Experience Tumblr Like Never Before
Dreaming of going to space? – Astronaut Victor Glover has you covered.
In his first video from space, take a look at our home through the window of SpaceX’s Crew Dragon “Resilience” spacecraft. Victor arrived to the International Space Station alongside his fellow Crew-1 astronauts on Nov. 16, 2020.
Follow his Instagram account HERE to stay up-to-date on station life and for more behind-the-scenes content like this.
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When you went into space for the first time, what was it like? Were you nervous?
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Take a look around Mars. Here’s where I’m working right now.
Click the link to see all my latest pictures from the surface of Mars.
The sky may not be falling, but it can certainly seem that way during a meteor shower. Shooting stars, as meteors are sometimes called occur when rock and debris in space fall through the Earth's atmosphere, leaving a bright trail as they are heated to incandescence by friction with the air. Sometimes the number of meteors in the sky increases dramatically, becoming meteor showers. Some showers occur annually or at regular intervals as the Earth passes through the trail of dusty debris left by a comet. Here's a guide to the top meteor showers expected in 2017.
At its peak this shower will have about 40 meteors per hour. The parent comet is 2003 EH1, which was discovered in 2003. First quarter moon sets after midnight and meteors radiate from the constellation Bootes.
This shower will have up to 60 meteors per hour at its peak and is produced by dust particles left behind by comet Halley, which has been known and observed since ancient times. The shower runs annually from April 19 to May 28. The waxing gibbous moon will block out many of the fainter meteors this year. Meteors will radiate from the constellation Aquarius.
The annual Perseid shower will have up to 60 meteors per hour at its peak. It is produced by comet Swift-Tuttle. The Perseids are famous for producing a large number of bright meteors. The shower runs annually from July 17 to August 24. The waning gibbous moon will block out many of the fainter meteors this year, but the Perseids are so bright and numerous that it should still be a good show. Meteors will radiate from the constellation Perseus.
This is a minor shower that will produce only about 10 meteors per hour. It is produced by dust grains left behind by comet 21P Giacobini-Zinner, which was first discovered in 1900. The Draconids is an unusual shower in that the best viewing is in the early evening instead of early morning like most other showers. The shower runs annually from October 6-10 and peaks this year on the the night of the 7th. Unfortunately, the nearly full moon will block all but the brightest meteors this year. If you are extremely patient, you may be able to catch a few good ones. Meteors will radiate from the constellation Draco.
The Geminids may be the best shower, producing up to 120 meteors per hour at its peak. It is produced by debris left behind by an asteroid known as 3200 Phaethon, which was discovered in 1982. The shower runs annually from December 7-17. The waning crescent moon will be no match for the Geminids this year. The skies should still be dark enough for an excellent show. Meteors will radiate from the constellation Gemini, but can appear anywhere in the sky.
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Something happened 100 years ago that changed forever the way we fly. And then the way we explore space. And then how we study our home planet. That something was the establishment of what is now NASA Langley Research Center in Hampton, Virginia. Founded just three months after America's entry into World War I, Langley Memorial Aeronautical Laboratory was established as the nation's first civilian facility focused on aeronautical research. The goal was, simply, to "solve the fundamental problems of flight."
From the beginning, Langley engineers devised technologies for safer, higher, farther and faster air travel. Top-tier talent was hired. State-of-the-art wind tunnels and supporting infrastructure was built. Unique solutions were found.
Langley researchers developed the wing shapes still used today in airplane design. Better propellers, engine cowlings, all-metal airplanes, new kinds of rotorcraft and helicopters, faster-than-sound flight - these were among Langley's many groundbreaking aeronautical advances spanning its first decades.
By 1958, Langley's governing organization, the National Advisory Committee for Aeronautics, or NACA, would become NASA, and Langley's accomplishments would soar from air into space.
Robert R. "Bob" Gilruth (1913–2000)
Considered the father of the U.S. manned space program.
He helped organize the Manned Spacecraft Center – now the Johnson Space Center – in Houston, Texas.
Gilruth managed 25 crewed spaceflights, including Alan Shepard's first Mercury flight in May 1961, the first lunar landing by Apollo 11 in July 1969, the dramatic rescue of Apollo 13 in 1970, and the Apollo 15 mission in July 1971.
Christopher C. "Chris" Kraft, Jr. (1924-)
Created the concept and developed the organization, operational procedures and culture of NASA’s Mission Control.
Played a vital role in the success of the final Apollo missions, the first manned space station (Skylab), the first international space docking (Apollo-Soyuz Test Project), and the first space shuttle flights.
Maxime "Max" A. Faget (1921–2004)
Devised many of the design concepts incorporated into all U.S. manned spacecraft.
The author of papers and books that laid the engineering foundations for methods, procedures and approaches to spaceflight.
An expert in safe atmospheric reentry, he developed the capsule design and operational plan for Project Mercury, and made major contributions to the Apollo Program’s basic command module configuration.
Caldwell Johnson (1919–2013)
Worked for decades with Max Faget helping to design the earliest experimental spacecraft, addressing issues such as bodily restraint and mobility, personal hygiene, weight limits, and food and water supply.
A key member of NASA’s spacecraft design team, Johnson established the basic layout and physical contours of America’s space capsules.
William H. “Hewitt” Phillips (1918–2009)
Provided solutions to critical issues and problems associated with control of aircraft and spacecraft.
Under his leadership, NASA Langley developed piloted astronaut simulators, ensuring the success of the Gemini and Apollo missions. Phillips personally conceived and successfully advocated for the 240-foot-high Langley Lunar Landing Facility used for moon-landing training, and later contributed to space shuttle development, Orion spacecraft splashdown capabilities and commercial crew programs.
Katherine Johnson (1918-)
Was one of NASA Langley’s most notable “human computers,” calculating the trajectory analysis for Alan Shepard’s May 1961 mission, Freedom 7, America’s first human spaceflight.
She verified the orbital equations controlling the capsule trajectory of John Glenn’s Friendship 7 mission from blastoff to splashdown, calculations that would help to sync Project Apollo’s lunar lander with the moon-orbiting command and service module.
Johnson also worked on the space shuttle and the Earth Resources Satellite, and authored or coauthored 26 research reports.
Dorothy Vaughan (1910–2008)
Was both a respected mathematician and NASA's first African-American manager, head of NASA Langley’s segregated West Area Computing Unit from 1949 until 1958.
Once segregated facilities were abolished, she joined a racially and gender-integrated group on the frontier of electronic computing.
Vaughan became an expert FORTRAN programmer, and contributed to the Scout Launch Vehicle Program.
William E. Stoney Jr. (1925-)
Oversaw the development of early rockets, and was manager of a NASA Langley-based project that created the Scout solid-propellant rocket.
One of the most successful boosters in NASA history, Scout and its payloads led to critical advancements in atmospheric and space science.
Stoney became chief of advanced space vehicle concepts at NASA headquarters in Washington, headed the advanced spacecraft technology division at the Manned Spacecraft Center in Houston, and was engineering director of the Apollo Program Office.
Israel Taback (1920–2008)
Was chief engineer for NASA’s Lunar Orbiter program. Five Lunar Orbiters circled the moon, three taking photographs of potential Apollo landing sites and two mapping 99 percent of the lunar surface.
Taback later became deputy project manager for the Mars Viking project. Seven years to the day of the first moon landing, on July 20, 1976, Viking 1 became NASA’s first Martian lander, touching down without incident in western Chryse Planitia in the planet’s northern equatorial region.
John C Houbolt (1919–2014)
Forcefully advocated for the lunar-orbit-rendezvous concept that proved the vital link in the nation’s successful Apollo moon landing.
In 1963, after the lunar-orbit-rendezvous technique was adopted, Houbolt left NASA for the private sector as an aeronautics, astronautics and advanced-technology consultant.
He returned to Langley in 1976 to become its chief aeronautical scientist. During a decades-long career, Houbolt was the author of more than 120 technical publications.
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#TBT to 1989 when Voyager 2 spotted Uranus looking like a seemingly perfect robin’s egg. 💙 When our Voyager 2 spacecraft flew by it in this image, one pole was pointing directly at the Sun. This means that no matter how much it spins, one half is completely in the sun at all times, and the other half is in total darkness.. Far-flung, Uranus – an ice giant of our solar system – is as mysterious as it is distant. Soon after its launch in 2021, our James Webb Space Telescope will change that by unlocking secrets of its atmosphere. Image Credit: NASA/JPL-Caltech
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Currently, six humans are living and working on the International Space Station, which orbits 250 miles above our planet at 17,500mph. Below you will find a real journal entry, written in space, by NASA astronaut Scott Tingle.
To read more entires from this series, visit our Space Blogs on Tumblr.
This is my last entry into the Captain’s Log. Drew Feustel, Ricky Arnold and Oleg Artymyev are now in charge after an excellent change of command ceremony where Drew took command of the International Space Station (ISS). We, the crew of the Soyuz MS-07 spacecraft, will undock from the International Space Station on Sunday morning (3 June), reenter the earth’s atmosphere and land on the steppe of Kazakhstan. I will be reunited with my family 24 hours later in Houston, and then begin recovery for living on Earth….with gravity….ugh.
I would like to thank all of you for following along on this incredible adventure, an adventure that started for me many years ago, and a journey that you have supported each step of the way.
To our Lead Flight Director, Gary Horlacher (Houston) and our Lead Payload Operations Director Patricia Patterson (Huntsville) – what an amazing job. Endless hours, minimal sleep, and herding a cast of thousands to establish the priorities that would define success for our Expedition. Thank you for your service, and for your outstanding leadership.
To our incredibly talented team supporting from Mission Control at all of our centers – Houston, Huntsville, Tsukuba, Cologne, and Moscow – you are incredible professionals without which our human spaceflight program could not exist. Thank you for your dedication, service and professionalism.
My life has been driven by dreams and goals. One of my concerns has always been that following my heart to achieve my dreams would have a deep impact on my family and friends. In the Navy, we endured multiple extended deployments onboard aircraft carriers, constant training cycles in locations away from home, and long days and weekends of training and work when we finally had some time at home.
In the space program, operational requirements demand the same attention and focus. I have moved my family 12 times in 30 years to make myself available for opportunities to serve that I would have otherwise not been afforded. I have always asked myself – is this worth it? I always assumed “yes”, but could not say definitively in the midst of the journey. My journey has brought my family to several new communities where we needed to learn, adjust, adapt and thrive. We are good at it. My family knows what it is like to live on the East Coast, the West Coast, the desert, the Midwest and the South. My family does not consider varying locations or diverse cultures as barriers to their success, but as opportunities to grow and excel. My children are embarking on their own dreams now, with an energy and focus even greater than I had at their age. My family maintains relationships with lifelong friends all over the country, and now the world. My family believes that dreams are attainable, and that the journey towards their dreams is where the value is found.
I am very lucky that I have lifelong friends that understand what it was that took me away from my childhood home. I am very lucky to have a family that “gets it”. My wife, Raynette, is amazing at being patient, and at making things work amidst unimaginable chaos. I am very proud of my military family for enduring all that they have over the years. Throughout the sacrifice and endurance, they decided to thrive – typical of our country’s incredible military families. My son, Sean Tingle, wrote and produced the song “To Touch the Stars” in honor of our journey that reached another level of success during ISS Expeditions 54 and 55. After hearing this song, I can definitively say, “Yes, it was worth it”.
To my family, friends and colleagues - THANK YOU for a LIFETIME OF INSPIRATION!
Now, it’s time to get busy again - chop chop hubba bubba!
Find more ‘Captain’s Log’ entries HERE.
Follow NASA astronaut Scott Tingle on Instagram and Twitter.
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On Saturday, October 20, NASA will host the ninth annual International Observe the Moon Night. 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 nearest celestial neighbor.
There are a number of ways to celebrate. You can attend an event, host your own, or just look up! Here are 10 of our favorite ways to observe the Moon:
Image credit: NASA’s Scientific Visualization Studio/Ernie Wright
The simplest way to observe the Moon is simply to look up. The Moon is the brightest object in our night sky, the second brightest in our daytime sky and can be seen from all around the world — from the remote and dark Atacama Desert in Chile to the brightly lit streets of Tokyo. On October 20, the near side of the Moon, or the side facing Earth, will be about 80 percent illuminated, rising in the early evening.
See the Moon phase on October 20 or any other day of the year!
The Moon and Venus are great targets for binoculars. Image Credit: NASA/Bill Dunford
With some magnification help, you will be able to focus in on specific features on the Moon, like the Sea of Tranquility or the bright Copernicus Crater. Download our Moon maps for some guided observing on Saturday.
Image credit: NASA/GSFC/ASU
Our Lunar Reconnaissance Orbiter (LRO) has taken more than 20 million images of the Moon, mapping it in stunning detail. You can see featured, captioned images on LRO’s camera website, like the one of Montes Carpatus seen here. And, of course, you can take your own photos from Earth. Check out our tips on photographing the Moon!
Image credit: NASA/JPL-Caltech
Plan a lunar hike with Moontrek. Moontrek is an interactive Moon map made using NASA data from our lunar spacecraft. Fly anywhere you’d like on the Moon, calculate the distance or the elevation of a mountain to plan your lunar hike, or layer attributes of the lunar surface and temperature. If you have a virtual reality headset, you can experience Moontrek in 3D.
Image credit: NASA GSFC/Jacob Richardson
Observe the Moon through touch! If you have access to a 3D printer, you can peruse our library of 3D models and lunar landscapes. This model of the Apollo 11 landing site created by NASA scientist Jacob Richardson, is derived from LRO’s topographic data. Near the center, you can actually feel a tiny dot where astronauts Neil Armstrong and Buzz Aldrin left the Lunar Descent Module.
Image credit: LPI/Andy Shaner
Enjoy artwork of the Moon and create your own! For messy fun, lunar crater paintings demonstrate how the lunar surface changes due to consistent meteorite impacts.
Image credit: NASA’s Scientific Visualization Studio/Ernie Wright
There are many movies that feature our nearest neighbor, from A Voyage to the Moon by George Melies, to Apollo 13, to the newly released First Man. You can also spend your evening with our lunar playlist on YouTube or this video gallery, learning about the Moon’s role in eclipses, looking at the Moon phases from the far side, and seeing the latest science portrayed in super high resolution. You’ll impress all of your friends with your knowledge of supermoons.
Video credit: NASA’s Scientific Visualization Studio/Ernie Wright
Make a playlist of Moon songs. For inspiration, check out this list of lunar tunes. We also recommend LRO’s official music video, The Moon and More, featuring Javier Colon, season 1 winner of NBC’s “The Voice.” Or you can just watch this video featuring “Clair de Lune,” by French composer Claude Debussy, over and over.
Image credit: NASA/GSFC/MIT
Visible light is just one tool that we use to explore our universe. Our spacecraft contain many different types of instruments to analyze the Moon’s composition and environment. Review the Moon’s gravity field with data from the GRAIL spacecraft or decipher the maze of this slope map from the laser altimeter onboard LRO. This collection from LRO features images of the Moon’s temperature and topography. You can learn more about our different missions to explore the Moon here.
Image credit: NASA’s Scientific Visualization Studio/Ernie Wright
An important part of observing the Moon is to see how it changes over time. International Observe the Moon Night is the perfect time to start a Moon journal. See how the shape of the Moon changes over the course of a month, and keep track of where and what time it rises and sets. Observe the Moon all year long with these tools and techniques!
However you choose to celebrate International Observe the Moon Night, we want to hear about it! Register your participation and share your experiences on social media with #ObserveTheMoon or on our Facebook page. Happy observing!
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Will NASA send astronauts to the moon again or any other planet within the next ten years?
@nasaorion spacecraft will launch on the Space Launch system (the largest spacecraft every built, even bigger than the Saturn V rocket!). Both are under construction @nasa currently, and this is the spacecraft that will take us beyond the low earth orbit of the International Space Station, whether that be the Moon, Mars, or beyond. We will conduct test missions with astronauts on Orion in the early 2020s, and a first mission will take us 40,000 miles beyond the Moon!
A Soyuz spacecraft is seen as it lands with astronaut Shane Kimbrough of NASA and Russian Flight Engineers Sergey Ryzhikov and Andrey Borisenko near the town of Zhezkazgan, Kazakhstan on Monday, April 10. Kimbrough, Ryzhikov, and Borisenko are returning after 173 days in space onboard the International Space Station.
While living and working aboard the space station, the crew members contributed to hundreds of experiments in biology, biotechnology, physical science and Earth science aboard the world-class orbiting laboratory. For example, the Microgravity Expanded Stem Cells investigation had crew members observe cell growth and other characteristics in microgravity.
Results from this investigation could lead to the treatment of diseases and injury in space, and provide a way to improve stem cell production for medical therapies on Earth. Photo Credit: (NASA/Bill Ingalls)
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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.
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!
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.
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.
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!
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March 20 marks the spring equinox. It’s the first day of astronomical spring in the Northern Hemisphere, and one of two days a year when day and night are just about equal lengths across the globe.
Because Earth is tilted on its axis, there are only two days a year when the sun shines down exactly over the equator, and the day/night line – called the terminator – runs straight from north to south.
In the Northern Hemisphere, the March equinox marks the beginning of spring – meaning that our half of Earth is slowly tilting towards the sun, giving us longer days and more sunlight, and moving us out of winter and into spring and summer.
An equinox is the product of celestial geometry, and there’s another big celestial event coming up later this year: a total solar eclipse.
A solar eclipse happens when the moon blocks our view of the sun. This can only happen at a new moon, the period about once each month when the moon’s orbit positions it between the sun and Earth — but solar eclipses don’t happen every month.
The moon’s orbit around Earth is inclined, so, from Earth's view, on most months we see the moon passing above or below the sun. A solar eclipse happens only on those new moons where the alignment of all three bodies are in a perfectly straight line.
On Aug. 21, 2017, a total solar eclipse will be visible in the US along a narrow, 70-mile-wide path that runs from Oregon to South Carolina. Throughout the rest of North America – and even in parts of South America, Africa, Europe and Asia – the moon will partially obscure the sun.
Within the path of totality, the moon will completely cover the sun’s overwhelmingly bright face, revealing the relatively faint outer atmosphere, called the corona, for seconds or minutes, depending on location.
It’s essential to observe eye safety during an eclipse. Though it’s safe to look at the eclipse ONLY during the brief seconds of totality, you must use a proper solar filter or indirect viewing method when any part of the sun’s surface is exposed – whether during the partial phases of an eclipse, or just on a regular day.
Learn more about the August eclipse at eclipse2017.nasa.gov.
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Matter makes up all the stuff we can see in the universe, from pencils to people to planets. But there’s still a lot we don’t understand about it! For example: How does matter work when it’s about to become a black hole? We can’t learn anything about matter after it becomes a black hole, because it’s hidden behind the event horizon, the point of no return. So we turn to something we can study – the incredibly dense matter inside a neutron star, the leftover of an exploded massive star that wasn’t quite big enough to turn into a black hole.
Our Neutron star Interior Composition Explorer, or NICER, is an X-ray telescope perched on the International Space Station. NICER was designed to study and measure the sizes and masses of neutron stars to help us learn more about what might be going on in their mysterious cores.
When a star many times the mass of our Sun runs out of fuel, it collapses under its own weight and then bursts into a supernova. What’s left behind depends on the star’s initial mass. Heavier stars (around 25 times the Sun’s mass or more) leave behind black holes. Lighter ones (between about eight and 25 times the Sun’s mass) leave behind neutron stars.
Neutron stars pack more mass than the Sun into a sphere about as wide as New York City’s Manhattan Island is long. Just one teaspoon of neutron star matter would weigh as much as Mount Everest, the highest mountain on Earth!
These objects have a lot of cool physics going on. They can spin faster than blender blades, and they have powerful magnetic fields. In fact, neutron stars are the strongest magnets in the universe! The magnetic fields can rip particles off the star’s surface and then smack them down on another part of the star. The constant bombardment creates hot spots at the magnetic poles. When the star rotates, the hot spots swing in and out of our view like the beams of a lighthouse.
Neutron stars are so dense that they warp nearby space-time, like a bowling ball resting on a trampoline. The warping effect is so strong that it can redirect light from the star’s far side into our view. This has the odd effect of making the star look bigger than it really is!
NICER uses all the cool physics happening on and around neutron stars to learn more about what’s happening inside the star, where matter lingers on the threshold of becoming a black hole. (We should mention that NICER also studies black holes!)
Scientists think neutron stars are layered a bit like a golf ball. At the surface, there’s a really thin (just a couple centimeters high) atmosphere of hydrogen or helium. In the outer core, atoms have broken down into their building blocks – protons, neutrons, and electrons – and the immense pressure has squished most of the protons and electrons together to form a sea of mostly neutrons.
But what’s going on in the inner core? Physicists have lots of theories. In some traditional models, scientists suggested the stars were neutrons all the way down. Others proposed that neutrons break down into their own building blocks, called quarks. And then some suggest that those quarks could recombine to form new types of particles that aren’t neutrons!
NICER is helping us figure things out by measuring the sizes and masses of neutron stars. Scientists use those numbers to calculate the stars’ density, which tells us how squeezable matter is!
Let’s say you have what scientists think of as a typical neutron star, one weighing about 1.4 times the Sun’s mass. If you measure the size of the star, and it’s big, then that might mean it contains more whole neutrons. If instead it’s small, then that might mean the neutrons have broken down into quarks. The tinier pieces can be packed together more tightly.
NICER has now measured the sizes of two neutron stars, called PSR J0030+0451 and PSR J0740+6620, or J0030 and J0740 for short.
J0030 is about 1.4 times the Sun’s mass and 16 miles across. (It also taught us that neutron star hot spots might not always be where we thought.) J0740 is about 2.1 times the Sun’s mass and is also about 16 miles across. So J0740 has about 50% more mass than J0030 but is about the same size! Which tells us that the matter in neutron stars is less squeezable than some scientists predicted. (Remember, some physicists suggest that the added mass would crush all the neutrons and make a smaller star.) And J0740’s mass and size together challenge models where the star is neutrons all the way down.
So what’s in the heart of a neutron star? We’re still not sure. Scientists will have to use NICER’s observations to develop new models, perhaps where the cores of neutron stars contain a mix of both neutrons and weirder matter, like quarks. We’ll have to keep measuring neutron stars to learn more!
Keep up with other exciting announcements about our universe by following NASA Universe on Twitter and Facebook.
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What future missions are you looking forward to the most?
Take a moment, look outside your window. 🌷🌼
Today is the #FirstDayOfSpring in the Northern Hemisphere, also known as the vernal equinox.
#DYK Earth’s tilted axis causes the season? Throughout the year, different parts of Earth receive the Sun’s most direct rays. So, when the North Pole tilts toward the Sun, it’s summer in the Northern Hemisphere. And when the South Pole tilts toward the Sun, it’s winter in the Northern Hemisphere.
These images are of Zinnias. They are part of the flowering crop experiment that began aboard the International Space Station on Nov. 16, 2015, when NASA astronaut Kjell Lindgren activated the Veggie system and its rooting "pillows" containing zinnia seeds.
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On April 7, Jupiter--the king of planets--reaches opposition, when it shines brightest and appears largest.
Jupiter will be almost directly overhead at midnight.
This is also a great time to observe the planet’s Galilean moons--Io, Ganymeade, Europa and Callisto. They can be easily seen through binoculars.
With binoculars, you can even see the Great Red Spot as the storm transits the planet every ten hours.
Looking east on April 22, look to the skies for the Summer Triangle, consisting of Deneb, in Cygnus, the Swan; Altair in Aquila, the Eagle; and Vega, in Lyre(the Harp).
Get ready for the Lyrids, the year’s second major meteor shower, as it pierces the Summer Triangle in the early morning hours of April 22. Since the shower begins close to the new moon, expect excellent almost moonless viewing conditions.
You can catch up on solar system and all of our missions at www.nasa.gov
Watch the full “What’s Up for April 2017″ video:
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The Moon, Mars and Saturn form a pretty triangle in early April, the Lyrid Meteors are visible in late April, peaking high overhead on the 22nd.
You won't want to miss red Mars and golden Saturn in the south-southeast morning skies this month. Mars shines a little brighter than last month.
By the 7th, the Moon joins the pair. From a dark sky you may see some glow from the nearby Milky Way.
Midmonth, start looking for Lyrid meteors, which are active from April 14 through the 30th. They peak on the 22nd.
The Lyrids are one of the oldest known meteor showers and have been observed for 2,700 years. The first recorded sighting of a Lyrid meteor shower goes back to 687 BC by the Chinese. The pieces of space debris that interact with our atmosphere to create the Lyrids originate from comet C/1861 G1 Thatcher. Comet Thatcher was discovered on 5 April 1861 by A. E. Thatcher.
In the early morning sky, a patient observer will see up to more than a dozen meteors per hour in this medium-strength shower, with 18 meteors per hour calculated for the peak. U.S. observers should see good rates on the nights before and after this peak.
A bright first quarter moon plays havoc with sky conditions, marring most of the typically faint Lyrid meteors. But Lyra will be high overhead after the moon sets at midnight, so that's the best time to look for Lyrids.
Jupiter will also be visible in the night sky this month!
Through a telescope, Jupiter's clouds belts and zones are easy to see.
And watch the Great Red Spot transit--or cross--the visible (Earth-facing) disk of Jupiter every 8 hours.
Our Juno spacecraft continues to orbit this gas giant, too!
And Juno's JunoCam citizen science team is creating exciting images of Jupiter's features based on the latest spacecraft data.
Next month Jupiter is at opposition--when it rises at sunset, sets at sunrise, and offers great views for several months!
Watch the full What’s Up for April Video:
There are so many sights to see in the sky. To stay informed, subscribe to our What’s Up video series on Facebook. Make sure to follow us on Tumblr for your regular dose of space: http://nasa.tumblr.com.
In the vastness of the universe, the life-bringing beauty of our home planet shines bright. During this tumultuous year, our satellites captured some pockets of peace, while documenting data and striking visuals of unprecedented natural disasters. As 2020 comes to a close, we’re diving into some of the devastation, wonders, and anomalies this year had to offer.
NASA’s fleet of Earth-observing satellites and instruments on the International Space Station unravel the complexities of the blue marble from a cosmic vantage point. These robotic scientists orbit our globe constantly, monitoring and notating changes, providing crucial information to researchers here on the ground.
Take a glance at 2020 through the lens of NASA satellites:
Seen from space, the icy Ili River Delta contrasts sharply with the beige expansive deserts of southeastern Kazakhstan.
When the Operational Land Imager (OLI) on Landsat 8 acquired this natural-color image on March 7, 2020, the delta was just starting to shake off the chill of winter. While many of the delta’s lakes and ponds were still frozen, the ice on Lake Balkhash was breaking up, revealing swirls of sediment and the shallow, sandy bed of the western part of the lake.
The expansive delta and estuary is an oasis for life year round. Hundreds of plant and animal species call it home, including dozens that are threatened or endangered.
A record-setting and deadly fire season marred the beginning of the year in Australia. Residents of the southeastern part of the country told news media about daytime seeming to turn to night, as thick smoke filled the skies and intense fires drove people from their homes.
This natural-color image of Southeastern Australia was acquired on January 4, 2020, by the Moderate Resolution Imaging Spectroradiometer (MODIS) on NASA’s Aqua satellite. The smoke has a tan color, while clouds are bright white. It is likely that some of the white patches above the smoke are pyrocumulonimbus clouds—clouds created by the convection and heat rising from a fire.
A team of scientists from NASA’s Goddard Space Flight Center (GSFC) and Universities Space Research Association (USRA) detected signs of the shutdown of business and transportation around Hubei province in central China. As reported by the U.S. State Department, Chinese authorities suspended air, road, and rail travel in the area and placed restrictions on other activities in late January 2020 in response to the COVID-19 outbreak in the region.
A research team analyzed images of Earth at night to decipher patterns of energy use, transportation, migration, and other economic and social activities. Data for the images were acquired with the Visible Infrared Imaging Radiometer Suite (VIIRS) on the NOAA–NASA Suomi NPP satellite (launched in 2011) and processed by GSFC and USRA scientists. VIIRS has a low-light sensor—the day/night band—that measures light emissions and reflections. This capability has made it possible to distinguish the intensity, types, and sources of lights and to observe how they change.
Though a seemingly serene oasis from above, there is more to this scene than meets the eye. On July 3, 2020, the Operational Land Imager (OLI) on Landsat 8 captured this false-color image of the river near Rosario, a key port city in Argentina. The combination of shortwave infrared and visible light makes it easier to distinguish between land and water. A prolonged period of unusually warm weather and drought in southern Brazil, Paraguay, and northern Argentina dropped the Paraná River to its lowest water levels in decades. The parched river basin has hampered shipping and contributed to an increase in fire activity in the delta and floodplain.
The drought has affected the region since early 2020, and low water levels have grounded several ships, and many vessels have had to reduce their cargo in order to navigate the river. With Rosario serving as the distribution hub for much of Argentina’s soy and other farm exports, low water levels have caused hundreds of millions of dollars in losses for the grain sector, according to news reports.
Climate and fire scientists have long anticipated that fires in the U.S. West would grow larger, more intense, and more dangerous. But even the most experienced among them have been at a loss for words in describing the scope and intensity of the fires burning in West Coast states during September 2020.
Lightning initially triggered many of the fires, but it was unusual and extreme meteorological conditions that turned some of them into the worst conflagrations in the region in decades.
Throughout the outbreak, sensors like the Visible Infrared Imaging Radiometer Suite (VIIRS) and the Ozone Mapping and Profiler Suite (OMPS) on the NOAA-NASA Suomi NPP satellite collected daily images showing expansive, thick plumes of aerosol particles blowing throughout the U.S. West on a scale that satellites and scientists rarely see.
This image shows North America on September 9th, 2020, as a frontal boundary moved into the Great Basin and produced very high downslope winds along the mountains of Washington, Oregon, and California. The winds whipped up the fires, while a pyrocumulus cloud from the Bear fire in California injected smoke high into the atmosphere. The sum of these events was an extremely thick blanket of smoke along the West Coast.
Though the bright blues of island waters are appreciated by many from a sea-level view, their true beauty is revealed when photographed from space. The underwater masterpiece photographed above is composed of sand dunes off the coast of the Bahamas.
The Great Bahama Bank was dry land during past ice ages, but it slowly submerged as sea levels rose. Today, the bank is covered by water, though it can be as shallow as two meters (seven feet) deep in places. The wave-shaped ripples in the image are sand on the seafloor. The curves follow the slopes of the dunes, which were likely shaped by a fairly strong current near the sea bottom. Sand and seagrass are present in different quantities and depths, giving the image it’s striking range of blues and greens.
This image was captured on February 15th, 2020, by Landsat 8, whose predecessor, Landsat 7, was the first land-use satellite to take images over coastal waters and the open ocean. Today, many satellites and research programs map and monitor coral reef systems, and marine scientists have a consistent way to observe where the reefs are and how they are faring.
Along with the plentiful harvest of crops in North America, one of the gifts of Autumn is the gorgeous palette of colors created by the chemical transition and fall of leaves from deciduous trees.
The folded mountains of central Pennsylvania were past peak leaf-peeping season but still colorful when the Operational Land Imager (OLI) on the Landsat 8 satellite passed over on November 9, 2020. The natural-color image above shows the hilly region around State College, Pennsylvania overlaid on a digital elevation model to highlight the topography of the area.
The region of rolling hills and valleys is part of a geologic formation known as the Valley and Ridge Province that stretches from New York to Alabama. These prominent folds of rock were mostly raised up during several plate tectonic collisions and mountain-building episodes in the Ordovician Period and later in the creation of Pangea—when what is now North America was connected with Africa in a supercontinent. Those events created the long chain of the Appalachians, one of the oldest mountain ranges in the world.
Ominous and looming, a powerful storm hovered off the US coastline illuminated against the dark night hues.
The Visible Infrared Imaging Radiometer Suite (VIIRS) on NOAA-20 acquired this image of Hurricane Laura at 2:20 a.m. Central Daylight Time on August 26, 2020. Clouds are shown in infrared using brightness temperature data, which is useful for distinguishing cooler cloud structures from the warmer surface below. That data is overlaid on composite imagery of city lights from NASA’s Black Marble dataset.
Hurricane Laura was among the ten strongest hurricanes to ever make landfall in the United States. Forecasters had warned of a potentially devastating storm surge up to 20 feet along the coast, and the channel might have funneled that water far inland. It did not. The outcome was also a testament to strong forecasting and communication by the National Hurricane Center and local emergency management authorities in preparing the public for the hazards.
From above, the Konsen Plateau in eastern Hokkaido offers a remarkable sight: a massive grid that spreads across the rural landscape like a checkerboard, visible even under a blanket of snow. Photographed by the Operational Land Imager (OLI) on Landsat 8, this man-made design is not only aesthetically pleasing, it’s also an agricultural insulator.
The strips are forested windbreaks—180-meter (590-foot) wide rows of coniferous trees that help shelter grasslands and animals from Hokkaido’s sometimes harsh weather. In addition to blocking winds and blowing snow during frigid, foggy winters, they help prevent winds from scattering soil and manure during the warmer months in this major dairy farming region of Japan.
Formidable, rare, and awe-inspiring — the first and only total solar eclipse of 2020 occurred on December 14, with the path of totality stretching from the equatorial Pacific to the South Atlantic and passing through southern Argentina and Chile as shown in the lower half of the image above. The Advanced Baseline Imager (ABI) on Geostationary Operational Environmental Satellite 16 (GOES-16) captured these images of the Moon’s shadow crossing the face of Earth.
The “path of totality” (umbral path) for the eclipse was roughly 90 kilometers (60 miles) wide and passed across South America from Saavedra, Chile, to Salina del Eje, Argentina. While a total eclipse of the Sun occurs roughly every 18 months, seeing one from any particular location on Earth is rare. On average, a solar eclipse passes over the same parcel of land roughly every 375 years. The next total solar eclipse will occur on December 4, 2021 over Antarctica, and its next appearance over North America is projected for April 8, 2024.
For additional information and a look at more images like these visit NASA’s Earth Observatory.
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The International Space Station is a microgravity laboratory in which an international crew of six people live and work while traveling at a speed of five miles per second (or 17,500 miles per hour), orbiting Earth every 90 minutes.
That’s more than 2,643,342,240 miles traveled! Which is also like 10 round trips to Mars, OR nearly the distance to Neptune!
The space station has been in orbit for over 17 years, and during that time, over 1,922 research investigations have been performed. More than 1,200 scientific results publications have been produced as a result.
Important studies like the VEGGIE experiment, which is working to grow plants in microgravity, and the Twin’s Study, which is studying the impacts of microgravity on the human body, are helping us on our journey to Mars. Using this unique orbiting laboratory as a place to conduct research is helping us learn important things for future deep space missions.
There have even been 222 different people that have visited the space station. This includes the current crew that is working and living on orbit.
Did you know that the space station is the third brightest object in the sky? If you know when and where to look up, you can spot it on your own! Find out when and where to look up HERE.
On Snapchat? Watch today’s Live Story to discover more about the orbiting laboratory and get a tour of the station! You can also add ‘nasa’ on Snapchat to get a regular dose of space.
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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.
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.
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.
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.
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.
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.
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