Milky Blue Water Near Prince Of Wales Island

Get Ready Stargazers: The Geminids Are Here!

The Geminid meteor shower, one of the biggest meteor showers of the year, will peak this weekend, December 13 to 14. We get a lot of questions about the Geminids—so we’ve put together some answers to the ones we’re most commonly asked. Take a look!  

What are the Geminids?

The Geminids are pieces of debris from an asteroid called 3200 Phaethon. Earth runs into Phaethon’s debris stream every year in mid-December, causing meteors to fly from the direction of the constellation Gemini – hence the name “Geminids.”  

Image Credit: Arecibo Observatory/NASA/NSF

When is the best time to view them?

This year, the peak is during the overnight hours of December 13 and into the morning of December 14. Viewing should still be good on the night of December 14 into the early morning hours of the 15th. Weather permitting, the Geminids can be viewed from around midnight to 4 a.m. local time. The best time to see them is around 2 a.m. your local time on December 14, when the Geminid radiant is highest in your night sky. The higher the radiant – the celestial point in the sky from which meteors appear to originate – rises into the sky, the more meteors you are likely to see.

Image Credit & Copyright: Jeff Dai

What is the best way to see them?

Find the darkest place you can and give your eyes about 30 minutes to adapt to the dark. Avoid looking at your cell phone, as it will disrupt your night vision. Lie flat on your back and look straight up, taking in as much sky as possible. You will soon start to see the Geminid meteors!

Image Credit: NASA/Bill Dunford

Can you see the Geminids from anywhere in the world?

The Geminids are best observed in the Northern Hemisphere, but no matter where you are in the world (except Antarctica), some Geminids will be visible.

Image Credit: Jimmy Westlake

How many Geminids can I expect to see?

Under dark, clear skies, the Geminids can produce up to 120 meteors per hour – but this year, a bright, nearly full moon will hinder observations of the shower. Still, observers can hope to see up to 30 meteors per hour. Happy viewing!  

Image Credit & Copyright: Yuri Beletsky

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The Pale Blue Dot and the Golden Record

Almost thirty years ago, on Feb. 14, 1990, our Voyager 1 spacecraft turned back toward its home for one last look. 40 astronomical units (almost 4 billion miles) from the Sun, Voyager snapped the first-ever “family portrait” of our solar system.

One image in particular highlights our own planet’s fragility in the vast cosmic arena that we call home. This image of Earth, a tiny point of light, is contained in a camera artifact that resembles a beam of sunlight.

The late Carl Sagan referred to this image of Earth in the title of his 1994 book, Pale Blue Dot. Sagan wrote: "That's here. That's home. That's us. On it everyone you love, everyone you know, everyone you ever heard of, every human being who ever was, lived out their lives. … There is perhaps no better demonstration of the folly of human conceits than this distant image of our tiny world. To me, it underscores our responsibility to deal more kindly with one another, and to preserve and cherish the pale blue dot, the only home we've ever known.”

We placed a message aboard Voyager 1 and 2 — a kind of time capsule intended to communicate a story of our world to extraterrestrials. The Voyager message is carried by a phonograph record: a 12-inch gold-plated copper disk containing sounds and images selected to portray the diversity of life and culture on Earth.

The Golden Record includes 115 images and a variety of natural sounds, such as those made by surf, wind and thunder, birds, whales and other animals. Musical selections from different cultures and eras were also added, as well as spoken greetings from Earth-people in fifty-five languages and printed messages from President Carter.

The Golden Record represents the whole of humanity, mounted to a feat of human engineering on a long voyage through interstellar space. 

You can listen to the sounds of Earth on the golden record here and take a moment to appreciate our pale blue dot. 

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This Week @ NASA

Astronauts conduct a spacewalk on the International Space Station to prepare it for future activities. Peggy Whitson became the new women’s record holder for number of spacewalks and more!

International Space Station

Work continued aboard the International Space Station. Spacewalkers Shane Kimbrough and Peggy Whitson used the station’s robotic arm to move the Pressurized Mating Adapter-3 on March 24 to move a module to accommodate U.S. commercial spacecraft carrying astronauts on future missions. They continued this work on March 30. Another spacewalk to complete the work is slated for April.

James Webb Space Telescope

Engineers at our Goddard Space Flight Center Center complete vibration and acoustic tesing on the James Webb Space Telescope, which was subjected to earsplitting noice and shaken 50-100 times per second to simulate the rigors of launch.

MAVEN

Data from our MAVEN, our Mars Atmosphere and Volatile EvolutioN, and published in the journal Science, concludes that solar wind and radiation are responsible for stripping Mars of its atmosphere and turning it into the frigid desert world it is today.

Most of the gas ever in the Red Planet’s atmosphere has been lost to space. The MAVEN team focused on the gas argon, estimating that 65% of it has been stripped from the planet. In 2015, the science team determined that atmospheric gas continues to be lost to space.

STEM Education

We participated in a Women’s History Month celebration and the Smithsonian Air and Space Museum. The program feature NASA astronauts and engineers. The were also projects to get girls interested in sciene, technology, engineering and math, or STEM, education. There was also a screening of the film ‘Hidden Figures,’ which relates the story of African-American female mathematicians who were instrumental in the agency’s efforts to launch humans to space.

NASA App on Fire TV

We’ve released our latest free NASA app on a whole new platform--Amazon Fire TV! The app is already available for Apple TV, iOS, and Android.Viewers can stream NASA TV, access 16,000+, download video and more!

Download the app: www.nasa.gov/nasaapp

What the full episode of This Week @ NASA:

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OMG! Ice is Melting from Below

Oceans Melting Greenland (OMG) scientists are heading into the field this week to better understand how seawater is melting Greenland’s ice from below. (Yes, those black specks are people next to an iceberg.) While NASA is studying ocean properties (things like temperature, salinity and currents), other researchers are eager to incorporate our data into their work. In fact, University of Washington scientists are using OMG data to study narwhals – smallish whales with long tusks – otherwise known as the “unicorns of the sea.”

 Our researchers are also in the field right now studying how Alaska’s ice is changing. Operation IceBridge, our longest airborne campaign, is using science instruments on airplanes to study and measure the ice below.

What happens in the Arctic doesn’t stay in the Arctic (or the Antarctic, really). In a warming world, the greatest changes are seen in the coldest places. Earth’s cryosphere – its ice sheets, sea ice, glaciers, permafrost and snow cover – acts as our planet’s thermostat and deep freeze, regulating temperatures and storing most of our freshwater. Next month, we’re launching ICESat-2, our latest satellite to study Earth’s ice!

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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.

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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.

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The Summer Solstice Has Arrived!

This year’s summer solstice for the northern hemisphere arrives at 11:54 a.m. EDT, meaning today is the longest day of the year! The number of daylight hours varies by latitude, so our headquarters in Washington, D.C. will see 14 hours, 53 minutes, and 51 seconds of daylight. A lot can happen in that time! Let’s find out more.

If you’re spending the day outside, you might be in the path of our Earth Science Satellite Fleet (ESSF)! The fleet, made up of over a dozen Earth observation satellites, will pass over the continental United States about 37 times during today’s daylight hours. 

These missions collect data on atmospheric chemistry and composition, cloud cover, ocean levels, climate, ecosystem dynamics, precipitation, and glacial movement, among other things. They aim to do everything from predicting extreme weather to helping informing the public and decision makers with the environment through GPS and imaging. Today, their sensors will send back over 200 gigabytes (GB) of data back to the ground by sunset. 

As the sun sets today, the International Space Station (ISS) will be completing its 10th orbit since sunrise. In that time, a little more than 1 terabyte-worth of data will be downlinked to Earth.

That number encompasses data from ground communications, payloads, experiments, and control and navigation signals for the station. Approximately 330 GB of that TB is video, including live broadcasts and downlinks with news outlets. But as recently-returned astronaut Serena Auñón-Chancellor likes to point out, there’s still room for fun. The astronauts aboard the ISS can request YouTube videos or movies for what she likes to call “family movie night.”

Astronauts aboard the station also send back images—LOTS of them. Last year, astronauts sent back an average of 66,912 images per month! During today’s long hours of daylight, we expect the crew to send back about 656 images. But with Expedition 59 astronauts David Saint-Jacques (CSA), Anne McClain (NASA), and Oleg Kononenko (RKA) hard at work preparing to return to Earth on Monday, that number might be a little less. 

Say you’re feeling left out after seeing the family dinners and want to join the crew. Would you have enough daylight to travel to the ISS and back on the longest day of the year? Yes, but only if you’re speedy enough, and plan your launch just right. With the current fastest launch-to-docking time of about six hours, you could complete two-and-a-half flights to the ISS today between sunrise and sunset.

When returning from orbit, it’s a longer ordeal. After the Expedition 59 trio arrives on Earth Monday night, they’ll have to travel from Kazakhstan to Houston to begin their post-flight activities. Their journey should take about 18 hours and 30 minutes, just a few hours longer than the hours of daylight we’ll see today.

Happy solstice! Make sure to tune in with us on Monday night for live coverage of the return of Expedition 59. Until then, enjoy the longest day of the year!

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The Sun Just Released the Most Powerful Flare of this Solar Cycle

The Sun released two significant solar flares on Sept. 6, including one that clocked in as the most powerful flare of the current solar cycle.

The solar cycle is the approximately 11-year-cycle during which the Sun’s activity waxes and wanes. The current solar cycle began in December 2008 and is now decreasing in intensity and heading toward solar minimum, expected in 2019-2020. Solar minimum is a phase when solar eruptions are increasingly rare, but history has shown that they can nonetheless be intense.

Footage of the Sept. 6 X2.2 and X9.3 solar flares captured by the Solar Dynamics Observatory in extreme ultraviolet light (131 angstrom wavelength)

Our Solar Dynamics Observatory satellite, which watches the Sun constantly, captured images of both X-class flares on Sept. 6.

Solar flares are classified according to their strength. X-class denotes the most intense flares, followed by M-class, while the smallest flares are labeled as A-class (near background levels) with two more levels in between. Similar to the Richter scale for earthquakes, each of the five levels of letters represents a 10-fold increase in energy output. 

The first flare peaked at 5:10 a.m. EDT, while the second, larger flare, peaked at 8:02 a.m. EDT.

Footage of the Sept. 6 X2.2 and X9.3 solar flares captured by the Solar Dynamics Observatory in extreme ultraviolet light (171 angstrom wavelength) with Earth for scale

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 Earth’s atmosphere in the layer where GPS and communications signals travel.

Both Sept. 6 flares erupted from an active region labeled AR 2673. This area also produced a mid-level solar flare on Sept. 4, 2017. This flare peaked at 4:33 p.m. EDT, and was about a tenth the strength of X-class flares like those measured on Sept. 6.

Footage of the Sept. 4 M5.5 solar flare captured by the Solar Dynamics Observatory in extreme ultraviolet light (131 angstrom wavelength)

This active region continues to produce significant solar flares. There were two flares on the morning of Sept. 7 as well. 

For the latest updates and to see how these events may affect Earth, please visit NOAA’s Space Weather Prediction Center at http://spaceweather.gov, the U.S. government’s official source for space weather forecasts, alerts, watches and warnings.

Follow @NASASun on Twitter and NASA Sun Science on Facebook to keep up with all the latest in space weather research.

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The California Wildfires from Above

As massive wildfires continue to rage in southern California, our satellites, people in space and aircraft are keeping an eye on the blazes from above. 

This data and imagery not only gives us a better view of the activity, but also helps first responders plan their course of action. 

A prolonged spell of dry weather primed the area for major fires. The largest of the blazes – the fast-moving Thomas fire in Ventura County – charred more than 65,000 acres.

Powerful Santa Ana winds fanned the flames and forecasters with the LA office of the National Weather Service warned that the region is in the midst of its strongest and longest Santa Ana wind event of the year. 

These winds are hot, dry and ferocious. They can whip a small brush fire into a raging inferno in just hours.

Our Aqua satellite captured the above natural-color image on Dec. 5. Actively burning areas are outlined in red. Each hot spot is an area where the thermal detectors on the satellite recognized temperatures higher than the background.

On the same day, the European Space Agency’s Sentinel-2 satellite captured the data for the above false-color image of the burn scar. This image uses observations of visible, shortwave infrared and near infrared light.

From the vantage point of space, our satellites and astronauts are able to see a more comprehensive view of the activity happening on the ground. 

The crew living and working 250 miles above Earth on the International Space Station passed over the fires on Dec. 6. The above view was taken by astronaut Randy Bresnik as the station passed over southern California.

During an engineering flight test of our Cloud-Aerosol Multi-Angle Lidar (CAMAL) instrument, a view from our ER-2 high-altitude research aircraft shows smoke plumes. From this vantage point at roughly 65,000 feet, the Thomas Fire was seen as it burned on Dec. 5.

Our satellites can even gather data and imagery of these wildfires at night. The above image on the right shows a nighttime view of the fires on Dec. 5. 

For comparison, the image on the left shows what this region looked like the day before. Both images were taken by the Suomi NPP satellite, which saw the fires by using a special “day-night band” to detect light in a range of wavelengths from green to near-infrared and uses light intensification to detect dim signals.

Having the capability to see natural disasters, like these wildfires in southern California, provides first responders with valuable information that helps guide their action in the field.

For more wildfire updates, visit: nasa.gov/fires.

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What Cargo is Launching in October to the International Space Station?

On Monday, Oct. 17, Orbital ATK is scheduled to send new science experiments to the International Space Station. 

The Cygnus spacecraft will blast off from our Wallops Flight Facility in Virginia at 7:40 p.m. EDT carrying more than 5,100 pounds of science, supplies and equipment.

Let’s take a look at a few of these experiments:

Cool Flames

Low-temperature fires with no visible flames are known as cool flames. The Cool flames experiment examines these low-temperature combustion of droplets of a variety of fuels and additives in low gravity.

Why are we studying this? Data from this experiment could help scientists develop more efficient advanced engines and new fuels for use in space and on Earth.

Lighting Effects

Light plays a powerful role in our daily, or circadian, rhythms. Astronauts aboard the space station experience multiple cycles of light and dark every 24 hours, which, along with night shifts and the stresses of spaceflight, can affect their sleep quantity and quality.

The Lighting Effects investigation tests a new lighting system aboard the station designed to enhance crew health and keep their body clocks in proper sync with a more regular working and resting schedule.

Why are we studying this? Lighting manipulation has potential as a safe, non-pharmacological way to optimize sleep and circadian regulation on space missions. People on Earth, especially those who work night shifts, could also improve alertness and sleep by adjusting lighting for intensity and wavelength.

EveryWear

A user-friendly tablet app provides astronauts with a new and faster way to collect a wide variety of personal data. The EveryWear experiment tests use of this French-designed technology to record and transmit data on nutrition, sleep, exercise and medications. Astronauts use the app to complete questionnaires and keep medical and clinical logs. They wear a Smartshirt during exercise that records heart activity and body positions and transmits these data to the app. Finally, rather than manually recording everything that they eat, crew members scan barcodes on food packets to collect real-time nutritional data.

Why are we studying this? EveryWear has the potential for use in science experiments, biomedical support and technology demonstrations.

Fast Neturon Spectrometer

Outside the Earth’s magnetic field, astronauts are exposed to space radiation that can reduce immune response, increase cancer risk and interfere with electronics.

The Fast Neutron Spectrometer (FNS) experiment will help scientists understand high-energy neutrons, part of the radiation exposure experienced by crews during spaceflight, by studying a new technique to measure electrically neutral neutron particles.

Why are we studying this? This improved measurement will help protect crews on future exploration missions, like our journey to Mars.

Watch Launch

Ahead of launch, there will be various opportunities to learn more about the mission:

What’s on Board Science Briefing Saturday, Oct. 15 at 4 p.m. EDT Scientists and researchers will discuss some of the experiments being delivered to the station. Watch HERE.

Prelaunch News Briefing Saturday, Oct. 15 at 6 p.m. EDT Mission managers will provide an overview and status of launch operations. Watch HERE.

LAUNCH!!! Monday, Oct. 17 coverage begins at 6:45 p.m. EDT Watch live coverage and liftoff! Launch is scheduled for 7:40 p.m. EDT. Watch HERE.

Facebook Live Starting at 7:25 p.m. EDT you can stream live coverage of the launch on NASA’s Facebook page. Watch HERE.

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