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.
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.
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):
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.
• 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.
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.
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
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