Sounding Rocket Science In The Arctic

Sounding Rocket Science in the Arctic

We sent three suborbital sounding rockets right into the auroras above Alaska on the evening of March 1 local time from the Poker Flat Research Range north of Fairbanks, Alaska.  

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Sounding rockets are suborbital rockets that fly up in an arc and immediately come back down, with a total flight time around 20 minutes. 

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Though these rockets don’t fly fast enough to get into orbit around Earth, they still give us valuable information about the sun, space, and even Earth itself. Sounding rockets’ low-cost access to space is also ideal for testing instruments for future satellite missions.

Sounding rockets fly above most of Earth’s atmosphere, allowing them to see certain types of light – like extreme ultraviolet and X-rays – that don’t make it all the way to the ground because they are absorbed by the atmosphere. These kinds of light give us a unique view of the sun and processes in space.

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The sun seen in extreme ultraviolet light by the Solar Dynamics Observatory satellite.

Of these three rockets, two were part of the Neutral Jets in Auroral Arcs mission, collecting data on winds influenced by the electric fields related to auroras. Sounding rockets are the perfect vehicle for this type of study, since they can fly directly through auroras – which exist in a region of Earth’s upper atmosphere too high for scientific balloons, but too low for satellites.

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The third rocket that launched on March 1 was part of the ISINGLASS mission (short for Ionospheric Structuring: In Situ and Ground-based Low Altitude Studies). ISINGLASS included two rockets designed to launch into two different types of auroras in order to collect detailed data on their structure, with the hope of better understanding the processes that create auroras. The initial ISINGLASS rocket launched a few weeks earlier, on Feb. 22, also from the Poker Flat Research Range in Alaska.

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Auroras are caused when charged particles trapped in Earth’s vast magnetic field are sent raining down into the atmosphere, usually triggered by events on the sun that propagate out into space. 

Team members at the range had to wait until conditions were just right until they could launch – including winds, weather, and science conditions. Since these rockets were studying aurora, that means they had to wait until the sky was lit up with the Northern Lights.

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Regions near the North and South Pole are best for studying the aurora, because the shape of Earth’s magnetic field naturally funnels aurora-causing particles near the poles. 

But launching sensitive instruments near the Arctic Circle in the winter has its own unique challenges. For example, rockets have to be insulated with foam or blankets every time they’re taken outside – including while on the launch pad – because of the extremely low temperatures.

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For more information on sounding rockets, visit www.nasa.gov/soundingrockets.

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

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5 years ago
Say Hello To The Saturn Nebula 👋

Say hello to the Saturn Nebula 👋

Garden-variety stars like the Sun live fairly placid lives in their galactic neighborhoods, casually churning out heat and light for billions of years. When these stars reach retirement age, however, they transform into unique and often psychedelic works of art. This Hubble Space Telescope image of the Saturn Nebula shows the result, called a planetary nebula. While it looks like a piece of wrapped cosmic candy, what we see is actually the outer layers of a dying star.

Stars are powered by nuclear fusion, but each one comes with a limited supply of fuel. When a medium-mass star exhausts its nuclear fuel, it will swell up and shrug off its outer layers until only a small, hot core remains. The leftover core, called a white dwarf, is a lot like a hot coal that glows after a barbecue — eventually it will fade out. Until then, the gaseous debris fluoresces as it expands out into the cosmos, possibly destined to be recycled into later generations of stars and planets.

Using Hubble’s observations, scientists have characterized the nebula’s composition, structure, temperature and the way it interacts with surrounding material. Studying planetary nebulas is particularly interesting since our Sun will experience a similar fate around five billion years down the road.

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


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4 years ago

Hello!! Its wonderful to be able to ask questions, thank you!

About Perseverance, does it have a self-repair option? And as Curiosity is still operational, will they run missions together? Or will they split up to cover more distance?

Is this a sign that we're close to being able to set foot on Mars?

My final question is how do you receive the messages from such a long distance?

Thanks for all your hard work! 加油/Good luck!

“Is this a sign that we are close to being able to set foot on Mars?”


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5 years ago
We Are Swooningggg Over This NEW Saturn Image. 

We are swooningggg over this NEW Saturn image. 

Saturn is so beautiful that astronomers cannot resist using the Hubble Space Telescope to take yearly snapshots of the ringed world when it is at its closest distance to Earth. 😍

These images, however, are more than just beauty shots. They reveal exquisite details of the planet as a part of the Outer Planets Atmospheres Legacy project to help scientists understand the atmospheric dynamics of our solar system's gas giants.

This year's Hubble offering, for example, shows that a large storm visible in the 2018 Hubble image in the north polar region has vanished. Also, the mysterious six-sided pattern – called the "hexagon" – still exists on the north pole. Caused by a high-speed jet stream, the hexagon was first discovered in 1981 by our Voyager 1 spacecraft.

Saturn's signature rings are still as stunning as ever. The image reveals that the ring system is tilted toward Earth, giving viewers a magnificent look at the bright, icy structure. 

Image Credit: NASA, ESA, A. Simon (GSFC), M.H. Wong (University of California, Berkeley) and the OPAL Team

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5 years ago

Get Ready Stargazers: The Geminids Are Here!

The Geminid meteor shower, one of the biggest meteor showers of the year, will peak this weekend, December 13 to 14. We get a lot of questions about the Geminids—so we’ve put together some answers to the ones we’re most commonly asked. Take a look!  

What are the Geminids?

The Geminids are pieces of debris from an asteroid called 3200 Phaethon. Earth runs into Phaethon’s debris stream every year in mid-December, causing meteors to fly from the direction of the constellation Gemini – hence the name “Geminids.”  

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Image Credit: Arecibo Observatory/NASA/NSF

When is the best time to view them?

This year, the peak is during the overnight hours of December 13 and into the morning of December 14. Viewing should still be good on the night of December 14 into the early morning hours of the 15th. Weather permitting, the Geminids can be viewed from around midnight to 4 a.m. local time. The best time to see them is around 2 a.m. your local time on December 14, when the Geminid radiant is highest in your night sky. The higher the radiant – the celestial point in the sky from which meteors appear to originate – rises into the sky, the more meteors you are likely to see.

Get Ready Stargazers: The Geminids Are Here!

Image Credit & Copyright: Jeff Dai

What is the best way to see them?

Find the darkest place you can and give your eyes about 30 minutes to adapt to the dark. Avoid looking at your cell phone, as it will disrupt your night vision. Lie flat on your back and look straight up, taking in as much sky as possible. You will soon start to see the Geminid meteors!

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Image Credit: NASA/Bill Dunford

Can you see the Geminids from anywhere in the world?

The Geminids are best observed in the Northern Hemisphere, but no matter where you are in the world (except Antarctica), some Geminids will be visible.

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Image Credit: Jimmy Westlake

How many Geminids can I expect to see?

Under dark, clear skies, the Geminids can produce up to 120 meteors per hour – but this year, a bright, nearly full moon will hinder observations of the shower. Still, observers can hope to see up to 30 meteors per hour. Happy viewing!  

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Image Credit & Copyright: Yuri Beletsky

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6 years ago

NASA Science Show & Tell

This week, we’re at one of the biggest science conferences in the country, where our scientists are presenting new results from our missions and projects. It’s called the American Geophysical Union’s Fall Meeting.

Here are a few of the things we shared this week...

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The Sun

A few months into its seven-year mission, Parker Solar Probe has already flown far closer to the Sun than any spacecraft has ever gone. The data from this visit to the Sun has just started to come back to Earth, and scientists are hard at work on their analysis.

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Parker Solar Probe sent us this new view of the Sun’s outer atmosphere, the corona. The image was taken by the mission’s WISPR instrument on Nov. 8, 2018, and shows a coronal streamer seen over the east limb of the Sun. Coronal streamers are structures of solar material within the Sun's atmosphere, the corona, that usually overlie regions of increased solar activity. The fine structure of the streamer is very clear, with at least two rays visible. Parker Solar Probe was about 16.9 million miles from the Sun's surface when this image was taken. The bright object near the center of the image is Mercury, and the dark spots are a result of background correction.

Hurricane Maria

Using a satellite view of human lights, our scientists watched the lights go out in Puerto Rico after Hurricane Maria. They could see the slow return of electricity to the island, and track how rural and mountainous regions took longer to regain power.

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In the spring, a team of scientists flew a plane over Puerto Rico’s forests, using a laser instrument to measure how trees were damaged and how the overall structure of the forests had changed.

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Earth’s Ice

Our scientists who study Antarctica saw some surprising changes to East Antarctica. Until now, most of the continent’s melting has been on the peninsula and West Antarctica, but our scientists have seen glaciers in East Antarctica lose lots of ice in the last few years.

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Our ICESat-2 team showed some of their brand new data. From the changing height of Antarctic ice to lagoons off the coast of Mexico, the little satellite has spent its first few months measuring our planet in 3D. The laser pulses even see individual ocean waves, in this graph.

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Scientists are using our satellite data to track Adélie penguin populations, by using an unusual proxy -- pictures of their poop! Penguins are too small to be seen by satellites, but they can see large amounts of their poop (which is pink!) and use that as a proxy for penguin populations.

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Asteroid Bennu

Our OSIRIS-REx mission recently arrived at its destination, asteroid Bennu. On approach, data from the spacecraft’s spectrometers revealed chemical signatures of water trapped in clay minerals.  While Bennu itself is too small to have ever hosted liquid water, the finding indicates that liquid water was present at some time on Bennu’s parent body, a much larger asteroid.

We also released a new, detailed shape model of Bennu, which is very similar to our ground-based observations of Bennu’s shape. This is a boon to ground-based radar astronomy since this is our first validation of the accuracy of the method for an asteroid! One change from the original shape model is the size of the large boulder near Bennu’s south pole, nicknamed “Benben.” The boulder is much bigger than we thought and overall, the quantity of boulders on the surface is higher than expected. Now the team will make further observations at closer ranges to more accurately assess where a sample can be taken on Bennu to later be returned to Earth.

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Jupiter

The Juno mission celebrated it’s 16th science pass of #Jupiter, marking the halfway point in data collection of the prime mission. Over the second half of the prime mission — science flybys 17 through 32 — the spacecraft will split the difference, flying exactly halfway between each previous orbit. This will provide coverage of the planet every 11.25 degrees of longitude, providing a more detailed picture of what makes the whole of Jupiter tick.

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Mars

The Mars 2020 team had a workshop to discuss the newly announced landing site for our next rover on the Red Planet. The landing site...Jezero Crater! The goal of Mars 2020 is to learn whether life ever existed on Mars. It's too cold and dry for life to exist on the Martian surface today. But after Jezero Crater formed billions of years ago, water filled it to form a deep lake about the same size as Lake Tahoe. Eventually, as Mars' climate changed, Lake Jezero dried up. And surface water disappeared from the planet.

Interstellar Space

Humanity now has two interstellar ambassadors. On Nov. 5, 2018, our Voyager 2 spacecraft left the heliosphere — the bubble of the Sun’s magnetic influence formed by the solar wind. It’s only the second-ever human-made object to enter interstellar space, following its twin, Voyager 1, that left the heliosphere in 2012.

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Scientists are especially excited to keep receiving data from Voyager 2, because — unlike Voyager 1 — its plasma science instrument is still working. That means we’ll learn brand-new information about what fills the space between the stars.

Learn more about NASA Science at science.nasa.gov. 

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


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5 years ago

Hii! I'm unsure if you've been asked this before, but I'd like to give it a shot anyway. What's the greatest legacy you hope to leave to the future generations? Whether it's one of the things you've accomplished already or are hoping to accomplish yet. Thank you very much!


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3 years ago

A Beginner’s Guide to Advanced Air Mobility

A Beginner’s Guide To Advanced Air Mobility

Soaring over traffic in an air taxi, receiving packages faster, and participating in a sustainable, safer mode of transportation: all could be possible with a revolutionary new type of air transportation system in development called Advanced Air Mobility (AAM).

AAM could include new aircraft developed by industry, called electric vertical takeoff and landing vehicles, or eVTOLs, for use in passenger, package, or cargo delivery. It may also include new places for these aircraft to take off and land called vertiports.

Our work in Advanced Air Mobility will transform the way people and goods will move through the skies. This includes using Advanced Air Mobility for public good missions such as disaster, medical, and wildfire response.

What is Advanced Air Mobility?

Our vision for Advanced Air Mobility is to map out a safe, accessible, and affordable new air transportation system alongside industry, community partners, and the Federal Aviation Administration.

A Beginner’s Guide To Advanced Air Mobility

Once developed, passengers and cargo will travel on-demand in innovative, automated aircraft called eVTOLs, across town, between neighboring cities, or to other locations typically accessed today by car.  

What are the benefits of Advanced Air Mobility?

The addition of Advanced Air Mobility will benefit the public in several ways: easier access for travelers between rural, suburban, and urban communities; rapid package delivery; reduced commute times; disaster response, and new solutions for medical transport of passengers and supplies.

A Beginner’s Guide To Advanced Air Mobility

What are the challenges associated with Advanced Air Mobility?

Various NASA simulation and flight testing efforts will study noise, automation, safety, vertiports, airspace development and operations, infrastructure, and ride quality, along with other focus areas like community integration.

These areas all need to be further researched before Advanced Air Mobility could be integrated into our skies. We’re helping emerging aviation markets navigate the creation of this new transportation system.

When will Advanced Air Mobility take off?

We provide various test results to the FAA to help with new policy and standards creation. We aim to give industry and the FAA recommendations for requirements to build a scalable Advanced Air Mobility system to help enable the industry to flourish by 2030.

A Beginner’s Guide To Advanced Air Mobility

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9 years ago

It’s a U.S. Record! Cumulative Days in Space: 383

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Today, Astronaut Scott Kelly has broken the record for longest time spent in space by a U.S. astronaut! Over the course of his four missions, Kelly has spent 383 cumulative days in space. This record was previously held by Astronaut Mike Fincke, with 382 days in space over three flights. Here are some more fun facts about this milestone:

4: The number of humans that have spent a year or more in orbit on a single mission

215 Days: The record currently held by Mike Lopez-Alegria for most time on a single spaceflight by U.S. astronaut. On Oct. 29, Kelly will break this record

377 Days: The current record for most days in space by a U.S. female astronaut, held by Peggy Whitson

879 Days: The record for most cumulative days in space by a human, currently held by Russian cosmonaut Gennady Padalka

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Why Spend a Year in Space?

Kelly’s One-Year Mission is an important stepping stone on our journey to Mars and other deep space destinations. These investigations are expected to yield beneficial knowledge on the medical, psychological and biomedical challenges faced by astronauts during long-duration spaceflight.

Kelly is also involved in the Twins Study, which consists of ten separate investigations that are being conducted with his twin brother, who is on Earth. Since we are able to study two individuals who have the same genetics, but are in different environments for one year, we can gain a broader insight into the subtle effects and changes that may occur in spaceflight.

For regular updates on Kelly’s one-year mission aboard the space station, follow him on social media: Facebook, Twitter, Instagram.

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


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8 years ago

10 Space & Football Facts You Probably Didn’t Know

There are more connections between space and football than you may have originally thought. Here are a few examples of how...

1. The International Space Station and a football field are basically the same size

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Yes, that’s right! The International Space Station measures 357 feet end-to-end. That’s almost equivalent to the length of a football field including the end zones (360 feet).

2. It would take over 4,000 footballs to fill the Orion spacecraft

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Our Orion spacecraft is being designed to carry astronauts to deep space destinations, like Mars! It will launch atop the most powerful rocket ever built, the Space Launch System rocket. If you were to fill the Orion spacecraft with footballs instead of crew members, you would fit a total of 4,625!

3. Our new Space Launch System rocket is taller than a football field is long

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We’re building the most powerful rocket ever, the Space Launch System. At its full height it will stand 384 feet – 24 feet taller than a football field is long.

4. The crew living on space station will see the day begin and end…twice…during the Super Bowl

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An average NFL game lasts more than three hours. Traveling at 17,500 mph, the crew on the space station will see two sunrises and two sunsets in that time…they see 16 sunrises and sunsets each day!

5. Playing football on Mars would be…lighter

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On Mars, a football would weigh less than half a pound, while a 200-pund football player would weigh just about 75 pounds.

6. It would take over 3,000 hours for a football to reach the Moon

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Talk about going long…if you threw a football to the Moon at 60 mph, the average speed of an NFL pass, it would take 3,982 hours, or 166 days, to get there. The quickest trip to the Moon was the New Horizons probe, which zipped pass the Moon in just 8 hours 35 minutes on its way to Pluto 

7. The longest field goal kick in history would’ve been WAY easier to make on Mars

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The longest field goal kick in NFL history is 64 yards. On Mars, at 1/3 the gravity of Earth, that same field goal, ignoring air resistance, could have been made from almost two football fields away (192 yards).

8. A quarterback would be able to throw even further on Mars

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Aerodynamic drag doesn’t happen on Mars. With a very thin atmosphere and low gravity to drag the ball down, a quarterback could throw the football three times as far as he could on Earth. A receiver would have to be much further down the field to catch the throw 

9. Football players and astronauts both need to exercise every day

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Football players must be quick and powerful, honing the physical skills necessary for their unique positions. In space, maintaining physical fitness is a top priority, since astronauts will lose bone and muscle mass if they do not keep up their strength and conditioning.

10. Clear team communication is important on the football field AND in space

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During football games, calling plays and relaying information from coaches on the sidelines or in the booth to players on the field is essential. Coaches communicate directly with quarterbacks and a defensive player between plays via radio frequencies. They must have a secure and reliable system that keeps their competitors from listening in and also keeps loud fan excitement from drowning out what can be heard. Likewise, reliable communication with astronauts in space and robotic spacecraft exploring far into the solar system is key to our mission success.

A radio and satellite communications network allows space station crew members to talk to the ground-based team at control centers, and for those centers to send commands to the orbital complex.

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


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6 years ago

Blowing Bubbles in the Gamma-ray Sky

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Did you know our Milky Way galaxy is blowing bubbles? Two of them, each 25,000 light-years tall! They extend above and below the disk of the galaxy, like the two halves of an hourglass. We can’t see them with our own eyes because they’re only apparent in gamma-ray light, the highest-energy light in the universe.

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We didn’t even know these humongous structures were smack in the middle of our galaxy until 2010. Scientists found them when they analyzed the first two years of data from NASA’s Fermi Gamma-ray Space Telescope. They dubbed them the “Fermi bubbles” and found that in addition to being really big and spread out, they seem to have well-defined edges. The bubbles’ shape and the light they give off led scientists to think they were created by a rapid release of energy. But by what? And when?

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One possible explanation is that they could be leftovers from the last big meal eaten by the supermassive black hole at the center of our galaxy. This monster is more than 4 million times the mass of our own Sun. Scientists think it may have slurped up a big cloud of hydrogen between 6 and 9 million years ago and then burped jets of hot gas that we see in gamma rays and X-rays.

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Another possible explanation is that the bubbles could be the remains of star formation. There are massive clusters of stars at very the center of the Milky Way — sometimes the stars are so closely packed they’re a million times more dense than in the outer suburb of the galaxy where we live. If there was a burst of star formation in this area a few million years ago, it could have created the surge of gas needed to in turn create the Fermi bubbles.

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It took us until 2010 to see these Fermi bubbles because the sky is filled with a fog of other gamma rays that can obscure our view. This fog is created when particles moving near light speed bump into gas, dust, and light in the Milky Way. These collisions produce gamma rays, and scientists had to factor out the fog to unveil the bubbles.

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Scientists continue to study the possible causes of these massive bubbles using the 10 years of data Fermi has collected so far. Fermi has also made many other exciting discoveries — like the the collision of superdense neutron stars and the nature of space-time. Learn more about Fermi and how we’ve been celebrating its first decade in space.

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