Weekly Space Hangout – Mar 31, 2017: The IDATA Project and Afterglow Access

Host: Fraser Cain (@fcain)

Special Guest:
This week’s special guests are Timothy Spuck, Kathryn Meredith, Dr. James Hammerman and Andreas Stefik of the Innovators Developing Accessible Tools for Astronomy (IDATA) Project Team. The IDATA project aims to design and develop Afterglow Access, a new software tool that will expand accessibility beyond touch, making the universe more accessible to those with visual impairments.

Yerkes Outreach website
Tim Spuck (email: [email protected]) (Associated Universities Inc. STEM Education Development Officer and IDATA PI) currently serves as PI on three NSF supported programs including, Innovators Developing Accessible Tools for Astronomy, the Chile-US Astronomy Education Outreach Summit, and the Astronomy in Chile Educator Ambassadors Program. Tim also remains active within the amateur astronomy community, has directed numerous outreach efforts, and led several small-scale observatory design and construction projects. He earned his Masters degree in Science Education from Clarion University or PA, and is completing his Ed.D. in Curriculum & Instruction at West Virginia University.

Kate Meredith (Yerkes Observatory – University of Chicago, Director of Education Outreach, and IDATA Project Educator) has engaged in curriculum development and project management for the Zooniverse, the Sloan Digital Sky Survey, the Lawrence Hall of Science, the Adler Planetarium Space and Science Museum, and Skynet Junior Scholars (University of Chicago Yerkes Observatory). Kate is passionate about programs that bring authentic research science to learners of all ages, languages, and abilities. As Education Lead on the IDATA project, Kate looks forward to being part of the team that takes accessibility to the next level by creating vision-neutral data acquisition and analysis tools as well as the instructional materials needed to teach new users how to use and apply those tools.

Dr. James K. L. Hammerman (TERC, Co-Director of SEEC and Senior Researcher and Evaluator, IDATA Co-PI) currently leads external evaluations for several projects, including an immersive computer environment for conducting experiments to explore causality and ecology, a state-wide initiative to engage rural youth in computing through programming an online game, and an effort to improve pedagogy among university STEM faculty. Jim has designed, implemented, and researched mathematics and science education curricula and professional development programs, as well as technology tools that support inquiry-oriented learning. Jim is especially interested in adult developmental differences in professional development, data and statistics learning, online and software tools that support exploration, and supporting deeper learning and more reflective practice in professional communities.

Andreas Stefik (University of Nevada – Las Vegas, Assistant Professor of Computer Science and IDATA Co-PI) – For the last decade, Dr. Stefik has been creating technologies that make it easier for people, including those with disabilities, to write computer software. With grants from the National Science Foundation, he helped establish the first national educational infrastructure for blind or visually impaired students to learn computer science. He is the inventor of Quorum, the first evidence-oriented programming language. As part of his work, he is a PI on the NSF-funded AccessCS10K grant that is helping CS 10K projects prepare K-12 teachers to be more inclusive in their computing courses with students with disabilities. Most recently, Dr. Stefik was honored with the 2016 White House Champions of Change award in computer science education.

Accessibility links mentioned in the show:
Quorum Language
CS for All
CS for All links

Guests:
Morgan Rehnberg (MorganRehnberg.com / @MorganRehnberg)

Their stories this week:

SpaceX relaunches a rocket for the first time

NASA fleshed out its human Mars program

We use a tool called Trello to submit and vote on stories we would like to see covered each week, and then Fraser will be selecting the stories from there. Here is the link to the Trello WSH page (http://bit.ly/WSHVote), which you can see without logging in. If you’d like to vote, just create a login and help us decide what to cover!

If you would like to join the Weekly Space Hangout Crew, visit their site here and sign up. They’re a great team who can help you join our online discussions!

If you’d like to join Fraser and Paul Matt Sutter on their tour to Iceland in February 2018, you can find the information at astrotouring.com.

We record the Weekly Space Hangout every Friday at 12:00 pm Pacific / 3:00 pm Eastern. You can watch us live on Universe Today, or the Universe Today YouTube page

ARCA Unveils the World’s first Single-Stage-to-Orbit Rocket

Artist's impression of the Haas 2CA deployed to orbit. Credit: ARCA

Since the beginning of the Space Age, scientists have relied on multi-stage rockets in order to put spacecraft and payloads into orbit. The same technology has allowed for missions farther into space, sending robotic spacecraft to every planet in the Solar System, and astronauts to the Moon. But looking to the future, it is clear that new ideas will be needed in order to cut costs and expand launch services.

Hence why the ARCA Space Corporation has developed a concept for a single-stage-to-orbit (SSTO) rocket. It’s known as the Haas 2CA, the latest in  a series of rockets being developed by the New Mexico-based aerospace company. If all goes as planned, this rocket will be the first SSTO rocket in history, meaning it will be able to place payloads and crew into Earth’s orbit relying on only one stage with one engine.

The rocket was unveiled on Tuesday, March 28th, at their company headquarters in Las Cruces. The rocket is currently seeking FAA approval, and ARCA is working diligently to get it ready for its test launch in 2018 – which will take place at NASA’s Wallops Flight Facility located on Virginia’s eastern shore. If successful, the company hopes to use this rocket to deploy small satellites to orbit in the coming decade.

Artist’s impression of the Haas 2C rocket ascending into orbit. Credit: ARCA

Established in 1999 by a group of Romanian rocket enthusiasts (led by company CEO Dumitru Popescu), ARCA’s original focus was on balloon-launched rockets. In the course of the company’s history, ARCA has launched two stratospheric rockets, four large scale stratospheric balloons, and has been awarded some lucrative governmental contracts to test aerospace and space exploration technologies.

In 2003, the company joined the $10 million Ansari X Prize Competition and began work on their first demonstrator rocket. Known as the Demonstrator 2B – a single stage suborbital rocket – the rocket was successfully launched on September 9th, 2004, from Cape Midia Air Force Base. In the years that followed, they expanded their repertoire to include other concepts – like the Helen rocket, the Stabilo crewed vehicle, and the Excelsior Aerospike.

In 2013, ARCA was contracted by the European Space Agency (ESA) to create a Drop Test Vehicle (DTV) that would test the atmospheric deceleration parachutes being used by the Schiaperelli lander (as part of the ExoMars mission). Being the same weight and using the same parachute deployment systems as Schiaperelli, the DTV conducted a freefall exercise which simulated the dynamic pressure conditions of entering the Martian atmosphere

In that same year, ARCA relocated to New Mexico, where they have continued working on their rocket series and other aerospace ventures from their headquarters at the Las Cruces Airport. It was here that they introduced the Haas rocket series – named in honor of Austrian-Romanian rocketry pioneer Conrad Haas – which now consists of the Haas 2B and 2C rockets.

The Haas 2CA rocket berthed at ARCA’s headqaurters at Las Cruces Air Port in Las Cruces, New Mexico. Credit: ARCA

The 2B is a proven concept, designed for suborbital flight for the sake of space tourism. But as of this week, the 2C is now part of ARCA’s rocket family. Relying on single stage and single Executor engine, this rocket will small satellites into orbit. The rocket is fueled by hydrogen peroxide and kerosene (which combines to create a nontoxic fuel), and measures (53 feet) long and (5 feet) in diameter.

The 2C weights about 550 kg (1210 pounds) empty, and 16280 kg (35,887 pounds) when fully fueled. It will also be able to provide 22900 kg (50,500 lbs) of thrust at sea level, and about 33,565 kg (74,000 lbs) in a vacuum. In this configuration, the rocket is capable of delivering 100kg (220lbs) to Low Earth Orbit (LEO), at a cost of $1 million per launch (or $10,000/kg; $4,545/lb).

This several times less what SpaceX can do with its Falcon 9 rocket, which can deliver 22,800 km payloads to orbit for $62 million a launch – which works out to about $2719/kg or $1233/lb. However, one must take into account that the Falcon 9 is a heavier launch vehicle, and that there are additional issues that come into play where larger launch vehicles are concerned. As Dumitru Popescu told Universe Today via email:

“With the Haas 2C, the customer can launch on the desired orbit parameter, when he/she wants. Basically, the launch will be tailored on the customer needs. A more fair comparison will be between the Haas 2CA and Falcon 1 and Electron. Falcon 1 had a launch cost of $6.7 millions for a proposed payload of 670kg, or a demonstrated one of 180kg. In the best case scenario, this leads us to the same price of $10,000/kg. In the case of the Electron rocket, the cost per launch is $4.9 million for a 150kg payload. This leads us to a price of a $32.600/kg. Falcon 1, Electron, Haas 2CA have their market and a comparison with a big launcher isn’t fair in my opinion. Overall, if we will be able to keep this price, the Haas 2CA, at $1 million/launch will become the cheapest launcher in history.”

Artist’s impression of the Haas 2C rocket, shown in its launch (top) and deployment configurations (bottom). Credit: ARCA

In addition, the Haas 2C rocket benefits from the fact that it is cheaper and easier to manufacture, and that it’s SSTO configuration offers greater flexibility and reliability. 

“In the case of staged rockets, we are literally talking about more rockets combined in one vehicle to achieve orbit,” said Popsecu. “It is definitely more cost effective to operate one rocket than a vehicle made of multiple rockets, as it requires less time, less qualified manpower and less demanding transport and launch operations. The SSTO may also offer the possibility to launch from an inland spaceport, as there are no first stages that will fall on the ground after burnout.”

To prepare the rocket for its 2018 launch, ARCA is currently collaborating with NASA through its Cooperative Opportunity Program and with the help of the Ames, Kennedy, Marshall,  Stennis, and Johnson Space Centers. Popescu is also entering into discussions with the New Mexico Spaceport Authority to conduct launches from Spaceport America, and is looking to secure a partnership with a US defense agency.

If all goes well, this little aerospace company will be making spaceflight history. As Popescu said in a company press release:

“When the Haas 2CA rocket launches, it will be the first rocket in history to place itself entirely into orbit. This opens new frontiers for exploration of the Solar System as the rocket can be refueled in-orbit and re-utilize its aerospike engine thus eliminating the need for additional upper stages. After the full qualification, the vehicle could be operated from inland spaceports as there are no stages that fall on the ground at burnout. Staged rockets, even though they provide more payload performance for the same takeoff mass, are less reliable because of an increased number of parts due to flight events requested by staging and ignition of the upper stage engine. Also, staged rockets are deemed to be more expensive because they are literally made up of more than one rocket. Manufacturing and assembling more rockets in one launcher requires more, time, money, and personnel. The SSTO technology, once implemented, will increase the space flight responsiveness and lower the cost to values expected by the industry for decades. This rocket will also be the fastest vehicle to reach orbit, taking less than 5 minutes.”

In addition, the aerospace industry will have another company looking to lower the costs of launches and expanding domestic launch capability. Be sure to check out the company’s video detailing the Haas 2C and its unique characteristics:

Further Reading: ARCA

SpaceX Accomplishes American ‘Science Triumph’ with ‘Mind Blowing’ Historic 2nd Launch and Landing of Used Rocket

The ‘used’ SpaceX Falcon 9 launches the SES-10 telecomsat to orbit from historic Launch Complex 39A as it zooms past US Flag by the countdown clock at NASA’s Kennedy Space Center in Florida at 6:27 p.m. EDT on March 30, 2017. Credit: Ken Kremer/Kenkremer.com
The ‘used’ SpaceX Falcon 9 launches the SES-10 telecomsat to orbit from historic Launch Complex 39A as it zooms past US Flag by the countdown clock at NASA’s Kennedy Space Center in Florida at 6:27 p.m. EDT on March 30, 2017. Credit: Ken Kremer/Kenkremer.com

KENNEDY SPACE CENTER, FL – SpaceX accomplished an American ‘Science Triumph’ with today’s “Mind Blowing” and history making second launch and landing of a previously flown Falcon 9 booster that successfully delivered a massive and powerful Hi Def TV satellite to orbit for telecom giant SES from the Kennedy Space Center. Note: Breaking News story being updated.

The milestone SpaceX mission to refly the first ever ‘used rocket’ blasted off right on time at dinnertime today, Thursday, March 30, at 6:27 p.m. EDT. It carried the SES-10 telecommunications payload to orbit atop a ‘Flight-Proven’ Falcon 9 rocket from seaside Launch Complex 39A at NASA’s Kennedy Space Center in Florida.

The recycled Falcon delivered the nearly six ton SES-10 satellite to geostationary transfer orbit where it will provide significantly improved TV, voice, data and maratime service to over 37 million customers across Central and South America.

The daring mission to relaunch a used booster dubbed ‘Flight-Proven’ seems like its straight out of a science fiction thriller.

Yet today’s stellar results fully vindicates billionaire SpaceX CEO and Chief Designer Elon Musk’s bold vision to slash launch costs by recovering and reusing spent first stage rockets from his firms Falcon 9 launch vehicle.

“My mind is blown,” Musk said in post launch remarks at the KSC press site. “This is one of the coolest things ever.”

“We just had an incredible day today – the first re-flight of an orbital-class booster.”

“It did its mission perfectly, dropped off the second stage, came back and landed on the drone ship, right on the bullseye. It’s an amazing day, I think, for space as a whole, for the space industry.”

Recycled SpaceX Falcon 9 skyrockets to orbit with SES-10 telecomsat from historic Launch Complex 39A as it zooms past US Flag by the countdown clock at NASA’s Kennedy Space Center in Florida at 6:27 p.m. EDT on March 30, 2017. Credit: Ken Kremer/Kenkremer.com

For the first time in world history a recovered and ‘Flight-Proven’ rocket has actually launched on a second mission and not only roared aloft but survived intact all the way to its intended orbit and delivered a second satellite to orbit for a paying customer- in this case the commercial TV broadcast satellite provider SES- one of the world’s largest.

“This will rock the space industry,” said SES CTO Martin Halliwell at the post launch media briefing. “And SpaceX already has!”

“We are confident in this booster,” Halliwell told me at a prelaunch press briefing on March 28.

“There is not a huge risk,” Halliwell stated emphatically. “In this particular case we know that the reusability capability is built into the design of the Falcon 9 vehicle.”

Reflown SpaceX Falcon 9 soars to orbit with SES-10 telecomsat from historic Launch Complex 39A at NASA’s Kennedy Space Center in Florida at 6:27 p.m. EDT on March 30, 2017. Credit: Ken Kremer/Kenkremer.com

This recycled Falcon 9 first stage booster had initially launched in April 2016 for NASA on the SpaceX Dragon CRS-8 resupply mission to the International Space Station (ISS) under contract for the space agency.

Furthermore, after the 156 foot tall first stage booster completed its primary mission task, SpaceX engineers successfully guided it to a second landing on the tiny OCISLY drone ship for a soft touchdown some eight and a half minutes after liftoff.

OCISLY had left Port Canaveral several days ahead of the March 30 launch and was prepositioned in the Atlantic Ocean some 400 miles (600 km) off the US East coast, just waiting for the boosters 2nd history making approach and pinpoint propulsive soft landing.

It thus became the first booster in history to launch twice and land twice.

SpaceX CEO and Chief Designer Elon Musk and SES CTO Martin Halliwell exuberantly shake hands of congratulation following the successful delivery of SES-10 TV comsat to orbit using the first reflown and flight proven booster in world history at the March 30, 2017 post launch media briefing at NASA’s Kennedy Space Center in Florida. Credit: Ken Kremer/Kenkremer.com

And this magnificent achievement was accomplished through the dedication and hard work of engineers and scientists who benefited from the American education system that cultivated and nurtured their talents – like generations before them – and that we as a country must continue to support and fortify with reliable and ample research and development (R&D) and educational funding – now and in the future – if we wish to remain leaders in science and space.

The entire Falcon 9/SES-10 launch and landing was broadcast live on the SpaceX hosted webcast.

SpaceX Falcon 9 recycled rocket carrying SES-10 telecomsat raised erect atop Launch Complex 39A at the Kennedy Space Center as seen from inside the pad ahead of liftoff slated for 6:27 p.m on 30 Mar 2017 on world’s first reflight of an orbit class rocket. Credit: Ken Kremer/Kenkremer.com

Watch for Ken’s continuing coverage direct from onsite at the Kennedy Space Center press site and Cape Canaveral Air Force Station.

Stay tuned here for Ken’s continuing Earth and Planetary science and human spaceflight news.

Ken Kremer

………….

Learn more about SpaceX SES-10, EchoStar 23 and CRS-10 launches to ISS, ULA SBIRS GEO 3 launch, GOES-R launch, Heroes and Legends at KSCVC, OSIRIS-REx, InSight Mars lander, Juno at Jupiter, SpaceX AMOS-6, ISS, ULA Atlas and Delta rockets, Orbital ATK Cygnus, Boeing, Space Taxis, Mars rovers, Orion, SLS, Antares, NASA missions and more at Ken’s upcoming outreach events at Kennedy Space Center Quality Inn, Titusville, FL:

Mar 31, Apr 1: “SpaceX SES-10, EchoStar 23, CRS-10 launch to ISS, ULA Atlas SBIRS GEO 3 launch, GOES-R weather satellite launch, OSIRIS-Rex, SpaceX and Orbital ATK missions to the ISS, Juno at Jupiter, ULA Delta 4 Heavy spy satellite, SLS, Orion, Commercial crew, Curiosity explores Mars, Pluto and more,” Kennedy Space Center Quality Inn, Titusville, FL, evenings

SpaceX Falcon 9 recycled rocket carrying SES-10 telecomsat poised atop Launch Complex 39A at the Kennedy Space Center ahead of liftoff slated for 6:27 p.m. on 30 Mar 2017 on world’s first reflight of an orbit class rocket. Credit: Ken Kremer/Kenkremer.com

The SES-10 satellite was manufactured by Airbus Defence & Space and is based on the Eurostar E3000 platform. It will operate in geostationary orbit.Credit: SES/Airbus
SpaceX Falcon 9 booster from Thaicom-8 launch on May 27, 2016 arrives at mouth of Port Canaveral, FL on June 2, 2016. Credit: Ken Kremer/kenkremer.com

The Ever-Working Mars Orbiter Passes 50,000 Orbits

This image is a mosaic of all the images captured by the Context Camera (CTX) on NASA's Mars Reconnaissance Orbiter. The CTX has imaged over 99% of the Martian surface. Image: NASA/JPL-Caltech/MSSS

Most of us never do one thing 50,000 times in our life. So for NASA’s Mars Reconnaissance Orbiter (MRO), completing 50,000 orbits around the red planet is a big deal. And, it only took 10 years to do so.

The MRO could be called one of NASA’s flagship missions. It’s presence in orbit around Mars has helped open up our understanding of that planet immensely. And it’s done so while providing us a steady stream of eye candy.

This recent image from MRO’s HiRise camera shows dune structure inside an impact crater. Image: NASA/JPL/University of Arizona

MRO was launched in 2005 and reached Mars orbit in March, 2006. After 10 years at work, it has accomplished a lot. In a recent press release, NASA calls the MRO “the most data-productive spacecraft yet.” Though most of us might know the orbiter because of it’s camera, the High-Resolution Imaging Science Experiment (HiRise), the MRO actually has a handful of other instruments that help the orbiter achieve its objectives. In broad terms, those objectives are:

  • to study the history of water on Mars
  • to look at small scale features on the surface, and identify landing sites for future Mars missions
  • to act as a communications relay between Mars and Earth
MRO investigating Martian water cycle – This artist’s concept represents the “Follow the Water” theme of NASA’s Mars Reconnaissance Orbiter mission. The orbiter’s science instruments monitor the present water cycle in the Mars atmosphere and the associated deposition and sublimation of water ice on the surface, while probing the subsurface to see how deep the water-ice reservoir extends. Image: By NASA/JPL/Corby Waste – http://photojournal.jpl.nasa.gov/catalog/PIA07241 (image link), Public Domain, https://commons.wikimedia.org/w/index.php?curid=374810 (Larger image here.

MRO’s HiRise camera gets all the glory, but it’s another onboard camera, the Context Camera (CTX), that is the real workhorse. The CTX is a much lower resolution than the HiRise, but its file sizes are much more manageable, an important consideration when every file has to travel from Mars to Earth—an average distance of about 225 million km.

CTX has captured 90,000 images so far in MRO’s mission, and each one captures details smaller than a tennis court. In the course of the mission so far, CTX has images that cover 99.1% of the Martian surface. Over 60% of the planet has been covered twice.

“Reaching 99.1-percent coverage has been tricky…” – Context Camera Team Leader Michael Malin

“Reaching 99.1-percent coverage has been tricky because a number of factors, including weather conditions, coordination with other instruments, downlink limitations, and orbital constraints, tend to limit where we can image and when,” said Context Camera Team Leader Michael Malin of Malin Space Science Systems, San Diego.

Malin said, “Single coverage provides a baseline we can use for comparison with future observations, as we look for changes. Re-imaging areas serves two functions: looking for changes and acquiring stereoscopic views from which we can make topographic maps.”

Because the CTX captures image of the same surface areas twice, it documents changes on the surface. There have been over 200 instances of impact craters appearing in a second image of the same area. Scientists have used this to calculate the rate that meteorites impact Mars.

The instruments on board the MRO work as a team. The CTX can capture images of areas of interest, and the HiRise can be used for higher-resolution images of the same area. By locating fresh impact craters, then studying them more closely, the MRO has helped discover the presence of what looked like sub-surface ice on Mars. A third instrument, the Compact Reconnaissance Imaging Spectrometer for Mars (CRISM), confirmed the presence of ice.

The CTX is the workhorse camera, and the HiRise is the diva, but MRO actually has a third camera: the Mars Color Imager (MARCI). MARCI is a very low resolution camera compared to the others. It’s also a wide-angle camera with really only one purpose: characterizing Martian weather. Every day, MARCI takes about 84 images which together create a daily global map of Mars. You can see a weekly Martian weather report from MARCI here.

The MRO recently manoeuvered itself into position for its next task—helping the InSight Lander. The MRO must receive critical radio transmissions from NASA’s InSight Lander as it descends to Mars. Insight will use its instruments to examine the interior of Mars for clues to how rocky planets form. Not only did MRO help find a landing spot for Insight, but it will hold the lander’s hand as it descends, and it will act as a data relay.

“After 11 and a half years in flight, the spacecraft is healthy and remains fully functional.” – MRO Project Manager Dan Johnston.

There’s no end in sight for the MRO. It just keeps going and going, and fulfilling its mission objectives on a continuing basis. “After 11 and a half years in flight, the spacecraft is healthy and remains fully functional,” said MRO Project Manager Dan Johnston at NASA’s Jet Propulsion Laboratory, Pasadena, California. “It’s a marvelous vehicle that we expect will serve the Mars Exploration Program and Mars science for many more years to come.”

SpaceX Attempting Launch of 1st Orbit Class Recycled Rocket March 30 – Watch Live

SpaceX Falcon 9 recycled rocket carrying SES-10 telecomsat raised erect atop Launch Complex 39A at the Kennedy Space Center as seen from inside the pad ahead of liftoff at 6:27 p.m on 30 Mar 2017 on world’s first reflight of an orbit class rocket. Credit: Ken Kremer/Kenkremer.com
SpaceX Falcon 9 recycled rocket carrying SES-10 telecomsat raised erect atop Launch Complex 39A at the Kennedy Space Center as seen from inside the pad ahead of liftoff slated for 6:27 p.m on 30 Mar 2017 on world’s first reflight of an orbit class rocket. Credit: Ken Kremer/Kenkremer.com

KENNEDY SPACE CENTER, FL – The moment of truth is rapidly approaching as SpaceX attempts the world’s first reflight of an orbital class rocket later today, Thursday, March 30, with the firms Falcon 9 standing proudly at historic launch complex 39A at NASA’s Kennedy Space Center in Florida – ready to deliver an advanced TV broadcast satellite to orbit for the America’s for telecom giant SES.

If successful, the launch will mightily advance billionaire SpaceX CEO Elon Musk’s bold vision to slash launch costs by recovering and reusing spent first stage rockets from his firms Falcon 9 launch vehicle.

“The SES-10 mission will mark a historic milestone on the road to full and rapid reusability,” say Space officials.

“We are confident in this booster,” SES CTO Martin Halliwell told Universe Today at a press briefing on March 28.

SpaceX Falcon 9 recycled rocket carrying SES-10 telecomsat poised atop Launch Complex 39A at the Kennedy Space Center ahead of liftoff slated for 6:27 p.m. on 30 Mar 2017 on world’s first reflight of an orbit class rocket. Credit: Ken Kremer/Kenkremer.com

The milestone SpaceX mission destined to refly the first ever ‘used rocket’ is slated for lift off on Thursday, March 30, at 6:27 p.m. EDT carrying the SES-10 telecommunications payload to orbit atop a ‘Flight-Proven’ Falcon 9 rocket from seaside Launch Complex 39A at NASA’s Kennedy Space Center in Florida.

So, if you want to witness this truly magnificent event in space history with your own eyes, there’s only a few hours left for you to ‘Get Your Ass to KSC!’ to paraphrase Apollo 11 moonwalker Buzz Aldrin.

The nearly six ton SES-10 satellite will provide significantly improved TV, voice, data and maratime service to over 37 million customers across Central and South America.

Eventually, Musk hopes to help establish a ‘City on Mars’ by building Interplanetary Colonial Transporters to transport human settlers to live on the Red Planet – the most Earth-like world in our Solar System.

You can watch the launch live on a SpaceX dedicated webcast starting about 20 minutes prior to the 6:27 pm EDT or 10:27 pm UTC liftoff time.

The two and a half hour launch window closes at 9:57 p.m. EDT.

Watch the SpaceX broadcast live at: SpaceX.com/webcast

The weather outlook is glorious along the Florida Space Coast with an 80% chance of favorable conditions at launch time in the latest AF prognosis.

However for the back-up launch date on Friday, the outlook worsens considerable to only 40% favorable.

“This thing is good to go!” Halliwell told me.

The SES-10 satellite was manufactured by Airbus Defence & Space and is based on the Eurostar E3000 platform. It will operate in geostationary orbit.Credit: SES/Airbus

The Falcon 9 booster to be recycled was initially launched in April 2016 for NASA on the SpaceX Dragon CRS-8 resupply mission to the International Space Station (ISS) under contract for the space agency.

The 156 foot tall first stage was recovered about eight and a half minutes after liftoff via a pinpoint propulsive soft landing on an tiny ocean going droneship prepositioned in the Atlantic Ocean some 400 miles (600 km) off the US East coast.

If all goes well SpaceX will also attempt to re-land the Falcon 9 first stage on an oceangoing barge for an unprecedented second time, provided there are sufficient fuel reserves remaining after accomplishing its primary mission of delivering SES-10 to GTO, Halliwell stated.

The SES-10 launch comes barely 2 weeks after the prior SpaceX launch of EchoStar XXIII on March 16.

SpaceX, founded by billionaire and CEO Elon Musk, inked a deal in August 2016 with telecommunications giant SES, to refly a ‘Flight-Proven’ Falcon 9 booster.

Luxembourg-based SES and Hawthrone, CA-based SpaceX jointly announced the agreement to “launch SES-10 on a flight-proven Falcon 9 orbital rocket booster.”

The flight proven SpaceX Falcon 9 rocket will deliver SES-10 to a Geostationary Transfer Orbit (GTO).

SES-10 has a launch mass of 5,300 kg or 11,700 pounds, which includes the dry mass and propellant.

The spacecraft utilizes for both chemical propulsion for orbit raising and electric propulsion for station keeping.

SES-10 will replace AMC-3 and AMC-4 to provide enhanced coverage and significant capacity expansion over Latin America, says SES.

“The satellite will be positioned at 67 degrees West, pursuant to an agreement with the Andean Community (Bolivia, Colombia, Ecuador and Peru), and will be used for the Simón Bolivar 2 satellite network.”

Up to 3 additional SES satellites could launch on SpaceX Falcon 9 rockets by the end of this year.

Watch for Kens’ continuing coverage direct from onsite at the Kennedy Space Center press site and Cape Canaveral Air Force Station.

Stay tuned here for Ken’s continuing Earth and Planetary science and human spaceflight news.

Ken Kremer

………….

Learn more about SpaceX SES-10, EchoStar 23 and CRS-10 launches to ISS, ULA SBIRS GEO 3 launch, GOES-R launch, Heroes and Legends at KSCVC, OSIRIS-REx, InSight Mars lander, Juno at Jupiter, SpaceX AMOS-6, ISS, ULA Atlas and Delta rockets, Orbital ATK Cygnus, Boeing, Space Taxis, Mars rovers, Orion, SLS, Antares, NASA missions and more at Ken’s upcoming outreach events at Kennedy Space Center Quality Inn, Titusville, FL:

Mar 31, Apr 1: “SpaceX SES-10, EchoStar 23, CRS-10 launch to ISS, ULA Atlas SBIRS GEO 3 launch, GOES-R weather satellite launch, OSIRIS-Rex, SpaceX and Orbital ATK missions to the ISS, Juno at Jupiter, ULA Delta 4 Heavy spy satellite, SLS, Orion, Commercial crew, Curiosity explores Mars, Pluto and more,” Kennedy Space Center Quality Inn, Titusville, FL, evenings

SES CTO Martin Halliway discusses the planned SES-10 telecomsat launch on March 30, 2017 on first ‘flight-proven’ SpaceX Falcon 9 from pad 39A on the Kennedy Space Center, FL. Credit: Ken Kremer/Kenkremer.com
Historic maiden blastoff of SpaceX Falcon 9 rocket from Launch Complex 39A at the Kennedy Space Center) at 9:38 a.m. EDT on Feb 19, 2017, on Dragon CRS-10 resupply mission to the International Space Station (ISS) for NASA. Credit: Ken Kremer/kenkremer.com

NASA Test Fires New Engine Controlling ‘Brain’ for First SLS MegaRocket Mission

NASA engineers conduct a test of the first RS-25 engine controller that will be used on an actual Space Launch System flight on the A-2 Test Stand at Stennis Space Center on March 23, 2017. The RS-25 engine, with the flight controller, was test fired for a full-duration 500 seconds. Credits: NASA/SSC
NASA engineers conduct a test of the first RS-25 engine controller that will be used on an actual Space Launch System flight on the A-2 Test Stand at Stennis Space Center on March 23, 2017. The RS-25 engine, with the flight controller, was test fired for a full-duration 500 seconds. Credits: NASA/SSC

Engineers carried out a critical hot fire engine test firing with the first new engine controlling ‘brain’ that will command the shuttle-era liquid fueled engines powering the inaugural mission of NASA’s new Space Launch System (SLS) megarocket.

The first integrated SLS launch combining the SLS-1 rocket and Orion EM-1 deep space crew capsule could liftoff as soon as late 2018 on a mission around the Moon and back.

The full duration static fire test involved an RS-25 engine integrated with the first engine controller flight unit that will actually fly on the maiden SLS launch and took place on Thursday, March 23 at the agency’s Stennis Space Center in Bay St. Louis, Mississippi.

The 500 second-long test firing was conducted with the engine controller flight unit installed on RS-25 development engine no. 0528 on the A-2 Test Stand at Stennis.

The RS-25 engine controller is the ‘brain’ that commands the RS-25 engine and communicates between the engine and the SLS rocket. It is about the size of a dorm refrigerator.

RS-25 new engine controller. Credit: NASA/SSC

The newly developed engine controller is a modern version from the RS-25 controller that helped propel all 135 space shuttle missions to space.

“This an important – and exciting – step in our return to deep space missions,” Stennis Director Rick Gilbrech said. “With every test of flight hardware, we get closer and closer to launching humans deeper into space than we ever have traveled before.”

The modernized RS-25 engine controller was funded by NASA and created in a collaborative effort of engineers from NASA, RS-25 prime contractor Aerojet Rocketdyne of Sacramento, California, and subcontractor Honeywell of Clearwater, Florida.

“The controller manages the engine by regulating the thrust and fuel mixture ratio and monitors the engine’s health and status – much like the computer in your car,” say NASA officials.

“The controller then communicates the performance specifications programmed into the controller and monitors engine conditions to ensure they are being met, controlling such factors as propellant mixture ratio and thrust level.”

A quartet of RS-25 engines, leftover from the space shuttle era and repeatedly reused, will be installed at the base of the core stage to power the SLS at liftoff, along with a pair of extended solid rocket boosters.

The four RS-25 core stage engine will provide a combined 2 million pounds of thrust at liftoff.

In addition to being commanded by the new engine controller, the engines are being upgraded in multiple ways for SLS. For example they will operate at a higher thrust level and under different operating conditions compared to shuttle times.

To achieve the higher thrust level required, the RS-25 engines must fire at 109 percent of capability for SLS compared to operating at 104.5 percent of power level capability for shuttle flights.

The RS-25 engines “also will operate with colder liquid oxygen and engine compartment temperatures, higher propellant pressure and greater exhaust nozzle heating.”
SLS will be the world’s most powerful rocket and send astronauts on journeys into deep space, further than human have ever travelled before.

For SLS-1 the mammoth booster will launch in its initial 70-metric-ton (77-ton) Block 1 configuration with a liftoff thrust of 8.4 million pounds – more powerful than NASA’s Saturn V moon landing rocket.

NASA engineers conduct a test of the first RS-25 engine controller that will be used on an actual Space Launch System flight on the A-2 Test Stand at Stennis Space Center on March 23, 2017. The RS-25 engine, with the flight controller, was test fired for a full-duration 500 seconds. Credits: NASA/SSC

The next step is evaluating the engine firing test results, confirming that all test objectives were met and certifying that the engine controller can be removed from the RS-25 development engine and then be installed on one of four flight engines that will help power SLS-1.

During 2017, two additional engine controllers for SLS-1 will be tested on the same development engine at Stennis and then be installed on flight engines after certification.

Finally, “the fourth controller will be tested when NASA tests the entire core stage during a “green run” on the B-2 Test Stand at Stennis. That testing will involve installing the core stage on the stand and firing its four RS-25 flight engines simultaneously, as during a mission launch,” says NASA.

Numerous RS-25 engine tests have been conducted at Stennis over more than 4 decades to certify them as flight worthy for the human rated shuttle and SLS rockets.

NASA engineers successfully conducted a development test of the RS-25 rocket engine Thursday, Aug. 18, 2016 at NASA’s Stennis Space Center near Bay St. Louis, Miss. The RS-25 will help power the core stage of the agency’s new Space Launch System (SLS) rocket for the journey to Mars. Credit: Ken Kremer/kenkremer.com

Although NASA is still targeting SLS-1 for launch in Fall 2018 on an uncrewed mission, the agency is currently conducting a high level evaluation to determine whether the Orion EM-1 capsule can be upgraded in time to instead fly a human crewed mission with two astronauts before the end of 2019 – as I reported here.

The Orion EM-1 capsule is currently being manufactured at the Neil Armstrong Operations and Checkout Building at the Kennedy Space Center by prime contractor Lockheed Martin.

Orion crew module pressure vessel for NASA’s Exploration Mission-1 (EM-1) is unveiled for the first time on Feb. 3, 2016 after arrival at the agency’s Kennedy Space Center (KSC) in Florida. It is secured for processing in a test stand called the birdcage in the high bay inside the Neil Armstrong Operations and Checkout (O&C) Building at KSC. Launch to the Moon is slated in 2018 atop the SLS rocket. Credit: Ken Kremer/kenkremer.com

Stay tuned here for Ken’s continuing Earth and Planetary science and human spaceflight news.

Ken Kremer

Aerojet Rocketdyne technicians inspect the engine controller that will be used for the first integrated flight of NASA’s Space Launch System and Orion in late 2018. The engine controller was installed on RS-25 development engine no. 0528 for testing at Stennis Space Center on the A-2 Test Stand on March 23, 2017. The RS-25 engine, with the flight controller, was test fired for a full-duration 500 seconds. Credits: NASA/SSC

Juno’s Monday Jupiter Flyby Promises New Batch of Images & Science

This image of Jupiter from the Juno probe shows an intricate dance of storms and swirls. The enhanced color image was captured on February 2nd, from only 14,500 km above the gas giant's cloud tops. Image: NASA/JPL-Caltech/SwRI/MSSS/Roman Tkachenko

Juno is only part way through its mission to Jupiter, and already we’ve seen some absolutely breathtaking images of the gas giant. On Monday, the Juno spacecraft will flyby Jupiter again. This will be the craft’s 5th flyby of the gas giant, and it’ll provide us with our latest dose of Jupiter science and images. The first 4 flybys have already exceeded our expectations.

Juno will approach to within 4,400 km of Jupiter’s cloud tops, and will travel at a speed of 207,600 km/h. During this time of closest approach, called a perijove, all of Juno’s eight science instruments will be active, along with the JunoCam.

The JunoCam is not exactly part of the science payload. It was included in the missions to help engage the public with the mission, and it appears to be doing that job well. The Junocam’s targets have been partly chosen by the public, and NASA has invited anyone who cares to to download and process raw Junocam images. You can see those results throughout this article.

This image of Jupiter’s dancing cloud tops was captured during perijove 3. Image: NASA / JPL-Caltech / SwRI / MSSS / Kootenay Nature Photos © cc nc sa

This is Juno’s 5th flyby, but only its 4th science pass. During Juno’s first encounter with Jupiter, the science instruments weren’t active. Even so, after only 3 science passes, we have learned some things about Jupiter.

“We are excited to see what new discoveries Juno will reveal.” – Scott Bolton, NASA’s Principal Investigator for the Juno Mission

“This will be our fourth science pass — the fifth close flyby of Jupiter of the mission — and we are excited to see what new discoveries Juno will reveal,” said Scott Bolton, principal investigator of Juno from the Southwest Research Institute in San Antonio. “Every time we get near Jupiter’s cloud tops, we learn new insights that help us understand this amazing giant planet.”

We’ve already learned that Jupiter’s intense magnetic fields are much more complicated than we thought. We’ve learned that the belts and zones in Jupiter’s atmosphere, which are responsible for the dazzling patterns on the cloud tops, extend much deeper into the atmosphere than we thought. And we’ve discovered that charged material expelled from Io’s volcanoes helps cause Jupiter’s auroras.

The South Pole of Jupiter, taken during perijove 3. Image: NASA / JPL-Caltech / SwRI / MSSS / Luca Fornaciari © cc nc sa

Juno has the unprecedented ability to get extremely close to Jupiter. This next flyby will bring it to within 4,400 km of the cloud tops. But to do so, Juno has to pay a price. Though the sensitive equipment on the spacecraft is protected inside a titanium vault, Jupiter’s powerful radiation belts will still take a toll on the electronics. But that’s the price Juno will pay to perform its mission.

Jupiter’s dazzle as revealed by JunoCam and Shane Drever. Image: NASA / JPL-Caltech / SwRI / MSSS / Shane Drever © cc nc sa

Other missions, like Cassini, have been measured in years, while Juno’s will be measured in orbits. And once it’s completed its final orbit, it will be sent to its destruction in Jupiter’s atmosphere.

But before that happens, there’s a lot of science to be done, and a lot of stunning images to be captured.

Here’s an interview with the man leading the Juno Mission: Understanding Juno’s Orbit: An Interview with NASA’s Scott Bolton.

Here is the page for the JunoCam: https://www.missionjuno.swri.edu/junocam

SpaceX & NASA Studying 2020 Landing Sites For Dragon

An artist's illustration of SpaceX's Dragon capsule entering the Martian atmosphere. Image: SpaceX
An artist's illustration of SpaceX's Dragon capsule entering the Martian atmosphere. Image: SpaceX

As part of their effort to kick-start the eventual colonization of Mars, SpaceX is sending an unmanned Dragon spacecraft to Mars. Initially, that mission was set for 2018, but is now re-scheduled for 2020. Now, SpaceX says they’re working with NASA to select a suitable landing site for their first Dragon mission to Mars.

At a presentation in Texas on March 18th, Paul Wooster of SpaceX said that they have been working with scientists at NASA’s Jet Propulsion Laboratory (JPL) to identify candidate landing sites on the surface of Mars. In order to aid colonization, the sites need to be:

  • near the equator, for solar power
  • near large quantities of ice, for water
  • at low elevation, for better thermal conditions

But finding a site that meets those conditions is difficult.

According to SpaceNews, the study done with NASA initially recognized 4 regions in Mars’ northern hemisphere, all within 40 degrees of the equator. They are Deuteronilus Mensae, Phlegra Montes, Utopia Planitia, and Arcadia Planitia.

Deuteronilus Mensae

Deuteronilus Mensae (DM) is located between older, cratered highlands and low plains. DM shows evidence of glacial activity in its surface features. In fact, there are still glaciers there, which makes it a desirable source of ice.

Deuteronilus Mensae (DM)has many rough surface features. The Mars Reconnaissance Orbiter has shown that many areas in DM are sub-surface glaciers covered by a thin layer of debris. Image: NASA/JPL/University of Arizona

Phlegra Montes

Phlegra Montes (PM) is a system of mountains on the Martian surface, over 1300 km across. It’s a complex system of basins, hills, and ridges. They are likely tectonic in origin, rather than volcanic, and the region probably contains large quantities of water ice, perhaps 20 meters below the surface.

This tongue shaped flow of material at Phlegra Montes may have been formed by a flow of ice-rich material. Image: NASA/JPL/University of Arizona

Utopia Planitia

Utopia Planitia (UP) is the region where the Viking 2 lander set down in 1976. At 3300 km in diameter, UP is the largest impact basin in the Solar System. In 2016, NASA found a huge deposit of underground ice there. The water is estimated to be the same volume as Lake Superior.

Periglacial features in a small crater in Utopia Planitia. Periglacial refers to the seasonal thawing of snow and ice which refreezes in other shapes. Image: NASA/JPL/University of Arizona

Arcadia Planitia

Arcadia Planitia (AP) is a smooth plain containing fresh lava flows. It also has a large region that was shaped by periglacial processes. This supports the idea that ice is present just beneath the surface, making it a candidate for colonization efforts.

Arcadia Planitia likely has ice just beneath its surface. The knobby pattern is probably caused by the uneven seasonal melting of sub-surface ice. Image: NASA/JPL/University of Arizona

The image below shows the Arcadia Planitia region in relation to some of its surroundings. Colonists at AP might have a great view of Olympus Mons, the largest volcano in the Solar System.

Colonists in Arcadia Planitia (upper left in map) might have a great view of Olympus Mons.

The four areas looked suitable in images from a medium resolution camera (CTX) on the Mars Reconnaissance Orbiter (MRO). But when the High Resolution Imaging Science Experiment (HiRISE) camera on the same orbiter was used to look more closely, the first three locations appeared to be much rockier. According to SpaceNews, Wooster said ““The team at JPL has been finding that, while the areas look very flat and smooth at CTX resolution, with HiRISE images, they’re quite rocky. That’s been unfortunate in terms of the opportunities for those sites.”

The fourth area, Arcadia Planitia, is a more promising site. HiRISE images showed that it is much less rocky and could be a suitable site for the first Dragon mission to Mars.

The Dragon mission to Mars is just the first step for SpaceX. They see themselves as an interplanetary transportation company eventually. SpaceX intends to send a craft to Mars every two years, when the launch window is optimal. SpaceX says they’ll have the ability to deliver one ton of payload to the Martian surface with each Dragon mission.

Their Interplanetary Transport System (ITS) might have the capability to make it to Mars in as little as 80 days, while carrying a payload of up to 450 tons. While still in the very initial stages of design, it may eventually revolutionize our ability to colonize Mars in any meaningful or enduring way. SpaceX envisions a fleet of craft in the ITS which will constantly make the return to trip to Mars.

If that ever happens, we may look at the first Dragon mission to Arcadia Planitia, or another eventual landing site, as the first step.

SpaceX Dragon Splashes Down in Pacific with Treasure Trove of Space Station Science

The SpaceX Dragon CRS-10 spacecraft is pictured seconds before splashing down in the Pacific Ocean on Mar. 19, 2017 after departing the International Space Station (ISS). Credit: SpaceX
The SpaceX Dragon CRS-10 spacecraft is pictured seconds before splashing down in the Pacific Ocean on Mar. 19, 2017 after departing the International Space Station (ISS). Credit: SpaceX

KENNEDY SPACE CENTER, FL – SpaceX’s tenth contracted resupply mission to the International Space Station came to a safe conclusion with a splashdown of the Dragon spacecraft in the Pacific Ocean Sunday and successfully returned a treasure trove of more than two tons of precious science experiments and research samples from the space station.

Researchers on Earth are eagerly awaiting the science data and samples in order to carry out high powered laboratory analysis that will eventually yield the fruits of the hard won labor – years in the making.

The Dragon CRS-10 cargo freighter departed the International Space Station (ISS) Sunday morning after Expedition 50 astronauts Thomas Pesquet of ESA (European Space Agency) and Shane Kimbrough of NASA released the spacecraft from the grip of the station’s 57.7-foot-long(17.6-meter) Canadian-built Canadarm2 robotic arm as planned at 5:11 a.m. EDT, March 19.

After carefully maneuvering away from the orbiting outpost and six person international crew at an altitude of appox. 250 miles (400 km), Dragon eased away to a safe distance.

SpaceX’s Dragon CRS-10 cargo vehicle is attached to the International Space Station on Feb 23, 2017 after early morning capture by astronauts Shane Kimbrough and Thomas Pesquet using the robotic arm and subsequent berthing at Earth facing port on the Harmony module. It will stay for a month. Credit: NASA

The vessel then fired its braking thrusters a few hours later to initiate the reentry burn that would set the craft on course for a fiery plummet through the Earth’s atmosphere.

Some five and a half hours later the spaceship carried out a parachute assisted splashdown in the Pacific Ocean at 10:46 a.m. EDT, about 200 miles southwest of Long Beach, California.

The highest priority research and technology cargo will be removed from Dragon immediately and returned to NASA.

SpaceX CRS-10 Dragon supply ship launched on Feb. 19, 2017 from NASA’s Kennedy Space Center in Florida successfully arrives at the International Space Station on Feb. 23, 2017 for capture and berthing at station port on the Harmony module. Credit: NASA

The rest will travel back to port and be prepared for a return trip to SpaceX’s test facility in McGregor, Texas, where the remaining scientific samples, research experiments and technology gear and hardware will be unloaded for NASA.

Dragon had spent nearly a month berthed at the Earth-facing port on the station’s Harmony module, since arriving on Feb 23.

Dragon begun its space voyage after it was launched from the Kennedy Space Center (KSC) on Sunday, Feb. 19 on the first Falcon 9 rocket ever to blast off from historic launch pad 39A in a blaze of glory – as I reported here.

Historic maiden blastoff of SpaceX Falcon 9 rocket from Launch Complex 39A at the Kennedy Space Center) at 9:38 a.m. EDT on Feb 19, 2017, on Dragon CRS-10 resupply mission to the International Space Station (ISS) for NASA. Credit: Ken Kremer/kenkremer.com

At liftoff, the Dragon CRS-10 space freighter was carrying more than 5500 pounds of equipment, gear, food, crew supplies, hardware and NASA’s Stratospheric Aerosol Gas Experiment III (SAGE III) ozone mapping science payload to the low Earth orbiting station in support of the Expedition 50 and 51 crew members.

After a four day chase, Dragon was captured and attached to the station using the Canadian arm on Feb 23 by the same two astronauts who released it on Sunday.

The research supplies and equipment brought up by Dragon will support over 250 scientific investigations to advance knowledge about the medical, psychological and biomedical challenges astronauts face during long-duration spaceflight.

SAGE III will measure stratospheric ozone, aerosols, and other trace gases by locking onto the sun or moon and scanning a thin profile of the atmosphere. It is one of NASA’s longest running earth science programs.

The LIS lightning mapper will measure the amount, rate and energy of lightning as it strikes around the world from the altitude of the ISS as it orbits Earth. Its data will complement that from the recently orbited GLM lighting mapper lofted to geosynchronous aboard the NASA/NOAA GOES-R spacecraft instrument.

NASA’s RAVEN experiment will test autonomous docking technologies for spacecraft.

SAGE III and RAVEN were stowed in the Dragon’s unpressurized truck. Astronauts plucked them out of the trunk using the robotic arm and attached them to specified locations on the stations exterior to carry out their objectives.

For the return trip to Earth, the astronaut crew loaded Dragon with more than 5,400 pounds of NASA cargo, and science and technology demonstration samples gathered and collected by the stations crewmembers.

“A variety of technological and biological studies are returning in Dragon. The Microgravity Expanded Stem Cells investigation had crew members observe cell growth and other characteristics in microgravity,” said NASA.

“This information will provide insight into how human cancers start and spread, which aids in the development of prevention and treatment plans. Results from this investigation could lead to the treatment of disease and injury in space, as well as provide a way to improve stem cell production for human therapy on Earth.”

“Samples from the Tissue Regeneration-Bone Defect study, a U.S. National Laboratory investigation sponsored by the Center for the Advancement of Science in Space (CASIS) and the U.S. Army Medical Research and Materiel Command, studied what prevents vertebrates such as rodents and humans from re-growing lost bone and tissue, and how microgravity conditions affect the process. Results will provide a new understanding of the biological reasons behind a human’s inability to grow a lost limb at the wound site, and could lead to new treatment options for the more than 30 percent of the patient population who do not respond to current options for chronic non-healing wounds.”

Dragon departed in order to make way for the arrival of the next cargo ship.

The ‘SS John Glenn’ Cygnus cargo freighter built by Orbital Sciences is due to lift off no earlier than March 27 on a United Launch Alliance (ULA) Atlas V rocket from Cape Canaveral Air Force Station.

The Orbital ATK Cygnus spacecraft named for Sen. John Glenn, one of NASA’s original seven astronauts, stands inside the Payload Hazardous Servicing Facility at NASA’s Kennedy Space Center in Florida behind a sign commemorating Glenn on March 9, 2017. Launch slated for March 21 on a ULA Atlas V. Credit: Ken Kremer/Kenkremer.com

Watch for Ken’s onsite launch and mission reports direct from the Kennedy Space Center and Cape Canaveral Air Force Station, Florida.

Stay tuned here for Ken’s continuing Earth and Planetary science and human spaceflight news.

Ken Kremer

NASA Twins Study Researchers Take Genetic Data To Next Level

NASA is beginning to integrate the results of its twin study on astronauts Mark and Scott Kelly. Image: NASA

People who plan and conduct space missions never tire of telling us how hard it is to do things in space.

Our next big goal is getting humans to Mars, and establishing a colony there. There are a multitude of technical and engineering hurdles to be overcome, but we think we can do it.

But the other side of the coin is the physiological hurdles to be overcome. Those may prove to be much more challenging to deal with. NASA’s twins study is poised to add an enormous amount of data to our growing body of knowledge on the effects of space travel on human beings.

NASA's astronauts twins, Scott Kelly (l) and Mark Kelly (r). Image: NASA
NASA’s astronaut twins, Scott Kelly (l) and Mark Kelly (r). Image: NASA

Astronaut twins Scott and Mark Kelly are the basis of NASA’s study. Scott spent a year in space, returning to Earth on March 1st 2016, after spending 340 days aboard the ISS. Mark, himself a retired astronaut, remained on Earth during Scott’s year in space, providing a baseline for studying the effects on the human body of such a prolonged period of time away from Earth.

In February of 2016, NASA released preliminary results of the study. Now, the team studying the results of the twins study has started integrating the data. The way they’re doing this sets it apart from other studies.

“No one has ever looked this deeply at a human subject and profiled them in this detail.” – Tejaswini Mishra, Ph.D., Stanford University School of Medicine.

Typically, individual studies are released to appropriate journals more or less one at a time. But in the twins study, the data will be integrated and summarized before individual papers are published on separate themes. The idea is that taken together, their impact on our understanding of prolonged time in space will be much greater.

“The beauty of this study is when integrating rich data sets of physiological, neurobehavioral and molecular information, one can draw correlations and see patterns,” said Tejaswini Mishra, Ph.D., research fellow at Stanford University School of Medicine, who is creating the integrated database, recording results and looking for correlations. “No one has ever looked this deeply at a human subject and profiled them in this detail. Most researchers combine maybe two to three types of data but this study is one of the few that is collecting many different types of data and an unprecedented amount of information.”

“Each investigation within the study complements the other.” – Brinda Rana, Ph.D., U of C, San Diego School of Medicine

Mike Snyder, Ph.D, is the head of a team of people at Stanford that will work to synthesize the data. There are roughly three steps in the overall process:

  1. Individual researchers in areas like cognition, biochemistry, and immunology will analyze and compile their data then share their results with the Stanford team.
  2. The Stanford team will then further integrate those results into larger data sets.
  3. Those larger data sets will then be reviewed and analyzed to confirm and modify the initial findings.

“There are a lot of firsts with this study and that makes it exciting,” said Brinda Rana, Ph.D., associate professor of psychiatry, University of California San Diego School of Medicine. “A comparative study with one twin in space and one on Earth has never been done before. Each investigation within the study complements the other.”

NASA compares the twins study, and the new integrated method of handling all the results, to conducting a symphony. Each study is like an instrument, and instead of each one playing a solo, they will be added into a greater whole. The team at Stanford is like the conductor. If you’ve ever listened to an orchestra, you know how powerful that can be.

“The human systems in the body are all intertwined which is why we should view the data in a holistic way,” said Scott M. Smith, Ph.D., NASA manager for nutritional biochemistry at the Johnson Space Center. He conducts biochemical profiles on astronauts and his research is targeted to specific metabolites, end products of various biological pathways and processes.

“It is a more comprehensive way to conduct research.” – Chris Mason, Ph.D., associate professor, Department of Physiology and Biophysics Weill Cornell Medicine

Chris Mason Ph.D., at Weill Cornell Medicine said, “Both the universe and the human body are complicated systems and we are studying something hard to see. It’s like having a new flashlight that illuminates the previously dark gears of molecular interactions. It is a more comprehensive way to conduct research.”

Scientists involved with the twins study are very clearly excited about this new approach. Having twin astronauts is an extraordinary opportunity, and will advance our understanding of spaceflight on human physiology enormously.

“There is no doubt, the learnings from integrating our data will be priceless,” said Emmanuel Mignot, M.D., Ph.D., director of Center for Sleep Science and Medicine, Stanford University School of Medicine. He studies the immune system and is enthusiastic to study specific immune cell populations because many of the other immune studies focus only on general factors.

A summary of the early results should be out by early 2018, or possible late 2017. Individual papers on more detailed themes will follow shortly.