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  1. nebula.tvNebula

    Nebula is the home of smart, thoughtful videos, podcasts, and classes from your favorite creators. A place for experimentation and exploration, with exclusive originals, bonus content, and no ads in sight.

  2. en.wikipedia.org › wiki › NebulaNebula - Wikipedia

    True color image of the Trifid Nebula, showing complex gas and plasma structure. A nebula (Latin for 'cloud, fog'; pl.: nebulae, nebulæ, or nebulas) is a distinct luminescent part of interstellar medium, which can consist of ionized, neutral, or molecular hydrogen and also cosmic dust.

  3. Several types of nebulae exist, and each individual nebula is a unique showcase of the phenomena and processes happening within. They often live side by side, with smaller nebulae populating larger clouds of gas and dust to form giant complexes of star birth and death.

  4. 6. Mai 2024 · A nebula is a giant cloud of dust and gas in space. Some nebulae (more than one nebula) come from the gas and dust thrown out by the explosion of a dying star, such as a supernova. Other nebulae are regions where new stars are beginning to form. For this reason, some nebulae are called "star nurseries."

  5. 18. Juli 2022 · Scott Dutfield. published 18 July 2022. Nebula are giant clouds of interstellar gas that play a key role in the life-cycle of stars. (Image credit: ESA/Hubble & NASA, Z. Levay) Jump to: Location...

  6. 29. Apr. 2024 · NASA’s James Webb Space Telescope has captured the sharpest infrared images to date of a zoomed-in portion of one of the most distinctive objects in our skies, the Horsehead Nebula. These observations show the top of the “horse’s mane” or edge of this iconic nebula in a whole new light, capturing the region’s complexity ...

  7. Nebula, any of the various tenuous clouds of gas and dust that occur in interstellar space. The term was formerly applied to any object outside the solar system that had a diffuse appearance rather than a pointlike image, as in the case of a star. This definition, adopted at a time when very.

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