Can We Call the Bright Spot in Ceres’ Occator Crater a Cryovolcano Yet?

Evidence is mounting around the cryovolcanic history of the solar system’s innermost dwarf planet — and its most recent eruptions may have happened within the last four million years.

NASA/JPL-Caltech/UCLA/MPS/DLR/IDA

Since NASA’s Dawn mission arrived at dwarf planet Ceres in 2015, we’ve been treated to some wonderfully detailed images of the small world’s pockmarked terrain. Understanding the underlying processes of what is believed to be an ice-filled celestial body, however, is taking some time to decipher. But with more observations comes more understanding and planetary scientists are getting close to realizing what lies beneath those craters and, possibly, unlocking the secrets behind a very icy and very alien phenomenon we have no experience of in our terrestrial lives.

That phenomenon is cryovolcanoes. And Ceres seems to have them.

The most startling feature on Ceres is Occator Crater. This 57 mile-wide feature is the result of a massive impact tens of millions of years ago. Large craters on small worlds isn’t necessarily a strange thing in our battered solar system, but what is strange about Occator is the very bright feature (and small bright patches surrounding it) in the crater’s center. Even before Dawn arrived in orbit and only fuzzy images of Ceres were available, hopes were high that this bright anomaly in the otherwise gray Cererian landscape could be indicative of ices or some mineral compound that was formed by the presence of water.

There have been many studies into Occator’s icy center, but new research into the crater’s age compared to the bright spot’s age appears to, once again, point to a cryovolcanic origin.

Cryovolcanoes — or, simply, ice volcanoes — are hypothetical features that are believed to be common throughout the outer solar system. These ice volcanoes are thought to erupt in a similar fashion to the volcanoes we have on Earth, but instead of molten rock, these volcanoes erupt ice-cold volatiles — like water, methane or ammonia. Dwarf planet Pluto, for example, has features that look like cryovolcanoes, as does Saturn’s moon Titan and Jupiter’s moon Ganymede. These locations are extremely cold and known to contain large quantities of methane and water, so internal heating (caused by radioactive decay or tidal processes) melt the ices and force them to the surface. When they vent through the crust, gases are released and the liquids quickly freeze and sublimate.

Around these vents, cryovolcanoes will grow, and if Ceres really does have its own ice volcanoes, this will be the closest planetary body to the sun (and Earth) known to have them.

Now, in research headed by the Max Planck Institute for Solar System Research (MPS) in Göttingen, Germany, scientists using Dawn data have, for the first time, taken a stab at dating the age of the bright material in the center of Occator Crater and realized that the location has likely been the site of many cryovolcanic eruptions in the recent past.

Occator Crater as observed by NASA’s Dawn spacecraft (NASA/JPL-Caltech/UCLA/MPS/DLR/IDA)

In the center of Occator, a pit measuring around 7 miles wide can be found, likely formed during the massive impact approximately 30 million years ago. But around the edges of that pit are mountains, some 750 meters high, and in the center is a cracked dome measuring 400 meters high and nearly 2 miles wide. This bright dome is called Cerealia Facula and surrounding it appears to be material that was spewed from a cryovolcanic vent. Analysis has shown that this material contains salts that were formed in the presence of water from Ceres’ interior and then deposited onto the surface. The minerals around Cerealia Facula has been dated to only four million years, meaning that there has been cryovolcanic eruptions long after the Occator impact punctured Ceres’ crust.

“The age and appearance of the material surrounding the bright dome indicate that Cerealia Facula was formed by a recurring, eruptive process, which also hurled material into more outward regions of the central pit,” said Andreas Nathues, lead investigator of Dawn’s Framing Camera. “A single eruptive event is rather unlikely.” As noted in an MPS news release, Jupiter moons Callisto and Ganymede have similar features that are also believed to be related to cryovolcanic eruptions.

“The large impact that tore the giant Occator crater into the surface of the dwarf planet must have originally started everything and triggered the later cryovolcanic activity,” added Nathues.

Previous imagery of haze inside Occator Crater has led to the suspicion that ices remain on the surface today; the haze could be vapor from sublimating water ice exposed on the surface having been forced to the surface from Ceres’ interior. Evidence for this haze has been supported by other studies and appears to vary throughout the day as one would expect — increased sunlight would accelerate sublimation (ice turning from a solid to a vapor without passing through the liquid phase).

If volatiles are still being extruded through this vent today, this would seem to indicate that, in addition to the cryovolcanic eruptions in the last four million years, some form of activity continues to this day. Add this to the recent discovery of organic material on Ceres’ surface, this small world has become a very big asset for planetary science.

For more on Ceres’ icy eruptions, check out one of my last DNews videos:

The White House Approves NASA’s ‘James Bond’ Asteroid Bagging Mission

Screengrab from the NASA "Asteroid Retrieval and Utilization Mission" animation (NASA LaRC/JSC)
Screengrab from the NASA “Asteroid Retrieval and Utilization Mission” animation (NASA LaRC/JSC)

It’s been a looooong time since I last updated Astroengine.com, so first off, apologies for that. But today seems as good a time as any to crank up the ‘engine’s servers as the White House has rubber-stamped a manned NASA mission to an asteroid! However, this isn’t what the President originally had in mind in 2009 when he mandated the US space agency with the task of getting astronauts to an asteroid by the mid-2020’s.

In a twist, it turns out that NASA will be basing their manned asteroid jaunt on a 2011 Keck Institute study. To cut a long story short (you can read the long story in my Discovery News article on the topic: “NASA to Hunt Down and Capture an Asteroid“), NASA will launch an unmanned spacecraft to hunt down a small space rock specimen, “lasso” it (although “bagging” it would be more accurate) and drag the wild asteroid to park it at the Earth-moon Lagrangian point, L2. Then we can treat it like a fast food store; we can fly to and from, chipping off pieces of space rock, return samples to Earth and do, well, SCIENCE!

Great? Great.

Overall, this robotic capture/manned exoplration of an asteroid saves cash and “optimizes” the science that can be done. It also lowers the risk associated with a long-duration mission into deep space. By snaring an asteroid in its natural habitat and dragging it back to the Earth-moon system, we avoid astronauts having to spend months in deep space. The EML2 point is only days away.

But when watching the exciting NASA video after the news broke today, I kept thinking…

asteroid-grab2

But that wasn’t the only thing I was thinking. I was also thinking: what’s the point? It’s flashy and patriotic, but where’s the meat?

The human component of this asteroid mission has now been demoted to second fiddle. Sure, it will utilize NASA’s brand new Orion spacecraft and be one of the first launches of the Space Launch System (SLS), but what will it achieve? Astronauts will fly beyond Moon orbit, dock with the stationary space rock and retrieve samples as they please, but why bother with astronauts at all?

It is hoped that the robotic asteroid bagging spacecraft could launch by 2017 and, assuming a few years to steer the asteroid to EML2, a human mission would almost certainly be ready by the mid-2020s. But by that time, sufficiently advanced robotics would be available for unmanned sample retrieval. Heck, as telepresence technology matures, the EML2 point will be well within the scope for a live feed — light-time between Earth and the EML2 point will only be a few seconds, perhaps a little more if communications need to be relayed around the Moon. Robotics could be controlled live by a “virtual astronaut” on Earth — we probably have this capability right now.

The most exciting thing for me is the robotic component of asteroid capture. The advances in asteroid rendezvous and trajectory modification techniques will be cool, although scaling the asteroid bagging technique up (for large asteroids that could actually cause damage should they hit Earth) would be a challenge (to put it mildly). At a push, it may even be of use to a theoretical future asteroid mining industry. The rationale is that if we can understand the composition of a small asteroid, we can hope to learn more about its larger cousins.

The human element seems to be an afterthought and purely a political objective. There will undoubtedly be advancements in life support and docking technologies, but it will only be a mild taster for the far grander (original) NASA plan to send a team of astronauts into deep space to study an asteroid far away from the Earth-Moon system. The argument will be “an asteroid is a stepping stone to Mars” — sadly, by watering down the human element in an already questionable asteroid mission, it’s hard to see the next step for a long-duration spaceflight to Mars.

From this logic, we may as well just keep sending robots. But that wasn’t the point, was it?

Take a look at the video and decide for yourself:

Hayabusa Re-Entry Video: Spacecraft Destruction at its Best

There’s not a lot to add to this video, it’s too awesome.

It was captured by NASA’s converted DC-8 jet that was flying over Australia when the Japanese Hayabusa spacecraft broke up during re-entry. I’ll let the video do the rest of the talking:

Oh yes, and that little dot ahead of the falling debris? That’s the sample return capsule before it was found int he Outback safely. Thank goodness its parachute worked (presumably).

For more spacecraft demolition awesomeness, read “NASA Aircraft Videos Hayabusa Re-Entry

Hayabusa Returns to Earth with a Flash

Hayabusa re-enters over the Australian Outback, generating a bright fireball (screen grabs from the JAXA video feed)

Staring hard at the live streaming video of the black Australian skies, I was hoping to see a faint streak of light glide across the camera’s field of view.

But no, it wasn’t that subtle.

Shortly after 9:51 am EDT on Sunday morning (or, for me, a far more civilized 2:51 pm GMT), the Japanese space agency’s (JAXA) Hayabusa’s mission officially came to an end, burning up in the atmosphere. However, a few hours before, the spacecraft released a 40 cm-wide capsule, sending it ahead of the main spacecraft. This sample return capsule would have a very different re-entry than its mothership.

As I watched the small dot of light on the horizon of the streaming video getting brighter and brighter — feverishly hitting the PRTSC button and using some rapid cut&paste-fu in Photoshop — suddenly it erupted, shedding light on the distant clouds that had been invisible in the night.

Far from the re-entry being a faint or dull event, it was dazzling (as seen in the screen grabs to the right).

So, after seven dramatic years in space, the Hayabusa mission has come to an end.

For the full story about how Hayabusa got hit by the largest solar flare in history, limped to visit an asteroid called Itokawa and how its sample-collecting kit malfunctioned, have a read of my main article on Discovery News: Hayabusa Generates Re-Entry Fireball Over Australia

Note: Thanks to everyone who re-tweeted the sequence of re-entry pics. As of this moment it has received over 30,000 views on Twitpic!

Jupiter Got Smacked, Again

Quite frankly, I’m stunned.

An Australian amateur astronomer has just observed his second ‘once-in-a-lifetime’ event: an impact in the atmosphere of Jupiter. Phil Plait was very quick to get the news out, describing it as a “major coincidence,” and he ain’t wrong!

Anthony Wesley’s first event was the famous July 2009 observation of what was thought to have been the immediate aftermath of a comet impact in the Jovian atmosphere. His second happened on Thursday at 20:31 UTC when he was observing Jupiter when something hit the atmosphere, generating a huge fireball.

It is not known whether this event was caused by a comet or asteroid, but in a bizarre case of serendipity, earlier on Thursday Hubble released more information on his original impact event. The July 2009 “bruise” in the gas giant’s atmosphere is now thought to have been caused by an asteroid, and not a comet.

The Hubble press release included details on how researchers deduced that it was actually more likely that a 500 meter-wide asteroid hit Jupiter in 2009. One clue was that newly installed cameras on the space telescope detected little dust in the halo surrounding the impact site — a characteristic that was detected after the impact of the shards of comet Shoemaker-Levy 9 in July 1994. Also, the calculated trajectory of the 2009 event indicated the object didn’t have an orbit commonly associated with comets. If the 2009 event was an asteroid, that means Wesley saw something never seen before: the site of a recent asteroid impact on a celestial body.

And now, less than a year after being the first to see that impact aftermath, Wesley has done it again. Another amateur astronomer, Christopher Go, was quick to confirm Thursday’s fireball with a video of the 2 second flash in Jupiter’s upper atmosphere.

These impact events serve as a reminder about Jupiter’s fortuitous role in our Solar System. As the gas giant is so massive, its gravitational pull has a huge influence over the outer planets, dwarf planets, comets and asteroids. Acting like an interplanetary ‘vacuum cleaner’ Jupiter can block potentially disastrous chunks of stuff from taking a dive into the inner Solar System. It is thought that this distant planet has helped Earth become the thriving world it is today, preventing many asteroids and comets from ruining our evolution.

Thank you Jupiter!

Gecksteroids! Asteroids and Geckos May Share Common Force

The asteroid Itokawa (as imaged by the Japanese Hayabusa probe) and a gecko tattoo. Bear with me, it'll make sense soon (JAXA)
The asteroid Itokawa (as imaged by the Japanese Hayabusa probe) and a gecko tattoo. Bear with me, it'll make sense soon (JAXA)

What do asteroids and geckos have in common? Not a lot, as you’d expect, but they may share a common force.

This rather strange notion comes from research being done by a team of University of Colorado scientists who have been studying the odd nature of the asteroid Itokawa. When the Japanese Hayabusa mission visited the space rock in 2005 (Hayabusa’s sample return capsule is set to return to Earth on June 13th by the way), it noticed the asteroid was composed of smaller bits of rubble, rather than one solid chunk. Although this isn’t a surprise in itself — indeed, many asteroids are believed to be floating “rubble piles” — the rate of spin of the asteroid posed a problem.

Itokawa spins rather fast and if only the force of gravity was keeping the lumps of rock together, they would have been flung out into space long ago. In short, the asteroid shouldn’t exist.

Although plenty of theories have been bandied around, one idea seems to stick.

More commonly found as a force that holds molecules together, the van der Waals force may bind the individual components of the asteroid together, acting against the centripetal force caused by its spin.

But where do the geckos come in?

Geckos are highly skilled in the “climbing up walls” department, and it’s the van der Waals force that makes this happen. Should the body of a gecko be tilted in such a way against a perfectly smooth, “impossible” to climb surface, the gravity acting on the little creature will trigger the force into action. Therefore geckos have evolved to exploit the practical application of van der Waals.

This has some rather interesting ramifications for asteroid evolution too. During early stages of asteroid formation, the larger fragments of rock are flung off; the centripetal force exceeds that of gravity. In the latter stages of development, only the smallest rocks remain behind, their mass small enough to allow van der Waals forces to overcome the spin.

So, there you have it, asteroids do have something in common with geckos. It seems only right to call these space rubble piles “Gecksteroids.”

Thanks to my Discovery News colleague Jennifer Ouellette for drawing the comparison between asteroids and geckos!

Source: Discovery News, arXiv.org

NASA’s Asteroid Mission: Scary but Useful

Things have been moving fast for NASA in recent weeks, culminating in President Obama’s inspiring speech at Kennedy Space Center on Thursday. I haven’t commented on the new direction for the US space agency’s direction thus far as I’ve needed some time to digest the ramifications of these plans. But generally, I’m positive about the scrapping of the moon goal in favor of a manned asteroid mission (by 2025) and Mars some time around 2035.

But it hasn’t been easy, especially after the Ares I-X test launch in October 2009.

The Ares I-X was the first new NASA manned vehicle my generation has seen take to the skies (I was only one year old when the first of the shuttle fleet launched, beginning nearly 30 years of low-Earth orbit operations, so that doesn’t count). Despite criticism that this test flight was nothing more than old tech dressed up as a sleek “new” rocket, I was thrilled to see it launch.

The end product didn’t matter on that day. Sure, we’ve been to the Moon before, but it just seemed like the best plan on the table. I was inspired, I felt excited about our future in space. Seeing how astronauts live and work on the lunar surface, using it as a stepping stone for further planetary exploration (i.e. Mars) seemed… sensible. Expensive, but sensible

But the overriding sentiment behind Obama’s new plans was that we’ve been there before, why waste billions on going back? Continuing with the bloated Constellation Program would have used up funds it didn’t have. Cost overruns and missed deadlines were already compiling.

So, the White House took on the recommendations of experts and decided to go for something far riskier than a “simple” moon hop. Things going to plan and on schedule, in the year 2025 we’ll see a team of astronauts launch for a much smaller and far more distant target than the moon.

The asteroid plan has many benefits, the key being that we need to study these potentially devastating chunks of rock up close. Should one be heading in the direction of Earth, it would be really nice to have the technological ability to deal with it. A manned mission may be necessary to send to a hazardous near-Earth asteroid. Think Armageddon but with less nukes, no Bruce Willis, but more science and planning. Besides, if a rock the size of a city is out there, heading right at us, I’m hopeful we’ll have more than 18 days to deal with the thing.

My Discovery News colleague Ray Villard agrees:

“A several month-long human round trip to an asteroid will test the sea legs of astronauts for interplanetary journeys. And, asteroids are something we have to take very seriously in coming up with an Earth defense strategy, so that we don’t wind up going extinct like the dinosaurs.”

Possibly even more exciting than the asteroid plan is what — according to Obama — will happen ten years after that: a manned mission to Mars. I can’t overemphasize my enthusiasm for a mission to the Red Planet; that will be a leap for mankind like no other. Granted, there is plenty of criticism flying around that we need to live on the moon first before we attempt to land on Mars, but looking at the new plan, we won’t be actually landing on Mars any time soon. A 2030’s mission to Mars will most likely be a flyby, or if we’re really lucky, an orbital manned mission.

And that’s why going to an asteroid will be a good first step. Spending months cramped inside a spaceship with a handful of crewmates will likely be one of the biggest challenges facing man in space, so popping over to a near-Earth asteroid first is a good idea. A Mars trip could take over a year (depending on the mission). Now, this is where technological development sure would help.

If NASA can plough dedicated funds into new technologies, new life support and propulsion systems can be developed. Those two things will really help astronauts get places quicker (avoiding boredom) and live longer (avoiding… death). For the “living longer” part, there appears to be genuine drive to increase the life of the space station and do more impressive science on it. As it’s our only manned outpost, perhaps we’ll be able to use it for what it’s designed for.

There are a lot of unknowns still, and Obama’s Thursday speech certainly wasn’t NASA’s silver bullet, but it’s a start. Allocating serious funding for space technology development whilst setting the space program’s sights on going where no human has been before will surely boost enthusiasm for space exploration. In fact, I’d argue that this is exactly what NASA should be doing.

Although I was dazzled by the Ares I-X, I can see that continuing with Constellation would have been a flawed decision. Launching a manned mission to explore an interplanetary threat sounds risky, but considering that asteroids are the single biggest cosmic threat to civilization, it sure would be useful to know we have the technology to send astronauts to asteroids, perhaps even dealing with a potential threat in the near future.

P/2010 A2 Was An Asteroid Collision (Says Hubble)

What you see here is something mankind has never seen before, the aftermath of an asteroid collision. This conclusion comes after the Hubble Space Telescope was commanded to take a closer look at a strange comet-like object pottering around in the asteroid belt between the orbits of Mars and Jupiter.

The truth is we’re still struggling to understand what this means,” said David Jewitt, a planetary physicist from UCLA. “It’s most likely the result of a recent collision between two asteroids.”

After P/2010 A2 was discovered in January, Jewitt managed to get observation time on Hubble to get a closer look of what was thought could be a rare asteroid-comet hybrid.

In the image, the object named P/2010 A2 has a very obvious “X” on its surface shaped pattern in its tale, possibly the location where a smaller body slammed into it at high speed. The result of this hyper-velocity impact produced a lot of debris and scientists think the comet-like tail being swept back by the pressure of the solar wind is dust and outgassing volatiles (like subliming water ice).

Although this kind of event has never been observed before, over the lifetime of the evolving solar system, events like this occur on a regular basis, in fact asteroid collisions have shaped the asteroid belt. Interestingly, it is thought this impact was caused by a collision of a “Flora family” asteroid, a type of object that may have wiped out the dinosaurs 65 million years ago. (Don’t worry, this collision won’t affect Earth in any way, the dinosaur thing is simply an interesting connection!)

What an incredible discovery, it’s fortunate that we have Hubble’s excellent eyesight to peer deep into the asteroid belt…

Sources: Reuters, Discovery News

Could P/2010 A2 be the First Ever Observation of an Asteroid Collision?

Something rather bizarre was observed in the asteroid belt on January 6. Ray Villard at Discovery News has just posted an exciting article about the discovery of a comet… but it’s not your average, run-of-the-mill kinda comet. This comet appears to orbit the Sun, embedded in the asteroid belt.

Comets don’t usually do that, they tend to have elliptical and inclined orbits, orbits that carry them close to the Sun (when they start to heat up, creating an attractive cometary tail as volatile ices sublimate into space, producing a dusty vapor). They are then flung back out into the furthest reaches of the Solar System where the heating stops and the comet tail disappears until the next solar approach.

But P/2010 A2 — discovered by the Lincoln Near-Earth Asteroid Research (LINEAR) sky survey — has a circular orbit and it still appears to be venting something into space.

P/2010 A2 (LINEAR): A comet or asteroid debris? (Spacewatch/U of Arizona)

There is the possibility that it is a member of a very exclusive bunch of objects known as main belt comets (MBCs). MBCs are confused asteroid/comet hybrids that appear to spontaneously vent vapor and dust into space and yet stay confined to the asteroid belt. But, if P/2010 A2 is confirmed to be one of these, it will only be the fifth such object to be discovered.

So what else could it be? If the potential discovery of an MBC doesn’t excite you enough, it could be something else entirely: the dust produced by a hyper-velocity impact between two asteroids. If this is the case, it would be the first ever observation of an asteroid impact in the Solar System.

The asteroid belt isn’t the same asteroid belt you might see in science fiction; although there are countless rocky bodies in our asteroid belt, it is rare that these rocky bodies encounter each other. Space is very big, and although the density of asteroids in this region might be considered to be “high”, this is space we’re talking about, you can fly a spaceship through the region without having to worry that you’ll bump into something. The average distance between asteroids is huge, making it a very rare occurrence any two should hit. But given enough asteroids, and enough time, eventually asteroid collisions do happen. And in the case of P/2010 A2, we might have been lucky.

Asteroid collisions: Rare, but possible.
Asteroid collisions: Rare, but possible.

The chatter between comet/asteroid experts is increasing, and on one message board posting, Javier Licandro (Instituto de Astrofísica de Canarias, Spain) reports observing a secondary asteroid traveling with the cloud-like P/2010 A2.

The asteroid moves in the same direction and at the same rate as the comet,” reports Licandro on The Minor Planet Mailing List. “In addition, the P/2010 A2 (LINEAR) image does not show any central condensation and looks like a ‘dust swarm’.”

A short lived event, such as a collision, may have produced the observed dust ejecta.”

Therefore, this ‘comet’ may actually be the debris that was ejected after a collision between two asteroids. Although these are preliminary findings and it’s going to take some serious observing time to understand the true nature of P/2010 A2, it’s exciting to think that we may just have observed an incredibly rare event, 250 million miles away.

Source: Discovery News

Much Ado About Apophis

Concept art for the ESA Don Quijote asteroid mission concept (ESA)
Concept art for the ESA Don Quijote asteroid mission (ESA)

Apophis is a 300 meter wide asteroid that caused a stir back in 2004. When NASA discovered the near-Earth asteroid (or NEO), it appeared to be tumbling in our direction Armageddon-style and the initial odds for a 2029 impact were 1-in-37. Understandably, people got scared, the media went nuts and astrophysicists were suddenly very interested in space rock deflection techniques.

Fortunately for us, NASA has downgraded the threat to a zero (note zero) chance of Apophis bumping into us in 2029, and lowered the risk of a follow-up impact in 2036 from a 1-in-45,000 chance to a 1-in-250,000 chance.

It’s important to note that NASA didn’t just pull these numbers out of a hat; the space agency has been tracking Apophis intently since its discovery, plotted its position and projected its location to a very high degree of precision. The more we watch Apophis, the more the world’s scientists are convinced that the asteroid poses a very tiny risk to life on Earth. In fact, giving anything a 1-in-250,000 chance of happening is more of a courtesy than a ‘risk.’ Granted, we’re talking about a global catastrophe should Apophis hit, but would you ever bet on those kinds of odds?

Apparently, the Russian space agency thinks it’s more of a game of Russian Roulette than NASA thinks.

I don’t remember exactly, but it seems to me it could hit the Earth by 2032,” said Anatoly Perminov, the head of Roscosmos, on December 30, 2009. “People’s lives are at stake. We should pay several hundred million dollars and build a system that would allow to prevent a collision, rather than sit and wait for it to happen and kill hundreds of thousands of people.”

What are the legal implications of asteroid deflection? Read: Space Experts to Discuss Threat of Asteroid Impact

Wait a minute. Does Perminov know something NASA doesn’t? Is he even referring to Apophis? You know, the same asteroid NASA has calculated that has a cat in hell’s chance of causing bother in 2036? And what’s this about the year 2032?

Just for the record, Perminov is indeed referring to Apophis, but he got the date wrong (Apophis does not make a flyby in 2032). Perminov also puts a price on saving hundreds of thousands of people… “several hundred million dollars” should do it, apparently.

On the one hand I’m impressed that Roscosmos is calling for some kind of anti-asteroid shield, but on the other, Perminov’s concern is terribly misplaced (and potentially damaging). His statement sounds as if he’s only just heard about Apophis and then thrown into a press conference unprepared, then asked what he’s going to do about this impending doom. Naturally, in that situation he would have blurted out the first thing that popped into his head: We need to save the world! However, this isn’t the first time he’d heard about Apophis.

Boris Shustov, the director of the Institute of Astronomy under the Russian Academy of Sciences, tried to repair the damage pointing out that Perminov was just using Apophis as a “symbolic example, there are many other dangerous objects we know little about.”

However, saving the world from a theoretical “dangerous object” that may or may not hit us for the next few hundred/thousand/million years is less likely to get funding that an imminent 2032… sorry, 2036 impact.

Although Perminov might sound reasonable in asking for asteroid deflection funding, using sensationalist means to try to leverage funding only serves to make the same funding hard to come by.

In the AGU 2009 meeting in San Fransisco last month, ex-Apollo astronaut Rusty Schweickart outlined his organization’s plans to deflect an asteroid should it pose a threat to Earth. The B612 Foundation points out that there is a ~2% chance of Earth being involved with an “unacceptable” collision in the next century (not by Apophis, but by another undiscovered asteroid), but Schweickart and his colleagues want to emphasize urgency, not panic.

An infrastructure needs to be put in place to deal with asteroid deflection, but this goal will only be hindered by unwarranted alarm by the likes of Perminov. Asteroid detection and deflection will be two critical skills mankind will need to develop for the long-term survival of life on Earth, but the head of Roscosmos is running the risk of making the issue sound more like a crazed rant than anything of substance.

Besides, when Perminov says, “Everything will be done according to the laws of physics,” perhaps he shouldn’t be in charge of messing around with the orbits of NEOs after all…