Nova Explosion

News Excerpt:

In September 2024, a once-in-a-lifetime nova explosion 3,000 light-years away from Earth is expected to light up our night sky.

What is a Nova Explosion?

  • Nova explosion occurs when a star, as it interacts with a nearby star, undergoes a massive thermonuclear explosion. 
  • This event happens repeatedly over time in some star systems.
  • This phenomenon involves a dramatic explosion as one star interacts with another nearby star, a recurring event during the long, slow death of stars in a binary system.

The Blaze Star

  • The star system known as T Coronae Borealis, or "Blaze Star" (T CrB), consists of two stars: a white dwarf and a red giant. 
  • The white dwarf, a dense remnant of a once larger star, is about the size of Earth but with the mass of the Sun.
  • Its neighbour, the red giant, is in its final stages of life and is being stripped of hydrogen by the gravitational pull of the white dwarf.
  • This process leads to a tremendous buildup of pressure and heat, triggering the nova explosion.

Recurrent Novas

  • T CrB experiences nova events roughly every 80 years, making it a "recurrent" nova.
  • Historical records suggest prior eruptions were observed as far back as December 1787 and October 1217 AD.

Nova vs. Supernova

  • A nova is not the same as a supernova. 
  • While a supernova is the final, destructive explosion of a star, a nova event does not destroy the white dwarf, allowing the process to repeat over time.

What Will the Nova Look Like?

  • To the naked eye, the nova will appear as a new star in the sky. 
  • High-powered telescopes will reveal more detail, showcasing the brightly coloured luminosity of the nova. 
  • The explosion will increase T CrB's brightness dramatically, making it visible to the naked eye for several days.

How to Find T CrB?

  • The T CrB system is located in the Northern Crown (Corona Borealis), a horseshoe-shaped curve of stars west of the Hercules constellation.
  • To locate the Northern Crown, find the two brightest stars in the Northern Hemisphere: Arcturus and Vega. 
    • Tracing a line between these stars will lead you to the Northern Crown, where T CrB lies.

Red Giant and Dwarf Star

  • A red giant is a late-stage star that has exhausted the hydrogen in its core, causing it to expand and cool, emitting a reddish light. 
  • A dwarf star is a small, dense star, often a white dwarf, which is the remnant of a star that has burned out its nuclear fuel, about the size of Earth but with a mass comparable to the Sun.

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