The Birth Of A New Island

The Birth of a New Island

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In late December 2014, an underwater volcano in the South Pacific Kingdom of Tonga erupted and sent a violent stream of steam, ash and rock into the air. The ash plumes rose as high as 30,000 feet (9 kilometers) into the sky and diverted airline flights.

Most new oceanic islands often wash away quickly within a few months. The island doesn't have an official name, and is referred to as Hunga Tonga-Hunga Ha'apai after two older islands to either side.

But this island was different. One of our satellites that detects volcanic eruptions alerted our scientists who were very excited because this type of explosive, undersea eruption is rare. In fact, the new Tongan island is one of only three of this kind of volcanic islands in the past 150 years to emerge and survive. It's now three years old.

Zooming in from Space

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The baby island is also the first of its kind to emerge in the modern satellite era. This is really important since it's difficult to send our researchers the South Pacific every month to see how the island has changed – which it did very rapidly, especially in the first six months. But satellites in space delivered monthly views which we used to make these high resolution, 3-D topographic maps. With these maps, we tracked the early life and evolution of the island in unprecedented detail.

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In April 2015, we watched an isthmus bridge begin forming from the new island to the older island neighboring it to the east. Soft volcanic material, especially on the island's southern side, was eroded by the ocean and deposited on the tail end, which grew and grew till it reached the other island. It's about 1600 feet (500 meters) across, or the length of 5 football fields.

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The erosive forces of the ocean broke down the southern wall of the crater lake in May 2015. We thought this might mean that the island wouldn't last much longer because the ocean could now attack the interior of the island's tuff cone. But in June, a sandbar formed, closing off the lake again and protecting the interior. The sandbar has been in place ever since.

Monitoring these changes of both erosion and growth, we now believe that the island will last from between 6 to 30 years!

Terranauts!

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Why has the island survived for three years? What makes eroding it away harder than for other blink-and-you-miss-it oceanic islands that disappear into the sea after a few months? To answer these questions, we need rock samples.

Working with the Tongan government, we recruited two French citizens sailing around the world who were in Tongan waters in June, 2017, to go to the new island on our behalf. We treated them like astronauts and gave them instructions to take pictures and samples of the volcanic rocks at locations we could see from space along the coasts, the interior of the crater lake, and from the top of the tuff cone.

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They did a fantastic job documenting each sample and where it came from, and then mailed the box of rocks back to our team at our Goddard Space Flight Center in Greenbelt, Maryland, where they are currently being analyzed. We believe that after the eruption, warm seawater mixed with volcanic ash to chemically alter it so that when it hardened into rock it was a tougher material. We're excited to see if the rock samples confirm this.

From Earth to Mars

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Link: https://svs.gsfc.nasa.gov/11372

Did these Martian volcanoes form in an ocean or lake? If they did, wet environments such as these combined with heat from volcanic processes may be prime locations to search for evidence of past life. We may not know until we arrive on the red planet, but by studying Earth's landforms, we'll be better prepared when we do.

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More Posts from Nasa and Others

9 years ago

Holiday Lights...In Space

Holiday lights don’t come in one shape or size, just like they don’t only appear on Earth. Take a look at a few of these celestial light shows:

1. Galactic Wreath of Lights

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This festive image captured by our Hubble Space Telescope resembles a holiday wreath made of sparkling lights. This galactic wreath is located around 6,500 light-years away.

2. Red and Green Aurora

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This beautiful aurora was captured by Astronaut Scott Kelly while aboard the International Space Station. He shared it with his Twitter followers on June, 22 during his Year in Space mission. This image of Earth’s aurora is festive with its red and green lights.

3. Holiday Snow Angel

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Our Hubble Space Telescope captured this stunning image of what looks like a soaring, celestial snow angel. This picture shows a bipolar star-forming region, called Sharpless 2-106.

4. Cosmic Holiday Ornament

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This festive-looking nearby planetary nebula resembles a glass-blown holiday ornament with a glowing ribbon entwined. This cosmic decoration was spotted by our Hubble Space Telescope.

5. Holiday Lights on the Sun

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Even the sun gets festive with it’s festive looking solar flares. This significant flare was seen by our Solar Dynamics Observatory (SOHO) on Dec. 19, 2014. Even though solar flares are powerful bursts of radiation, it cannot pas through Earth’s atmosphere to physically affect humans on the ground. That said, when intense enough, the radiation can disturb the atmosphere in the layer where GPS and communications signals travel.

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


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9 years ago

What Did Astronaut Scott Kelly Do After a #YearInSpace?

Astronaut Scott Kelly just returned from his One-Year Mission aboard the International Space Station. After spending 340 days on orbit, you can imagine that he started to miss a few Earthly activities. Here are a few things he did after his return home:

Watched a Sunset

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While on the International Space Station for his One-Year Mission, astronaut Scott Kelly saw 16 sunrises/sunsets each day...so he definitely didn’t miss out on the beauty. That said, watching a sunset while on Earth is something that he had to wait to see. Tweet available HERE. 

Ate Fresh Food

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After spending a year on the International Space Station, eating precooked food, anyone would be excited to dig into a REAL salad. Astronaut Scott Kelly was no exception, and posted about his first salad on Earth after his one-year mission. Learn more about what astronauts eat while in space HERE. Tweet available HERE.

Jumped into a Pool

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Water is a precious resource in space. Unfortunately, that means that there isn’t a pool on the space station. Luckily, astronaut Scott Kelly was able to jump into some water after his return to Earth. Tweet/video available HERE.

Sat at a Dinner Table

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While living on the International Space Station, crew members regularly enjoy their meals together, but do so while floating in microgravity. The comfort of pulling up a chair to the dinner table is something they can only experience once they’re back home on Earth. Tweet available HERE.

Enjoyed the Weather

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When crew members live on the space station they can’t just step outside for a stroll. The only time they go outside the orbiting laboratory is during a spacewalk. Even then, they are confined inside a bulky spacesuit. Experiencing the cool breeze or drops of rain are Earthly luxuries. Tweet available HERE.

Stopped by the Doctor’s Office

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The One-Year Mission doesn’t stop now that astronaut Scott Kelly is back on Earth. Follow-up exams and tests will help scientists understand the impacts of microgravity on the human body during long-duration spaceflight. This research will help us on our journey to Mars. Tweet available HERE. 

Visited the Denist

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When you spend a year in space, you’ll probably need to catch up on certain things when you return to Earth. Astronaut Scott Kelly made sure to include a visit to the dentist on his “return home checklist”. Tweet available HERE.

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


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5 years ago

Swift: Our Sleuth for the Universe’s Gamma-ray Bursts

The universe is full of mysteries, and we continue to search for answers. How can we study matter and energy that we can’t see directly? What’s it like inside the crushed core of a massive dead star? And how do some of the most powerful explosions in the universe evolve and interact with their surrounding environment? 

Luckily for us, NASA’s Neil Gehrels Swift Observatory is watching the skies and helping astronomers answer that last question and more! As we celebrate its 15-year anniversary, let’s get you up to speed about Swift.

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What are gamma-ray bursts and why are they interesting?

Gamma-ray bursts are the most powerful explosions in the universe. When they occur, they are about a million trillion times as bright as the Sun. But these bursts don’t last long — from a few milliseconds (we call those short duration bursts) to a few minutes (long duration). In the 1960s, spacecraft were watching for gamma rays from Earth — a sign of nuclear testing. What scientists discovered, however, were bursts of gamma rays coming from space!

Gamma-ray bursts eventually became one of the biggest mysteries in science. Scientists wanted to know: What events sparked these fleeting but powerful occurrences?

So how do gamma-ray bursts and Swift connect?

When it roared into space on a rocket, Swift’s main goals included understanding the origin of gamma-ray bursts, discovering if there were additional classes of bursts (besides the short and long ones), and figuring out what these events could tell us about the early universe.

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With Swift as our eyes on the sky, we now know that gamma-ray bursts can be some of the farthest objects we’ve ever detected and lie in faraway galaxies. In fact, the closest known gamma-ray burst occurred more than 100 million light-years from us. We also know that these explosions are associated with some of the most dramatic events in our universe, like the collapse of a massive star or the merger of two neutron stars — the dense cores of collapsed stars.

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Swift is still a powerful multiwavelength observatory and continues to help us solve mysteries about the universe. In 2018 it located a burst of light that was at least 10 times brighter than a typical supernova. Last year Swift, along with NASA’s Fermi Gamma-ray Space Telescope, announced the discovery of a pair of distant explosions which produced the highest-energy light yet seen from gamma-ray bursts.

Swift can even study much, much closer objects like comets and asteroids!

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Why is Swift unique?

How do we study events that happen so fast? Swift is first on the scene because of its ability to automatically and quickly turn to investigate sudden and fascinating events in the cosmos. These qualities are particularly helpful in pinpointing and studying short-lived events.

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The Burst Alert Telescope, which is one of Swift’s three instruments, leads the hunt for these explosions. It can see one-sixth of the entire sky at one time. Within 20 to 75 seconds of detecting a gamma-ray burst, Swift automatically rotates so that its X-ray and ultraviolet telescopes can view the burst.

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Because of the “swiftness” of the satellite, it can look at a lot in 24 hours — between 50 and 100 targets each day! Swift has new “targets-of-opportunity” to look at every day and can also look at objects for follow up observations. By doing so, it can see how events in our cosmos change over time.

How did Swift get its name?

You may have noticed that lots of spacecraft have long names that we shorten to acronyms. However, this isn’t the case for Swift. It’s named after the bird of the same name, and because of the satellite’s ability to move quickly and re-point its science instruments.

When it launched, Swift was called NASA’s Swift Observatory. But in January 2018, Swift was renamed the Neil Gehrels Swift Observatory in memory of the mission’s original principal investigator, Neil Gehrels.

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Follow along with Swift to see a typical day in the life of the satellite:


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1 year ago
NASA astronaut Deniz Burnham, a white woman, poses for a portrait at NASA's Johnson Space Center in Houston, Texas. She looks directly into the camera as the light highlights her blonde hair. Credit: NASA/Josh Valcarcel

Deniz Burnham

A former NASA intern, Deniz Burnham started her career as an engineer on an oil rig in Prudhoe Bay, Alaska, and went on to lead operations on drilling rigs in Canada, Ohio, and Texas. https://go.nasa.gov/3wDpfBo

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


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7 years ago

Tracking a Warming Arctic – From Underground to High in the Sky

The Arctic is warming much faster than the rest of Earth. This warming is creating big and small changes, some of which could ripple beyond the planet’s frozen regions and affect us world-wide – possibly raising sea levels, increasing greenhouse warming and affecting wildlife.

Our Arctic Boreal Vulnerability Experiment, known as ABoVE, just began a 10-year mission in Alaska and western Canada, studying these changes.

Underground: Permafrost is the layer of frozen soil beneath some Arctic forests and tundra. 

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Like the name suggests, this icy layer stays solid year-round, so when it does melt, it can create big problems. The soil above the thawing permafrost can collapse, creating this wobbly, unstable surface.

7 feet above sea level: As the permafrost thaws, the soil above it can fall away. 

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Along the banks of the Itkillik River in Alaska, thawing permafrost has dripped into the water, eroding the cliff side. Known as the “Stinky Bluffs,” this permafrost contains lots of frozen organic matter from dead plants and animals. As the permafrost thaws, this organic matter doesn’t just smell, it also releases carbon dioxide and methane into the atmosphere, adding to the warming effect.

446 feet above sea level: Wildfires aren’t unusual in the forests and shrub lands of Alaska, but as the climate continues to warm, they burn longer and do more damage. 

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People who live off the land in the region help researchers understand where plant life isn’t growing back after fires.

100-1000 feet above sea level: Researchers set up 100-foot tall towers at strategic locations throughout Alaska to measure carbon dioxide and methane emissions from right above the forest canopy. 

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This provides an up-close look at what gases are released or absorbed from the trees, or swirl in from neighboring regions. These data are combined with measurements taken from airplanes and satellites to create a clearer picture of how much carbon is entering the atmosphere.

3,369 feet above sea level: Dall sheep live in several Alaskan mountain ranges, where they’re critical to both the tourism and sports hunting economies. 

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Credit: National Park Service

Changes in temperature and vegetation can profoundly affect their behavior, like grazing habits, and so researchers study how changing plant life and snow cover affect the sheep.

100-30,000 feet above sea level: Carbon emissions in the air come from thawing permafrost, fossil fuel burning, decaying vegetation and wildfires burning across the Arctic-boreal regions. 

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One experiment in the ABoVE campaign measures these emissions with instruments on a DC-8 plane.

About 30,000 feet about sea level: When wildfires burn through vegetation, the effects extend far beyond what we see on the ground. 

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Fires release carbon stored in the plants into the atmosphere, where it affects air quality and contributes to the greenhouse effect.

438 miles: Our ABoVE campaign combines research on the ground and from planes with data collected by a fleet of Earth-observing satellites, orbiting Earth hundreds of miles above the surface. 

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Data from these satellites provides information on vegetation, atmospheric particles and gasses, and how humans are impacting our planet. With all these data sets analyzed by computer programs, the result is a comprehensive picture of our warming planet.

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3 years ago

Questions coming up from….

@monicagellar: Is it open for international students?

@Anonymous: How should high school students get involved?

@Anonymous: Can I apply if my subjects are physics and chemistry in college

@unsuspicious-nobody: Do you have plans to repeat this/do something similar for students in the future?


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9 years ago

Solar System: 10 Things to Know This Week

Real-life space travel across the solar system’s vast expanse is not for the impatient – it can take many years to reach a destination. The positive side is that our hardy robots are well engineered to take the abuse that the harsh space environment dishes out. This means they can return good science over the course of many years, sometimes for decades.

This week, we take a look at a few of our longest-lived planetary missions. All of them have been returning deep space dispatches to Earth for more than five years. Combined, their flight time adds up to more than a century and a half. The legacy of their exploration is likely to endure even longer.

1. Lunar Reconnaissance Orbiter (LRO) - Launched June 18, 2009

Solar System: 10 Things To Know This Week

LRO captures crystal-clear views of the lunar landscape on almost a daily basis – and has been doing it for years. Thanks to LRO, we’ve nearly mapped the entire surface now at very high resolution. Learn more about LRO HERE.

2. Dawn – Launched Sept. 27, 2007

Solar System: 10 Things To Know This Week

The Dawn mission has been exploring the dwarf planet Ceres for just over a year now — but the Dawn spacecraft’s journey began long before that. After a trek from Earth to the asteroid belt, it made a stop at the giant asteroid Vesta before moving on to Ceres.

3. New Horizons – Launched Jan. 19, 2006

Solar System: 10 Things To Know This Week

With its ongoing discoveries based on the July 2015 Pluto flyby, the New Horizons mission is in the news all the time. It’s easy to forget the mission is not new — the spacecraft has been traversing the dark of space for more than a decade. New Horizons is now more than 3 billion miles (5 billion km) from Earth as it delves deeper into the outer solar system.

4. Mars Reconnaissance Orbiter (MRO) – Launched Aug. 12, 2005

Solar System: 10 Things To Know This Week

MRO recently marked a decade of returning spectacular images from Mars, in many more colors than just red. Peruse 10 years of MRO discoveries at Mars HERE.

5. Cassini – Launched Oct. 15, 1997

Solar System: 10 Things To Know This Week

As it circles through the Saturn system, the Cassini spacecraft is currently about 975 million miles (1.57 billion km) from Earth, but its total odometer reads much more than that. This long, spectacular mission is slated to end next year. In the meantime, it’s about to enter the “Grande Finale” stage.

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


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8 years ago

NASA and Star Trek

Star Trek debuted in September 1966 and in its various incarnations, the series has been an inspiration to many, even some of us at NASA. The series allowed its fans to explore “strange new worlds” and to dream of what could be right in their living rooms. To celebrate the show’s 50th anniversary, we’ve collected some Trek-themed photos featuring Star Trek cast members and NASA astronauts. 

Serious Business

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The STS-54 crew of the space shuttle Endeavour in their official "gag" photo are costumed as the bridge crew of the Enterprise as depicted in the movie "Star Trek II: The Wrath of Khan.” The photo was taken on the Star Trek Adventure set of the Universal Studios California theme park in Los Angeles, California, while the crew was on a west coast training and public relations tour during the Summer of 1992. From left to right: 

Greg Harbaugh (Mission Specialist/Engineering Officer)

Mario "Spock" Runco Jr. (Mission Specialist/1st Officer/Science Officer) 

John Casper (Commander/Captain) 

Susan Helms (Mission Specialist/Communications Officer) 

Don McMonagle (Pilot/Navigation-Helm Officer) 

“I have been, and always shall be, your friend”

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Astronaut John Creighton shows the on board Graphical Retrieval Information Display (GRID) computer, which displays a likeness of Mr. Spock aboard STS-051G, June 18, 1985.

“A Keyboard. . . How Quaint”

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Actor James Doohan (who played engineering genius Montgomery Scott in Star Trek) sits in the commanders seat of the Full Fuselage Trainer while astronaut Mario Runco explains the control panel during a tour of Johnson Space Center on Jan. 18, 1991. 

“You Wanted Excitement, How's Your Adrenaline?”

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Actress Nichelle Nichols (Uhura in Star Trek) toured Johnson Space Center in Houston on March 4, 1977, while Apollo 12 lunar module pilot and Skylab II commander Alan Bean showed her what it felt like inside the Lower Body Negative Pressure Device and showed her how the Shuttle Procedures Simulator operated. 

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Nichols paid us another visit in 2012 and 2015 with the Space Traveling Museum. 

Infinite Diversity, Infinite Combinations

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European Space Agency astronaut Samantha Cristoforetti gave the Vulcan salute aboard the International Space Station shortly after the passing of Leonard Nimoy on Feb. 28, 2015. She commented on Tweeter: " ‘Of all the souls I have encountered.. his was the most human.’ Thx @TheRealNimoy for bringing Spock to life for us"

Live Long And Prosper

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While visiting Johnson Space Center in Houston, TX, George Takei (Hikaru Sulu on the original series) had the chance to exchange Vulcan salutes with Robonaut on May 29, 2012. 

“Let’s See What’s Out There”

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Scott Bakula, who played Captain Jonathan Archer on Star Trek: Enterprise, stands with astronauts Terry Virts and Mike Fincke on set. The two astronauts made guest appearances on the series finale episode “These Are The Voyages . . .” March 2005.

Boldly Going For Real

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Above is the crew of STS-134, the next to last shuttle mission, in their version of the 2009 Star Trek movie poster. 

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The crew of Expedition 21 aboard the International Space Station also made a Trek-themed poster in 2009, wearing uniforms from Star Trek: The Next Generation with the Enterprise NX-01 silhouette in the background.

Learn more about Star Trek and NASA.

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


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8 years ago

Solar System: Things to Know About the August Eclipse

We’re counting down until the August 21 total solar eclipse that will be visible across most of North America. Here are some things you can do to prepare.

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1. Find A Spot 

The eclipse should be visible to some extent across the continental U.S. Here’s map of its path.

Our eclipse page can help you find the best viewing locations by longitude and latitude: eclipse.gsfc.nasa.gov/SEgoogle/SEgoogle2001/SE2017Aug21Tgoogle.html

2. Citizen Science

Want to know more about citizen science projects? Find a list of citizen science projects for the eclipse: https://eclipse.aas.org/resources/citizen-science

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3. Never look directly at the sun! Even during the early phases of the eclipse!

Get your eclipse viewing safety glasses beforehand: eclipse2017.nasa.gov/safety

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4. Get Our Interactive Eclipse Module App

In this interactive, 3D simulation of the total eclipse on August 21, 2017, you can see a view of the eclipse from anywhere on the planet: 

http://eyes.jpl.nasa.gov/eyes-on-eclipse.html

5. Got questions? 

Join the conversation on social media. Tag your posts: #Eclipse2017.

Twitter: @NASASolarSystem, @NASA, @NASASunEarth Facebook: NASA Solar System

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

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8 years ago

Five Things to Know About NASA Astronaut Kate Rubins

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Among the newest crew on the International Space Station is U.S. astronaut Kate Rubins, who will assume the role of Flight Engineer for Expeditions 48 and 49. Here are five things you should know about her:

1. She was chosen from a pool of over 3,500 applicants to receive a spot on our 2009 astronaut training class.

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After being selected, Rubins spent years training at Johnson Space Center to become an astronaut. She learned how to use the complex station systems, perform spacewalks, exercise in space and more. Some training even utilized virtual reality.

2. She has a degree in cancer biology.

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After earning a Bachelor of Science degree in Molecular Biology from the University of California, San Diego in 1999, Rubins went on to receive a doctorate in Cancer Biology from Stanford University Medical School Biochemistry Department and Microbiology and Immunology Department in 2005. In other words, she’s extremely smart.

3. Her research has benefited humanity.

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Rubins helped to create therapies for Ebola and Lassa viruses by conducting research collaboratively with the U.S. Army. She also aided development of the first smallpox infection model with the U.S. Army Medical Research Institute of Infectious Diseases and the Centers for Disease Control and Prevention. NBD. It will be exciting to see the research come out of a mission with a world-class scientist using a world-class, out-of-this-world laboratory!

4. She is scheduled to be the first person to sequence DNA in space.

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During her time at the space station, Rubins will participate in several science experiments. Along with physical science, Earth and space science and technology development work, she will conduct biological and human research investigations. Research into sequencing the first genome in microgravity and how the human body’s bone mass and cardiovascular systems are changed by living in space are just two examples of the many experiments in which Rubins may take part.

5. In her spare time, she enjoys scuba diving and triathlons...among other things.

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Rubins was on the Stanford Triathlon team, and also races sprint and Olympic distance. She is involved with health care/medical supply delivery to Africa and started a non-profit organization to bring supplies to Congo. Her recent pursuits involve flying airplanes and jumping out of them -- not simultaneously. 

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Rubins is scheduled to arrive at the International Space Station at 12:12 a.m. Saturday, July 9. After her launch on Wednesday, July 6, the three crew members traveled 2 days before docking to the space station’s Rassvet module. 

Watch live coverage of docking and their welcoming starting at 11:30 p.m. EDT Friday, July 8 on NASA Television.

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


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