Friday, October 28, 2011

LiveChat Roundup: Oct. 28, 2011

By Jim Gerard, INSPIRE Education Specialist, KSC, FL


What difference would it make if we could give a population a three-day warning of an impending earthquake?  Evacuations could occur, resources made ready, and safety measures but in place. But how would we make such a forecast?  That was the subject of the LiveChat presented by Dr. Friedemann Freund of the Ames Research Center in California to 155 memebrs of the INSPIRE Online Learning Community.  Dr. Freund told of an interesting property of crystals he has discovered where a compressive force on a rock could generate an electrical current.  This current may effect the ionosphere, produce ultra-low frequency waves and may effect the health of humans and animals.  Dr. Freund’s presentation took up most of the hour, so not a lot of questions were answered, but he agreed to answer them off line so watch the Discussion Board for those answers!

Speaking of questions and answers:  Our goal with the LiveChat is to connect our OLC members to NASA subject matter experts, and the Q & A is a great way to do this.  We plan to have 20 – 25 minutes set aside for Q & A, allowing for 25 – 30 questions.  Typically, we’ve had an accumulated 60 hands raised at the end of the chat, so we’ve tried to solve this by asking our presenters to answer questions offline.  When the answers are returned they are posted in the LiveChat thread on the Discussion Board.  I will change the thread title by adding “w/ Q&A” to notify you when they are posted.

Now, here is how the Q & A works: When the chat is over, I will ask for questions.  At that time, you may raise your virtual hand (any hands raised before that time will be lowered) to queue up for a question.  Type your question into the text box in the Chat window but DO NOT SEND!  I will only respond to the question I called for and ask that question to our speaker.  Everything else will be ignored.  Imagine a class where each student is shouting out a question at the same time; this only produces chaos and no one gets any answers.  Sometimes, you hit send by mistake, and if I see you are queued up I note where it is and can come back to it.  No worries.  But several students are sending in questions without raising hands or waiting for their turn, creating a very confusing situation as the question I may be reading gets pushed up out of the window.  I ask for your patience and understanding, and for you to be polite to our presenter by following this simple rule: Send your question only when called.  Thank you!

Two LiveChats next week: our featured NASA Center is the Marshall Space Flight Center, and Scott Anderson from the Digital Learning Network will talk about the center at 4pm CT on Tuesday Nov. 1, and then our regular Thursday chat at 8pm CT with Sten Odenwald from Goddard Space Flight Center talking about Space Weather.  Sign up now on the Discussion Board!

Wednesday, October 26, 2011

12 Noon: a.m or p.m?

By Karthik Uppalari,

What do you consider 12 noon; a.m. or p.m.? Have you ever wondered or
confused? This is a very important question for international travelers. Most
of the international flights leave around midnight and it is a confusing issue
for less experienced travelers. It is an important issue which confuses both
local and international people.

In order to find out the proper way to write 12 noon, we should first learn
about the abbreviations. The abbreviation a.m. stands for ante meridian in
Latin (before the sun has crossed the line or before midday), and p.m. or
post meridian in Latin ( after the sun has crossed the line or after midday).
At 12 noon the sun is at its highest point in the sky and directly over the
meridian. That's why it is neither ante or post meridian, so the proper way
to write 12 midday is 12 Noon, and 12 at night is 12 midnight.

The idea of time is based on the rotation of the earth relative to sun and our
understanding of the day is the length of the time for the earth to rotate
once. The early pendulum clocks were corrected by means of astronomical
observations and they had an accuracy rate of about a second a year.
Later the clocks were replaced by quartz crystal controlled clocks which
used an atomic transition of frequency. The second was redefined and the
clocks were more accurate to one second in thousand of years.

The time measured based on the rotation of Earth on its axis with respect
to stars is called Universal time. Coordinated Universal time(UTC) was
created to keep 0.9 seconds of the time determined by the mean position of
the Sun (UT1). Leap seconds are added to keep the difference between
UTC and UT1 to a minimum. The rotation of the earth is measured by
artificial satellites in earth’s orbit to a precise determination of the location.

Time is measured in many different ways. The measure of time based on
orbital motion of Earth and other planets in the solar system is called
Dynamical Time. The measurement of time based on the rotation of the
Earth on its axis with respect to the stars is called Universal Time. Finally,
the measure o time through the oscillations of atoms is called International
Atomic Time.

The earth rotates to the Sun once a day, but in the course of the year it
makes one extra rotation due to its orbit. This will amount to a difference in
the position of the stars in the sky by about one degree, or four minutes of
time. The clocks run at slightly different rate to show this difference.
Universal Time is based on the mean sidereal time as measured in
Greenwich, England.

Eclipse predictions are presented in terms of Universal time and hours are
added to local time according to Time zone to convert local time to
Universal Time. For Example;
Atlantic Standard Time (AST)    UT - 4 hours
Eastern Standard Time (EST)     UT - 5 hours
Central Standard Time(CST)      UT - 6 hours
Mountain Standard Time (CST) UT - 7 hours
Pacific Standard Time (PST)      UT - 8 hours
The official source of the time used in the United States is the Time Service
Department of the U.S Naval Observatory.

For more information on Time please visit:
http://eclipse.gsfc.nasa.gov/SEhelp/TimeZone.html

Sources:1. NASA - Time Zones and Universal Time
2. Astronomy & time, National Maritime Museum

Friday, October 21, 2011

LiveChat Roundup: Oct. 20, 2011

By Jim Gerard, INSPIRE Education Specialist, KSC, FL


Is it possible to build an office complex that is not only environmentally sensitive to the area around it but actually produces more energy than it consumes? It is, and NASA did it!  Located at the Ames Research Center in California, the Sustainability Base was the topic of our LiveChat with Associate Director Steven Zornetzer.  149 were on hand to hear Mr. Zornetzer present how engineering and technology were used to produce one of the greenest buildings on the planet.

Here are some questions we did not get to in the chat:
Deshmukh, Rohan asks: How long do you expect this building to be top-class before another one is created that has higher standards? Will you keep updating the building to be top-of-the-line? Thank you! 
SZ:  I hope new buildings quickly overtake Sustainability Base in performance!  I wanted to set a high standard with this building but I am eager for others to set even higher standards.  We do expect to use our building as a living test bed for new energy efficient technologies as they become available in the future, so our building will continue to evolve and improve in performance. 

Vo, Ashley-Grace asks: If you changed the shape of solar panels, would it work better/worse? What about a slightly concave shape, not deeply curved so there won't be shadowed? Is there a better shape for solarpanels than rectangular? 
SZ:  I know companies have been experimenting with different shaped solar panels (cylindrical, concave, thin film, etc.).  Currently, due to cost of manufacturing primarily, nearly all commercially available solar panels are rectangular.  I would not be surprised if in the future that changes as the technology evolves or is replace by an entirely new photo-voltaic technology. 

Kahl, Rebecca asks: Was there anything else you would do if you had a bigger budget? Is the building structurally safe in the event of an earthquake or other natural disasters if the technology was implemented around the country? 
SZ;  If I had a larger budget I would have used electrochromic windows in the building.  These windows change heat transmissivity as a function of UV absorption.  They are relatively new and therefore still quite expensive.  Regarding earthquake resilience,  because the building has an exoskeleton, in other words, has all its structural steel support outside the skin of the building, it is very earthquake resilient.  In fact, it is the safest building on our entire campus.
More questions and answers are found on the Discussion Board.

Returning students may have noticed some changes in our weekly LiveChats.  We have new chat software by Blackboard Collaborate that provides more functionality to moderators, and better controls for presenters.  You shouldn’t have any different experience other than the color of the frames.  We will be using Collaborate on all future chats.

Another change is the number of students who are able to attend our LiveChat.  We have doubled in size from last year, which makes our presenters and us happy to see so many students interested.   This increase has presented a problem at the question and answer period following the chat.  Last night, for instance, we had 30 unanswered questions when our time ran out.  These questions were captured and sent to the presenter and will be posted with answers on the Discussion Board.   This is a big job and our presenters have been gracious to spend extra time for us, but I’d like to have a better way to ask questions.  If you have ideas, post them to the Discussion Board under Chat Talk.  We want it to be fair, but I hate disappointing students who wait in line only to end right before their question is taken.  I’m interested in hearing your ideas!

One more thing: All LiveChat quizzes are set for unlimited attempts and saving the highest score.  If you miss a question, keep taking it until you get the full 25 points.  A question from the NASA Going Green quiz that opened last night was scoring at .5 points instead of 5 points, so if you finished the quiz with 20.5 points, please retake it and get your full 25 points.

Wednesday, October 19, 2011

Science Fiction Come True?


By Leeann Hu, INSPIRE OLC, 9th Grade

Recently, many of us have heard the news of how scientists have found a planet much like Tatooine from Star Wars. As a result, the new planet that was discovered to be orbiting two suns was nicknamed as “Tatooine”.

However lately, another idea heard in many science fiction stories has been shown to might be possible- life could possibly exist in black holes.

Could this all be a hoax? Well, the idea was worked on by physicist Professor Vyacheslav Dokuchaev from the Russian Academy of Sciences, Moscow. In addition, the new was posted onto DiscoveryNews and MIT’s blog.

The theory is based on previous theories, so if the previous theories are proven wrong, his theory may be incorrect as well. Dokuchaev studied hypothetical orbits and the singularity in order to understand the dynamics of subatomic particles such as photons. This is because his theory is based on the previous theory that subatomic particles can have stable orbits inside the structure of black holes.

If this theory is correct, it would be an amazing breakthrough. Civilizations other than us may be living on the other “side” of the black holes. Other planets holding life could be hidden behind the darkness. For all we know, another universe may be there.

At this point though, nothing is completely sure. Dokuchaev admitted himself that there are some possible problems, where rules of space-time do not apply. But, this sure does open up some new, interesting philosophical questions.

Monday, October 17, 2011

Inside The J-2X Doghouse: A2J006 & Turbopump Thrust Balance

By William Greene, MSFC, Ala.

Okay, before I even get to the subject of thrust balance, I want to report that J-2X development engine E10001 got back into the stand and that the next test, A2J006, was conducted.  The test went the full planned duration of 40 seconds and the issues that caused us to remove the engine after the previous test all appear to be fixed.  In other words, it was a complete success.  Here's a video for your viewing pleasure:

http://www.nasa.gov/multimedia/videogallery/index.html?media_id=113620611

Now, speaking of issues on E10001 that appear to be resolved, I want to talk about turbopump thrust balance.  While I hadn't previously mentioned it, the data from the first several tests showed that there was a thrust balance issue with the oxidizer turbopump (OTP).  So, that naturally leads to the question:  What is "thrust balance?"

Here is a crude drawing of a turbopump for this discussion (And, please, save your cards and letters telling me that I am a terrible artist.  I will already catch plenty of grief from the turbo guys over this drawing.).  The arrows are intended to illustrate fluid flows.
I've drawn this in three colors because a turbopump can be thought of as having three fundamental elements.  The first element, the one in blue, is the part that spins.  This is the rotor onto which is attached the pumping stuff (i.e., the inducer and the impeller) on the pump side and the turbine stuff (i.e., the disks and blades) on the turbine side.

The second element, shown in green, is the part that doesn't spin.  This is the housing.  It is the shell within which the rotor spins.

The third element, shown in red, is the bearings.

Whenever you've got one thing spinning and another thing stationary, you've got to have some way of communicating between the two pieces.  Maybe the rotor just spins and slides around in some kind of restraint holding it in place.  Well that might work except that you can't put grease into a cryogenic oxygen environment and, should too much heat build-up due to friction, then you've got a very combustible situation.  Mix heat with a pure oxygen environment and anything and everything will burn, including metal.

What we do instead is typically use ball bearings between the rotor and the housing.  In some other pumps we use roller bearings that look like little cylinders rather than little balls, and there are other solutions as well.  These bearings do two things, they allow the rotor to spin and they hold the rotor in place.  So they need to be loose enough to spin yet tight enough to maintain control of a heavy hunk of metal spinning at over 10,000 rpm.  How much force the bearing put on the rotor to maintain control and, conversely, how much the rotor puts back on the bearings is called the bearing load.

When you are designing a turbopump, you design it so that the bearings have a specific load, and that means more than just a value, it also means a direction as shown in the sketch above.  You design the whole bearing package assuming that you know the magnitude and direction of the forces loaded through the package.  This then allows you to do some calculations that tell you, "Yep, I've got the rotor properly and sufficiently controlled."  Those calculations are part of what is often referred to as rotordynamics (and, by the way, NASA MSFC has some of the world's best experts in that area).

Question: How do you get different bearing loads in a turbopump?  Answer: Pressures.

Here is a nifty little fact: Pressure is all around us.  We don't feel the atmospheric pressure of 14.7 pounds-force over every square inch of your body because, well, it's always been there.  That's the environment within which we've evolved.  Now, go to the bottom of the ocean and you'll find a whole other pressure environment, one that would crush our delicate bodies into mess.  The basic principle to remember is this: Pressure applied over an area equals force.

Within a turbopump, you are explicitly manipulating pressure.  That's the whole purpose of a pump: to move fluid through the use of pressure.  So, in the pump end you have a low pressure coming in at the inlet and a very high pressure at the outlet.  On the turbine end, it's the opposite since on that end you're extracting energy (and therefore pressure) from the fluid.  So, on the turbine end you have high pressure at the inlet and lower pressure at the outlet.  Thus, throughout the turbopump, you've got pressures of all sorts and those pressures are pushing on the different pieces of the rotor.  This means that you've got all kinds of forces pushing on the rotor.  Some of the forces push the rotor towards the turbine end.  Some of the forces push the rotor towards the pump end.  Getting the right balance of forces is called your thrust balance.
So, what's the "right" thrust balance?  It is the one to which you've designed your bearings.  You design your bearings to have a certain load and a big part of that load is determines by the thrust balance on the rotor.  So, if your thrust balance is off, i.e., not what you intended, then your bearing loads are off and you're therefore not controlling the rotor the way that you wanted.  In the worst of circumstances, an out-of-control rotor represents a catastrophic situation.  In less-than-worst circumstances, operating with a thrust balance significantly different than the design intent could lead to unexpected wear on components and therefore limited operational life.

The next question is this: How do you create the thrust balance that you want and need to accomplish all this?

That's a matter of designing the internal guts of the turbopump and analytically modeling all of the internal flows within these guts.  In addition to the big flows coming into and out of the pump and turbine, you've got internal flows around seals, between pump or turbine stage, and through the bearings (as coolant).  When operating, the whole turbopump is full of fluid.  And, everywhere you have fluid, you have a pressure; and everywhere you have pressure applied to an area, you have a force.  So you calculate pressure drops through small passages or through seals and figure out a whole detailed map of different pressures and forces throughout the whole unit and you can understand your thrust balance.  And then, as necessary, you manipulate your clearances and seals and passages designs until you achieve the thrust balance you need.


Getting back to the E10001 OTP, what appears to have been the issue was that we had some seals that were too tight.  The tight seals overly restricted internal flows and, basically, messed up the intended force balance on the rotor.  This could be seen in the data collected from the testing.  Remember when I said several articles ago that this engine is instrumented to the max so that we can learn all about how it is working.  Here is a case where special instrumentation identified an issue.  The interesting part is that these seals were kinda sorta fine in terms of design but the processing of the material of which they are made -- it feels like hard plastic -- was not quite refined enough so that when subjected to operational conditions it changes dimensions and actually tightened up.

Prior to test A2J006, while we had the engine out of the stand, our contractor Pratt & Whitney Rocketdyne was able to partially disassemble the engine and the OTP just enough to change out the seals in question and then get the whole thing buttoned up and ready for test in record time.  They truly did some excellent work here.  And the success of test A2J006 is the proof!

Friday, October 14, 2011

LiveChat Roundup: Oct. 13, 2011

By Jim Gerard, INSPIRE Education Specialist, KSC, FL

Somewhere, Earth is burning. That inflammatory statement (pun intended!) merely means that fire is a natural part of the environment of our planet.  Of course, humans contribute their share as well, and investigating the effect of these fires is a goal of Dr. Douglas Morton at the Goddard Space Flight Center.  Dr. Morton is a specialist in the rainforest ecosystem, and he uses NASA's constellation of Earth observing satellites to study fires from space.

Dr. Morton presented to 159 INSPIRE OLC members about the effect of fires contributing to atmospheric carbon and its role in climate change.  All the fires in the world contribute as much carbon to the atmosphere as petroleum based vehicles.  Most of these are natural, the result of weather conditions and lightning. But in some areas, most notably the Amazon rain forest, clearing of land by fire for agriculture has reduced the size of the forest and contributed to carbon and aerosol pollution in the region.

Next week, continuing with this month's Earth theme, we bring back Steve Zornetzer of the Ames Research Center in California.  Mr. Zornetzer will present "NASA Going Green", how NASA is upgrading it's facilities to meet new energy and environmental standards.  Sign up now on the OLC Discussion Board, then join us at 8:00pm CT Thursday, October 20.  See you then!

Thursday, October 13, 2011

Be Careful With Faster-Than-Light Implications


By Allan Ko, INSPIRE OLC, 11th Grade
On Thursday, September 22, a team of scientists from all over the world announced that they had measured neutrinos (subatomic particles) traveling faster than the speed of light. Using a machine based at CERN in Geneva, Switzerland, the researches beamed neutrinos to detectors in Gran Sasso, Italy over a period of three years while working on a project called OPERA.

The distance from CERN to Gran Sasso is about 730 kilometers. Light would take roughly 2.4 milliseconds to traverse this distance, but the researches say that the neutrinos took 60 nanoseconds less time to reach Gran Sasso.

If this experiment is replicated and verified (Fermilab is one of the centers that is able to repeat this experiment), it would necessitate at the very least a revision of Einstein’s 1905 theory of special relativity, which is built on the axiom that nothing can travel faster than light speed.

Special relativity, the stuff that fills the last chapters of every physics textbook, is always presented as new, exotic science with consequences like time dilation and length contraction. With light speed being the ultimate speed limit, we can make statements about causality, which events can influence other events, and how everything except light is relative. If light speed is broken, most of these concepts are broken along with it.

Granted, faster-than-light movement opens a whole new world of possibilities. Sending information or particles back in time is the coolest science-fiction consequence, but this could also be a glimpse into a completely new theory of the universe. Maybe the particles took a shortcut through higher dimensions (think tessering, in Madeleine L’Engle’s A Wrinkle In Time), bringing the possibility of teleportation. Maybe they jumped through wormholes or “subspace”, Star Trek warp drive style.

At this point, however, it’s just as likely that the team of scientists simply made a mistake: overlooked a factor, or had slightly faulty machinery. When 105 years of science are on the line, caution before proceeding is advisable. Keep a stance of hopeful skepticism; skeptical, as all scientists should be, but hopeful that this data will lead mankind to an even better understanding of how the cosmos works. Who knows? Maybe in a few decades, these events will appear in the final chapters of our children’s physics textbooks.

Wednesday, October 12, 2011

Visiting the Kennedy Space Center

By Charles Bolden, NASA Administrator

Earlier today (Oct. 11), I got a first-hand look at the future of space exploration during a visit to Florida’s Kennedy Space Center. The new 6.75 million-ton Mobile Launcher is one more tangible step on our path forward to launching deep space missions.

When I was at Kennedy a little more than two months ago, I joined the dedicated team there in celebrating the achievements of our space shuttle program as it concluded an amazing 30 years of ground-breaking exploration and discovery. Since then, we have made great strides toward implementing the bipartisan vision agreed to by President Obama and Congress just one year ago.
  • We continued to work on the Orion spacecraft, the next vehicle in which astronauts will travel into deep space.
  • We’ve launched exciting science missions.
  • We expanded our agreements with our American commercial partners who are making great strides toward transporting cargo and crew to the International Space Station.
  • We’ve established a non-profit – located in the Space Coast – to manage the U.S. portion of the International Space Station.
  • We made significant progress on upgrading our ground-based operations here at KSC to support a range of launch activities, including commercial and deep space launches.
  • And we announced our plan forward with a Space Launch System, our heavy lift rocket.
And today, we got to see the progress Kennedy is making with the new Mobile Launcher, which will be carried to Launch Pad 39B, a modernized clean pad that will launch those missions to the ISS and farther destinations.

The Mobile Launcher is tangible evidence of our bright future and the critical path forward we are on to new destinations and new exploration achievements. It was built in large part by a Florida company, and it represents the jobs of the future as we continue to move toward reinvigorating Kennedy's world-class launch capabilities.

All around Kennedy, from the Operations and Checkout facility for the Orion multipurpose crew vehicle, to the establishment of a Commercial Crew program office to the ongoing science launches that regularly take-off here, it is clear the Space Coast is open for business and ready for a bright future.

As we've ramped up our work on the Orion multipurpose crew vehicle, for example, we brought on more than 250 workers at the Operations and Checkout facility – bringing that number to more than 350 in 2012.

This is also further proof that as our nation looks for ways to compete and win in the 21st century, NASA continues to be an engine of job growth and economic opportunity. From California to Florida, the space industry is strong and growing.

The history of NASA is tied to Florida. The next generation of explorers will not fly a space shuttle, but they may be able to walk on Mars. And those journeys are starting at the Kennedy Space Center today.

Administrator Bolden speaks in front of the Mobile Launcher at the Kennedy Space Center in Florida.

Friday, October 7, 2011

LiveChat Roundup: Oct. 6, 2011

By Jim Gerard, INSPIRE Education Specialist, KSC, FL

Our LiveChat was heating up last night as 151 OLC members were on hand to hear a presentation on 'Studying the Weather of the 21st Century' by Goddard Institute of Space Science's Ron Miller.  Dr. Miller works at the GISS office in downtown New York City, and uses satellite and ground based data to create climate models to help predict the trends in climate change.  While this topic does have a political angle, Dr. Miller stuck to the science (as we will in our Discussion Board!) as he shared the data and analysis coming from the GISS.

Do you want to be part of a LiveChat?  First you have to sign up on the Discussion Board.  Two opportunities are open right now: a Center Chat on Goddard Space Flight Center on Tuesday, Oct.11 at 3pm CT, and Oceans, on Thursday Oct. 13 at 8pm CT.  Click on either link or both and leave a post titled "Sign me up".  After the sign up closes (when we reach our room limit or two hours before the chat), you will receive an email reminder with extra instructions.  At the appointed time, navigate to the LiveChat room list (OLC>Connect>LiveChat) and the link for your chat should be in blue.  If not, you may be too early* (the chat opens 15 minutes before the event begins), or you may just need to refresh your browser.  Don't forget to turn off your pop-up blocker!  We have produced a short video tutorial to step you through the procedure.  If all else fails, send a description of your problem to nasainspire@okstate.edu.

What if you miss a chat?  The next morning you can usually find it available in the LiveChat archive on the LiveChat room list page.  The same file will also be placed in the Home page archive the following Monday, along with a version transcribed as a .mov and a .mp3 file that can be downloaded to your mobile device.  Don't forget to watch until the very end, when the password is given to allow you to take the quiz.  25 points are available for each LiveChat.

We're trying to increase the number of students that we can invite into our LiveChats, so we appreciate your patience and cooperation as we test out some new procedures.  Our objective is, as always, to connect the students of the INSPIRE Online Learning Community to NASA subject matter experts wherever they may be.

*Or too late!  Remember, all time listed on the OLC are Central Time.  Why? Since our home base is Oklahoma State University, that is where the server that supports the INSPIRE OLC is located.  We also serve students across 7 time zones (not including Guam and our overseas members), so Central Time is, well, central.  Please figure out for your location whether you need to add or subtract to find out when our events start.

Wednesday, October 5, 2011

Visiting the Future

By Charles Bolden, NASA Administrator

This past weekend, I had the opportunity to get a first-hand glimpse at the future of human space exploration.

NASA is working with multiple industry partners so that American companies can develop a capacity for carrying crew and cargo to the International Space Station, stop the outsourcing of this work to foreign governments and create good jobs right here at home. What I saw in Boulder, Colo. was Sierra Nevada’s amazing Dream Chaser vehicle – a kind of space plane that could be soaring into low Earth orbit in the coming years.

Sierra Nevada is one of the participants in NASA’s Commercial Crew Development program, and last week we decided to exercise additional milestones in their agreement with us to accelerate development of their transportation system. The company has already met four of the nine milestones under the CCDev2 Space Act Agreement (SAA) with NASA, and our amended agreement adds four new milestones -- bringing the potential value of Sierra Nevada's SAA to $105.6 million, if all milestones are completed successfully, to help them create jobs and get our economy back on track.

The Boeing Company, another CCDEV2 participant, also will now pursue additional milestones, and all four of the CCDEV2 participants are performing well. Boeing will receive $112.9 million, if all milestones are reached, money that is being pumped into our economy at a critical time. Transporting crew to the ISS is crucial, and we are focusing hard on ensuring that American companies will be carrying our astronauts and our cargo to space as we ramp up a new era of the station’s potential as an orbiting laboratory without peer. After all, the ISS is the centerpiece of our human space flight activities for the coming years with international crews of six living aboard it 24/7 right now.

Because of the progress Sierra Nevada and our other commercial space partners have made, I am confident that NASA will soon have access to multiple capabilities for reaching low Earth orbit.

And while American innovators open up a new segment of the economy by creating these new capabilities, NASA can focus its energy and resources on deep space exploration.

As President Obama looks for ways to put America back to work, NASA continues to be an engine of job growth and economic opportunity. Our collaborations with private industry are enhancing our ability to design and build the most technologically advanced spacecraft in the world. These partnerships are building an economic sector that will create new high-tech, high-paying jobs in communities like Boulder all across the country – all while ensuring a bright future that ensures America’s leadership in space.
NASA Administrator Charles Bolden flies Sierra Nevada's Dream Chaser simulator.