Meet Dragon V2 - SpaceX CEO Elon pulls the curtain off manned Dragon V2 on May 29, 2014 for worldwide unveiling of SpaceX's new astronaut transporter for NASA. Credit: SpaceX
Caption: Animation of SpaceX Dragon V2 astronaut transporter. Credit: SpaceX
Would you like to meet and fly aboard SpaceX’s next generation manned Dragon V2 spacecraft?
Well hop aboard for a ride, take a seat and prepare for the thrill of a lifetime to the International Space Station (ISS) and back.
Watch the cool animation above to see exactly ‘How it Works!’
Now you can experience the opening salvo in the exciting new chapter of ‘Commercial Human Spaceflight.’
The commercial crew effort is led by a trio of private American aerospace company’s (SpaceX, Boeing & Sierra Nevada) in an intimate partnership with NASA to get American’s back in space on American rockets from American Soil – rather than being totally dependent on Russian rocket technology and Soyuz capsules for astronaut rides to orbit.
“We need to have our own capability to get our crews to space. Commercial crew is really, really, really important,” NASA Administrator Charles Bolden told me in an exclusive interview.
Billionaire entrepreneur and SpaceX CEO Elon Musk let the curtain to the future drop on Thursday, May 29 to reveal his company’s new manned Dragon V2 astronaut transporter for all the world to see during a live streaming webcast direct from SpaceX’s state-of-the-art design and manufacturing facility and Headquarters in Hawthorne, CA.
And with a flair worthy of the premiere of a blockbuster Hollywood Science Fiction movie he unveiled the gum-dropped shaped Dragon V2 – and the lively animation. Although its not known if he’ll provide the crews with musical entertainment during the trip too.
As you’ll quickly notice watching the animation, the sleek styled V2 manned Dragon is a far cry ahead of the current V1 cargo Dragon.
“We wanted to take a big step in spacecraft technology. It is a big leap forward in technology and takes things to the next level,” said Musk.
The top of the V2 is equipped to open up and expose a docking probe so it’s able to dock autonomously at the ISS – and at the same port as NASA’s now retired space shuttle orbiters.
‘Catching a Dragon by the tail’- with the Canadian built robot arm as the stations astronauts like to say and berthing it at an Earth-facing port on the Harmony module, will be a thing of the past.
“No robotic arm necessary!” Musk explained.
SpaceX Dragon V2 docks at the ISS. Credit: SpaceX
And for departure there’s another big difference – powerful SuperDraco landing rockets for pinpoint touchdown accuracy rather than an ocean splashdown.
The animation shows a thrilling land landing back at the Kennedy Space Center launch base.
“An important characteristic of that is its ability to land anywhere on land, propulsively. It can land anywhere on Earth with the accuracy of a helicopter,” Musk said.
“I think that’s what a spaceship should be able to do.”
Musk and SpaceX are not alone aiming to get Americans back to space.
Boeing and Sierra Nevada are competing with SpaceX to build the next generation spaceship to ferry astronauts to and from the ISS by 2017 using seed money from NASA’s Commercial Crew Program in a public/private partnership.
The BoeingCST-100 and Sierra Nevada Dream Chaser ‘space taxis’ are also vying for funding in the next round of contracts to be awarded by NASA around late summer 2014.
Read my earlier “Dragon V2” unveiling event articles – here, here and here.
Enjoy!
SpaceX CEO Elon Musk unveils SpaceX Dragon V2 next generation astronaut spacecraft on May 29, 2014. Credit: Robert Fisher/America Space
Stay tuned here for Ken’s continuing SpaceX, Boeing, Sierra Nevada, Orbital Sciences, commercial space, Orion, Mars rover, MAVEN, MOM and more planetary and human spaceflight news.
The 'face' on Mars, a popular landform in Cydonia Region on Mars. Credit: NASA/JPL/University of Arizona.
Intrigued by the thought of alien artifacts on Mars, with structures like a Martian-built statue of a giant face surrounded by pyramids or even cities? Better check the math on that. Better yet, Stuart Robbins has already checked that math and BOOM! it doesn’t check out.
So called “Mars anomalists” like Richard Hoagland have already been debunked mightily by folks like Phil Plait, but Robbins — who hosts the “Exposing Pseudo Astronomy” podcast — takes it to a whole new level. He’s just put out a video version of his podcast about claims about the Cydonia region on Mars, some of the math behind it, an exploration of the “null hypothesis” (what the results would be if it were purely random), and draws conclusions based on the latest orbital imagery of Mars.
Hoagland and others claim some of the features in Cydonia display special geometry and numbers that are encoded within them. And, the only way those numbers and that geometry could be there is if it was created by some sort of intelligence, i.e aliens. Robbins provides detailed explanations of the mathematical simulations and the arguments against these claims.
“What the Mars anomalists do is a really good example of cherry picking/the Texas Sharpshooter fallacy,” Robbins told Universe Today. He concludes the video by basically saying, “Hey! Space exploration is still awesome and cool, and you really don’t NEED the pseudoscience to make it amazing and rewarding.”
Artist's impression of "mega-Earth" Kepler 10c. Credit: David A. Aguilar (CfA)
Can you imagine a world that is 17 times as massive as Earth, but still rocky? Or two planets that are doomed to be swallowed up by their parent star in just a blink of astronomical time?
While these scenarios sound like science fiction, these are real-life finds released today (June 2) at the American Astronomical Association meeting in Boston.
Here’s a rundown of the finds about these planets in our ever-more-amazing universe.
‘Mega-Earth’ Kepler-10c
Spinning around its star every 45 days is Kepler-10c, which is about 2.3 times as large as Earth but a heavyweight, at 17 times more massive. The planet was discovered by the prolific NASA Kepler space telescope (which was sidelined after a reaction wheel failed last year, but now has been tasked with a new planet-hunting mandate.)
While initially astronomers thought Kepler-10c was a “mini-Neptune”, or a world that is similar to that planet in our solar system, its mass measured by the HARPS-North instrument on the Galileo National Telescope showed it was a rocky world. What’s more, astronomers believe the planet did not “let go” of any atmosphere over time, which implies the planet’s past is similar to what it was today.
Here’s the other neat thing: astronomers found that the system was 11 billion years old, at a time when the universe was young (it was formed 13.7 billion years ago) and the elements needed to make rocky planets were scarce. This implies that rocky planets could have formed earlier than previously thought.
“I was wrong that old stars do not have rocky planets, which has consequences about the Fermi Paradox,” the Harvard-Smithsonian Center for Astrophysics’s (CfA) Dimitar Sasselov said in a webcast press conference today (June 2). The Fermi Paradox, simply put, refers to the question of why we can’t see civilizations since they are assumed to have spread quite a ways since the universe was formed.
Artist’s impression of Kepler-56b being torn apart by its star about 130 million years from today. Its sibling planet, Kepler-56c, will last until 155 million years from now. Credit: David A. Aguilar (CfA)
‘We’re doomed!’ Kepler-56b and Kepler-56c
If there was anybody in the vicinity of these two planets, you’d want to move out of the way fairly quickly — at least when talking about astronomical time. Both of these planets, whose orbits are within the equivalent distance of Mercury to the sun, are expected to be swallowed up by their star in 130 million years (for Kepler-56b) and 155 million years (Kepler-56c). It’s the first time two doomed planets have been found in a single system.
“Possibly the core of planet will be left behind and you [will] see this dead corpse floating behind in the universe,” said CfA’s Gongjie Li in the press conference.
There are two factors behind this: the size of the star will enlarge as it gets older (which is typical among stars) and the tidal forces between the planets and their star will also cause them to slow down in their orbits and rip apart. Interestingly enough, another gas giant planet called Kepler-56d will remain safe from most of the chaos since its orbit is equivalent to the asteroid belt in our own solar system.
“Looking at this system is like foreseeing our own solar system,” added Li, referring to the fact that in another five billion years or so our sun will enlarge and swallow Mercury and Venus at the least, boiling off all the oceans on our planet and killing anything left.
Artist’s conception of an exoplanet orbiting a red dwarf star. Credit: David A. Aguilar (CfA)
Windy City: Why living near a red dwarf might be a bad idea
One fertile ground for exoplanet discoveries — particularly when looking for planets about Earth’s size in the habitable zone — is red dwarfs, because they are smaller and therefore have less light to obscure any rocky worlds orbiting nearby. A new study warns that they could be less friendly to life than previously believed.
CfA’s Ofer Cohen said that red dwarfs can have intense stellar winds, when looking at the model of a known red dwarf with three planets around it: KOI 1422.02, KOI 2626.01, KOI 584.01. Even a magnetic field the size of Earth would not be able to protect the planet from being stripped of its atmosphere assuming a certain intensity of stellar flares.
A member of the audience pointed out that the red dwarf star under study likely has stronger winds than 95% of all red dwarfs, however. Cohen acknowledged that, but added “the main effect is not the stellar activity, but these giants are close to the star.” All the same, this could require a more nuanced understanding of the habitable zone around these stars, he added.
Artist’s impression of exoplanets. Credit: J. Jauch
Heavy metal: Figuring out how much planets have
In astronomical terms, any elements heavier than hydrogen and helium are considered to be “metallic”. Past research found that metal-rich stars tend to have hot Jupiter exoplanets, while the smaller planets have a larger span of metal possibilities.
A team led by CfA’s Lars Buchhave surveyed more than 400 stars with 600 exoplanets, and found that planets smaller than 1.7 times the size of Earth are more likely to be rocky, while those than are 3.9 times the size of Earth or larger are likely gassy.
In between is a zone called “gas dwarfs”, which are planets 1.7 and 3.9 times the size of Earth that likely have hydrogen and helium atmospheres blanketing their surface.
Also intriguing: the researchers discovered that planets far away from their stars can get larger before picking up a lot of gas and becoming a “gas dwarf”, presumably because there isn’t as much gas material out there.
The team also discovered that stars with smaller, Earth-like worlds metallicities like our sun, while stars with “gas dwarfs” have more metals, and stars with gas giants have even more metals. But bear in mind these are for planets close to their host star, which are easiest for Kepler to find. Buchhave plans to do work for planets further away.
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.
A coal-fired plant in Glenrock, Wyoming. Image Credit: Greg Goebel
At the end of his first year in office, President Obama made a bold promise: the United States would cut its greenhouse gas emissions substantially by 2020.
Unfortunately it was a risky pledge that hinged on Congress. After President Obama was unable to get his major climate change proposal through Congress in his first term, it seemed as though his pledge to the rest of the World and planet Earth might disintegrate into thin air.
But today, President Obama announced plans to bypass Congress entirely. By using his executive authority under the Clean Air Act, he proposed an Environmental Protection Agency regulation to cut carbon pollution from the nation’s power plants 30 percent from 2005 levels by 2030. It’s one of the strongest actions ever taken by the United States government to fight climate change.
“The shift to a cleaner-energy economy won’t happen overnight, and it will require tough choices along the way,” President Obama said Saturday in his weekly radio and Internet address, previewing Monday’s announcement. “But a low-carbon, clean-energy economy can be an engine of growth for decades to come. America will build that engine. America will build the future, a future that’s cleaner, more prosperous and full of good jobs.”
The regulation targets the largest source of carbon pollution in the United States: coal-fired power plants. So naturally it has already met huge opposition.
“The administration has set out to kill coal and its 800,000 jobs,” said Senator Michael B. Enzi of Wyoming, the nation’s top coal-producing state, in response to President Obama’s Saturday address. “If it succeeds in death by regulation, we’ll all be paying a lot more money for electricity — if we can get it. Our pocketbook will be lighter, but our country will be darker.”
But rather than forcing coal plants to immediately shutdown, the E.P.A. will allow States several years to retire existing plants. They estimate that by 2030, 30 percent of U.S. electricity will still come from coal, down from about 40 percent today.
The regulation also gives a wide range of options to achieve the pollution cuts. States are encouraged to reduce emissions by making changes across the electricity systems. They’re encouraged to install new wind and solar generation technology. This will create a huge demand for designing and building energy-efficient technology.
The plan is flexible. “That’s what makes it ambitious, but achievable,” said Gina McCarthy, the E.P.A. administrator, in a speech this morning. “That’s how we can keep our energy affordable and reliable. The glue that holds this plan together — and the key to making it work — is that each state’s goal is tailored to its own circumstances, and states have the flexibility to reach their goal in whatever way works best for them.”
The proposal will also help the economy, not hurt it. The E.P.A. estimates that the regulation will cost $7.3 billion to $8.8 billion annually, but will lead to economic benefits of $55 billion to $93 billion throughout the regulation’s lifetime.
The proposal unveiled today is only a draft, open to public comment. Already it has received criticism and praise from industry groups and environmentalists alike. President Obama plans to finalize the regulation by June 2015 so that it will be in place before he leaves office.
To see why Universe Today writes on climate change, and even climate policy, please read a past article on the subject.
A sun pillar among the clouds at sunset create the look of second Sun on May 31, 2014. Credit: Dave Walker.
Sunset on Tatooine? Nah, just an unusual combination of a dazzling orange sunset, clouds and a sun pillar that creates an “echo” effect of the setting Sun. As seen by astrophotographer Dave Walker in the UK on May 31, 2014.
Want to get your astrophoto featured on Universe Today? Join our Flickr group or send us your images by email (this means you’re giving us permission to post them). Please explain what’s in the picture, when you took it, the equipment you used, etc.
Sunset-lit clouds swirl over Perth on May 31, 2014 (Reid Wiseman/NASA)
On May 28 the crew of Expedition 40/41 launched from Baikonur Cosmodrome, their Soyuz TMA-13M arriving at the International Space Station about eight and a half hours later. And it didn’t take much time for the newly-arrived NASA astronaut Reid Wiseman to start taking photos from his new vantage point in orbit and sharing them on Twitter for the rest of us to enjoy! Here are some of Reid’s latest images from the edge of space, looking down on the beautiful blue world we call home.
One of Reid Wiseman’s first few tweets from space!A “beautiful pass over the Falkland Islands” (aka Islas Malvinas) on May 30 with docked Soyuz in the foregroundReid confirmed that the Earth is indeed round with a 12mm lens on June 1Looking down on glacial flows near the Strait of MagellanPink clouds at sunset may look beautiful from Earth but “not as pretty here” according to Reid WisemanMay 31 was a “nice day to hit the beach” in Santos, Brazil“Our planet is almost all ocean and so pretty,” Tweeted Reid on June 1A “Soyuz group selfie” in the cupola with Expedition 40/41 crew members Alexander Gerst, Oleg Artemyev, and Reid Wiseman, shared on June 2“Chile just left me speechless,” Reid tweeted on June 4“Clouds turn 2D into 3D” tweeted Reid on Thursday, June 5Just a week into his stay aboard the ISS microgravity is already second nature!
A series of All-Sky (fish eye) images showing the plasma trail left by a fireball, which extends 92 degrees across the northern half of the sky. These images are 5 second snapshots captured at 37.8 MHz with the LWA1 radio telescope. The bright steady sources (Cygnus A, Cassiopeia A, the galactic plane, etc) have been removed using image subtraction. Image Credit: Gregory Taylor (University of New Mexico)
At any given moment, it seems, the sky is sizzling with celestial phenomena waiting to be stumbled upon. New research using the Long Wavelength Array (LWA), a collection of radio dishes in New Mexico, found quite the surprise. Fireballs — those brilliant meteors that leave behind glowing streaks in the night sky — unexpectedly emit a low radio frequency, hinting at new unexplored physics within these meteor streaks.
The LWA keeps its eyes to the sky day and night, probing a poorly explored region of the electromagnetic spectrum. It’s one of only a handful of blind searches carried out below 100 MHz.
Over the course of 11,000 hours, graduate student Kenneth Obenberger from the University of New Mexico and colleagues found 49 radio bursts, 10 of which came from fireballs.
Most of the bursts appear as large point sources, limited to four degrees, roughly eight times the size of the full Moon. Some, however, extend several degrees across the sky. On January 21, 2014, a source left a trail covering 92 degrees in less than 10 seconds (see above). The end point continued to glow for another 90 seconds.
The only known astrophysical object with this ability is a fireball. So Obenberger and colleagues set out to see if NASA’s All Sky Fireball Network had detected anything at the same location and time as the bursts.
While the network shares only a portion of the sky with the LWA, the fireballs seen in this direction matched fireballs caught by NASA. Additionally, most bursts did occur directly after the peak of a bright meteor shower.
The top panel is a histogram showing the number of events per day as compared to several major meteor showers (red lines).
The fireballs detected here are extremely energetic, traveling with an average velocity of 68 km/s, near the upper end of the meteorite velocity spectrum (from 11 km/s to 72 km/s).
They can be seen in the radio due to radio forward scattering. When fast-moving meteoroids strike Earth’s atmosphere they heat and ionize the air in their path. The luminous ionized trails reflect radio waves. During a meteor shower these waves can not only be picked up by vast arrays, such as the one in New Mexico, but by your TV and AM/FM radio transmitter.
Whereas most fireballs have been detected well over 100 MHz, “we’ve discovered that they also produce a low frequency pulse,” says Obenberger’s PhD advisor, Gregory Taylor.
This pulse is telling us something about the physical conditions in the plasma created by the meteor. “It could be cyclotron radiation (emitted from moving charges in a magnetic field), or perhaps some sort of plasma wave leakage from the trail, or maybe something completely different,” says Obenberger. “It’s too early to tell at the moment.”
Meteors come in a range of energies and sizes. So investigating this unexpected signature further will yield new insights into the interaction between meteors and our atmosphere.
“This is just the beginning,” says Taylor. “Now we have to put this new technique to use — find out more about the spectrum of the pulse and the meteors that produce it. It’s an entirely new way of looking at meteors and how they interact with our atmosphere.”
If you’re curious what’s currently emitting radio waves in the New Mexico sky check out the LWA’s live radio cam.
The paper was published in Astrophysical Journal Letters today and is available for download here.
Near Earth asteroid 2014 KH39, discovered on May 24, 2014, is the faint 'star' in the crosshairs in this photo made on May 31. The telescope tracked the asteroid, so the stars are trailed. The streak is a satellite. Credit: Gianluca Masi
Got any plans Tuesday? Good. Keep them but know this. That day around 3 p.m. CDT (20:00 UT) asteroid 2014 KH39 will silently zip by Earth at a distance of just 272,460 miles (438,480 km) or 1.14 LDs (lunar distance). Close as flybys go but not quite a record breaker. The hefty space rock will buzz across the constellation Cepheus at nearly 25,000 mph (11 km/sec) near the Little Dipper at the time.
Observers in central Europe and Africa will have dark skies for the event, however at magnitude +17 the asteroid will be too faint to spot in amateur telescopes. No worries. The Virtual Telescope Project, run by astrophysicist Gianluca Masi, will be up and running with real-time images and live commentary during the flyby. The webcast begins at 2:45 p.m. CDT June 3.
2014 KH39 was discovered on May 24 by Richard Kowalski of the Catalina Sky Survey. (Kowalski is the same astronomer who discovered asteroid 2008 TC3, the small asteroid that impacted in Sudan in 2008). Further observations by the CSS and additional telescopes like Pan-STARRS 1 in Hawaii nailed down its orbit as an Earth-approacher with an approximate size of 72 feet (22 meters). That’s a tad larger than the 65-foot Chelyabinsk asteroid that exploded into thousands of small stony meteorites over Russia in Feb. 2013.
Diagram showing the orbit of 2014 KH39. Yellow shows the portion of its orbit above the plane of Earth’s orbit (grey disk); blue is below the plane. When farthest, the asteroid travels beyond Mars into the asteroid belt. It passes closest to Earth around 3 p.m. CDT June 3. Credit: IAU Minor Planet Center
Since this asteroid will safely miss Earth we have nothing to fear from the flyby. I only report it here to point out how common near-Earth asteroids are and how remarkable it is that we can spot them at all. While we’re a long ways from finding and tracking all potentially hazardous asteroids, dedicated sky surveys turn up dozens of close-approaches every year. On the heels of 2014 KH39, the Earth-approaching asteroid 2014 HQ124 will pass 3.3 LDs away 5 days later on June 8. With a diameter estimated at more than 2,100 feet (650-m) it’s expected to become as bright as magnitude +13.7. Southern hemisphere observers might track it with 8-inch and larger telescopes as its speeds across Horologium and Eridanus the morning before closest approach.
The chart shows the cumulative known total of near-Earth asteroids (NEAs) vs. time. The blue area shows all NEAs while the red shows those roughly 1 km and larger. Thanks to many ground-based surveys underway as well as space probes like the Wide-field Infrared Survey Explorer (WISE), discovery totals have ramped up in recent years. There are probably millions of NEOs smaller than 140 meters waiting to be discovered. Credit: NASA
Perusing the current list of upcoming asteroid approaches, these two will be our closest visitors at least through early August. Near-Earth objects (NEOs) are comets and asteroids whose original orbits have been re-worked by the gravity of the planets – primarily Jupiter – into new orbits that allow them to approach relatively close to Earth. The ones we’re most concerned about are a subset called Potentially Hazardous Asteroids or PHAs, defined as objects that approach within 4.65 million miles (7.48 million km) of Earth and span 500 feet (150-m) across or larger. The key word here is ‘potential’. PHAs won’t necessarily hit the Earth – they only have the potential to do so over the vastness of time. On the bright side, PHAs make excellent targets for sampling missions.
Most near-Earth asteroids fall into three classes named after the first asteroid discovered in that class. Apollo and Aten asteroids cross Earth’s orbit; Amors orbit just beyond Earth but cross Mars’ orbit. Credit: Wikipedia
As of May 30, 2014, 11,107 near-Earth objects have been discovered with 860 having a diameter of 1 km or larger. 1,481 of them have been further classified as potentially hazardous. NASA’s Near-Earth Object Program estimates that over 90% of NEOs larger than 1 km (the most potentially lethal to the planet) have been discovered and they’re now working to find 90% of those larger than 459 feet (140 meters) across. Little by little we’re getting to better know the neighborhood.
The probability that either 2014 KH39 and 2014 HQ124 will hit Earth on this round is zero. Nor do we know of any asteroid in the near future on a collision course with the planet. Enjoy the day.
Lockheed Martin and NASA engineers are installing the largest heat shield ever built onto the Orion EFT-1 spacecraft’s crew module at the Kennedy Space Center. Liftoff is slated for late Fall 2014. Credit: Lockheed Martin
Lockheed Martin and NASA engineers are installing the largest heat shield ever built onto the Orion EFT-1 spacecraft’s crew module at the Kennedy Space Center. Liftoff is slated for late Fall 2014. Credit: Lockheed Martin
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In a key milestone, technicians at the Kennedy Space Center (KSC) in Florida have attached the world’s largest heat shield to a pathfinding version of NASA’s Orion crew capsule edging ever closer to its inaugural unmanned test flight later this Fall on a crucial mission dubbed Exploration Flight Test-1 (EFT-1).
One of the primary goals of NASA’s eagerly anticipated Orion EFT-1 uncrewed test flight is to test the efficacy of the heat shield in protecting the vehicle – and future human astronauts – from excruciating temperatures reaching 4000 degrees Fahrenheit (2200 C) during scorching re-entry heating.
A trio of parachutes will then unfurl to slow Orion down for a splashdown in the Pacific Ocean.
Orion is NASA’s next generation human rated vehicle now under development to replace the now retired space shuttle. The state-of-the-art spacecraft will carry America’s astronauts on voyages venturing farther into deep space than ever before – past the Moon to Asteroids, Mars and Beyond!
“The Orion heat shield is the largest of its kind ever built. Its wider than the Apollo and Mars Science Lab heat shields,” Todd Sullivan told Universe Today. Sullivan is the heat shield senior manager at Lockheed Martin, Orion’s prime contractor.
The heat shield measures 16.5 feet (5 m) in diameter.
Lockheed Martin and NASA technicians mated the heat shield to the bottom of the capsule during assembly work inside the Operations and Checkout High Bay facility at KSC.
“Holes were drilled into the heat shield from the inside to the outside at the structural attached points at the underside of the crew module,” said Jules Schneider, Orion Project manager for Lockheed Martin at KSC, during a recent exclusive interview by Universe Today inside the Orion clean room at KSC.
“Then its opened up from the outside and bolted in place underneath. Closeout plugs made of Avcoat are then installed to close it up and seal the gaps,” Schneider explained.
The heat shield is constructed from a single seamless piece of Avcoat ablator, that was applied by engineers at Textron Defense System near Boston, Mass.
“They applied the Avcoat ablater material to the outside. That’s what protects the spacecraft from the heat of reentry,” Sullivan explained.
The ablative material will wear away as it heats up during the capsules atmospheric re-entry thereby preventing the 4000 degree F heat from being transferred to the rest of the capsule and saving it and the human crew from utter destruction.
Coming together! Orion’s heat shield and crew module in position for mating operations at NASA KSC. Credit: NASA
Orion EFT-1 is slated to launch in December 2014 atop the mammoth, triple barreled United Launch Alliance (ULA) Delta IV Heavy rocket, currently the most powerful booster in America’s fleet.
The Delta IV Heavy is the only rocket with sufficient thrust to launch the Orion EFT-1 capsule and its attached upper stage to its intended orbit of 3600 miles altitude above Earth – about 15 times higher than the International Space Station (ISS) and farther than any human spacecraft has journeyed in 40 years.
At the conclusion of the two-orbit, four- hour EFT-1 flight, the detached Orion capsule plunges back and re-enters the Earth’s atmosphere at 20,000 MPH (32,000 kilometers per hour).
“That’s about 80% of the reentry speed experienced by the Apollo capsule after returning from the Apollo moon landing missions,” Scott Wilson, NASA’s Orion Manager of Production Operations at KSC, told me during an interview at KSC.
“The big reason to get to those high speeds during EFT-1 is to be able to test out the thermal protection system, and the heat shield is the biggest part of that.”
“Numerous sensors and instrumentation have been specially installed on the EFT-1 heat shield and the back shell tiles to collect measurements of things like temperatures, pressures and stresses during the extreme conditions of atmospheric reentry,” Wilson explained.
Orion heat shield attached to the bottom of the capsule by engineers during assembly work inside the Operations and Checkout High Bay facility at KSC. Credit: NASA
The heat shield arrived at KSC in December 2013 loaded inside NASA’s Super Guppy aircraft while I was onsite. Read my story – here.
The data gathered during the unmanned EFT-1 flight will aid in confirming. or refuting, design decisions and computer models as the program moves forward to the first flight atop NASA’s mammoth SLS booster in late 2017 on the EM-1 mission and more human crewed missions thereafter.
Orion EFT-1 heat shield is off loaded from NASA’s Super Guppy aircraft after transport from Manchester, N.H., and arrival at the Kennedy Space Center in Florida on Dec. 5, 2013. Credit: Ken Kremer/kenkremer.com
Recently, the EFT-1 launch was postponed three months from its long planned slot in mid-September to December 2014 when NASA was ordered to make way for the accelerated launch of recently declassified US Air Force Space Surveillance satellites that were given a higher priority.
The covert Geosynchronous Space Situational Awareness Program, or GSSAP, satellites were only unveiled in Feb. 2014 during a speech by General William Shelton, commander of the US Air Force Space Command.
Despite the EFT-1 launch postponement, Kennedy Space Center Director Bob Cabana said technicians are pressing forward and continue to work around the clock at KSC in order to still be ready in time to launch by the original launch window that opens in mid- September 2014.
“The contractor teams are working to get the Orion spacecraft done on time for the December 2017 launch,” said Cabana.
“They are working seven days a week in the Operations and Checkout High Bay facility to get the vehicle ready to roll out for the EFT-1 mission and be mounted on top of the Delta IV Heavy.”
“I can assure you the Orion will be ready to go on time, as soon as we get our opportunity to launch that vehicle on its first flight test and that is pretty darn amazing.”
“Our plan is to have the Orion spacecraft ready because we want to get EFT-1 out so we can start getting the hardware in for Exploration Mission-1 (EM-1) and start processing for that vehicle that will launch on the Space Launch System (SLS) rocket in 2017,” Cabana told me
Concurrently, new American-made private crewed spaceships are under development by SpaceX, Boeing and Sierra Nevada – with funding from NASA’s Commercial Crew Program (CCP) – to restore US capability to ferry US astronauts to the International Space Station (ISS) and back to Earth by late 2017.
Read my exclusive new interview with NASA Administrator Charles Bolden explaining the importance of getting Commercial Crew online – here.
Two of the three United Launch Alliance (ULA) Delta IV heavy boosters for NASA’s upcoming Orion Exploration Flight Test-1 (EFT-1) mission were unveiled during a media event inside the Horizontal Integration Facility at Launch Complex 37 at Cape Canaveral Air Force Station in Florida. Kennedy Space Center Director Bob Cabana spoke to the media along with NASA Associate Administrator Robert Lightfoot and Tony Taliancich, ULA director of East Coast Launch Operations. Credit: Ken Kremer- kenkremer.com
Stay tuned here for Ken’s continuing Orion, Boeing, SpaceX, Orbital Sciences, commercial space, Curiosity, Mars rover, MAVEN, MOM and more planetary and human spaceflight news.
Ken Kremer Delta 4 Heavy rocket and super secret US spy satellite roar off Pad 37 on June 29, 2012 from Cape Canaveral, Florida. NASA’s Orion EFT-1 capsule will blastoff atop a similar Delta 4 Heavy Booster in December 2014. Credit: Ken Kremer- kenkremer.com[/caption]
Delta 4 Heavy rocket and super secret US spy satellite roar off Pad 37 on June 29, 2012 from Cape Canaveral, Florida. NASA’s Orion EFT-1 capsule will blastoff atop a similar Delta 4 Heavy Booster in December 2014. Credit: Ken Kremer- kenkremer.com[/caption]