The Sun started September 2017 with flair, emitting 31 sizable solar flares and releasing several powerful coronal mass ejections, or CMEs, between Sept. 6-10.
Solar flares are powerful bursts of radiation. Harmful radiation from a flare cannot pass through Earth’s atmosphere to physically affect humans on the ground, however — when intense enough — they can disturb the atmosphere in the layer where GPS and communications signals travel.
CMEs are massive clouds of solar material and magnetic fields that erupt from the Sun at incredible speeds. Depending on the direction they’re traveling in, CMEs can spark powerful geomagnetic storms in Earth’s magnetic field.
As always, we and our partners had many missions observing the Sun from both Earth and space, enabling scientists to study these events from multiple perspectives. With this integrated picture of solar activity, scientists can better track the evolution of solar eruptions and work toward improving our understanding of space weather.
The National Oceanic and Atmospheric Administration (NOAA)’s Geostationary Operational Environmental Satellite-16, or GOES-16, watches the Sun’s upper atmosphere — called the corona — at six different wavelengths, allowing it to observe a wide range of solar phenomena. GOES-16 caught this footage of an X9.3 flare on Sept. 6, 2017.
This was the most intense flare recorded during the current 11-year solar cycle. X-class denotes the most intense flares, while the number provides more information about its strength. An X2 is twice as intense as an X1, an X3 is three times as intense, and so on. GOES also detected solar energetic particles associated with this activity.
Our Solar Dynamics Observatory captured these images of X2.2 and X9.3 flares on Sept. 6, 2017, in a wavelength of extreme ultraviolet light that shows solar material heated to over one million degrees Fahrenheit.
JAXA/NASA’s Hinode caught this video of an X8.2 flare on Sept. 10, 2017, the second largest flare of this solar cycle, with its X-ray Telescope. The instrument captures X-ray images of the corona to help scientists link changes in the Sun’s magnetic field to explosive solar events like this flare.
Key instruments aboard our Solar and Terrestrial Relations Observatory, or STEREO, include a pair of coronagraphs — instruments that use a metal disk called an occulting disk to study the corona. The occulting disk blocks the Sun’s bright light, making it possible to discern the detailed features of the Sun’s outer atmosphere and track coronal mass ejections as they erupt from the Sun.
On Sept. 9, 2017, STEREO watched a CME erupt from the Sun. The next day, STEREO observed an even bigger CME. The Sept. 10 CME traveled away from the Sun at calculated speeds as high as 7 million mph, and was one of the fastest CMEs ever recorded. The CME was not Earth-directed: It side-swiped Earth’s magnetic field, and therefore did not cause significant geomagnetic activity. Mercury is in view as the bright white dot moving leftwards in the frame.
Like STEREO, ESA/NASA’s Solar and Heliospheric Observatory, or SOHO, uses a coronagraph to track solar storms. SOHO also observed the CMEs that occurred during Sept. 9-10, 2017; multiple views provide more information for space weather models. As the CME expands beyond SOHO’s field of view, a flurry of what looks like snow floods the frame. These are high-energy particles flung out ahead of the CME at near-light speeds that struck SOHO’s imager.
Our Interface Region Imaging Spectrometer, or IRIS, captured this video on Sept. 10, 2017, showing jets of solar material swimming down toward the Sun’s surface. These structures are sometimes observed in the corona during solar flares, and this particular set was associated with the X8.2 flare of the same day.
Our Solar Radiation and Climate Experiment, or SORCE, collected the above data on total solar irradiance, the total amount of the Sun’s radiant energy, throughout Sept. 2017. While the Sun produced high levels of extreme ultraviolet light, SORCE actually detected a dip in total irradiance during the month’s intense solar activity.
A possible explanation for this observation is that over the active regions — where solar flares originate — the darkening effect of sunspots is greater than the brightening effect of the flare’s extreme ultraviolet emissions. As a result, the total solar irradiance suddenly dropped during the flare events.
Scientists gather long-term solar irradiance data in order to understand not only our dynamic star, but also its relationship to Earth’s environment and climate. We are ready to launch the Total Spectral solar Irradiance Sensor-1, or TSIS-1, this December to continue making total solar irradiance measurements.
The intense solar activity also sparked global aurora on Mars more than 25 times brighter than any previously seen by NASA’s Mars Atmosphere and Volatile Evolution, or MAVEN, mission. MAVEN studies the Martian atmosphere’s interaction with the solar wind, the constant flow of charged particles from the Sun. These images from MAVEN’s Imaging Ultraviolet Spectrograph show the appearance of bright aurora on Mars during the September solar storm. The purple-white colors show the intensity of ultraviolet light on Mars’ night side before (left) and during (right) the event.
For all the latest on solar and space weather research, follow us on Twitter @NASASun or Facebook.
GOES images are courtesy of NOAA. Hinode images are courtesy of JAXA and NASA. SOHO images are courtesy of ESA and NASA.
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For the first time in history, a spacecraft has touched the Sun. Our Parker Solar Probe flew right through the Sun’s atmosphere, the corona. (That’s the part of the Sun that we can see during a total solar eclipse.)
This marks one great step for Parker Solar Probe and one giant leap for solar science! Landing on the Moon helped scientists better understand how it was formed. Now, touching the Sun will help scientists understand our star and how it influences worlds across the solar system.
Unlike Earth, the Sun doesn’t have a solid surface (it’s a giant ball of seething, boiling gases). But the Sun does have a superheated atmosphere. Heat and pressure push solar material away from the Sun. Eventually, some of that material escapes the pull of the Sun’s gravity and magnetism and becomes the solar wind, which gusts through the entire solar system.
But where exactly does the Sun’s atmosphere end and the solar wind begin? We’ve never known for sure. Until now!
In April 2021, Parker Solar Probe swooped near the Sun. It passed through a massive plume of solar material in the corona. This was like flying into the eye of a hurricane. That flow of solar stuff — usually a powerful stream of particles — hit the brakes and went into slow-motion.
For the first time, Parker Solar Probe found itself in a place where the Sun’s magnetism and gravity were strong enough to stop solar material from escaping. That told scientists Parker Solar Probe had passed the boundary: On one side, space filled with solar wind, on the other, the Sun’s atmosphere.
Parker Solar Probe’s proximity to the Sun has led to another big discovery: the origin of switchbacks, zig-zag-shaped magnetic kinks in the solar wind.
These bizarre shapes were first observed in the 1990s. Then, in 2019, Parker Solar Probe revealed they were much more common than scientists first realized. But they still had questions, like where the switchbacks come from and how the Sun makes them.
Recently, Parker Solar Probe dug up two important clues. First, switchbacks tend to have lots of helium, which scientists know comes from the solar surface. And they come in patches.
Those patches lined up just right with magnetic funnels that appear on the Sun’s surface. Matching these clues up like puzzle pieces, scientists realized switchbacks must come from near the surface of the Sun.
Figuring out where switchbacks come from and how they form will help scientists understand how the Sun produces the solar wind. And that could clue us into one of the Sun’s biggest mysteries: why the Sun’s atmosphere is much, much hotter than the surface below.
Parker Solar Probe will fly closer and closer to the Sun. Who knows what else we’ll discover?
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Feast your eyes on the magnificent galaxy M51, also known as the Whirlpool Galaxy! This hypnotic spiral galaxy was captured in visible light with Hubble’s Advanced Camera for Surveys. Living up to its nickname, the Whirlpool Galaxy has the traits of a typical spiral galaxy, like beautifully curving arms, pink star-forming regions, and brilliant blue strands of star clusters.
The Whirlpool Galaxy is located about 31 million light-years away in the constellation Canes Venatici.
Discover more about the Whirlpool Galaxy here.
Right now, the Hubble Space Telescope is exploring #GalaxiesGalore! Find more galaxy content and spectacular new images by following along on Hubble’s Twitter, Facebook, and Instagram.
Credit: NASA, ESA, S. Beckwith (STScI), and the Hubble Heritage Team (STScI/AURA)
Through November 3, catch glimpses of a gibbous Venus, a crescent moon and ringed Saturn in the southwest sky just after sunset.
Wake up before sunrise every day this month to see Jupiter just above Spica, the brightest star in the constellation Virgo, shining in the east-southeast sky.
Just before dawn on November 23-24, see the waning crescent moon just above Jupiter.
November is a great time to see the constellation Ceres as it glides past Cetus, the Whale and you will be able to see the dwarf planet move relative to the background stars, but you’ll need a telescope for this one.
This month, just like last month, there will be three meteor showers--the Northern Tuarids, the Leonids and the November Orionids.
Watch the full November “What’s Up" video for more:
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As we remember the devastation that Hurricane Katrina caused ten years ago, we also look to the improvements made in the past decade in storm prediction and forecasting.
Hurricane Katrina impacted many people, businesses and communities; and even two NASA facilities were hit by the storm. Marshall Space Flight Center and Michoud Assembly Facility were both hit by the harsh storm (seen below).
During Hurricane Katrina in 2005, our satellites were hard at work monitoring and watching the storm from above. Thanks to the higher resolution models we have today, simulations can recreate historical storms, like the below of Hurricane Katrina. Scientists can then study these and learn about past events.
Surprisingly, the United States hasn’t experienced the landfall of a Category 3 hurricane or lager since 2005. This is the longest period of time that has passed without a major hurricane making landfall in the U.S. since reliable records began in 1850.
Although we don’t know when a severe storm will form, we do know that advancements in technology can help us better prepare and predict its path. So, on this ten year mark of this devastating storm, we look back to remember what we saw: https://www.flickr.com/photos/gsfc/sets/72157656646633089
October 28th is International Observe the Moon Night, a worldwide, public celebration of lunar science and exploration held annually since 2010 thanks to our Lunar Reconnaissance Orbiter (LRO) mission team and partners. One day each year, everyone on Earth is invited to observe and learn about the Moon together, and to celebrate the cultural and personal connections we all have with our planet’s nearest neighbor.
1. There has been a spacecraft there for 100 lunar days
In October 2017, LRO celebrates one hundred days of collecting scientific data at the Moon. One hundred Moon days. From our perspective on Earth, one lunar day is one full phase cycle, or about 29.5 Earth days. That's 100 opportunities to observe changes from night to day, photograph the surface at different Sun angles, measure rising and falling temperatures, study the way certain chemicals react to the daily light and temperature cycle, and increase our understanding of the Moon as a dynamic place.
2. You can still see the paths left by Apollo astronauts’ boot prints and rovers
Much of the lunar surface is covered in very fine dust. When Apollo astronauts landed on the Moon, the descent stage engine disturbed the dust and produced a distinct bright halo around the lunar module. As astronauts moved around, their tracks exposed the darker soil underneath, creating distinct trails that we know, thanks to LRO, are still visible today. The Moon has no atmosphere, so there is no wind to wipe away these tracks.
3. The Moon has tattoos!
Observations from LRO show mysterious patterns of light and dark that are unique to the Moon. These lunar swirls look painted on, like the Moon got ‘inked.’ Lunar swirls, like these imaged at Reiner Gamma by LRO, are found at more than 100 locations across the lunar surface. Lunar swirls can be tens of miles across and appear in groups or as isolated features.
Researchers think these patterns form in places where there’s still a remnant of the Moon’s magnetic field. There are still many competing theories about how swirls form, but the primary idea is that the local magnetic field deflects the energetic particles in the solar wind, so there’s not as much weathering of the surface. The magnetically shielded areas would then look brighter than everything around them.
4. There were once active volcanoes, that shaped what we see now
Early astronomers named the large dark spots that we see on the near side of the Moon “maria,” Latin for “seas,” because that’s what they thought they were. We now know that the dark spots are cooled lava, called basalt, formed from ancient volcanic eruptions. The Moon’s volcanoes are no longer active, but their past shapes the Moon that we see today. The Moon doesn’t have large volcanoes like ones in Hawaii, but it does have smaller cones and domes.
Other small features derived from volcanic activity include rivers of dried lava flows, like the ones visible in this image of Vallis Schroteri taken by LRO, and dark areas formed from eruptive volcanoes that spewed fire. For many years, scientists thought the Moon’s volcanic activity died out long ago, but there’s some evidence for relatively “young” volcanism, suggesting that the activity gradually slowed down instead of stopping abruptly.
5. Anyone, anywhere can participate in International Observe the Moon Night.
How to celebrate International Observe the Moon Night
Attend an event – See where events are happening near you by visiting http://observethemoonnight.org
Host an event – Call up your neighbors and friends and head outdoors – no special equipment is needed. Let us know how you celebrated by registering your event!
Don’t let cloudy weather get you down! Observe the Moon in a variety of ways from the comfort of indoors – View stunning lunar vistas through images and videos, or explore the Moon on your own with QuickMap or Moon Trek
Join the worldwide conversation with #ObserveTheMoon on Twitter, Instagram and Facebook
For regular Moon-related facts, updates and science, follow @NASAMoon on Twitter
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We have always been in the transportation business, whether launching astronauts to the Moon or improving airplanes to make them fly faster and safer on less fuel. And whether directly – like more aerodynamic wings for passenger jets – or indirectly – like more comfortable driver seats in sedans – this is yet another way our innovations benefit the public.
Today, the world of transportation is on the brink of some big changes. Drones are poised to make more efficient deliveries, crop surveillance and even disaster relief efforts. Taxis may soon take to the skies as well. And self-driving cars are ever closer to reality.
As we release our latest edition of NASA Spinoff, our yearly publication that celebrates the many ways our technology helps people on Earth, let’s take a closer look at some ways we’re helping augment transportation — and keeping everyone on the roads and in the skies safe.
If cars are going to drive themselves, they need to be able to “see” and assess the world around them, from other cars to pedestrians and bicyclists to a construction cone in the road. This is accomplished with the help of 3D cameras, or light detection and ranging (lidar), which sends out laser pulses and calculates where obstacles are by how long it takes that laser to bounce back.
But that, says engineer Farzin Amzajerdian at our Langley Research Center, is like building a 3D picture one pixel at a time. Instead, a new kind of lidar grabs a full array of pixels all at once. This “flash lidar” is faster and, because it has fewer moving parts, more reliable. It sailed through initial tests for possible use on a future Moon lander, and our partner has also sold the technology to a major car parts manufacturer, for autonomous cars.
Air traffic control has largely been a human operation so far, with people in control towers actively directing all 50,000 or so flights daily across the United States. But add in drones, and humans won’t be able to keep up: experts estimate there will soon be millions of aircraft in flight every day.
We’re helping automate and streamline flight control, working with the Federal Aviation Administration (FAA) and private companies to build the new technology needed to manage the anticipated challenges. Among other advances as a result, one company has built a platform used at airports, by air traffic controllers, and by drone operators around the world to more easily file flight plans, view the airspace, get clearance in restricted areas and more.
It may sound like something from the Jetsons, but real people are imagining the technology needed to make flying taxis a thing. And they’re probably not going to look anything like the passenger planes that we’re used to.
But when you start with a totally new design, there are all sorts of variables, including how much it will weigh. When it comes to flying, weight is a critical factor. For one thing, a heavier craft needs more fuel, but more fuel makes it even heavier. And all that weight stresses the structure, which means reinforcing it (more weight again!). Do it wrong, and all these factors cycle endlessly until you have something too heavy to get off the ground.
New software, designed with our help, generates fast and accurate weight estimates of novel aircraft designs, helping engineers figure out what works and how to make it better. Among other customers? UberElevate, which is trying to take rideshares to the skies.
We’ve even played a part in improving different kinds of joysticks, for everything from planes and video games, over the years. We had to because—especially in the early days of space travel—spacesuits were pretty unwieldy under the high g forces of launch and re-entry, so we needed to develop easy-to-use hand controls.
One former astronaut, Scott Parazynski, had acquired a wealth of experience training on and using NASA joysticks for jobs like maneuvering the International Space Station’s robotic arm. He realized similar technology could have even more of an impact on Earth. Parazynski, who is also a medical doctor, envisions improving robotic surgery with the new joystick he created; in the meantime, it’s already on the market for drones, making it easier than ever to use them to record aerial video, inspect a gas pipeline or even assess damage after a hurricane.
The “bird’s-eye view” is an expression for a reason: flying overhead provides a perspective you just can’t get with two feet planted on the ground. For the first time ever, we are going to get that bird’s eye view on Mars, and the same expertise that got us there is also giving farmers a new way to keep track of their crops.
The Mars Helicopter is poised to hitch a ride to the Red Planet with our latest rover, Perseverance, later this year. Designing it was a challenge: because there is so little air to provide lift on Mars, we needed something incredibly light (less than four pounds!) with large rotors that spin incredibly fast (nearly 3,000 times per minute).
We teamed up with a company we’ve worked with in the past on high-altitude, solar-powered, unmanned flyers. That company had something else in the works, using the same expertise: a drone equipped with two high-res cameras to capture images of crops as it flies overhead. The data from these images tells farmers where plants are thriving and where they’re not, informing them where they might need more (or less) water or fertilizer.
You can learn more about all these innovations, and dozens more, in the 2020 edition of NASA Spinoff. Read it online or request a limited quantity print copy and we’ll mail it to you!
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It’s time to get crafty with some needle and thread. At NASA, we hope to inspire art of all kinds. To highlight #WorldEmbroideryDay on July 30, we want to know: does our imagery inspire you? Show us your art and we may feature it on social media.
Search for a NASA image that inspires you. Here are a few places to get you started: Hubble, James Webb Space Telescope, Ocean Color, Landsat and Earth Observatory
Create. Over the years, we've seen a growing number of embroidered pieces that showcase our organization's research, especially with needlepoint.
Share your creation, along with the image it was inspired by, on social media using the hashtag #NASAEmbroidery. We will share selected pieces on July 30 for World Embroidery Day
NASA imagery has many functions. From studying distant galaxies to tracking ocean health, our scientists use these images to not only monitor our home planet, but better understand life beyond our solar system.
Embroidery is an ancient craft that has experienced a revival over the years. It involves decorating fabric or other materials using a needle to apply thread or yarn. Have you recently taken up embroidery? What images are you inspired by? We’d love to see it.
NASA Images
Hubble Image Gallery
NASA’s Ocean Color Image Gallery
James Webb Space Telescope
Landsat Image Gallery
Take a picture of your piece and upload it to Twitter, Instagram, Tumblr or Facebook. Make sure you use the hashtag #NASAEmbroidery so we know that you are taking part in the event and make sure that your privacy permissions allow us to view your post.
If the piece catches our eye, we may share your work on NASA’s main social media accounts as well as theme-related ones. We may also feature your art in a NASA Flickr gallery and our Tumblr pages. We’ll contact you directly to grant us permission to feature your work. You can follow @NASA on Twitter, Instagram and Facebook for embroidery creations, which will be featured from July 30-Aug. 1
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What does it feel like to float?? Do you have trouble adjusting to walking on the earth after that ??
On #WorldTeachersDay, we are recognizing our two current astronauts who are former classroom teachers, Joe Acaba and Ricky Arnold, as well as honoring teachers everywhere. What better way to celebrate than by learning from teachers who are literally out-of-this-world!
During the past Year of Education on Station, astronauts connected with more than 175,000 students and 40,000 teachers during live Q & A sessions.
Let’s take a look at some of the questions those students asked:
Taking a look at our home planet from the International Space Station is one of the most fascinating things to see! The views and vistas are unforgettable, and you want to take everyone you know to the Cupola (window) to experience this. Want to see what the view is like? Check out earthkam to learn more.
There are several experiments that take place on a continuous basis aboard the orbiting laboratory - anything from combustion to life sciences to horticulture. Several organizations around the world have had the opportunity to test their experiments 250 miles off the surface of the Earth.
If you are a good listener and follower, you can be successful on the space station. As you work with your team, you can rely on each other’s strengths to achieve a common goal. Each astronaut needs to have expeditionary skills to be successful. Check out some of those skills here.
Nothing excites Serena Auñón-Chancellor more than seeing a living, green plant on the International Space Station. She can’t wait to use some of the lettuce harvest to top her next burger! Learn more about the plants that Serena sees on station here.
While aboard the International Space Station, taste buds may not react the same way as they do on earth but the astronauts have access to a variety of snacks and meals. They have also grown 12 variants of lettuce that they have had the opportunity to taste.
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You seem to have spent a lot of time in some pretty isolated locations during your career, what are some challenges to that? Was there anything you enjoyed about it?
Explore the universe and discover our home planet with the official NASA Tumblr account
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