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More than 100,000 asteroids hurtle past our planet. But only one—that we know of—may hit us in the next 30 years. Tag the killer asteroid and win $50,000 B612 and NASA Dialog on how to Deal with Apophis List Of The Potentially Hazardous Asteroids (PHAs) Asteroid 99942 Apophis Approaching Earth

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Planning For The End!
We Are Beginning The Process Of Thinking About Planetary Defense


From the 2007 NASA Report to Congress

In essence we only think we know of less than 10%
of the objects that threaten the Earth!

In 2008, the Future Concepts and Transformation Division (AF/A8XC) hosted a Natural Impact Event Interagency Planning Exercise, 4 Dec 2008, in Alexandria, Virginia. Twenty Seven Subject Matter Experts from across US Government, including DOD, DOE, DOS, DHS, NASA, and NSC participated in a single day tabletop exercise to explore "whole of government" response to an impending asteroid strike.

New Challenge Space - NEO Near Earth Objects


The specific scenario involved a mythical asteroid, "2008 Innoculatus." It was a binary asteroid consisting of a 270m rocky rubble pile projected to strike the Gulf of Guinea and a 50m metallic companion asteroid projected to strike in the National Capital Region (NCR). The scenario was selected to maximize exposure to the diversity of threat (variation in size, composition, land/water strike), stress both national and international notification, and provide useful pre-planning should an actual effort need to be mounted against the asteroid Apophis when it has a small probability to pass through a gravitational keyhole in 2029 and perhaps return to strike the Earth seven years later in 2036.

Players were broken into two teams. The first team focused on disaster response and was told the asteroid was discovered 72 hrs from impact. The second team focused on deflection/mitigation was told the asteroid had been discovered seven years from impact, and to design a "strawman" deflection plan using existing capabilities.

The major insights are summarized below (for an expanded discussion, see section 6):

1.1 The NEO impact scenario is not captured in existing plans.

While a number of useful analogs exist, as well as procedures that could be used or adapted, at the present time they have not been so adapted, and attempts to do so in the moment are likely to be much less successful than advance preparation.

1.2 The NEO impact scenario should be elevated to higher level exercises with more senior players.

Players suggested that the scenario was mature enough, interesting and compelling enough for elevation to higher levels of visibility and increased levels of detailed examination. Players suggested that National Planning Scenarios need to include a NEO impact as one of the scenarios. Players recommended incorporation of a NEO impact scenario into a number of formal planning exercises.

1.3 Proper planning and response to a NEO emergency requires delineation of organizational responsibilities including lead agency & notification standards.

Players consistently remarked that the complexities and overlapping nature of this contingency required advance delineation of responsibilities, formalization of the notification process, and clarification of authorities and chains of command, including authorities for delegation and supported/supporting relationships. Players thought it was important to think through and document this prior to any actual NEO emergency.

Understanding the Risk of High Consequence Low Frequency Events - Asteroid Impact

1.4 Players were not able to achieve consensus on which agency should lead the NEO deflection/mitigation effort.

No obvious consensus emerged on which agency should have lead for a deflection effort. Expertise is widely distributed across US government agencies. Players held widely divergent views in terms of organizational equities whose resolution will require a policy decision at a higher level. In the absence of policy guidance, players felt an actual deflection attempt would likely mirror the Manhattan Project

1.5 There is a deficit in software tools to support senior decision-making and strategic communication for disaster response & mitigation for an NEO scenario.
None of our command centers to support decision makers have the necessary tools to make quick assessments. Players expressed a need for a "National Decision Support System" for natural impact scenarios and events. Such a system would need to tighten up the federated nature of impact prediction and impact effects prediction, integrating models for impact location and uncertainty prediction, kinetic effects prediction, plume, and tsunami effects, and feed evacuation planning models

1.6 There are significant effects a NEO impact would generate that are not adequately captured in existing models.
Players highlighted the fact that current models inadequately address several effects likely to significantly affect accurate damage / effect estimates. These include the effect of blast plumes on Low Earth Orbit (LEO) satellites, electromagnetic effects that could affect electrical power infrastructure, seismic effects, effect of terrain on blast dissipation and focusing, coupling of airblast to tsunami response, and atmospheric distribution/dispersion of hazardous materials.

1.7 The public may be aware of an impending NEO impact before senior decisionmakers.
The NEO detection community conducts its work openly using Internet communications and Webbased datasets, so it is very likely that information on a new discovery of high interest will be available to the public before NASA can complete adequate verification and validation of potential impact and provide a news release, or even speed notification to the POTUS and appropriate agencies.

> 1.8 Lead time for evacuation requires decisions be made before best information is available
States and local authorities require a certain lead time in order to plan and implement evacuation, and the error ellipse under current capabilities is not likely to adequately constrain the possibilities to allow effective decisions.

1.9 Public safety and tranquility require that the federal government be able to rapidly establish a single authoritative voice & tools to present critical information
Given the concern of what the public might know before it even gets to leadership, there needs to be a plan to put forward a single authoritative voice backed up with tools that clearly present information to support state and local authorities and reduce the chance of panic and counterproductive movement.

1.10 The preferred approach for short-notice NEO deflection was stand-off nuclear
In this scenario, given the short lead time (less than a decade), players chose to go with a solution they felt was low mass, provided high energy density for deflection, leveraged existing national capabilities, and had comparatively high technological readiness level (TRL). Some players suggested a Memorandum of Understanding (MOU) between NASA, DOE and DOS may be necessary to preserve the required capabilities and infrastructure to execute the nuclear option.

Note: The full report is available here (PDF - 3.0 MB):


Click Here For The Planetary Defense Conference White Paper


NATIONAL AERONAUTICS AND SPACE ADMINISTRATION Near-Earth Object Survey and Deflection Analysis of Alternatives Report to Congress March 2007

 

The objectives of the George E. Brown, Jr. NEO Survey Program are to detect, track, catalogue, and characterize the physical characteristics of NEOs equal to or larger than 140 meters in diameter with a perihelion distance of less than 1.3 AU (Astronomical Units) from the Sun, achieving 90 percent completion of the survey within 15 years after enactment of the NASA Authorization Act of 2005. The Act was signed into law by President Bush on December 30, 2005.

A study team, led by NASA’s Office of Program Analysis and Evaluation (PA&E), conducted the analysis of alternatives with inputs from several other U.S. government agencies, international organizations, and representatives of private organizations. The team developed a range of possible options from public and private sources and then analyzed their capabilities and levels of performance including development schedules and technical risks.

Key Findings for the Survey Program:

• The goal of the Survey Program should be modified to detect, track, catalogue, and characterize, by the end of 2020, 90 percent of all Potentially Hazardous Objects (PHOs) greater than 140 meters whose orbits pass within 0.05 AU of the Earth’s orbit (as opposed to surveying for all NEOs).

• The Agency could achieve the specified goal of surveying for 90 percent of the potentially hazardous NEOs by the end of 2020 by partnering with other government agencies on potential future optical ground-based observatories and building a dedicated NEO survey asset assuming the partners’ potential ground assets come online by 2010 and 2014, and a dedicated asset by 2015.

• Together, the two observatories potentially to be developed by other government agencies could complete 83 percent of the survey by 2020 if observing time at these observatories is shared with NASA’s NEO Survey Program.

• New space-based infrared systems, combined with shared ground-based assets, could reduce the overall time to reach the 90 percent goal by at least three years. Space systems have additional benefits as well as costs and risks compared to ground-based alternatives.

• Radar systems cannot contribute to the search for potentially hazardous objects, but may be used to rapidly refine tracking and to determine object sizes for a few NEOs of potentially high interest. Existing radar systems are currently oversubscribed by other missions.

• Determining a NEO’s mass and orbit is required to determine whether it represents a potential threat and to provide required information for most alternatives to mitigate such a threat. Beyond these parameters, characterization requirements and capabilities are tied directly to the mitigation strategy selected.

Key Findings for Diverting a Potentially Hazardous Object (PHO):

The study team assessed a series of approaches that could be used to divert a NEO potentially on a collision course with Earth. Nuclear explosives, as well as non-nuclear options, were assessed.

• Nuclear standoff explosions are assessed to be 10-100 times more effective than the non-nuclear alternatives analyzed in this study. Other techniques involving the surface or subsurface use of nuclear explosives may be more efficient, but they run an increased risk of fracturing the target NEO. They also carry higher development and operations risks.

• Non-nuclear kinetic impactors are the most mature approach and could be used in some deflection/mitigation scenarios, especially for NEOs that consist of a single small, solid body.

• "Slow push" mitigation techniques are the most expensive, have the lowest level of technical readiness, and their ability to both travel to and divert a threatening NEO would be limited unless mission durations of many years to decades are possible.

• 30-80 percent of potentially hazardous NEOs are in orbits that are beyond the capability of current or planned launch systems. Therefore, planetary gravity assist swingby trajectories or on-orbit assembly of modular propulsion systems may be needed to augment launch vehicle performance, if these objects need to be deflected.

Alternatives Considered to Detect, Track, Characterize, and Deflect/Mitigate NEOs

The following tables provide a summary of the options considered. Technical descriptions of each option, as well as other combinations of alternatives, can be found in subsequent sections of this report. For each option, Table 1 shows the percentage of PHOs that would be found by the survey by the end of 2020 and the year each option would achieve 90 percent completion, starting with the option of sharing the use of potential ground-based observatories, which will be referred to as the "Reference" architecture through the rest of this document. Details regarding the availability of assets for each option are also found in subsequent sections. Table 1 shows that individually each of the first three options fall short of meeting the Congressional goal. As shown in the last line of Table 1, the minimum survey architecture that achieves the goal would be a combination of the shared ground-based assets plus one of two dedicated asset options.

Detection and Tracking Capability Options
& Summary Results

Option*

through 2020

Year 90%

Shared ground-based (Reference)

83%

2026

Dedicated ground-based

85%

2024

Dedicated Infrared sensor in Venus-like orbit

89%

2021

Reference + One Dedicated Asset

At least 90%

Not Later than 2020

Details of each option are found in this report.


Characterization Options

Options

Descriptions (O1 = Option 1)

Option 1

Use Existing Assets + Detection and Tracking Systems

Option 2

O1 + Dedicated Ground Systems

Option 3

O1 + Dedicated Space-Based Remote Sensing (L1/L2)

Option 4

O1 + Dedicated Space-Based Remote Sensing (Venus-Like Orbit)

Option 5

O1+ O2+ O3 + 2 Flyby Missions to 8 Objects

Option 6

O1 + O2 + O3 + 8 Orbiter Missions

Option 7

O1 + O2 + O3 + Orbiters at a Fixed Threshold Probability of Impact

Details of each option are found in this report.


Impulsive Deflection/Mitigation Options

Impulsive Technique*

Description

Conventional Explosive (surface)

Detonate on impact

Conventional Explosive (subsurface)

Drive explosive device into PHO, detonate

Nuclear Explosive (standoff)

Detonate on flyby via proximity fuse

Nuclear Explosive (surface)

Impact, detonate via contact fuse

Nuclear Explosive (delayed)

Land on surface, detonate at optimal time

Nuclear Explosive (subsurface)

Drive explosive device into PHO, detonate

Kinetic Impact

High velocity impact

Details of each option are found in this report.


Slow Push Deflection/Mitigation Options

Slow Push Technique*

Description

Focused Solar

Use large mirror to focus solar energy on a spot, heat surface, "boil off" material

Pulsed Laser

Rendezvous, position spacecraft near PHO, focus laser on surface, material "boiled off" surface provides small force

Mass Driver

Rendezvous, land, attach, mine material, eject material from PHO at high velocity

Gravity Tractor

Rendezvous with PHO, fly in close proximity for extended period, gravitational attraction provides small force

Asteroid Tug

Rendezvous with PHO, attach to PHO, push

Enhanced Yarkovsky

Change albedo of a rotating PHO; radiation from sun-heated material will provide small force as body rotates

Details of each option are found in this report.

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