By Jim Gerard, INSPIRE Education Specialist, KSC, FL
The Space Shuttle program is over, and the hardware it utilized has been transferred to museums across the country. You can visit flown orbiters in Los Angelos, California (Endeavour), and Dulles airport in Virginia (Discovery), but the first dedicated facility to the program is the new home for Atlantis at the Kennedy Space Center Visitor Complex in Florida. "Space Shuttle Atlantis," which debuts on Saturday (June 29), showcases the retired winged spacecraft as part of a $100 million exhibit that has been more than a year in the making. It succeeds in bringing the public nose-to-nose — and nose-to-wing and nose-to-tail — with Atlantis in a way that is unique to every other museum display of a shuttle orbiter.
With a reveal worthy of the 'magical' theme park in nearby Orlando, visitors will experience an encounter with the mighty spacecraft similar to an astronaut walking in space. Seemingly within touching distance, with its payload bay open and a replica of its Canadarm robotic arm extended, Atlantis looks less like a museum's static display than it does a still active vehicle, somehow frozen in place, as if it could soar back into orbit at any time. What's more, thanks to theatrical lighting and a 40-foot-long (12-meter) animated digital backdrop, the orbiter comes alive as the changing hues and resulting shadows stretch across its surface.
INSPIRE Students attending the upcoming Student Unconference will get to witness this new display during their stay, while others vacationing near KSC will see it as part of their Visitor Complex experience.
Discuss this blog here: http://tinyurl.com/bloginspire12
Wednesday, June 26, 2013
Wednesday, June 19, 2013
First Day of Summer
By Jim Gerard, INSPIRE, KSC
This Friday, June 21, is the first day of summer. The Summer Solstice, when the earth's tilt is most directly pointed at the sun, occurs at 1:04am EDT. This has created some confusion in our western states as it would still technically be Thursday, June 20.
But two points to consider:
1) The sun, as does most of the world, does not follow Daylight Saving Time so it would be 12:04am EST which would make the Solstice in all the country on Thursday except the east coast by 4 minutes. 2) When do we celebrate day at night? It would always be the next dawning which is Friday for everyone.
So if you west coasters start your summer celebrations on Thursday, remember it is still spring until almost midnight and you are being a little premature. But then it is never to early to party.
Discuss this blog here: http://tinyurl.com/bloginspire12
This Friday, June 21, is the first day of summer. The Summer Solstice, when the earth's tilt is most directly pointed at the sun, occurs at 1:04am EDT. This has created some confusion in our western states as it would still technically be Thursday, June 20.
But two points to consider:
1) The sun, as does most of the world, does not follow Daylight Saving Time so it would be 12:04am EST which would make the Solstice in all the country on Thursday except the east coast by 4 minutes. 2) When do we celebrate day at night? It would always be the next dawning which is Friday for everyone.
So if you west coasters start your summer celebrations on Thursday, remember it is still spring until almost midnight and you are being a little premature. But then it is never to early to party.
Discuss this blog here: http://tinyurl.com/bloginspire12
Tuesday, June 18, 2013
Why Should I Participate in NASA Challenges?
By Abigail Radford,
Rising Senior,
Alchemists
One reason why we love the OLC so much is because of the numerous opportunities it offers each one of us. Scholarly programs, internships, competitions—anything that we can utilize to our benefit is just a click away on the Equip page. From my personal experiences, I have concluded that the best and most rewarding opportunities lie in the various Challenges offered throughout the year. From lunar science, to product innovation, to robotics, to spacecraft engineering, there is bound to be a Challenge meant for your interests and passions.
This year I competed in the RealWorld-InWorld Engineering Design Challenge. A team of myself, Jonathan Hernandez, Kate Denner, and Joshua Dijamco worked together to design a sunshield that would protect the James Webb Space Telescope from cosmic radiation to allow it to detect infrared light from far away galaxies. Sounds simple, right? It certainly wasn’t. We had to incorporate many factors into its design like minimizing cost, maximizing the telescope’s pointing angle, unfolding the shield in space, and more.
We became engineers as we brainstormed possible design solutions, criticized each other’s work, and implemented the best attributes of each into our final design. We outlined our progress in an extensive 28-page paper. We advanced to the next round of the challenge and had to transfer the same information in the paper into a 3-D world called NIA Universe, an impressive computer program that took weeks to learn how to navigate in and use. After weeks of working during many late, coffee-filled nights, we finally finished our “world”. We anxiously awaited the final results from the judges, and finally, the announcement was made: Team Metropolitan (that’s us) won first place!
I cannot explain to you the overwhelming triumph and happiness I felt after receiving such good news. Our hard work had paid off and our ideas had been acknowledged and approved. There was even a cash prize of $833 for each of us that could be used to help with the costs of traveling up to the Goddard Spaceflight Center in Greenbelt, MD. There, we were all reunited after months of collaboratively working on a huge project through virtual tools like Google Docs and Skype hundreds and thousands of miles away. We were treated like royalty upon our arrival. We even met the Director of GSC Christopher Scolese, who awarded each of us our very own flag that had been flown aboard the final flight of the Space Shuttle Atlantis. For the next few hours we were given a VIP tour of GSC and saw a Hyperwall demonstration, as well as the behind-the-scenes of NASA TV. Later we met with the 2006 Nobel Prize winner Dr. John Mather, who gave a presentation on some of his work.
We ended this amazing day with a bang: a viewing of the James Webb Space Telescope clean room. This telescope means so much to us. For months we slaved over every one of its details: its mission goals, size, orbit, and more. Before, we had imagined the JWST as something that seemed so intangible, unreal and far away. But finally, the awesome piece of technology we had been studying for so long was sitting right in front of us. It was surrounded by people who care about it just as much as we do. That moment was huge for me because I realized that I was on the right path: I want to grow up to become a part of a large NASA team that works together to produce an extraordinary work of art like the James Webb Space Telescope. Whether it will go to the Moon, Mars, or a near-Earth asteroid, I want to contribute to its success.
So why should you participate in one or more of the NASA Challenges next year? There are many reasons why, ranging from the people you will meet to the experience you will gain. Completing a group challenge will bring all of your teammates closer together, helping you discover a teammate that you work extremely well with. You will also learn effective means of communication, time management, and how to distribute tasks to achieve the highest level of efficiency. You will also learn a great deal about the topic you chose to do your Challenge on, helping you gain experience in that field which will put you at an advantage among your peers in the future. If your team works hard and functions smoothly, you could be next year’s first place winner. Who knows what exciting prizes and opportunities could come your way.
If you find yourself struggling while completing a Challenge, just remember to keep a positive attitude and that patience pays off in the long run.
Discuss this blog here: http://tinyurl.com/bloginspire12
One reason why we love the OLC so much is because of the numerous opportunities it offers each one of us. Scholarly programs, internships, competitions—anything that we can utilize to our benefit is just a click away on the Equip page. From my personal experiences, I have concluded that the best and most rewarding opportunities lie in the various Challenges offered throughout the year. From lunar science, to product innovation, to robotics, to spacecraft engineering, there is bound to be a Challenge meant for your interests and passions.
This year I competed in the RealWorld-InWorld Engineering Design Challenge. A team of myself, Jonathan Hernandez, Kate Denner, and Joshua Dijamco worked together to design a sunshield that would protect the James Webb Space Telescope from cosmic radiation to allow it to detect infrared light from far away galaxies. Sounds simple, right? It certainly wasn’t. We had to incorporate many factors into its design like minimizing cost, maximizing the telescope’s pointing angle, unfolding the shield in space, and more.
We became engineers as we brainstormed possible design solutions, criticized each other’s work, and implemented the best attributes of each into our final design. We outlined our progress in an extensive 28-page paper. We advanced to the next round of the challenge and had to transfer the same information in the paper into a 3-D world called NIA Universe, an impressive computer program that took weeks to learn how to navigate in and use. After weeks of working during many late, coffee-filled nights, we finally finished our “world”. We anxiously awaited the final results from the judges, and finally, the announcement was made: Team Metropolitan (that’s us) won first place!
I cannot explain to you the overwhelming triumph and happiness I felt after receiving such good news. Our hard work had paid off and our ideas had been acknowledged and approved. There was even a cash prize of $833 for each of us that could be used to help with the costs of traveling up to the Goddard Spaceflight Center in Greenbelt, MD. There, we were all reunited after months of collaboratively working on a huge project through virtual tools like Google Docs and Skype hundreds and thousands of miles away. We were treated like royalty upon our arrival. We even met the Director of GSC Christopher Scolese, who awarded each of us our very own flag that had been flown aboard the final flight of the Space Shuttle Atlantis. For the next few hours we were given a VIP tour of GSC and saw a Hyperwall demonstration, as well as the behind-the-scenes of NASA TV. Later we met with the 2006 Nobel Prize winner Dr. John Mather, who gave a presentation on some of his work.
We ended this amazing day with a bang: a viewing of the James Webb Space Telescope clean room. This telescope means so much to us. For months we slaved over every one of its details: its mission goals, size, orbit, and more. Before, we had imagined the JWST as something that seemed so intangible, unreal and far away. But finally, the awesome piece of technology we had been studying for so long was sitting right in front of us. It was surrounded by people who care about it just as much as we do. That moment was huge for me because I realized that I was on the right path: I want to grow up to become a part of a large NASA team that works together to produce an extraordinary work of art like the James Webb Space Telescope. Whether it will go to the Moon, Mars, or a near-Earth asteroid, I want to contribute to its success.
So why should you participate in one or more of the NASA Challenges next year? There are many reasons why, ranging from the people you will meet to the experience you will gain. Completing a group challenge will bring all of your teammates closer together, helping you discover a teammate that you work extremely well with. You will also learn effective means of communication, time management, and how to distribute tasks to achieve the highest level of efficiency. You will also learn a great deal about the topic you chose to do your Challenge on, helping you gain experience in that field which will put you at an advantage among your peers in the future. If your team works hard and functions smoothly, you could be next year’s first place winner. Who knows what exciting prizes and opportunities could come your way.
If you find yourself struggling while completing a Challenge, just remember to keep a positive attitude and that patience pays off in the long run.
Discuss this blog here: http://tinyurl.com/bloginspire12
Friday, June 14, 2013
LiveChat Round Up 6/13/2013
By Jim Gerard, NASA INSPIRE Education Specialist, KSC, FL
Summer is upon us, and next week begins our first Virtual STEM Experience (VSE). We wanted to provide more in-depth classes for the OLC, and the VSE was created to give you deeper understanding of a STEM related field. Thus includes content from experts in the field, similar to what we try to do every Thursday night. In order to spend more time during the VSE withinstruction, we decided to move the subject matter expert (SME) to our regular Thursday night chat and open it for everyone in the community. This is what we did last night, when Dr. Shawn Donnegal-Goldman from Goddard Space Flight Center talked about his job of searching for evidence of life on other planets.
Dr Shawn talked first about finding other planets (around other stars), a task that the space probe Kepler does very well. (You can build a model of the Kepler spacecraft by clicking here.) With Kepler we have found hundreds of planet candidates, but even then our ability to directly observe them is very slight. A planet like the earth would be orbiting too close and be too dim to distinguish from the central star's light. Future projects like the star-shade could help us in observing these faint objects.
The following animation illustrate every star to date that Kepler has detected as having planets and the relative size and orbits of those planets.
Summer is upon us, and next week begins our first Virtual STEM Experience (VSE). We wanted to provide more in-depth classes for the OLC, and the VSE was created to give you deeper understanding of a STEM related field. Thus includes content from experts in the field, similar to what we try to do every Thursday night. In order to spend more time during the VSE withinstruction, we decided to move the subject matter expert (SME) to our regular Thursday night chat and open it for everyone in the community. This is what we did last night, when Dr. Shawn Donnegal-Goldman from Goddard Space Flight Center talked about his job of searching for evidence of life on other planets.
Dr Shawn talked first about finding other planets (around other stars), a task that the space probe Kepler does very well. (You can build a model of the Kepler spacecraft by clicking here.) With Kepler we have found hundreds of planet candidates, but even then our ability to directly observe them is very slight. A planet like the earth would be orbiting too close and be too dim to distinguish from the central star's light. Future projects like the star-shade could help us in observing these faint objects.
The following animation illustrate every star to date that Kepler has detected as having planets and the relative size and orbits of those planets.
To learn more about Dr. Shawn's work, you can follow his blog at http://paleblueblog.org.
Next week, more on the search for extraterrestrial life, but this time on Icy Worlds!
P.S. If you are in the Life on Other Planets VSE and were not able to attend the LiveChat, make sure to view it in the archives!
Discuss this blog here: http://tinyurl.com/bloginspire12
Tuesday, June 11, 2013
Summer Stargazing: What’s Up Tonight?
By Olivia Humes, Grade 11, Imagineers
Astronomically speaking, the beginning of summer brings long days and short nights. Here on Earth, summer tends to bring fantastic weather and clear skies. Though you’ll have to stay up late in order to see them, summer constellations offer a rich number of targets for naked-eye, binocular, or telescopic viewing.
The Summer Triangle is an easy to find group of bright stars that can help point you to interesting
observing targets. Facing south, the Summer Triangle will appear as a large, nearly right triangle defined by the three brightest stars in view. The Summer Triangle contains the alpha stars of three different constellations: Vega in Lyra, Deneb in Cygnus, and Altair in Aquila. This area of the sky is particularly rich since it lies in the plane of the Milky Way. A quick glance through a telescope will uncover dense star fields and gas clouds, such as the Ring Nebula in Lyra. The Summer Triangle also marks the location of the Kepler target stars between Vega and Deneb.
Deneb is the faintest of the trio and is the tail of Cygnus, which is a cross-shaped constellation representing a swan flying roughly to the south. At the head of the swan, nearly halfway between Vega and Altair is a binary star called Alberio. With a telescope, the two stars making up the system can be easily resolved. Albireo is a particularly special binary system because the two stars that make it up are two different colors!
Later in the night, the constellations Pegasus and Andromeda rise in the east. Pegasus contains the “great square” located just east of Cygnus’s wingtip. The constellation Andromeda shares a star with the northernmost corner of the great square. The nearest large galaxy, the Andromeda galaxy is located in this constellation. In especially dark conditions, it can be seen with the naked eye as a fuzzy blob, but in cities and suburbs, it is accessible with binoculars or a small telescope.
Circumpolar constellations are visible throughout the year, but the clear skies of summer can give an observer a great chance to view them as well. Depending on your latitude, the number of circumpolar constellations vary. The closer you are to the poles, the more you will see. However, for the United States and Europe, both the Big and Little Dippers can be seen all night and all year long.
The brighter, Big Dipper can also be used as a guide to find other interesting observing targets. Within the Big Dipper itself, another multiple star system can be seen. With good eyes and a dark sky, the second star in the “handle” of the Big Dipper reveals itself as two stars, called Alcor and Mizar! The system is actually composed of six different stars. Mizar, the brighter, is a quadruple binary system, and Alcor is itself a two-star system. Though a small telescope and binoculars won’t reveal all six stars, they will help you get a better view of the double.
The last two stars of the Big Dipper’s “scoop” point towards the North Star, Polaris, in the Little Dipper. This constellation is fainter, but it is important for navigation. Not only does the star indicate the direction of north, but its elevation from the horizon indicates your latitude. If you travel further north, the Polaris will rise higher and higher in the sky. In the early summer, following the arc of the handle of the Big Dipper allows you to “arc to Arcturus” and find a red giant star in the constellation Bootes. After that, continue to follow the arc and “speed on to Spica,” a blue giant star in Virgo. Other circumpolar constellations visible near the Dippers include Cassiopea, the M or W, and Draco, a faint constellation that snakes its way between the two Dippers and ends near the familiar bright summer star Vega.
As summer comes, take the opportunity provided by clear nights and the end of school to learn some new constellations or telescopic targets. Besides the objects mentioned here, other great telescope and binocular targets are the Messier Objects, a catalogue of galaxies, nebulae, and clusters; or any planets that are visible. Be sure to find a star chart to help you get an accurate picture of what the skies look like at your latitude. Using a red flashlight will help you while working in the dark, but won’t ruin your night vision. Most of all, have fun exploring the night sky!
Printable star charts can be found here: http://www.skymaps.com/downloads.html
Discuss this blog here: http://tinyurl.com/bloginspire12
Astronomically speaking, the beginning of summer brings long days and short nights. Here on Earth, summer tends to bring fantastic weather and clear skies. Though you’ll have to stay up late in order to see them, summer constellations offer a rich number of targets for naked-eye, binocular, or telescopic viewing.
The Summer Triangle is an easy to find group of bright stars that can help point you to interesting
observing targets. Facing south, the Summer Triangle will appear as a large, nearly right triangle defined by the three brightest stars in view. The Summer Triangle contains the alpha stars of three different constellations: Vega in Lyra, Deneb in Cygnus, and Altair in Aquila. This area of the sky is particularly rich since it lies in the plane of the Milky Way. A quick glance through a telescope will uncover dense star fields and gas clouds, such as the Ring Nebula in Lyra. The Summer Triangle also marks the location of the Kepler target stars between Vega and Deneb.
Deneb is the faintest of the trio and is the tail of Cygnus, which is a cross-shaped constellation representing a swan flying roughly to the south. At the head of the swan, nearly halfway between Vega and Altair is a binary star called Alberio. With a telescope, the two stars making up the system can be easily resolved. Albireo is a particularly special binary system because the two stars that make it up are two different colors!
Later in the night, the constellations Pegasus and Andromeda rise in the east. Pegasus contains the “great square” located just east of Cygnus’s wingtip. The constellation Andromeda shares a star with the northernmost corner of the great square. The nearest large galaxy, the Andromeda galaxy is located in this constellation. In especially dark conditions, it can be seen with the naked eye as a fuzzy blob, but in cities and suburbs, it is accessible with binoculars or a small telescope.
Circumpolar constellations are visible throughout the year, but the clear skies of summer can give an observer a great chance to view them as well. Depending on your latitude, the number of circumpolar constellations vary. The closer you are to the poles, the more you will see. However, for the United States and Europe, both the Big and Little Dippers can be seen all night and all year long.
The brighter, Big Dipper can also be used as a guide to find other interesting observing targets. Within the Big Dipper itself, another multiple star system can be seen. With good eyes and a dark sky, the second star in the “handle” of the Big Dipper reveals itself as two stars, called Alcor and Mizar! The system is actually composed of six different stars. Mizar, the brighter, is a quadruple binary system, and Alcor is itself a two-star system. Though a small telescope and binoculars won’t reveal all six stars, they will help you get a better view of the double.
The last two stars of the Big Dipper’s “scoop” point towards the North Star, Polaris, in the Little Dipper. This constellation is fainter, but it is important for navigation. Not only does the star indicate the direction of north, but its elevation from the horizon indicates your latitude. If you travel further north, the Polaris will rise higher and higher in the sky. In the early summer, following the arc of the handle of the Big Dipper allows you to “arc to Arcturus” and find a red giant star in the constellation Bootes. After that, continue to follow the arc and “speed on to Spica,” a blue giant star in Virgo. Other circumpolar constellations visible near the Dippers include Cassiopea, the M or W, and Draco, a faint constellation that snakes its way between the two Dippers and ends near the familiar bright summer star Vega.
As summer comes, take the opportunity provided by clear nights and the end of school to learn some new constellations or telescopic targets. Besides the objects mentioned here, other great telescope and binocular targets are the Messier Objects, a catalogue of galaxies, nebulae, and clusters; or any planets that are visible. Be sure to find a star chart to help you get an accurate picture of what the skies look like at your latitude. Using a red flashlight will help you while working in the dark, but won’t ruin your night vision. Most of all, have fun exploring the night sky!
Printable star charts can be found here: http://www.skymaps.com/downloads.html
Discuss this blog here: http://tinyurl.com/bloginspire12
Friday, June 7, 2013
LiveChat Round Up 6/6/2013
By Jim Gerard, NASA INSPIRE Education Specialist, KSC, FL
Last night's chat with Paulo Younce, a robotics engineer at the Jet Propulsion laboratory in California, gave great insight in to new typrs of robots being planned for future missions. Highlighting Curiosity, Paulo gave a good rundown of the science that has been accomplished in the short time since landing on Mars. He also gave some great tips on how to prepare for a career in robotics.
Because of bandwidth limitations during our chat, we were unable to present the three video clips that went along with the presentation. I've posted these below. If you were not at the chat, look it up in the chat archive to learn more about these robots.
First is the Lemur robot, which can climb a wall or cliff.
Next, is a spider type that may oneday maintain a space telescope mirror.
And finally, a jumping robot. Wait for it....
Next week we hear about Life on Exo-Planets, a prerequisite chat if you are taking the Life On Other Planets VSE. But it is open for everyone one who is interested, whether you are in the VSE or not! So come and have a great time in the INSPIRE Cafe, open at 6pm and then stay for the chat at 8pm (all Central Time).
Discuss this blog here: http://tinyurl.com/bloginspire12
Last night's chat with Paulo Younce, a robotics engineer at the Jet Propulsion laboratory in California, gave great insight in to new typrs of robots being planned for future missions. Highlighting Curiosity, Paulo gave a good rundown of the science that has been accomplished in the short time since landing on Mars. He also gave some great tips on how to prepare for a career in robotics.
Because of bandwidth limitations during our chat, we were unable to present the three video clips that went along with the presentation. I've posted these below. If you were not at the chat, look it up in the chat archive to learn more about these robots.
First is the Lemur robot, which can climb a wall or cliff.
Next, is a spider type that may oneday maintain a space telescope mirror.
And finally, a jumping robot. Wait for it....
Next week we hear about Life on Exo-Planets, a prerequisite chat if you are taking the Life On Other Planets VSE. But it is open for everyone one who is interested, whether you are in the VSE or not! So come and have a great time in the INSPIRE Cafe, open at 6pm and then stay for the chat at 8pm (all Central Time).
Discuss this blog here: http://tinyurl.com/bloginspire12
Monday, June 3, 2013
LEO Progress: RS-25 Adaptation
By William Greene, MSFC, AL
I love dictionaries (yes, I know, you're shocked; shocked!). I have several at home and at work including a two-volume abridged Oxford English Dictionary (OED) that was a wonderful gift from my mother several years ago.
The definitions and word origin above comes from the OED on-line site. Embedded within our language is so much condensed history and accumulated knowledge that it's amazing. While I have no doubt that this is true of every language, I only know my own to any significant degree. Indeed, I've been babbling my own language for a long time now -- forty-some years -- but I can always pick up a dictionary and learn something new with just the flick of a page or two. You really can't say that about too many other things.
As the title for the article and the definitions above suggest, for this article we're going to talk about "adaptation," specifically about adaptation of the RS-25 engine. As part of the Space Launch System Program, we are undertaking something a bit unusual for the world of rocket engines. We are taking engines designed for one vehicle and finding a way to use them on another vehicle. Now, this is not a completely unique circumstance. The Soviets/Russians really were/are masters of this kind of thing. But for us, it is not something that we do very often. In terms of the big NASA program rocket engines, I can only think of the RL10 that was originally part of the Saturn I vehicle as an engine design that has had a long second and even third career on other vehicle systems. The truth is that engines and vehicles are, for us, generally a matched set and the reason is that we just don't frequently enough build that many of either. Note that, technically speaking, we are also adapting the J-2X from a previous program, Constellation/Ares, but that's obviously a bit different in scope and scale given where we are in the development cycle.
The name "RS-25" is, as I've mentioned in past articles, the generic name for the engine that everyone has known for years as the "SSME," i.e., the Space Shuttle Main Engine. There is much to talk about the RS-25. Lots and lots of stuff. More stuff that I could possibly fit into a single article. Here are just some of the RS-25 topics that we'll have to defer to future articles:
• History and evolution
• A tour of the schematic
• Engine control, performance, and capabilities
For this article, I want to just talk about the scope of work that will be necessary to adapt RS-25 to suit the Space Launch System Program.
Clear Communication
The most significant thing that has to be done to the RS-25 to make suitable for the new program is that it has to be able to respond to and talk to vehicle. Remember, the Space Shuttle was developed in the 1970s and first flown in the 1980s. Yes, many things were updated over the years, but given the lightning-fast speed of computer evolution and development, it is not surprising that what RS-25 is carrying around a controller basically can't communicate with the system being developed today for the SLS vehicle. The SLS vehicle would say, "Commence purge sequence three," and the engine would respond, "Like, hey dude, no duh, take a chill pill" and then do nothing (my lame imitation of 1980s slang as best I remember it).
But here are the neato things that we'll be able to do: We can use almost all of the work now completed on the J-2X engine controller hardware to inform the new RS-25 controller and we can use the exact same basic software algorithms from the SSME. Because the RS-25 has a different control scheme from the J-2X, we cannot use the exact controller unit design from J-2X, but we can use a lot of what we've learned over the past few years. And, because we can directly port over the basic control algorithms, we don't have to re-validate these vital pieces from the ground up. We just have to validate their operation within the new controller. That's a huge savings.
This is work that is happening right now, as I'm typing. Pratt & Whitney Rocketdyne, the RS-25 developer and manufacturer, is working together with Honeywell International, the electronic controller developer, on this activity. Within the next couple of months, they will have progressed beyond the point of the critical design review for both the hardware and software.
In the long term, it is our hope that we will evolve to the utopian plain of having one universal engine controller, a "common engine controller," that can be easily fitted to any engine, past, present, or future. Such a vision has in mind a standardization of methods and architecture such that we could largely minimize controller development efforts in the future to the accommodation of obsolescence issues. The simple truth is that development work is always expensive. It would be nice to avoid as much as that cost as possible. With the new RS-25 controller, we're getting pretty close to that kind of situation.
Under Pressure
Have you ever spent much time thinking about water towers? As in, for instance, why are they
towers in the first place? As you might have guessed, this is something that I wondered about many years ago as a pre-engineering spud. They seemed to be an awfully silly thing to build when you could just turn on the faucet and have water spurt out whenever you want. Ah, the wonderful simplicity of childhood logic: Things work just because they do and every day is Saturday.
The reason that you go to the trouble of sticking water way up in a tower is so that you have a reliable source of water pressure that can absorb the varying demands on the overall system. In the background, you can have a little pump going "chug, chug, chug" twenty-four hours per day pushing water all of the way up there, but by having this large, reserve quantity always in the tower, the system can respond with sufficient pressure when, at six in the morning, everyone in town happens to turn on the shower at the same time to start their day. The pressure comes from the elevation of tower, the height of the column of water from top to bottom.
On the Space Launch System vehicle we have something of a water tower situation except that, in this case, we're dealing with liquid oxygen. In the picture below, you can see roughly scaled images of the Space Shuttle and the Block 2 Space Launch System vehicle. On both of these vehicles, the liquid oxygen tank is above the liquid hydrogen tank. This means that for the very tall SLS vehicle, the top of oxygen tank is approximately fifty feet higher relative to the inlet to the engines (as illustrated). This additional fifty feet of elevation translates to more pressure at the bottom just as if it were a taller water tower. However, in this case liquid oxygen is heavier than water (meaning more pressure) and the SLS vehicle will be flying, sometimes, at accelerations much higher than a water tower sitting still in the Earth's gravitational field. Greater acceleration also amplifies the pressure seen by the engines at the bottom of the rocket.
"So what?" you're saying to yourself as you read this. After all, higher pressure is a good thing, right? If you have more pressure at the inlet to the engine, then you don't need as much pumping power. So, life should be easier for the engines with this longer, taller configuration. There are two reasons why this is not quite the case.
First, think about when the vehicle is sitting on the pad at the point of engine start. The pumps aren't spinning so all the pressure you're dealing with is coming from the propellant feed system. And now, simply, for the SLS vehicle it will be different than before. One of the tricky things about a staged-combustion engine, in general, is that the start sequence (i.e., the sequence of opening valves, igniting combustion, getting turbopumps spun up) is touchy. Given that the RS-25 has two separate pre-burners -- and therefore three separate combustion zones -- and four separate turbopumps, the RS-25 start sequence especially touchy. You have to maintain a very careful balance of combustion mixture ratios that allow things to light robustly, but not too hot, and a careful balance of pressures throughout the system so as to keep the flow headed in the right direction and keep the slow build to full power level as smooth as possible. We have an RS-25 start sequence that works for Space Shuttle. Now, for the SLS vehicle, we will have to modify it to adapt to these new conditions.
The second issue to overcome with regards to the longer vehicle configuration and the liquid oxygen inlet conditions is due total range of pressures that the engines have to accommodate. When sitting on the launch pad, you have the pressure generated by the acceleration of gravity. During flight, as you're burning up and expelling propellants, the vehicle is getting lighter and lighter and you're accelerating faster and faster, you can reach the equivalent of three or four times the acceleration of gravity. So that's the top end pressure.
On the low end, you have the effect of when the boosters burn out and are ejected at approximately two minutes into flight. When this happens, the acceleration of the vehicle usually becomes less than the acceleration of gravity meaning that the propellant pressure at the bottom of the column of liquid oxygen can get pretty low. Momentarily, the vehicle seems to hang, almost seemingly falling, despite the fact that the RS-25 engines continue to fire. Pretty quickly, however, the process of picking up acceleration begins again. (In the movie Apollo 13, they illustrated a similar effect with the separation of the first and second stages of Saturn V. The astronauts are pushed back in their seats by the acceleration until, boom, first stage shutdown and separation happens and they're effectively thrown forward. With the Space Shuttle and the SLS vehicle, however, the return to acceleration is not as abrupt as it was on Saturn V where they show the astronauts slammed back into their seats with the lighting of the second stage.) The point is that the RS-25 has to accommodate a very wide range of inlet pressures while maintaining a set thrust level and engine mixture ratio. While this has always been the case for the SSME/RS-25, the longer SLS vehicle configuration simply exacerbates the situation.
You'll note that I've not talked about the liquid hydrogen here. That's because, as I've mentioned in the past, liquid hydrogen is very, very light. Think of fat-free, artificial whipped cream. Yes, the top of the hydrogen tank is much higher, but due to the lightness of the liquid, it doesn't make much difference at the engine inlet even when the vehicle is accelerating at several times the acceleration of gravity.
Some Like it...Insulated
Look again at the pictorial comparison of the Space Shuttle and the Space Launch System vehicles shown above. Do you see where the SSME/RS-25 engines are relative to the big boosters on the sides of the vehicles? On the Space Shuttle, the engines were on the Orbiter and they were forward of the booster nozzles. On the SLS vehicle, there is no Orbiter so the engines are right on the bottom of the tanks and their exit planes line up with the booster nozzle exit planes. In short, the engines are now closer to those great big, loud, powerful, and HOT boosters. We are in the process now of determining whether this poses any thermal environments issues for the RS-25. Thus far, based upon analyses to date, there do not appear to be any thermal issues that cannot be obviated through the judicious use of insulation.
Other environments also have to be checked such as the dynamic loads transmitted to the engine through the vehicle or the acoustic loads or whatever else is different for this vehicle. The point is not that all of these environments are necessarily worse than what they were on the Space Shuttle. It is only that they all need to be checked to make sure that our previous certification of the engine is still valid for all of these considerations.
The Tropic of Exploration
So those are the three most obvious and primary pieces of the RS-25 adaptation puzzle: a new engine controller, dealing with different propellant inlet conditions, and understanding the new vehicle and mission environments. Each of these pieces carries with it analysis and testing and the appropriate documentation so there is plenty of work scope to accomplish. We are extremely lucky to be starting with an engine of such extraordinary pedigree, performance, and flexibility.
Henry Miller once said, "Whatever there be of progress in life comes not through adaptation but through daring." It is our intent to prove Mr. Miller wrong in this case. We will make progress by using the adaptation of RS-25 to enable the daring of our exploration mission.
Discuss this blog here: http://tinyurl.com/bloginspire12
I love dictionaries (yes, I know, you're shocked; shocked!). I have several at home and at work including a two-volume abridged Oxford English Dictionary (OED) that was a wonderful gift from my mother several years ago.
The definitions and word origin above comes from the OED on-line site. Embedded within our language is so much condensed history and accumulated knowledge that it's amazing. While I have no doubt that this is true of every language, I only know my own to any significant degree. Indeed, I've been babbling my own language for a long time now -- forty-some years -- but I can always pick up a dictionary and learn something new with just the flick of a page or two. You really can't say that about too many other things.
As the title for the article and the definitions above suggest, for this article we're going to talk about "adaptation," specifically about adaptation of the RS-25 engine. As part of the Space Launch System Program, we are undertaking something a bit unusual for the world of rocket engines. We are taking engines designed for one vehicle and finding a way to use them on another vehicle. Now, this is not a completely unique circumstance. The Soviets/Russians really were/are masters of this kind of thing. But for us, it is not something that we do very often. In terms of the big NASA program rocket engines, I can only think of the RL10 that was originally part of the Saturn I vehicle as an engine design that has had a long second and even third career on other vehicle systems. The truth is that engines and vehicles are, for us, generally a matched set and the reason is that we just don't frequently enough build that many of either. Note that, technically speaking, we are also adapting the J-2X from a previous program, Constellation/Ares, but that's obviously a bit different in scope and scale given where we are in the development cycle.
The name "RS-25" is, as I've mentioned in past articles, the generic name for the engine that everyone has known for years as the "SSME," i.e., the Space Shuttle Main Engine. There is much to talk about the RS-25. Lots and lots of stuff. More stuff that I could possibly fit into a single article. Here are just some of the RS-25 topics that we'll have to defer to future articles:
• History and evolution
• A tour of the schematic
• Engine control, performance, and capabilities
For this article, I want to just talk about the scope of work that will be necessary to adapt RS-25 to suit the Space Launch System Program.
Clear Communication
The most significant thing that has to be done to the RS-25 to make suitable for the new program is that it has to be able to respond to and talk to vehicle. Remember, the Space Shuttle was developed in the 1970s and first flown in the 1980s. Yes, many things were updated over the years, but given the lightning-fast speed of computer evolution and development, it is not surprising that what RS-25 is carrying around a controller basically can't communicate with the system being developed today for the SLS vehicle. The SLS vehicle would say, "Commence purge sequence three," and the engine would respond, "Like, hey dude, no duh, take a chill pill" and then do nothing (my lame imitation of 1980s slang as best I remember it).
But here are the neato things that we'll be able to do: We can use almost all of the work now completed on the J-2X engine controller hardware to inform the new RS-25 controller and we can use the exact same basic software algorithms from the SSME. Because the RS-25 has a different control scheme from the J-2X, we cannot use the exact controller unit design from J-2X, but we can use a lot of what we've learned over the past few years. And, because we can directly port over the basic control algorithms, we don't have to re-validate these vital pieces from the ground up. We just have to validate their operation within the new controller. That's a huge savings.
This is work that is happening right now, as I'm typing. Pratt & Whitney Rocketdyne, the RS-25 developer and manufacturer, is working together with Honeywell International, the electronic controller developer, on this activity. Within the next couple of months, they will have progressed beyond the point of the critical design review for both the hardware and software.
In the long term, it is our hope that we will evolve to the utopian plain of having one universal engine controller, a "common engine controller," that can be easily fitted to any engine, past, present, or future. Such a vision has in mind a standardization of methods and architecture such that we could largely minimize controller development efforts in the future to the accommodation of obsolescence issues. The simple truth is that development work is always expensive. It would be nice to avoid as much as that cost as possible. With the new RS-25 controller, we're getting pretty close to that kind of situation.
Under Pressure
Have you ever spent much time thinking about water towers? As in, for instance, why are they
towers in the first place? As you might have guessed, this is something that I wondered about many years ago as a pre-engineering spud. They seemed to be an awfully silly thing to build when you could just turn on the faucet and have water spurt out whenever you want. Ah, the wonderful simplicity of childhood logic: Things work just because they do and every day is Saturday.
The reason that you go to the trouble of sticking water way up in a tower is so that you have a reliable source of water pressure that can absorb the varying demands on the overall system. In the background, you can have a little pump going "chug, chug, chug" twenty-four hours per day pushing water all of the way up there, but by having this large, reserve quantity always in the tower, the system can respond with sufficient pressure when, at six in the morning, everyone in town happens to turn on the shower at the same time to start their day. The pressure comes from the elevation of tower, the height of the column of water from top to bottom.
On the Space Launch System vehicle we have something of a water tower situation except that, in this case, we're dealing with liquid oxygen. In the picture below, you can see roughly scaled images of the Space Shuttle and the Block 2 Space Launch System vehicle. On both of these vehicles, the liquid oxygen tank is above the liquid hydrogen tank. This means that for the very tall SLS vehicle, the top of oxygen tank is approximately fifty feet higher relative to the inlet to the engines (as illustrated). This additional fifty feet of elevation translates to more pressure at the bottom just as if it were a taller water tower. However, in this case liquid oxygen is heavier than water (meaning more pressure) and the SLS vehicle will be flying, sometimes, at accelerations much higher than a water tower sitting still in the Earth's gravitational field. Greater acceleration also amplifies the pressure seen by the engines at the bottom of the rocket.
"So what?" you're saying to yourself as you read this. After all, higher pressure is a good thing, right? If you have more pressure at the inlet to the engine, then you don't need as much pumping power. So, life should be easier for the engines with this longer, taller configuration. There are two reasons why this is not quite the case.
First, think about when the vehicle is sitting on the pad at the point of engine start. The pumps aren't spinning so all the pressure you're dealing with is coming from the propellant feed system. And now, simply, for the SLS vehicle it will be different than before. One of the tricky things about a staged-combustion engine, in general, is that the start sequence (i.e., the sequence of opening valves, igniting combustion, getting turbopumps spun up) is touchy. Given that the RS-25 has two separate pre-burners -- and therefore three separate combustion zones -- and four separate turbopumps, the RS-25 start sequence especially touchy. You have to maintain a very careful balance of combustion mixture ratios that allow things to light robustly, but not too hot, and a careful balance of pressures throughout the system so as to keep the flow headed in the right direction and keep the slow build to full power level as smooth as possible. We have an RS-25 start sequence that works for Space Shuttle. Now, for the SLS vehicle, we will have to modify it to adapt to these new conditions.
The second issue to overcome with regards to the longer vehicle configuration and the liquid oxygen inlet conditions is due total range of pressures that the engines have to accommodate. When sitting on the launch pad, you have the pressure generated by the acceleration of gravity. During flight, as you're burning up and expelling propellants, the vehicle is getting lighter and lighter and you're accelerating faster and faster, you can reach the equivalent of three or four times the acceleration of gravity. So that's the top end pressure.
On the low end, you have the effect of when the boosters burn out and are ejected at approximately two minutes into flight. When this happens, the acceleration of the vehicle usually becomes less than the acceleration of gravity meaning that the propellant pressure at the bottom of the column of liquid oxygen can get pretty low. Momentarily, the vehicle seems to hang, almost seemingly falling, despite the fact that the RS-25 engines continue to fire. Pretty quickly, however, the process of picking up acceleration begins again. (In the movie Apollo 13, they illustrated a similar effect with the separation of the first and second stages of Saturn V. The astronauts are pushed back in their seats by the acceleration until, boom, first stage shutdown and separation happens and they're effectively thrown forward. With the Space Shuttle and the SLS vehicle, however, the return to acceleration is not as abrupt as it was on Saturn V where they show the astronauts slammed back into their seats with the lighting of the second stage.) The point is that the RS-25 has to accommodate a very wide range of inlet pressures while maintaining a set thrust level and engine mixture ratio. While this has always been the case for the SSME/RS-25, the longer SLS vehicle configuration simply exacerbates the situation.
You'll note that I've not talked about the liquid hydrogen here. That's because, as I've mentioned in the past, liquid hydrogen is very, very light. Think of fat-free, artificial whipped cream. Yes, the top of the hydrogen tank is much higher, but due to the lightness of the liquid, it doesn't make much difference at the engine inlet even when the vehicle is accelerating at several times the acceleration of gravity.
Some Like it...Insulated
Look again at the pictorial comparison of the Space Shuttle and the Space Launch System vehicles shown above. Do you see where the SSME/RS-25 engines are relative to the big boosters on the sides of the vehicles? On the Space Shuttle, the engines were on the Orbiter and they were forward of the booster nozzles. On the SLS vehicle, there is no Orbiter so the engines are right on the bottom of the tanks and their exit planes line up with the booster nozzle exit planes. In short, the engines are now closer to those great big, loud, powerful, and HOT boosters. We are in the process now of determining whether this poses any thermal environments issues for the RS-25. Thus far, based upon analyses to date, there do not appear to be any thermal issues that cannot be obviated through the judicious use of insulation.
Other environments also have to be checked such as the dynamic loads transmitted to the engine through the vehicle or the acoustic loads or whatever else is different for this vehicle. The point is not that all of these environments are necessarily worse than what they were on the Space Shuttle. It is only that they all need to be checked to make sure that our previous certification of the engine is still valid for all of these considerations.
The Tropic of Exploration
So those are the three most obvious and primary pieces of the RS-25 adaptation puzzle: a new engine controller, dealing with different propellant inlet conditions, and understanding the new vehicle and mission environments. Each of these pieces carries with it analysis and testing and the appropriate documentation so there is plenty of work scope to accomplish. We are extremely lucky to be starting with an engine of such extraordinary pedigree, performance, and flexibility.
Henry Miller once said, "Whatever there be of progress in life comes not through adaptation but through daring." It is our intent to prove Mr. Miller wrong in this case. We will make progress by using the adaptation of RS-25 to enable the daring of our exploration mission.
Discuss this blog here: http://tinyurl.com/bloginspire12
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