The 2021 Perseid Meteor Shower Is Here!

Meet Our ICONic New Satellite

The boundary between Earth and space is complicated and constantly changing. Unlike the rest of the atmosphere, the upper atmosphere near the edge of space has a mix of both neutral particles similar to the air we breathe, as well as electrically charged particles called ions. Changes in this region are unpredictable, but they can affect satellites and garble signals, like GPS, that pass through this region. That’s why we’re launching ICON (the Ionospheric Connection Explorer) to get our first-ever comprehensive look at our interface to space.

About 60 miles above Earth’s surface, Earth’s atmosphere gives way to space. The change is gradual: The gases of the atmosphere get steadily thinner the higher you go. On the edge of space, the Sun’s radiation cooks some of those thin gases until they lose an electron (or two or three), creating a population of electrically charged particles swarming alongside the neutral particles. These charged particles make up the ionosphere.

Because the particles of the ionosphere are electrically charged, they respond uniquely to electric and magnetic fields. Dynamic conditions in space — including shifting fields and surges of charged particles, collectively called space weather — induce shifts in the ionosphere that can have far-reaching effects. The ionosphere is where space weather manifests on Earth, and it’s inextricably connected with the neutral upper atmosphere — so distortions in one part affect the other.  

Changes in the ionosphere and upper atmosphere — including sudden shifts in composition, density, temperature, and conductivity — can affect satellites, building up electric charge that has the potential to disrupt instruments, and garble signals like those used by GPS satellites. Predicting these variances is hard, because the causes are so complex: They’re driven not only by space weather — usually a product of solar activity — but also by regular weather down near Earth’s surface.  

Differences in pressure caused by events like hurricanes, or even something as simple as a sustained wind over a mountain range, can ripple upwards until they reach this region and trigger fluctuations. Weather’s influence on the upper atmosphere was only discovered in the past ten years or so — and ICON is the first mission designed specifically to look at that interaction.

ICON carries four types of instruments to study the ionosphere and upper atmosphere. Three of them rely on taking far-away pictures of something called airglow, a faint, global glow produced by reactive compounds in the upper atmosphere. The fourth type collects and analyzes particles directly.

MIGHTI (the Michelson Interferometer for Global High-resolution Thermospheric Imaging) uses Doppler shift — the same effect that makes a siren change pitch as an ambulance passes you — to precisely track the speed and direction of upper-atmosphere winds.

FUV (the Far Ultraviolet instrument) measures airglow produced by certain types of oxygen and nitrogen molecules on Earth’s day side, as well as oxygen ions on Earth’s night side.

EUV (the Extreme Ultraviolet instrument) measures shorter wavelengths of light than FUV. Airglow measured by EUV is produced by oxygen ions on Earth’s day side, which make up the lion’s share of Earth’s daytime ionosphere.

The two identical IVMs (Ion Velocity Meters) make very precise measurements of the angle at which ionized gas enters the instruments, helping us build up a picture of how this ionized gas around the spacecraft is moving.

We’re launching ICON on June 14 Eastern Time on an Orbital ATK Pegasus XL rocket from Kwajalein Atoll in the Marshall Islands, which will deploy from Orbital’s L-1011 Stargazer aircraft. NASA TV will cover the launch — stay tuned to nasa.gov/live for updates and follow the mission on Twitter and Facebook.

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

Today we successfully tested one of our RS-25 engines, four of which will help power our Space Launch System (SLS) to deep space destinations, like Mars! This 500-second engine test concludes a summer of successful hot fire testing for flight controllers at our Stennis Space Center near Bay St. Louis, Mississippi.

The controller serves as the “brain” of the engine, communicating with SLS flight computers to ensure engines are performing at needed levels. The test marked another step toward the nation’s return to human deep-space exploration missions.

We launched a series of summer tests with a second flight controller unit hot fire at the end of May, then followed up with three additional tests. The flight controller tests are critical preparation for upcoming SLS flights to deep space– the uncrewed Exploration Mission-1 (EM-1), which will serve as the first flight for the new rocket carrying an uncrewed Orion spacecraft, and EM-2, which will transport a crew of astronauts aboard the Orion spacecraft. 

Each SLS rocket is powered at launch by four RS-25 engines firing simultaneously and working in conjunction with a pair of solid rocket boosters. The engines generate a combined 2 million pounds of thrust at liftoff. With the boosters, total thrust at liftoff will exceed 8 million pounds!

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

Can You #SpotHubble?

Hey Tumblr! We’re Inviting You to #SpotHubble

Since its launch in 1990, the Hubble Space Telescope has sent back mind-blowing images that not only changed our understanding of our universe, but also changed where we see our universe.

Hubble is more than a science instrument; it’s a cultural phenomenon! Take a moment to think about where you’ve seen the Hubble Space Telescope or Hubble images in your daily life. 

Maybe you walk by a mural inspired by Hubble images everyday on your way to work. 

Perhaps you’ve even created art based on Hubble images.

We want to see the Hubble impact in your life! Share your photos with us on Instagram, Twitter, Flickr and Facebook. If a #SpotHubble image catches our eye, we may share your post on our NASA Hubble social media accounts.

Here’s how to #SpotHubble!

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

Flickr: Submit your photos to the Spot Hubble Flickr Group

Instagram: Use the Instagram app to upload your photo, and in the description include #SpotHubble and #NASAGoddard

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

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

Please note, submissions are subject to certain terms and conditions.

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

Tournament Earth: The Earthly Eight

To celebrate Earth Observatory’s 20th anniversary and the 50th anniversary of Earth Day, we asked readers to pick our all-time best image. We have already completed two rounds of voting, which led to two rounds of stunning upsets. As we head into round 3, only two of the top eight seeds (#1s and #2s) remain. It is time now to cast your votes for the best of the Earthly 8. Voting ends on April 13 at 9 a.m. U.S. Eastern Time.

The nominees are separated into four groups: Past Winners, Home Planet, Land & Ice, and Sea & Sky. Check out the contenders still in the game:

Past Winners: Ocean Sand, Bahamas (#5 seed) vs. A View from Saturn (#2 seed)

Though the above image may resemble a new age painting straight out of an art gallery in Venice Beach, California, it is in fact a satellite image of the sands and seaweed in the Bahamas. The image was taken by the Enhanced Thematic Mapper plus (ETM+) instrument aboard the Landsat 7 satellite. Tides and ocean currents in the Bahamas sculpted the sand and seaweed beds into these multicolored, fluted patterns in much the same way that winds sculpted the vast sand dunes in the Sahara Desert.

This beautiful image of Saturn and its rings looks more like an artist’s creation than a real image, but in fact, the image is a composite (layered image) made from 165 images taken by the wide-angle camera on the Cassini spacecraft over nearly three hours on September 15, 2006. Scientists created the color in the image by digitally compositing ultraviolet, infrared, and clear-filter images and then adjusting the final image to resemble natural color. (A clear filter is one that allows in all the wavelengths of light the sensor is capable of detecting.) This image is a closeup view of the upper left quadrant of the rings, through which Earth is visible in the far, far distance. The full image can be seen here.

Home Planet: Twin Marbles (#1 seed) vs. Fire in the Sky and on the Ground (#7 seed)

A day’s clouds. The shape and texture of the land. The living ocean. City lights as a beacon of human presence across the globe. This amazingly beautiful view of Earth from space is a fusion of science and art, a showcase for the remote-sensing technology that makes such views possible, and a testament to the passion and creativity of the scientists who devote their careers to understanding how land, ocean, and atmosphere—even life itself—interact to generate Earth’s unique (as far as we know!) life-sustaining environment.

Astronauts on the International Space Station (ISS) used a digital camera to capture several hundred photographs of the aurora australis, or “southern lights,” while passing over the Indian Ocean on September 17, 2011. If you click on this movie, you can see the flowing ribbons and rays below as the ISS passed from south of Madagascar to just north of Australia between 17:22 and 17:45 Universal Time. Solar panels and other sections of the ISS fill some of the upper right side of the photograph.

Auroras are a spectacular sign that our planet is electrically and magnetically connected to the Sun. These light shows are provoked by energy from the Sun and fueled by electrically charged particles trapped in Earth’s magnetic field, or magnetosphere. In this case, the space around Earth was stirred up by an explosion of hot, ionized gas from the Sun—a coronal mass ejection—that left the Sun on September 14, 2011.

Ice and Land: Sand Dunes (#8 seed) vs. Retreat of Columbia Glacier (#6 seed)

Mountains of sand, some as tall as 300 meters (1000 feet), reach from the floor of Africa’s Namib Desert toward the sky. Driven by wind, these dunes march across the desert, bordered to the west by the Atlantic Ocean and in other directions by solid, rocky land.

The abrupt transition from sand to land is visible in this image, acquired on November 13, 2019, by the Operational Land Imager (OLI) on Landsat 8. They show the northern extent of the Namib Sand Sea—a field of sand dunes spanning more than 3 million hectares (more than 10,000 square miles) within the Namib-Naukluft Park, which was named a UNESCO World Heritage site in 2013. Sand appears red, painted by a layer of iron oxide.

Scientists have long studied Alaska's fast-moving Columbia Glacier, a tidewater glacier that descends through the Chugach Mountains into Prince William Sound. Yet the river of ice continues to deliver new surprises.

The image series begins in July 1986 (bottom image) with a false-color image captured by the Thematic Mapper (TM) sensor on the Landsat 5 satellite. The false-color image from July 2014 (top image), acquired by the Operational Land Imager on the Landsat 8 satellite, shows the extent of retreat after 28 years. Use the image comparison tool to better see the details.

Sea and Sky: Atafu Atoll, Tokelau (#8 seed) vs. Raikoke Erupts (#6 seed)

At roughly eight kilometers wide, Atafu Atoll is the smallest of three atolls and one island (Nukunonu and Fakaofo Atolls to the southeast and Swains Island to the south are not shown) comprising the Tokelau Islands group located in the southern Pacific Ocean. The primary settlement on Atafu is a village located at the northwestern corner of the atoll. The typical ring shape of the atoll is the result of coral reefs building up around a former volcanic island.

Unlike some of its perpetually active neighbors on the Kamchatka Peninsula, Raikoke Volcano on the Kuril Islands rarely erupts. The small, oval-shaped island most recently exploded in 1924 and in 1778.

The dormant period ended around 4:00 a.m. local time on June 22, 2019, when a vast plume of ash and volcanic gases shot up from its 700-meter-wide crater. Several satellites—as well as astronauts on the International Space Station—observed as a thick plume rose and then streamed east as it was pulled into the circulation of a storm in the North Pacific.

On the morning of June 22, astronauts shot this photograph of the volcanic plume rising in a narrow column and then spreading out in a part of the plume known as the umbrella region. That is the area where the density of the plume and the surrounding air equalize and the plume stops rising. The ring of clouds at the base of the column appears to be water vapor.

See all of the images and vote now HERE. 

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

Flying Observatory Has Big Plans for New Zealand

Our flying observatory, called SOFIA, carries a 100-inch telescope inside a Boeing 747SP aircraft. Scientists onboard study the life cycle of stars, planets (including the atmospheres of Pluto and Jupiter), nearby planetary systems, galaxies, black holes and complex molecules in space.

Flying South

Usually based in California, SOFIA and its team are returning to the Southern Hemisphere to study objects that aren't visible from the Northern Hemisphere and to take advantage of the long winter nights. The team operates from Christchurch, New Zealand, regularly between June and August and continues with more big plans for this year.

Working with New Horizons 

Our SOFIA and New Horizons teams are working together again, to learn more about the next object that the New Horizons spacecraft will fly past, Kuiper Belt Object 2014 MU69, or MU69. This will be the farthest object ever encountered by any spacecraft, but little is known about it. Our team on SOFIA will be searching for possible debris around MU69 that could damage the spacecraft and will measure its size, helping the New Horizons team plan their next flyby.

How We Study Distant Celestial Objects from Earth

Our SOFIA team will study MU69 on July 10, 2017, well before New Horizons arrives in January 2019. We can study this distant object from Earth by flying in the faint shadow that it will cast on Earth’s surface as it passes in front of a star. SOFIA will fly directly into the center of this shadow as it moves across the Pacific Ocean. From inside the shadow, the team onboard will study how the light from the star changes as MU69 passes in front it, allowing them to measure its size and to establish if there are any rings or debris around it. The observations will work in the same way that we studied Pluto using SOFIA two weeks before New Horizon’s Pluto Flyby in 2015.

Observing Other Galaxies

The Magellanic Clouds are neighboring galaxies to our own Milky Way Galaxy. We’re studying how stars are forming in the Large and Small Magellanic clouds to compare those processes to star formation in our own galaxy. The Magellanic Clouds are best observed from the southern hemisphere.

And Supernova 1987A

Inside the Large Magellanic Cloud is Supernova 1987A, the closest supernova explosion witnessed in almost 400 years. Our team onboard SOFIA will continue studying this supernova to better understand the material expanding out from it, which may become the building blocks of future stars and planets. Many of our telescopes have studied Supernova 1987A, including the Hubble Space Telescope, the Chandra X-ray Observatory and SOFIA’s predecessor, the Kuiper Airborne Observatory, but the instruments on SOFIA are the only tools we can use to study the debris around it at infrared wavelengths, to better understand characteristics of the dust that cannot be measured using other wavelengths of light.

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

Solar System: Things to Know This Week

See our home planet from Mars, learn about our latest Discovery missions, see stunning imagery from the Cassini mission and more!

1. Our Home

The powerful HiRISE camera on the Mars Reconnaissance Orbiter took this incredible image of our home and moon. The image combines two separate exposures taken on Nov. 20, 2016. 

+ See more 

2. Our Latest Missions of Discovery

We’ve selected two new missions to explore the early solar system. Lucy, a robotic spacecraft scheduled to launch in October 2021, is slated to arrive at its first destination, a main belt asteroid, in 2025. From 2027 to 2033, Lucy will explore six Jupiter Trojan asteroids. These asteroids are trapped by Jupiter's gravity in two swarms that share the planet's orbit, one leading and one trailing Jupiter in its 12-year circuit around the sun.

+Learn more

Psyche, targeted to launch in October 2023, will explore one of the most intriguing targets in the main asteroid belt--a giant metal asteroid, known as 16 Psyche. The asteroid is about 130 miles (210 kilometers) in diameter and thought to be comprised mostly of iron and nickel, similar to Earth's core.

+ Details

3. Image From Cassini  

Cassini took so many jaw-dropping photos last year, how could anyone choose just 10? Well, the Cassini team didn't. Here are 17 amazing photos from Saturn and its moons last year.

4. The Colors of Mars

Impact craters have exposed the subsurface materials on the steep slopes of Mars. However, these slopes often experience rockfalls and debris avalanches that keep the surface clean of dust, revealing a variety of hues, like in this enhanced-color image from our Mars Reconnaissance Orbiter, representing different rock types. 

+ Learn more

5. More From New Horizons

Even though our New Horizons mission flew by Pluto in 2015, the scientific discoveries keep coming. Using a model similar to what meteorologists use to forecast weather and a computer simulation of the physics of evaporating ices, scientists have found evidence of snow and ice features that, until now, had only been seen on Earth.

Discover the full list of 10 things to know about our solar system this week HERE.

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

Studying Storms from Air and Space

Technology we’ve developed is helping study the movement of storms.  

From satellites that can slice through a hurricane with 3-D vision to computer models of gale force winds, scientists now have unprecedented ways of viewing extreme weather.

This August, we’re sending an unmanned aircraft called a Global Hawk to study hurricanes. This mission is called the “East Pacific Origins and Characteristics of Hurricanes,” or EPOCH. It will fly over developing tropical storms to investigate how they progress and intensify. 

The three instruments aboard this Global Hawk aircraft will map out 3-D patterns of temperature, pressure, humidity, precipitation and wind speed as well as the role of the East Pacific Ocean in global cyclone formation. These measurements will help scientists better understand the processes that control storm intensity and the role of the East Pacific Ocean in global cyclone formation.

To better understand hurricane formation and intensity, scientists also utilize models and other observations.

Satellites such as our Global Precipitation Measurement Mission, or GPM, and computer models can analyze key stages of storm intensification.  

In September 2016, GPM captured Hurricane Matthew’s development from a Category 1 to Category 5 hurricane in less than 24 hours.  

Extreme rainfall was seen in several stages of the storm, causing significant flooding and landslides when it passed by Cuba, Haiti and the Dominican Republic.

By combining model and observed data, scientists can analyze storms like never before. They can also better understand how hurricanes and other powerful storms can potentially impact society.

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

What You Didn’t Know About Scott Kelly and Living in Space (Floating Urine is Involved)

First Ever NASA Reddit AMA from Space Recap

NASA astronaut Scott Kelly hosted a Reddit Ask Me Anything on Jan. 23 where people, well, asked him anything.

Kelly answered a range of questions from whether the crew members play space pranks on one another ("Occasionally…" Kelly said without elaboration.) to whether Kelly's recovery plan will be different than normal ("I think my rehab plan is the same as if I were here for 6 months, but I'm not positive.").

To start off, here are a few quick facts we learned about Kelly during the AMA:

The advice he would've given himself before going into space on day 1 would be to pack lighter.

His favorite David Bowie song is "Modern Love," and his favorite non-space related movie is "The Godfather." 

He uses a Nikon D4 when taking pictures (camera settings and lenses vary).

He thought it was cool to watch the movie "Gravity" while he was on the space station, because that's where the movie took place.

Once he lands, Kelly will miss the challenge of being aboard the space station the most.

Here are a few fun questions that astronaut Scott Kelly answered:

What’s the creepiest thing you’ve encountered while on the job?

Could a rogue spaceship sneak up on the space station?

We finally got an answer for one thing so many of you have been curious about…why does Scott Kelly always fold his arms?

When astronauts go up to space, they experience something very few others have and see Earth from a very unique perspective. What’s one thing Kelly will do differently once he returns home?

Kelly also told one user something unusual about being in space that people normally don’t think about: feet calluses.

Another user wanted to know what the largest societal misconception about space/space travel is. According to Kelly, it has nothing to do with science.

To read the entire Reddit AMA with Kelly, visit his IAmA thread.

Kelly's #YearInSpace ends Mar. 2. Follow him until the end of the journey (and beyond) on Twitter, Instagram and Facebook.

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

The Roasted Planet

Can you hear this exoplanet screaming? As the exoplanet known as HD 80606 b approaches its star from an extreme, elliptical orbit, it suffers star-grazing torture that causes howling, supersonic winds and shockwave storms across this world beyond our solar system. Its torturous journey boils its atmosphere to a hellish 2,000 degrees Fahrenheit every 111 days, roasting both its light and dark sides. HD 80606b will never escape this scorching nightmare. Download this free poster in English and Spanish and check out the full Galaxy of Horrors.

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

Solar System: 10 Things to Know This Week

Every day, our spacecraft and people are exploring the solar system. Both the public and the private sectors are contributing to the quest. For example, here are ten things happening just this week:

1. We deliver. 

The commercial space company Orbital ATK is targeting Saturday, Nov. 11 for the launch of its Cygnus spacecraft on an Antares rocket from Wallops Flight Facility in Wallops Island, Virginia. Cygnus is launching on a resupply mission to the International Space Station, carrying cargo and scientific experiments to the six people currently living on the microgravity laboratory. 

2. See for yourself. 

Social media users are invited to register to attend another launch in person, this one of a SpaceX Falcon 9 rocket carrying the Dragon spacecraft from Cape Canaveral Air Force Station in Florida. This launch, currently targeted for no earlier than December, will be the next commercial cargo resupply mission to the International Space Station. The deadline to apply is Nov. 7. Apply HERE.

3. Who doesn't like to gaze at the Moon?

Our Lunar Reconnaissance Orbiter (LRO) sure does—and from very close range. This robotic spacecraft has been orbiting Earth's companion since 2009, returning views of the lunar surface that are so sharp they show the footpaths made by Apollo astronauts. Learn more about LRO and the entire history of lunar exploration at NASA's newly-updated, expanded Moon site: moon.nasa.gov

4. Meanwhile at Mars...

Another sharp-eyed robotic spacecraft has just delivered a fresh batch of equally detailed images. Our Mars Reconnaissance Orbiter (MRO) surveys the Red Planet's surface daily, and you can see the very latest pictures of those exotic landscapes HERE. We currently operate five—count 'em, five—active missions at Mars, with another (the InSight lander) launching next year. Track them all at: mars.nasa.gov.

5. Always curious. 

One of those missions is the Curiosity rover. It's currently climbing a rocky highland dubbed Vera Rubin Ridge, turning its full array of instruments on the intriguing geology there. Using those instruments, Curiosity can see things you and I can't.

6. A new Dawn. 

Our voyage to the asteroid belt has a new lease on life. The Dawn spacecraft recently received a mission extension to continue exploring the dwarf planet Ceres. This is exciting because minerals containing water are widespread on Ceres, suggesting it may have had a global ocean in the past. What became of that ocean? Could Ceres still have liquid today? Ongoing studies from Dawn could shed light on these questions.

7. There are eyes everywhere. 

When our Mars Pathfinder touched down in 1997, it had five cameras: two on a mast that popped up from the lander, and three on the rover, Sojourner. Since then, photo sensors that were improved by the space program have shrunk in size, increased in quality and are now carried in every cellphone. That same evolution has returned to space. Our Mars 2020 mission will have more "eyes" than any rover before it: a grand total of 23, to create sweeping panoramas, reveal obstacles, study the atmosphere, and assist science instruments.

8. Voyage to a hidden ocean.

One of the most intriguing destinations in the solar system is Jupiter's moon Europa, which hides a global ocean of liquid water beneath its icy shell. Our Europa Clipper mission sets sail in the 2020s to take a closer look than we've ever had before. You can explore Europa, too: europa.nasa.gov

9. Flight of the mockingbird. 

On Nov. 10, the main belt asteroid 19482 Harperlee, named for the legendary author of To Kill a Mockingbird, makes its closest approach to Earth during the asteroid's orbit around the Sun. Details HERE. Learn more about asteroids HERE. Meanwhile, our OSIRIS-REx mission is now cruising toward another tiny, rocky world called Bennu.

10. What else is up this month? 

For sky watchers, there will be a pre-dawn pairing of Jupiter and Venus, the Moon will shine near some star clusters, and there will be meteor activity all month long. Catch our monthly video blog for stargazers HERE.

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