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  2. File:A Coronal Mass Ejection strikes the Earth.ogv - Wikipedia

    en.wikipedia.org/wiki/File:A_Coronal_Mass...

    The NASA website hosts a large number of images from the Soviet/Russian space agency, and other non-American space agencies. These are not necessarily in the public domain. Materials based on Hubble Space Telescope data may be copyrighted if they are not explicitly produced by the STScI. See also {{PD-Hubble}} and {{Cc-Hubble}}.

  3. Timeline of first images of Earth from space - Wikipedia

    en.wikipedia.org/wiki/Timeline_of_first_images...

    First image of Earth from another astronomical object (the Moon) and first picture of both Earth and the Moon from space. [32] [33] [34] [7] [19] December 11, 1966 ATS-1: First picture of both Earth and the Moon from the Earth's orbit. [35] First full-disk pictures of the Earth from a geostationary orbit. [35] [image needed] January 1967

  4. Ejecta - Wikipedia

    en.wikipedia.org/wiki/Ejecta

    In planetary geology, the term "ejecta" includes debris ejected during the formation of an impact crater. When an object massive enough hits another object with enough force, it creates a shockwave that spreads out from the impact. The object breaks and excavates into the ground and rock, at the same time spraying material known as impact ejecta.

  5. STEREO - Wikipedia

    en.wikipedia.org/wiki/STEREO

    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.

  6. Earth about to pull tiny space rock into its orbit as ... - AOL

    www.aol.com/earth-pull-tiny-space-rock-113254445...

    Earth tends to pull asteroids into partial or full orbits around it regularly before they are flung back out into space. For instance, one such space rock 2022 NX 1 was a short-lived “mini-moon ...

  7. Solar prominence - Wikipedia

    en.wikipedia.org/wiki/Solar_prominence

    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 .

  8. When We Left Earth: The NASA Missions - Wikipedia

    en.wikipedia.org/wiki/When_We_Left_Earth:_The...

    When We Left Earth: The NASA Missions (or NASA's Greatest Missions: When We Left Earth in the UK) is a 2008 Discovery Channel HD documentary miniseries consisting of six episodes documenting American human spaceflight from the first Mercury flights and the Gemini program, to the Apollo program and its Moon missions and landings, to the Space Shuttle missions and the construction of the ...

  9. Stellar mass loss - Wikipedia

    en.wikipedia.org/wiki/Stellar_mass_loss

    This causes their hold on their upper layers to weaken allowing small disturbances to blast large amounts of the outer layers into space. Events such as solar flares and coronal mass ejections are mere blips on the mass loss scale for low mass stars (like our sun). However, these same events cause catastrophic ejection of stellar material into ...

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