The Sun Is Not Silent. The Low, Pulsing Hum Of Our Star's Heartbeat Allows Scientists To Peer Inside,

Vote for Space at SXSW 2017

We need your help! There are a number of exciting space-related panels proposed for next year’s South by Southwest Interactive Festival in Austin, Texas. SXSW is a community-driven event and voting accounts for 30% of the decision-making process for any given programming slot. The selection process is extremely competitive and the more votes we submit for the space panels, the more likely a panel related to space exploration will be included in the final SXSW program. 

To help you out as you consider what to vote for, we’ve put together a list of all the NASA-related panel proposals. 

These proposals look at ways we explore the solar system and beyond:

New Eyes on our Home System: NASA's Next Telescope

Dark Energy and Exoplanets: NASA's WFIRST Mission

Capturing NASA's James Webb Space Telescope

Lessons from the Fringes of the Solar System

Into the Unknown: The People Behind Webb Telescope

These proposals looks at how we’re using out-of-this-world tech and data to create incredible experiences here on Earth and helping solve challenges through your participation:

Space 360: Experience NASA Missions in VR/AR/video

The Power of Many: Wisdom from the Crowd 

It’s Time to Ask More of Open Data

A little closer to home, this proposal explores our work to study and observe our dynamic home world, Earth:

NASA - Doing Work to Keep it Cool 

We want to send humans on a journey to Mars. How? These proposals would dive into this question and more: 

So you want to go to Mars?

Humans, Robots + Microbes: The Challenge of Mars

"Because They Are Hard": NASA & Mars

Lastly, we’re proposing a meetup for NASA and the entire space community at SXSW 2017:

Space Meetup

Community voting and commenting for SXSW 2017 is open through September 2, 2016.

We look forward to seeing you in Austin in March at the SXSW Interactive Festival. Thanks!

Hubble’s Guide to Viewing Deep Fields

They say a picture is worth a thousand words, but no images have left a greater impact on our understanding of the universe quite like the Hubble Space Telescope’s deep fields. Like time machines, these iconic images transport humanity billions of light-years back in time, offering a glimpse into the early universe and insight into galaxy evolution!

You’ve probably seen these images before, but what exactly do we see within them? Deep field images are basically core samples of our universe. By peering into a small portion of the night sky, we embark on a journey through space and time as thousands of galaxies appear before our very eyes.

So, how can a telescope the size of a school bus orbiting 340 miles above Earth uncover these mind-boggling galactic masterpieces? We’re here to break it down. Here’s Hubble’s step-by-step guide to viewing deep fields:

Step 1: Aim at the darkness

Believe it or not, capturing the light of a thousand galaxies actually begins in the dark. To observe extremely faint galaxies in the farthest corners of the cosmos, we need minimal light interference from nearby stars and other celestial objects. The key is to point Hubble’s camera at a dark patch of sky, away from the outer-edge glow of our own galaxy and removed from the path of our planet, the Sun, or the Moon. This “empty” black canvas of space will eventually transform into a stunning cosmic mosaic of galaxies.

The first deep field image was captured in 1995. In order to see far beyond nearby galaxies, Hubble’s camera focused on a relatively empty patch of sky within the constellation Ursa Major. The results were this step-shaped image, an extraordinary display of nearly 3,000 galaxies spread across billions of light-years, featuring some of the earliest galaxies to emerge shortly after the big bang.

Step 2: Take it all in

The universe is vast, and peering back billions of years takes time. Compared to Hubble’s typical exposure time of a few hours, deep fields can require hundreds of hours of exposure over several days. Patience is key. Capturing and combining several separate exposures allows astronomers to assemble a comprehensive core slice of our universe, providing key information about galaxy formation and evolution. Plus, by combining exposures from different wavelengths of light, astronomers are able to better understand galaxy distances, ages, and compositions.

The Hubble Ultra Deep Field is the deepest visible-light portrait of our universe. This astonishing display of nearly 10,000 galaxies was imaged over the course of 400 Hubble orbits around Earth, with a total of 800 exposures captured over 11.3 days.

Step 3: Go beyond what’s visible

The ability to see across billions of light-years and observe the farthest known galaxies in our universe requires access to wavelengths beyond those visible to the human eye. The universe is expanding and light from distant galaxies is stretched far across space, taking a long time to reach us here on Earth. This  phenomenon, known as “redshift,” causes longer wavelengths of light to appear redder the farther they have to travel through space. Far enough away, and the wavelengths will be stretched into infrared light. This is where Hubble’s infrared vision comes in handy. Infrared light allows us to observe light from some of the earliest galaxies in our universe and better understand the history of galaxy formation over time.

In 2009, Hubble observed the Ultra Deep Field in the infrared. Using the Near Infrared Camera and Multi-Object Spectrometer, astronomers gathered one of the deepest core samples of our universe and captured some of the most distant galaxies ever observed.

Step 4: Use your time machine

Apart from their remarkable beauty and impressive imagery, deep field images are packed with information, offering astronomers a cosmic history lesson billions of years back in time within a single portrait. Since light from distant galaxies takes time to reach us, these images allow astronomers to travel through time and observe these galaxies as they appear at various stages in their development. By observing Hubble’s deep field images, we can begin to discover the questions we’ve yet to ask about our universe.

Credit: NASA, ESA, R. Bouwens and G. Illingworth (University of California, Santa Cruz)

Hubble’s deep field images observe galaxies that emerged as far back as the big bang. This image of the Hubble Ultra Deep Field showcases 28 of over 500 early galaxies from when the universe was less than one billion years old. The light from these galaxies represent different stages in their evolution as their light travels through space to reach us.

Step 5: Expand the cosmic frontier

Hubble’s deep fields have opened a window to a small portion of our vast universe, and future space missions will take this deep field legacy even further. With advancements in technologies and scientific instruments, we will soon have the ability to further uncover the unimaginable.

Slated for launch in late 2021, NASA’s James Webb Space Telescope will offer a new lens to our universe with its impressive infrared capabilities. Relying largely on the telescope’s mid-infrared instrument, Webb will further study portions of the Hubble deep field images in greater detail, pushing the boundaries of the cosmic frontier even further.

And there you have it, Hubble’s guide to unlocking the secrets of the cosmos! To this day, deep field images remain fundamental building blocks for studying galaxy formation and deepening not only our understanding of the universe, but our place within it as well.

Still curious about Hubble Deep Fields? Explore more and follow along on Twitter, Facebook, and Instagram with #DeepFieldWeek!

Make sure to follow us on Tumblr for your regular dose of space!

Hello!  @Astro_Jessica here ready to take your @nasa questions! @sxsw 

Whilst practicing solar distancing, Parker Solar Probe caught this rare glimpse of the twin tails on comet NEOWISE.☄

The twin tails are seen more clearly in this WISPR instrument processed image, which increased contrast and removed excess brightness from scattered sunlight, revealing more de-"tails". C/2020 F3 NEOWISE was discovered by our Near-Earth Object Wide-field Infrared Survey Explorer (NEOWISE), on March 27. Since it's discovery the comet has been spotted by several NASA spacecraft, including Parker Solar Probe, NASA’s Solar and Terrestrial Relations Observatory, the ESA/NASA Solar and Heliospheric Observatory, and astronauts aboard the International Space Station.

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

What’s the best piece of advice you have ever received?

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

Does Webb have resolution to look more closely at nearby objects, like Mars or even Earth? Or just far things?

Want to Help Save Earth’s Coral Reefs? Here’s Your Chance

Coral reefs are one of the most diverse ecosystems on the planet. They’re also in serious danger. Rising ocean temperatures, pollution and other threats are pushing corals towards extinction. But there’s hope. Using techniques originally developed to look at the stars, a team of scientists at our Ames Research Center in California’s Silicon Valley have developed a way to image corals in unprecedented detail. Now, the same team has launched a citizen science project, called NeMO-Net, to classify and assess the health of coral reefs across the globe. 

NeMO-Net is a coral classification game that lets you embark on a virtual research vessel and travel the oceans, analyzing actual images of corals on the sea floor. As you explore, you learn about the different types of corals and how to identify them. Your actions in-game train a supercomputer in the real world to classify corals on its own. Each classification you make will help researchers better understand how coral reefs are changing, and ultimately, find a way to save these amazing underwater worlds. Ready to play? Here’s a quick guide to getting started:

Download NASA NeMO-Net

Explore 3D images of the sea floor

Learn about the different types of corals

Identify and classify corals by painting images

Gain experience points, track your progress and be part of a global community of citizen scientists

NeMO-Net is available now on the Apple App Store, and is playable on iOS devices and Mac computers, with a forthcoming release for Android systems.  

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

Packing for a Journey into the Twilight Zone

Submitted for your consideration: A team of researchers from more than 20 institutions, boarding two research vessels, heading into the ocean’s twilight zone.

The twilight zone is a dimly lit region between 650 and 3300 feet below the surface, where we’re unfolding the mystery of how tiny ocean organisms affect our planet’s climate.

These tiny organisms – called phytoplankton – are plant-like and mostly single-celled. They live in water, taking in carbon dioxide and releasing oxygen.

Two boats, more than 100 researchers from more than 20 partner institutions, and a whole fleet of robotic explorers make up the EXport Processes in the Ocean from RemoTe Sensing (EXPORTS) team. We’re learning more about what happens to carbon dioxide after phytoplankton digest it.

The Equipment to Find Phytoplankton

Phytoplankton have predators in the ocean called zooplankton. They absorb the phytoplankton’s carbon, carrying it up the food chain. The EXPORTS mission will focus partly on how that happens in the ocean’s twilight zone, where some zooplankton live.  When phytoplankton die, sometimes their bodies sink through the same area. All of this carries carbon dioxide into the ocean’s depths and out of Earth’s atmosphere.

Counting Life

Studying the diversity of these organisms is important to better understand what’s happening to the phytoplankton as they die. Researchers from the Virginia Institute of Marine Science are using a very fine mesh net to sample water at various depths throughout the ocean to count various plankton populations.

Researchers from the University of Rhode Island are bringing the tools to sequence the DNA of phytoplankton and zooplankton to help count these organism populations, getting a closer look at what lives below the ocean’s surface.

Science at 500 Feet

Taking measurements at various depths is important, because phytoplankton, like plants, use sunlight to digest carbon dioxide. That means that phytoplankton at different levels in the ocean absorb and digest carbon differently. We’re bringing a Wirewalker, an instrument that glides up and down along a vertical wire to take in water samples all along its 500-foot long tether.

This journey to the twilight zone will take about thirty days, but we’ll be sending back dispatches from the ships. Follow along as we dive into ocean diversity on our Earth Expeditions blog: https://blogs.nasa.gov/earthexpeditions.

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

What Would These Astronauts Put in Their #NASAMoonKit?

NASA is hard at work to land the first woman and the next man on the Moon, and we want to know: what would you pack for a trip to the Moon?   

We will be soon conducting our last in a series of Green Run tests for the core stage of our Space Launch System (SLS) — the most powerful rocket ever built.

The series of tests is designed to gradually bring the rocket stage and all its systems to life for the first time — ensuring that it’s ready for missions to the Moon through the Artemis program.  

To mark this critical time in the history of American spaceflight, we’ve been asking people like you — what would you take with you on a trip to the Moon? Social media users have been regaling us with their images, videos, and illustrations with the hashtag #NASAMoonKit!

Looking for a little inspiration? We asked some of our astronauts and NASA leaders the same question:

1. NASA Astronaut Chris Cassidy

NASA astronaut Chris Cassidy recently took this photo from the International Space Station and posted it to his Twitter account with this caption:

“If I was on the next mission to the Moon, I would have to bring this tiny spaceman with me! He’s flown with me on all of my missions and was in my uniform pocket for all the SEAL missions I have been a part of. Kind of like a good luck charm.”

2. European Space Agency Astronaut Tim Peake

European Space Agency astronaut Tim Peake asked his two sons what they would take with them to the Moon. This is what they decided on!

3. NASA Astronaut Scott Tingle

Based on previous missions to space, NASA astronaut Scott Tingle would put a can of LiOH, or Lithium Hydroxide, into his #NASAMoonKit. 

A LiOH can pulls carbon dioxide out of the air — very important when you're in a closed environment for a long time! Apollo 13 enthusiasts will remember that the astronauts had to turn off their environmental system to preserve power. To keep the air safe, they used LiOH cans from another part of the vehicle, but the cans were round and the fitting was square. Today we have interoperability standards for space systems, so no more square pegs in round holes!

4. NASA Astronaut Drew Morgan

NASA astronaut Drew Morgan received some feedback from his youngest daughter when she was in kindergarten about she would put into her #NASAMoonKit.

5. Head of Human Spaceflight Kathy Lueders

Although Kathy Lueders is not an astronaut, she is the head of human spaceflight at NASA! Her #NASAMoonKit includes activities to keep her entertained as well as her favorite pillow.

6. NASA Astronaut Kenneth Bowersox

NASA astronaut Kenneth Bowersox knows from his past space shuttle experience what the “perfect space food” is — peanut butter. He would also put a hooded sweatshirt in his #NASAMoonKit, for those long, cold nights on the way to the Moon.

7. NASA Astronaut Michael Collins

NASA astronaut Michael Collins has actually made a real-life #NASAMoonKit — when he flew to the Moon on the Apollo 11 mission! But for this time around, he tweeted that would like to bring coffee like he did the first time — but add on a good book.  

How to Show Us What’s In Your #NASAMoonKit:

There are four social media platforms that you can use to submit your work:

Instagram: Use the Instagram app to upload your photo or video, and in the description include #NASAMoonKit  

Twitter: Share your image on Twitter and include #NASAMoonKit in the tweet  

Facebook: Share your image on Facebook and include #NASAMoonKit in the post  

Tumblr: Share your image in Tumblr and include #NASAMoonKit in the tags

If your #NASAMoonKit catches our eye, we may share your post on our NASA social media accounts or share it on the Green Run broadcast!

Click here for #NASAMoonKit Terms and Conditions.  

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