Solar System: Things To Know This Week

Solar System: Things to Know This Week

Learn all about the end of the Rosetta Mission and more about the weather on Mars, the Moon’s colorful palette.

1. Rosetta’s Last Dance

The Rosetta mission was one of firsts: the first to orbit a comet and the first to dispatch a lander to a comet's surface. Rosetta transformed our understanding of these ancient wanderers, and this week, mission controllers will command the spacecraft to execute a series of maneuvers to bring it out of orbit around Comet 67P/Churyumov-Gerasimenko. Watch live on Sept. 30 from 6:15-8 a.m. EDT, the Rosetta mission's 12-year odyssey in space reaches its conclusion. Rosetta will descend to make a planned impact on the comet’s surface with its instruments recording science data during descent.

+Watch live as Rosetta crash lands on NASA TV, recording data along the way

+More on the mission’s final descent

+Mission highlights

2.  Hubble Spots Possible Water Plumes Erupting on Jupiter's Moon Europa

On Monday, Sept. 26, our scientists announced what may be water vapor plumes erupting off the surface of Jupiter's moon Europa, based on data from the Hubble Space Telescope. This finding bolsters other Hubble observations suggesting the icy moon erupts with high altitude water vapor plumes.

+Learn the latest on Europa

3. Not So Impossible After All

Scientists have found an "impossible" ice cloud on Saturn's moon Titan. The puzzling appearance of an ice cloud prompted our researchers to suggest that a different process than previously thought could be forming clouds on Titan. The process may be similar to one seen over Earth's poles. Today, the Cassini spacecraft will perform a targeted Titan flyby, skimming just 1,079 miles (1,736 kilometers) above its hazy surface. Several of Cassini's instruments will be watching for clouds and other phenomena in the atmosphere, as well as taking measurements of the surface.

+Learn more about Titan’s clouds

4. Lunar Intrigue

Earth's moon is a colorless world of grays and whites, right? Not really. As seen in these images from the Lunar Reconnaissance Orbiter, some landscapes on the moon reveal a whole range of color. One such place is the mountainous complex of ancient lava flows known as the Lassell Massif, one of the moon's so-called "red spots."

+Take a look

5. Weather Report: Mars

A camera aboard our Mars Reconnaissance Orbiter monitors global weather patterns daily. The most recent report includes the remains of a large dust storm in the Noachis region, and smaller tempests spotted along the edge of the south polar ice cap and water-ice clouds over the volcano Arsia Mons.

+ Learn more and see Mars weather videos

Discover the full list of 10 things to know about our solar system this week HERE.

Make sure to follow us on Tumblr for your regular dose of space: http://nasa.tumblr.com

Studying the tiny life of phytoplankton

Phytoplankton. Have you ever heard of them? At NASA, these tiny organisms are kind of a big deal.

Biodiversity in the ocean is a delicate, but essential balance for life on Earth. One way NASA studies this balance is by observing phytoplankton – microalgae that contain chlorophyll, require light to grow, and form the base of the marine food chain.

Phytoplankton even have an essential role in an upcoming NASA mission.

This mission is called PACE- "Plankton, Aerosol, Cloud, ocean Ecosystem.” It will reveal interactions between the ocean and atmosphere, including how they exchange carbon dioxide and how atmospheric aerosols might fuel phytoplankton growth in the surface ocean.

Here are four areas main areas the mission will focus on as part of #WorldOceansMonth.

1. Harmful algal blooms: Not the good kind of bloom

The word “bloom” sounds pretty, but harmful algal blooms (HABs) are anything but.

When an ocean region is rich in nutrients – think of it as adding fertilizer to the ocean -  phytoplankton such as cyanobacteria multiply much faster than usual. This is called a “bloom.”

Some blooms are smelly and ugly but harmless. Others, like HABs, release toxins into the water that can make fish, shellfish, turtles and even humans very sick.

NASA’s PACE mission will help track phytoplankton growth and ocean health to make sure all of us stay healthy, balanced and blooming. In a good way.

2. Aerosols: The sea-sky connection

What do phytoplankton and clouds have in common? More than you might think.

PACE will also study aerosols, which are any particles or droplets suspended in our atmosphere. Humans create aerosols, like soot or car exhaust, but some phytoplankton release aerosols too.

For example, dust – also an aerosol – can blow into the ocean, depositing iron that helps phytoplankton grow. These phytoplankton then release dimethyl sulfide, a gas that turns into an aerosol, which can influence how clouds form.

Whether the aerosols in our atmosphere come from the ocean or land, it’s important to know how they are impacting our environment. PACE will help clear up some of our questions about what is in our air.

3. Biodiversity: The more, the merrier

A healthy ocean supports healthy industries and economies, contributes to a healthy atmosphere and helps keep plants, animals and humans healthy and happy. One key to a healthy, balanced ocean is lots of biodiversity.

Biodiversity means having a wide variety of plant and animal species in an ecosystem. It’s important to have many different species of phytoplankton, because each species plays a different role in processing carbon, providing food for tiny animals, and keeping the ocean healthy.

PACE will track the size and movements of phytoplankton populations from space to help our seas stay diverse and bountiful.

4. Fisheries: Phytoplankton feed fish feed friends

One simple reason for tracking the ocean’s health is that fish eat tiny animals that eat phytoplankton, and people eat fish.

Fisheries and aquaculture support about 12 percent of jobs around the world, including employing more than 3 million people in the United States. By better understanding our ocean’s health and how it might change in the future, we can make predictions about impacts to our economies and food supply.

To learn more about phytoplankton, visit our website.

Make sure to follow us on Tumblr for your regular dose of space: http://nasa.tumblr.com.

What dose it feel like being inside a space suit?

The suit weighs about 300 pounds. We are made neutrally buoyant in the pool, but over time we can become negatively buoyant. The suit can feel heavy, even the bearings can become stiff, so it can be difficult to operate in the suit. With practice and the help of a great spacewalk team, we can make a spacewalk look seamless.

Why We Celebrate Search and Rescue Technologies on 4/06

Today (4/06), we celebrate the special radio frequency transmitted by emergency beacons to the international search and rescue network. 

This 406 MHz frequency, used only for search and rescue, can be "heard" by satellites hundreds of miles above the ground! The satellites then "forward" the location of the beacon back to Earth, helping first responders locate people in distress worldwide, whether from a plane crash, a boating accident or other emergencies.

Our Search and Rescue office, based out of our Goddard Space Flight Center, researches and develops emergency beacon technology, passing the technology to companies who manufacture the beacons, making them available to the public at retail stores. The beacons are designed for personal, maritime and aviation use.

The search and rescue network, Cospas-Sarsat, is an international program that ensures the compatibility of distress alert services with the needs of users. Its current space segment relies on instruments onboard low-Earth and geosynchronous orbiting satellites, hundreds to thousands of miles above us. 

Space instruments forward distress signals to the search and rescue ground segment, which is operated by partner organizations around the world! They manage specific regions of the ground network. For example, the National Oceanic and Atmospheric Administration (NOAA) operates the region containing the United States, which reaches across the Atlantic and Pacific Oceans as well as parts of Central and South America.

NOAA notifies organizations that coordinate search and rescue efforts of a 406 MHz distress beacon's activation and location. Within the U.S., the U.S. Air Force responds to land-based emergencies and the U.S. Coast Guard responds to water-based emergencies. Local public service organizations like police and fire departments, as well as civilian volunteers, serve as first responders.

Here at NASA, we research, design and test search and rescue instruments and beacons to refine the existing network. Aeronautical beacon tests took place at our Langley Research Center in 2015. Using a 240-foot-high structure originally used to test Apollo spacecraft, our Search and Rescue team crashed three planes to test the survivability of these beacons, developing guidelines for manufacturers and installation into aircraft.

In the future, first responders will rely on a new constellation of search and rescue instruments on GPS systems on satellites in medium-Earth orbit, not hundreds, but THOUSANDS of miles overhead. These new instruments will enable the search and rescue network to locate a distress signal more quickly than the current system and achieve accuracy an order of magnitude better, from a half mile to approximately 300 feet. Our Search and Rescue office is developing second-generation 406 MHz beacons that make full use of this new system.

We will also incorporate these second-generation beacons into the Orion Crew Survival System. The Advanced Next-Generation Emergency Locator (ANGEL) beacons will be attached to astronaut life preservers. After splashdown, if the Orion crew exits the capsule due to an emergency, these beacons will make sure we know the exact location of floating astronauts! Our Johnson Space Center is testing this technology for used in future human spaceflight and exploration missions.

If you're the owner of an emergency beacon, remember that beacon registration is free, easy and required by law. 

To register your beacon, visit: beaconregistration.noaa.gov

Make sure to follow us on Tumblr for your regular dose of space: http://nasa.tumblr.com

How Do We Learn About a Planet’s Atmosphere?

The first confirmation of a planet orbiting a star outside our solar system happened in 1995. We now know that these worlds – also known as exoplanets – are abundant. So far, we’ve confirmed more than 4000. Even though these planets are far, far away, we can still study them using ground-based and space-based telescopes.

Our upcoming James Webb Space Telescope will study the atmospheres of the worlds in our solar system and those of exoplanets far beyond. Could any of these places support life? What Webb finds out about the chemical elements in these exoplanet atmospheres might help us learn the answer.

How do we know what’s in the atmosphere of an exoplanet?

Most known exoplanets have been discovered because they partially block the light of their suns. This celestial photo-bombing is called a transit.

During a transit, some of the star's light travels through the planet's atmosphere and gets absorbed.

The light that survives carries information about the planet across light-years of space, where it reaches our telescopes.

(However, the planet is VERY small relative to the star, and VERY far away, so it is still very difficult to detect, which is why we need a BIG telescope to be sure to capture this tiny bit of light.)

So how do we use a telescope to read light?

Stars emit light at many wavelengths. Like a prism making a rainbow, we can separate light into its separate wavelengths. This is called a spectrum. Learn more about how telescopes break down light here. 

Visible light appears to our eyes as the colors of the rainbow, but beyond visible light there are many wavelengths we cannot see.

Now back to the transiting planet...

As light is traveling through the planet's atmosphere, some wavelengths get absorbed.

Which wavelengths get absorbed depends on which molecules are in the planet's atmosphere. For example, carbon monoxide molecules will capture different wavelengths than water vapor molecules.

So, when we look at that planet in front of the star, some of the wavelengths of the starlight will be missing, depending on which molecules are in the atmosphere of the planet.

Learning about the atmospheres of other worlds is how we identify those that could potentially support life...

...bringing us another step closer to answering one of humanity's oldest questions: Are we alone?

Watch the full video where this method of hunting for distant planets is explained:

To learn more about NASA’s James Webb Space Telescope, visit the website, or follow the mission on Facebook, Twitter and Instagram. 

Text and graphics credit Space Telescope Science Institute

Make sure to follow us on Tumblr for your regular dose of space: http://nasa.tumblr.com.  

Rocket Fuel in Her Blood: The Story of JoAnn Morgan

As the Apollo 11 mission lifted off on the Saturn V rocket, propelling humanity to the surface of the Moon for the very first time, members of the team inside Launch Control Center watched through a window.

The room was crowded with men in white shirts and dark ties, watching attentively as the rocket thrust into the sky. But among them sat one woman, seated to the left of center in the third row in the image below. In fact, this was the only woman in the launch firing room for the Apollo 11 liftoff.

This is JoAnn Morgan, the instrumentation controller for Apollo 11. Today, this is what Morgan is most known for. But her career at NASA spanned over 45 years, and she continued to break ceiling after ceiling for women involved with the space program.

“It was just meant to be for me to be in the launching business,” she says. “I’ve got rocket fuel in my blood.”

Morgan was inspired to join the human spaceflight program when Explorer 1 was launched into space in 1958, the first satellite to do so from the United States. Explorer 1 was instrumental in discovering what has become known as the Van Allen radiation belt. 

“I thought to myself, this is profound knowledge that concerns everyone on our planet,” she says. “This is an important discovery, and I want to be a part of this team. I was compelled to do it because of the new knowledge, the opportunity for new knowledge.”

The opportunity came when Morgan spotted an advertisement for two open positions with the Army Ballistic Missile Agency. The ad listed two Engineer’s Aide positions available for two students over the summer.

 “Thank God it said ‘students’ and not ‘boys’” says Morgan, “otherwise I wouldn’t have applied.”

After Morgan got the position, the program was quickly rolled into a brand-new space exploration agency called NASA. Dr. Kurt Debus, the first director of Kennedy Space Center (KSC), looked at Morgan’s coursework and provided Morgan with a pathway to certification. She was later certified as a Measurement and Instrumentation Engineer and a Data Systems Engineer.

There was a seemingly infinite amount of obstacles that Morgan was forced to overcome — everything from obscene phone calls at her station to needing a security guard to clear out the men’s only restroom.

“You have to realize that everywhere I went — if I went to a procedure review, if I went to a post-test critique, almost every single part of my daily work — I’d be the only woman in the room,” reflects Morgan. “I had a sense of loneliness in a way, but on the other side of that coin, I wanted to do the best job I could.”

To be the instrumentation controller in the launch room for the Apollo 11 liftoff was as huge as a deal as it sounds. For Morgan, to be present at that pivotal point in history was ground-breaking: “It was very validating. It absolutely made my career.”

Much like the Saturn V rocket, Morgan’s career took off. She was the first NASA woman to win a Sloan Fellowship, which she used to earn a Master of Science degree in management from Stanford University in California. When she returned to NASA, she became a divisions chief of the Computer Systems division.

From there, Morgan excelled in many other roles, including deputy of Expendable Launch Vehicles, director of Payload Projects Management and director of Safety and Mission Assurance. She was one of the last two people who verified the space shuttle was ready to launch and the first woman at KSC to serve in an executive position, associate director of the center.

To this day, Morgan is still one of the most decorated women at KSC. Her numerous awards and recognitions include an achievement award for her work during the activation of Apollo Launch Complex 39, four exceptional service medals and two outstanding leadership medals. In 1995, she was inducted into the Florida Women's Hall of Fame.

After serving as the director of External Relations and Business Development, she retired from NASA in August 2003.

Today, people are reflecting on the 50th anniversary of Apollo 11, looking back on photos of the only woman in the launch firing room and remembering Morgan as an emblem of inspiration for women in STEM. However, Morgan’s takeaway message is to not look at those photos in admiration, but in determination to see those photos “depart from our culture.”

“I look at that picture of the firing room where I’m the only woman. And I hope all the pictures now that show people working on the missions to the Moon and onto Mars, in rooms like Mission Control or Launch Control or wherever — that there will always be several women. I hope that photos like the ones I’m in don’t exist anymore.”

Follow Women@NASA for more stories like this one, and make sure to follow us on Tumblr for your regular dose of space: http://nasa.tumblr.com.

Our Galaxy is Caught Up in a Giant Cosmic Cobweb! 🕸️

If we could zoom waaaay out, we would see that galaxies and galaxy clusters make up large, fuzzy threads, like the strands of a giant cobweb. But we'll work our way out to that. First let's start at home and look at our planet's different cosmic communities.

Our home star system

Earth is one of eight planets — Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, and Neptune — that orbit the Sun. But our solar system is more than just planets; it also has a lot of smaller objects.

An asteroid belt circles the Sun between Mars and Jupiter. Beyond Neptune is a doughnut-shaped region of icy objects called the Kuiper Belt. This is where dwarf planets like Pluto and Makemake are found and is likely the source of short-period comets (like Haley’s comet), which orbit the Sun in less than 200 years.

Scientists think that even farther out lies the Oort Cloud, also a likely source of comets. This most distant region of our solar system is a giant spherical shell storing additional icy space debris the size of mountains, or larger! The outer edge of the Oort Cloud extends to about 1.5 light-years from the Sun — that’s the distance light travels in a year and a half (over 9 trillion miles).

Sometimes asteroids or comets get ejected from these regions and end up sharing an orbit with planets like Jupiter or even crossing Earth’s orbit. There are even interstellar objects that have entered the inner solar system from even farther than the Oort Cloud, perhaps coming all the way from another star!

Our home galaxy

Let's zoom out to look at the whole Milky Way galaxy, which contains more than 100 billion stars. Many are found in the galaxy’s disk — the pancake-shaped part of a spiral galaxy where the spiral arms lie. The brightest and most massive stars are found in the spiral arms, close to their birth places. Dimmer, less massive stars can be found sprinkled throughout the disk. Also found throughout the spiral arms are dense clouds of gas and dust called nebulae. The Sun lies in a small spiral arm called the Orion Spur.

The Milky Way’s disk is embedded in a spherical “halo” about 120,000 light-years across. The halo is dotted with globular clusters of old stars and filled with dark matter. Dark matter doesn’t emit enough light for us to directly detect it, but we know it’s there because without its mass our galaxy doesn’t have enough gravity to hold together!

Our galaxy also has several orbiting companion galaxies ranging from about 25,000 to 1.4 million light-years away. The best known of these are the Large and Small Magellanic Clouds, which are visible to the unaided eye from Earth’s Southern Hemisphere.

Our galactic neighborhood

The Milky Way and Andromeda, our nearest neighboring spiral galaxy, are just two members of a small group of galaxies called the Local Group. They and the other members of the group, 50 to 80 smaller galaxies, spread across about 10 million light-years.

The Local Group lies at the outskirts of an even larger structure. It is just one of at least 100 groups and clusters of galaxies that make up the Virgo Supercluster. This cluster of clusters spans about 110 million light-years!

Galaxies aren’t the only thing found in a galaxy cluster, though. We also find hot gas, as shown above in the bright X-ray light (in pink) that surrounds the galaxies (in optical light) of cluster Abell 1413, which is a picturesque member of a different supercluster. Plus, there is dark matter throughout the cluster that is only detectable through its gravitational interactions with other objects.

The Cosmic Web

The Virgo Supercluster is just one of many, many other groups of galaxies. But the universe’s structure is more than just galaxies, clusters, and the stuff contained within them.

For more than two decades, astronomers have been mapping out the locations of galaxies, revealing a filamentary, web-like structure. This large-scale backbone of the cosmos consists of dark matter laced with gas. Galaxies and clusters form along this structure, and there are large voids in between.

The scientific visualizations of this “cosmic web” look a little like a spider web, but that would be one colossal spider! <shudder>

And there you have the different communities that define Earth’s place in the universe. Our tiny planet is a small speck on a crumb of that giant cosmic web!

Want to learn even more about the structures in the universe? Check out our Cosmic Distance Scale!

Make sure to follow us on Tumblr for your regular dose of space.

Welcome Home HERA Mission XVII!

With the Human Exploration Research Analog (HERA) habitat, we complete studies to prepare us for exploration to asteroids, Mars, and the Moon… here on Earth! The studies are called analogs, and they simulate space missions to study how different aspects of deep space affect humans. During a HERA mission, the crew (i.e., the research participants) live and work very much as astronauts do, with minimal contact with anyone other than Mission Control for 45 days.

The most recent study, Mission XVII, just “returned to Earth” on June 18. (i.e., the participants egressed, or exited the habitat at our Johnson Space Center in Houston after their 45-day study.) We talked with the crew, Ellie, Will, Chi, and Michael, about the experience. Here are some highlights!

Why did you decide to participate in HERA Mission XVII?

HERA Mission VXII participants (from left to right) Ellie, Will, Chi, and Michael.

“My master’s is in human factors,” said Chi, who studies the interaction between humans and other systems at Embry-Riddle Aeronautical University. “I figured this would be a cool way to study the other side of the table and actually participate in an analog.” For Michael, who holds a PhD in aerospace engineering and researches immunology and radio biology, it was an opportunity to experience life as an astronaut doing science in space. “I’ve flown [experiments] on the space station and shuttle,” he said. “Now I wanted to see the other side.” For Will, a geosciences PhD, it provided an opportunity to contribute to space exploration and neuroscience, which he considers two of the biggest fields with the most potential in science. “Here, we have this project that is the perfect intersection of those two things,” he said. And Ellie, a pilot in the Air Force, learned about HERA while working on her master’s thesis on Earth and space analogs and how to improve them for deep-space studies. “A lot of my interests are similar to Chi’s,” she said. “Human factors and physiological aspects are things that I find very fascinating.”

NASA missions all have patches, and HERA Mission XVII is no different. Did you get to design your patch?

HERA Mission VXII patch, which reads “May the Force be with you” in Latin and features Star Wars iconography. It’s a reference to the mission’s start date, May 4th aka Star Wars Day!

“We did!” They said …with a little the help from Michael’s brother, who is a designer. He drew several different designs based on the crew’s ideas. They picked one and worked together on tweaks. “We knew we were going [inside the habitat] on May Fourth,” Michael said. “We knew it would be Star Wars Day. So we did a Star Wars theme.” The patch had to come together fairly quickly though, since a Star Wars Day “launch” wasn’t the initial plan. “We were supposed to start two weeks earlier,” Ellie said. “It just so happened the new start date was May the Fourth!” Along with the Star Wars imagery, the patch includes a hurricane symbol, to pay tribute to hurricane Harvey which caused a previous crew to end their mission early, and an image of the HERA habitat. Will joked that designing the patch was “our first team task.”

How much free time did you have and what did you do with it?

HERA Mission XVII crew looking down the ladders inside the habitat.

“It was a decent amount,” Michael said. “I could have used more on the harder days, but in a way it’s good we didn’t have more because it’s harder to stay awake when you have nothing to do.” (The mission included a sleep reduction study, which meant the crew only got five hours of sleep a night five days a week.) “With the time I did have, I read a lot,” he said. He also drew, kept a journal, and “wrote bad haikus.” Because of the sleep study, Ellie didn’t read as much. “For me, had I tried to read or sit and do anything not interactive, I would have fallen asleep,” she said.

The crew’s art gallery, where they hung drawing and haikus they wrote.

Journaling and drawing were popular ways to pass the time. “We developed a crew art gallery on one of the walls,” Will said. They also played board games—in particular a game where you score points by making words with lettered tiles on a 15×15 grid. (Yes that one!) “Playing [that game] with two scientists wasn’t always fun though,” Ellie joked, referencing some of the more obscure vocabulary words Will and Michael had at the ready. “I was like, ‘What does that word mean?’ ‘Well that word means lava flow,” she said laughing. (The rest of the crew assured us she fared just fine.)

Chi tried reading, but found it difficult due to the dimmed lights that were part of an onboard light study. She took on a side project instead: 1000 paper cranes. “There is a story in Japan—I’m half Japanese—that if you make a 1000 cranes, it’s supposed to grant you a wish,” she said. She gave hers to her grandmother.

The whole crew having dinner together on “Sophisticated Saturdays!” From left to right: Will, Ellie, Chi, and Michael. They’re wearing their Saturday best, which includes the usual research equipment.

On weekends, the crew got eight hours of sleep, which they celebrated with “Sophisticated Saturdays!” “Coming in, we all brought an outfit that was a little fancy,” Ellie said. (Like a tie, a vest, an athletic dress—that kind of thing.) “We would only put it on Saturday evenings, and we’d have dinner on the first level at the one and only table we could all sit at and face each other,” she said. “We would pretend it was a different fancy restaurant every week.”

The table set for a “civilized” Saturday dinner. Once the crew’s hydroponics grew, they were able to add some greenery to the table.

“It was a way to feel more civilized,” Will said, who then offered another great use of their free time: establishing good habits. “I would use the free time to journal, for example. I’d just keep it up every day. That and stretching. Hydrating. Flossing.”

Like real astronauts, you were in contact with Mission Control and further monitored by HERA personnel. Was it weird being on camera all the time?

HERA personnel and the monitors they use for a typical HERA mission.

“I was always aware of it,” Michael said, “but I don’t think it changed my behavior. It’s not like I forgot about it. It was always there. I just wasn’t willing to live paranoid for 45 days.” Ellie agreed. “It was always in the back of my mind,” she said, further adding that they wore microphones and various other sensors. “We were wired all the time,” she said.

After the study, the crew met up with the people facilitating the experiments, sometimes for the first time. “It was really fun to meet Mission Control afterwards,” Will said. “They had just been this voice coming from the little boxes. It was great getting to meet them and put faces to the voices,” he said. “Of course, they knew us well. Very well.”

For more information on HERA, visit our analogs homepage.

Make sure to follow us on Tumblr for your regular dose of space: http://nasa.tumblr.com

Why are we studying them? What’s purpose of this field for us on earth?

Solar System: 10 Things to Know This Week

Rockets We Love-Saturn V

Fifty years ago, with President Kennedy’s Moon landing deadline looming, the powerful Saturn V had to perform. And perform it did—hurling 24 humans to the Moon.

The race to land astronauts on the Moon was getting tense 50 years ago this week. Apollo 6, the final uncrewed test flight of America’s powerful Moon rocket, launched on April 4, 1968. Several technical issues made for a less-than-perfect launch, but the test flight nonetheless convinced NASA managers that the rocket was up to the task of carrying humans. Less than two years remained to achieve President John F. Kennedy’s goal to put humans on the Moon before the decade was out, meaning the Saturn V rocket had to perform.

1—“The only chance to get to the Moon before the end of 1969.”

After the April 1968 Apollo 6 test flight (pictured above), the words of Deke Slayton (one of the original Mercury 7 astronauts) and intense competition with a rival team in the Soviet Union propelled a 12-member panel to unanimously vote for a Christmas 1968 crewed mission to orbit the Moon.

2—Four Hundred Elephants...

The Saturn V rocket stood about the height of a 36-story-tall building, and 60 feet (18 meters) taller than the Statue of Liberty. Fully fueled for liftoff, the Saturn V weighed 6.2 million pounds (2.8 million kilograms), or the weight of about 400 elephants.

3—...and Busloads of Thrust

Stand back, Ms. Frizzle. The Saturn V generated 7.6 million pounds (34.5 million newtons) of thrust at launch, creating more power than 85 Hoover Dams. It could launch about 130 tons (118,000 kilograms) into Earth orbit. That's about as much weight as 10 school buses. The Saturn V could launch about 50 tons (43,500 kilograms) to the Moon. That's about the same as four school buses.

4—Christmas at the Moon

On Christmas Eve 1968, the Saturn V delivered on engineers’ promises by hurling Frank Borman, Jim Lovell and Bill Anders into lunar orbit. The trio became the first human beings to orbit another world. The Apollo 8 crew broadcast a special holiday greeting from lunar orbit and also snapped the iconic earthrise image of our home planet rising over the lunar landscape.

5—Gumdrop and Spider

The crew of Apollo 9 proved that they could pull the lunar module out of the top of the Saturn V’s third stage and maneuver it in space (in this case high above Earth). The crew named their command module “Gumdrop.” The Lunar Module was named “Spider.”

6—The Whole Enchilada

Saturn-V AS-505 provided the ride for the second dry run to the Moon in 1969. Tom Stafford, Gene Cernan and John Young rode Command Module “Charlie Brown” to lunar orbit and then took Lunar Module “Snoopy” on a test run in lunar orbit. Apollo 10 did everything but land on the Moon, setting the stage for the main event a few months later. Young and Cernan returned to walk on the Moon aboard Apollo 16 and 17 respectively. Cernan, who died in 2017, was the last human being (so far) to set foot on the Moon.

7—The Main Event

The launch of Apollo 11—the first mission to land humans on the Moon—provided another iconic visual as Saturn-V AS-506 roared to life on Launch Pad 39A at Kennedy Space Center in Florida. Three days later, Neil Armstrong and Buzz Aldrin made the first of many bootprints in the lunar dust (supported from orbit by Michael Collins).

8—Moon Men

Saturn V rockets carried 24 humans to the Moon, and 12 of them walked on its surface between 1969 and 1972. Thirteen are still alive today. The youngest, all in their early 80s, are moonwalkers Charles Duke (Apollo 16) and Harrison Schmitt (Apollo 17) and Command Module Pilot Ken Mattingly (Apollo 16, and also one of the heroes who helped rescue Apollo 13). There is no single image of all the humans who have visited the Moon.

9—The Flexible Saturn V

The Saturn V’s swan song was to lay the groundwork for establishing a permanent human presence in space. Skylab, launched into Earth orbit in 1973, was America’s first space station, a precursor to the current International Space Station. Skylab’s ride to orbit was a Saturn IV-B 3rd stage, launched by a Saturn 1-C and SII Saturn V stages.

This was the last launch of a Saturn V, but you can still see the three remaining giant rockets at the visitor centers at Johnson Space Center in Texas and Kennedy Space Center in Florida and at the United States Space and Rocket Center in Alabama (near Marshall Space Flight Center, one of the birthplaces of the Saturn V).

10—The Next Generation

The Saturn V was retired in 1973. Work is now underway on a fleet of rockets. We are planning an uncrewed flight test of Space Launch System (SLS) rocket to travel beyond the Moon called Exploration Mission-1 (EM-1). “This is a mission that truly will do what hasn’t been done and learn what isn’t known,” said Mike Sarafin, EM-1 mission manager at NASA Headquarters in Washington.

Read the web version of this 10 Things to Know article HERE. 

Make sure to follow us on Tumblr for your regular dose of space: http://nasa.tumblr.com