My notes on the 2013 Planetary Defense Conference


In my last post, I reported on a white paper summarizing the proceedings of the 2013 Planetary Defense Conference, which I attended April 15-19 in Flagstaff, Arizona. In this post I’ll offer some observations on the meeting.

At the PDC, I heard a lot of numbers, and I heard a lot of differing numbers: How big is that asteroid? How old is that crater? How many asteroids are potentially hazardous? How many asteroids are accessible for human exploration? I heard competing claims about what’s possible and what’s not – with regard, for example, to delivering “kinetic impactors” to NEOs. I heard differing rationales – for sending humans to asteroids, for example.

I noted that much of the NEO community is immersed in an abstract world of computer modeling, probabilistic risk assessments, Monte Carlo simulations ….a virtual world of sorts, a world constructed of numbers. If one lives in that world and speaks the language of that world, that world makes sense. If one lives in the material, concrete world, maybe not.

In the middle of the week, we PDCers took a break from presentations and had tours of Meteor Crater – diameter 4,100 feet (1.2 kilometers), depth 570 feet (173 meters), mass of impactor “several hundred thousand tons,” rock displaced 300 million-400 million tons. Thanks to Northern Arizona University planetary scientist Nadine Barlow, who studies craters on Earth, Mars, and other planetary bodies, for being our guide.

Meteor Crater is a family-owned, for-profit business. The visitors center there shows two short films (each 6-7 minutes long). One tells the story of Meteor Crater – how it was formed, what its geology is like, and who put the crater on the map, so to speak. The other is a sales pitch – a solicitation for contributions – for the B612 Foundation’s Project Sentinel, a space-based NEO survey telescope for which the foundation is in the process of raising funding.

Returning to PDC presentations, I heard a lot of talks about a variety of missions to asteroids, for study and for deflection. I heard way too many talks about concepts for sending nuclear “devices” (I call them bombs or weapons) to deflect asteroids that might be on an impact course with Earth by exploding on, in, or near the asteroids. Some of these concepts are coming out of the U.S. Department of Energy’s weapons laboratories, including Los Alamos National Lab and Sandia National Lab. Some are coming out of Bong Wie’s Asteroid Detection Research Center at Iowa State University. Some are coming out of NASA field centers. Here’s a sampling.

For example, Brian Kaplinger of Bong Wie’s lab gave a talk about “GPU accelerated 3-D modeling and simulation of a blended kinetic impact and nuclear subsurface explosion,” intended to determine “mission effectiveness of a two-body Hypervelocity Asteroid Intercept Vehicle…being developed to overcome key difficulties in coupling energy from nuclear explosives to an asteroid target at high relative velocities of 5 – 30 km/s…. All methods of disruption using a 100 [kiloton] nuclear energy source were quite effective for 100 m diameter targets for 15 days lead time, regardless of the orbit considered.” (Feel better? I don’t.)

NASA Goddard Space Flight Center’s Brent Barbee reported to the conference on “conceptual design of a flight validation mission for a hypervelocity asteroid intercept vehicle,” developed in collaboration with Bong Wie’s lab – that is, the HAIV that Kaplinger talked about – “as part of a Phase 2 NASA Innovative Advanced Concepts (NIAC) research project.” Barbee and co-authors’ rationale for launching nuclear weapons to asteroids? “At present there have been no flight missions to validate planetary defense techniques or technologies…. [W]hile the impressive scientific missions that have been sent to asteroids and comets so far have certainly provided future planetary defense missions with good heritage on which to build, we are clearly not ready to respond reliably to a threatening NEO scenario. When a hazardous NEO on a collision course with Earth is discovered we will not have the luxury of selecting a NEO target suitable for our mission design purposes or changing our choice of target if our development schedule slips…. Making preparations now is essential because we will only have one chance to deploy an effective and reliable defense. (Mission cost est: $530mm+).”

I heard a number of talks at the PDC about human exploration of asteroids. Barbee and colleagues presented the results of a NASA “near-Earth object human space flight accessible targets study [NHATS]: an ongoing effort to identify near-Earth asteroid destinations for human explorers…. Since its inception during the fourth quarter of 2010, the NHATS has provided an unprecedented comprehensive view of the NEA accessibility landscape for future exploration missions [and] defined a unique sub-population of NEAs, the NHATS-compliant NEAs, that are unusually accessible relative to the NEA population as a whole. NHATS-compliant NEAs currently comprise approximately 11% of known NEAs, and approximately 8 to 12% of the NHATS-compliant NEAs are also classified as Potentially Hazardous Asteroids (PHAs), depending on PHA size definition.” (I’ve heard differing opinions on these conclusions.)

As to the rationale driving this study, “NEAs are among the most potent threats and richest opportunities found in nature,” according to Barbee and colleagues, “their high accessibility, compositions, and lack of strong gravitational fields make them prime targets for the development and application of in-situ resource utilization techniques that may prove vital to future expansion of human presence in our solar system and perhaps, someday, beyond.”

One of Barbee’s colleagues, Dan Mazarek of NASA Langley Research Center, gave a talk on an “asteroid retrieval mission concept – trailblazing our future in space and helping to protect us from Earth impactors.” As all space wonks now know, an Asteroid Retrieval Mission (ARM) has been proposed in President Obama’s fiscal year 2014 budget request – a concept, according to Mazarek, “with the goal of returning a small (~7 m diameter) near-Earth asteroid (NEA), or part of a large NEA, to cislunar space using a 50 kW-class solar electric propulsion (SEP) robotic spacecraft (~40 kW available to the electric propulsion system) and currently available technologies. The mass of the asteroidal material returned from this mission is anticipated to be up to 1,000 metric tons, depending on the orbit of the target NEA and the thrust-to-weight and control authority of the SEP spacecraft. Even larger masses could be returned in the future as technological capability and operational experience improve.”

As to the rationale for an ARM, Mazarek offered Russian mystic Konstantin Tsiolkovskii’s early 20th-century dreams of human expansion into space using extraterrestrial resources.  As to the benefits of an ARM, he offered “providing a near-Earth source of space resources for human and robotic space exploration, developing technologies and techniques to enable a future space-based economy based on the processing of asteroidal materials, and providing invaluable operational experience critical to future planetary defense efforts.”

Terrestrial mining has been and continues to be problematic, to say the least, and the overall exploitation of Earth’s resources has benefited the developed world to the detriment of the developing world – or, more simply, the “haves” to the detriment of the “have-nots.” I don’t expect space-based mining to change this equation. I’m also not at all sure that the idea of expanding human presence into space resonates with people and cultures around the world. And if human colonies in space were ever to come to pass – which I’m doubtful about, at least in the foreseeable future – I suspect that, again, developing countries would move their people off the Earth, leaving those less fortunate to live in the mess we’ve made of Earth.

Discovering, tracking, observing, and otherwise learning as much as we can about near-Earth objects makes sense. NEO impacts with Earth have occurred throughout the history of our planet. The difference between the present – say, the past few hundred years) – and the past – the previous 4.5 billion years of Earth’s existence – is that 7 billion people now live on the planet. In 1950, according to the United Nations, in 1950 the global population totaled 2.5 billion. In 2000, it reached 6.1 billion. Today it’s over 7 billion. Global population projections for 2050 range from 8.9 billion to 10.6 billion.

For billions of years, Earth and the life on it have recovered from NEO impacts. It’s all the people on the planet today that render future NEO impacts such “threats.” Working on options to deflect potentially hazardous asteroids is a good idea, as is preparing for NEO impact migitation. Building a NEO deflection mission around the use of nuclear weapons is problematic on many levels, starting on the ground, where the mining and processing and handling of radioactive material is still unsafe, not to mention that, in my humble opinion, continuing to build and stockpile nuclear weapons is an idea whose time has gone. As to the ARM, thus far, beyond proponents in the White House and at NASA, neither the space policy community nor the broader “public” has wholeheartedly embraced the ARM idea. Meanwhile, Congress and the White House have a long way to go toward approving a budget for NASA for 2014. Stay tuned to the discourse on the ARM….


One Response to “My notes on the 2013 Planetary Defense Conference”

  1. Library: A Round-up of Reading | Res Communis Says:

    […] My notes on the 2013 Planetary Defense Conference – doctorlinda […]

Leave a Reply

Fill in your details below or click an icon to log in: Logo

You are commenting using your account. Log Out /  Change )

Google photo

You are commenting using your Google account. Log Out /  Change )

Twitter picture

You are commenting using your Twitter account. Log Out /  Change )

Facebook photo

You are commenting using your Facebook account. Log Out /  Change )

Connecting to %s

%d bloggers like this: