Whilst the mainstream media would have you believe that the bright spots on Ceres were a surprise to everyone they’ve actually been something we’ve known about for quite some time. However in the past they seemed to come and go making consistent observations of them rather difficult. With the Dawn craft now in a stable orbit around Ceres we are now in the position to observe them much more closely, bringing us ever closer to understanding what the heck it is. There’s still a lot more for us to understand but the first round of preliminary observations have provided some very good insight into the bright spot’s composition and its likely origin.
The first revelation to come out of Dawn’s observations was that the bright spot was in fact not a singular entity and is made up of several spots. There’s 2 large primary bright spots that are accompanied by a bunch of smaller ones which indicates that, as we make better observations, that those larger spots are most likely made up of multiple smaller spots as well. As the above ground map indicates there are actually a bunch of other bright spots dotted over Ceres’ landscape however none of them were close enough together to be observable before Dawn began making closer approaches. The origins of these spots remain something of a mystery however there are several prevailing theories about how they could have been created.
Ceres has been observed as having a very tenuous atmosphere which could only have arisen from outgassing or sublimation from its core. In early 2014 observations of Ceres detected some localized cryovolcanoes which are dumping some 3KG of water out into space every second supporting the theory that there’s some form of water hidden within Ceres. This supports the theory that these bright spots are most likely water ice (which would have the required reflectivity) but at the same time water in a vacuum tends to sublimate very quickly which begs the question of how long these bright spots have been around and how long they’ll last.
It’s quite possible that the ice in the crater was revealed by a recent impact and thus we’re just lucky that the bright spot is there for us to observe it. Considering that Ceres sits within the asteroid belt between Mars and Jupiter this is a very real possibility although that does then raise the question of why we’re not seeing more bright spots than we currently are. This is what then fuels other, more exotic, theories about what’s at the base of that crater such as a large metallic deposit. However evidence to support those theories isn’t yet forthcoming however once Dawn starts making closer approaches there is potential for some to come to light.
Needless to say the next few months of observations will prove extremely valuable in determining the bright spots’ elusive nature. Whilst the reality is likely to be far more dull and boring than any of the exotic theories make it out to be it’s still an exciting prospect, one that will give us insight into how solar systems like ours form.
We’ve known for a long time now that Mars once contained vast reservoirs of water and that even in its apparently dry state there was indications of water still hiding in various places. The search for water on Mars is a twofold with the two main objectives being finding environments suitable to life and secondly for potential use by future manned missions. Whilst we’ve succeed in confirming that yes, water once covered Mars and it still exists there today, we’re still finding out just how extensive the reservoirs are. As it turns out Mars may be flush with more water than we first expected and it’s been right under our noses this entire time.
The surface of Mars is a barren wasteland, covered in the same monotonous coloring that gives it that signature red tinge. The poles are the exception to this, harboring large water ice caps that get blanketed with a layer of dry ice (frozen carbon dioxide) in the winter. The reason for this is that due to the low pressure of Mars’ atmosphere exposed water anywhere else on the planet simply subliminates, turning straight from ice to water vapor before being swept away by Mars’ turbulent winds. However new research from the University of Copenhagen has revealed that water ice has managed to survive in other places around Mars and has done so in great quantities.
As it turns out many of the geological features we’ve observed on Mars that we’ve assumed to simply be mountains or hills are in fact dust covered glaciers which pepper the martian surface near the poles. This thick layer of dust has protected them from Mars’ atmosphere, preventing the ice from sublimation away. This dust also makes them appear like any other geological feature that you’d find on Mars’ surface instead of the towering walls of ice that we’re used to seeing here on Earth. The researchers were able to determine that these were water ice glaciers by using radar measurements from the numerous spacecraft we have orbiting the red planet and how they’re flowing under their protective dust blankets.
The amount of ice that these glaciers contain is quite staggering, enough that if it was spread out over the surface of Mars it would blanket it in a layer 1.1m thick. Such giant reservoirs provide huge opportunities for both exploration and scientific purposes and potentially paves a way for a sustainable human settlement. Whilst liquid water is always the most viable place to look for life we’ve found dozens of examples of microbial life living in some pretty harsh conditions and these glaciers might be a great place to start looking. That and water is one of the main components in several types of rocket fuel, something we’ll need if we want to do multiple return missions to Mars.
It’s incredible to note that our view of Mars has changed so drastically over the past couple decades, going from a barren wasteland that could never have housed life to a viable candidate, flush with water reserves everywhere. This latest discovery just goes to show that we can’t simply rely on visual data alone as even a well studied planet like Mars can still hide things from us and can do it in plain sight. The next step is to dig beneath Mars’ thick dust blanket to peer into these glaciers and, potentially, find something wriggling down there.
Thanks to our northern hemisphere counter-parts I’ve been privy to all sorts of interesting cold weather things from making instant snow to the ingenuity that people come up with when they’re snowed in. Here in Australia we do get the up on the other end of the spectrum quite often during summer however although that doesn’t really drive us to do much more than sit around a pool and drink copious amounts of beer. So you can imagine then that anything involving sub-zero temperatures is going to be somewhat intriguing to us, especially something as cool as this:
There’s nothing particularly complicated about what’s going on here but the demonstration is quite novel. What you’re seeing is the formation of ice crystals on the surface of a soap bubble which starts off slow but ramps up significantly as more crystals form. I think this is partially due to the way crystals form as they usually need a rough surface to attach to. This is how those instant ice videos work as the bottles don’t have any anchor points for the crystals to form but once you shake it up a bit you give them a surface to attach to.
There was one question that was left unanswered due to the video cutting off at the end however: whether or not it’d still float after it was frozen.
Now the bubble isn’t increasing in mass, it’s simply changing forms. There’s the possibility that some of the moisture from the air outside the bubble will condense onto the crystalline surface however I don’t think that’d change the mass by an appreciable amount. The density would also be going down as well thanks to water’s intriguing property of getting less dense as changes into ice. All those factors together would indicate that a frozen soap bubble would behave in much the same way as a regular one but I’d still like to see this hypothesis tested.
Although I do much prefer warmer climates, so this will have to be an exercise that’s left up to the reader.
Carl Sagan is quote as saying that “life looks for life”. Indeed if our own history is anything to go by we’re in a constant state of searching out other forms of life and just recently we’ve extended that search beyond the confines of the world that gave rise to us. So far our search beyond our home world has proved fruitless as we’ve been unable to find any direct indications of life on any other heavenly body that’s within our reach. Thus we find Earth in what appears to be some great isolation which is a somewhat disconcerting notion given the age of the universe and the number of potential habitable planets in our galactic backyard. We should not be discouraged however as our quest to find life elsewhere is only just beginning.
Of all the other heavenly bodies that inhabit our solar system there’s one that stands out as the best candidate for housing life. Now if I was to ask the question of which body it was most people would respond with Mars as it’s the only planet that resembles Earth in some fashion, with the next closest candidate being the raging hell of Venus. It’s not a bad guess either as we’ve proven several times over that there was once vast amounts of water there and there’s still a very good chance there’s liquid water present today. However Mars is a very inhospitable place so much so that the best hope for life there is nothing above microbial and even that seems like a far reaching prospect.
Europa on the other hand is quite the curiosity. As far as moons go it really is something out of left field being a striking combination of bright whites and browns. It’s surface is also one of the smoothest in the solar system thanks to it being made almost entirely of water ice. That doesn’t mean it’s featureless however as the entire surface is criss-crossed with fracture lines from the giant ice sheet breaking apart and reforming. Many have speculated that this is because the surface actually lies on top of a giant subsurface ocean and when cracks form the ocean rushes up to fill it, forming the characteristic lines. It’s this undersea ocean that makes Europa one of the best candidates for life forming outside of Earth and recent studies show it just got a little better.
The potential ocean on Europa would be some 3KM below the surface, quite a ways away from any direct sunlight or other potential energy sources. It’s theorized then that the ocean is kept liquid by the tidal flexing that Europa undergoes every time it orbits Jupiter which could also drive the same kinds of volcanism processes that gives rise to life in the depths of our oceans. However recent research shows that there’s potential for some subsurface lakes that are much closer to the surface than the great ocean below. These lakes would have a higher rate of churn between water and ice providing a much a habitat that’d be more nutrient rich and hopefully more hospitable to life. Of both these recently modelled oceans and the great subsurface ocean haven’t yet been conclusively proven, but that just makes Europa a really tantalizing target for exploration.
Quite a few missions have swung past Europa already with the most detailed analysis being done by the Galileo craft from 1995 to 2003. However we haven’t been back there recently save for a short flyby by the New Horizons craft that imaged it on its way to Pluto. If we were to go back there my favourite mission candidate would be the Crybot style mission. In essence it’s a probe that’s fitted with a giant heater on the front of it, capable of plunging through several kilometres of ice. Once it broke through it would then deploy a small autonomous underwater vehicle that could investigate the subsurface ocean. This mission hasn’t got past the back of the napkin style planning stages yet, but I’m hopeful that we’ll one day attempt such a mission.
Europa is a curiosity unlike any other in our solar system and there’s so much we could learn from it if we were to send a mission there. Whilst the environment there isn’t really human friendly (the radiation at the surface is quite large, about 450 chest x-rays a day worth) it’s definitely within our current capabilities of robotic exploration. I know that one day we’ll see a dedicate mission there but until then I’m quite content to continue fantasizing about the undersea world that it contains and the tantalizing possibility that as of yet unknown life forms exist there.