One Stellar Watch - BitCoin Wealth 247 News Blog
SUBTOTAL :

Follow Us

One Stellar Watch
One Stellar Watch

One Stellar Watch

One Stellar Watch
Short Description:

Product Description

Lux Ultra - Stellar One

Women Heart Attack Patients Do Much Better When Treated By Female Doctors

Europa Is Whistling. Finding The Cause May Solve A Magnetic Mystery

One Stellar Watch,<br />            	<br />
Astronomers Watch a Dying Star Enjoy One Last Spark of Life

Astronomerswatched a dying star, dubbed HuBi 1, get a brief second lease on life. (

Credit: Nature Astronomy (2018). DOI: 10.1038/s41550-018-0551-8

Often when stars die, they go out with a bang in the form of a supernova, leaving a small, dim stellar corpse in the center of a gaseous nebula. But sometimes, these leftover stars can get a new spark of life.

Astronomers used a telescope in the Canary Islands to watch a dying star, dubbed HuBi 1, get a brief second wind. And as they observed, they noticed a strange side effect: a shockwave sent from the fading star struck the surrounding gas in a way that made it appear “inside out.”

, marks the first time astronomers have seen such behavior from a sun-sized star. And it hints at how our own star may perish.

One Stellar Watch,<br />            	<br />
When a star like our sun dies, it typically leaves behind a stable core of carbon and oxygen at the heart of a beautiful and gaseous nebula. But if there’s a thin layer of helium on top of that core, One Stellar Watch

One Stellar Watch,<br />            	<br />
“There are estimates that 10 to 15 percent of planetary nebulae undergo these events,” says Martin Guerrero of Instituto de Astrofísica de Andalucía in Spain, a lead researcher on the discovery team. “But the timescale it takes [for] material ejected at high speeds to disperse is short, maybe shorter than 200 years. Thus, One Stellar Watch

As the shockwave pushed away from HuBi 1, the surrounding nebulous gas was altered.

Normally, ultraviolet radiation from these stellar corpses strip nearby gas of its electrons (a process called ionization). But gas that’s farther away is largely spared from this electron strip down, remaining neutral.

However, if a shockwave ripples through the nebula, it dramatically heats and ionizes the gas. As the shockwave continues outward, the material in the post-shock regions quickly cools and recombines. This is what gave HuBi 1 its “inside out” appearance.

The observations provide us with a possible preview into our own sun’s final outcome. Guerrero estimates there’s a one in 10 chance that our own life-supporting star may experience its final breath of life as HuBi 1 did. Of course, by then the sun would have already swelled into a red giant, so our planets would likely have been wiped out. Hopefully by then humans would have boarded their spaceships and set up camp in a new solar system.

Editor’s Note: An earlier version of this article erroneously indicated that our sun would go supernova at the end of its life.

“Of course, by then the sun would have already swelled into a red giant and exploded in a supernova” Please do your homework before writing an article like this. Our sun will never go nova.

One Stellar Watch,<br />            	<br />

Sign up to get the latest science news delivered weekly right to your inbox!

One Stellar Watch,<br />            	<br />
Quitting Smoking Makes You Gain Weight. It's Still Healthier

Black Holes Bolster Case For Quantum Physics' Spooky Action

This Element's Weird Behavior Could Lead to Faster Electronics

2005 Hurricane Season in the North Atlantic Approached Theoretical Limit

0 Reviews:

Post Your Review