enow.com Web Search

Search results

  1. Results from the WOW.Com Content Network
  2. Betelgeuse - Wikipedia

    en.wikipedia.org/wiki/Betelgeuse

    The time until Betelgeuse explodes depends on the predicted initial conditions and on the estimate of the time already spent as a red supergiant. The total lifetime from the start of the red supergiant phase to core collapse varies from about 300,000 years for a rotating 25 M ☉ star, 550,000 years for a rotating 20 M ☉ star, and up to a ...

  3. The red giant star Betelgeuse is closer than we thought ... - AOL

    www.aol.com/news/red-giant-star-betelgeuse...

    Betelgeuse is one of the best-known stars in the night sky, as well as the easiest to find. ... By studying movements (like sound waves) on the surface of the star suggest Betelgeuse is still ...

  4. An asteroid will temporarily eclipse one of the brightest ...

    www.aol.com/asteroid-block-one-brightest-stars...

    Scientists observing the occultation could get more detailed and accurate measurements of the asteroid’s size and insight into what’s happening with Betelgeuse, which suddenly dimmed in 2019 ...

  5. Betelgeuse mystery solved? New deep-space image stirs up ...

    www.aol.com/news/betelgeuse-mystery-solved-deep...

    One of the biggest and brightest stars in the night sky has left astronomers puzzled after it has faded dramatically over the last year. Some have speculated that this is a sign of an impending ...

  6. Hypernova - Wikipedia

    en.wikipedia.org/wiki/Hypernova

    Hypernovae are one of the mechanisms for producing long gamma ray bursts (GRBs), which range from 2 seconds to over a minute in duration. They have also been referred to as superluminous supernovae , though that classification also includes other types of extremely luminous stellar explosions that have different origins.

  7. Extinction (astronomy) - Wikipedia

    en.wikipedia.org/wiki/Extinction_(astronomy)

    One prominent feature in measured extinction curves of many objects within the Milky Way is a broad 'bump' at about 2175 Å, well into the ultraviolet region of the electromagnetic spectrum. This feature was first observed in the 1960s, [ 26 ] [ 27 ] but its origin is still not well understood.

  8. The most fascinating star in our sky inches closer to exploding

    www.aol.com/news/most-fascinating-star-sky...

    Humanity has marveled at the vivid star Betelgeuse for many millennia. Over two thousand years ago, this imperious red object in the constellation Orion caught the eye of the Roman poet Horace:But ...

  9. Breaking wave - Wikipedia

    en.wikipedia.org/wiki/Breaking_wave

    The short, sharp burst of wave energy means that the swash/backwash cycle completes before the arrival of the next wave, leading to a low value of Kemp's phase difference (< 0.5). Surging waves are typical of reflective beach states. On steeper beaches, the energy of the wave can be reflected by the bottom back into the ocean, causing standing ...