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Rare Nova to Explode in 2024

Rare Nova to Explode in 2024

March 14, 2024
This six-panel illustration of a tidal disruption event around a supermassive black hole shows the following: 1) A supermassive black hole is adrift inside a galaxy, its presence only detectable by gravitational lensing; 2) A wayward star gets swept up in the black hole's intense gravitational pull; 3) The star is stretched or "spaghettified" by gravitational tidal effects; 4) The star's remnants form a disk around the black hole; 5) There is a period of black hole accretion, pouring out radiation across the electromagnetic spectrum, from X-rays to radio wavelengths; and 6) The host galaxy, seen from afar, contains a bright flash of energy that is offset from the galaxy's nucleus, where an even more massive black hole dwells. Credit: NASA, ESA, STScI, Ralf Crawford (STScI)

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Image captured by Juno during its 66th perijove, then further processed with color enhancement by Gerald Eichstädt and Thomas Thomopoulos. NASA / JPL / SwRI / MSSS / Gerald Eichstädt / Thomas Thomopoulos CC BY 3.0

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Rare Nova to Explode in 2024

by nasaspacenews
March 14, 2024
in Uncategorized
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Rare Nova to Explode in 2024

Rare Nova to Explode in 2024

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Dazzling Nova to Grace Night Skies in 2024

Skywatchers, rejoice! A rare celestial phenomenon known as a nova outburst is expected to occur sometime between February and September 2024. This awe-inspiring event will be visible to the naked eye, offering a glimpse into the dynamic nature of stars.

A Once-in-a-Lifetime Spectacle

The star system responsible for this extraordinary display is called T Coronae Borealis (T CrB). Located roughly 3,000 light-years away, T CrB is a binary system consisting of a red giant star and a white dwarf locked in a celestial dance.

Fueling the Fire: The Binary Dance

The red giant, nearing the end of its stellar lifespan, has ballooned in size, shedding its outer layers. This stellar material is gradually siphoned by its companion, the white dwarf. As the white dwarf accumulates this hydrogen-rich fuel, a dramatic event unfolds.

A Stellar Explosion: The Nova Outburst

When a critical mass of hydrogen accumulates on the white dwarf’s surface, a thermonuclear explosion ignites. This sudden burst of energy releases tremendous amounts of light, temporarily transforming the binary system into a luminous beacon. This spectacular event is known as a nova outburst.

Catching a Glimpse of the “New Star”

The upcoming nova outburst is predicted to peak in brightness around the magnitude of +2, comparable to the North Star, Polaris. This means the outburst will be readily visible without any special equipment during the peak period, potentially lasting for several days.

A Celestial Treasure in Corona Borealis

The outburst will take place within the constellation Corona Borealis, also known as the Northern Crown. This small constellation resembles a semicircle of stars and can be found nestled between the constellations Boötes and Hercules.

A fleeting visitor: After reaching peak brightness, the nova will gradually fade over the course of a week, becoming too faint to be seen with the naked eye. This celestial spectacle is a rare event, occurring only about every 80 years for T CrB. The last recorded outburst for this system happened in 1946.

A Testament to Stellar Evolution

The occurrence of a nova outburst signifies a crucial stage in the evolution of the binary system. The expelled material from the red giant enriches the white dwarf, setting the stage for a future outburst once enough fuel accumulates again. This cycle of stellar cannibalism and thermonuclear ignition will continue, shaping the destiny of this fascinating binary system.

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Witnessing the Power of the Universe

The upcoming nova outburst presents a unique opportunity for skywatchers to witness the raw power of stellar processes. Observing this celestial event allows us to gain a deeper understanding of the dynamic nature of stars and the intricate dance they perform throughout their lifespans.

Tips for Observing the Nova Outburst:

NOVA Universe Revealed | NOVA | PBS
  • Look for the constellation Corona Borealis: Locate the semicircle of stars between Boötes and Hercules.
  • Time your observation: The outburst is expected between February and September 2024. Monitor astronomical news and resources for updates on the peak brightness period.
  • Find a dark location: Light pollution can hinder your ability to observe faint celestial objects.
  • Embrace the naked eye experience: The nova is predicted to be visible without any special equipment during peak brightness.
  • Enhance your view with binoculars: Binoculars can offer a magnified view of the nova, particularly after the initial peak.

This extraordinary celestial event is a reminder of the vast and dynamic nature of the universe. By taking the time to observe the night sky, we can witness firsthand the awe-inspiring power and beauty of stellar phenomena.

Tags: NASAspace explorationspace observation

FEATURED POST

This six-panel illustration of a tidal disruption event around a supermassive black hole shows the following: 1) A supermassive black hole is adrift inside a galaxy, its presence only detectable by gravitational lensing; 2) A wayward star gets swept up in the black hole's intense gravitational pull; 3) The star is stretched or "spaghettified" by gravitational tidal effects; 4) The star's remnants form a disk around the black hole; 5) There is a period of black hole accretion, pouring out radiation across the electromagnetic spectrum, from X-rays to radio wavelengths; and 6) The host galaxy, seen from afar, contains a bright flash of energy that is offset from the galaxy's nucleus, where an even more massive black hole dwells. Credit: NASA, ESA, STScI, Ralf Crawford (STScI)

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May 10, 2025
A storm is pictured in the Arabian Sea less than 700 miles off the coast of Oman as the International Space Station orbited 260 miles above. NASA / Jasmin Moghbeli

Storm Warning: JWST Detects Violent Weather on Nearby Substars

May 7, 2025
Image captured by Juno during its 66th perijove, then further processed with color enhancement by Gerald Eichstädt and Thomas Thomopoulos. NASA / JPL / SwRI / MSSS / Gerald Eichstädt / Thomas Thomopoulos CC BY 3.0

Juno Strikes Gold: Uncovering Jupiter’s Monster Storms and Io’s Super Volcano

May 5, 2025
This artist's illustration shows a protoplanetary disk swirling around a young star. New research showing how a young star can send some material back into the disk helps explain an observational discrepancy. Image Credit: NASA/JPL-Caltech/T. Pyle (SSC)

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This six-panel illustration of a tidal disruption event around a supermassive black hole shows the following: 1) A supermassive black hole is adrift inside a galaxy, its presence only detectable by gravitational lensing; 2) A wayward star gets swept up in the black hole's intense gravitational pull; 3) The star is stretched or "spaghettified" by gravitational tidal effects; 4) The star's remnants form a disk around the black hole; 5) There is a period of black hole accretion, pouring out radiation across the electromagnetic spectrum, from X-rays to radio wavelengths; and 6) The host galaxy, seen from afar, contains a bright flash of energy that is offset from the galaxy's nucleus, where an even more massive black hole dwells. Credit: NASA, ESA, STScI, Ralf Crawford (STScI)

Star Meets Doom: Hubble Reveals Wandering Black Hole’s Deadly Snack

May 10, 2025
A storm is pictured in the Arabian Sea less than 700 miles off the coast of Oman as the International Space Station orbited 260 miles above. NASA / Jasmin Moghbeli

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