Cassini Top 10 Images And Science Results Of 2015

Another Station Upgrade:

Spacewalkers Jeff Williams and Kate Rubins to install new TV cameras 

On Thursday, Sept. 1, U.S. astronauts Jeff Williams and Kate Rubins will conduct the station’s 195th American spacewalk. As part of their activities, the pair will install the first of several enhanced high-definition television cameras that will monitor activities outside the station, including the comings and goings of visiting cargo and crew vehicles

Working on the station’s backbone, or truss, Williams and Rubins will retract a thermal radiator that is part of the station’s cooling system. 

As was the case for their first spacewalk together on Aug. 19, Williams will be designated as extravehicular crew member 1 (EV1), wearing a spacesuit with a red stripe, while Rubins will be EV2, wearing a suit with no stripes.

Watch LIVE!

Coverage of the spacewalk begins at 6:30 a.m. EDT on Thursday, Sept. 1; with the spacewalk scheduled to begin at 8:05 a.m. EDT. Stream live online HERE.

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What’s Up for August 2017

The total solar eclipse on August 21 will trace a narrow path across the nation, although most of the U.S. will see a partial eclipse. Here's what to do before, during and after the eclipse, plus how you can become a citizen scientist helping us with eclipse observations.

Not everyone can travel to the path of totality, so here are some things you can do whether you see totality or a partial eclipse. 

Collecting Citizen Science

Want to be a citizen scientist? 

Before the eclipse, make and pack your very own eclipse toolkit, containing a notebook, pen, a clock, a stopwatch, the front page of a newspaper, a thermometer, and a stick with a piece of crepe paper tied to it. Don’t forget your assistant, who will help conduct science observations. 

Practice using a citizen scientist phone app, like our GLOBE app to study clouds, air and surface temperatures and other observations. Go to the location where you plan to observe the eclipse and check for any obstructions. You may want to focus on only one activity as the eclipse will last less than 3 minutes ... or just really experience the eclipse. 

Cell phones don’t take eclipse video! And plan to have your safe eclipse-viewing glasses within reach for before and after totality. Just before totality, if you have a good view of the horizon, look west to see the approaching shadow. After totality, look east low on the horizon for the departing shadow.

During totality, look for stars. You should be able to see the star Regulus in the solar corona or the stars of Orion.

During totality, we may see moving bands of shadows, like on the bottom of a swimming pool.

How dark does it get at totality? Look at the newspaper you brought with you. What is the smallest print you can read?

How much does the temperature drop? Does the wind stop or change direction?

Use your hands, a sheet of paper with a hole in it, a kitchen colander or any other object with one or more holes to use as a pinhole projector. You’ll be able to see the crescent shape of the sun projected through the holes.

Find out more about the eclipse, including eclipse safety, at https://eclipse2017.nasa.gov

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Would you smooch an alien?

Depends what he looks like!

Our Space Launch System Rocket’s “Green Run” Engine Testing By the Numbers

We continue to make progress toward the first launch of our Space Launch System (SLS) rocket for the Artemis I mission around the Moon. Engineers at NASA’s Stennis Space Center near Bay St. Louis, Mississippi are preparing for the last two tests of the eight-part SLS core stage Green Run test series.

The test campaign is one of the final milestones before our SLS rocket launches America’s Orion spacecraft to the Moon with the Artemis program. The SLS Green Run test campaign is a series of eight different tests designed to bring the entire rocket stage to life for the first time.

As our engineers and technicians prepare for the wet dress rehearsal and the SLS Green Run hot fire, here are some numbers to keep in mind:

212 Feet

The SLS rocket’s core stage is the largest rocket stage we have ever produced. From top to bottom of its four RS-25 engines, the rocket stage measures 212 feet.

35 Stories

For each of the Green Run tests, the SLS core stage is installed in the historic B-2 Test Stand at Stennis. The test stand was updated to accommodate the SLS rocket stage and is 35 stories tall – or almost 350 feet!

4 RS-25 Engines

All four RS-25 engines will operate simultaneously during the final Green Run Hot Fire. Fueled by the two propellant tanks, the cluster of engines will gimbal, or pivot, and fire for up to eight minutes just as if it were an actual Artemis launch to the Moon.

18 Miles

Our brawny SLS core stage is outfitted with three flight computers and special avionics systems that act as the “brains” of the rocket. It has 18 miles of cabling and more than 500 sensors and systems to help feed fuel and direct the four RS-25 engines.

733,000 Gallons

The stage has two huge propellant tanks that collectively hold 733,000 gallons of super-cooled liquid hydrogen and liquid oxygen. The stage weighs more than 2.3 million pounds when its fully fueled.

114 Tanker Trucks

It’ll take 114 trucks – 54 trucks carrying liquid hydrogen and 60 trucks carrying liquid oxygen – to provide fuel to the SLS core stage.

6 Propellant Barges

A series of barges will deliver the propellant from the trucks to the rocket stage installed in the test stand. Altogether, six propellant barges will send fuel through a special feed system and lines. The propellant initially will be used to chill the feed system and lines to the correct cryogenic temperature. The propellant then will flow from the barges to the B-2 Test Stand and on into the stage’s tanks.

100 Terabytes

All eight of the Green Run tests and check outs will produce more than 100 terabytes of collected data that engineers will use to certify the core stage design and help verify the stage is ready for launch.

For comparison, just one terabyte is the equivalent to 500 hours of movies, 200,000 five-minute songs, or 310,000 pictures!

32,500 holes

The B-2 Test Stand has a flame deflector that will direct the fire produced from the rocket’s engines away from the stage. Nearly 33,000 tiny, handmade holes dot the flame deflector. Why? All those minuscule holes play a huge role by directing constant streams of pressurized water to cool the hot engine exhaust.

One Epic First

When NASA conducts the SLS Green Run Hot Fire test at Stennis, it’ll be the first time that the SLS core stage operates just as it would on the launch pad. This test is just a preview of what’s to come for Artemis I!

The Space Launch System is the only rocket that can send NASA astronauts aboard NASA’s Orion spacecraft and supplies to the Moon in a single mission. The SLS core stage is a key part of the rocket that will send the first woman and the next man to the Moon through NASA’s Artemis program.

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What’s it like having the coolest job ever?

Take a moment, look outside your window. 🌷🌼

Today is the #FirstDayOfSpring in the Northern Hemisphere, also known as the vernal equinox.

#DYK Earth’s tilted axis causes the season? Throughout the year, different parts of Earth receive the Sun’s most direct rays. So, when the North Pole tilts toward the Sun, it’s summer in the Northern Hemisphere. And when the South Pole tilts toward the Sun, it’s winter in the Northern Hemisphere.

These images are of Zinnias. They are part of the flowering crop experiment that began aboard the International Space Station on Nov. 16, 2015, when NASA astronaut Kjell Lindgren activated the Veggie system and its rooting "pillows" containing zinnia seeds.

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Guy Bluford Changed the Course of Space History

On Aug. 30, 1983, Guion Bluford, better known as Guy, became the first African American to fly to space. An accomplished jet pilot and aerospace engineer, Bluford became part of NASA’s 1978 astronaut class that included the first African American, the first Asian American, and the first women astronauts.

He and the other crew members of mission STS-8 were aboard the orbiter Challenger as it lifted off from Kennedy Space Center in Florida; it was the first nighttime launch and landing of the Space Shuttle program. While aboard, he and the other crew members deployed the Indian National Satellite (INSAT-1B), operated a Canadian-built robot arm, conducted experiments with live cell samples, and participated in studies measuring the effects of spaceflight on humans.

Guy Bluford chased his childhood dream of becoming an aerospace engineer, and in doing so, changed history and encouraged other Black astronauts to follow in his footsteps.

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Does space have a standard time or do you rely on the time zones on Earth while you are in space?

Great question.  Really it is up to the particular space agency/mission which time zone they use.  For example, since the International Space Station is a collaboration between NASA, the Russian Space Agency, the European Space Agency, the Japanese Space Agency, and the Canadian Space Agency, we came up with the compromise of operating on Greenwich Mean Time (GMT).  So, Space Station time is the same as London time!  The International Space Station orbits our planet every 90 minutes, so of course we’re transiting across multiple time zones constantly.  

Five Technologies Taking Aeronautics into the Future

Martian helicopters? Electric planes? Quiet supersonic flight?

The flight technologies of tomorrow are today’s reality at NASA. We’re developing a number of innovations that promise to change the landscape (skyscape?) of aviation. Here are five incredible aeronautic technologies currently in development:

 1. The X-59 QueSST and Quiet Supersonic Technology

It might sound like an oxymoron, but ‘quiet boom’ technology is all the rage with our Aeronautics Mission Directorate. The X-59 QueSST is an experimental supersonic jet that hopes to reduce the sound of a supersonic boom to a gentle thump. We will gauge public reaction to this ‘sonic thump,’ evaluating its potential impact if brought into wider use. Ultimately, if the commercial sector incorporates this technology, the return of supersonic passenger flight may become a reality!

 2. The X-57 Electric Plane

Electric cars? Pfft. We’re working on an electric PLANE. Modified from an existing general aviation aircraft, the X-57 will be an all-electric X-plane, demonstrating a leap-forward in green aviation. The plane seeks to reach a goal of zero carbon emissions in flight, running on batteries fed by renewable energy sources!

3. Second-Generation Search and Rescue Beacons

Our Search and Rescue office develops technologies for distress beacons and the space systems that locate them. Their new constellation of medium-Earth orbit instruments can detect a distress call near-instantaneously, and their second-generation beacons, hitting shelves soon, are an order of magnitude more accurate than the previous generation!

(The Search and Rescue office also recently debuted a coloring book that doesn’t save lives but will keep your crayon game strong.)

4. Earth from the Air

Earth science? We got it.

We don’t just use satellite technology to monitor our changing planet. We have a number of missions that monitor Earth’s systems from land, sea and air. In the sky, we use flying laboratories to assess things like air pollution, greenhouse gasses, smoke from wildfires and so much more. Our planet may be changing, but we have you covered.

5. Icing Research

No. Not that icing.

Much better.

Though we at NASA are big fans of cake frosting, that’s not the icing we’re researching. Ice that forms on a plane mid-flight can disrupt the airflow around the plane and inside the engine, increasing drag, reducing lift and even causing loss of power. Ice can also harm a number of other things important to a safe flight. We’re developing tools and methods for evaluating and simulating the growth of ice on aircraft. This will help aid in designing future aircraft that are more resilient to icing, making aviation safer.

There you have it, five technologies taking aeronautics into the future, safely down to the ground and even to other planets! To stay up to date on the latest and greatest in science and technology, check out our website: www.nasa.gov.

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Hunting for Organic Molecules on Mars

Did Mars once have life? To help answer that question, an international team of scientists created an incredibly powerful miniature chemistry laboratory, set to ride on the next Mars rover.

The instrument, called the Mars Organic Molecule Analyzer Mass Spectrometer (MOMA-MS), will form a key part of the ExoMars Rover, a joint mission between the European Space Agency (ESA) and Roscosmos. A mass spectrometer is crucial to send to Mars because it reveals the elements that can be found there. A Martian mass spectrometer takes a sample, typically of powdered rock, and distinguishes the different elements in the sample based on their mass.

After 8 years of designing, building, and testing, NASA scientists and engineers from NASA’s Goddard Space Flight Center said goodbye to their tiny chemistry lab and shipped it to Italy in a big pink box. Building a tiny instrument capable of conducting chemical analysis is difficult in any setting, but designing one that has to launch on a huge rocket, fly through the vacuum of space, and then operate on a planet with entirely different pressure and temperature systems? That’s herculean. And once on Mars, MOMA has a very important job to do. NASA Goddard Center Director Chris Scolese said, “This is the first intended life-detecting instrument that we have sent to Mars since Viking.”

The MOMA instrument will be capable of detecting a wide variety of organic molecules. Organic compounds are commonly associated with life, although they can be created by non-biological processes as well. Organic molecules contain carbon and hydrogen, and can include oxygen, nitrogen, and other elements.

To find these molecules on Mars, the MOMA team had to take instruments that would normally occupy a couple of workbenches in a chemistry lab and shrink them down to roughly the size of a toaster oven so they would be practical to install on a rover.

MOMA-MS, the mass spectrometer on the ExoMars rover, will build on the accomplishments from the Sample Analysis at Mars (SAM), an instrument suite on the Curiosity rover that includes a mass spectrometer. SAM collects and analyzes samples from just below the surface of Mars while ExoMars will be the first to explore deep beneath the surface, with a drill capable of taking samples from as deep as two meters (over six feet). This is important because Mars’s thin atmosphere and spotty magnetic field offer little protection from space radiation, which can gradually destroy organic molecules exposed on the surface. However, Martian sediment is an effective shield, and the team expects to find greater abundances of organic molecules in samples from beneath the surface.

On completion of the instrument, MOMA Project Scientist Will Brinckerhoff praised his colleagues, telling them, “You have had the right balance of skepticism, optimism, and ambition. Seeing this come together has made me want to do my best.”

In addition to the launch of the ESA and Roscosmos ExoMars Rover, in 2020, NASA plans to launch the Mars 2020 Rover, to search for signs of past microbial life. We are all looking forward to seeing what these two missions will find when they arrive on our neighboring planet.

Learn more about MOMA HERE.

Learn more about ExoMars HERE.

Follow @NASASolarSystem on Twitter for more about our missions to other planets.

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