High_Above_Down_Under_Series_Trailer
#NASA, #Space, #Astronomy, #SpaceExploration, and #ScienceFiction.
NASA___Fiery_Looping_Rain_on_the_Sun
"NASA's Fiery Looping Rain on the Sun" likely refers to a solar phenomenon known as solar prominences or solar loops. These are large, arching structures of plasma that erupt from the Sun's surface into the corona, the Sun's outermost layer. These loops are often referred to as "fiery" because they emit intense heat and energy. They can be observed during solar events like solar flares and coronal mass ejections, where magnetic energy stored in the Sun's atmosphere is released, causing these loops to form and create a mesmerizing display of looping rain-like patterns. #NASA #SolarProminences #SolarLoops #SunPhenomena #SolarFlares #CoronalMassEjections
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High_above_down_under
"High above down under" could be a phrase used to describe something that is located at a higher altitude or elevation in the region of Australia or Oceania. It might refer to mountains, cliffs, or other elevated geographical features in that area.#HighAboveDownUnder #AussieElevation #OceaniaViews #AustraliasPeaks #ElevatedLandscapes #MountainAdventures #DownUnderHorizons
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Nasa_evolution_off_the_moon.
NASA's understanding of the moon's evolution has evolved over time. Initially thought to be a solid, unchanging body, modern observations reveal a more dynamic history. The moon likely formed around 4.5 billion years ago from debris created by a collision between Earth and a Mars-sized object.
Over millions of years, intense volcanic activity shaped its surface, creating vast plains called maria. The moon's surface was also heavily bombarded by asteroids, leaving behind craters of various sizes. Gradually, volcanic activity ceased, and the moon's interior cooled, leading to the quiet, cratered landscape we see today.
NASA missions like Apollo and more recent spacecraft have helped scientists learn about the moon's composition, structure, and history. Ongoing research continues to refine our understanding of its evolution and its potential role in the broader understanding of the solar system's history.
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