Ocean Worlds Beyond Earth

Pluto Continues to Amaze

This dwarf planet sure knows how to get a BIG reaction because we’re stunned by the latest images from our New Horizons spacecraft!

Back on July 14, the spacecraft completed it’s historic Pluto flyby, and is now in an intensive downlink phase. During this time, New Horizons will send us some of the best data and images we’ve seen!

These latest images were taken just 15 minutes after New Horizons’ closest approach to Pluto. The spacecraft looked back toward the sun and captured this near-sunset view. Icy mountains, flat plains and the horizon can all be seen in detail.

When we take a closer look, these features truly begin to stand out. Mountains up to 11,000 feet high are met by flat icy plains that extend out to Pluto’s horizon. There, more than a dozen layers of haze in the dwarf planet’s atmosphere can be seen. It’s almost as if we’re flying over the surface with the New Horizons spacecraft.

Speaking of flyover, this new animation of Pluto has been created from images returned from the spacecraft this month. This view shows us what it might be like to take an aerial tour through Pluto’s thin atmosphere and soar above the surface. 

These images and videos are not only stunning, but also provide us with important information about the dwarf planet. So far, scientists can tell that the weather changes from day to day on Pluto. These images, combined with others that have been downloaded, provide evidence for a remarkably Earth-like “hydrological” cycle on Pluto.

For updates on the data and images received by the New Horizons spacecraft, check our blog: https://blogs.nasa.gov/pluto/

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Astronaut Journal Entry - Week 6

Currently, six humans are living and working on the International Space Station, which orbits 250 miles above our planet at 17,500mph. Below you will find a real journal entry, written in space, by NASA astronaut Scott Tingle.

To read more entires from this series, visit our Space Blogs on Tumblr.

I did an interview with some students today, and I was asked a two-part question by one of the students. He asked, “What is the most exciting thing about being in space, and how did you keep yourself motivated to get there?”  

I answered, “When you were very young, did you ever dream or wish you could fly? We all know it’s impossible, right? Imagine waking up one day and finding out you actually can fly! THAT is exciting! Now consider the contrary thought, what if you grew up and realized that flying wasn’t possible for humans, and you were at peace with this reality, and at peace shedding your childhood dream of flying? You will have several crossroads in your life, and you will have to decide which of these people you want to be. I too am amazed that I had the staying power to continue to dream as I did when I was a child. Words cannot describe how I feel when I fly through the International Space Station every day.”

Find more ‘Captain’s Log’ entries HERE.

Follow NASA astronaut Scott Tingle on Instagram and Twitter.

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Space Station Science: Biological Research

Each month, we highlight a different research topic on the International Space Station. In August, our focus is biological research. Learning how spaceflight affects living organisms will help us understand potential health risks related to humans on long duration missions, including our journey to Mars.

Cells, microbes, animals and plants are affected by microgravity, and studying the processes involved in adaptation to spaceflight increases our fundamental understanding of biological processes on Earth. Results on Earth from biological research in space include the development of new medications, improved agriculture, advancements in tissue engineering and regeneration, and more. 

Take a look at a few of the biological research experiments performed on space station:

Biomolecule Sequencer

Living organisms contain DNA, and sequencing DNA is a powerful way to understand how they respond to changing environments. The Biomolecule Sequencer experiment hopes to demonstrate (for the first time) that DNA sequencing is feasible in an orbiting spacecraft. Why? A space-based DNA sequencer could identify microbes, diagnose diseases and understand crew member health, and potentially help detect DNA- based life elsewhere in the solar system.

Ant-stronauts

Yes, ant-stronauts…as in ants in space. These types of studies provide insights into how ants answer collective search problems. Watching how the colony adapts as a unit in the quest for resources in extreme environments, like space, provides data that can be used to build algorithms with varied applications. Understanding how ants search in different conditions could have applications for robotics.

TAGES

The TAGES experiment (Transgenic Arabidopsis Gene Expression System) looks to see how microgravity impacts the growth of plant roots. Fluorescent markers placed on the plant’s genes allow scientists to study root development of Arabidopsis (a cress plant) grown on the space station. Evidence shows that directional light in microgravity skews root growth to the right, rather than straight down from the light source. Root growth patters on station mimic that of plants grown at at 45% degree angle on Earth. Space flight appears to slow the rate of the plant’s early growth as well.

Heart Cells

Spaceflight can cause a suite of negative health effects, which become more problematic as crew members stay in orbit for long periods of time. Effects of Microgravity on Stem Cell-Derived Cardiomycytes (Heart Cells) studies the human heart, specifically how heart muscle tissue contracts, grows and changes in microgravity. Understanding how heart muscle cells change in space improves efforts for studying disease, screening drugs and conducting cell replacement therapy for future space missions.

Medaka Fish

Chew on these results…Jaw bones of Japanese Medaka fish in microgravity show decreased mineral density and increased volume of osteoclasts, cells that break down bone tissue. Results from this study improve our understanding of the mechanisms behind bone density and organ tissue changes in space.

These experiments, and many others, emphasize the importance of biological research on the space station. Understanding the potential health effects for crew members in microgravity will help us develop preventatives and countermeasures.

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Other than joy, why do you do the things you do?

Perfect 10: A Decade of Studying Ice from the Sky

From 2009 through 2019, our Operation IceBridge flew planes above the Arctic, Antarctic and Alaska, measuring the height, depth, thickness, flow and change of sea ice, glaciers and ice sheets.

IceBridge was designed to “bridge” the years between NASA’s two Ice, Cloud, and land Elevation Satellites, ICESat and ICESat-2. IceBridge made its final polar flight in November 2019, one year after ICESat-2’s successful launch.

A lot of amazing science happens in a decade of fundamentally changing the way we see ice. Here, in chronological order, are 10 of IceBridge’s most significant and exciting achievements.

2009: Go for launch

The first ICESat monitored ice, clouds, atmospheric particles and vegetation globally beginning in 2003. As ICESat neared the end of its life, we made plans to keep measuring ice elevation with aircraft until ICESat-2’s launch.

ICESat finished its service in August 2009, leaving IceBridge in charge of polar ice tracking for the next decade.

2009: Snow on sea ice

To measure how thick sea ice is, we first have to know how much snow is accumulated on top of the ice. Using a snow radar instrument, IceBridge gathered the first widespread data set of snow thickness on top of both Arctic and Antarctic sea ice.

2009: Getting to the bottom of glaciers 

IceBridge mapped hundreds of miles of grounding lines in both Antarctica and Greenland. Grounding lines are where a glacier’s bottom loses contact with the bedrock and begins floating on seawater – a grounding line that is higher than rock that the ice behind it is resting on increases the possibility of glaciers retreating in the future. 

The team mapped 200 glaciers along Greenland’s coastal areas, as well as coastal areas, the interior of the Greenland Ice Sheet and high-priority areas in Antarctica.

2011: Spotting cracks in the ice

While flying Antarctica in 2011, IceBridge scientists spotted a massive crack in Pine Island Glacier, one of the fastest-changing glaciers on the continent. The crack produced a new iceberg that October.

Pine Island has grown thinner and more unstable in recent decades, spawning new icebergs almost every year. IceBridge watched for cracks that could lead to icebergs and mapped features like the deep water channel underneath Pine Island Glacier, which may bring warm water to its underside and make it melt faster.

2013: Making a map of rock

Using surface elevation, ice thickness and bedrock topography data from ICESat, IceBridge and international partners, the British Antarctic Survey created an updated map of the bedrock beneath Antarctic ice.

Taking gravity and magnetic measurements helps scientists understand what kind of rock lies below the ice sheet. Soft rock and meltwater make ice flow faster, while hard rock makes it harder for the ice to flow quickly.

2013: Surprises under the ice

IceBridge’s airborne radar data helped map the bedrock underneath the Greenland Ice Sheet, revealing a previously unknown canyon more than 400 miles long and up to a half mile deep slicing through the northern half of the country.

The “grand canyon” of Greenland may have once been a river system, and today likely transports meltwater from Greenland’s interior to the Arctic Ocean.

2015: It’s what’s inside (the ice sheet) that counts

After mapping the bedrock under the Greenland Ice Sheet, scientists turned their attention to the middle layers of the ice. Using both ice-penetrating radar and ice samples taken in the field, IceBridge created the first map of the ice sheet’s many layers, formed as thousands of years of snow became compacted downward and formed ice.

Making the 3D map of Greenland’s ice layers gave us clues as to how the ice sheet has warmed in the past, and where it may be frozen to bedrock or slowly melting instead.

2018: Gap bridged!

ICESat-2 launched on September 15, 2018, rocketing IceBridge into the final phase of its mission: Connecting ICESat and ICESat-2.

IceBridge continued flying after ICESat-2’s launch, working to verify the new satellite’s measurements. By conducting precise underflights, where planes traced the satellite’s orbit lines and took the same measurements at nearly the same time, the science teams could compare results and make sure ICESat-2’s instruments were functioning properly.

2018: An impact crater under the ice

Using IceBridge data, an international team of scientists found an impact crater from a meteor thousands of years in the past. The crater is larger than the city of Washington, D.C., likely created by a meteor more than half a mile wide.

2019: Flying into the sunset

In 2019, IceBridge continued flying in support of ICESat-2 for its Arctic and Antarctic campaigns. The hundreds of terabytes of data the team collected over the decade will fuel science for years to come.

IceBridge finished its last polar flight on November 20, 2019. The team will complete one more set of Alaska flights in 2020.

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Sing About NASA with Our Interns

Each semester, interns at Johnson Space Center (JSC) have the opportunity to contribute to our agency’s missions and help us lead the frontier of human space exploration. Interns at JSC also have the opportunity to enhance their experience through weekly meetings to discuss social and professional development topics, and can also get involved in many different committees.

The intern video committee from each semester comes up with ideas and carries out the entire process of creating a video that puts a creative, youthful spin on spreading NASA messages.

Here are a few highlights from some of the great intern videos that have been created:

Welcome to NASA

“Welcome to NASA” is based off of Flo Rida’s “My House” and was created to raise interest for our Journey to Mars. The lyrics and scenes in the video have been re-imagined in order to inform the public about the amazing work going on at NASA and the Johnson Space Center. 

Created in 2016

NASA is Good

This latest intern video is based off of Andy Grammer’s “Honey, I’m Good”. This video is designed as an outreach video to raise interest around the One-Year Mission aboard the International Space Station and the Pathways and Student Intern opportunities. 

Created in 2015

NASA Johnson Style

NASA Johnson Style was created as an educational parody of Psy’s "Gangnam Style". The intent of the video is to inform the public about the work being done at Johnson Space Center and throughout the agency. 

Created in 2012

I.S.S. Baby

A group of NASA interns collaborated to create the I.S.S Baby video based off of Vanilla Ice’s “Ice, Ice, Baby”. The video was designed as an outreach video to raise interest around the International Space Station. 

Created in 2008

There are plenty more JSC intern videos. You can watch more and learn about the work done at JSC and throughout the agency HERE.

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Help us put the ART in Artemis! Our step-by-step draw Artemis guide will help you learn how to draw the space suit that will keep our astronauts safe during their trip to the Moon.  Have fun, get creative and share your drawings using the hashtag #drawArtemis! 

Make sure to follow us on Tumblr for your regular dose of space: http://nasa.tumblr.com

Do illustrations suit you? Then enjoy NASA at Home fun while learning to draw Orion’s Space Suit that will keep Astronauts safe during Artemis missions to the Moon! Visit https://go.nasa.gov/2SRacx2 for instructions and be sure to share your tailor-made suits to #drawARTEMIS

A Wrinkle in Space-Time: The Eclipse That “Proved” Einstein Right

One hundred years ago a total solar eclipse turned an obscure scientist into a household name. You might have heard of him — his name is Albert Einstein. But how did a solar eclipse propel him to fame?

First, it would be good to know a couple things about general relativity. (Wait, don’t go! We’ll keep this to the basics!)

A decade before he finished general relativity, Einstein published his special theory of relativity, which demonstrates how space and time are interwoven as a single structure he dubbed “space-time.” General relativity extended the foundation of special relativity to include gravity. Einstein realized that gravitational fields can be understood as bends and curves in space-time that affect the motions of objects including stars, planets — and even light.

For everyday situations the centuries-old description of gravity by Isaac Newton does just fine. However, general relativity must be accounted for when we study places with strong gravity, like black holes or neutron stars, or when we need very precise measurements, like pinpointing a position on Earth to within a few feet. That makes it hard to test!

A prediction of general relativity is that light passing by an object feels a slight "tug", causing the light's path to bend slightly. The more mass the object has, the more the light will be deflected. This sets up one of the tests that Einstein suggested — measuring how starlight bends around the Sun, the strongest source of gravity in our neighborhood. Starlight that passes near the edge of the Sun on its way to Earth is deflected, altering by a small amount where those stars appear to be. How much? By about the width of a dime if you saw it at a mile and a quarter away! But how can you observe faint stars near the brilliant Sun? During a total solar eclipse!

That’s where the May 29, 1919, total solar eclipse comes in. Two teams were dispatched to locations in the path of totality — the places on Earth where the Moon will appear to completely cover the face of the Sun during an eclipse. One team went to South America and another to Africa.

On eclipse day, the sky vexed both teams, with rain in Africa and clouds in South America. The teams had only mere minutes of totality during which to take their photographs, or they would lose the opportunity until the next total solar eclipse in 1921! However, the weather cleared at both sites long enough for the teams to take images of the stars during totality.

The teams took two sets of photographs of the same patch of sky – one set during the eclipse and another set a few months before or after, when the Sun was out of the way. By comparing these two sets of photographs, researchers could see if the apparent star positions changed as predicted by Einstein. This is shown with the effect exaggerated in the image above.

A few months after the eclipse, when the teams sorted out their measurements, the results demonstrated that general relativity correctly predicted the positions of the stars. Newspapers across the globe announced that the controversial theory was proven (even though that’s not quite how science works). It was this success that propelled Einstein into the public eye.

The solar eclipse wasn’t the first test of general relativity. For more than two centuries, astronomers had known that Mercury’s orbit was a little off. Its perihelion — the point during its orbit when it is closest to the Sun — was changing faster than Newton’s laws predicted. General relativity easily explains it, though, because Mercury is so close to the Sun that its orbit is affected by the Sun’s dent in space-time, causing the discrepancy.  

In fact, we still test general relativity today under different conditions and in different situations to see whether or not it holds up. So far, it has passed every test we’ve thrown at it.

Curious to know where we need general relativity to understand objects in space? Tune into our Tumblr tomorrow to find out!

You can also read more about how our understanding of the universe has changed during the past 100 years, from Einstein's formulation of gravity through the discovery of dark energy in our Cosmic Times newspaper series.

Make sure to follow us on Tumblr for your regular dose of space: http://nasa.tumblr.com.

Celebrating the Earth (Off the Earth!)

To find the perfect perch for Earth observation research, just look up – about 240 miles up. The International Space Station serves as an optimal platform for studying our dynamic planet, where spectacular views support science.

With currently active instruments and facilities like High Definition Earth Viewing, Crew Earth Observations, Lightning Imaging Sensor, SAGE-III and Meteor, researchers on the ground are able to use the station’s unique (and useful!) vantage point to track Earth’s weather patterns, obtain images documenting changes on the planet’s surface, understand the origin of meteors falling towards Earth, and better understand the atmosphere.

The space station’s 90-minute orbit allows it to cover 90% of the Earth’s populated surfaces. That means we are able to study A LOT of that big blue marble.

Let’s talk a little about how the space station serves as a platform for Earth observation:

Each day, as the space station passes over regions of the Earth, crew members photograph the area below as a part of the Crew Earth Observations Facility investigation, one of the longest-running experiments on the orbiting laboratory. Crew members are able to photograph large-scale weather events like the recent Hurricane Harvey from the space station’s Cupola. These little science postcards from space can be used by researchers and the public to learn more about our home planet.

Want to see a picture of your hometown from space? Search for it in the Gateway to Astronaut Photography of Earth (GAPE).

The High Definition Earth Viewing (HDEV) experiment streams live video of Earth for online viewing. This investigation not only provides hours and hours of footage of the Earth below, but also demonstrates how the technology holds up against the harsh environment of space. High school students helped design some of the cameras' components, through the High Schools United with NASA to Create Hardware (HUNCH) program, and student teams perform most of the HDEV operation. (Whoa! Check out HUNCH and STEM on Station for more opportunities for student involvement!)

Useful for weather forecasting, hurricane monitoring, and observations of large-scale climate phenomena such as El Niño, RapidScat used radar pulses reflected off the ocean to measure wind speed and direction over the ocean.

RapidScat completed its successful two-year mission, outlasting its original decommission date before suffering a power loss. Although RapidScat is no longer transmitting data back to Earth, the station hosts many other Earth-observation tools the Cyclone Intensity Measurements from the ISS (CyMISS) an experiment that seeks to develop detailed information on tropical storm structure to better estimate storm intensity, which will help government agencies to better prepare communities for impending natural disasters; and the Cloud-Aerosol Transport System (CATS), a previously-flown lidar instrument which measured atmospheric profiles of aerosols and clouds to better understand their properties and interactions, as well as provided data useful to improving climate change models.

Learn more about RapidScat’s mission conclusion HERE! Take a look at CATS mission data HERE!

Watch more inspiring videos and learn about how we’re capturing the beauty of Earth HERE.

Crew members are able to photograph large-scale weather events like the recent Hurricane Harvey from the space station’s Cupola. These little science postcards from space can be used by researchers and the public to learn more about our home planet.

Plants in space!

Future long-duration missions into the solar system will require a fresh food supply to supplement crew diets, which means growing crops in space. Growing food in such a harsh environment also teaches us a little bit about growing in harsh environments here on Earth.

Here are a few plant-based investigations currently happening aboard the orbiting laboratory:

Veggie is a chamber on the space station that helps scientists grow, harvest and study different space crops. This experiment is called VEG-03D and they’ve been able to grow six rounds of crops so far.

SpaceX's 13th Commercial Resupply vehicle carried many valuable items to the orbiting laboratory, including Plant Gravity Perception, an investigation that uses the European Modular Cultivation System (EMCS) to simulate gravity to help plants grow its roots downward, and shoots upwards. The shoots need to face upwards, towards the light, so they can absorb sunlight and nutrients. Without this, plants wouldn’t know which way to grow. Yikes!

Learn more about Plant Gravity Perception HERE!

The Advanced Plant Habitat is a large chamber that supports commercial and fundamental plant research for at least one year of continuous use. A great feature to this habitat is that the astronauts can view the plant’s progress through a window on the door.

Whether astronauts are taking pictures of the planet or growing crops in space, all science aboard the space station plants seeds for a better life on Earth. Biology investigations directly grow our knowledge of agricultural techniques for harsh environments and imagery from space can give us a clearer idea of our planet’s health and emerging weather patterns.

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It’s National Composites Week! Wait, what’s a composite?

This week, we’re celebrating National Composites Week, which CompositesWorld says is about shedding some light on how “composite materials and composites manufacturing contributes to the products and structures that shape the American manufacturing landscape today.”

What exactly are composites and why are we talking about them?

Composites are building materials that we use to make airplanes, spacecraft and structures or instruments, such as space telescopes. But why are they special?

Composites consist of two or more materials, similar to a sandwich. Each ingredient in a sandwich could be eaten individually, but combining them is when the real magic happens. Sure, you could eat a few slices of cold cheese chased with some floppy bread. But real talk: buttery, toasted bread stuffed with melty, gooey Gouda makes a grilled cheese a much more satisfying nosh.

With composites—like our sandwich—the different constituent parts each have special properties that are enhanced when combined. Take carbon fibers which are strong and rigid. Their advantage compared to other structural materials is that they are much lighter than metals like steel and aluminum. However, in order to build structures with carbon fibers, they have to be held together by another material, which is referred to as a matrix. Carbon Fiber Reinforced Polymer is a composite consisting of carbon fibers set in a plastic matrix, which yields an extremely strong, lightweight, high-performing material for spacecraft.

Composites can also be found on the James Webb Space Telescope. They support the telescope’s beryllium mirrors, science instruments and thermal control systems and must be exquisitely stable to keep the segments aligned.

We invest in a variety of composite technology research to advance the use of these innovative materials in things like fuel tanks on spacecraft, trusses or structures and even spacesuits. Here are a few exciting ways our Space Technology Mission Directorate is working with composites:

Deployable structures on small spacecraft

We’re developing deployable composite booms for future deep space small satellite missions. These new structures are being designed to meet the unique requirements of small satellites, things like the ability to be packed into very small volumes and stored for long periods of time without getting distorted.

A new project, led by our Langley Research Center and Ames Research Center, called the Advanced Composite Solar Sail System will test deployment of a composite boom solar sail system in low-Earth orbit. This mission will demonstrate the first use of composite booms for a solar sail in orbit as well as new sail packing and deployment systems.

Nano (teeny tiny) composites

We are working alongside 11 universities, two companies and the Air Force Research Laboratory through the Space Technology Research Institute for Ultra-Strong Composites by Computational Design (US-COMP). The institute is receiving $15 million over five years to accelerate carbon nanotube technologies for ultra-high strength, lightweight aerospace structural materials. This institute engages 22 professors from universities across the country to conduct modeling and experimental studies of carbon nanotube materials on an atomistic molecular level, macro-scale and in between. Through collaboration with industry partners, it is anticipated that advances in laboratories could quickly translate to advances in manufacturing facilities that will yield sufficient amounts of advanced materials for use in NASA missions.

Through Small Business Innovative Research contracts, we’ve also invested in Nanocomp Technologies, Inc., a company with expertise in carbon nanotubes that can be used to replace heavier materials for spacecraft, defense platforms, and other commercial applications.

Nanocomp’s Miralon™ YM yarn is made up of pure carbon nanotube fibers that can be used in a variety of applications to decrease weight and provide enhanced mechanical and electrical performance. Potential commercial use for Miralon yarn includes antennas, high frequency digital/signal and radio frequency cable applications and embedded electronics. Nanocomp worked with Lockheed Martin to integrate Miralon sheets into our Juno spacecraft.

Composites for habitats

At last spring’s 3D-Printed Habitat Challenge the top two teams used composite materials in their winning habitat submissions. The multi-phase competition challenged teams to 3D print one-third scale shelters out of recyclables and materials that could be found on deep space destinations, like the Moon and Mars.

After 30 hours of 3D-printing over four days of head-to-head competition, the structures were subjected to several tests and evaluated for material mix, leakage, durability and strength. New York-based AI. SpaceFactory won first place using a polylactic acid plastic, similar to materials available for Earth-based, high-temperature 3D printers.

This material was infused with micro basalt fibers as well, and the team was awarded points during judging because major constituents of the polylactic acid material could be extracted from the Martian atmosphere.

Second place was awarded to Pennsylvania State University who utilized a mix of Ordinary Portland Cement, a small amount of rapid-set concrete, and basalt fibers, with water.

These innovative habitat concepts will not only further our deep space exploration goals, but could also provide viable housing solutions right here on Earth.

Student research in composites

We are also supporting the next generation of engineers, scientists and technologists working on composites through our Space Technology Research Grants. Some recently awarded NASA Space Technology Fellows—graduate students performing groundbreaking, space technology research on campus, in labs and at NASA centers—are studying the thermal conductivity of composites and an optimized process for producing carbon nanotubes and clean energy.

We work with composites in many different ways in pursuit of our exploration goals and to improve materials and manufacturing for American industry. If you are a company looking to participate in National Composites Week, visit: https://www.nationalcompositesweek.com.

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