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Home / Science / Hubble's Crystal Clear Egg Nebula View

Hubble's Crystal Clear Egg Nebula View

10 Feb

•

Summary

  • Hubble captures the clearest view of the Egg Nebula, 3,000 light-years away.
  • The nebula's name comes from its star hidden by gas and dust.
  • Concentric rings suggest successive bursts of gas ejected from the star.
Hubble's Crystal Clear Egg Nebula View

The Hubble Space Telescope has delivered its most detailed image to date of the Egg Nebula, a cosmic formation approximately 3,000 light-years away. This nebula is aptly named for its dense shroud of gas and dust surrounding a central star.

The newly released photograph showcases the intricate structure of the Egg Nebula, highlighting four distinct beams of starlight escaping from its central shell. These beams illuminate striking concentric rings of gas, arranged in a ripple-like pattern.

Astronomers interpret this pattern as evidence of the star periodically expelling material in successive bursts over thousands of years. Fast-moving outflows of hot molecular hydrogen are also visible on either side of the disc-like cloud, with orange hues indicating infrared light emission.

Discovered in 1975 within the constellation Cygnus, the Egg Nebula represents a rare preplanetary phase in stellar evolution. Such nebulae are difficult to observe due to their short duration and faintness. By comparing this latest Hubble image with previous observations, scientists aim to gain deeper insights into its formation and processes.

Disclaimer: This story has been auto-aggregated and auto-summarised by a computer program. This story has not been edited or created by the Feedzop team.
The Egg Nebula is a celestial object approximately 3,000 light-years away, named for its dense shell of gas and dust hiding a central star.
The image reveals four beams of starlight escaping the nebula's shell, illuminating concentric rings of gas that suggest periodic material ejections from the central star.
The Egg Nebula was discovered in 1975 and is rare because it represents a preplanetary phase in stellar evolution, which is short-lived and difficult to observe.

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