NASA’s Fleet Of Planet-hunters And World-explorers

How had your background in the US Air Force as a flight test engineer prepare you for the challenges and demands of being an astronaut?

So you want to work at NASA?

An out of this world career or internship might not be as far out of reach as you think. Check out all the ways you can get involved!

If you’re a student…

Our internships are the perfect place to start! We offer paid internships for spring, summer, and fall semesters to U.S. citizens currently attending an accredited university full time. Learn more at: https://intern.nasa.gov

Seriously considering a job in the Federal civil service? Check out the Pathways Internship Program which allows you to do multiple work tours while you finish school: http://nasajobs.nasa.gov/studentopps/employment/iep.htm

If you’re a recent graduate…

If you’re a U.S. citizen who has graduated from an accredited college or university within the past 2 years (or 6 if you have served in the military), then the our Recent Graduates program is just for you. Accepted applicants are placed in a 1 year career development program with the possibility of an additional year, or even granted term or permanent jobs within the agency. Learn more at: http://nasajobs.nasa.gov/studentopps/employment/rgp.htm.

If you’re a professional…

You can search for our job openings any time at USAJobs.com. Create an account, then use the USAJobs resume builder. Want to make sure your resume maximizes your opportunity for a job at NASA? Check out our Applicant Guide: https://applyonline.nasa.gov/applicant_guide.html.

You can then search for our job openings here: https://nasai.usajobs.gov/.

If you want to be an astronaut…

Astronaut candidate applications are accepted every few years- including right now! Get yours in before the current application closes on February 18, 2016.

Do you have a bachelor’s degree in a STEM field and 3 years of related professional experience? You might be eligible. Find out more and apply online at: https://nasai.usajobs.gov/GetJob/ViewDetails/423817000.

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Counting Down to the Solar Eclipse on August 21

On Aug. 21, 2017, everyone in North America will have the chance to see a solar eclipse if skies are clear. We’re giving you a preview of what you’ll see, how to watch and why scientists are particularly excited for this eclipse.

On Aug. 21, within a narrow band stretching from Oregon to South Carolina – called the path of totality – the Moon will completely obscure the Sun, giving people on the ground a view of the total solar eclipse. Outside this path – throughout North America, and even in parts of South America – the Moon will block only a portion of the Sun’s face, creating a partial solar eclipse.

Image credit: T. Ruen

Eclipses happen when the Moon, Sun and Earth line up just right, allowing the Moon to cast its shadow on Earth. Because the Moon’s orbit is tilted with respect to the Sun-Earth plane, its shadow usually passes above or below Earth. But when they all line up and that shadow falls on Earth, we get a solar eclipse.

How to Watch the Eclipse Safely  

It’s never safe to look directly at the un-eclipsed or partially eclipsed Sun – so you’ll need special solar viewing glasses or an indirect viewing method, like pinhole projection, to watch at the eclipse.

If you’re using solar viewing glasses or a handheld solar filter, there are a few important safety tips to keep in mind:

Check a few key characteristics to make sure that you have proper solar filters – sunglasses (even very dark ones) or homemade filters are NOT safe  

Double-check that your solar filter is not scratched or damaged before you use it

Always put your solar filter over your eyes before looking up at the Sun, and look away from the Sun before removing it 

Do NOT use your solar filter while looking through telescopes, binoculars, or any other optical device, such as a camera viewfinder – the concentrated solar rays will damage the filter and enter your eyes, causing serious injury

Get all the details on safety at eclipse2017.nasa.gov/safety.

No solar viewing glasses? Pinhole projection is an easy and safe way to watch the eclipse. You can create a pinhole projector from a box, or simply use any object with tiny holes – like a colander or a piece of cardstock with a hole – to project an image of the Sun onto the ground or a piece of paper.

If you are in the path of totality, there will come a time when the Moon completely obscures the Sun’s bright face. This is called totality, and it is only during this phase – which may last only a few seconds, depending on your location – that it is safe to look directly at the eclipse.

Wherever you are, you can tune into nasa.gov/eclipselive throughout the day on Aug. 21 to hear from our experts and see the eclipse like never before – including views from our spacecraft, aircraft, and more than 50 high-altitude balloons.

A Unique Chance for Scientists

Total solar eclipses provide a unique opportunity to study the Sun and Earth. During a total eclipse, the lower parts of the Sun's atmosphere, or corona, can be seen in a way that cannot completely be replicated by current human-made instruments.

The lower part of the corona is key to understanding many processes on the Sun, including why the Sun’s atmosphere is so much hotter than its surface and the origins of the Sun’s constant stream of solar material and radiation – which can cause changes in the nature of space and impact spacecraft, communications systems, and orbiting astronauts.

Photo credit: S. Habbal, M. Druckmüller and P. Aniol

For those in the path of totality, the few moments of the total solar eclipse will reveal the Sun’s atmosphere, the corona. 

Total solar eclipses are also a chance to study Earth under uncommon conditions: In contrast to the global change in light that occurs every day at dusk and dawn, a solar eclipse changes illumination of Earth and its atmosphere only under a comparatively small region of the Moon’s shadow. This localized blocking of solar energy is useful in evaluating our understanding of the Sun’s effects – temperature, for example – on our atmosphere. Of particular interest is the impact on Earth’s upper atmosphere, where solar illumination is primarily responsible for the generation of a layer of charged particles called the ionosphere.

We’re also inviting eclipse viewers around the country to become citizen scientists and participate in a nationwide science experiment by collecting cloud and air temperature data and reporting it via the GLOBE Observer smartphone app.

For more eclipse info, visit eclipse2017.nasa.gov and follow @NASASun on Twitter and NASA Sun Science on Facebook.  

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Get Ready to Watch Us Go for GOLD

The boundary where Earth’s atmosphere gives way to outer space is a complex place: Atmospheric waves driven by weather on Earth compete with electric and magnetic fields that push charged particles, all while our signals and satellites whiz by.

On Jan. 25, we’re launching the GOLD instrument (short for Global-scale Observations of the Limb and Disk) to get an exciting new birds-eye view of this region, Earth’s interface to space.

High above the ozone layer, the Sun’s intense radiation cooks some of the particles in the upper atmosphere into an electrically charged soup, where negatively charged electrons and positively charged ions flow freely. This is the ionosphere. The ionosphere is co-mingled with the highest reaches of our planet’s neutral upper atmosphere, called the thermosphere.

Spanning from just a few dozen to several hundred miles above Earth’s surface, the ionosphere is increasingly part of the human domain. Not only do our satellites, including the International Space Station, fly through this region, but so do the signals that are part of our communications and navigation systems, including GPS. Changes in this region can interfere with satellites and signals alike.  

Conditions in the upper atmosphere are difficult to predict, though. Intense weather, like hurricanes, can cause atmospheric waves to propagate all the way up to this region, creating winds that change its very makeup.

Because it’s made up of electrically charged particles, the upper atmosphere also responds to space weather. Space weather – which is usually driven by activity on the Sun – often results in electric and magnetic fields that push and pull on the ionosphere’s charged particles, changing the region’s makeup. On top of that, space weather can also mean incoming showers of high-energy particles that can affect satellites or endanger astronauts, and, in extreme cases, even cause power outages on Earth.

That’s where GOLD comes in. GOLD takes advantage of its host satellite’s geostationary orbit over the Western Hemisphere to maintain a constant view of the upper atmosphere, day and night. By scanning across, GOLD builds up a complete picture of Earth’s disk every half hour.

GOLD is an imaging spectrograph, a type of instrument that breaks light down into its component wavelengths. Studying light in this way lets scientists track the movement and temperatures of different chemical species and build up a picture of how the upper atmosphere changes over time. Capturing these measurements several times a day means that, for the first time, scientists will be able to record the short-term changes in the region -- our first look at its day-to-day ‘weather.’

GOLD is our first-ever mission to fly as a hosted payload on a commercial satellite. A hosted payload flies aboard an otherwise unrelated satellite, hitching a ride to space. GOLD studies the upper atmosphere, while its host satellite supports commercial communications.

Later this year, we’re launching another mission to study the ionosphere: ICON, short for Ionospheric Connection Explorer. Like GOLD, ICON studies Earth’s interface to space, but with a few important distinctions. ICON employs a suite of different instruments to study the ionosphere both remotely and in situ. The direct in situ measurements are possible because ICON flies in low-Earth orbit, giving us a detailed view to complement GOLD’s global perspective of the regions that both missions study.  

How to watch the launch on Jan. 25

Arianespace, a commerical aerospace company, is launching GOLD’s host commercial communications satellite, SES-14, for SES from Kourou, French Guiana.

Watch liftoff live on NASA Television - nasa.gov/live Launch Coverage starts at 5 p.m. EST  (2 p.m. PST, 7 p.m. Kourou local time)

We’ll be streaming the launch live on NASA TV! You can also follow along on Twitter (@NASA and @NASASun), Facebook (NASA and NASA Sun Science), Instagram, and on our Snapchat (NASA). 

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LIFTOFF!

On July 7, three crew members launched from Earth; headed to their new home on the International Space Station. 

Crewmembers Kate Rubins of NASA, Anatoly Ivanishin of Roscosmos and Takuya Onishi of the Japan Aerospace Exploration Agency (JAXA) will spend approximately four months on the orbital complex, returning to Earth in October. 

Photo Credit: (NASA/Bill Ingalls)

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Do not go where the path may lead, go instead where there is no path and leave a trail.  —Ralph Waldo Emerson 

How visible will the stars be compared to a normal night sky if I'm in the path of totality? (Sun completely covered)

I’m not entirely sure, but you will be able to see some stars that you normally wouldn’t see. https://eclipse2017.nasa.gov/sites/default/files/publications/Eclipse_brochure-bookmark_508.pdf In fact, during the 1919 eclipse, Sir Arthur Eddington and others used our ability to see stars close to the Sun during the eclipse to help confirm Einstines’ theory of general relativity. https://eclipse2017.nasa.gov/testing-general-relativity

Solar System: Things to Know This Week

Be a scientist for a day, solstice on the Red Planet, historic launches and more!

1. Scientist for a Day!

This year's Scientist for a Day essay contest was announced last week. Write an essay on one of the three images above. Essays are due in Feb. 2017. Students in grades 5-12 in U.S. schools, after-school and home-school programs, scout troops and museum programs are eligible to participate.

+ Learn more

2. Tuesday is Winter Solstice on Mars' Northern Hemisphere

Mars' orbit is much more eccentric than Earth's. The winters in the northern hemisphere are warm and short, as Mars is near perihelion—closer to the sun. This means that the winters in the southern hemisphere are long and cold.

+ Read Mars: The Other Terrestrial Planet

+ Seasons on Mars (Malin Space Science Systems) 

3. Launch-iversaries!

We’re celebrating two launch anniversaries. Before Curiosity. Before Spirit and Opportunity, there was Pathfinder and the hardy Sojourner rover, launched on Dec. 4, 1996. Pathfinder was a demonstration of the technology necessary to deliver a lander and a free-ranging robotic rover to the surface of Mars in a cost-effective and efficient manner. The lander, formally named the Carl Sagan Memorial Station following its successful touchdown, and the rover, named Sojourner after American civil rights crusader Sojourner Truth, both outlived their design lives — the lander by nearly three times, and the rover by 12 times! We continued the tradition with Spirit and Opportunity. Now there is the Mars Science Laboratory (with the Curiosity rover in stowage), which was launched on Nov. 26, 2011. It landed successfully in Gale Crater at 1:31 am EDT on Aug. 6, 2012. 

+ Go Back in Time

+ Video: Where Were You When Curiosity Landed on Mars? 

4. Mars Ice Deposit Holds as Much Water as Lake Superior

Water ice makes up half or more of an underground layer in a large region of Mars, about halfway from the equator to the north pole. The amount of water in this deposit—assessed using a radar aboard NASA's Mars Reconnaissance Orbiter—is about as much as in Lake Superior.

+ Read More

5. A Little Bit of History

Finally, it’s been seven years since Cassini caught one of its most stunning views of the plume on Saturn's moon Enceladus.

+ Read More

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

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NASA’s Artemis I Rocket is on the Launch Pad — and in Your Living Room

Artemis I will be the first integrated flight test of the Space Launch System (SLS) rocket and Orion spacecraft: the rocket and spacecraft that will send future astronauts to the Moon!

Before we embark on the uncrewed Artemis I mission to the Moon and back, the rocket and spacecraft will need to undergo a test at the launch pad called a “wet dress rehearsal.” This test will take the team at NASA’s Kennedy Space Center in Florida through every step of the launch countdown, including filling the rocket’s tanks with propellant.

But in the meantime, you can take a closer look at SLS and the Orion spacecraft by downloading the 3D model for free on the NASA app! You can view the SLS model in augmented reality by placing it virtually in your own environment – on your desk, for example. Or standing beside your family pet!

SLS and Orion join more than 40 other 3D models in the app, including BioSentinel, one of 10 CubeSats flying aboard Artemis I.

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The Geminids Are Now Playing in a Sky Near You

The Geminids, which peak during mid-December each year, are considered to be one of the best and most reliable annual meteor showers. 

This month, they're active from Dec. 4-17, and peak the evening of Dec. 13-14 for a full 24 hours, meaning more worldwide meteor watchers will get to enjoy the show. 

Below are 10 things to know about this beautiful spectacle.

1. The forecast. 

From our resident night sky expert, Jane Jones: If you can see Orion and Gemini in the sky, you'll see some Geminids. Expect to see about 60 meteors per hour before midnight on Dec. 13 and from midnight-3:30 a.m. on Dec. 14 from a dark sky. You'll see fewer meteors after moonrise at 3:30 a.m. local time. In the southern hemisphere, you won't see as many, perhaps 10-20 per hour, because the radiant—the point in the sky where the meteor shower appears to originate—never rises above the horizon.

2. Viewing tips.

Kids can join in on the fun as early as 9 or 10 p.m. You'll want to find an area well away from city or street lights. Come prepared for winter temperatures with a sleeping bag, blanket, or lawn chair. Lie flat on your back and look up, taking in as much of the sky as possible. After about 30 minutes in the dark, your eyes will adapt and you'll begin to see meteors. Be patient—the show will last until dawn, so you have plenty of time to catch a glimpse.

3. Late bloomer.

The Geminids weren't always such as a spectacular show. When they first began appearing in the mid-1800s, there were only 10-20 visible meteors per hour. Since then, the Geminids have grown to become one of the major showers of the year.

4. Remind me—where do meteor showers come from?

Meteors come from leftover comet particles and bits from asteroids. When these objects come around the Sun, they leave a dusty trail behind them. Every year, the Earth passes through these debris trails, which allows the bits to collide with our atmosphere, where they disintegrate to create fiery and colorful streaks in the sky.

5. That said...

While most meteor showers come from comets, the Geminids originate from an asteroid: 3200 Phaethon. Asteroid 3200 Phaethon takes 1.4 years to orbit the Sun once. It is possible that Phaethon is a "dead comet" or a new kind of object being discussed by astronomers called a "rock comet." Phaethon's comet-like, highly-elliptical orbit around the Sun supports this hypothesis. That said, scientists aren't too sure how to define Phaethon. When it passes by the Sun, it doesn't develop a cometary tail, and its spectra looks like a rocky asteroid. Also, the bits and pieces that break off to form the Geminid meteoroids are several times denser than cometary dust flakes.

6. Tell me more. 

3200 Phaethon was discovered on Oct. 11, 1983 by the Infrared Astronomical Satellite. Because of its close approach to the Sun, Phaethon is named after the Greek mythological character who drove the Sun-god Helios' chariot. Phaethon is a small asteroid: its diameter measures only 3.17 miles (5.10 kilometers) across. And we have astronomer Fred Whipple to thank—he realized that Phaethon is the source for the Geminids.

7. A tale of twins. 

The Geminids' radiant is the constellation Gemini, a.k.a. the "Twins." And, of course, the constellation of Gemini is also where we get the name for the shower: Geminids.

8. In case you didn't know. 

The constellation for which a meteor shower is named only helps stargazers determine which shower they're viewing on a given night; the constellation is not the source of the meteors. Also, don't just look to the constellation of Gemini to view the Geminids—they're visible throughout the night sky. 9. And in case you miss the show. 

There's a second meteor shower in December: the Ursids, radiating from Ursa Minor, the Little Dipper. If Dec. 22 and the morning of Dec. 23 are clear where you are, have a look at the Little Dipper's bowl—you might see about 10 meteors per hour. 10. Endless opportunities. There are so many sights to see in the sky. Use the Night Sky Network, the Solar System Ambassadors, and the Museum Alliance to look up local astronomy clubs, and join them for stargazing events in town, and under dark skies.

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