Africa is home to 7 out of 10 of the world’s fastest-growing economies. It’s population is also the “youngest” in the world, with 50% of the population being 19 years old or younger. And amongst these young people are scores of innovators and entrepreneurs who are looking to bring homegrown innovation to their continent and share it with the outside world.
Nowhere is this more apparent than with the #Africa2Moon Mission, a crowdfunded campaign that aims to send a lander or orbiter to the Moon in the coming years.
Spearheaded by the Foundation for Space Development – a non-profit organization headquartered in Capetown, South Africa – the goal of this project is to fund the development of a robotic craft that will either land on or establish orbit around the Moon. Once there, it will transmit video images back to Earth, and then distribute them via the internet into classrooms all across Africa.
In so doing, the project’s founders and participants hope to help the current generation of Africans realize their own potential. Or, as it says on their website: “The #Africa2Moon Mission will inspire the youth of Africa to believe that ‘We Can Reach for the Moon’by really reaching for the moon!”
Through their crowdfunding and a social media campaign (Twitter hashtag #Africa2Moon) they hope to raise a minimum of $150,000 for Phase I, which will consist of developing the mission concept and associated feasibility study. This mission concept will be developed collaboratively by experts assembled from African universities and industries, as well as international space experts, all under the leadership of the Mission Administrator – Professor Martinez.
Martinez is a veteran when it comes to space affairs. In addition to being the convener for the space studies program at the University of Cape Town, he is also the Chairman of the South African Council for Space Affairs (the national regulatory body for space activities in South Africa). He is joined by Jonathan Weltman, the Project Administrator, who is both an aeronautical engineer and the current CEO of the Foundation for Space Development.
Phase I is planned to run from Jan to Nov 2015 and will be the starting point for Phase II of #Africa2Moon, which will be a detailed mission design. At this point, the #Africa2Moon mission planners and engineering team will determine precisely what will be needed to see it through to completion and to reach the Moon.
Beyond inspiring young minds, the program also aims to promote education in the four major fields of Science, Technology, Engineering, and Mathematics (aka STEM). Towards this end, they have pledged to commit 25% of all the funds they raise towards STEM education through a series of #Africa2Moon workshops for educators and students. In addition, numerous public engagement activities will be mounted in partnership with other groups committed to STEM education, science awareness, and outreach.
Africa is so often thought of as a land in turmoil – a place that is perennially plagued by ethnic violence, dictators, disease, drought, and famine. This popular misconception belies very positive facts about the growing economy of world’s second-largest and second-most populous continent.
That being said, all those working on the #Africa2Moon project hope it will enable future generations of Africans to bridge the humanitarian and economic divide and end Africa’s financial dependence on the rest of the world. It is also hoped that the mission will provide a platform for one or more scientific experiments, contribute to humankind’s knowledge of the moon, and form part of Africa’s contribution to global space exploration activities.
The project’s current list of supporters include the SpaceLab at the University of Cape Town, The South African Space Association, Women in Aerospace Africa, The Cape Town Science Centre, Space Commercial Services Group, Space Advisory Company, and the Space Engineering Academy. They have also launched a seed-funding campaign drive through its partnership with the UN Foundation’s #GivingTuesday initiative.
For more information, go to the Foundation’s website, or check out the mission’s Indiegogo or CauseVox page.
What fate awaits Phobos, one of the moons of Mars?
“All these worlds are yours except Europa, attempt no landing there.”
As much as I love Arthur C. Clarke and his books, I’ve got to disagree with his judgement on which moons we should be avoiding. Europa is awesome. It’s probably got a vast liquid ocean underneath its icy surface. There might even be life swimming down there, ready to be discovered. Giant freaky Europa whales or some kind of alien sharknado. Oh man, I just had the BEST idea for a movie.
So yea, Europa’s fine. The place we should really be avoiding is the Martian Moon Phobos. Why? What’s wrong with Phobos? Have I become some kind of Phobo…phobe? Is there any good reason to avoid this place?
Well first, its name tells us all we need to know. Phobos is named for the Greek god of Horror, and I don’t mean like the usual gods of horror as in Clive Barker, John Carpenter or Wes Craven, I mean that Phobos is the actual personification of Fear… possibly with a freaky lion’s head. And… there’s also the fact that Phobos is doomed.
Literally doomed. Living on borrowed time. Its days are numbered. It’s been poisoned and there’s no antidote. It’s got metal shards in its heart and the battery on it’s electro-magnet is starting to brown out. More specifically, in a few million years, the asteroid-like rock is going to get torn apart by the Martian gravity and then get smashed onto the planet.
It all comes down to tidal forces. Our Moon takes about 27 days to complete an orbit, and our planet takes around 24 hours to complete one rotation on its axis. Our Moon is pulling unevenly on the Earth and slowing its rotation down.
To compensate, the Moon is slowly drifting away from us. We did a whole episode about this which we’ll link at the end of the episode. On Mars, Phobos only takes 8 hours to complete an orbit around the planet. While the planet takes almost 25 hours to complete one rotation on its axis. So Phobos travels three times around the planet for every Martian day. And this is a problem.
It’s actually speeding up Mars’ rotation. And in exchange, it’s getting closer and closer to Mars with every orbit. The current deadpool gives the best odds on Phobos taking 30 to 50 million years to finally crash into the planet. The orbit will get lower and lower until it reaches a level known as the Roche Limit. This is the point where the tidal forces between the near and far sides of the moon are so different that it gets torn apart. Then Mars will have a bunch of teeny moons from the former Phobos.
And then good news! Those adorable moonlets will get further pulverized until Mars has a ring. But then bad news… that ring will crash onto the planet in a cascade of destruction to be described as “the least fun balloon drop of all time”. So, you probably wouldn’t want to live on Mars then either.
Count yourself lucky. What were the chances that we would exist in the Solar System at a time that Phobos was a thing, and not a string of impacts on the surface of Mars.
Enjoy Phobos while you can, but remember that real estate there is temporary. Might I suggest somewhere in the alien sharknado infested waters of Europa instead?
What do you think. Did Arthur C Clarke have it wrong? Should we explore Europa?
And if you like what you see, come check out our Patreon page and find out how you can get these videos early while helping us bring you more great content!
The various companies that had stuff sitting on the failed Orbital Sciences Antares rocket launch last month are busy looking for alternatives. One example is Planet Labs, which is best known for deploying dozens of tiny satellites from the International Space Station this year.
The company lost 26 satellites in the explosion. But within nine days of the Oct. 28 event, Planet Labs had a partial backup plan — send two replacements last-minute on an upcoming SpaceX Falcon 9 launch.
In what Planet Labs’ Robbie Schingler calls “the future of aerospace”, almost immediately after the explosion Planet Labs began working with NanoRacks, which launches its satellites from the space station, to find a replacement flight. Half of Planet Labs’ employees began building satellites, while the other half began working through the regulations and logistics. They managed to squeeze two satellites last-minute on to the next SpaceX manifest, which is scheduled to launch in December.
“In space, each element is very difficult to get right by itself, and it takes an ecosystem to deliver a capability this quickly,” wrote Schingler, a president and co-founder of the company, in a blog post last week.
“Central to making this possible was developing our own custom design of the satellite that is free from specialty suppliers (thus decreasing lead time) and having a spacecraft design optimized for manufacturing and automated testing. Moreover, we certainly couldn’t have done it without the collaboration from NanoRacks and support from NASA, and we thank them for their support. This is a great example for how to create a resilient aerospace ecosystem.”
There’s no word on how they will replace the other satellites, nor how this will affect Planet Labs’ vision (explained in this March TED talk) to have these small sentinels frequently circling Earth to provide near-realtime information on what is happening with our planet. But the company acknowledged that space is hard and satellites do get lost from time to time.
The quest for optimal sites to carry out astronomical observations has taken scientists to the frigid Arctic. Eric Steinbring, who led a team of National Research Council Canada experts, noted that a high Arctic site can, “offer excellent image quality that is maintained during many clear, calm, dark periods that can last 100 hours or more.” The new article by Steinbring and colleagues conveys recent progress made to obtain precise observations from a 600 m high ridge near the Eureka research base on Ellesmere Island, which is located in northern Canada.
The new telescope that Steinbring and his colleagues tested was located at the Polar Environment Atmospheric Research Laboratory (PEARL). The observatory can be accessed in winter by 4 x 4 trucks via a 15 km long road from a base facility at sea-level. That base camp is operated by Environment Canada and serviced by an airstrip and resupply ship in summer. Recently, wide-field cameras developed at the University of Toronto were deployed near Eureka to monitor thousands of stars, with the objective of expanding the exoplanet database.
Earlier work by Steinbring and colleagues indicated that data obtained from PEARL imply that clear weather prevails 68% of the time. After significant testing, the team concluded that the site “can allow reliable, uninterrupted temporal coverage during successive dark periods, in roughly 100 hour blocks with clear skies and good seeing.”
However, the optimal conditions can be interrupted by brief but potentially intense storms. In the article the team added that, “the primary issue is wind rather than the cold temperatures.” The PEARL facility is equipped with an important weather probe that conveys on-site conditions at 10 minute intervals, thanks to the Canadian Network for the Detection of Atmospheric Change (CANDAC).
There are numerous challenges that arise when observing from the Arctic, but scientists like Steinbring have worked to overcome them, potentially enabling new studies of gravitational lenses and other pertinent phenomena. Indeed, astronomical observations are likewise being obtained from Antarctica. For example, there is the Antarctic Search for Transiting Exoplanets (ASTEP) 40 cm telescope at Dome C, and three 50 cm Antarctic Survey Telescopes (AST3) at Dome A, Antarctica. Steinbring remarked that floorspace is potentially available for up to 5 more telescopes at PEARL, if the compact design they studied was adopted.
E. Steinbring and his colleagues B. Leckie and R. Murowinski are associated with the National Research Council Canada, Herzberg Astronomy and Astrophysics in Victoria, Canada. An electronic preprint of their article is available on arXiv, and the findings were presented recently at theAdapting to the Atmosphere Conference in Durham, UK.
There are so many fun sights to see in the sky that are pure astronomical magic. And then there are the spectacular human-created sights. One of those sights is watching satellites from the Iridium constellation that — because of their odd shape — produce spectacular flares that can be brighter than the planet Venus.
Because most of these satellites are still under control by their parent company, their flare timings are easy to predict. And now astrophotographer Thierry Legualt has caught them in action on a video.
“Usually they are photographed in long exposures,” Legault told Universe Today via email. “But last summer I filmed three of them in the Big Dipper and Orion, and they were so bright a pond reflected the flare. In video you can see the real speed of the event.”
The third sequence on the video might look a little odd, but Legault said he rotated the camera 90°. “I found it funny like that,” he said. “Tilt your head or your screen!?”
According to a July Sky & Telescope article, the constellation includes 66 satellites — down from the planned 77 — and is named after element 77 in the periodic table. Normally these machines drift along like a faint star, but when the sunlight catches the side just right, out comes the flash.
“A really bright one can take your breath away,” wrote Bob King, who is also a writer here on Universe Today. “I’ve been lucky enough to witness a few –8 passes and can only describe the experience as alarming. It’s not natural to see a starlike object glow so brilliantly. If you’ve ever wondered what a nearby supernova might look like, treat yourself to one of these.”
And now we have six people in space again — including the first-ever Italian woman to reach orbit. Samantha Cristoforetti has been delighting people worldwide with her behind-the-scenes training posts as she prepares for her “Futura” mission, which will see her spend 5.5 months on the International Space Station with her crewmates. We have the NASA video from the big day above, and some photos from the launch below.
Cristoforetti has been sharing Spotify playlists and amusing tweets with more than 131,000 Twitter followers, not to mention people on Flickr and Google Plus. Her sense of humor and eye for the unusual will make for a fun few months in orbit along with the rest of her crew, NASA’s Terry Virts and Russia’s Anton Shkaplerov.
Just had what was probably my longest shower ever. Good Russian wisdom to leave plenty of time for it on the schedule! #NoRushOnLaunchDay
On station for their arrival last night was the second half of their crew: Barry Wilmore (NASA), Elena Serova (Russia) and Alexander Samoukutyaev (Russia). And in March 2015, a big event occurs: the first one-year mission on the International Space Station will begin with the arrival of the next crew.
The launch took place at 4:01 p.m. EDT (9:01 p.m. UTC) from the Baikonur Cosmodrome in Kazakhstan aboard a Soyuz rocket.
Up close launch pad camera view as Antares descended into a hellish inferno after the first stage propulsion system at the base of Orbital Sciences’ Antares rocket exploded moments after blastoff from NASA’s Wallops Flight Facility, VA, on Oct. 28, 2014, at 6:22 p.m. The south side engine nozzle is clearly intact in this image. Credit: Ken Kremer – kenkremer.com
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NASA WALLOPS FLIGHT FACILITY, VA – All was calm, the air was crisp with hope, and the skies were clear as far as the eye could see as the clock ticked down to T MINUS Zero for the Oct. 28, 2014, blastoff of an Orbital Sciences commercial Antares rocket from NASA’s Wallops Flight Facility, VA, on a mission of critical importance bound for the International Space Station and stocked with science and life support supplies for the six humans living and working aboard.
Tragically it was not to be – as I reported live from the NASA Wallops press site on that fateful October day. The 133 foot tall rocket’s base exploded violently and unexpectedly just seconds after a beautiful evening liftoff due to the failure of one of the refurbished AJ26 first stage “Americanized” Soviet-era engines built four decades ago.
And now for the first time, I can show you precisely what the terrible incendiary view was like through exclusive, up close launch pad photos and videos from myself and a group of space journalists working together from Universe Today, AmericaSpace, and Zero-G news.
I was an eyewitness to the awful devastation suffered by the Antares/Cygnus Orb-3 mission from the press viewing site at NASA Wallops located at a distance of about 1.8 miles away from the launch complex.
Our remote cameras were placed directly adjacent to the Antares pad OA at the Mid-Atlantic Regional Spaceport (MARS) on Wallops Island, VA, and miraculously survived the rocket’s destruction as it plunged to the ground very near and just north of the seaside launch pad.
All of our team’s cameras and image cards were impounded by Orbital’s Accident Investigation Board (AIB) that was assembled quickly in the aftermath of the disaster and charged with determining the root cause of the launch failure.
The photos captured on our image cards were used as evidence and scrutinized by the investigators searching for clues as to the cause, and have only just been returned to us in the past two days. Similar NASA and Orbital Sciences photos have not been publicly released.
Collected here in Part 1 is a gallery of images from our combined journalist team of Universe Today, AmericaSpace, and Zero-G news. Part 2 will follow shortly and focus on our up close launch pad videos.
My lead image shows Antares’ descent into a hellish inferno. And more below clearly show that the south side engine nozzle was intact after the explosion. Thus it was the north side engine that blew up. See my up close AJ26 engine photo below.
Images from my colleagues Matthew Travis, Elliot Severn, Alex Polimeni, Charles Twine, and Jeff Seibert also show exquisite views of the explosion, fireball, and wreckage from various positions around the launch pad.
Moments after liftoff, the highly anticipated Antares launch suddenly devolved into utter catastrophe and a doomed descent into a hellish inferno of bloodcurdling terror – falling as a flaming incinerating carcass of unspeakable horror that ended in a mammoth deafening explosion as the pitiful wreckage smashed into the ground and blew back upwards as a raging fireball and hurtling debris that was visible across a wide swath of the sky.
The awful scene was seen by hordes of expectant spectators for miles around the Wallops area.
The disaster’s cause has almost certainly been traced to a turbopump failure in one of the rocket’s Soviet-era first stage engines, according to official statements from David Thompson, Orbital’s Chairman and Chief Executive Officer.
The AJ26 engines were originally manufactured some 40 years ago in the then Soviet Union as the NK-33.
They were refurbished and “Americanized” by Aerojet Rocketdyne.
“While still preliminary and subject to change, current evidence strongly suggests that one of the two AJ26 main engines that powered Antares first stage failed about 15 seconds after ignition. At this time, we believe the failure likely originated in or directly affected the turbopump machinery of this engine, but I want to stress that more analysis will be required to confirm that this finding is correct,” said Thompson.
Overall this was the 5th Antares launch using the AJ26 engines.
The 14 story Antares rocket is a two stage vehicle.
The liquid fueled first stage is filled with about 550,000 pounds (250,000 kg) of Liquid Oxygen and Refined Petroleum (LOX/RP) and powered by a pair of AJ26 engines that generate a combined 734,000 pounds (3,265kN) of sea level thrust.
The Oct. 28 launch disaster was just the latest in a string of serious problems with the AJ-26/NK-33 engines.
Earlier this year an AJ26 engine failed and exploded during pre launch acceptance testing on a test stand on May 22, 2014 at NASA’s Stennis Space Center in Mississippi.
Besides completely destroying the AJ26 engine, the explosion during engine testing also severely damaged the Stennis test stand. It has taken months of hard work to rebuild and restore the test stand and place it back into service.
Antares was carrying Orbital’s privately developed Cygnus pressurized cargo freighter loaded with nearly 5000 pounds (2200 kg) of science experiments, research instruments, crew provisions, spare parts, spacewalk and computer equipment and gear on a critical resupply mission dubbed Orb-3 bound for the International Space Station (ISS).
It was the heaviest cargo load yet lofted by a Cygnus. Some 800 pounds additional cargo was loaded on board compared to earlier flights. That was enabled by using the more powerful ATK CASTOR 30XL engine to power the second stage for the first time.
The astronauts and cosmonauts depend on a regular supply train from the ISS partners to kept it afloat and productive on a 24/7 basis.
The Orbital-3, or Orb-3, mission was to be the third of eight cargo resupply missions to the ISS through 2016 under the NASA Commercial Resupply Services (CRS) contract award valued at $1.9 Billion.
Orbital Sciences is under contract to deliver 20,000 kilograms of research experiments, crew provisions, spare parts, and hardware for the eight ISS flights.
Enjoy the photo gallery herein.
And watch for Part 2 shortly with exquisite videos, more photos, and personal reflections from our team.
Watch here for Ken’s ongoing reporting about Antares and NASA Wallops.
Stay tuned here for Ken’s continuing Earth and Planetary science and human spaceflight news.
And if you’re interested in looking back, here’s an archive to all the past Carnivals of Space. If you’ve got a space-related blog, you should really join the carnival. Just email an entry to [email protected], and the next host will link to it. It will help get awareness out there about your writing, help you meet others in the space community – and community is what blogging is all about. And if you really want to help out, sign up to be a host. Send an email to the above address.
After a decade of hard work, numerous twists and turns, and ups and downs, NASA’s new Orion deep space crew vehicle is finally, and officially, marching towards its maiden blastoff in less than two week’s time.
The Orion spacecraft cleared one of the final hurdles to its first launch when top managers from NASA and Lockheed Martin successfully completed a key review of the vehicle’s systems ahead of the looming Dec. 4 flight test.
Orion passed the Flight Readiness Review (FRR) on Thursday, Nov. 20, and officials announced that the spacecraft is “GO” for proceeding on the road to launch – and one day on to Mars!
The FRR is a rigorous assessment of the spacecraft, its systems, mission operations, and support functions needed to successfully complete Orion’s first voyage to space.
Lockheed Martin is the prime contractor for Orion and recently completed its fabrication in the Neil Armstrong Operations and Checkout Building at the Kennedy Space Center in September 2014.
Orion will lift off on a Delta IV Heavy rocket on its inaugural test flight to space on the uncrewed Exploration Flight Test-1 (EFT-1) mission at 7:05 a.m. EST on December 4, 2014, from Space Launch Complex 37 (SLC-37) at Cape Canaveral Air Force Station in Florida.
The United Launch Alliance Delta IV Heavy rocket is the world’s most powerful rocket and the only booster sufficiently powerful to launch the 50,000 pound Orion EFT-1 spacecraft to orbit.
The rocket was transported to pad 37 in late September. Then, on Nov. 12, this path finding Orion spacecraft was itself rolled out to the launch pad and hoisted and bolted atop the Delta IV Heavy.
The critical December test flight will pave the way for the first human missions to deep space in more than four decades since NASA’s Apollo moon landing missions ended in 1972.
To learn more about the major events and goals happening during Orion’s EFT-1 mission be sure to check out NASA’s cool new set of infographics explaining the 8 key events in my story – here.
The two-orbit, four and a half hour Orion EFT-1 flight around Earth will lift the Orion spacecraft and its attached second stage to an orbital altitude of 3,600 miles, about 15 times higher than the International Space Station (ISS) – and farther than any human spacecraft has journeyed in 40 years.
EFT-1 will test the rocket, second stage, jettison mechanisms, as well as avionics, attitude control, computers, and electronic systems inside the Orion spacecraft.
Then the spacecraft will carry out a high speed re-entry through the atmosphere at speeds approaching 20,000 mph and scorching temperatures near 4,000 degrees Fahrenheit to test the heat shield, before splashing down for a parachute assisted landing in the Pacific Ocean.
Orion is NASA’s next generation human rated vehicle that will carry America’s astronauts beyond Earth on voyages venturing farther into deep space than ever before – beyond the Moon to Asteroids, Mars, and other destinations in our Solar System.
Watch for Ken’s ongoing Orion coverage and he’ll be onsite at KSC in the days leading up to the historic launch on Dec. 4.
Stay tuned here for Ken’s continuing Orion and Earth and planetary science and human spaceflight news.
Europa, Jupiter’s sixth-closest moon, has long been a source of fascination and wonder for astronomers. Not only is it unique amongst its Jovian peers for having a smooth, ice-covered surface, but it is believed that warm, ocean waters exist beneath that crust – which also makes it a strong candidate for extra-terrestrial life.
And now, combining a mosaic of color images with modern image processing techniques, NASA has produced a new version of what is perhaps the best view of Europa yet. And it is quite simply the closest approximation to what the human eye would see, and the next best thing to seeing it up close.
The high-resolution color image, which shows the largest portion of the moon’s surface, was made from images taken by NASA’s Galileo probe. Using the Solid-State Imaging (SSI) experiment, the craft captured these images during it’s first and fourteenth orbit through the Jupiter system, in 1995 and 1998 respectively.
The view was previously released as a mosaic with lower resolution and strongly enhanced color (as seen on the JPL’s website). To create this new version, the images were assembled into a realistic color view of the surface that approximates how Europa would appear to the human eye.
As shown above, the new image shows the stunning diversity of Europa’s surface geology. Long, linear cracks and ridges crisscross the surface, interrupted by regions of disrupted terrain where the surface ice crust has been broken up and re-frozen into new patterns.
Images taken through near-infrared, green, and violet filters have been combined to produce this view. The images have been corrected for light scattered outside of the image to provide a color correction that is calibrated by wavelength. Gaps in the images have been filled with simulated color based on the color of nearby surface areas with similar terrain types.
These color variations across the surface are associated with differences in geologic feature type and location. For example, areas that appear blue or white contain relatively pure water ice, while reddish and brownish areas include non-ice components in higher concentrations.
The polar regions, visible at the left and right of this view, are noticeably bluer than the more equatorial latitudes, which look more white. This color variation is thought to be due to differences in ice grain size in the two locations.
This view of Europa stands out as the color view that shows the largest portion of the moon’s surface at the highest resolution. An earlier, lower-resolution version of the view, published in 2001, featured colors that had been strongly enhanced. Space imaging enthusiasts have produced their own versions of the view using the publicly available data, but NASA has not previously issued its own rendition using near-natural color.
The image also features many long, curving, and linear fractures in the moon’s bright ice shell. Scientists are eager to learn if the reddish-brown fractures, and other markings spattered across the surface, contain clues about the geological history of Europa and the chemistry of the global ocean that is thought to exist beneath the ice.
This is of particular interest to scientists since this supposed ocean is the most promising place in our Solar System, beyond Earth, to look for present-day environments that are suitable for life. The Galileo mission found strong evidence that a subsurface ocean of salty water is in contact with a rocky seafloor. The cycling of material between the ocean and ice shell could potentially provide sources of chemical energy that could sustain simple life forms.
Future missions to Europa, which could involve anything from landers to space penetrators, may finally answer the question of whether or not life exists beyond our small, blue planet. Picturing this world in all of its icy glory is another small step along that path.
In addition to the newly processed image, JPL has released a new video that explains why this likely ocean world is a high priority for future exploration: