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It will take incredible power to send the first woman and the next man to the Moon’s South Pole by 2024. That’s where America’s Space Launch System (SLS) rocket comes in to play.
Providing more payload mass, volume capability and energy to speed missions through deep space than any other rocket, our SLS rocket, along with our lunar Gateway and Orion spacecraft, creates the backbone for our deep space exploration and Artemis lunar mission goals.
Here’s why our SLS rocket is a deep space rocket like no other:
The Artemis missions will send humans 280,000 miles away from Earth. That’s 1,000 times farther into space than the International Space Station. To accomplish that mega feat, you need a rocket that’s designed to lift — and lift heavy. With help from a dynamic core stage — the largest stage we have ever built — the 5.75-million-pound SLS rocket can propel itself off the Earth. This includes the 57,000 pounds of cargo that will go to the Moon. To accomplish this, SLS will produce 15% more thrust at launch and during ascent than the Saturn V did for the Apollo Program.
Where do our rocket’s lift and thrust capabilities come from? If you take a peek under our powerful rocket’s hood, so to speak, you’ll find a core stage with four RS-25 engines that produce more than 2 million pounds of thrust alongside two solid rocket boosters that each provide another 3.6 million pounds of thrust power. It’s a bold design. Together, they provide an incredible 8.8 million pounds of thrust to power the Artemis missions off the Earth. The engines and boosters are modified heritage hardware from the Space Shuttle Program, ensuring high performance and reliability to drive our deep space missions.
While our rocket’s core stage design will remain basically the same for each of the Artemis missions, the SLS rocket’s upper stage evolves to open new possibilities for payloads and even robotic scientific missions to worlds farther away than the Moon like Mars, Saturn and Jupiter. For the first three Artemis missions, our SLS rocket uses an interim cryogenic propulsion stage with one RL10 engine to send Orion to the lunar south pole. For Artemis missions following the initial 2024 Moon landing, our SLS rocket will have an exploration upper stage with bigger fuel tanks and four RL10 engines so that Orion, up to four astronauts and larger cargoes can be sent to the Moon, too. Additional core stages and upper stages will support either crewed Artemis missions, science missions or cargo missions for a sustained presence in deep space.
Crews at our Michoud Assembly Facility in New Orleans are in the final phases of assembling the core stage for Artemis I— and are already working on assembly for Artemis II.
Through the Artemis program, we aim not just to return humans to the Moon, but to create a sustainable presence there as well. While there, astronauts will learn to use the Moon’s natural resources and harness our newfound knowledge to prepare for the horizon goal: humans on Mars.
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The Apollo 11 Moon landing was a feat for the ages. With the help of the NASA History Office, we’ve identified some of the most frequently asked questions surrounding the first time humans walked on the surface of another world. Click here to check out our post from last week.
Believe it or not, yes! The Apollo guidance computer not only had less computing power than a smartphone, it had less computing power than the calculator you use in your algebra class. The computer, designed by MIT, had a fixed memory of 36 kilobytes and an erasable memory of 2 kilobytes. That’s fairly advanced for the time!
A substantial portion of the Apollo 11 crew’s checklist was taking photographs. Taking closeup shots of the "very fine” moon dust was a critical component of mission objectives and helped scientists better understand the surface makeup of the Moon.
Armstrong and Aldrin wore lunar overboots over their main spacesuit boots to protect them from ultraviolet radiation and hazardous rocks. To make room for the nearly 50 pounds (22 kilograms) of lunar samples, the crew left all their pairs of boots on the Moon. But don’t worry; they wouldn’t get charged an overweight baggage fee anyway.
That’s somewhat subject to interpretation. Once the Lunar Module’s surface sensor touched the surface, Buzz Aldrin called out "Contact Light” to Mission Control. After the engine shut down, he said “ACA out of detent,” simply meaning that the Eagle’s Attitude Control Assembly, or control stick, was moved from its center position.
But the first words heard by the entire world after Apollo 11 touched down were delivered by Neil Armstrong: "Houston, Tranquility Base here. The Eagle has landed.” More than six hours later, Armstrong stepped off the Eagle’s footpad and delivered the most famous words ever spoken from the surface of another world: "That's one small step for [a] man, one giant leap for mankind." And although we have a hard time hearing it in the recording, Armstrong clarified in a post-flight interview that he actually said, “That’s one small step for a man...”
We can’t say for sure what our next moonwalkers will decide to say, but perhaps the better question is: What would be your first words if you were to land on the Moon? There’s no doubt that the astronauts of the Artemis Generation will inspire a new crop of explorers the way Apollo Generation astronauts did 50 years ago. Make sure to follow us on Tumblr for your regular dose of space: http://nasa.tumblr.com.
Image Credit: NOAA
Earth’s ocean has been the backdrop for ancient epics, tales of fictional fish and numerous scientific discoveries. It was, and will always be, a significant piece of the Earth's story. Most of the ocean is unexplored– about 95% of this underwater realm is unseen by human eyes (NOAA). There is only one global Ocean. In fact, the ocean represents over 70% of the Earth's surface and contains 96.5% of the Earth’s water.
We and the NOAA Office of Ocean Exploration and Research work together alongside organizations like the Schmidt Ocean Institute and Ocean Exploration Trust to better understand our oceans and its processes. While space may be the final frontier, understanding our own planet helps scientists as they explore space and study how our universe came to be.
On #WorldOceansDay let’s explore how Earth’s ocean informs our research throughout the solar system.
“In interpreting what we see elsewhere in the solar system and universe, we always compare with phenomena that we already know of on Earth...We work from the familiar toward the unknown.” - Norman Kuring, NASA Goddard
We know of only one living planet: our own. As we move to the next stage in the search for alien life, the effort will require the expertise of scientists of all disciplines. However, the knowledge and tools NASA has developed to study life on Earth will also be one of the greatest assets to the quest.
The photo above shows what Earth would look like at a resolution of 3 pixels, the same that exoplanet-discovering missions would see. What should we look for, in the search of other planets like our own? What are the unmistakable signs of life, even if it comes in a form we don't fully understand? Liquid water; every cell we know of -- even bacteria around deep-sea vents that exist without sunlight -- requires water.
Jupiter’s storms are mesmerizing in their beauty, captured in many gorgeous photos throughout the decades from missions like Voyager 1 and Juno. The ethereal swirls of Jupiter are the result of fluids in motion on a rotating body, which might come as a surprise, since its atmosphere is made of gas!
The eddies in Jupiter’s clouds appear very similar to those found in Earth’s ocean, like in the phytoplankton (or algae) bloom in the Baltic Sea, pictured above. The bloom was swept up in a vortex, just a part of how the ocean moves heat, carbon, and nutrients around the planet. Blooms like this, however, are not all beauty - they create “dead zones” in the areas where they grow, blooming and decaying at such a high rate that they consume all the oxygen in the water around them.
While the Arctic (North Pole) and the Antarctic (South Pole) are “polar opposites,” there is one huge difference between the North and South Poles– land mass. The Arctic is ocean surrounded by land, while the Antarctic is land surrounded by ocean. The North Pole is located in the middle of the Arctic Ocean amid waters that are almost permanently covered with constantly shifting sea ice.
By studying this sea ice, scientists can research its impact on Earth system and even formation processes on other bodies like Europa, an icy moon of Jupiter. For example, it is possible that the reddish surface features on Europa’s ice may have communicated with a global subsurface ocean layer during or after their formation.
As new missions are being developed, scientists are using Earth as a testbed. Just as prototypes for our Mars rovers made their trial runs on Earth's deserts, researchers are testing both hypotheses and technology on our oceans and extreme environments.
NEEMO, our Extreme Environment Mission Operations project, is an analog mission that sends groups of astronauts, engineers and scientists to live in Aquarius, the world's only undersea research station located off the Florida Keys, 62 feet (19 meters) below the surface. Much like space, the undersea world is a hostile, alien place for humans to live. NEEMO crew members, known as aquanauts, experience some of the same challenges there that they would on a distant asteroid, planet or moon.
Video credit: Deep Sea Robotics/Schmidt Ocean Institute and Mars Curiosity rover/NASA
From mapping the seafloor through bathymetry to collecting samples on the surface of Mars, researchers are utilizing new technologies more than ever to explore. Satellite and robotic technology allow us to explore where humans may not be able to– yet. They teach us valuable lessons about the extreme and changing environments, science, as well as provide a platform to test new technologies.
River deltas, the point where a river meets the ocean, are sites of rich sediment and incredible biodiversity. The nutrients that rivers carry to the coastlines make a fertile place for fish and shellfish to lay their eggs.
The Jezero crater on Mars (pictured in false-color on the right) has been selected as the Mars2020 landing site, and has a structure that looks much like a river delta here on Earth! Pictures from our Mars Global Surveyor orbiter show eroded ancient deposits of transported sediment long since hardened into interweaving, curved ridges of layered rock. This is one of many hints that Mars was once covered in an ancient ocean that had more water than the Arctic Ocean. Studying these deltas on Earth helps us spot them on other planets, and learning about the ocean that was once on Mars informs how our own formed.
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Our Space Launch System isn’t your average rocket. It is the only rocket that can send our Orion spacecraft, astronauts and supplies to the Moon. To accomplish this mega-feat, it has to be the most powerful rocket ever built. SLS has already marked a series of milestones moving it closer to its first launch, Artemis.
Here are four highlights you need to know about — plus one more just on the horizon.
Earlier this month, Boeing technicians at our Michoud Assembly Facility in New Orleans successfully joined the top part to the core stage with the liquid hydrogen tank. The core stage will provide the most of the power to launch Artemis 1. Our 212-foot-tall core stage, the largest the we have ever built, has five major structural parts. With the addition of the liquid hydrogen tank to the forward join, four of the five parts have been bolted together. Technicians are finishing up the final part — the complex engine section — and plan to bolt it in place later this summer.
This August, to be exact. That’s when the engines for Artemis 1 will be added to the core stage. Earlier this year, all the engines for the first four SLS flights were updated with controllers, tested and officially cleared “go” for launch. We’ve saved time and money by modifying 16 RS-25 engines from the space shuttle and creating a more powerful version of the solid rocket boosters that launched the shuttle. In April, the last engine from the shuttle program finished up a four-year test series that included 32 tests at our Stennis Space Center near Bay St. Louis, Mississippi. These acceptance tests proved the engines could operate at a higher thrust level necessary for deep space travel and that new, modernized flight controllers —the “brains” of the engine — are ready to send astronauts to the Moon in 2024.
Our industry partners have completed the manufacture and checkout of 10 motor segments that will power two of the largest propellant boosters ever built. Just like the engines, these boosters are designed to be fast and powerful. Each booster burns six tons of propellant every second, generating a max thrust of 3.6 million pounds for two minutes of pure awesome. The boosters will finish assembly at our Kennedy Space Center in Florida and readied for the rocket’s first launch in 2020. In the meantime, we are well underway in completing the boosters for SLS and Orion’s second flight in 2022.
Meanwhile, other parts of the rocket are finished and ready for the ride to the Moon. The final piece of the upper part of the rocket, the launch vehicle stage adapter, will soon head toward Kennedy Space Center in Florida. Two other pieces, including the interim cryogenic propulsion stage that will provide the power in space to send Orion on to the Moon, have already been delivered to Kennedy.
Our engineers evaluated thousands of designs before selecting the current SLS rocket design. Now, they are performing critical testing and using lessons learned from current assembly to ensure the initial and future designs are up to the tasks of launching exploration missions for years to come. This real-time evaluation means engineers and technicians are already cutting down on assembly time for future mission hardware, so that we and our partners can stay on target to return humans to the Moon by 2024 — to stay so we can travel on to Mars.
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In celebration of the 50th anniversary of Apollo 11, we’ll be sharing answers to some frequently asked questions about the first time humans voyaged to the Moon. Answers have been compiled from archivists in the NASA History Office.
At the height of Apollo in 1965, about 409,900 people worked on some aspect of the program, but that number doesn’t capture it all.
It doesn’t represent the people who worked on mission concepts or spacecraft design, such as the engineers who did the wind tunnel testing of the Apollo Command Module and then moved on to other projects. The number also doesn’t represent the NASA astronauts, mission controllers, remote communications personnel, etc. who would have transferred to the Apollo program only after the end of Gemini program (1966-1967). There were still others who worked on the program only part-time or served on temporary committees. In the image above are three technicians studying an Apollo 14 Moon rock in the Lunar Receiving Laboratory at Johnson Space Center. From left to right, they are Linda Tyler, Nancy Trent and Sandra Richards.
This artwork portrait done by spaceflight historian Ed Hengeveld depicts the 12 people who have walked on the Moon so far. In all, 24 people have flown to the Moon and three of them, John Young, Jim Lovell and Gene Cernan, have made the journey twice.
But these numbers will increase.
Every successful Apollo lunar landing mission left a flag on the Moon but we don’t know yet whether all are still standing. Some flags were set up very close to the Lunar Module and were in the blast radius of its ascent engine, so it’s possible that some of them could have been knocked down. Neil Armstrong and Buzz Aldrin both reported that the flag had been knocked down following their ascent.
Our Lunar Reconnaissance Orbiter took photographs of all the Apollo lunar landing sites. In the case of the Apollo 17 site, you can see the shadow of the upright flag.
The flags appear to “wave” or “flap” but actually they’re swinging. Swinging motions on Earth are dampened due to gravity and air resistance, but on the Moon any swinging motion can continue for much longer. Once the flags settled (and were clear of the ascent stage exhaust), they remained still. And how is the flag hanging? Before launching, workers on the ground had attached a horizontal rod to the top of each flag for support, allowing it to be visible in pictures and television broadcasts to the American public. Armstrong and Aldrin did not fully extend the rod once they were on the Moon, giving the flag a ripple effect. The other astronauts liked the ripple effect so much that they also did not completely extend the rod.
Have you ever taken a photo of the night sky with your phone or camera? You likely won’t see any stars because your camera’s settings are likely set to short exposure time which only lets it quickly take in the light off the bright objects closest to you. It’s the same reason you generally don’t see stars in spacewalk pictures from the International Space Station. There’s no use for longer exposure times to get an image like this one of Bruce McCandless in 1984 as seen from Space Shuttle Challenger (STS-41B).
The Hasselblad cameras that Apollo astronauts flew with were almost always set to short exposure times. And why didn’t the astronauts photograph the stars? Well, they were busy exploring the Moon!
The first giant leap was only the beginning. Work is under way to send the first woman and the next man to the Moon in five years. As we prepare to launch the next era of exploration, the new Artemis program is the first step in humanity’s presence on the Moon and beyond.
Keep checking back for more answers to Apollo FAQs.
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If #NationalCheeseDay has you thinking about the Moon, you're not alone. 🧀
In 1965, the Ranger 9 probe captured these sharp images of a cratered lunar surface just moments before its planned impact. What we learned paved the way for Apollo. #Apollo50th