Showing posts with label #ESA. Show all posts
Showing posts with label #ESA. Show all posts

Saturday, May 17, 2014

Mission to Europa: Life as We Thought We Knew It


We’ve talked about Europa and the search for extraterrestrial life on the ice giant here at To Infinity and…In Theory before. We’ve delved into life’s ability to thrive in some of the most hostile environments imaginable. (Missed those entries? Catch up on the four part series “Livin’ Life to the Extremophile” by following these links. Part 1: Vostok. Part 2: Europa. Part 3: Chemosynthesis. Part 4: Biodiversity.)
But when we talked about all that stuff before we didn’t talk very much about the most important thing. How exactly are we going to get underneath the huge sheet of ice surrounding Europa to the ocean of frozen mystery beneath? Scientists at several different agencies, from the big ones like NASA and the ESA to other firms like Stone Aerospace and Honeybee Robotics, are coming together to help answer that question.
The answer seems to lie in a multi-stage plan that will play out over the course of a few decades. Further testing still needs to be done to decide what will be the best approach for drilling into the ice for starters. Then the funding has to be raised in order to launch a mission of this scale. Luckily, researchers think they have an answer to that as well.
Today we’re going to talk about Jupiter and her moons, a program called JUICE, a payload delivery system called The Penetrator, cryobots, and a mission to Europa just to listen to the ice.
But first, a quick recap on why Europa is so promising in the search for life.

Sometimes You Just Have To Vent


For the longest time scientists purported that life could not exist at the depths of the ocean. The pressure was too high, it would crush anything organic. The light didn’t reach, nothing could possibly see to hunt and forage. Above all it would be far too cold. Then a mission to the outskirts of the Marianas Trench changed everyone’s tune. Not only was life discovered at the deepest depths at that time reached, but it was thriving.
Now we know that life is even capable of existing around some of the most hostile environments imaginable by using a process called Chemosynthesis. These hostile environments I’m talking about are the hydrothermal vents at the bottom of the ocean. Think of it like an underwater volcano.
As the ocean floor shifts due to tectonic activity from the way gravity affects our planet as it whirls through space, it causes buildups of pressure. This internal pressure has to be released somehow, so it vents it out to the ocean floor. Amongst this debris are little organic bits. Not stuff you and I like, but the kind of stuff microorganisms flourish on.
The same kind of thing is happening on Europa. It’s believed to have a rocky mantle and a molten iron core just like us. As it orbits around Jupiter, the stress from the gas giant’s gravitational force causes geothermal activity within the core. Just like our planet it has to be vented, hence the proposal for hydrothermal vents.
Only the surface is thought to be ice, the thickest ice in our solar system, but underneath that is believed to be a liquid ocean. If scientists are right the hydrothermal activity is what would make this possible, heating the water just enough to keep it from freezing near the mantle. How can they guess this from a few flybys and satellite snapshots?



The surface of Europa’s ice sheet is heavily scarred, and most of it isn’t from collisions with interstellar objects. Like Lake Vostok, a pocket lake within a sheet of ice in Antarctica, Europa is believed to be dotted with miniature bodies of water. The reason is because of the pattern of the scarring, there is no uniform structure to it.
It’s possible that as the moon orbits Jupiter the stress causes the ice to crack, but it wouldn’t be quite so varied and so jagged. When hydrothermal activity increases on the ice it may briefly unthaw some of the ice above the pocket lake (not entirely) and shift the ice around, causing the terrain patterns.
So now that we know what’s probably happening underneath the ice, what’s the plan for getting us to it? I’m going to ask you to try to keep your mind out of the gutter as we move on to our next section…

The Penetrator: Between the Ice Sheets


Europa had better prepare its Uranus for scientist Sanjay Vijendran’s payload delivery system because it looks like whatever method the mission chooses to drill into the planet “The Penetrator” is what’s going to be getting it there. It’s already been “drilled” through its paces, and is officially marked as ready for space travel. It’s fairly light given what it does, meaning an orbiting craft could launch several at a time, and it’s extremely durable.
So what is it and how does it work?


During testing the Penetrator was aimed at a 10 ton block of ice in order to simulate the effects of what it will be like to land (or crash really) on the surface of Europa. Weighing 44 pounds, it hit the block at 760 MPH showing a peak deceleration of 24-25,000g. For a point of reference, an ejecting fighter pilot experiences 14gs and typical soft-landing spacecraft experience 30-40gs.
What’s even more incredible is it was fully loaded with instruments and everything was just fine. All that happened was a little cosmetic damage, a few scratches in the paint. Being that it’s capable of burrowing up to 3m into the surface without the use of a drill, this could be the most useful tool in planetary exploration to date. It could deliver a vast array of scientific equipment for analysis of various factors. From seismometers to chemical labs.
The Penetrator is split into two different sections, the warm bay and the cold bay. The cold bay is for taking in samples and the warm bay houses instruments and keeps them from being damaged by the extreme temperatures on Europa (minus 200 degrees Celsius).
Its designer, Vijendran, has made note of its advantages over soft landers. Where they have to slow down, this can hit at full force, so all the space wasted from expensive instrumentation meant to decelerate a craft can be utilized by other items.
And just what might those other things be? Let’s take a look at some of the other toys possibly going along for the ride to Europa.

Lasers, Auto-Gophers, And Cryobots, Oh My!



So now that we know how they intend to get onto the surface and drop off the equipment, what exactly are they bringing? And not just that, what exactly is this equipment going to do and how does it work? That’s a very good question and I’m so glad you asked it. The answer however is sort of difficult because as of the time of this writing, even the scientists aren’t sure what to pack in their lunchbox yet.
First and foremost they’re going to need something to drill into the ice. Secondly they’re going to need something to obtain and analyze samples. Lastly the equipment needs to be extremely durable and able to withstand the tremendously frigid temperatures.
Two scientists named Victoria Siegel and Kris Zacny have two very separate approaches to this same problem.

The Cryobot


According to Siegel’s team at Stone Aerospace the ocean is where it’s at, “That’s where the big stuff is going to be happening,” she says. But in order to get down to that “big stuff” we have to be able to drill through 10 km of ice. (That’s a little over 6 miles.) There is nowhere on Earth with a sheet of ice 6 miles thick. The Antarctic Ice Sheet is the closest we have at 2.6, but we’re still talking about something over double that. And it’s an exponentially colder and harsher environment trillions of miles away.
Not to mention drilling creates problems. There’s a lot of moving parts, in order to go deeper extensions need to be added, and if something breaks it’s not like a maintenance crew can just catch an interstellar taxi to Europa to fix it. The VALKYRIE cryobots hope to solve all of those problems and give the team just what they’re shooting for.
They have been working on a device since 2011 that is capable of using meltwater (water sucked up through the jets and heated) to bore its way through the ice. Once it reaches the ocean it will launch a small submarine from its belly to get a bird’s eye view of the world beneath the ice and to collect water samples to scan for signs of life.
Listen to how ScienceNews.org describes the working of the cryobot.

“The cryobot, a tube about as long as a compact car, holds wires coiled within a sleek aluminum frame and five jets arranged in a domed head. By heating aluminum blocks within the head, the cryobot can melt ice, and then suck in the water and shoot out hot streams. To thaw the ultracold ice of Europa, the bot will need to carry some sort of onboard nuclear reactor. Siegel and colleagues are testing their device on Earth using laser light pumped down a fiber optics wire connected to the machine.”

As of now the cryobot has moved into Phase-II of its development and the underwater submersible, being developed by NASA are solid candidates for the mission to Europa. The only thing (like most ambitious missions) that could possibly hold them back is funding. Launching a piece of equipment like that is costly and time will tell if the government is willing to shell out the funds necessary to give Stone Aerospace the chance to prowl the depths of Jupiter’s moon, and the go-ahead to launch a nuclear device to the surface of a foreign and pristine world.

The Auto-Gopher


The Auto-Gopher is a wire-line rotary hammer drill. In other words, it smashes its way through the ground as it digs into it. Kris Zacny of the company Honeybee Robotics believes that this is the way to go. It’s cheaper to use a drill then a robot, not to mention this will require a significant amount less power to operate. So how does it all work?
“It’s like a fishing rod,” Zacny says, “and at the end of the fishing line, you have a drill.” I suppose that’s an apt description if you’re used to fishing with explosives. (Metaphorically speaking) The teeth that jut out on the end of the drill are made of tungsten carbide and to get it through the particularly rough spots in the ice they gave it the ability to “thump” its way through by adding in a percussive system.
It only draws about 350 watts of power all in all. That’s less than your microwave uses. The whole thing is attached to a wire and pulley system so that sections don’t need to be added or removed. And now they have funding for an even better drill. From the same ScienceNews.org article check out this excerpt.

“Now the team is working on a new and improved drill, the AMNH Deep Drill, named after its funding source, the American Museum of Natural History. This drill will shuttle rock or ice cuttings to a container inside the tube instead of creating cores that have to be pulled from the borehole. And researchers plan to pack electronics and equipment, such as a microscope and sensors, inside the tube.”

This method has several advantages. It means every foot that the device goes down will be analyzed for scientific record and the Kevlar coated wire is strong and avoids using bulky extensions that would be difficult to add and remove. They’re also doing research into carbon nano-tubes (so did we! “Nano-Tech:Big Problems, Small Answers”) in order to make the device even more lightweight, making the Auto-Gopher just as, if not more, appealing to potential backers.
In my personal opinion they should combine the underwater submersible with the drill and go for broke. But what do I know? I do know that this is all expensive, and while the president wants to give funding to space programs, there isn’t a whole lot of money to spare, (what with the bankers needing bailouts for gold Cadillac’s, Rolex’s, and private jet fuel.) So what’s the plan?

Budget “Clipper”


NASA’s got a plan for Europa exploration as well. It’s called Clipper. It’s a highly advanced, extremely durable satellite that will optimally perform 45 flybys of the ice moon at varying altitudes. It will take highly advanced pictures of the surface, scan the exact thickness of the ice (right now the thickness is just an educated guess), document radiation levels in the atmosphere and record exact temperatures on the entirety of Europa, there are a host of other possibilities this device brings to the table as well.
The problem is the $2.2 billion price tag. The Obama administration is willing to work with NASA, but only to the extent of $1 billion. Dr. Britney Schmidt who is spear-heading Clipper is thrilled the President has brought Space Exploration to the party finally but the budget is less than ideal.
Another scientist however, by the name of Christopher McKay thinks that that will be plenty enough. If the whole goal is to examine the surface of Europa and scan under the ice then he has just the plan for them. He intends to land a camera and a microphone on the surface to “listen” to the ice.
No that isn’t a joke. As the ice moves around scientists will be able to tell exactly what’s going on beneath the surface. How they are able to do this eludes me but if there’s a person who can translate it then I can get behind it. While I doubt Europa will be appearing on the next Santana album for a live duet with the guitar playing legend, this “ice noise” could bring us one step closer to missions like Spiegel’s, Schmidt’s, and Zacny’s.
This kind of exploration builds confidence and public interest, which is exactly what missions like Clipper and the Auto-Gopher are hinging on now. But while America is scrambling for the scraps, the ESA grabbed a V-8 and got juiced up for a little mission of their own.

Europe JUICE-in’ Up For Europa



While NASA is tuned into the Europa station, the European Space Agency is looking at the whole picture. All three Galilean moons are thought to contain liquid water somewhere beneath the surface. If we’re going to be in the neighborhood, why not see all the sights? The ESA is planning to send a probe called JUICE (JUpiter ICy moons Explorer) into orbit around Callisto, Europa, and Ganymede.
The goal is to study the composition of water beneath, survey the topographical features of the planets more thoroughly, investigate their potentiality to contain life as we think we know it, and many, many other awesome plans. There’s something even better, this is already in the works.
The time frame to deliver JUICE to the Jovian system is 2030 with a launch from Earth taking place as early as 2022. The prospect of this is exciting and they have plenty of time to make revisions and add other instrumentation. Russia is developing most of the components and say what you will about their foreign policy, they make some really good stuff.
With all the options open to us above and many others that could become potential candidates in the future we will certainly be seeing some kind of landing within the next twenty to forty years. Time will tell. Speaking of time, here at TI&IT we like to delve into the history of things as well as the science, after all, what are we without our past?
The question really isn’t who discovered these moons, we attribute that to astronomer Galileo, but what some may not know is while he is credited, someone may have discovered them first. Let’s take a look at the remarkable past of Jupiter’s biggest satellites.

Galileo and the Medicean Planets


The photo above that looks like the scribbling of a madman in a ward is actually the handwriting of the brilliant Galileo Galilei himself. He discovered the planets sometime around 1609-1610 while he was making improvements to his telescope. He originally named them the Medicean Stars in honor of the Medici family, but later it was discovered they were moons.
And it wasn’t much later either. In fact, it may have been earlier. A man named Simon Marius, a German astronomer, had made observations a few days prior of the same nature. In 1614 he published his paper  “Mundus Lovialis” detailing his discovery of Jupiter’s moons. You can imagine this led to some heated debates between him and Galileo.


In the end it is irrelevant who discovered it first, Marius ultimately won out the name-calling as the celestial bodies Io, Ganymede, Europa, and Callisto were the names he selected. And thankfully history was kind enough to remember him for that. Remnants of his work are scarce but he’s credited as “a clever observer” which is probably not the most sought after title in the scientific community.
But then again, what are all of us now?
Jupiter’s moons are named after Greek mythology. To be exact they are named after the lovers of Zeus. For the sake of the length of this article already we won’t go into too much about this now, but I’m sure in the future we will be talking about Europa once again.

Europa’s Cold Future


While we probably won’t find space penguins orbiting around the moons of Jupiter or Saturn we may find some sort of life. That is if we can get the funding to get off the ground and get there. From cryobots to satellites there are a number of possibilities for exploring these intriguing heavenly worlds.
But as usual, money will hold scientific progress back. While that is depressing I hope you enjoyed this article on the future of Europa. Please share this around on Facebook and Twitter, I would be eternally grateful. Thank you all for reading, and enjoy this comical pun.


-Ryan Sanders

If you want to know more about any of the topics discussed above feel free to follow any of the links below! As always, thanks for reading and Happy Learning!

-       Wiki on Europa Clipper












Wednesday, January 22, 2014

Earth to Rosetta, Time to Wake Up


After napping for a little over two years, the European Space Agency’s Rosetta is ready to stretch her…panels. On the 20th of January this year the ESA held a competition to see who could issue the best wake-up call to the hibernating spacecraft. While I don’t know who won I do know they are quite lucky, as they win a free trip to Mission Control in Germany to see what Rosetta discovers.
In 2008 it passed a comet while flying by Mars. While 2867 Å teins had been discovered in 1969, this was the first time clear images of the comet were transmitted and its massive 5.6 km size could be clearly determined. In 2010 she flew by another one, 21 Lutetia, once again transmitting crystal clear images of an asteroid discovered in 1852. How was it discovered in 1852 with the limited technology available you ask? Probably because it’s over 1,000 km in diameter. That’s astronomically huge! (pun intended)
What makes this spacecraft so unique an sets her apart from other satellites is that Rosetta is the first one to be powered solely by solar technology! As it hibernated during its orbit around the sun to gain momentum its instruments were powered down in order to conserve energy. But while it was powered down it was gaining energy from the sun by gathering it on its massive solar arrays. Hopefully this will give Rosetta the extra “umph!” she needs to survive her mission out in deep space where she will only receive 4% of the sun’s power.
It’s been awhile since we’ve flown out into the deep reaches of space here at To Infinity And…In Theory. So let’s strap on our rocket boots, throw on some Elton John, and climb aboard the red eye to see what Rosetta and her little buddy Philae the Lander have in store for scientists at the ESA.

Comets, Asteroids, and Meteoroids

Yay! We get to start with terminology. I know what you’re saying, “my favorite…” but it’s important to understand there are very important differences between comets, asteroids, and meteoroids. The only reason I do this is because technically these words aren’t really interchangeable like so many others in Astronomy. There are a few key variances.
Let’s start with a comet.


Quite possibly one of the most well-known comets is Halley’s. It was discovered in 1531. Then discovered again in 1607…and again in 1682. It wasn’t until a man named Edmond Halley dug through the various reports of these sightings that he came to one very important conclusion. This comet was the same one. He also predicted that it would come back in 1758. While he didn’t live long enough to see that he was right, plenty of other astronomers did, which led to this comet being named after him.
So what makes a comet a comet? A comet is defined as a relatively small solar system body that orbits the Sun. When close enough to the Sun they display a visible coma (a fuzzy outline or atmosphere due to solar radiation) and sometimes a tail. But what creates the tail on a comet?
As it passes by the sun (which as we know is pretty darn warm…) it begins to burn gases and ice off the surface of the orbiting rock. These superheated gases trail behind the asteroid, sometimes miles long, as it rockets through space. This is what turns the space rock from an asteroid into a comet.
Speaking of asteroids, let’s talk about those next.


That’s Ceres. I know, I know, you’ve seen Armageddon and you’re saying “woah dude, that isn’t an asteroid, that’s totally a planet.” Well you’re half right. It was discovered in 1801 by Sicilian astronomer Giuseppi Piazzi. Originally he thought it was a comet but upon further observation it was determined that it was indeed a planet. Well…a dwarf planet. (They prefer to be called “Little Celestial People”) But seeing as it floats within the asteroid belt, it’s earned its moniker as an asteroid.
Asteroids are small solar system bodies that orbit the Sun. Made of rock and metal, they can also contain organic compounds. Asteroids are similar to comets but do not have a visible coma (fuzzy outline and tail) like comets do. It floats happily between Mars and Jupiter and actually contains one third of the mass of the entire asteroid belt. (Once again…huge) That’s not to say that if it broke orbit and passed close enough to the sun it couldn’t develop a tail, after all, the surface is believed to be made of dust and ice, perfect conditions to grow a coma. However that scenario is quite unlikely considering it’s been content with its lot in life to this point.
The third space rock type we’re going to talk about now is the Meteoroid. This particular floating stone actually has three forms like a Dragonball Z villain. Meteoroids are the first stage, Meteors are the second, and Meteorites are the last. We’ll break down all three in the next section.


A meteoroid is a small rock or particle of debris in our solar system. They range in size from dust to around 10 meters in diameter (larger objects are usually referred to as asteroids). But don’t mistake their smaller diameters for cute and cuddly. Once they enter the atmosphere of Earth they become known as a Meteor. Most of the time they’ll burn up in orbit, but as the blast in Chelyabinsk, Russia in February of last year showed us that’s not always the case.


Once a Meteoroid enters our atmosphere and becomes a Meteor about to cause an impending strike it is officially classified as a Meteorite. The effects of a Meteorite impact can be devastating, equivalent to several nuclear megaton blasts. (Time to call in Bruce Willis) That’s why NASA’s new Near Earth Object monitoring program is so important so we are able to identify threats like this long before they enter our atmosphere in the future so we don’t end up embedded in the crust of the Earth next to the dinosaurs.
So why am I telling you all this? Because the ESA is looking to land on a comet and it’s important to know the extreme challenges they face in doing this. Comets slingshot through the solar system gradually gaining speed as they play off the gravitational forces of the bodies they orbit. Asteroids like Ceres are essentially locked in orbit unless a huge impact was to send them rocketing out of alignment. (Typically that’s how an asteroid becomes a comet or a meteoroid)
Next we’ll talk about the challenges the ESA faces, how they intend to overcome them, and what they expect to learn from this unique mission into the far reaches of space. Let’s start with the biggest one of all, how exactly they intend to make contact with this orbiting mass. The details are far more intricate than you may think.

Space Darts


We’ve all played darts, but space agencies around the world have adapted the game to a whole new level. Think of it like this. When you look at a dart board you select the spot you want to hit. You close one eye, pull your arm back, take a couple practice swings and release it. If you’re experienced, nine times out of ten you hit what you’re aiming at.
Now imagine that dart board is several million miles away. It takes more than closing one eye and a deep breath to hit what they’re aiming for. It takes a series of complicated mathematical equations, physics, and a whole plethora of very expensive technology. Luckily, the ESA has all three down to a…well…a science.
When Rosetta was initially conceptualized in 1993 they were aiming at a different dartboard altogether. Comet 46 P/Wirtanen was caught in the crosshairs but due to postponements and complications with the rocket Ariane 5 ECA they switched it up. So in 2004, when Rosetta was launched its new target was designated 67 P/Churyumov-Gerasimenko.
But in order for Rosetta to “dock” with this comet certain parameters needed to be met at the outset. First and foremost speeds have to be matched. But 67 P/Churyumov-Gerasimenko has been orbiting for a long time. It’s had thousands upon thousands of years to gather the speed it moves at. Unfortunately, we don’t have thousands of years to follow it in orbit trying to play catch up. So how are they going to dock with it?
Through a process called a Gravity Assist Maneuver or Gravitational Slingshot. What it’s doing is moving around the sun and using its gravitational mass in order to gain momentum. The process can be used to accelerate or even decelerate depending on the arc of the object in motion. During its approach vector it makes a wide loop first, then, in order to garner further velocity, the orbit gets smaller and smaller on each approach until finally it’s commanded to break free toward its target.


Think of it in terms of a tether ball. The ball tied to the end of the string in this analogy would be Rosetta; the pole that the string is attached to is the sun. When the ball is struck hard enough it makes a lazy, slow loop around the pole. As the string gets shorter and shorter the speed at which the ball is moving begins to increase until it reaches its terminal velocity. If the ball were to be released from the string it would rocket off in the direction of its trajectory until outside factors like gravity and resistance pulled it down.
However, as we all should know, the voids of space have no gravity or atmosphere; therefore there is no resistance to slow the object down until it enters the gravity of another celestial body. Because of this the object maintains its velocity and is able to quickly get up to the speed of its intended target. But this is just the first problem the ESA has to overcome, the second one, believe it or not, is far more difficult in comparison to that.
The gravity on 67 P/Churyumov-Gerasimenko is a million times less than that of Earth’s. In other words, one wrong step and you’re floating off into deep space. (Yikes!) This poses a huge obstacle to the European Space Agency in getting Rosetta’s lander Philae to catch a piggyback ride through space.


With the gravity being so low on the surface of this comet one misstep could destroy over two decades of hard work and effort. Because of this Philae was outfitted with some special equipment to help it “stick” to the comet. Two harpoons will inject themselves into the surface to anchor it in place. Philae has also been equipped with self-righting landing gear to make sure he doesn’t tip over and once the feet make contact they will drill into the surface, further ensuring this multi-million dollar piece of tech doesn’t just fling off into space.
Outfitted with several different instruments including radio-spectrographs and sub-surface drills to take samples of the rock to determine the composition, this may be one of the most ambitious projects launched in recent years. But what exactly are they intending to learn from this mission? Would you believe me if I told you they’re looking to answer the question of where we came from? I hope so, because it’s basically the goal here.
But how exactly will some barren ice rock in space tell us where the complicated diversity of life on our planet originated from. Glad you asked. Let’s briefly explore that next in our final section today.

From Space Rocks to Building Blocks


Comet’s, Asteroid’s, and Meteoroids are all capable of containing a variety of materials. Certain classes of the space rocks contain mostly metals, some have been found to be highly dense carbon (diamonds), and some are even stranger still, because they contain organic compounds. If you don’t know, we’re organic compounds, and if you subscribe to the theory of evolution such as I do, then you know we all evolved from single celled organisms that likely were transported here by these tourists of the solar system.
Our planet didn’t start out as a planet. It started out as superheated gasses that formed into heavy elements. As gravity pulled those elements together it formed a solid mass. That solid mass slowly became heavier and generated more gravity and passing comets, asteroids, and meteoroids were pulled into its gravity. That is how we ended up with such a diversity of elements on the planets in our solar system…well, theoretically anyway.
But if some of the bacteria and organic compounds hitching a ride on the backs of these objects survived the entry into atmosphere that would certainly explain how we got here. That’s why landing on this comet is so important. By studying the subterranean composition of it and the formation of its coma as it passes the sun it will give scientists a much clearer understanding of exactly how comets play into the evolution of our solar system.
Philae is expected to make its daring descent onto the surface of 67 P/Churyumov-Gerasimenko later this autumn. I’ll be following this mission closely in the news and when new information develops I’ll be sure to write a follow-up blog on Rosetta and Philae. Until then, good morning, good morrow, and Godspeed Rosetta. I hope you enjoyed your nap, because now it’s time to get down to business.

-       Ryan Sanders


Thanks as always for reading and be sure to share this on Twitter, Facebook and Reddit and EVERYWHERE ELSE! J You guys and gals continue to make this one of the most enjoyable and ambitious undertakings for me to write and I hope they are just as enjoyable for you to read. Comments, questions, or corrections are always welcome so feel free to post them below. For further reading you can follow-up on any of the links listed below. Happy learning everyone!

-       Wiki entry on Rosetta