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The world’s most powerful rocket – our Space Launch System (SLS) – may experience ground wind gusts of up to 70 mph as it sits on the launch pad before and during lift off for future missions. Understanding how environmental factors affect the rocket will help us maintain a safe and reliable distance away from the launch tower during launch.
How do we even test this? Great question! Our Langley Research Center’s 14x22-Foot Subsonic Wind Tunnel in Hampton, Virginia, is designed to simulate wind conditions. Rather than having to test a full scale rocket, we’re able to use a smaller, to-scale model of the spacecraft.
Wind tunnel tests are a cost effective and efficient way to simulate situations where cross winds and ground winds affect different parts of the rocket. The guidance, navigation, and control team uses the test data as part of their simulations to identify the safety distance between the rocket and the launch tower.
SLS is designed to evolve as we move crew and cargo farther into the solar system than we have ever been before. The Langley team tested the second more powerful version of the SLS rocket, known as the Block 1B, in both the crew and cargo configuration.
Below, an engineer simulates ground winds on the rocket during liftoff by using what’s called smoke flow visualization. This technique allows engineers to see how the wind flow behaves as it hits the surface of the launch tower model.
The 6-foot model of the SLS rocket undergoes 140 mph wind speeds in Langley’s 14x22-Foot Subsonic Wind Tunnel. Engineers are simulating ground winds impacting the rocket as it leaves the launch pad.
The cargo version of the rocket is positioned at a 0-degree angle to simulate the transition from liftoff to ascent as the rocket begins accelerating through the atmosphere.
Here, engineers create a scenario where the rocket has lifted off 100 feet in the air past the top of the launch tower. At this point in the mission, SLS is moving at speeds of about 100 mph!
Engineers at Langley collect data throughout the test which is used by the rocket developers at our Marshall Space Flight Center in Huntsville, Alabama, to analyze and incorporate into the rocket’s design.
Learn more about our Space Launch System rocket HERE.
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In schools across the country, many students just finished final exams. Now, part of the world’s most powerful rocket, the Space Launch System (SLS), is about to feel the pressure of testing time. The first SLS engine section has been moving slowly upriver from Michoud Assembly Facility near New Orleans, but once the barge Pegasus docks at our Marshall Space Flight Center in Huntsville, Alabama, the real strength test for the engine section will get started.
The engine section is the first of four of the major parts of the core stage that are being tested to make sure SLS is ready for the challenges of spaceflight.
The engine section is located at the bottom of the rocket. It has a couple of important jobs. It holds the four RS-25 liquid propellant engines, and it serves as one of two attach points for each of the twin solid propellant boosters. This first engine section will be used only for ground testing.
Of all the major parts of the rocket, the engine section gets perhaps the roughest workout during launch. Millions of pounds of core stage are pushing down, while the engines are pushing up with millions of pounds of thrust, and the boosters are tugging at it from both sides. That’s a lot of stress. Maybe that’s why there’s a saying in the rocket business: “Test like you fly, and fly like you test.”
After it was welded at Michoud, technicians installed the thrust structure, engine supports and other internal equipment and loaded it aboard the Pegasus for shipment to Marshall.
Once used to transport space shuttle external tanks, Pegasus was modified for the longer SLS core stage by removing 115 feet out of the middle of the barge and added a new 165-foot section with a reinforced main deck. Now as long as a football field, Pegasus – with the help of two tugboats – will transport core stage test articles to Marshall Space Flight Center as well as completed core stages to Stennis Space Center in Mississippi for test firing and then to Kennedy Space Center for launch.
The test article has no engines, cabling, or computers, but it will replicate all the structures that will undergo the extreme physical forces of launch. The test article is more than 30 feet tall, and weighs about 70,000 pounds. About 3,200 sensors attached to the test article will measure the stress during 59 separate tests. Flight-like physical forces will be applied through simulators and adaptors standing in for the liquid hydrogen tank and RS-25 engines.
The test fixture that will surround and secure the engine section weighs about 1.5 million pounds and is taller than a 5-story building. Fifty-five big pistons called “load lines” will impart more than 4.5 million pounds of force vertically and more than 428,000 pounds from the side.
The engineers and their computer design tools say the engine section can handle the stress. It’s the test team’s job prove that it can.
For more information about the powerful SLS rocket, check out: http://nasa.gov/SLS.
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The United Launch Alliance’s Atlas V rocket carrying the Orbital ATK Cygnus module rolls to Cape Canaveral Air Force Station's Launch Pad 41 in this time-lapse video. The rollout is in preparation for the Orbital ATK CRS-7 mission to deliver supplies to the International Space Station.
Launch is currently scheduled for 11:11 a.m. EDT, watch live coverage: http://www.nasa.gov/live
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We recently completed a structural integrity evaluation on the test version of the Orion service module at our Plum Brook Station in Sandusky, Ohio. Designed to ensure the module can withstand launch atop the Space Launch System (SLS) rocket, the battery of tests was conducted in stages over a 16-month period.
The 13-ton European service module will power, propel and cool Orion, while supplying vital oxygen and water to its crew during future missions.
The Powerhouse: Space Launch System and Orion
Our Space Launch System is an advanced launch vehicle that will usher in a new era of human exploration beyond Earth’s orbit. SLS, with its unparalleled power and capabilities, will launch missions to explore deep-space destinations aboard our Orion spacecraft.
What is Orion? Named after one of the largest constellations in the night sky and drawing from more than 50 years of spaceflight research and development, the Orion spacecraft will be the safest, most advanced spacecraft ever built. It will be flexible and capable enough to take astronauts to a variety of deep destinations, including Mars.
Welcome to the Buckeye State
In November 2015, the full-sized test version of the Orion service module arrived at Cleveland Hopkins Airport aboard an Antonov AN-124. After being unloaded from one of the world’s largest transport aircraft, the module was shipped more than 50 miles by truck to Plum Brook for testing.
Spread Your Wings
The first step of the service module’s ground test journey at Plum Brook’s Space Power Facility, saw one of its 24-foot solar array wings deployed to verify operation of the power system. The test confirmed the array extended and locked into place, and all of the wing mechanisms functioned properly.
Can You Hear SLS Now?
The SLS will produce a tremendous amount of noise as it launches and climbs through our atmosphere. In fact, we’re projecting the rocket could produce up to 180 decibels, which is louder than 20 jet engines operating at the same time.
While at the Reverberant Acoustic Test Facility, the service module was hit with more than 150 decibels and 20-10,000 hertz of sound pressure. Microphones were placed inside the test environment to confirm it matched the expected acoustic environment during launch.
After being blasted by sound, it was time to rock the service module, literally.
Shake Without the Bake
Launching atop the most powerful rocket ever built – we’re talking more than eight million pounds of thrust – will subject Orion to stresses never before experienced in spaceflight.
To ensure the launch doesn’t damage any vital equipment, the engineering team utilized the world’s most powerful vibration table to perform nearly 100 different tests, ranging from 2.5 Hz to 100 Hz, on the module in the summer of 2016.
Gotta Keep ‘Em Separated
The team then moved the Orion test article from the vibration table into the high bay for pyroshock tests, which simulated the shock the service module will experience as it separates from the SLS during launch.
Following the sound, vibration and separation tests, a second solar array wing deployment was conducted to ensure the wing continued to properly unfurl and function.
Headed South for the Summer
The ground test phase was another crucial step toward the eventual launch of Exploration Mission-1, as it validated extensive design prep and computer modeling, and verified the spacecraft met our safety and flight requirements.
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Soaring through the skies! This view looks from the window of our F-18 support aircraft during a 2016 Orbital ATK air-launch of its Pegasus rocket.
The CYGNSS mission, led by the University of Michigan, will use eight micro-satellite observatories to measure wind speeds over Earth’s oceans, increasing the ability of scientists to understand and predict hurricanes.
CYGNSS launched at 8:37 a.m. EST on Thursday, Dec. 15, 2016 from our Kennedy Space Center in Florida. CYGNSS launched aboard an Orbital ATK Pegasus XL rocket, deployed from Orbital’s “Stargazer” L-1011 carrier aircraft.
Pegasus is a winged, three-stage solid propellant rocket that can launch a satellite into low Earth orbit. How does it work? Great question!
After takeoff, the aircraft (which looks like a commercial airplane..but with some special quirks) flies to about 39,000 feet over the ocean and releases the rocket.
Make sure to follow us on Tumblr for your regular dose of space: http://nasa.tumblr.com
The Geostationary Operational Environmental Satellite-R Series (GOES-R) is the nation’s next generation of geostationary weather satellites. It is the first of four satellites to be launched for the National Oceanic and Atmospheric Administration (NOAA).
The GOES-R satellite will provide advanced imaging with increased spatial resolution and faster coverage for more accurate forecasts, real-time mapping of lightning activity and improved monitoring of solar activity. For the first time, GOES-R will be able to monitor the Earth in near real-time.
Once in geostationary orbit (the orbit around the Earth’s equator), it will provide images of weather patterns and severe storms across the continental U.S. as regularly as every five minutes. Images of smaller, more detailed areas, where storm activity is present, will be taken as frequently as every 30 seconds.
These images can be used to aid in formulating regular forecasts, term forecasting, such as seasonal predictions and drought outlooks.
In addition, the satellite will constantly monitor space weather conditions, such as solar flares, to provide advance notice of potential communication and navigation disruptions.
The satellite will also assist researchers in understanding the interactions between land, oceans, the atmosphere and climate.
Improve hurricane tracking and intensity forecasts
Increase thunderstorm and tornado warning lead time
Give earlier warning of ground lightning strike hazards
Improve detection of heavy rainfall and flash flooding risks
Improve air quality warnings and alerts
Give better fire detection and intensity estimation
Improve solar flare warnings for communications and navigation disruptions
Give more accurate monitoring of energetic particles responsible for radiation hazards to humans and spacecraft
Improve monitoring of space weather to get better geomagnetic storm forecasting.
The better we can predict what’s coming, the better we can prepare.
The GOES-R satellite is targeted for a launch on Saturday, Nov. 19, aboard a United Launch Alliance Atlas V rocket.
The one-hour launch window opens at 5:42 p.m. EST. Liftoff will occur from our Kennedy Space Center in Florida.
Join us leading up to launch by tuning in during the following times:
Thursday, Nov. 17 Prelaunch News Conference - 1 p.m. EST Watch HERE
GOES-R Mission Briefing - 2 p.m. EST Watch HERE
Friday, Nov. 18 GOES-R Social Presentations – 1:30 p.m. EST Watch HERE
Saturday, Nov. 19 NASA Edge Prelaunch Program – 3:45 p.m. EST Watch HERE
Launch Coverage & Commentary – 4:45 p.m. EST Watch HERE
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On Monday, Oct. 17, Orbital ATK is scheduled to send new science experiments to the International Space Station.
The Cygnus spacecraft will blast off from our Wallops Flight Facility in Virginia at 7:40 p.m. EDT carrying more than 5,100 pounds of science, supplies and equipment.
Let’s take a look at a few of these experiments:
Low-temperature fires with no visible flames are known as cool flames. The Cool flames experiment examines these low-temperature combustion of droplets of a variety of fuels and additives in low gravity.
Why are we studying this? Data from this experiment could help scientists develop more efficient advanced engines and new fuels for use in space and on Earth.
Light plays a powerful role in our daily, or circadian, rhythms. Astronauts aboard the space station experience multiple cycles of light and dark every 24 hours, which, along with night shifts and the stresses of spaceflight, can affect their sleep quantity and quality.
The Lighting Effects investigation tests a new lighting system aboard the station designed to enhance crew health and keep their body clocks in proper sync with a more regular working and resting schedule.
Why are we studying this? Lighting manipulation has potential as a safe, non-pharmacological way to optimize sleep and circadian regulation on space missions. People on Earth, especially those who work night shifts, could also improve alertness and sleep by adjusting lighting for intensity and wavelength.
A user-friendly tablet app provides astronauts with a new and faster way to collect a wide variety of personal data. The EveryWear experiment tests use of this French-designed technology to record and transmit data on nutrition, sleep, exercise and medications. Astronauts use the app to complete questionnaires and keep medical and clinical logs. They wear a Smartshirt during exercise that records heart activity and body positions and transmits these data to the app. Finally, rather than manually recording everything that they eat, crew members scan barcodes on food packets to collect real-time nutritional data.
Why are we studying this? EveryWear has the potential for use in science experiments, biomedical support and technology demonstrations.
Outside the Earth’s magnetic field, astronauts are exposed to space radiation that can reduce immune response, increase cancer risk and interfere with electronics.
The Fast Neutron Spectrometer (FNS) experiment will help scientists understand high-energy neutrons, part of the radiation exposure experienced by crews during spaceflight, by studying a new technique to measure electrically neutral neutron particles.
Why are we studying this? This improved measurement will help protect crews on future exploration missions, like our journey to Mars.
Ahead of launch, there will be various opportunities to learn more about the mission:
What’s on Board Science Briefing Saturday, Oct. 15 at 4 p.m. EDT Scientists and researchers will discuss some of the experiments being delivered to the station. Watch HERE.
Prelaunch News Briefing Saturday, Oct. 15 at 6 p.m. EDT Mission managers will provide an overview and status of launch operations. Watch HERE.
LAUNCH!!! Monday, Oct. 17 coverage begins at 6:45 p.m. EDT Watch live coverage and liftoff! Launch is scheduled for 7:40 p.m. EDT. Watch HERE.
Facebook Live Starting at 7:25 p.m. EDT you can stream live coverage of the launch on NASA’s Facebook page. Watch HERE.
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Our solar system is huge, let us break it down for you. Here are a few things you should know this week:
1. Closeup of a King
For the first time since it entered orbit around Jupiter in July, our Juno spacecraft has flown close to the king of planets—this time with its eyes wide open. During the long, initial orbit, Juno mission managers spent time checking out the spacecraft "from stem to stern," but the science instruments were turned off as a precaution. During this latest pass, Juno's camera and other instruments were collecting data the whole time. Initial reports show that all went well, and the team has released a new close-up view that Juno captured of Jupiter's north polar region. We can expect to see more close-up pictures of Jupiter and other data this week.
+Check in with Juno
2. Getting Ready to Rocket
Our OSIRIS-REx mission leaves Earth next week, the first leg of a journey that will take it out to an asteroid called Bennu. The mission will map the asteroid, study its properties in detail, then collect a physical sample to send back home to Earth. The ambitious endeavor is slated to start off on Sept. 8.
+See what it takes to prep for a deep space launch
3. New Moon Rising
The Lunar Reconnaissance Orbiter (LRO) has already mapped the entire surface of Earth's moon in brilliant detail, but the mission isn't over yet. Lunar explorers still have questions, and LRO is poised to help answer them.
+See what’s next for the mission
4. A Mock-Eclipse Now
We don't have to wait until next year to see the moon cross in front of the sun. From its vantage point in deep space, our Solar Dynamics Observatory (SDO) sometimes sees just that. Such an event is expected on Sept. 1.
+See the latest sun pictures from SDO
5. Jupiter’s Cousins
Our galaxy is home to a bewildering variety of Jupiter-like worlds: hot ones, cold ones, giant versions of our own giant, pint-sized pretenders only half as big around. Astronomers say that in our galaxy alone, a billion or more such Jupiter-like worlds could be orbiting stars other than our sun. And we can use them to gain a better understanding of our solar system and our galactic environment, including the prospects for finding life.
Want to learn more? Read our full list of the 10 things to know this week about the solar system HERE.
Make sure to follow us on Tumblr for your regular dose of space: http://nasa.tumblr.com
Do you know what the structural backbone is of our new rocket, the Space Launch System? If you answered the core stage, give yourself a double thumbs up! Or better yet, have astronaut Scott Kelly do it!
We’re on a journey to Mars. For bolder missions to deep space, we need a big, powerful rocket like SLS to take astronauts in the Orion spacecraft to places we've never gone before. The core stage is a major part of that story, as it will house the fuel and avionics systems that will power and guide the rocket to those new destinations beyond Earth’s orbit. Here's how:
It's Big, and It's Fast.
The core stage will be the largest rocket stage ever built and is under construction right now at our Michoud Assembly Facility in New Orleans. It will stand at 212 feet tall and weigh more than 2.3 million pounds with propellant. That propellant is cryogenic liquid hydrogen and liquid oxygen that will feed the vehicle’s RS-25 engines. In just 8.5 minutes, the core stage will reach Mach 23, which is faster than 17,000 mph!
It's Smart.
Similar to a car, the rocket needs all the equipment necessary for the "drive" to deep space. The core stage will house the vehicle’s avionics, including flight computers, instrumentation, batteries, power handling, sensors and other electronics. That's a lot of brain power behind those orange-clad aluminum walls. *Fun fact: Orange is the color of the rocket's insulation.
It's a Five-Parter.
The core stage is made up of five parts. Starting from the bottom is the engine section, which will deliver the propellants to the four RS-25 engines. It also will house avionics to steer the engines, and be an attachment point for the two, five-segment solid rocket boosters. The engine section for the first SLS flight has completed welding and is in the final phases of manufacturing at Michoud.
Next up is the liquid hydrogen tank. It will hold 537,000 gallons of liquid hydrogen cooled to -423 degrees Fahrenheit. Right now, engineers are building the tank for the first SLS mission. It will look very similar to the qualification test article that just finished welding at Michoud. That's an impressive piece of rocket hardware!
The next part of the core stage is the intertank, which will join the propellant tanks. It has to be super strong because it is the attachment point for the boosters and absorbs most of the force when they fire 3.6 million pounds of thrust each. It's also a "think tank" of sorts, as it holds the SLS avionics and electronics. The intertank is even getting its own test structure at our Marshall Space Flight Center in Huntsville, Alabama.
And then there's the liquid oxygen tank. It will store 196,000 gallons of liquid oxygen cooled to -297 degrees. If you haven't done the math, that's 733,000 gallons of propellant for both tanks, which is enough to fill 63 large tanker trucks. Toot, toot. Beep, beep! A confidence version of the tank has finished welding at Michoud, and it's impressive. Just ask this guy.
The topper of the core stage is the forward skirt. Funny name, but serious hardware. It's home to the flight computers, cameras and avionics. The avionics system is being tested right now in a half-ring structure at the Marshall Center.
You can click here for more SLS core stage facts. We'll continue building, and see you at the launch pad for the first flight of SLS with Orion in 2018!
Make sure to follow us on Tumblr for your regular dose of space: http://nasa.tumblr.com
The countdown to our last full-scale test firing of NASA’s Space Launch System (SLS) solid rocket boosters has begun (mark your calendars: June 28, 8:05 a.m. MDT [local time] 10:05 a.m. EDT). SLS is NASA’s new rocket that can go to deep space destinations, and this test is one more step on our Journey to Mars. This test will be broadcast live on NASA TV and our Facebook page. For those watching at home or work, here are four cool things that might not be so obvious on the screen.
With expanding gases and flames exiting the nozzle at speeds in excess of Mach 3 and temperatures reaching 3,700 degrees Fahrenheit, say goodbye to some of the sand at Orbital ATK’s test facility in the Utah desert because after the test, the sand at the aft, or rear, end of the booster motor will be glass.
This motor has been chilling — literally, down to 40 degrees — since the first week in May in Orbital ATK’s “booster house,” a special building on rails that moves to enclose the booster and rolls back so the motor can be test-fired. Even though SLS will launch from the normally balmy Kennedy Space Center in Florida, temperatures can vary there and engineers need to be sure the booster will perform as expected whether the propellant inside the motor is 40 degrees or 90 degrees (the temperature of the propellant during the first full-scale test, Qualification Motor 1 or QM-1).
If you happen to be near Promontory, Utah, on June 28, you can view the test for yourself in the public viewing area off State Route 83. And don’t worry, this booster’s not going anywhere — engineers have it locked down. The motor is held securely in place by Orbital ATK’s T-97 test stand. During the test, the motor will push against a forward thrust block with more than three million pounds of force. Holding down the rocket motor is more than 13 million pounds of concrete — most of which is underground. The test stand contains a system of load cells that enable engineers to measure the thrust the motor produces and verify their predictions.
These solid rocket boosters are the largest and most powerful ever built for flight. They’ve been tested and retested in both full-scale and smaller subsystem-level tests, and vital parts like the nozzle, insulation and avionics control systems have been upgraded and revamped. Most of this work was necessary because, plainly put, SLS needs bigger boosters. Bigger boosters mean bolder missions – like around the moon during the first integrated mission of SLS and Orion. So the next time we see these solid rocket motors fire, they will be propelling SLS off the launch pad at Kennedy Space Center and on its first flight with NASA’s Orion spacecraft. For real.
Have you ever packed for a long trip with a friend and ran out of space in your suitcase? Maybe your friend was nice and let your spare items hitchhike a ride in their bag? The following science experiments are doing something similar on our Space Launch System rocket.
Our Space Launch System (SLS) will be the most powerful rocket we’ve ever built and will enable astronauts in the Orion spacecraft to travel deeper into the solar system. This advanced launch vehicle will launch astronauts to an asteroid and eventually to Mars, while opening new possibilities for other payloads including robotic scientific missions to places like Mars, Saturn and Jupiter.
The primary goal of SLS and the Orion spacecraft is to launch future crewed, deep space missions. That said, an added bonus of this powerful rocket is the extra science it can carry. On it’s first mission (known as Exploration Mission-1, EM-1) SLS will carry 13 CubeSats (small satellites, each the size of a large shoebox) on its first flight as secondary payloads. These small satellites will perform various in-space experiments. In a way, these 13 CubeSats are ‘space hitchhikers’, catching a ride to deep space where they can gather data valuable to future exploration missions.
How were these 13 experiments selected? Great question. They were selected through a series of announcements of flight opportunities, a public contest and negations with our international partners.
These secondary payloads have a vast array of functions, from taking pictures of asteroids, to using yeast to detect impacts of deep-space radiation. Each month we will highlight one of these experiments on Tumblr and talk about all the exciting science they will do. Just to give you an idea of what these shoebox-sized satellites will do, we’ll give you a preview:
1. NEA Scout
NEA Scout, stands for: Near-Earth Asteroid Scout. This CubeSat will investigate an asteroid, taking pictures and observe its position in space.
2. BioSentinel
BioSentinel will be the first time living organisms have traveled to deep space in more than 40 years. It will use yeast to detect, measure and compare the impact of deep-space radiation on living organisms over long durations in deep space.
3. Lunar Flashlight
This experiment will look for ice deposits and identify locations where resources may be extracted from the lunar surface. It will demonstrate the capability to scout for useful materials and resources from lunar orbit.
4. Skyfire
Lockheed Martin’s Skyfire will perform a lunar flyby, collecting data to address both Moon and Mars Strategic Knowledge Gaps, or gaps in information required to reduce risk, increase effectiveness and improve the design of robotic and human space exploration missions, for surface characterization, remote sensing and site selection.
5. Lunar IceCube
Morehead State University’s Lunar IceCube will look for water in ice, liquid and vapor forms from a very low orbit of only 62 miles above the surface of the moon. The ability to search for useful resources can potentially help astronauts manufacture fuel and necessities to sustain a crew.
6. CuSP
The CubeSat mission to study Solar Particles, or CuSP, will be the first protype of an interplanetary CubeSat space weather station. It will observe space weather events hours before they reach Earth.
7. Luna-H-Map
Lunar Polar Hydrogen Mapper (LunaH) will enter a polar orbit around the moon with a low altitude. From there, it will produce maps of near-surface hydrogen.
8, 9, 10. Three Tournament Payloads
Three of the payloads riding along on this journey will be the winners of the Ground Tournaments portion of our CubeQuest Challenge. This challenge is designed to foster innovation in small spacecraft propulsion and communications techniques. Learn more about this challenge HERE.
11, 12, 13. International Partners
The remaining three payloads are reserved for international partners, and will be announced at a later time.
To stay updated on these experiments, visit: http://www.nasa.gov/launching-science-and-technology.html
Make sure to follow us on Tumblr for your regular dose of space: http://nasa.tumblr.com
Our Space Launch System (SLS) is an advanced launch vehicle for exploration beyond Earth’s orbit into deep space. SLS, the world’s most powerful rocket, will launch astronauts in our Orion spacecraft on missions to an asteroid and eventually to Mars!
A launch system required to carry humans faster and farther than ever before will need a powerful engine, aka the RS-25 engine. This engine makes a modern race car or jet engine look like a wind-up toy. With the ability to produce 512,000 pounds of trust, the RS-25 engine will produce 10% more thrust than the Saturn V rockets that launched astronauts on journeys to the moon!
Another consideration for using these engines for future spaceflight was that 16 of them already existed from the shuttle program. Using a high-performance engine that already existed gave us a considerable boost in developing its next rocket for space exploration.
Once ready, four RS-25 engines will power the core stage of our SLS into deep space and Mars.