Space & Space

Moon Footage : Breath taking oin us on an unforgettable journey as we unveil captivating glimpses of our closest celestial neighbor. From the Apollo missions to cutting-edge lunar exploration, witness the beauty and intrigue of the lunar landscape like never before. #MoonFootage #LunarExploration #ApolloMissions #SpaceExploration #MoonLanding #SpaceDiscovery #NASA #Cosmos #Astronomy #Science #MoonSurface #Astrophotography #MoonWalk #SpaceTravel Moon, Moon Footage, Lunar Exploration, Apollo Missions, Space Exploration, Moon Landing, NASA, Cosmos, Astronomy, Science, Moon Surface, Astrophotography, Moon Walk, Space Travel, Unseen Footage, Exclusive Footage, Space Discovery, Astronauts, Lunar Landscape.

This abstract 8K video was inspired by the visual similarity of the cosmic nebula and the iris of the eye. The iris, with its intricate patterns and colors, shares a striking resemblance to the vibrant and colorful cosmic nebula. Just as the eye is a window to the soul, the nebula serves as a window to the vast universe beyond. Both the iris and the cosmic nebula contain a variety of hues and shades that blend and dance together to create a unique and mesmerizing visual display. The iris's delicate curves and lines mirror the sweeping curves and swirls of the nebula's gaseous clouds. The iris, with its distinctive central pupil, recalls the cosmic nebula's central star or black hole, around which the colorful gases and dust swirl. The cosmic nebula and the iris share a deep artistic connection, as both offer a glimpse into something beyond ourselves, whether it is the inner world of emotions and thoughts or the vast expanse of the cosmos.

December 27, 2023 After 1,000 Martian days of exploration, NASA’s Perseverance rover is studying rocks that show several eras in the history of a river delta billions of years old. Scientists are investigating this region of Mars, known as Jezero Crater, to see if they can find evidence of ancient life recorded in the rocks. Perseverance project scientist Ken Farley provides a guided tour of a richly detailed panorama of the rover’s location in November 2023, taken by the Mastcam-Z instrument. Composed of 993 individual images and 2.38 billion pixels, this 360-degree mosaic looks in all directions from a location the rover science team calls "Airey Hill." Portions of the rover itself are visible in the scene, appearing more distorted toward the edges as a result of the image processing. A color enhancement applied to the image increases contrast and accentuates color differences. By approximating what the scene would look like under Earth-like lighting conditions, the adjustment allows mission scientists to use their everyday experience to interpret the landscape. The view on Mars would be darker and more reddish.

Seasons change even on Mars and NASA's fleet of explorers are helping scientists learn more about the effects on the Red Planet. NASA's Perseverance and Curiosity rovers provide daily weather reports by measuring conditions such as humidity, temperature, and wind speed on the surface. Orbiters including Odyssey, Mars Atmosphere and Volatile EvolutioN (MAVEN), and the Mars Reconnaissance Orbiter (MRO) survey the scope and scale of storms from above. Changing weather conditions can be challenging for the spacecraft. The Ingenuity Mars Helicopter recently increased its rotor speed from 2,537 rpm to 2,700 rpm to fly in a thinner summer atmosphere. Meanwhile, NASA’s InSight lander, which is studying Mars’ interior, recently measured one of the biggest, longest-lasting marsquakes the mission has ever detected. For more information on NASA's Mars missions, visit mars.nasa.gov.

As of June 2020, NASA’s Solar Dynamics Observatory — SDO — has now been watching the Sun non-stop for over a full decade. From its orbit in space around the Earth, SDO has gathered 425 million high-resolution images of the Sun, amassing 20 million gigabytes of data over the past 10 years. This information has enabled countless new discoveries about the workings of our closest star and how it influences the solar system. With a triad of instruments, SDO captures an image of the Sun every 0.75 seconds. The Atmospheric Imaging Assembly (AIA) instrument alone captures images every 12 seconds at 10 different wavelengths of light. This 10-year time lapse showcases photos taken at a wavelength of 17.1 nanometers, which is an extreme ultraviolet wavelength that shows the Sun’s outermost atmospheric layer — the corona. Compiling one photo every hour, the movie condenses a decade of the Sun into 61 minutes. The video shows the rise and fall in activity that occurs as part of the Sun’s 11-year solar cycle and notable events, like transiting planets and eruptions. The custom music, titled “Solar Observer,” was composed by musician Lars Leonhard (https://www.lars-leonhard.de/). While SDO has kept an unblinking eye pointed towards the Sun, there have been a few moments it missed. The dark frames in the video are caused by Earth or the Moon eclipsing SDO as they pass between the spacecraft and the Sun. A longer blackout in 2016 was caused by a temporary issue with the AIA instrument that was successfully resolved after a week. The images where the Sun is off-center were observed when SDO was calibrating its instruments. SDO and other NASA missions will continue to watch our Sun in the years to come, providing further insights about our place in space and information to keep our astronauts and assets safe.

It’s always shining, always ablaze with light and energy that drive weather, biology and more. In addition to keeping life alive on Earth, the sun also sends out a constant flow of particles called the solar wind, and it occasionally erupts with giant clouds of solar material, called coronal mass ejections, or explosions of X-rays called solar flares. These events can rattle our space environment out to the very edges of our solar system. In space, NASA’s Solar Dynamics Observatory, or SDO, keeps an eye on our nearest star 24/7. SDO captures images of the sun in 10 different wavelengths, each of which helps highlight a different temperature of solar material. In this video, we experience SDO images of the sun in unprecedented detail. Presented in ultra-high definition, the video presents the dance of the ultra-hot material on our life-giving star in extraordinary detail, offering an intimate view of the grand forces of the solar system. Credit: NASA's Goddard Space Flight Center

2023 was Earth’s warmest year since 1880, and the last 10 consecutive years have been the warmest 10 on record. But why does NASA, a space agency, look at Earth’s temperature? And how do we even measure global temperature? Universal Music Production: “Busy Life Instrumental” “Spiritual Engineering Instrumental” “Promenade Instrumental” “Trusty Scalpel Instrumental” “Box of Tricks Instrumental” “Breaking Instrumental” and “Fast Progress Instrumental.” Credit: NASA's Goddard Space Flight Center

Amazing

When the Hubble Space Telescope launched, one of its main goals was to measure the rate at which our universe is expanding. That rate is called the “Hubble Constant” – named after the astronomer Edwin Hubble, who contributed to the discovery of the universe’s expansion. However, the expected value of the expansion rate is different depending on what equipment is being used to determine it. In this video, Nobel Laureate Dr. Adam Riess explains this phenomenon known as “Hubble Tension,” and how important this mystery is to our understanding of the universe.

Hubble's launch and deployment in April 1990 marked the most significant advance in astronomy since Galileo's telescope. Thanks to five servicing missions and more than 30 years of operation, our view of the universe and our place within it has never been the same. This documentary celebrates not only the scientific and technological achievements of this telescope, but also the human spirit that’s helped to keep it up and operational for all these years. Along with its views on YouTube, this documentary has gone on to receive over 400,000 combined views across the Hubble Space Telescope’s other social media platforms.

May 24, 2002 Even after the landers and airbags safely bounce to a complete stop on Mars, the challenges of getting to Mars continue. It will take each rover a minimum of nine days to emerge from its lander cocoon, stand up, orient itself, safely unlock its body from the lander, and roll down to the martian ground. In this last episode of the Challenges of Getting to Mars video series, the rover team describes the Impact to Egress phase of getting six wheels on the surface.

This animation features the Mars Exploration Rover's entry into the martian atmosphere and final soft landing using airbags.

August 02, 2017 The Curiosity rover has taught us a lot about the history of Mars and its potential to support life. Take a tour of its landing site, Gale Crater. TRANSCRIPT In 2012, NASA’s Curiosity Rover went to Mars to explore Gale Crater, a large impact basin with a massive, layered mountain in the middle. How did this strange landscape come to be? And what can its history teach us about the potential for life on Mars? After several years of exploration, here’s what we think could have happened. Around 3.7 billion years ago, a large meteor impact blasts out the initial crater, cracking the rock below and leaving a central peak as the surface rebounds. It’s a wetter time in Mars’ history. Groundwater seeps into the new crater, while rivers fed by rain or melting snow also flow in, forming a large lake – and carrying in gravel, sand and silt. This material keeps building up over millions of years. And as each layer cements into rock, it records a snapshot of the environment that shaped it. In time, the gradual drying of Mars shuts off the rivers. But sediment keeps piling up as sand and dust blow into the crater, deeply burying the deposits laid down in water. Meanwhile, groundwater remains deep below the dusty surface. At some point, winds that once carried sediment in begin scouring it back out. In areas closer to the crater rim, these winds dig all the way down into the ancient lake deposits. And as the heavy weight above is lifted, these layers crack, which helps groundwater flow through and alter them again before they dry out. By about 3 billion years ago, we’re left with the basic form we see today. It’s in this version of Gale Crater that Curiosity has helped piece together the story: Sediment patterns show a lot of water was present, continually, over many millions of years – both as persistent groundwater, and a long-standing lake (with occasional dry spells). Mineral and chemical readings show that water from both the lake and subsurface was friendly for potential microbes. Drill samples from the lakebed show key elements, organic molecules, nutrients and energy sources that microbes could have used. Water flowing through underground fractures could have supported life even in deeply buried rocks. And the composition of some layers makes them good for preserving potential signs of past life. Taken together, the evidence points to Gale Crater (and Mars in general) as a place where life — if it ever arose — might have survived for some time. With our primary mission fulfilled, we continue exploring: uncovering the history of Mars, and learning more about how and where future missions can search for the signatures that ancient life may have left behind.

This 11-minute animation depicts key events of NASA's Mars Science Laboratory mission, which will launch in late 2011 and land a rover, Curiosity, on Mars in August 2012.

n the past 60 years, NASA has advanced our understanding of our solar system and beyond. We continually ask “What’s out there?” as we advance humankind and send spacecraft to explore. Congress passed the National Aeronautics and Space Act, on July 16 and President Eisenhower signed it into law on July 29, 1958. NASA opened for business on Oct. 1, 1958. Our history tells a story of exploration, innovation and discoveries. The next 60 years, that story continues.

NASA studies the makeup and workings of the universe, from the smallest particles of matter and energy to its large-scale structure and evolution. Scientists look far back in space and time to learn the full cosmic history of stars and galaxies. They tease out details of the environments around black holes and observe the most powerful explosions since the big bang. NASA is discovering numerous planets beyond our solar system, decoding how planetary systems form, and learning how environments hospitable for life develop. “Cosmic Cycles: A Space Symphony" is a groundbreaking collaboration between acclaimed composer Henry Dehlinger, NASA, and the National Philharmonic, featuring a unique fusion of music and video in seven multimedia works on the Sun, Earth, Moon, Planets, and Cosmos. This transformative project takes the audience on a captivating voyage through the universe, showcasing the beauty and power of the marriage between music and science.

NASA’s Nancy Grace Roman Space Telescope will provide one of the deepest-ever views into the heart of our Milky Way galaxy. The mission will monitor hundreds of millions of stars in search of tell-tale flickers that betray the presence of planets, distant stars, small icy objects that haunt the outskirts of our solar system, isolated black holes, and more. Roman will likely set a new record for the farthest-known exoplanet, offering a glimpse of a different galactic neighborhood that could be home to worlds quite unlike the more than 5,500 that are currently known. Roman’s long-term sky monitoring, which will enable these results, represents a boon to what scientists call time-domain astronomy, which studies how the universe changes over time. Roman will join a growing, international fleet of observatories working together to capture these changes as they unfold. Roman’s Galactic Bulge Time-Domain Survey will focus on the Milky Way, using the telescope’s infrared vision to see through clouds of dust that can block our view of the crowded central region of our galaxy. When Roman launches, expected by May 2027, the mission will scour the center of the Milky Way for microlensing events, which occur when an object such as a star or planet comes into near-perfect alignment with an unrelated background star from our viewpoint. Because anything with mass warps the fabric of space-time, light from the distant star bends around the nearer object as it passes close by. The nearer object therefore acts as a natural magnifying glass, creating a temporary spike in the brightness of the background star’s light. That signal lets astronomers know there’s an intervening object, even if they can’t see it directly. In current plans, the survey will involve taking an image every 15 minutes around the clock for about two months. Astronomers will repeat the process six times over Roman’s five-year primary mission for a combined total of more than a year of observations. Astronomers expect the survey to reveal more than a thousand planets orbiting far from their host stars and in systems located farther from Earth than any previous mission has detected. That includes some that could lie within their host star’s habitable zone – the range of orbital distances where liquid water can exist on the surface – and worlds that weigh in at as little as a few times the mass of the Moon. A similar type of shadow play will reveal 100,000 transiting planets between Earth and the center of the galaxy. These worlds cross in front of their host star as they orbit and temporarily dim the light we receive from the star. This method will reveal planets orbiting much closer to their host stars than microlensing reveals, and likely some that lie in the habitable zone. All of these scientific discoveries and more will come from Roman’s Galactic Bulge Time-Domain Survey, which will account for less than a fourth of the observing time in Roman’s five-year primary mission. Its broad view of space will allow astronomers to conduct many of these studies in ways that have never been possible before, giving us a new view of an ever-changing universe.

Using NASA’s Neil Gehrels Swift Observatory, which launched in 2004, scientists have discovered a black hole in a distant galaxy repeatedly nibbling on a Sun-like star. The object heralds a new era of Swift science made possible by a novel method for analyzing data from the satellite’s X-ray Telescope (XRT). When a star strays too close to a monster black hole, gravitational forces create intense tides that break the star apart into a stream of gas. The leading edge swings around the black hole, and the trailing edge escapes the system. These destructive episodes are called tidal disruption events. Astronomers see them as flares of multiwavelength light created when the debris collides with a disk of material already orbiting the black hole. Recently, astronomers have been investigating variations on this phenomena, which they call partial or repeating tidal disruptions. During these events, every time an orbiting star passes close to a black hole, the star bulges outward and sheds material, but survives. The process repeats until the star looses too much gas and finally breaks apart. The characteristics of the individual star and black hole system determine what kind of emission scientists observe, creating a wide array of behaviors to categorize. On June 22, 2022, XRT captured Swift J0230 for the first time. It lit up in a galaxy around 500 million light-years away in the northern constellation Triangulum. Swift’s XRT has observed nine additional outbursts from the same location roughly every few weeks. Scientists propose that Swift J0230 is a repeating tidal disruption of a Sun-like star orbiting a black hole with over 200,000 times the Sun’s mass. They estimate the star loses around three Earth masses of material on each pass. This system provides a bridge between other types of suspected repeating disruptions and allowed scientists to model how interactions between different star types and black hole sizes affect what we observe. Swift J0230’s discovery was possible thanks to a new, automated search of XRT observations called the Swift X-ray Transient Detector. After the instrument observes a portion of the sky, the data is transmitted to the ground, and the program compares it to previous XRT snapshots of the same spot. If that portion of the X-ray sky has changed, scientists get an alert. In the case of Swift J0230, astronomers were able to rapidly coordinate additional observations of the region.

Original Mission Video as aired in July 1969 depicting the Apollo 11 astronauts conducting several tasks during extravehicular activity (EVA) operations on the surface of the moon. The EVA lasted approximately 2.5 hours with all scientific activities being completed satisfactorily. The Apollo 11 (EVA) began at 10:39:33 p.m. EDT on July 20, 1969 when Astronaut Neil Armstrong emerged from the spacecraft first. While descending, he released the Modularized Equipment Stowage Assembly on the Lunar Module's descent stage. A camera on this module provided live television coverage of man's first step on the Moon. On this, their one and only EVA, the astronauts had a great deal to do in a short time. During this first visit to the Moon, the astronauts remained within about 100 meters of the lunar module, collected about 47 pounds of samples, and deployed four experiments. After spending approximately 2 hours and 31 minutes on the surface, the astronauts ended the EVA at 1:11:13 a.m. EDT on July 21.

From high above the Earth, the International Space Station (ISS) provides a unique vantage point to view our home planet. Stunning time-lapse photography of cities, aurora, lightning and other sights are seen from orbit. Famed astronomer Galileo imagined these views from space and now through the technological marvel of the space station, we can see them for ourselves. For more time-lapse imagery

NASA’s Armstrong Flight Research Center in Edwards, California collaborated with University of Bergen, Norway to create the ALOFT project, Airborne Lightning Observatory for Fly’s eye simulator and Terrestrial gamma ray flashes. The team included from scientists and investigators from the University of Bergen, Norway, and pilots, engineers, and technicians from NASA who investigated lightning glows and terrestrial gamma ray flashes. Flying just above the height of thunderclouds over the Floridian and Caribbean coastlines, NASA’s ER-2 aircraft collect more accurate data that can advance the study of high-energy radiation emissions from thunderstorms.

This sonification turns the orbits of a new seven-planet system, discovered by NASA’s retired Kepler space telescope, into sound. It begins at the center of the system with the innermost orbit and builds toward the outermost, introducing each orbit with a new sound that plays once per rotation around the central Sun-like star. It then focuses on two specific orbits in resonance, which creates a beating sound with the inner rotating twice in the same period as the outer rotates three times. Next, only the three outer-most planets are singled out as an orbital resonance chain before blending all seven together again. This is the first planetary system in which each planet bathed in more radiant heat from their host star per area than any in our solar system.

Today, ESA’s Euclid space mission reveals its first full-colour images of the cosmos. Never before has a telescope been able to create such razor-sharp astronomical images across such a large patch of the sky, and looking so far into the distant Universe. These five images illustrate Euclid's full potential; they show that the telescope is ready to create the most extensive 3D map of the Universe yet, to uncover some of its hidden secrets.

NASA Johnson Style is a volunteer outreach video project created by the students of NASA's Johnson Space Center. It was created as an educational parody of Psy's Gangnam Style. The lyrics and scenes in the video have been re-imagined in order to inform the public about the amazing work going on at NASA and the Johnson Space Center.

This video features a series of time lapse sequences photographed by the Expedition 30 crew aboard the International Space Station. Set to the song "Walking in the Air," by Howard Blake, the video takes viewers around the world, through auroras, and over dazzling lightning displays.