The Age-old Mystery Of Why Otherwise Healthy Dolphins, Whales And Porpoises Get Stranded Along Coasts

Follow NASA’s Artemis I Moon Mission: Live Tracker, Latest Images, and Videos

On Nov. 16, 2022, the Artemis I mission officially began with the launch of the Orion spacecraft atop the Space Launch System rocket. The rocket and spacecraft lifted off from historic Launch Complex 39B at NASA’s Kennedy Space Center in Florida.

Now, the Orion spacecraft is about halfway through its journey around the Moon. Although the spacecraft is uncrewed, the Artemis I mission prepares us for future missions with astronauts, starting with Artemis II.

Stay up-to-date with the mission with the latest full-resolution images, mission updates, on-demand and live video.

Imagery:

Find full-resolution images from the Orion spacecraft as they are released here.

Launch imagery can be found here. When Orion splashes down in the Pacific Ocean on Dec. 11, the images will be available here, as well!

Videos:

This playlist contains informational videos, as well as upcoming and past live events, about Artemis I.

You can watch a livestream of the Artemis I mission here. (Just a note: the livestream may cut off during moments when the Orion team needs higher bandwidth for activities.)

Keep yourself updated on the upcoming broadcasts of Artemis milestones with the NASA TV schedule.

Trackers:

Our Artemis I Tracker uses live telemetry data streamed directly from Mission Control Center in Houston to show Orion position, attitude, solar array positions, and thruster firings throughout the mission.

“Eyes on the Solar System” shows Orion's position along the Artemis I trajectory and in relation to other NASA spacecraft and objects in the solar system.

“DSN Now” shows which antenna on Earth’s Deep Space Network is communicating with Orion.

Updates:

Read up on where Orion is and what’s next in the Artemis I mission with the Mission Blog.

Thank you so much for following with us on this historic mission. Go Artemis!

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

Which Landsat Image Do You Love?

Feeling competitive? We’ve got a game for you to play in! Tournament Earth: The Landsat Games is happening right now, and as we get to the final entries, the competition is heating up.

You can help us pick the winner by voting for one of the remaining four Landsat images of our home planet! Our competition started with 32 images, divided into categories by what they show: land, water, ice & snow, and human impact.

So, what do you think? Which one of these images is going for gold?

Land

First up, we have an image of the Markha River and surrounding Central Siberian Plateau, acquired in 2020 by Landsat 8. The hypnotic undulations of striping across the landscape carried this image to victory over the rest of the Land images -- a particularly tough category, given that these images all come from Landsat.

Water

It’s not all land, though! The bright blues and greens of this false-color image of the Atchafalaya Delta in Louisiana helped carry it to victory in the Water category. The image, taken in 2020 by Landsat 8, shows a region that’s subject to erosion of land by wind and rising sea levels.

Ice & Snow

Brrr! Did it get cold in here? That’s the finalist from the Ice and Snow category, an image of sea ice around Russia’s New Siberian Islands. The image, collected by Landsat 8 in June 2016, shows sea ice during its annual seasonal breakup.

Human Impact

Humans have been shaping the planet around us for hundreds of years. Some changes, like rice fields in the Sacramento Valley, are visible from space. Landsat 8 collected this false-color image of flooded rice fields in December 2018.

So, now it’s up to you! Which image is your favorite? There can only be one winner of Tournament Earth: The Landsat Games. Get your vote in, and then get ready to watch as we launch the next Landsat satellite, Landsat 9, in September.

The Landsat mission is a partnership between us at NASA and the U.S. Geological Survey. Together, we’ve been using Landsat satellites to collect nearly 50 years of images of our home planet.

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

Here’s What Actually Happens Inside Our Lunar Lab

Water is a precious resource -- especially on the Moon! In the near future, robotic rovers may roam the Moon’s poles in search of hidden reservoirs of water beneath the lunar surface. But traversing the poles can be a perilous journey. Depending on the Sun’s position in the sky and the way that its light falls on the surface, hazards such as boulders and craters can be difficult, if not impossible, to see. 

Inside our Lunar Lab at Ames Research Center, researchers are using Hollywood light kits and a giant sandbox filled with 8 tons of artificial Moon dirt to simulate driving conditions at the poles. The research aims to provide rovers and their human supervisors with 3-D hazard maps of the Moon’s terrain, helping them to avoid potential obstacles that lie ahead. 

Here’s how it works:

STEP 1: GENERATE A MOON MAP

Researchers begin with a map of the Moon’s terrain that’s randomly generated by a computer. Each scene is based on observations made from lunar orbit. The map indicates the number, location and size of features like rocks and craters that should be placed inside the 12x12-foot testbed.

STEP 2: BUILD A MOONSCAPE

Using the map as a guide, researchers build the terrain by hand with everyday tools. The terrain is then dusted with a top layer of artificial Moon dirt to eliminate shovel and brush marks.

STEP 3: CAPTURE IMAGES

Lights are positioned at different locations around the testbed. One by one, the lights are switched on and off while a camera captures images of the terrain. Notice how the appearance of the terrain changes depending on the source of illumination.

STEP 4: CREATE A 3-D MODEL

Using a computer algorithm, a 3-D hazard detection model of the terrain is generated from the images. The model provides important information about the size of an obstacle, its height and where it’s located.

STEP 5: GO EXPLORING

With this technique, researchers can teach a rover to recognize the effect of different lighting conditions on the Moon’s poles. The tool could come in handy for future lunar rover missions like Resource Prospector, which will use a drill to search for subsurface water and other compounds on the Moon.

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

Solar System: Things to Know This Week

From images to virtual reality and interactive simulations, NASA offers plenty of ways to explore our solar system -- and beyond -- in 3-D.

1. Step One: Get the Glasses

Many of the images and interactive features require special glasses with red and blue lenses.

Make regular 3-D glasses: http://go.nasa.gov/2lwQOoP

Make fancy Mars rover 3-D glasses: http://go.nasa.gov/2lwEmWe

2. Breaking News (Virtual Reality Edition)

Big news from 40 light-years away (235 trillion miles). Our Spitzer Space Telescope revealed the first known system of seven Earth-size planets around a single star. Three of these planets are firmly located in the habitable zone, all of them have the potential for water on their surfaces.

No glasses required.

Get to know one of those planets, TRAPPIST-1d in virtual reality: http://go.nasa.gov/2ldaGKY

Try the virtual reality panorama (especially great for a phone or tablet): 

http://go.nasa.gov/2ld5jvt

This image was created by combining two images from STEREO B (Feb. 24, 2008) taken about 12 hours apart, during which the sun's rotation provides sufficient perspective to create a nice 3-D effect.

3. Free-Range 3-D Exploration

Our Eyes on the Solar System app allows free exploration of Earth, our Solar System and thousands of worlds discovered orbiting distant stars. And, you also can explore it all in 3-D!

Under visual controls just check 3-D, pop on your glasses and explore.

Download Eyes on the Solar System: http://eyes.nasa.gov/

4. Your Star in 3-D

The STEREO (Solar TErrestrial RElations Observatory) mission studied the sun in 3-D with twin satellites.

Explore the Stereo 3D gallery: http://go.nasa.gov/2ldrzFv

5. National Parks in 3-D

The Earth-orbiting Terra satellite’s Multiangle Imaging SpectroRadiometer (MISR) instrument provides 3-D views while orbiting Earth, including some great shots of our National Parks.

Go to the parks: http://go.nasa.gov/2bk5XHP

6. Get in the Pilot's Seat

Take a look inside the cockpit of our high altitude ER-2 aircraft as it descends for landing at Kaneohe Bay, Hawaii. This month, scientists used used the aircraft to collect data on coral reef health and volcanic emissions and eruptions. Flying at 65,000 feet, above 95 percent of Earth's atmosphere, the ER-2 has a unique ability to replicate the data a future satellite could collect. Data from this mission will help in developing a planned NASA satellite mission to study natural hazards and ecosystems called Hyperspectral Infrared Imager, or HyspIRI.

Explore the 360 video: youtu.be/Zwkr-nsbaus

Read more: http://go.nasa.gov/2m8RJ0f

7. Moon Views

The Lunar Reconnaissance Orbiter creates 3-D images from orbit by taking an image of the moon from one angle on one orbit and a different angle on a separate orbit.

See the results: http://go.nasa.gov/2lvooeZ

This stereo scene looking back at where Curiosity crossed a dune at "Dingo Gap" combines several exposures taken by the Navigation Camera (Navcam) high on the rover's mast.

8. Martian 3D

Our Mars fleet of rovers and orbiters captures the Red Planet from all angles - often in 3-D.

Suit up and start exploring: http://go.nasa.gov/2lddjN4

9. Saturn in 3-D

The Cassini spacecraft’s mission to Saturn is well-known for its stunning images of the planet and its complex system of rings and moons. Now you can see some of them in 3-D.

See Saturn: http://go.nasa.gov/2mCQhiZ

10. Want More? Do It Yourself!

Put a new dimension to your vacation photos. Our Mars team created this handy how-to guide to making your own eye-popping 3-D images.

Get started: http://go.nasa.gov/2lddc46

BONUS: Printer-Friendly

Why stop with images? The Ames Research Center hosts a vast collection of 3-D printable models ranging from the moon craters to spacecraft.

Start printing: http://go.nasa.gov/2ldsMg1

Discover more lists of 10 things to know about our solar system HERE.

Follow us on Tumblr for your regular dose of space: http://nasa.tumblr.com

This photo contains both flight (flat in the foreground) and qualification assembly (upright in the background) versions of the Solar Array Sun Shield for NASA’s Nancy Grace Roman Space Telescope. These panels will both shade the mission’s instruments and power the observatory.

Double Vision: Why Do Spacecraft Have Twin Parts?

Seeing double? You’re looking at our Nancy Grace Roman Space Telescope’s Solar Array Sun Shield laying flat in pieces in the foreground, and its test version connected and standing upright in the back. The Sun shield will do exactly what it sounds like –– shade the observatory –– and also collect sunlight for energy to power Roman.

These solar panels are twins, just like several of Roman’s other major components. Only one set will actually fly in space as part of the Roman spacecraft…so why do we need two?

Sometimes engineers do major tests to simulate launch and space conditions on a spare. That way, they don’t risk damaging the one that will go on the observatory. It also saves time because the team can do all the testing on the spare while building up the flight version. In the Sun shield’s case, that means fitting the flight version with solar cells and eventually getting the panels integrated onto the spacecraft.

Our Nancy Grace Roman Space Telescope's primary structure (also called the spacecraft bus) moves into the big clean room at our Goddard Space Flight Center (top). While engineers integrate other components onto the spacecraft bus in the clean room, the engineering test unit (also called the structural verification unit) undergoes testing in the centrifuge at Goddard. The centrifuge spins space hardware to ensure it will hold up against the forces of launch.

Engineers at our Goddard Space Flight Center recently tested the Solar Array Sun Shield qualification assembly in a thermal vacuum chamber, which simulates the hot and cold temperatures and low-pressure environment that the panels will experience in space. And since the panels will be stowed for launch, the team practiced deploying them in space-like conditions. They passed all the tests with flying colors!

The qualification panels will soon pass the testing baton to the flight version. After the flight Solar Array Sun Shield is installed on the Roman spacecraft, the whole spacecraft will go through lots of testing to ensure it will hold up during launch and perform as expected in space.

For more information about the Roman Space Telescope, visit: www.nasa.gov/roman. You can also virtually tour an interactive version of the telescope here.

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

Falling Into Jupiter

Twenty-five years ago, an object roughly the size of an oven made space history when it plunged into the clouds of Jupiter, the largest planet in our solar system. On Dec. 7, 1995, the 750-pound Galileo probe became the first probe to enter the gas giant. Traveling at a blistering speed of 106,000 miles per hour, the probe’s protective heat shield experienced temperatures as hot as the Sun’s surface generated by friction during entry. As the probe parachuted through Jupiter’s dense atmosphere, its science instruments made measurements of the planet’s chemical and physical makeup. The probe collected data for nearly an hour before its signal was lost. Its data was transmitted to Earth via the Galileo spacecraft, an orbiter that carried the probe to Jupiter and stayed within contact during the encounter. Learn more about the mission.

The Galileo probe was launched to space aboard space shuttle Atlantis in 1989

The probe consisted of a descent module and a protective deceleration module

The probe traveled to Jupiter attached to the Galileo spacecraft

The probe was released from the spacecraft in July 1995

The probe entered Jupiter’s atmosphere five months later on Dec. 7, 1995

Parachutes were deployed to slow the probe’s descent

The probe collected science data for 58 minutes as it fell into the planet’s atmosphere

The Galileo probe was managed by NASA’s Ames Research Center in California’s Silicon Valley.

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

For scientists watching the Red Planet from our orbiters, the past month has been a windfall. "Global" dust storms, where a runaway series of storms create a dust cloud so large they envelop the planet, only appear every six to eight years (that’s 3-4 Mars years). Scientists still don't understand why or how exactly these storms form and evolve.

Read the full story HERE. 

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

When Dead Stars Collide!

Gravity has been making waves - literally.  Earlier this month, the Nobel Prize in Physics was awarded for the first direct detection of gravitational waves two years ago. But astronomers just announced another huge advance in the field of gravitational waves - for the first time, we’ve observed light and gravitational waves from the same source.

There was a pair of orbiting neutron stars in a galaxy (called NGC 4993). Neutron stars are the crushed leftover cores of massive stars (stars more than 8 times the mass of our sun) that long ago exploded as supernovas. There are many such pairs of binaries in this galaxy, and in all the galaxies we can see, but something special was about to happen to this particular pair.

Each time these neutron stars orbited, they would lose a teeny bit of gravitational energy to gravitational waves. Gravitational waves are disturbances in space-time - the very fabric of the universe - that travel at the speed of light. The waves are emitted by any mass that is changing speed or direction, like this pair of orbiting neutron stars. However, the gravitational waves are very faint unless the neutron stars are very close and orbiting around each other very fast.

As luck would have it, the teeny energy loss caused the two neutron stars to get a teeny bit closer to each other and orbit a teeny bit faster.  After hundreds of millions of years, all those teeny bits added up, and the neutron stars were *very* close. So close that … BOOM! … they collided. And we witnessed it on Earth on August 17, 2017.  

Credit: National Science Foundation/LIGO/Sonoma State University/A. Simonnet

A couple of very cool things happened in that collision - and we expect they happen in all such neutron star collisions. Just before the neutron stars collided, the gravitational waves were strong enough and at just the right frequency that the National Science Foundation (NSF)’s Laser Interferometer Gravitational-Wave Observatory (LIGO) and European Gravitational Observatory’s Virgo could detect them. Just after the collision, those waves quickly faded out because there are no longer two things orbiting around each other!

LIGO is a ground-based detector waiting for gravitational waves to pass through its facilities on Earth. When it is active, it can detect them from almost anywhere in space.

The other thing that happened was what we call a gamma-ray burst. When they get very close, the neutron stars break apart and create a spectacular, but short, explosion. For a couple of seconds, our Fermi Gamma-ray Telescope saw gamma-rays from that explosion. Fermi’s Gamma-ray Burst Monitor is one of our eyes on the sky, looking out for such bursts of gamma-rays that scientists want to catch as soon as they’re happening.

And those gamma-rays came just 1.7 seconds after the gravitational wave signal. The galaxy this occurred in is 130 million light-years away, so the light and gravitational waves were traveling for 130 million years before we detected them.

After that initial burst of gamma-rays, the debris from the explosion continued to glow, fading as it expanded outward. Our Swift, Hubble, Chandra and Spitzer telescopes, along with a number of ground-based observers, were poised to look at this afterglow from the explosion in ultraviolet, optical, X-ray and infrared light. Such coordination between satellites is something that we’ve been doing with our international partners for decades, so we catch events like this one as quickly as possible and in as many wavelengths as possible.

Astronomers have thought that neutron star mergers were the cause of one type of gamma-ray burst - a short gamma-ray burst, like the one they observed on August 17. It wasn’t until we could combine the data from our satellites with the information from LIGO/Virgo that we could confirm this directly.

This event begins a new chapter in astronomy. For centuries, light was the only way we could learn about our universe. Now, we’ve opened up a whole new window into the study of neutron stars and black holes. This means we can see things we could not detect before.

The first LIGO detection was of a pair of merging black holes. Mergers like that may be happening as often as once a month across the universe, but they do not produce much light because there’s little to nothing left around the black hole to emit light. In that case, gravitational waves were the only way to detect the merger.

Image Credit: LIGO/Caltech/MIT/Sonoma State (Aurore Simonnet)

The neutron star merger, though, has plenty of material to emit light. By combining different kinds of light with gravitational waves, we are learning how matter behaves in the most extreme environments. We are learning more about how the gravitational wave information fits with what we already know from light - and in the process we’re solving some long-standing mysteries!

Want to know more? Get more information HERE.

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4 people are living in an isolated habitat for 30 days. Why? Science!

This 30 day mission will help our researchers learn how isolation and close quarters affect individual and group behavior. This study at our Johnson Space Center prepares us for long duration space missions, like a trip to an asteroid or even to Mars.

The Human Research Exploration Analog (HERA) that the crew members will be living in is one compact, science-making house. But unlike in a normal house, these inhabitants won't go outside for 30 days. Their communication with the rest of planet Earth will also be very limited, and they won’t have any access to internet. So no checking social media kids!

The only people they will talk with regularly are mission control and each other.

The crew member selection process is based on a number of criteria, including the same criteria for astronaut selection.

What will they be doing?

Because this mission simulates a 715-day journey to a Near-Earth asteroid, the four crew members will complete activities similar to what would happen during an outbound transit, on location at the asteroid, and the return transit phases of a mission (just in a bit of an accelerated timeframe). This simulation means that even when communicating with mission control, there will be a delay on all communications ranging from 1 to 10 minutes each way. The crew will also perform virtual spacewalk missions once they reach their destination, where they will inspect the asteroid and collect samples from it. 

A few other details:

The crew follows a timeline that is similar to one used for the ISS crew.

They work 16 hours a day, Monday through Friday. This includes time for daily planning, conferences, meals and exercises.  

They will be growing and taking care of plants and brine shrimp, which they will analyze and document.

But beware! While we do all we can to avoid crises during missions, crews need to be able to respond in the event of an emergency. The HERA crew will conduct a couple of emergency scenario simulations, including one that will require them to maneuver through a debris field during the Earth-bound phase of the mission. 

Throughout the mission, researchers will gather information about cohabitation, teamwork, team cohesion, mood, performance and overall well-being. The crew members will be tracked by numerous devices that each capture different types of data.

Past HERA crew members wore a sensor that recorded heart rate, distance, motion and sound intensity. When crew members were working together, the sensor would also record their proximity as well, helping investigators learn about team cohesion.

Researchers also learned about how crew members react to stress by recording and analyzing verbal interactions and by analyzing “markers” in blood and saliva samples.

In total, this mission will include 19 individual investigations across key human research elements. From psychological to physiological experiments, the crew members will help prepare us for future missions.

UPDATE:

Mission success! After a simulated mission to an asteroid, the crew “splashed down” around 10:30 p.m. EST on Wednesday, Feb. 24 and exited the habitat for the first time in 30 days.

Want a full, 360 degree look at HERA? Check out and explore the inside of the habitat.

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

Ever want to ask a real life astronaut a question? Here's your chance!

Astronaut Jessica Meir will be taking your questions in an Answer Time session on Saturday, March 11 from 4:30-5:30pm ET/1:30-2:30pm PT here on NASA’s Tumblr. Make sure to ask your question now by visiting http://nasa.tumblr.com/ask!

Jessica Meir was selected to become an astronaut in 2013 and was part of NASA’s first astronaut class that was 50% female. She and her astronaut classmates are training to fly to space now and are involved in the future of our human exploration program. She’d like to be one of the first astronauts to set foot on Mars and pursue technological and scientific advances. 

She holds a Bachelor of Arts in Biology from Brown University, a Master of Science in Space Studies from the International Space University, and a Doctorate in Marine Biology from Scripps Institution of Oceanography (UCSD). In her research, the Caribou, Maine native studied the physiology of animals in extreme environments.  Follow Jessica on Twitter at @Astro_Jessica and follow NASA on Tumblr for your regular dose of space.