Asteroid 2011 AG5 could pose threat to Earth in 2040
An artist's illustration of asteroids, or near-Earth objects, that highlight the need for a complete Space Situational Awareness system. / ESA - P.Carril
Scientists are keeping a close eye on a big asteroid that may pose an impact threat to Earth in a few decades.
The space rock, which is called 2011 AG5, is about 460 feet (140 meters) wide. It may come close enough to Earth in 2040 that some researchers are calling for a discussion about how to deflect it.
Talk about the asteroid was on the agenda during the 49th session of the Scientific and Technical Subcommittee of the United Nations Committee on the Peaceful Uses of Outer Space (COPUOS), held earlier this month in Vienna.
A UN Action Team on near-Earth objects (NEOs) noted the asteroid's repeat approaches to Earth and the possibility - however remote - that 2011 AG5 might smack into our planet 28 years from now.
The object was discovered in January 2011 by Mount Lemmon Survey observers in Tucson, Ariz. While scientists have a good bead on the space rock's size, its mass and compositional makeup are unknown at present. [The 7 Strangest Asteroids in the Solar System]
An asteroid desktop exercise
"2011 AG5 is the object which currently has the highest chance of impacting the Earth ... in 2040. However, we have only observed it for about half an orbit, thus the confidence in these calculations is still not very high," said Detlef Koschny of the European Space Agency's Solar System Missions Division in Noordwijk, The Netherlands.
"In our Action Team 14 discussions, we thus concluded that it not necessarily can be called a 'real' threat. To do that, ideally, we should have at least one, if not two, full orbits observed," Koschny told SPACE.com.
Koschny added that the Action Team did recommend to the NEO Working Group of COPUOS to use 2011 AG5 as a "desktop exercise" and link ongoing studies to the asteroid.
"We are currently also in the process of making institutions like the European Southern Observatory aware of this object," Koschny said. "We hope to make the point that this object deserves the allocation of some special telescope time."
Non-zero impact probability
The near-Earth asteroid 2011 AG5 currently has an impact probability of 1 in 625 for Feb. 5, 2040, said Donald Yeomans, head of the Near-Earth Object Observations Program at NASA's Jet Propulsion Laboratory in Pasadena, Calif.
This impact probability isn't set in stone, however. So far, researchers have been able to watch the asteroid for just a short time -- the first nine months of 2011 -- and the numbers may change after further observation, Yeomans told SPACE.com. [Photos: Asteroids in Deep Space]
"Fortunately, this object will be observable from the ground in the 2013-2016 interval," Yeomans said. In the very unlikely scenario that its impact probability does not significantly decrease after processing these additional observations, "there would be time to mount a deflection mission to alter its course before the 2023 keyhole," he added.
Keyholes are small regions in space near Earth through which a passing NEO's orbit may be perturbed due to gravitational effects, possibly placing it onto a path that would impact Earth.
Prudent course of action
2011 AG5 may zip through such a keyhole on its close approach to Earth in February 2023, which will bring the asteroid within 0.02 astronomical units (1.86 million miles, or 2.99 million kilometers) of Earth.
One astronomical unit is the average distance between Earth and sun, which is approximately 93 million miles (150 million km).
According to a JPL estimate, the 2023 keyhole -- through which 2011 AG5 must pass in order for there to be a real chance of an Earth impact in 2040 - is roughly 62 miles (100 km) wide.
"Although this keyhole is considerably larger than the Apophis keyhole in 2029, it would still be a straightforward task to alter the asteroid's trajectory enough to miss the keyhole - and hence the impact in 2040," Yeomans noted, referring to the asteroid Apophis, which could threaten Earth in 2036 if it zips through a keyhole in 2029.
"The prudent course of action is then to wait at least until the 2013 observations are processed before making any preliminary plans for a potential deflection mission," Yeomans said.
Processing additional observations in the 2013-2016 time period, he added, "will almost certainly see the impact probability for 2011 AG5 significantly decrease."
Wanted: Higher-fidelity assessment
"Yes, the object 2011 AG5 was much discussed at the AT 14 meetings last week, but perhaps prematurely," said Lindley Johnson, NASA's NEO Observations Program Executive in Washington, D.C.
Johnson said NEO watchers have flagged the asteroid "as one we should keep an eye on." At present, he said, while researchers have better preliminary orbit data for 2011 AG5 than for many other asteroids in the NEO catalog, "we have only medium confidence in the derived orbital parameters."
"Fortunately, we are confident our uncertainties in the current orbit model will be reduced when we will have good observation opportunities in September 2013 with the larger follow-up assets," Johnson told SPACE.com. Observing opportunities are even better, he added, starting in November 2015 and for several months thereafter.
"This, in turn, will enable us to better assess the likelihood of any 'keyhole' passage in 2023 and therefore a much higher fidelity assessment of any impact probability for the 2040 time frame," Johnson said. [5 Reasons to Care About Asteroids]
"So, rather than a need to immediately jump to space mission solutions, the situation with 2011 AG5 shows the value of finding potentially hazardous objects early enough so that there is time for a methodical approach of observation and assessment as input to any need for an expensive spacecraft mission," Johnson said. "A more robust survey capability would improve the data available to make such assessments."
Decision challenge
Long-time NEO specialist and former Apollo astronaut Russell Schweickart played an active role in the dialogue about 2011 AG5. He represented the Association of Space Explorers (ASE) Committee on Near Earth Objects and presented to the Action Team an analysis of the situation with 2011 AG5.
The space rock presents a "decision challenge" to the international community, Schweickart suggested, "in the unlikely chance that its current low, but significant probability of impacting Earth in 2040 continues to increase after additional tracking becomes available."
Schweickart spotlighted a rough Association of Space Explorers analysis of the options to deflect the asteroid in the future, in the unlikely scenario that the Earth impact probability continues to increase.
He also provided to the Action Team several new appraisals of options for deflection of asteroid 2011 AG5 to avoid a potentially dangerous Earth encounter in 2040.
Delayed deflection campaign
A decision date for a keyhole deflection is very soon, if not now, Schweickart suggested. Asteroid 2011 AG5 represents an actual threat that underscores the need for a NEO hazard decision-making structure within the UN COPUOS, he said.
Based on the latest analysis, Schweickart reported, a deflection campaign delayed until after the 2023 close approach appears marginally possible, as long as a decision to commit is made immediately thereafter.
In the low-probability case in which the impact threat of the asteroid persists beyond its 2013 apparition, "should a keyhole deflection campaign be foregone -- for whatever reason -- the international community may be faced with the difficult decision of choosing between an expensive multikinetic impactor or a nuclear explosive to prevent an impact should the NEO indeed pass through the keyhole," Schweickart said.
The timelines that would be required to mount a successful deflection of the asteroid, Schweickart told SPACE.com, might be challenging.
But first things first -- researchers stress that more study of the asteroid's trajectory is called for. The next tracking opportunities of 2011 AG5 will occur in September 2013, and then again in November 2015.
NASA chief: We still have time
In response to a letter from Schweickart regarding 2011 AG5, NASA Administrator Charles Bolden said that 2011 AG5 is "high on NASA's list of NEOs to monitor for impact hazard potential," adding that "we take these duties very seriously."
Bolden also noted the opportunities for highly accurate ground-based observations in the near future.
"Based on these observations, a more informed assessment can then be made on the need for any type of mitigation," he said.
Bolden also remarked that the asteroid makes an apparition in 2015, more than seven years before the close keyhole passage in 2023 that could set in motion an Earth impact in the 2040 time frame.
"As a point of comparison, NASA's Deep Impact mission [the Deep Impact probe smashed into comet Tempel 1 in July 2005] was conducted in six years from selection to impact under much less urgency, demonstrating the adequacy of a seven-year period for any necessary response," Bolden said.
Leonard David has been reporting on the space industry for more than five decades. He is a winner of last year's National Space Club Press Award and a past editor-in-chief of the National Space Society's Ad Astra and Space World magazines. He has written for SPACE.com since 1999.
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So, how much damage could a 450 (or so) foot wide chunk of rock do? The last for-sure asteroid strike of any consequence was the one that created the meteor crater in northern Arizona about 50000 years ago. Is is locally known as the Barringer Crater and the critter that created it was about 1/3 the diameter of the one of concern now. Since we have a square law relationship working here, this bad boy actually has 9 times the volume and presumably mass.
Best guess is the "Barringer" meterorite weighed in at 300000 tons, impacted at about 29000 miles per hour (actually that's relatively slow - believe it or not) and roughly half of it's mass never made it to the ground. We're taking about 150000 tons hitting a hardened basalt field with enough oomph to carve out a hole some eight tenths of a mile across. Scientists in the know think the result generated about 10 to 15 million tons of TNT equivalent in energy; or for those of you who remember it, about the same bang as 1000 Hiroshima sized nukes.
So if this one scores a bull anywhere on earth's land surface we're talking a minimum of 9 times the energy assuming the same loss of mass during its pass through the atmosphere and assuming it hits with the same pokey velocity.
We can't assume either. In fact, given it's much larger size a far smaller ratio of mass will be burnt up as it transects the atmosphere and it is also likely to pass through much quicker, say 45000 miles per hour.....
So, instead of 9 times the impact energy, a worst case scenario could possibly see a global crack on the chin of upwards of 12 to 15x what the Barringer strike did. 120 to 150 million ton equivalents of TNT.
Not an earth killer but certainly one that wouldn't pass un-noticed.
It may not be this one that gets us but another one not yet found or one that has it's orbit disturbed.
No doubt that some kind of orbital system needs to be developed to handle these threats. Really. Of all the problems the world faces, this is a big one.
Yet we won't do squat because nobody can agree on anything until it's a full-blown crises someday, but by then, it may be too late to do anything.
Knowing that, it seems the only way for us to survive is to get luck and either get hit by a small one that really messes up someplace, but doesn't kill everyone, or we have a really close miss. Only then people will get up and do something. Let's hope we have the time to deal with it when it comes.