Eclipse 2017: A Unique Chance For Science

Studying the tiny life of phytoplankton

Phytoplankton. Have you ever heard of them? At NASA, these tiny organisms are kind of a big deal.

Biodiversity in the ocean is a delicate, but essential balance for life on Earth. One way NASA studies this balance is by observing phytoplankton – microalgae that contain chlorophyll, require light to grow, and form the base of the marine food chain.

Phytoplankton even have an essential role in an upcoming NASA mission.

This mission is called PACE- "Plankton, Aerosol, Cloud, ocean Ecosystem.” It will reveal interactions between the ocean and atmosphere, including how they exchange carbon dioxide and how atmospheric aerosols might fuel phytoplankton growth in the surface ocean.

Here are four areas main areas the mission will focus on as part of #WorldOceansMonth.

1. Harmful algal blooms: Not the good kind of bloom

The word “bloom” sounds pretty, but harmful algal blooms (HABs) are anything but.

When an ocean region is rich in nutrients – think of it as adding fertilizer to the ocean -  phytoplankton such as cyanobacteria multiply much faster than usual. This is called a “bloom.”

Some blooms are smelly and ugly but harmless. Others, like HABs, release toxins into the water that can make fish, shellfish, turtles and even humans very sick.

NASA’s PACE mission will help track phytoplankton growth and ocean health to make sure all of us stay healthy, balanced and blooming. In a good way.

2. Aerosols: The sea-sky connection

What do phytoplankton and clouds have in common? More than you might think.

PACE will also study aerosols, which are any particles or droplets suspended in our atmosphere. Humans create aerosols, like soot or car exhaust, but some phytoplankton release aerosols too.

For example, dust – also an aerosol – can blow into the ocean, depositing iron that helps phytoplankton grow. These phytoplankton then release dimethyl sulfide, a gas that turns into an aerosol, which can influence how clouds form.

Whether the aerosols in our atmosphere come from the ocean or land, it’s important to know how they are impacting our environment. PACE will help clear up some of our questions about what is in our air.

3. Biodiversity: The more, the merrier

A healthy ocean supports healthy industries and economies, contributes to a healthy atmosphere and helps keep plants, animals and humans healthy and happy. One key to a healthy, balanced ocean is lots of biodiversity.

Biodiversity means having a wide variety of plant and animal species in an ecosystem. It’s important to have many different species of phytoplankton, because each species plays a different role in processing carbon, providing food for tiny animals, and keeping the ocean healthy.

PACE will track the size and movements of phytoplankton populations from space to help our seas stay diverse and bountiful.

4. Fisheries: Phytoplankton feed fish feed friends

One simple reason for tracking the ocean’s health is that fish eat tiny animals that eat phytoplankton, and people eat fish.

Fisheries and aquaculture support about 12 percent of jobs around the world, including employing more than 3 million people in the United States. By better understanding our ocean’s health and how it might change in the future, we can make predictions about impacts to our economies and food supply.

To learn more about phytoplankton, visit our website.

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

How to Connect with NASA

We're the nation’s space agency, but that doesn’t mean you have to travel to the depths of the universe to stay connected with the awesome stuff we’re doing. There are actually some really easy ways to stay updated on all things space. Check them out:

Apps

We have lots of apps for smartphones and tablets that will make it easier than ever to stay connected to space. Here are a few to pique your interest:  

NASA App: Showcases a huge collection of the latest content, including images, videos, mission information, stories, space station sighting opportunities and more! Download: Apple/Android

NASA Spinoff App: This application profiles the best examples of technology that have been transferred from NASA research and missions into commercial products. From life-saving satellite systems to hospital robots, our technologies benefit society. Download: Apple

NASA 3DV App: The 3DV mobile app allows you to examine several of our Deep Space Exploration projects that will take our space program to asteroids, Mars and beyond! Download: Apple/Android

Spacecraft 3D: This augmented reality (AR) application lets you learn about and interact with a variety of spacecraft that are used to explore our solar system, study Earth and observe the universe. Download: Apple/Android

Competitions and Challenges

NASA Solve is an invitation to members of the public to contribute their time and expertise to solving problems and potentially winning prizes as a result of their work. This is a great way for individual members of the public to be a part of the nation’s space program. For a complete list of current challenges and competitions, visit THIS page.

Citizen Science

You don’t have to be a NASA employee to engage in the fun of interpreting scientific data and imagery from our many spacecraft and missions. As part of our Open Government plan, our goal is to promote transparency, participation and collaboration. By expanding the research base and using open innovation, we are all able to benefit from the accumulated findings. You can find data from our missions, research and activities HERE.

Email and Social Media

We have a wide-range of social media accounts here at NASA. Everything from Earth Science to the Mars Curiosity Rover, you can stay updated on many of our missions on many popular social media sites. For a full list of our accounts, visit THIS page.

If you’d like to get space news delivered straight to your inbox, you can sign up for updates and manage preferences HERE.

NASA Socials

What is a NASA Social? We’re glad you asked! These programs provide opportunities for our social media followers to learn and share information about our missions, people and programs. NASA Social includes both special in-person events and social media credentials for individuals who share the news in a significant way. Social events provide the participants with the opportunity to go behind-the-scenes at our facilities and events and speak with scientists engineers, astronauts and managers. Visit THIS page for a list of upcoming NASA Social opportunities.

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

Researchers Just Found (For The First Time) An 8th Planet Orbiting A Star Far, Far Away

Our Milky Way galaxy is full of hundreds of billions of worlds just waiting to be found. In 2014, scientists using data from our planet-hunting Kepler space telescope discovered seven planets orbiting Kepler-90, a Sun-like star located 2,500 light-years away. Now, an eighth planet has been identified in this planetary system, making it tied with our own solar system in having the highest number of known planets. Here’s what you need to know:

The new planet is called Kepler-90i.

Kepler-90i is a sizzling hot, rocky planet. It’s the smallest of eight planets in the Kepler-90 system. It orbits so close to its star that a “year” passes in just 14 days.

Average surface temperatures on Kepler-90i are estimated to hover around 800 degrees Fahrenheit, making it an unlikely place for life as we know it.

Its planetary system is like a scrunched up version of our solar system.

The Kepler-90 system is set up like our solar system, with the small planets located close to their star and the big planets farther away. This pattern is evidence that the system’s outer gas planets—which are about the size of Saturn and Jupiter—formed in a way similar to our own.

But the orbits are much more compact. The orbits of all eight planets could fit within the distance of Earth’s orbit around our Sun! Sounds crowded, but think of it this way: It would make for some great planet-hopping.

Kepler-90i was discovered using machine learning.

Most planets beyond our solar system are too far away to be imaged directly. The Kepler space telescope searches for these exoplanets—those planets orbiting stars beyond our solar system—by measuring how the brightness of a star changes when a planet transits, or crosses in front of its disk. Generally speaking, for a given star, the greater the dip in brightness, the bigger the planet!

Researchers trained a computer to learn how to identify the faint signal of transiting exoplanets in Kepler’s vast archive of deep-space data. A search for new worlds around 670 known multiple-planet systems using this machine-learning technique yielded not one, but two discoveries: Kepler-90i and Kepler-80g. The latter is part of a six-planet star system located 1,000 light-years away.

This is just the beginning of a new way of planet hunting.

Kepler-90 is the first known star system besides our own that has eight planets, but scientists say it won’t be the last. Other planets may lurk around stars surveyed by Kepler. Next, researchers are using machine learning with sophisticated computer algorithms to search for more planets around 150,000 stars in the Kepler database.

In the meantime, we’ll be doing more searching with telescopes.

Kepler is the most successful planet-hunting spacecraft to date, with more than 2,500 confirmed exoplanets and many more awaiting verification. Future space missions, like the Transiting Exoplanet Survey Satellite (TESS), the James Webb Space Telescope and Wide-Field Infrared Survey Telescope (WFIRST) will continue the search for new worlds and even tell us which ones might offer promising homes for extraterrestrial life.

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

*All images of exoplanets are artist illustrations.

What would happen if a Black hole would be near the earth? What would be the consequences to humans?

What was your favorite part of being a Flight Director?

A cluster of newborn stars herald their birth in this interstellar picture obtained with our Spitzer Space Telescope. These bright young stars are found in a rosebud-shaped (and rose-colored) nebulosity. The star cluster and its associated nebula are located at a distance of 3300 light-years in the constellation Cepheus.

A recent census of the cluster reveals the presence of 130 young stars. The stars formed from a massive cloud of gas and dust that contains enough raw materials to create a thousand Sun-like stars. In a process that astronomers still poorly understand, fragments of this molecular cloud became so cold and dense that they collapsed into stars. Most stars in our Milky Way galaxy are thought to form in such clusters.

The Spitzer Space Telescope image was obtained with an infrared array camera that is sensitive to invisible infrared light at wavelengths that are about ten times longer than visible light. In this four-color composite, emission at 3.6 microns is depicted in blue, 4.5 microns in green, 5.8 microns in orange, and 8.0 microns in red. The image covers a region that is about one quarter the size of the full moon.

As in any nursery, mayhem reigns. Within the astronomically brief period of a million years, the stars have managed to blow a large, irregular bubble in the molecular cloud that once enveloped them like a cocoon. The rosy pink hue is produced by glowing dust grains on the surface of the bubble being heated by the intense light from the embedded young stars. Upon absorbing ultraviolet and visible-light photons produced by the stars, the surrounding dust grains are heated and re-emit the energy at the longer infrared wavelengths observed by Spitzer. The reddish colors trace the distribution of molecular material thought to be rich in hydrocarbons.

The cold molecular cloud outside the bubble is mostly invisible in these images. However, three very young stars near the center of the image are sending jets of supersonic gas into the cloud. The impact of these jets heats molecules of carbon monoxide in the cloud, producing the intricate green nebulosity that forms the stem of the rosebud.

Not all stars are formed in clusters. Away from the main nebula and its young cluster are two smaller nebulae, to the left and bottom of the central 'rosebud,'each containing a stellar nursery with only a few young stars.

Astronomers believe that our own Sun may have formed billions of years ago in a cluster similar to this one. Once the radiation from new cluster stars destroys the surrounding placental material, the stars begin to slowly drift apart.

Additional information about the Spitzer Space Telescope is available at http://www.spitzer.caltech.edu.

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

What range/area will Perseverance be able to cover on the Martian surface? I'm assuming it's greater than the other rovers but by how much?

Demo-1: What’s the Deal?

Whether or not you caught the SpaceX Crew Dragon launch this past weekend, here’s your chance to learn why this mission, known as Demo-1, is such a big deal.

The First of its Kind

Demo-1 is the first flight test of an American spacecraft designed for humans built and operated by a commercial company. 

Liftoff

The SpaceX Crew Dragon lifted off at 2:49 a.m. EST Saturday, March 2, on the company’s Falcon 9 rocket from Kennedy Space Center. 

This was the first time in history a commercially-built American crew spacecraft and rocket launched from American soil. 

A New Era in Human Spaceflight

Upon seeing the arriving spacecraft, NASA astronaut Anne McClain snapped a photo from the International Space Station: “Welcome to a new era in human spaceflight.” 

Docking the Dragon

After making 18 orbits of Earth, the Crew Dragon spacecraft successfully attached to the International Space Station’s Harmony module at 5:51 a.m. EST Sunday, March 3. The Crew Dragon used the station’s new international docking adapter for the first time since astronauts installed it in August 2016. 

The docking phase, in addition to the return and recovery of Crew Dragon, are critical to understanding the system’s ability to support crew flights.

Opening the Hatch

After opening the hatch between the two spacecraft, the crewmates configured Crew Dragon for its stay. 

They installed a ventilation system that cycles air from Crew Dragon to the station, installed window covers and checked valves. After that, the crew was all set for a welcoming ceremony for the visiting vehicle. 

Ripley and Little Earth

Although the test is uncrewed, that doesn’t mean the Crew Dragon is empty. Along for the ride was Ripley, a lifelike test device outfitted with sensors to provide data about potential effects on future astronauts. (There is also a plush Earth doll included inside that can float in the microgravity!)

Inside the Dragon

For future operational missions, Crew Dragon will be able to launch as many as four crew members and carry more than 220 pounds of cargo. This will increase the number of astronauts who are able to live onboard the station, which will create more time for research in the unique microgravity environment.

Integration

Since the arrival of SpaceX Crew Dragon, the three Expedition 58 crew members have returned to normal operations (with some new additions to the team!) 

Undocking

The Crew Dragon is designed to stay docked to station for up to 210 days, although the spacecraft used for this flight test will remain docked to the space station for only five days, departing Friday, March 8. (We will be providing live coverage — don’t miss it!)

SpaceX and NASA

Elon Musk, CEO and lead designer at SpaceX, expressed appreciation for NASA’s support: “SpaceX would not be here without NASA, without the incredible work that was done before SpaceX even started and without the support after SpaceX did start.”

Preparation for Demo-2

NASA and SpaceX will use data from Demo-1 to further prepare for Demo-2, the crewed flight test that will carry NASA astronauts and Doug Hurley and Bob Behnken to the International Space Station. NASA will validate the performance of SpaceX’s systems before putting crew on board for the Demo-2 flight, currently targeted for July 2019.

Demo-1: So What?

Demo-1 is a big deal because it demonstrates NASA and commercial companies working together to advance future space exploration! With Demo-1’s success, NASA and SpaceX will begin to prepare to safely fly astronauts to the orbital laboratory.

Follow along with mission updates with the Space Station blog.

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

On June 19, engineers on the ground remotely operated the International Space Station’s robotic arm to remove the Roll-Out Solar Array (ROSA) from the trunk of SpaceX’s Dragon cargo vehicle. Here, you see the experimental solar array unfurl as the station orbits Earth.

Solar panels are an efficient way to power satellites, but they are delicate and large, and must be unfolded when a satellite arrives in orbit. The Roll-Out Solar Array (ROSA) is a new type of solar panel that rolls open in space like a party favor and is more compact than current rigid panel designs.

ROSA is 20% lighter and 4x smaller in volume than rigid panel arrays!

This experiment remained attached to the robotic arm over seven days to test the effectiveness of the advanced, flexible solar array that rolls out like a tape measure. During that time, they also measured power produced by the array and monitored how the technology handled retraction.

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

Launching Rockets from the Top of the World 🚀

Over the next 14 months, our scientists will join a group of international researchers to explore a special region — Earth's northern polar cusp, one of just two places on our planet where particles from the Sun have direct access to our atmosphere.

Earth is surrounded by a giant magnetic bubble known as a magnetosphere, which protects our planet from the hot, electrically charged stream of particles from the Sun known as the solar wind. The northern and southern polar cusps are two holes in this protection — here, Earth's magnetic field lines funnel the solar wind downwards, concentrating its energy before injecting it into Earth’s atmosphere, where it mixes and collides with particles of Earthly origin.

The cusp is the only place where dayside auroras are found — a special version of northern and southern lights, visible when the Sun is out and formed by a different process than the more familiar nighttime aurora. That's what makes this region so interesting for scientists to study: The more we learn about auroras, the more we understand about the fundamental processes that drive near-Earth space — including those processes that disrupt our technology and endanger our astronauts.

Photo credit: Violaene Kaeser

The teams working on the Grand Challenge Initiative — Cusp will fly sounding rockets from two Norwegian rocket ranges that fall under the cusp for a short time each day. Sounding rockets are sub-orbital rockets that shoot up into space for a few minutes before falling back to Earth, giving them access to Earth's atmosphere between 30 and 800 miles above the surface. Cheaper and faster to develop than large satellite missions, sounding rockets often carry the latest scientific instruments on their first-ever flights, allowing for unmatched speed in the turnaround from design to implementation.

Each sounding rocket mission will study a different aspect of Earth's upper atmosphere and its connection to the Sun and particles in space. Here's a look at the nine missions coming up.

1. VISIONS-2 (Visualizing Ion Outflow via Neutral Atom Sensing-2) — December 2018

The cusp isn’t just the inroad into our atmosphere — it’s a two-way street. Counteracting the influx of particles from the Sun is a process called atmospheric escape, in which Earthly particles acquire enough energy to escape into space. Of all the particles that escape Earth’s atmosphere, there’s one that presents a particular mystery: oxygen.

At 16 times the mass of hydrogen, oxygen should be too heavy to escape Earth’s gravity. But scientists have found singly ionized oxygen in near-Earth space, which suggests that it came from Earth. The two VISIONS-2 rockets, led by NASA's Goddard Space Flight Center in Greenbelt, Maryland, will create maps of the oxygen outflow in the cusp, tracking where these heavy ions are and how they’re moving to provide a hint at how they escape.

2. TRICE-2 (Twin Rockets to Investigate Cusp Electrodynamics 2) — December 2018

If the cusp is like a funnel, then magnetic reconnection is what turns on the faucet. When the solar wind collides with Earth’s magnetic field, magnetic reconnection breaks open the previously closed magnetic field lines, allowing some solar wind particles to stream into Earth’s atmosphere through the cusp.

But researchers have noticed that the stream of particles coming in isn’t smooth: instead, it has abrupt breaks in it. Is magnetic reconnection turning on and off? Or is the solar wind shooting in from different locations? TRICE-2, led by the University of Iowa in Iowa City, will fly two separate rockets through a single magnetic field line in the cusp, to help distinguish these possibilities. If reconnection sputters on and off over time, then the two rockets should get quite different measurements, like noting how it feels to run your finger back and forth under a faucet that is being turned on and off. If instead reconnection happens consistently in multiple locations — like having ten different faucets, all running constantly — then the two rockets should have similar measurements whenever they pass through the same locations.

Magnetic reconnection is a process by which magnetic field lines explosively realign  

3. CAPER-2 (Cusp Alfvén and Plasma Electrodynamics Rocket) — January 2019

The CAPER-2 rocket, led by Dartmouth College in Hanover, New Hampshire, will examine how fast-moving electrons — particles that can trigger aurora — get up to such high speeds. The team will zero in on the role that Alfvén waves, a special kind of low-frequency wave that oscillates along magnetic field lines, play in accelerating auroral electrons.

An illustration of rippling Alfvén waves

4. G-CHASER (Grand Challenge Student Rocket) — January 2019

G-CHASER is made up entirely of student researchers from universities in the United States, Norway and Japan, many of whom are flying their experiments for the first time. The mission, led by the Colorado Space Grant Consortium at the University of Colorado Boulder, is a collaboration between seven different student-led missions, providing a unique opportunity for students to design, test and ultimately fly their experiment from start to finish. The students involved in the mission — mostly undergraduates but including some graduate teams — are responsible for all aspects of the mission, from developing the initial idea, to securing the funding, to making sure it passes all the tests before flight.

5 & 6. AZURE (Auroral Zone Upwelling Rocket Experiment) and CHI (Cusp Heating Investigation) — April & November/December 2019

When the aurora shine, they don’t just emit light — they also release thermal and kinetic energy into the atmosphere. Some of this energy escapes back into space, but some of it stays with us. Which way this balance tips depends, in part, on the winds in the cusp. AZURE, led by Clemson University in South Carolina, will measure the vertical winds that swish energy and particles around within the auroral oval, the larger ring around the pole where the aurora are most common.

Later that year, the same team will launch the CHI mission, using a methodology similar to AZURE to measure the flow of charged and neutral gases inside the cusp. The goal is to better understand how particles, flowing in horizontal and vertical directions, interact with each other to produce heating and acceleration.

7. C-REX-2 (Cusp-Region Experiment) — November 2019

The cusp is a place where strange physics happens, producing some anomalies in the physical structure of the atmosphere that can make our technology go haywire. For satellites that pass through the cusp, density increases act like potholes, shaking up their orbits. Scientists don’t currently understand what causes these density increases, but they have some clues. C-REX-2, led by the University of Alaska Fairbanks, aims to figure out which variables — wind, temperature or ion velocity — are responsible.

8. ICI-5 (Investigation of Cusp Irregularities-5) — December 2019

Recent research has uncovered mysterious hot patches of turbulent plasma inside the auroral region that rain energetic particles towards Earth. GPS signals become garbled as they pass through these turbulent plasma patches, affecting so many of today’s technologies that depend on them. ICI-5, led by the University of Oslo, will launch into the cusp to take measurements from inside these hot patches. To measure their structure as several scales, the rocket will eject 12 daughter payloads in concentric squares which will achieve a variety of different separations.

9. JAXA's SS-520-3 mission — January 2020

Exploring the phenomenon of atmospheric escape, the Japan Aerospace Exploration Agency's SS-520-3 mission will fly 500 miles high over the cusp to take measurements of the electrostatic waves that heat ions up and get them moving fast enough to escape Earth.

For updates on the Grand Challenge Initiative and other sounding rocket flights, visit nasa.gov/soundingrockets or follow along with NASA Wallops and NASA heliophysics on Twitter and Facebook.

@NASA_Wallops | NASA's Wallops Flight Facility | @NASASun | NASA Sun Science

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