How We Are Going to the Moon - 4K
While Apollo placed the first steps on the Moon, Artemis opens the door for humanity to sustainably work and live on another world for the first time. Using the lunar surface as a proving ground for living on Mars, this next chapter in exploration will forever establish our presence in the stars. ✨ We are returning to the Moon – to stay – and this is how we are going! Actress Kelly Marie Tran of “Star Wars: The Rise of Skywalker” lent her voice to this project.
Top 17 Earth From Space Images of 2017 in 4K
The astronauts and cosmonauts on the International Space Station take pictures of Earth out their windows nearly every day, and over a year that adds up to thousands of photos. The people at the Earth Science and Remote Sensing Unit at NASA’s Johnson Space Center in Houston had the enviable job of going through this year’s crop to pick their top 17 photos of Earth for 2017—here’s what they chose! Gateway to Astronaut Photography of Earth: https://eol.jsc.nasa.gov/Collections/CEO-Top-Picks/2017 Download this video: https://archive.org/details/jsc2017m001088_Top-17-Earth-Images-of-2017
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133 Days on the Sun
video chronicles solar activity from Aug. 12 to Dec. 22, 2022, as captured by NASA’s Solar Dynamics Observatory (SDO). From its orbit in space around Earth, SDO has steadily imaged the Sun in 4K x 4K resolution for nearly 13 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 133-day 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 images taken 108 seconds apart, the movie condenses 133 days, or about four months, of solar observations into 59 minutes. The video shows bright active regions passing across the face of the Sun as it rotates. The Sun rotates approximately once every 27 days. The loops extending above the bright regions are magnetic fields that have trapped hot, glowing plasma. These bright regions are also the source of solar flares, which appear as bright flashes as magnetic fields snap together in a process called magnetic reconnection. While SDO has kept an unblinking eye pointed toward the Sun, there have been a few moments it missed. Some of the dark frames in the video are caused by Earth or the Moon eclipsing SDO as they pass between the spacecraft and the Sun. Other blackouts are caused by instrumentation being down or data errors. SDO transmits 1.4 terabytes of data to the ground every day. 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. The music is a continuous mix from Lars Leonhard’s “Geometric Shapes” album, courtesy of the artist. Credit: NASA's Goddard Space Flight Center Scott Wiessinger (PAO): Lead Producer Tom Bridgman (SVS): Lead Visualizer Scott Wiessinger (PAO): Editor This video can be freely shared and downloaded at https://svs.gsfc.nasa.gov/14263. While the video in its entirety can be shared without permission, the music and some individual imagery may have been obtained through permission and may not be excised or remixed in other products. Specific details on such imagery may be found here: https://svs.gsfc.nasa.gov/14263. For more information on NASA’s media guidelines, visit https://nasa.gov/multimedia/guidelines. Video Description: On the left side of the frame is the full circle of the Sun. It appears in a golden yellow color, but splotchy and with thin yellow wisps extending from the surface. Some areas are very bright and others almost black. The whole Sun rotates steadily, with one full rotation taking 12 minutes in this time lapse. There are usually only a few bright regions visible at a time and they shift and flash like small fires. From these regions there are wispy loops reaching up above the surface that rapidly change shape and size. On the right side of the frame are two white-outlined squares with enlargements of interesting regions of the Sun. If you liked this video, subscribe to the NASA Goddard YouTube channel: https://www.youtube.com/NASAGoddard Follow NASA’s Goddard Space Flight Center · Instagram http://www.instagram.com/nasagoddard · Twitter http://twitter.com/NASAGoddard · Twitter http://twitter.com/NASAGoddardPix · Facebook: http://www.facebook.com/NASAGoddard · Flickr http://www.flickr.com/photos/gsfc
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Bigelow expandable activity module
The Bigelow Expandable Activity Module (BEAM) is an inflatable habitat module designed for use in space exploration. Developed by Bigelow Aerospace, BEAM provides additional living and working space for astronauts aboard the International Space Station (ISS) or other space habitats. It is constructed using lightweight and compact materials that allow it to be transported to space efficiently, and it expands after deployment to provide a larger interior volume.
BEAM's innovative design allows it to be launched in a compact form and then inflated to its full size once attached to the ISS or other compatible platforms. This expandable technology offers several advantages, including reduced launch volume and mass, as well as potential improvements in radiation protection and micrometeoroid resistance compared to traditional rigid modules.
The module is equipped with sensors and instruments to monitor its performance, structural integrity, and its interaction with the space environment. It serves as a demonstration of expandable habitat technology and provides valuable data for future developments in space habitat design and construction.
BEAM was launched to the ISS in 2016 as a part of NASA's Commercial Resupply Services program and has been used for various experiments and evaluations to assess its viability for long-duration space missions.
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Launching of rocket
The rocket soared into the sky with a deafening roar, its powerful engines propelling it upwards against the Earth's gravity. Flames erupted from the base, creating a dazzling display of light and energy. As it gained altitude, the rocket left behind a trail of white smoke, marking its path through the atmosphere. The ground shook beneath the spectators' feet as they watched in awe, feeling the immense force being harnessed for this incredible journey. As it reached the edge of space, the rocket's engines cut off, and it entered a state of weightlessness, floating for a brief moment before beginning its planned mission among the stars.
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