSP has a number of substantial advantages over other energy sources...
All of these technologies are consistent with the laws of physics, are reasonably nearterm, and have multiple attractive approaches. However, a great deal of work is needed to develop economically competitive space solar power. The NSS encourages both the private sector and governments to devote substantial resources toward SSP research and development.
SSP deserves a place alongside ground-based solar collectors, nuclear power plants, and
wind turbines as potential solutions to energy dependence and global greenhouse-gasinduced
warming
. If SSP is given serious consideration, NSS expects it will play a growing, and perhaps dominant, role in providing safe, clean, renewable energy for our planet for the foreseeable future and beyond.
The Vision of NSS is people living and working in thriving communities beyond the Earth, and the use of the vast resources of space for the dramatic betterment of humanity.
The Mission of NSS is to promote social, economic, technological, and political change in order to expand civilization beyond Earth, to settle space and to use the resulting resources to build a hopeful and prosperous future for humanity. Accordingly, we support steps toward this goal, including human spaceflight, commercial space development, space exploration, space applications, space resource utilization, robotic precursors, defense against asteroids, relevant science, and space settlement oriented education.

Read more about Space Solar at NSS web page: http://www.nss.org/settlement/ssp/index.htm

By the way, recently the National Space Society has constructed tremendous on-line resources for information on Space Solar and Planetary Defense can be found here:
Space Solar Library:http://www.nss.org/settlement/ssp/library/index.htm

New Space Industrialization Video & Libraries

New pro-Space Industrialization video:
http://www.youtube.com/watch?v=MBnJLPpGIGQ

US Chamber Endorses Space Solar

From:
The appropriate policy question is: "Should the U.S. Government invest in SBSP research, as part of a diversified portfolio of renewable energy programs, including consideration of new approaches that may not have been previously studied?" Our answer to that question is yes. We must explore all potentially significant sources of sustainable energy that might contribute, even if only to a limited extent in the near term, to assurance of security and prosperity. Facing this challenge represents a responsibility not only to our own nation but also to the global community in which we live.
SBSP should be addressed through an incremental roadmap approach, involving both Government and private sector investment. This roadmap should be constructed to address at the outset key questions about SBSP, including technical viability and cost-effectiveness. The roadmap should consist of a series of milestones, each built on the availability of information generated by prior research. If research results are positive, each milestone should lead to increased government and private sector effort and investment. If justified by research findings, a move from research to demonstration projects should be initiated. Beyond this, milestones should be designed to maximize opportunities for multiple applications of research results, so that improvements in existing technologies and development of new ones could have near-term applications in addition to SBSP (e.g., communications satellite power supplies, terrestrial solar power generation).
The Space Enterprise Council of the U.S. Chamber of Commerce supports the National Security Space Office recommendation of a research program addressing space-based solar power, to explore whether or not this potential energy source could enhance commerce and security. The importance of alternative energy research is becoming increasingly clear, given the urgency of the national and global need for energy that is inexhaustible, affordable, and environmentally clean. Assuring access to energy is particularly relevant to U.S. national security, not only for supply of reliable power to deployed forces but also for avoiding international conflicts that might arise because of energy shortages.

SBSP is unusual among renewable energy options because it might satisfy all four of the following criteria critical to investment decisions: environmental cleanliness, sustainability of supply, flexibility of location, and capacity to generate continuous rather than intermittent power. The cost of SBSP-generated electricity would initially be greater than that provided by fossil fuel or nuclear power but could be comparable to other alternative energy sources, particularly for baseload power. In addition, SBSP might offer an attractive approach, not only for satisfying today's needs but also for meeting tomorrow’s much greater requirements. We cannot accurately predict environmental and other consequences of harvesting energy from natural Earthbound sources (e.g., wind, ocean current, geothermal, biofuels), when these methods are scaled up to considerably higher levels. By providing an additional source of renewable energy, SBSP might help avoid potentially negative consequences if limits to the cost-effective expansion of other renewable sources become evident. Beyond enhancement of energy production per se, SBSP might help create new economic opportunities through resultant technology advances in space launch, space utilization, and technological spin-offs applicable to a host of materials and processes. For example, SBSP research might lead to improvements in the efficiency of solar cells that power communications satellites, as well as power management systems for terrestrial solar power systems. Also, to the extent that SBSP is integrated into terrestrial solar power production, development of SBSP ground infrastructure might generate revenue even before deployment of systems in space. In this and related applications, SBSP could emerge as an enhancement for, rather than a competitor with, terrestrial solar power generation.



Space Solar News

From: http://indiapost.com/article/usnews/4044/
Targeting India on climate change is unfair: PranabSunday, 10.05.2008, 09:24pm (GMT-7)India Post News Service. Indian External Affairs Minister Pranab Mukherjee before an enlightened audience at the Asia Society in New York on Sept 30...his speech on 'India and Global Challenges: Climate Change and Energy Security', which was part of a series of talks by Asian leaders hosted by the Asia Society at its New York headquarters in conjunction with the opening of the United Nations General Assembly (UNGA) from September 22 to October 3.
"Later, during a question-answer session, the External Affairs Minister said that despite having vast deposits of thorium, India could not pursue production of nuclear energy as access to critical nuclear technology was denied to it over the last 30 years. He said India was now collaborating closely with the US to tap space solar power."
His remarks follow the call at the 2007 International Astronomical Congress for a Global Aerospace Mission in Space and Energy to realize Space Solar Power. Dr. Kalam's speech here, particularly about 40 minutes in:
And Dr. Kalam (then India's President), laid out space as among the greenest technologies, laying out the challenge of space solar power:
Perhaps significant, considering the recent headline:
Obama says India will be top priority
A stronger relationship with India and a close strategic partnership will be a 'top priority' of a Barack Obama administration, says the Democratic presidential candidate. "The US should be working with India on a range of critical issues from preventing terrorism to promoting peace and stability in Asia," Senator Obama said in an exclusive interview. "Joe Biden and I will make building a stronger relationship, including a close strategic partnership, with India a top priority." On his agenda for working with New Delhi, he said, "I also believe India is a natural strategic partner for America in the 21st century and that the US should be working with India on a range of critical issues from preventing terrorism to promoting peace and stability in Asia."
This follows earlier, and longstanding remarks of his running mate:
http://www.cfr.org/bios/1451/joseph_r_biden_jr.html
Biden (D-DE) called U.S. ties with India the “single most important relationship that we have to get right for our own safety's sake” (Rediff.com).
And for the United States, no relationship is more important than the one we are building with India.” — Senator Joseph Biden, November 16, 2006

Neil Tyson on CNN/D.L. Hughley Obama & Asteroids

Hillarious interview with Neil Tyson tonight on CNN late night comedy news talk show host D.L. Hughley:
http://www.youtube.com/watch?v=uhXOwlXfsug


25 October 2008

HR 6063 Becomes Law!

On Oct 15, the President signed HR 6063, the 2008 NASA Authorization Act into Law. Find the full text here: http://www.govtrack.us/congress/billtext.xpd?bill=h110-6063
Most significantly, it contains the following language:
TITLE VIII--NEAR-EARTH OBJECTS
SEC. 801. REAFFIRMATION OF POLICY.
(a) Reaffirmation of Policy on Surveying Near-Earth Asteroids and Comets- Congress reaffirms the policy (g)) (relating to surveying42 U.S.C. 2451set forth in section 102(g) of the National Aeronautics and Space Act of 1958 (near-Earth42 U.S.C. 2451(g)) (relating to surveying near-Earth asteroids and comets).
(b) Sense of Congress on Benefits of Near-Earth Object Program Activities- It is the sense of Congress that the near-Earth object program activities of NASA will provide benefits to the scientific and exploration activities of NASA.
SEC. 802. FINDINGS.
Congress makes the following findings:
(1) Near-Earth objects pose a serious and credible threat to humankind, as many scientists believe that a major asteroid or comet was responsible for the mass extinction of the majority of the Earth’s species, including the dinosaurs, nearly 65,000,000 years ago.
(2) Several such near-Earth objects have only been discovered within days of the objects’ closest approach to Earth and recent discoveries of such large objects indicate that many large near-Earth objects remain undiscovered.
(3) Asteroid and comet collisions rank as one of the most costly natural disasters that can occur.
(4) The time needed to eliminate or mitigate the threat of a collision of a potentially hazardous near-Earth object with Earth is measured in decades.
(5) Unlike earthquakes and hurricanes, asteroids and comets can provide adequate collision information, enabling the United States to include both asteroid-collision and comet-collision disaster recovery and disaster avoidance in its public-safety structure.
(6) Basic information is needed for technical and policy decisionmaking for the United States to create a comprehensive program in order to be ready to eliminate and mitigate the serious and credible threats to humankind posed by potentially hazardous near-Earth asteroids and comets.
(7) As a first step to eliminate and to mitigate the risk of such collisions, situation and decision analysis processes, as well as procedures and system resources, must be in place well before a collision threat becomes known.
SEC. 803. REQUESTS FOR INFORMATION.
The Administrator shall issue requests for information on--
(1) a low-cost space mission with the purpose of rendezvousing with, attaching a tracking device, and characterizing the Apophis asteroid; and
(2) a medium-sized space mission with the purpose of detecting near-Earth objects equal to or greater than 140 meters in diameter.
SEC. 804. ESTABLISHMENT OF POLICY WITH RESPECT TO THREATS POSED BY NEAR-EARTH OBJECTS.
Within 2 years after the date of enactment of this Act, the Director of the OSTP shall--
(1) develop a policy for notifying Federal agencies and relevant emergency response institutions of an impending near-Earth object threat, if near-term public safety is at risk; and
(2) recommend a Federal agency or agencies to be responsible for--
(A) protecting the United States from a near-Earth object that is expected to collide with Earth; and
(B) implementing a deflection campaign, in consultation with international bodies, should one be necessary.
SEC. 805. PLANETARY RADAR CAPABILITY.
The Administrator shall maintain a planetary radar that is comparable to the capability provided through the Deep Space Network Goldstone facility of NASA.
SEC. 806. ARECIBO OBSERVATORY.
Congress reiterates its support for the use of the Arecibo Observatory for NASA-funded near-Earth object-related activities. The Administrator, using funds authorized in section 101(a)(1)(B), shall ensure the availability of the Arecibo Observatory’s planetary radar to support these activities until the National Academies’ review of NASA’s approach for the survey and deflection of near-Earth objects, including a determination of the role of Arecibo, that was directed to be undertaken by the Fiscal Year 2008 Omnibus Appropriations Act, is completed.
SEC. 807. INTERNATIONAL RESOURCES.
It is the sense of Congress that, since an estimated 25,000 asteroids of concern have yet to be discovered and monitored, the United States should seek to obtain commitments for cooperation from other nations with significant resources for contributing to a thorough and timely search for such objects and an identification of their characteristics.
SEC. 1105. INNOVATION PRIZES.
(a) In General- Prizes can play a useful role in encouraging innovation in the development of technologies and products that can assist NASA in its aeronautics and space activities, and the use of such prizes by NASA should be encouraged.
(b) Amendments- Section 314 of the National Aeronautics and Space Act of 1958 is amended--
(1) by amending subsection (b) to read as follows:
‘(b) Topics- In selecting topics for prize competitions, the Administrator shall consult widely both within and outside the Federal Government, and may empanel advisory committees. The Administrator shall give consideration to prize goals such as the demonstration of the ability to provide energy to the lunar surface from space-based solar power systems, demonstration of innovative near-Earth object survey and deflection strategies, and innovative approaches to improving the safety and efficiency of aviation systems.’; and
(2) in subsection (i)(4) by striking ‘$10,000,000’ and inserting ‘$50,000,000’.

Canadian Asteroid Defense & Schedule of Events

Check out this new Canadian-based Global Asteroid Protection Society:

http://stoprocks.com/

They join a long-line of organizations which have called for action:
Space Frontier Foundation: https://webmail.hq.af.mil/exchweb/bin/redir.asp?URL=http://www.space-frontier.org/Projects/TheWatch/
Association of Space Explorers: https://webmail.hq.af.mil/exchweb/bin/redir.asp?URL=http://www.space-explorers.org/
B612: https://webmail.hq.af.mil/exchweb/bin/redir.asp?URL=http://www.b612foundation.org/press/press.html
ProSpace: https://webmail.hq.af.mil/exchweb/bin/redir.asp?URL=http://www.prospace.org/
Planetary Society: https://webmail.hq.af.mil/exchweb/bin/redir.asp?URL=http://www.planetary.org/programs/projects/apophis_competition/
AIAA: https://webmail.hq.af.mil/exchweb/bin/redir.asp?URL=http://www.aero.org/conferences/planetarydefense/ & position paper: https://webmail.hq.af.mil/exchweb/bin/redir.asp?URL=http://www.planetarydefense.info/resources/pdf/Asteroids-Final.pdf
Gaia Shield Group: https://webmail.hq.af.mil/exchweb/bin/redir.asp?URL=http://gaiashield.com/two.html
Lifeboat Foundation: https://webmail.hq.af.mil/exchweb/bin/redir.asp?URL=http://www.lifeboat.com/ex/asteroid.shield
Secure World: https://webmail.hq.af.mil/exchweb/bin/redir.asp?URL=http://75.125.200.178/~admin23/index.php?id=16%26page=Near_Earth_Objects
National Space Society: https://webmail.hq.af.mil/exchweb/bin/redir.asp?URL=http://www.nss.org/settlement/asteroids/
Marsdrive: https://webmail.hq.af.mil/exchweb/bin/redir.asp?URL=http://marsdrive.com/news/asteroid-to-hit-mars.html

Which reminds me, the Canadians have a project called NEOSat, which will spend half its time doing Space Situational Awarness, and the other half doing search for Asteroids. It will use a 15cm diameter telescope. It is about the size of suitcase, and weighs 65kg. They hope to launch it in 2010. Unfortunately, it still apparently needs to find an opportune ride to orbit...perhaps on a polar weather satellite.
http://mithridates.blogspot.com/2008/07/canada-to-launch-neosat-satellite-to.html
http://www.ctv.ca/servlet/ArticleNews/story/CTVNews/20080629/NEOsat_asteroids_080630?s_name=&no_ads=
http://www.ctv.ca/servlet/ArticleNews/story/CTVNews/20080626/asteroid_hunter_080626/20080626

The Europeans are also doing interesting work. They are pushing the asteroids onto the agenda for SSA. Currently they still have Don Quiote mission on the books, and one can hope against their troubles that they will not completely abandon it. Particularly in Britain, leading Study Group 14 for the UN COPUOS, and Dr. M. Vasile who is comparing a number of different methods continues to turn out useful work comparing various options.
http://space.newscientist.com/article/dn12761
Another interesting site that will get quite a bit more press early next year is the international Association of Space Explorers (ASE), theinternational organization of astronauts and cosmonauts from 33 countries:
http://www.space-explorers.org/committees/NEO/neo.html
Not in particular this paper, which says:
http://www.space-explorers.org/committees/NEO/docs/COSPAR-paper.pdf
- Within 10-15 will be tracking~300,000 NEOS =>45m (Tunguska Size) due to projected upgrades, of which 10,000 will have non-zero probability of earth impact in next 100 years and 50-100(.5-1%) are likely to appear threatening enough to warrant active monitoring or deflection!

Back in the US, the official site for the Iowa State Asteroid Deflection Center (ADRC), where eventually the presentations will be posted.
http://www.adrc.iastate.edu/

In fact, here is the layout for near term events:
- Dec 2008 - Dedicated National Space Society (NSS) Ad Astra magazine
- Spring 2009, Association of Space Explorers (ASE) issues its report, "Asteroid Threats: A Call for Global Response" to the United Nation's Committee on the Peaceful Uses of Outer Space
- March 23-27 Lunar & Planetary Science Conference
- April 23-24 Space Law Conference: Near Earth Objects (NEOs): Risks and Opportunities, Lincoln, Nebraska
- April 27-30 International Planetary Defense Conference, Grenada, Spain
www.congrex.nl/09c04/First_Announcement.pdf
- October 2010 National Research deadline of review of NASA NEO report to congress
- October 2010 The deadline for the Office of Science and Technology Policy (OSTP) to recommend a lead agency to Congress