How Could Your Research In Diseases Help Missions To The Moon, Mars And Other Places In Our Solar System?

A Mesmerizing Model of Monster Black Holes

Just about every galaxy the size of our Milky Way (or bigger) has a supermassive black hole at its center. These objects are ginormous — hundreds of thousands to billions of times the mass of the Sun! Now, we know galaxies merge from time to time, so it follows that some of their black holes should combine too. But we haven’t seen a collision like that yet, and we don’t know exactly what it would look like. 

A new simulation created on the Blue Waters supercomputer — which can do 13 quadrillion calculations per second, 3 million times faster than the average laptop — is helping scientists understand what kind of light would be produced by the gas around these systems as they spiral toward a merger.

The new simulation shows most of the light produced around these two black holes is UV or X-ray light. We can’t see those wavelengths with our own eyes, but many telescopes can. Models like this could tell the scientists what to look for. 

You may have spotted the blank circular region between the two black holes. No, that’s not a third black hole. It’s a spot that wasn’t modeled in this version of the simulation. Future models will include the glowing gas passing between the black holes in that region, but the researchers need more processing power. The current version already required 46 days!

The supermassive black holes have some pretty nifty effects on the light created by the gas in the system. If you view the simulation from the side, you can see that their gravity bends light like a lens. When the black holes are lined up, you even get a double lens!

But what would the view be like from between two black holes? In the 360-degree video above, the system’s gas has been removed and the Gaia star catalog has been added to the background. If you watch the video in the YouTube app on your phone, you can moved the screen around to explore this extreme vista. Learn more about the new simulation here. 

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What do you hope to find using this new technology? When you were a kid, did you ever dream of landing on Mars? Even if you may not be visiting, tech that you have sway over is.

“When you wer a kid, did you ever dream of landing on Mars?”

Hello everyone.  This is NASA astronaut Peggy Whitson ready to answer your questions about being an astronaut, mission training, and what it’s like to live in space.

Have a question for me? Ask it here, then watch the answers here.

The As, Gs, Cs and Ts of the Space Station: First In-Space Microbe Identification

Being able to identify microbes in real-time aboard the International Space Station, without having to send them back to Earth for identification first, would be totally amazing for the world of microbiology and space exploration.

The Genes in Space 3 team turned that possibility into a reality this year, when it completed the first-ever sample-to-sequence process entirely aboard the space station.

The ability to identify microbes in space could aid in the ability to diagnose and treat astronauts in real time, as well as assisting in the identification of life on other planets. It could also benefit other experiments aboard the space station.

HELPFUL SCIENCE HINT: Identifying microbes involves isolating the DNA of samples, and then amplifying – or making lots and lots (and LOTS) of copies - of that DNA that can then be sequenced, or identified.  

As part of regular monitoring, petri plates were touched to various surfaces of the space station. NASA astronaut Peggy Whitson transferred cells from growing bacterial colonies on those plates into miniature test tubes, something that had never been done before in space (first OMG moment!).

Once the cells were successfully collected, it was time to isolate the DNA and prepare it for sequencing, enabling the identification of the unknown organisms – another first for space microbiology.

Enter Hurricane Harvey. *thunder booms*

“We started hearing the reports of Hurricane Harvey the week in between Peggy performing the first part of collecting the sample and gearing up for the actual sequencing,” said Sarah Wallace, the project’s primary investigator.

When our Johnson Space Center (JSC) in Houston became inaccessible due hurricane conditions, Marshall Space Flight Center’s Payload Operations Integration Center in Huntsville, Alabama worked to connect Wallace to Whitson using Wallace’s personal cell phone.

With a hurricane wreaking havoc outside, Wallace and Whitson set out to make history.

The data were downlinked to the team in Houston for analysis and identification.

“Once we actually got the data on the ground we were able to turn it around and start analyzing it,” said Aaron Burton, the project’s co-investigator. “You get all these squiggle plots and you have to turn that into As, Gs, Cs and Ts.”

Those As, Gs, Cs and Ts are more than just a nerdy alphabet – they are Adenine, Guanine, Cytosine and Thymine – the four bases that make up each strand of DNA and can tell you what organism the strand of DNA came from. 

“Right away, we saw one microorganism pop up, and then a second one, and they were things that we find all the time on the space station,” said Wallace. “The validation of these results would be when we got the sample back to test on Earth.”

Soon after, the samples returned to Earth aboard the Soyuz spacecraft, along with Whitson.

With the samples now in the team’s JSC lab, tests were completed in ground labs to confirm the findings from the space station. They ran the tests again and again, and then once more, to confirm accuracy. Each time, the results were exactly the same on the ground as in orbit. (second OMG moment!)

“We did it. Everything worked perfectly,” said Sarah Stahl, microbiologist.

This capability could change future space exploration.

“As a microbiologist,” said Wallace, “My goal is really so that when we go and we move beyond ISS and we’re headed towards Mars or the moon or wherever we are headed to, we have a process that the crew can have that great understanding of the environment, based on molecular technology.”

For more information, follow @ISS_Research. 

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Sometimes... there’s more than meets the eye. 👀 You’re looking at two very different takes on an iconic image. ⁣

Human eyes can see only a small portion of the range of radiation given off by the objects around us. We call this wide array of radiation the electromagnetic spectrum, and the part we can see visible light.

In the first image, researchers revisited one of Hubble Space Telescope’s most popular sights: the Eagle Nebula’s Pillars of Creation. Here, the pillars are seen in infrared light, which pierces through obscuring dust and gas and unveil a more unfamiliar — but just as amazing — view of the pillars. ⁣ ⁣ The entire frame is peppered with bright stars and baby stars are revealed being formed within the pillars themselves. The image on the bottom is the pillars in visible light.

Image Credit: NASA, ESA/Hubble and the Hubble Heritage Team⁣

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From Apollo to Commercial Crew: Get To Know Historic Launch Pad 39A

Originally built for the massive Saturn V rockets that sent astronauts on Apollo missions to the Moon, Launch Complex 39A also served as one of the two launch pads used by the space shuttle. Between Apollo, Skylab, Apollo-Soyuz and the space shuttle, this launch pad has been the starting point for many of the nation’s most challenging and inspiring missions.

In 2014, SpaceX signed a property agreement with NASA for use and operation of the launch complex for 20 years, and the company modified the facility to prepare for the processing and launch of its Falcon 9 and Falcon Heavy rockets.

The SpaceX Falcon 9 rocket carrying the company’s Crew Dragon on its Demo-2 flight test to the International Space Station with NASA astronauts Robert Behnken and Douglas Hurley will lift off from the same historic site where astronauts first launched to the moon. Launch Complex 39A at NASA’s Kennedy Space Center in Florida is also the site of dozens of space shuttle launches that helped build the orbital laboratory.

Launch Complexes 39A and B were constructed in the 1960s. Both launch pads have a long history of supporting launches for the Apollo and Space Shuttle Programs. Launch Pad 39A was the launch site for 11 Saturn V Apollo missions, including Apollo 11, the first Moon landing. The pad also was the launch site for 82 space shuttle missions, including STS-1, the first shuttle launch, the STS-125 final servicing mission for the Hubble Space Telescope, and STS-135, the final shuttle mission.

After the space shuttle was retired in 2011, we began the process to transform Kennedy Space Center from a historically government-only launch facility into a multi-user spaceport for both government and commercial use. On April 14, 2014, the agency signed a property agreement with SpaceX for use of the launch site for the next 20 years.

SpaceX upgraded and modified the launch pad to support its Falcon 9 and Falcon Heavy rockets. The company also built a horizontal processing hangar at the base of the pad to perform final vehicle integration prior to flight. The first SpaceX launch from the pad was the company’s 10th commercial resupply services (CRS-10) mission for us. A SpaceX Falcon 9 launched a Dragon cargo spacecraft on CRS-10 on Feb. 19, 2017. The Dragon delivered about 5,500 pounds of supplies to the space station, including the Stratospheric Aerosol and Gas Experiment (SAGE) III instrument to further study ozone in the Earth’s atmosphere. Combined with SpaceX, we’ve launched more than 100 missions from Pad 39A.

Because of our partnership with SpaceX within our agency’s Commercial Crew Program, Launch Complex 39A will once again be the site of crewed missions to the space station.

🚀 TUNE IN starting at 12:15 p.m. EDT on Wednesday, May 27 as NASA and SpaceX launch astronauts Robert Behnken and Douglas Hurley to the International Space Station aboard the Crew Dragon spacecraft: www.nasa.gov.live.

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What do you hope to find on the mars? / What would be the best possible outcome?

We're using our unique vantage point in space to provide observations and data of Hurricane Irma and other tropical storms. Hurricanes Irma and Jose are seen here in a 12-hour long infrared loop. Scientists monitor storms in infrared to closely monitor clouds and storm intensity. We continue to provide satellite imagery for these storms, tracking its trajectory, force and precipitation to inform forecasters at the National Hurricane Center.

As these storms continue their westward drive in the coming days, they will be passing over waters that are warmer than 30 degrees Celsius (86 degrees Fahrenheit)—hot enough to sustain a category 5 storm. Warm oceans, along with low wind shear, are two key ingredients that fuel and sustain hurricanes. Get the latest imagery and data from us at www.nasa.gov/hurricane For information on making preparations for Hurricanes, visit the FEMA website at: ready.gov/hurricanes. Credit: NASA-SPoRT/NOAA 

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Don’t Say “Bye, Bye, Bye” To Your Vision: Solar Eclipse Safety Tips

On Oct. 14, 2023, many people across North, Central, and South America will have an opportunity to view a “ring of fire” eclipse – an annular solar eclipse – when the Moon passes between the Earth and Sun! During an annular eclipse, it is never safe to look directly at the Sun without specialized eye protection designed for solar viewing. To spread the word, *NSYNC's Lance Bass stopped by to share some tips on how to stay safe while viewing a solar eclipse.

Check out these detailed viewing maps to see if you will be able to see the entire or partial solar eclipse. If you are, make sure your solar viewing glasses have the ISO certification 12312-2. You can also check with local libraries or science museums to see if they have safe solar viewing glasses to hand out. You can also make a simple pinhole camera at home with some paper and aluminum foil: go.nasa.gov/pinholeprojector

Everyone online can watch the eclipse with NASA. Set a reminder to watch live: https://www.youtube.com/watch?v=LlY79zjud-Q

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Experience How Microgravity Affects the Human Body

Now is your chance to experience what it’s like to live and work on the International Space Station! The new NASA Science: Humans in Space app will let you explore the station while virtually experiencing what it does to your body.

Life in space is no float in the park. Astronauts contend with everything from motion sickness to face swelling to loss of bone density. That’s why many research investigations on the space station study how humans can better adapt to microgravity both in Earth's orbit as well as on longer missions to the Moon and Mars. 

Deal with these challenges and perform crucial daily workouts as you explore the orbiting laboratory and ensure the H-II Transfer Vehicle successfully berths to the station. 

You can even collect mission patches along the way for completing tasks, counteracting the effects of microgravity and making discoveries. 

Download the application for Android here and iPhone here. Find more NASA apps here.

Want to learn about more investigations heading to the space station (or even ones currently under way)? Make sure to follow @ISS_Research on Twitter and Space Station Research and Technology News on Facebook.

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