While the world was enchanted with Chris Hadfield’s social media posts last year, a new video has the retired astronaut talking about loftier things. Say, for example, how humanity landed a camera on the Saturn moon Titan back in 2005. Or to be more practical, the fact that smallpox was eradicated in its naturally occurring form.
In his talks and books, Hadfield describes himself as one who never focuses on complaining. He was almost yanked from his command of the International Space Station due to a medical issue, but he pressed on and convinced the doctors to let him fly. And in this new video, he focuses on what humans do generally to make the world better — imperfect as it is.
“There are problems with everything, and nothing’s perfect, but that shouldn’t be cause to moan. That should be cause to achieve. Our world is a better place than we often claim it to be,” Hadfield said. “We live the way we do,” he added, “because people chose to tackle their problems, head on.”
The video appears to have a heavy emphasis on the Bill & Melinda Gates Foundation, a gigantic philanthropic network that works to improve lives in the developing world and also for the disadvantaged in the United States. But there are many ways to give back to your community, even through gestures as simple as volunteering.
Here are some examples in the space world (note that these aren’t necessarily endorsements for the organizations, but just ideas for making contributions in space and astronomy):
Cosmoquest, which runs online astronomy courses and also allows citizens to map extraterrestrial bodies right alongside astronomers.
Astronomers Without Borders brings astronomy education across the world, particularly to developing countries.
Uwingu says that half of its donations goes to grants to support learning in astronomy.
Other examples of space-y charity could include volunteering or donating to a local school or university, joining one of the numerous volunteer organizations in astronomy, or getting involved in a space advocacy group.
From a distance, Saturn’s rings look like a sheer sheet, but peer up close and you can see that impression is a mistake. Shadows from rubble believed to be two miles (3.2 kilometers) high are throwing shadows upon the planet’s B ring in this image from the Cassini spacecraft.
While the picture is from 2009, it caught the eye of the lead of the Cassini imaging team, who wrote eloquently about it in a blog post recently celebrating the link between wonder and the holidays.
“I have often thought: What a surreal sight this would be if you were flying low across the rings in a shuttle craft. To your eyes, the rings would seem like a gleaming white, scored, gravelly sheet below you, extending nearly to infinity,” wrote Carolyn Porco, the lead imager for the mission at the Cassini Imaging Central Laboratory for Operations (CICLOPS).
“And as you flew, you would see in the distance a wall of rubble that, eventually, as it neared, you would come to realize towered two miles above your head. There isn’t another sight like it in the Solar System!”
Besides the inherent beauty and delicacy of this picture, another notable feature is how hard it is to capture. According to CICLOPS, one can only take this photo during Saturn’s equinox — once every 15 years in Earth time! That’s because the angle of the Sun’s light reaches the plane of the rings, allowing shadows to fall. The area itself is likely filled with moonlets of a kilometer (0.62 miles) in size.
“It is possible that these bodies significantly affect the ring material streaming past them and force the particles upward, in a ‘splashing’ manner,” the CICLOPS website notes.
We’ve included more pictures of Saturn’s rings below, all taken from the Cassini spacecraft. The machine is healthy and working hard after about 10.5 years working at the planet. One of its major tasks now is to observe changes in the planet and particularly its large moon, Titan, as the system nears the solstice.
Sunlight. Moonlight. Starlight. I saw all three for the first time in weeks yesterday. Filled with photons, I feel lighter today, less burdened. Have you been under the clouds too? Let’s hope it’s clear tonight because there’s a nice event you’ll want to see if only because it’s so effortless.
The half-moon will pass very close to the planet Uranus for skywatchers across North America this evening Sunday, Dec. 28th. Pop the rubber lens caps off those binoculars and point them at the Moon. If you look a short distance to the left you’ll notice a star-like object. That’s the planet!
You can do this anytime it’s dark, but the later you look the better because the Moon moves eastward and closer to the planet as the hours tick by. Early in the evening, the two will be separated by a couple degrees, but around 11:30 p.m. CST (9:30 p.m. PST) when the Moon reclines in the western sky, the planet will dangle like an solitary diamond less than a third of a lunar diameter away. When closest to the Moon, Uranus may prove tricky to see in its glare. If you hide the Moon behind a chimney, roofline or power pole, you’ll find it easier to see the planet.
The farther north you live, the closer the twain will be. Skywatchers in Japan, the northeastern portion of Russia, northern Canada and Alaska will see the Moon completely hide Uranus for a time. The farther west you are, the higher the Moon will be when they conjoin. West Coast states see the pair highest when they’re closest, but everyone will get a good view.
When closest, the radically different character of each world can best be appreciated in a telescope. Pump the magnification up to 150x and slide both planet and Moon into the same field of view. Uranus, a pale blue dot, wears a permanent cover of methane-laced clouds where temperatures hover around -350°F (-212°C).
The fantastically large-appearing Moon in contrast has precious little atmosphere and its sunny terrain bakes at 250°F (121°C). And just look at those craters! First-quarter phase is one of the best times for Moon viewing. The terminator or shadow-line that divides lunar day from night slices right across the middle of the lunar landscape.
Shadows cast by mountain peaks and crater rims are longest and most dramatic around this time because we look squarely down upon them. At crescent and gibbous phases, the terminator is off to one side and craters and their shadows appear scrunched and foreshortened.
Enjoy the tonight’s conjunction and consider the depth of space your view encompasses. Uranus is 1.85 billion miles (2.9 billion km) from Earth today, some 7,700 times farther away than the half-moon.
Maybe you’ve seen Comet Q2 Lovejoy. It’s a big fuzzy ball in binoculars low in the southern sky in the little constellation Lepus the Hare. That’s the comet’s coma or temporary atmosphere of dust and gas that forms when ice vaporizes in sunlight from the nucleus. Until recently a faint 3° ion or gas tail trailed in the coma’s wake, but on and around December 23rd it snapped off and was ferried away by the solar wind. Just as quickly, Lovejoy re-grew a new ion tail but can’t seem to hold onto that one either. Like a feather in the wind, it’s in the process of being whisked away today.
Easy come, easy go. Comets usually have two tails, one of dust particles that reflect sunlight and another of ionized gases that fluoresce in Sun’s ultraviolet radiation. Ion tails form when cometary gases, primarily carbon monoxide, are ionized by solar radiation and lose an electron to become positively charged. Once “electrified”, they’re susceptible to magnetic fields embedded in the high-speed stream of charged particles flowing from the Sun called the solar wind. Magnetic field lines embedded in the wind drape around the comet and draw the ions into a long, skinny tail directly opposite the Sun.
Disconnection events happen when fluctuations in the solar wind cause oppositely directed magnetic fields to reconnect in explosive fashion and release energy that severs the tail. Set free, it drifts away from the comet and dissipates. In active comets, the nucleus continues to produce gases, which in turn are ionized by the Sun and drawn out into a replacement appendage. In one of those delightful coincidences, comets and geckos both share the ability to re-grow a lost tail.
Comet Encke tail disconnection April 20, 2007 as seen by STEREO
Comet Halley experienced two ion tail disconnection events in 1986, but one of the most dramatic was recorded by NASA’s STEREO spacecraft on April 20, 2007. A powerful coronal mass ejection (CME) blew by comet 2P/Encke that spring day wreaking havoc with its tail. Magnetic field lines from the plasma blast reconnected with opposite polarity magnetic fields draped around the comet much like when the north and south poles of two magnets snap together. The result? A burst of energy that sent the tail flying.
Comet Lovejoy may have also crossed a sector boundary where the magnetic field carried across the Solar System by Sun’s constant breeze changed direction from south to north or north to south, opposite the magnetic domain the comet was immersed in before the crossing. Whether solar wind flutters, coronal mass ejections or sector boundary crossings, more tail budding likely lies in Lovejoy’s future. Like the chard in your garden that continues to sprout after repeated snipping, the comet seems poised to spring new tails on demand.
If you haven’t seen the comet, it’s now glowing at magnitude +5.5 and faintly visible to the naked eye from a dark sky site. Without an obvious dust tail and sporting a faint ion tail(s), the comet’s basically a giant coma, a fuzzy glowing ball easily visible in a pair of binoculars or small telescope.
In a very real sense, Comet Lovejoy experienced a space weather event much like what happens when a CME compresses Earth’s magnetic field causing field lines of opposite polarity to reconnect on the back or nightside of the planet. The energy released sends millions of electrons and protons cascading down into our upper atmosphere where they stimulate molecules of oxygen and nitrogen to glow and produce the aurora. One wonders whether comets might even experience their own brief auroral displays.
Excellent visualization showing how magnetic fields line on Earth’s nightside reconnect to create the rain of electrons that cause the aurora borealis. Notice the similarity to comet tail loss.
Video Caption: Watch the Earth roll by through the perspective of German astronaut Alexander Gerst in this 4K six-minute timelapse video of images taken from on board the International Space Station (ISS) during 2014. Credit: Alexander Gerst/ESA
ESA astronaut Alexander Gerst from Germany who recently returned from a six month voyage to the International Space Station (ISS) has a special Christmas gift for all – a stunning six-minute timelapse compilation of his favorite images of Earth taken during his “Blue Dot” mission in 2014.
“A 4K timelapse showing our planet in motion, from my favourite Earth images taken during the Blue Dot mission,” wrote Gerst in connection with his spectacular timelapse video released to coincide with Christmastime.
“I wish all of you a merry Christmas! It was a wild year for me, thanks for joining me on this fascinating journey!” said Gerst in English.
“Wünsche euch allen fröhliche Weihnachten! War ein wildes Jahr für mich, vielen Dank, dass ihr mit dabei wart!” said Gerst in German.
You can watch the Earth roll by through Gerst’s perspective in this six-minute timelapse video combining over 12,500 images taken during his six-month mission aboard the ISS that shows the best our beautiful planet has to offer.
“Marvel at the auroras, sunrises, clouds, stars, oceans, the Milky Way, the International Space Station, lightning, cities at night, spacecraft and the thin band of atmosphere that protects us from space,” according to the video’s description.
Gerst would often would set cameras to automatically take pictures at regular intervals while doing his science research or preparing for the docking of other spacecraft at the ISS in order to get the timelapse effect shown in the video.
The robotic arm capture and berthing of the SpaceX Dragon cargo ship and the release of the Orbital Sciences Cygnus cargo freighter are particularly magnificent in a rarely seen timelapse glimpse of visiting vehicles that are absolutely essential to keeping the station afloat, stocked, and humming with research activities.
Gerst served aboard the ISS between May and November this year as a member of the Expedition 40 and 41 crews.
Gerst launched to the ISS on his rookie space flight on May 28, 2014, aboard the Russian Soyuz TMA-13M capsule along with Russian cosmonaut Maxim Suraev and NASA astronaut Reid Wiseman.
They joined the three station flyers already aboard – cosmonauts Alexander Skvortsov & Oleg Artemyev, and astronaut Steve Swanson – to restore the station crew complement to six.
Gerst and Wiseman became well known and regarded for their prolific and expertly crafted photography skills.
They returned to Earth safely on Nov. 10, 2014, with a soft landing on the Kazakh steppes.
Alex is Germany’s third astronaut to visit the ISS. He conducted a spacewalk with Wiseman on Oct. 7 while aboard. He is trained as a geophysicist and a volcanologist.
Read my story detailing Christmas 2014 festivities with the new crews at the ISS – here.
Stay tuned here for Ken’s continuing Earth and planetary science and human spaceflight news.
When sending spacecraft to Mars, the current, preferred method involves shooting spacecraft towards Mars at full-speed, then performing a braking maneuver once the ship is close enough to slow it down and bring it into orbit.
Known as the “Hohmann Transfer” method, this type of maneuver is known to be effective. But it is also quite expensive and relies very heavily on timing. Hence why a new idea is being proposed which would involve sending the spacecraft out ahead of Mars’ orbital path and then waiting for Mars to come on by and scoop it up.
This is what is known as “Ballistic Capture”, a new technique proposed by Professor Francesco Topputo of the Polytechnic Institute of Milan and Edward Belbruno, a visiting associated researcher at Princeton University and former member of NASA’s Jet Propulsion Laboratory.
In their research paper, which was published in arXiv Astrophysics in late October, they outlined the benefits of this method versus traditional ones. In addition to cutting fuel costs, ballistic capture would also provide some flexibility when it comes to launch windows.
Currently, launches between Earth and Mars are limited to period where the rotation between the two planets is just right. Miss this window, and you have to wait another 26 months for a new one to come along.
At the same time, sending a rocket into space, through the vast gulf that separates Earth’s and Mars’ orbit, and then firing thrusters in the opposite direction to slow down, requires a great deal of fuel. This in turn means that the spacecraft responsible for transporting satellites, rovers, and (one day) astronauts need to be larger and more complicated, and hence more expensive.
As Belbruno told Universe Today via email: “This new class of transfers is very promising for giving a new approach to future Mars missions that should lower cost and risk. This new class of transfers should be applicable to all the planets. This should give all sorts of new possibilities for missions.”
The idea was first proposed by Belbruno while he was working for JPL, where he was trying to come up with numerical models for low-energy trajectories. “I first came up with the idea of ballistic capture in early 1986 when working on a JPL study called LGAS (Lunar Get Away Special),” he said. “This study involved putting a tiny 100 kg solar electric spacecraft in orbit around the Moon that was first ejected from a Get Away Special Canister on the Space Shuttle.”
The test of the LGAS was not a resounding success, as it would be two years before it got to the Moon. But in 1990, when Japan was looking to rescue their failed lunar orbiter, Hiten, he submitted proposals for a ballistic capture attempt that were quickly incorporated into the mission.
“The time of flight for this one was 5 months,” he said. “It was successfully used in 1991 to get Hiten to the Moon.” And since that time, the LGAS design has been used for other lunar missions, including the ESA’s SMART-1 mission in 2004 and NASA’s GRAIL mission in 2011.
But it is in future missions, which involve much greater distances and expenditures of fuel, that Belbruno felt would most benefit from this method. Unfortunately, the idea met with some resistance, as no missions appeared well-suited to the technique.
“Ever since 1991 when Japan’s Hiten used the new ballistic capture transfer to the Moon, it was felt that finding a useful one for Mars was not possible due to Mars much longer distance and its high orbital velocity about the Sun. However, I was able to find one in early 2014 with my colleague Francesco Topputo.”
Granted, there are some drawbacks to the new method. For one, a spacecraft sent out ahead of Mars’ orbital path would take longer to get into orbit than one that slows itself down to establish orbit.
In addition, the Hohmann Transfer method is a time-tested and reliable one. One of the most successful applications of this maneuver took place back in September, when the Mars Orbiter Mission (MOM) made its historic orbit around the Red Planet. This not only constituted the first time an Asian nation reached Mars, it was also the first time that any space agency had achieved a Mars orbit on the first try.
Nevertheless, the possibilities for improvements over the current method of sending craft to Mars has people at NASA excited. As James Green, director of NASA’s Planetary Science Division, said in an interview with Scientific American: “It’s an eye-opener. This [ballistic capture technique] could not only apply here to the robotic end of it but also the human exploration end.”
Don’t be surprised then if upcoming missions to Mars or the outer Solar System are performed with greater flexibility, and on a tighter budget.
While scientists believe that at one time, billions of years ago, Mars had an atmosphere similar to Earth’s and was covered with flowing water, the reality today is quite different. In fact, the surface of Mars is so hostile that a vacation in Antarctica would seem pleasant by comparison.
In addition to the extreme cold, there is little atmosphere to speak of and virtually no oxygen. However, a team of students from Germany wants to change that. Their plan is to introduce cyanobacteria into the atmosphere which would convert the ample supplies of CO² into oxygen gas, thus paving the way for possible settlement someday.
The team, which is composed of students and volunteer scientists from the University of Applied Science and the Technical University in Darmstadt, Germany, call their project “Cyano Knights”. Basically, they plan to seed Mars’ atmosphere with cyanobacteria so it can convert Mars’ most abundant gas (CO2, which accounts for 96% of the Martian atmosphere) into something breathable by humans.
Along with teams from other universities and technical colleges taking part in the Mars One University Competition, the Cyano Knights hope that their project will be the one sent to the Red Planet in advance of the company’s proposed settlers.
This competition officially began this past summer, as part of the Mars One’s drive to enlist the support and participation of universities from all around the world. All those participating will have a chance to send their project aboard the company’s first unmanned lander, which will be sent to Mars in 2018.
Working out of the laboratory of Cell Culture Technology of the University of Applied Science, the Cyano Knights selected cyanobacteria because of its extreme ruggedness. Here on Earth, the bacteria lives in conditions that are hostile to other life forms, hence why they seemed like the perfect candidate.
As the team leader Robert P. Schröder, said to astrowatch.net: “Cyanobacteria do live in conditions on Earth where no life would be expected. You find them everywhere on our planet! It is the first step on Mars to test microorganisms.”
The other reason for sending cyanobacteria to Mars, in advance of humans, is the biological function they perform. As an organism that produces oxygen gas through photosynthesis to obtain nutrients, cyanobacteria are thought to have played a central role in the evolution of Earth’s atmosphere.
It is estimated that 2.7 billion years ago, they were pivotal in converting it from a toxic fume to the nitrogen and oxygen-rich one that we all know and love. This, in turn, led to the formation of the ozone layer which blocks out harmful UV rays and allowed for the proliferation of life.
According to their project description, the cyanobacteria, once introduced, will “deliver oxygen made of their photosynthesis, reducing carbon dioxide and produce an environment for living organisms like us. Furthermore, they can supply food and important vitamins for a healthy nutrition.”
Of course, the team is not sure how much of the bacteria will be needed to make a dent in Mars’ carbon-rich atmosphere, nor how much of the oxygen could be retained. But much like the other teams taking part in this competition, the goal here is to find out how terrestrial organisms will fare in the Martian environment.
The Cyano Knights hope that one day, manned mission will be able to take advantage of the oxygen created by these bacteria by either combining it with nitrogen to create breathable air, or recuperating it for consumption over and over again.
Not only does their project call for the use of existing technology, it also takes advantage of studies being conducted by NASA and other space agencies. As it says on their team page: “On the international space station they do experiments with cyanobacteria too. So let us take it to the next level and investigate our toughest life form on Mars finding the best survival species for mankind! We are paving the way for future Mars missions, not only to have breathable air!”
Other concepts include germinating seeds on Mars to prove that it is possible to grow plants there, building a miniature greenhouse, measuring the impact of cosmic surface and solar radiation on the surface, and processing urine into water.
All of these projects are aimed at obtaining data that will contribute to our understanding of the Martian landscape and be vital to any human settlements or manned missions there in the future.
For more information on the teams taking part in the competition, and to vote for who you would like to win, visit the Mars One University Competition page. Voting submission will be accepted until Dec. 31, 2014 and the winning university payload will be announced on Jan. 5, 2015.
You know the quote, we’re made of stardust. Generation after generation of stars created the materials that make us up. How? And how many stars did it take?
Carl Sagan once said, “The nitrogen in our DNA, the calcium in our teeth, the iron in our blood, the carbon in our apple pies were made in the interiors of collapsing stars. We are made of star stuff.” To an average person, this might sound completely bananas. I feel it could easily be adopted into the same dirty realm as “My grandpappy wasn’t no gorilla”.
After all, if my teeth are made of stars, and my toothpaste supplier can be believed, why aren’t they brighter and whiter? If my bones are made of stars, shouldn’t I have this creepy inner glow like the aliens from Cocoon? Does this mean everything I eat is made of stars? And conversely, the waste products of my body then are also made of stars? Shouldn’t all this star business include some cool interstellar powers, like Nova? Also, shouldn’t my face be burning?
When the Big Bang happened, 13.8 billion years ago, the entire Universe was briefly the temperature and pressure of a star. And in this stellar furnace, atoms of hydrogen were fused together to make helium and heavier elements like lithium and a little bit of beryllium.
This all happened between 100 and 300 seconds after the Big Bang, and then the Universe wasn’t star-like enough for fusion to happen any more. It’s like someone set a microwave timer and cooked the heck of the whole business for 5 minutes. DING! Your Universe is done! All the other elements in the Universe, including the carbon in our bodies to the gold in our jewelry were manufactured inside of stars.
But how many stars did it take to make “us”? Main sequence stars, like our own Sun, create elements slowly, but surely within their cores. As we speak, the Sun is relentlessly churning hydrogen into helium. Once when it runs out of hydrogen, it’ll switch to crushing helium into carbon and oxygen. More massive stars keep going up the periodic table, making neon and magnesium, oxygen and silicon. But those elements aren’t in you. Once a regular star gets going, it’ll hang onto its elements forever with its intense gravity. Even after it dies and becomes a white dwarf.
No, something needs to happen to get those elements out. That star needs to explode. The most massive stars, ones with dozens of times the mass of our Sun don’t know when to stop. They just keep on churning more and more massive elements, right on up the periodic table. They keep fusing and fusing until they reach iron in their cores. And as iron is the stellar equivalent of ash, fusion reactions no longer generate energy, and instead require energy. Without the fusion energy pushing against the force of gravity pulling everything inward, the massive star collapses in on itself, creating a neutron star or black hole, or detonating as a supernova.
It’s in this moment, a fraction of a second, when all the heavier elements are created. The gold, platinum, uranium and other rare elements that we find on Earth. All of them were created in supernovae in the past. The materials of everything around you was either created during the Big Bang or during a supernova detonation. Only supernovae “explode” and spread their material into the surrounding nebula. Our Solar System formed within a nebula of hydrogen that was enriched by multiple supernovae. Everything around you was pretty much made in a supernova.
So how many? How many times has this cycle been repeated? We don’t know. Lots. There were the original stars that formed shortly after the Big Bang, and then successive generations of massive stars that formed in various nebulae. Astronomers are pretty sure it was a least 3 generations of supernovae, but there’s no way to know exactly.
Carl Sagan said you’re made of star-stuff. But actually you’re made up mostly of Big Bang stuff and generations of supernova stuff. Tasty tasty supernova stuff.
What’s your favorite supernova remnant? Tell us in the comments below.
ISS astronauts Barry “Butch” Wilmore, NASA, Samantha Cristoforetti, ESA and Terry Virts, NASA send Christmas 2014 greetings from the space station to the people of Earth. Credit: NASA/ESA
Story/pics expanded. Send holiday tweet to crew below![/caption]
There is a long tradition of Christmas greetings from spacefarers soaring around the High Frontier and this year is no exception!
The Expedition 42 crew currently serving aboard the International Space Station has decorated the station for the Christmas 2014 holiday season and send their greetings to all the people of Earth from about 240 miles (400 km) above!
“Merry Christmas from the International Space Station!” said astronauts Barry Wilmore and Terry Virts of NASA and Samantha Cristoforetti of ESA, who posed for the group shot above.
“It’s beginning to look like Christmas on the International Space Station,” said NASA in holiday blog update.
“The stockings are out, the tree is up and the station residents continue advanced space research to benefit life on Earth and in space.”
And the six person crew including a trio of Russian cosmonauts, Aleksandr Samokutyayev, Yelena Serova, and Anton Shkaplerov who celebrate Russian Orthodox Christmas, are certainly hoping for and encouraging a visit from Santa. Terry Virts even tweeted a picture of the special space style milk and cookies awaiting Santa and his Reindeer for the imminent arrival!
“No chimney up here- so I left powdered milk and freeze dried cookies in the airlock. Fingers crossed,” tweeted Virts.
And here’s a special Christmas video greeting from Wilmore and Virts:
Video Caption: Aboard the International Space Station, Expedition 42 Commander Barry Wilmore and Flight Engineer Terry Virts of NASA offered their thoughts and best wishes to the world for the Christmas holiday during downlink messages from the orbital complex on Dec. 17. Wilmore has been aboard the research lab since late September and will remain in orbit until mid-March 2015. Virts arrived at the station in late November and will stay until mid-May 2015. Credit: NASA
“We wish you all a Merry Christmas and Happy New Year. Christmas for us is a time of worship. It’s a time that we think back to the birth of what we consider our Lord. And we do that in our homes and we plan to do the same thing up here and take just a little bit of time just to reflect on those topics and, also, just as the Wise Men gave gifts, we have a couple of gifts,” Wilmore says in the video.
“It’s such an honor and so much fun to be able to celebrate Christmas up here. This is definitely a Christmas that we’ll remember, getting a chance to see the beautiful Earth,” added Virts. “Have fun with your family. Merry Christmas!”
And you can send a holiday tweet to the crew – here:
Meanwhile the crew is still hard at work doing science and preparing for the next space station resupply mission launch by SpaceX from Cape Canaveral, Florida.
A SpaceX Falcon 9 rocket is now set to blastoff on Jan. 6, 2015 carrying the Dragon cargo freighter on the CRS-5 mission bound for the ISS.
The launch was postponed from Dec. 19 when a static fire test of the first stage engines on Dec. 17 shut down prematurely.
A second static fire test of the SpaceX Falcon 9 went the full duration and cleared the path for the Jan. 6 liftoff attempt.
Among the science studies ongoing according to NASA are:
“Behavioral testing for the Neuromapping study to assess changes in a crew member’s perception, motor control, memory and attention during a six-month space mission. Results will help physicians understand brain structure and function changes in space, how a crew member adapts to returning to Earth and develop effective countermeasures.”
“Another study is observing why human skin ages at a quicker rate in space than on Earth. The Skin B experiment will provide scientists a model to study the aging of other human organs and help future crew members prepare for long-term missions beyond low-Earth orbit.”
Merry Christmas to All!
Stay tuned here for Ken’s continuing Earth and planetary science and human spaceflight news.
Fans of Elon Musk and high-speed transit are sure to remember the Hyperloop. Back in 2013, Musk dropped the idea into the public mind with a paper that claimed that using the right technology, a high-speed train could make the trip from San Fransisco to Los Angeles in just 35 minutes.
However, Musk also indicated that he was too busy to build such a system, but that others were free to take a crack at it. And it seems that a small startup from El Segundo, California is prepared to do just that.
That company is JumpStartFund, a startup that combines elements of crowdfunding and crowd-sourcing to make innovation happen. Dirk Ahlborn, the CEO of JumpStartFund, believes they can build Musk’s vision of a solar-powered transit system that would transport people at up to speeds of 1280 km/h (800 mph).
Together with SpaceX, JumpStartFund has created a subsidiary called Hyperloop Transportation Technologies (HTT), Inc. to oversee all the necessary components to creating the system. This included bringing together 100 engineers from all over the country who work for such giants of industry as Boeing, NASA, Yahoo!, Airbus, SpaceX, and Salesforce.
Last week, these engineers came together for the first time to get the ball rolling, and what they came up with a 76-page report (entitled “Crowdstorm”) that spelled out exactly how they planned to proceed. By their own estimates, they believe they can complete the Hyperloop in just 10 years, and at a cost of $16 billion.
A price tag like that would be sure to scare most developers away. However, Ahlborn is undeterred and believes that all obstacles, financial or otherwise, can be overcome. As he professed in an interview with Wired this week: “I have almost no doubt that once we are finished, once we know how we are going to build and it makes economical sense, that we will get the funds.”
The HTT report also covered the basic design and engineering principles that would go into the building of the train, as Musk originally proposed it. Basically, this consists of pods cars that provide their own electricity through solar power, and which are accelerated through a combination of linear induction motors and low air pressure.
Much has been made of this latter aspect of the idea, and has often compared to the kinds of pneumatic tubes that used to send messages around office buildings in the mid-20th century. But of course, what is called for with the Hyperloop is bit more sophisticated.
Basically, the Hyperloop will operate by providing each capsule with a soft air cushion to float on, avoiding direct contact with rails or the tube, while electromagnetic induction is used to speed up or slow the capsules down, depending on where they are in the transit system.
However, the HTT engineers indicated that such a system need not be limited to California. As it says in the report: “While it would of course be fantastic to have a Hyperloop between LA and SF as originally proposed, those aren’t the only two cities in the US and all over the world that would seriously benefit from the Hyperloop. Beyond the dramatic increase in speed and decrease in pollution, one of the key advantages the Hyperloop offers over existing designs for high-speed rail is the cost of construction and operations.”
The report also indicated the kind of price bracket they would be hoping to achieve. As it stands, HTT’s goal is “to keep the ticket price between LA and SF in the $20-$30 range,” with double that amount for return tickets. But with an overall price tag of $16 billion, the report also makes allowances for going higher: “[Our] current projected cost is closer to $16 billion,” they claim, “implying a need for a higher ticket price, unless the loop transports significantly more than 7.4 million annually, or the timeline for repayment is extended.”
In addition, the report also indicates that they are still relying heavily on Musk’s alpha document for much of their cost assessment. As a result, they can’t be specific on pricing or what kinds of revenues the Hyperloop can be expected to generate once its up and running.
Also, there’s still plenty of logistical issues that need to be worked out, not to mention the hurdles of zoning, local politics and environmental assessments. Basically, HTT can look forward to countless challenges before they even begin to break ground. And since they are depending on crowdfunding to raise the necessary funds, it is not even certain whether or not they will be able to meet the burden of paying for it.
However, both Ahlborn and the HTT engineering team remain optimistic. Ahlborn believes the financial hurdles will be overcome, and if there was one thing that came through in the team’s report, it was the belief that something like the Hyperloop needs to happen in the near future. As the team wrote in the opening section of “Crowdstorm”:
“It quickly becomes apparent just how dramatically the Hyperloop could change transportation, road congestion and minimize the carbon footprint globally. Even without naming any specific cities, it’s apparent that the Hyperloop would greatly increase the range of options available to those who want to continue working where they do, but don’t wish to live in the same city, or who want to live further away without an unrealistic commute time; solving some of the major housing issues some metropolitan areas are struggling with.”
Only time will tell if the Hyperloop will become the “fifth mode of transportation” (as Musk referred to it initially) or just a pipe-dream. But when it was first proposed, it was clear that what the Hyperloop really needed was someone who believed in it and enough money to get it off the ground. As of now, it has the former. One can only hope the rest works itself out with time.