NASA’s new countdown clock was powered up at the Press Site at the Kennedy Space Center in Florida for the first time on Dec. 1, 2014 for use with Orion’s first launch on Dec. 4, 2014. Note former shuttle launch pad 39A in the background above clock. Credit: Ken Kremer – kenkremer.com
KENNEDY SPACE CENTER – Just in the nick of time, NASA powered up its new countdown clock at the Press Site to tick down towards blastoff of the first launch of the agency’s new Orion crew capsule on Dec. 4 that will carry a new generation of explorers to exciting new destinations further into deep space than ever before.
Without any fanfare, NASA premiered the new digital clock today, Monday, Dec. 1, to replace the world famous analog clock – seen by countless billions across the globe – that was recently retired and detailed in my story – here.
Check out and compare the new and old countdown clocks in my exclusive photos herein.
“We were in a race against time to remove the old clock and replace it with the new clock over the Thanksgiving holiday period,” said NASA Kennedy Space Center spokesman George Diller in an exclusive interview with Universe Today on Monday.
“The plan was to have it ready in time for the first launch of Orion on Dec. 4,” Diller told me.
A new countdown display has been constructed in the place of the former analog countdown clock at the Press Site at NASA’s Kennedy Space Center in Florida for Orion’s first launch. The display is a modern, digital LED display akin to stadium monitors. It allows television images to be shown along with numbers. Credit: Ken Kremer – kenkremer.com
A team was working during the holiday.
Why replace the old clock?
“It was getting harder and harder to find the spare parts needed to fix the clock”.
“The original clock was designed in the 1960s”, Diller explained. It has been counting down launches, both manned and unmanned, for more than four decades.
“The clock has been in use since the Apollo 12 moon landing mission in November 1969.”
NASA’s 135th, and final, shuttle mission takes flight on July 8, 2011, at 11:29 a.m. from the Kennedy Space Center in Florida bound for the ISS and the high frontier with Chris Ferguson as Space Shuttle Commander. Credit: Ken Kremer/kenkremer.com
It was used continuously throughout the remaining Apollo launches and then for all 135 shuttle launches until the final shuttle mission STS-135 blastoff in July 2011. Since then it has been used exclusively on a plethora of unmanned NASA science launches and resupply missions to the International Space Station.
The old countdown clock was last used in September 2014 during the SpaceX CRS-4 launch to the ISS, which I attended along with the STS-135 launch.
The clock and adjacent US flag are officially called “The Press Site: Clock and Flag Pole” and were listed in the National Register of Historic Places on Jan. 21, 2000.
In the past few days workers dismantled and hauled off the old clock and installed the new one in place.
But the original base was left in place. The new clock is about the same length as the historic one, with a screen nearly 26 feet wide by 7 feet high.
While not true high-definition, the video resolution will be 1280 x 360.The new countdown clock sports a widescreen capability utilizing the latest breakthroughs in outdoor LED display technology, says NASA.
Space Shuttle Endeavour blasts off on her 25th, and final, mission from Pad 39 A on May 16, 2011, at 8:56 a.m. View from the world famous countdown clock at T-Plus 5 Seconds. Credit: Ken Kremer – kenkremer.com
The display can provide images from multiple sources, as well as the countdown launch time. It was cool to see the new clock in action today.
As currently envisaged, the historic Countdown Clock was moved to the nearby Kennedy Space Center Visitor Complex (KSCVC).
It will be placed on permanent display for the public to see for the first time at the KSCVC main entrance sometime early next year, Diller explained.
The new countdown clock in contact view with the VAB, Launch Control Center (LCC), US Flag, and SLS Mobile Launcher at the Press Site at the Kennedy Space Center in Florida will be used for the first time with Orion’s first launch on Dec. 4, 2014. Credit: Ken Kremer – kenkremer.com
NASA TV will provide several hours of live Orion EFT-1 launch coverage with the new countdown clock – starting at 4:30 a.m. on Dec. 4.
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.
Ken Kremer
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Learn more about Orion, SpaceX, Antares, NASA missions and more at Ken’s upcoming outreach events:
Dec 1-5: “Orion EFT-1, SpaceX CRS-5, Antares Orb-3 launch, Curiosity Explores Mars,” Kennedy Space Center Quality Inn, Titusville, FL, evenings
Orion atop Delta 4 Heavy Booster. Credit: NASA/Kim Shiflett
Video Caption: Animation details NASA’s Orion Exploration Flight Test-1 (EFT-1) mission launching on Dec. 4. 2014. Credit: NASA
It’s not Science Fiction! It’s Not Star Trek!
No. It’s a really, really big NASA Mission! It’s Orion!
In fact, it’s the biggest and most important development in US Human Spaceflight since the end of the Space Shuttle Program in 2011.
Orion is launching soon on its first flight, the pathfinding Exploration Flight Test-1 (EFT-1) mission and sets NASA on the path to send humans to Mars in the 2030s.
Watch this cool NASA animation beautifully detailing every key step of Orion’s First Launch!
Orion is designed to take humans farther than they’ve ever gone before. Even farther into deep space than NASA’s Apollo moon landing which ended more than four decades ago!
We are T-MINUS 4 Days and Counting to the inaugural blastoff of Orion as of today, Sunday, November 30, 2014.
To learn even more about the 8 major events and goals happening during Orion’s EFT-1 mission be sure to check out my recent story with NASA’s fabulous new set of infographics – here.
Every aspect of the final processing steps now in progress by engineers and technicians from NASA, rocket provider United Launch Alliance, and Orion prime contractor Lockheed Martin is proceeding smoothly and marching towards launch.
Orion’s move to Launch Complex-37. Credit: Mike Killian
Orion will lift off on a United Launch Alliance 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 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.
NASA TV will provide several hours of live coverage
Here’s how Orion EFT-1 Launch will look!
Delta 4 Heavy rocket and super secret US spy satellite roars 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
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.
Launch – It’s going to be loud. It’s going to be bright. It’s going to be smoky. Engines are fired, the countdown ends and Orion lifts off into space atop the United Launch Alliance Delta IV Heavy rocket from the launch pad at Cape Canaveral in Florida. Credit: NASA
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Learn more about Orion, SpaceX, Antares, NASA missions and more at Ken’s upcoming outreach events:
Dec 1-5: “Orion EFT-1, SpaceX CRS-5, Antares Orb-3 launch, Curiosity Explores Mars,” Kennedy Space Center Quality Inn, Titusville, FL, evenings
Dive teams attach tow lines to Orion test capsule during Aug. 15, 2013 recovery test at Norfolk Naval Base, VA. Credit: Ken Kremer/kenkremer.com
This artist's conception illustrates a supermassive black hole (central black dot) at the core of a young, star-rich galaxy. Now astronomers have found a rogue SMBH travelling through space. Image credit: NASA/JPL-Caltech
Scientists have long suspected that supermassive black holes (SMBH) reside at the center of every large galaxy in our universe. These can be billions of times more massive than our sun, and are so powerful that activity at their boundaries can ripple throughout their host galaxies.
In the case of the Milky Way galaxy, this SMBH is believed to correspond with the location of a complex radio source known as Sagittarius A*. Like all black holes, no one has even been able to confirm that they exist, simply because no one has ever been able to observe one.
But thanks to researchers working out of MIT’s Haystack Observatory, that may be about to change. Using a new telescope array known as the “Event Horizon Telescope” (EHT), the MIT team hopes to produce this “image of the century” very soon.Initially predicted by Einstein, scientists have been forced to study black holes by observing their apparent effect on space and matter in their vicinity. These include stellar bodies that have periodically disappeared into dark regions, never to be heard from again.
As Sheperd Doeleman, assistant director of the Haystack Observatory at Massachusetts Institute of Technology (MIT), said of black holes: “It’s an exit door from our universe. You walk through that door, you’re not coming back.”
Image of the M87, a giant elliptical galaxy that is believed to have a SMBH at its center. Credit: NASA/CXC/KIPAC/NSF/NRAO/AUI
As the most extreme object predict by Einstein’s theory of gravity, supermassive black holes are the places in space where, according to Doeleman, “gravity completely goes haywire and crushes an enormous mass into an incredibly close space.”
To create the EHT array, the scientists linked together radio dishes in Hawaii, Arizona, and California. The combined power of the EHT means that it can see details 2,000 times finer than what’s visible to the Hubble Space Telescope.
These radio dishes were then trained on M87, a galaxy some 50 million light years from the Milky Way in the Virgo Cluster, and Sagittarius A* to study the event horizons at their cores.
Other instruments have been able to observe and measure the effects of a black hole on stars, planets, and light. But so far, no one has ever actually seen the Milky Way’s Supermassive black hole.
According to David Rabanus, instruments manager for ALMA: “There is no telescope available which can resolve such a small radius,” he said. “It’s a very high-mass black hole, but that mass is concentrated in a very, very small region.”
Doeleman’s research focuses on studying super massive black holes with sufficient resolution to directly observe the event horizon. To do this his group assembles global networks of telescopes that observe at mm wavelengths to create an Earth-size virtual telescope using the technique of Very Long Baseline Interferometry (VLBI).
Image of Sagittarius A*, the complex radio source at the center of the Milky Way, and believed to be a SMBH. Credit: NASA/Chandra
“We target SgrA*, the 4 million solar mass black hole at the center of the Milky Way, and M87, a giant elliptical galaxy,” says Doeleman. “Both of these objects present to us the largest apparent event horizons in the Universe, and both can be resolved by (sub)mm VLBI arrays.” he added. “We call this project The Event Horizon Telescope (EHT).”
Ultimately, the EHT project is a world-wide collaboration that combines the resolving power of numerous antennas from a global network of radio telescopes to capture the first image ever of the most exotic object in our Universe – the event horizon of a black hole.
“In essence, we are making a virtual telescope with a mirror that is as big as the Earth,” said Doeleman who is the principal investigator of the Event Horizon Telescope. “Each radio telescope we use can be thought of as a small silvered portion of a large mirror. With enough such silvered spots, one can start to make an image.”
“The Event Horizon Telescope is the first to resolve spatial scales comparable to the size of the event horizon of a black hole,” said University of California, Berkeley astronomer Jason Dexter. “I don’t think it’s crazy to think we might get an image in the next five years.”
First postulated by Albert Einstein’s Theory of General Relativity, the existence of black holes has since been supported by decades’ worth of observations, measurements, and experiments. But never has it been possible to directly observe and image one of these maelstroms, whose sheer gravitational power twists and mangle the very fabric of space and time.
Finally being able to observe one will not only be a major scientific breakthrough, but could very well provide the most impressive imagery ever captured.
Image of the spiral galaxy NGC 4151, aka. "Sauron's Eye". Credit: X-ray: NASA/CXC/CfA/J.Wang et al.; Optical: Isaac Newton Group of Telescopes, La Palma/Jacobus Kapteyn Telescope; Radio: NSF/NRAO/VLA.
Determining the distance of galaxies from our Solar System is a tricky business. Knowing just how far other galaxies are in relation to our own is not only key to understanding the size of the universe, but its age as well. In the past, this process relied on finding stars in other galaxies whose absolute light output was measurable. By gauging the brightness of these stars, scientists have been able to survey certain galaxies that lie 300 million light years from us.
However, a new and more accurate method has been developed, thanks to a team of scientists led by Dr. Sebastian Hoenig from the University of Southampton. Similar to what land surveyors use here on Earth, they measured the physical and angular (or apparent) size of a standard ruler in the galaxy to calibrate distance measurements.
Orion atop Delta 4 Heavy Booster. Credit: NASA/Kim Shiflett
At T MINUS 1 Week on this Thanksgiving Holiday, all launch processing events remain on track for the first blast off of NASA’s new Orion crew vehicle on Dec. 4, 2014 which marks the first step on the long road towards sending Humans to Mars in the 2030s.
Orion will lift off on a United Launch Alliance 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.
Technicians and engineers installed Orion’s batteries and have been conducting a thorough checkout of all the electrical and battery connections between the crew module, service module and Delta IV Heavy second stage while working inside the mobile service tower at pad 37.
With access doors at Space Launch Complex 37 opened, the Orion and Delta IV Heavy stack is visible in its entirety inside the Mobile Service Tower where the vehicle is undergoing launch preparations. Credit: NASA/Kim Shiflett
There is some margin time available in the schedule in case additional testing and checkouts are required.
Orion’s launch window opens at 7:05 a.m. EST on Dec. 4 at the beginning of a launch window that extends 2 hours, 39 minutes.
One week ago, top NASA and Lockheed Martin managers gave the “GO” to continue with launch preparations after the vehicle passed the Flight Readiness Review (FRR) on Thursday, Nov. 20.
This past week the doors of the Mobile Servicing Tower (MST) at pad 37 were opened to reveal the Orion spacecraft stack atop the Delta IV Heavy that will carry the spacecraft into orbit.
NASA’s Orion EFT-1 spacecraft atop Delta 4 Heavy Booster at Cape Canaveral, Florida ahead of launch set for Dec. 4, 2014. Credit: NASA/Kim Shiflett
The Delta IV Heavy is the world’s most powerful rocket.
The MST will be rolled back from the rocket stack on Wednesday evening, Dec. 3 starting 8 hours, 15 minutes before launch to allow the rocket to be fueled and continue into the final stage of launch operations and the countdown to liftoff on Thursday morning Dec. 4.
I’ll be at the pad during MST rollback reporting live for Universe Today.
Orion’s move to Launch Complex-37. Credit: Mike Killian
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.
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.
NASA’s Orion EFT 1 crew module enters the Payload Hazardous Servicing Facility on Sept. 11, 2014 at the Kennedy Space Center, FL, beginning the long journey to the launch pad and planned liftoff on Dec. 4, 2014. Credit: Ken Kremer – kenkremer.com
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.
Learn more about Orion, SpaceX, Antares, NASA missions and more at Ken’s upcoming outreach events:
Dec 1-5: “Orion EFT-1, SpaceX CRS-5, Antares Orb-3 launch, Curiosity Explores Mars,” Kennedy Space Center Quality Inn, Titusville, FL, evenings
These three RS-68 engines will power each of the attached Delta IV Heavy Common Booster Cores (CBCs) that will launch NASA’s maiden Orion on the EFT-1 mission in December 2014. Credit: Ken Kremer/kenkremer.com Orion flight test profile for the Exploration Flight Test-1 (EFT-1) launching on Dec. 4, 2014. Credit: NASA
Visualization of the radiation belts with confined charged particles (blue & yellow) and plasmapause boundary (blue-green surface). Image Credit:
NASA/Goddard
It’s a well-known fact that Earth’s ozone layer protects us from a great deal of the Sun’s ultra-violet radiation. Were it not for this protective barrier around our planet, chances are our surface would be similar to the rugged and lifeless landscape we observe on Mars.
Beyond this barrier lies another – a series of shields formed by a layer of energetic charged particles that are held in place by the Earth’s magnetic field. Known as the Van Allen radiation belts, this wall prevents the fastest, most energetic electrons from reaching Earth.
And according to new research from NASA’s Van Allen probes, it now appears that these belts may be nearly impenetrable, a finding which could have serious implications for future space exploration and research.
The existence of a belt of charged particles trapped by the Earth’s magnetosphere has been the subject of research since the early 20th century. However, it was not until 1958 that the Explorer 1 and Explorer 3 spacecrafts confirmed the existence of the belt, which would then be mapped out by the Explorer 4, Pioneer 3, and Luna 1 missions.
Two giant belts of radiation surround Earth. The inner belt is dominated by protons and the outer one by electrons. Credit: NASA
Since that time, scientists have discovered much about this belt, including how it interacts with other fields around our planet to form a nearly-impenetrable barrier to incoming electrons.
This discovery was made using NASA’s Van Allen Probes, launched in August 2012 to study the region. According to the observations made by the probes, this region can wax and wane in response to incoming energy from the sun, sometimes swelling up enough to expose satellites in low-Earth orbit to damaging radiation.
“This barrier for the ultra-fast electrons is a remarkable feature of the belts,” said Dan Baker, a space scientist at the University of Colorado in Boulder and first author of the paper. “We’re able to study it for the first time, because we never had such accurate measurements of these high-energy electrons before.”
Understanding what gives the radiation belts their shape and what can affect the way they swell or shrink helps scientists predict the onset of those changes. Such predictions can help scientists protect satellites in the area from the radiation.
In the decades since they were first discovered, scientists have learned that the size of the two belts can change – or merge, or even separate into three belts occasionally. But generally the inner belt stretches from 644 km to 10,000 km (400 – 6,000 mi) above the Earth’s surface while the outer belt stretches from 13,500 t0 58,000 km (8,400 – 36,000 mi).
Artist’s rendition of Van Allen Probes A and B in Earth orbit. Credit: NASA
Up until now, scientists have wondered why these two these belts have existed separately. Why, they have wondered, is there a fairly empty space between the two that appears to be free of electrons? That is where the newly discovered barrier comes in.
The Van Allen Probes data showed that the inner edge of the outer belt is, in fact, highly pronounced. For the fastest, highest-energy electrons, this edge is a sharp boundary that, under normal circumstances, cannot be penetrated.
“When you look at really energetic electrons, they can only come to within a certain distance from Earth,” said Shri Kanekal, the deputy mission scientist for the Van Allen Probes at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, and a co-author on the Nature paper. “This is completely new. We certainly didn’t expect that.”
The team looked at possible causes. They determined that human-generated transmissions were not the cause of the barrier. They also looked at physical causes, asking if the shape of the Earth’s magnetic field could be the cause of the boundary. However, NASA scientists studied and eliminated that possibility and determined that the presence of other space particles appears to be the more likely cause.
A cloud of cold, charged gas around Earth called the plasmasphere (seen here in purple), interacts with the particles in Earth’s radiation belts (shown in grey). Image Credit: NASA/Goddard
The radiation belts are not the only particle structures surrounding Earth. A giant cloud of relatively cool, charged particles called the plasmasphere fills the outermost region of Earth’s atmosphere, beginning at about 600 miles up and extending partially into the outer Van Allen belt. The particles at the outer boundary of the plasmasphere cause particles in the outer radiation belt to scatter, removing them from the belt.
This scattering effect is fairly weak and might not be enough to keep the electrons at the boundary in place, except for a quirk of geometry – the radiation belt electrons move incredibly quickly, but not toward Earth. Instead, they move in giant loops around Earth.
The Van Allen Probes’ data show that in the direction toward Earth, the most energetic electrons have very little motion at all – just a gentle, slow drift that occurs over the course of months. This movement is so slow and weak that it can be rebuffed by the scattering caused by the plasmasphere.
This also helps explain why – under extreme conditions, when an especially strong solar wind or a giant solar eruption such as a coronal mass ejection sends clouds of material into near-Earth space – the electrons from the outer belt can be pushed into the usually-empty slot region between the belts.
“The scattering due to the plasmapause is strong enough to create a wall at the inner edge of the outer Van Allen Belt,” said Baker. “But a strong solar wind event causes the plasmasphere boundary to move inward.”
A massive inflow of matter from the sun can erode the outer plasmasphere, moving its boundaries inward and allowing electrons from the radiation belts the room to move further inward too.
The Johns Hopkins Applied Physics Laboratory in Laurel, Maryland, built and operates the Van Allen Probes for NASA’s Science Mission Directorate. The mission is the second in NASA’s Living With a Star program, managed by Goddard.
A paper on these results appeared in the Nov. 26, 2014, issue of Nature magazine. And be sure to watch this animated video produced by the Goddard Space Center that explains the Van Allen belt in brief:
Antares destruction after the first stage propulsion system at the base of Orbital Sciences’ rocket exploded moments after blastoff from NASA’s Wallops Flight Facility, VA, on Oct. 28, 2014. Credit: Ken Kremer – kenkremer.com
Video Caption: This up close launch pad camera view is a time lapse sequence of images showing the sudden catastrophic explosion of Orbital Sciences Antares Orb 3 rocket seconds after blastoff and destructive incineration as it plummets into a hellish inferno at NASA’s Wallops Flight Facility, VA, on Oct. 28, 2014, at 6:22 p.m. Credit: Ken Kremer – kenkremer.com/Universe Today/AmericaSpace/Zero-G News.
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NASA WALLOPS FLIGHT FACILITY, VA – Moments after a seemingly glorious liftoff on Oct. 28, 2014, the Orbital Sciences Corp. commercial Antares rocket suffered a catastrophic failure as one of the Soviet-era first stage engines exploded and cascaded into a spectacular aerial fireball just above the launch pad at NASA’s Wallops Flight Facility on the doomed Orb-3 mission to the International Space Station (ISS).
Although I witnessed and photographed the launch failure from the media viewing area on site at NASA Wallops from a distance of about 1.8 miles away, myself and a small group of space journalists working together from Universe Today, AmericaSpace, and Zero-G News had also placed sound activated cameras directly at the launch pad to capture the most spectacular up close views for what we all expected to be a “nominal” launch. Our imagery had been impounded by accident investigators – until being released to us now.
Now in part 2 of this exclusive series of video and photos our team can show you the terrible fate suffered by Antares after its destructive descent and frightening incineration as it was consumed by a hellish inferno.
My time lapse video above clearly shows the explosion and incendiary descent of Antares into a mammoth fireball.
As I reported in Part 1, all of our team’s cameras and image cards were impounded for nearly a month by Orbital’s official and independent Accident Investigation Board (AIB) that was assembled quickly in the aftermath of the Antares launch failure disaster and charged with determining the root cause of the launch failure.
The videos and 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 few days.
One image clearly shows that the south side engine nozzle of the AJ26 first stage engine was intact and had shut down after the initial explosion and during the plummet. Therefore it was the north side engine that blew up and led to the launch failure. See my up close AJ26 engine photo below.
Video Caption: AmericaSpace and Zero-G News video compilation of four cameras surrounding the launch pad to capture liftoff. The video runs through each at full speed before slowing down to give viewers a slow motion replay of the explosion. One of the cameras was right in the middle of the fireball, with chunks of broken rocket showering down around. CREDITS: Mike Barrett / Jeff Seibert / Matthew Travis / Elliot Severn / Peter Greenwood for www.ZeroGNews.com and www.AmericaSpace.com
Similar launch pad photos taken by NASA and Orbital Sciences cameras have not been publicly released and may not be released for some time to come.
The videos and images collected here are the work of my colleagues Matthew Travis, Elliot Severn, Alex Polimeni, Charles Twine, Jeff Seibert, Mike Barrett, and myself, and show exquisite, heretofore unreleased, views of the explosion, fireball, and wreckage from various positions all around the launch pad.
Our remote cameras were placed all around the Antares pad OA at the Mid-Atlantic Regional Spaceport (MARS) on Wallops Island, VA, and somehow miraculously survived the rocket’s destruction as it plunged to the ground very near and just north of the seaside launch pad.
A turbopump failure in one of the rocket’s Soviet-era first stage engines has been identified as the most likely cause of the Antares’ destruction 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.
Antares loses thrust after rocket explosion and begins falling back after blastoff from NASA’s Wallops Flight Facility, VA, on Oct. 28, 2014, at 6:22 p.m. Credit: Ken Kremer – kenkremer.comClose up view of Antares’ descent into a hellish inferno shows the south side first stage engine intact after the north side engine at the base of Orbital Sciences’ Antares rocket exploded moments after blastoff from NASA’s Wallops Flight Facility, VA, on Oct. 28, 2014. Credit: Ken Kremer – kenkremer.com
Overall this was the 5th Antares launch using the AJ26 engines.
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).
Antares doomed descent to incendiary destruction after first stage propulsion system of Orbital Sciences’ rocket exploded moments after blastoff from NASA’s Wallops Flight Facility, VA, on Oct. 28, 2014. Credit: Ken Kremer – kenkremer.com
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.
Examine the video and photo gallery herein.
Orbital Sciences Antares rocket explodes into a fireball seconds after blastoff from NASA’s Wallops Flight Facility, VA, on Oct. 28, 2014, at 6:22 p.m. Credit: Ken Kremer – kenkremer.com
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.
Pre-launch seaside panorama of Orbital Sciences Corporation Antares rocket at the NASA’s Wallops Flight Facility launch pad on Oct 26 – 2 days before the Orb-3 launch failure on Oct 28, 2014. Credit: Ken Kremer – kenkremer.comSoviet era NK-33 engines refurbished as the AJ26 exactly like pictured here probably caused Antares’ rocket failure on Oct. 28, 2014. Orbital Sciences technicians at work on two AJ26 first stage engines at the base of an Antares rocket during exclusive visit by Ken Kremer/Universe Today at NASA Wallaps. These engines powered the successful Antares liftoff on Jan. 9, 2014 at NASA Wallops, Virginia bound for the ISS. Credit: Ken Kremer – kenkremer.comRemote cameras set up around launch pad 0A at the Mid-Atlantic Regional Spaceport at NASA’s Wallops Flight Facility in Virginia captured incredible up-close views of an Orbital Sciences Corporation Antares rocket exploding seconds after liftoff several weeks ago. The mission was to deliver the company’s Orb-3 Cygnus spacecraft to deliver supplies and experiments to the orbiting International Space Station. Photo Credits: Elliot Severn / Matthew Travis / Mike Barrett / Jeff Seibert for Zero-G News and AmericaSpaceUp Close Launch Pad remote camera photographers during prelaunch setup for Orb-3 mission at NASA Wallops launch pad. Credit: Ken Kremer – kenkremer.com
Antares descended into hellish inferno after first stage propulsion system at 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. Credit: Ken Kremer – kenkremer.com
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.
Antares descended to doom 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. Credit: Ken Kremer – kenkremer.com
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.
Close up view of Antares’ destruction shows the south side first stage engine intact after the north side engine at the base of Orbital Sciences’ rocket exploded moments after blastoff from NASA’s Wallops Flight Facility, VA, on Oct. 28, 2014. Credit: Ken Kremer – kenkremer.comAntares 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. Credit: Ken Kremer – kenkremer.com
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.
Antares destruction after the first stage propulsion system at the base of Orbital Sciences’ rocket exploded moments after blastoff from NASA’s Wallops Flight Facility, VA, on Oct. 28, 2014. Credit: Ken Kremer – kenkremer.com
Close up view of Antares’ destructive fall shows the south side first stage engine intact after the north side engine at the base of Orbital Sciences’ rocket exploded moments after blastoff from NASA’s Wallops Flight Facility, VA, on Oct. 28, 2014. Credit: Ken Kremer – kenkremer.com
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.
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. Credit: Ken Kremer – kenkremer.comAntares rocket stand erect, reflecting off the calm waters the night before the planned first night launch from NASA’s Wallops Flight Facility, VA, that ended in tragic failure on Oct. 28. Credit: Ken Kremer – kenkremer.com
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.
Orbital Sciences Antares rocket explodes into an aerial fireball seconds after blastoff from NASA’s Wallops Flight Facility, VA, on Oct. 28, 2014 at 6:22 p.m. Credit: Ken Kremer – kenkremer.comSoviet era NK-33 engines refurbished as the AJ26 exactly like pictured here probably caused Antares’ rocket failure on Oct. 28, 2014. Orbital Sciences technicians at work on two AJ26 first stage engines at the base of an Antares rocket during exclusive visit by Ken Kremer/Universe Today at NASA Wallops. These engines powered the successful Antares liftoff on Jan. 9, 2014, at NASA Wallops, Virginia, bound for the ISS. Credit: Ken Kremer – kenkremer.comUp Close Launch Pad remote camera photographers during prelaunch setup for Orb-3 mission at NASA Wallops launch pad. Credit: Ken Kremer – kenkremer.com
At NASA's Kennedy Space Center in Florida, the agency's Orion spacecraft pauses in front of the spaceport's iconic Vehicle Assembly Building as it is transported to Launch Complex 37 at Cape Canaveral Air Force Station. After arrival at the launch pad, United Launch Alliance engineers and technicians will lift Orion and mount it atop its Delta IV Heavy rocket.
Credit: NASA/Frankie Martin
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 in orbit in this artists concept. Credit: NASA
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 United Launch Alliance Delta-IV Heavy rocket tasked with launching NASA’s Orion EFT-1 mission being hoisted vertical atop Space Launch Complex-37B at Cape Canaveral Air Force Station in Florida on the morning of Oct. 1, 2014. Photo Credit: Alan Walters / AmericaSpace
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.
NASA’s completed Orion EFT 1 crew module loaded on wheeled transporter during move to the Payload Hazardous Servicing Facility (PHFS) on Sept. 11, 2014, at the Kennedy Space Center, FL. Credit: Ken Kremer – kenkremer.com
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.
Orion flight test profile for the Exploration Flight Test-1 (EFT-1) launching on Dec. 4, 2014. Credit: NASASide view shows trio of Common Booster Cores (CBCs) with RS-68 engines powering the Delta IV Heavy rocket resting horizontally in ULA’s HIF processing facility at Cape Canaveral that will launch NASA’s maiden Orion on the EFT-1 mission in December 2014 from Launch Complex 37. Credit: Ken Kremer/kenkremer.com
Europa. CThe cracked, icy surface of Europa. The smoothness of the surface has led many scientists to conclude that oceans exist beneath it. Credit: NASA/JPLredit: NASA
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.
This newly-reprocessed color view of Europa was made from images taken by NASA’s Galileo spacecraft in the late 1990s. Image credit: NASA/JPL-Caltech/SETI Institute
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.
Artist’s concept of the Galileo space probe passing through the Jupiter system. Credit: NASA
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:
