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Images featured on the Astronomy Picture of the Day (APOD) web site may be copyrighted. The National Space Science Data Center (NSSDC) site has been known to host copyrighted content. Its photo gallery FAQ states that all of the images in the photo gallery are in the public domain "Unless otherwise noted."
Get closer to the in-space experience and see how the international partnership-powered human spaceflight is improving lives on Earth, while enabling humanity to explore the universe. More: https://go.nasa.gov/2zgPY5o Special thanks to the European Space Agency, the ISS National Lab, and astronauts Alexander Gerst, Serena Auñón-Chancellor ...
False color ultraviolet image. Some prominences are ejected from the Sun in what is known as a prominence eruption. These eruptions can have speeds ranging from 600 km/s to more than 1000 km/s. [1] At least 70% of prominence eruptions are associated with an ejection of coronal material into the solar wind known as a coronal mass ejection. [18]
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STEREO (Solar TErrestrial RElations Observatory) is a solar observation mission. [2] Two nearly identical spacecraft (STEREO-A, STEREO-B) were launched in 2006 into orbits around the Sun that cause them to respectively pull farther ahead of and fall gradually behind the Earth.
The system is composed of four commercial high definition video cameras which were built to record video of the Earth from multiple angles by having them mounted on the International Space Station. The cameras streamed live video of Earth to be viewed online and on NASA TV on the show Earth Views. Previously-recorded video now plays in a ...
Today's Wordle Answer for #1259 on Friday, November 29, 2024. Today's Wordle answer on Friday, November 29, 2024, is HIPPO. How'd you do? Next: Catch up on other Wordle answers from this week.
James Webb Space Telescope NIRCam and MIRI composite image of the Wolf–Rayet star WR 124 and its surrounding nebula. The star's mass loss history is encoded in the structure of the nebula. The lack of spherical symmetry in the nebular structure points to random, asymmetrical ejections. The clumps of dust and gas highlight the star's strong wind.
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