Showing posts with label Doom. Show all posts
Showing posts with label Doom. Show all posts

Tuesday, June 3, 2014

Harsh space weather may doom potential life on red-dwarf planets

This artist's conception shows a hypothetical alien world orbiting a red dwarf star. 

Although it is in the star’s habitable zone, this planet faces an extreme space environment that is stripping its atmosphere and generating powerful aurorae. 

Since they are subjected to such harsh physical conditions, red-dwarf planets may not be habitable after all, so life in the universe might be even rarer than we thought.

Credit: Harvard-Smithsonian Center for Astrophysics (CfA)

Life in the universe might be even rarer than we thought. Recently, astronomers looking for potentially habitable worlds have targeted red dwarf stars because they are the most common type of star, comprising 80 percent of the stars in the universe.

But a new study shows that harsh space weather might strip the atmosphere of any rocky planet orbiting in a red dwarf's habitable zone.

"A red-dwarf planet faces an extreme space environment, in addition to other stresses like tidal locking," says Ofer Cohen of the Harvard-Smithsonian Center for Astrophysics (CfA).

Cohen is presenting their findings today in a press conference at a meeting of the American Astronomical Society.

Earth is protected from solar eruptions and space weather by its magnetic field. Just like the shields of the Starship Enterprise, Earth's magnetic field deflects incoming energy blasts.

We also are protected by distance since Earth orbits 93 million miles from the Sun.

Red dwarf stars are smaller and cooler than the Sun. To be in the star's habitable zone, where the temperature is warm enough for liquid water, a planet would have to be much closer to its star than the Earth is to the Sun. As a result, such a planet would be subjected to severe space weather.

Previous work has looked at the impact of stellar flares from a red dwarf on a nearby planet. In contrast, the new research examines the effect of the red dwarf's constantly blowing stellar wind.

The team used a computer model developed at the University of Michigan to represent three known red-dwarf planets circling a simulated, middle-aged red dwarf.

They found that even an Earth-like magnetic field could not necessarily protect a habitable-zone world from the star's continuous bombardment.

Although there were moments when the planet's magnetic shields held firm, it spent far more time with weak shields than strong shields.

"The space environment of close-in exoplanets is much more extreme than what the Earth faces," explains co-author Jeremy Drake (CfA).

"The ultimate consequence is that any planet potentially would have its atmosphere stripped over time."

The extreme space weather also would trigger spectacular aurorae, or Northern Lights. The aurora on a red-dwarf planet could be 100,000 times stronger than those on Earth, and extend from the poles halfway to the equator.

"If Earth were orbiting a red dwarf, then people in Boston would get to see the Northern Lights every night," adds Cohen.

"Oh the other hand, we'd also be in constant darkness because of tidal locking, and blasted by hurricane-force winds because of the dayside-nightside temperature contrast. I don't think even hardy New Englanders want to face that kind of weather."

Monday, October 17, 2011

Comet Elenin: Debris of 'Doomsday' comet to Flyby Earth

Amateur astronomer Michael Mattiazzo of Castlemaine, Australia caught these two images of comet Elenin on Aug. 19 (left) and Sept. 6, 2011.

The images show a rapid dimming in the comet, possibly hinting at its disintegration.
CREDIT: Michael Mattiazzo

The moment long feared by conspiracy theorists is nearly upon us: The "doomsday comet" Elenin will make its closest approach to Earth Sunday (Oct. 16). Or what's left of it will, anyway.

Russian amateur astronomer Leonid Elenin had the good fortune to discover a comet on Dec. 10, 2010, and it's turned out to be quite a skywatching curiosity.

Initially, comet Elenin received quite a bit of attention from astronomers because its orbit would take it quite close to Earth, within 22 million miles (35 million kilometers), on Oct. 16, 2011. It looked like it was going to put on a good show.

Even as recently as Aug. 19, the comet was brighter than predicted, as observed and photographed by amateur astronomers in Australia, notably Michael Mattiazzo.

Comet Elenin started breaking up in August after being blasted by a huge solar storm, and a close pass by the sun on Sept. 10 apparently finished it off, astronomers say.

So what will cruise within 22 million miles (35.4 million kilometers) of our planet Sunday is likely to be a stream of debris rather than a completely intact comet.

The debris of Comet Elenin won't return to Earth for 12,000 years, astronomers say.

Monday, October 5, 2009

Massive Black Holes Puching Universe to Doom

A composite Chandra image of Centaurus A showing the effects of an active supermassive black hole (Image: NASA/CXC/CfA/R.Kraft et al/NSF/VLA/Univ.Hertfor dshire/M.Hardcastle/ESO/VLT/ISAAC/M.Rejk uba et al.)

A composite Chandra image of Centaurus A showing the effects of an active supermassive black hole

THE mammoth black holes at the centre of most galaxies may be pushing the universe closer to its final fade-out. And it is all down to the raging disorder within those dark powerhouses.

Disorder is measured by a quantity called entropy, something which has been on the rise ever since the big bang. Chas Egan and Charles Lineweaver of the Australian National University in Canberra used the latest astrophysical data to calculate the total entropy of everything in the universe, from gas to gravitons. It turns out that supermassive black holes are by far the biggest contributors to the universe's entropy. Entropy reflects the number of possible arrangements of matter and energy in an object. The number of different configurations of matter a black hole could contain is staggering because its internal state is completely mysterious.

Egan and Lineweaver found that everything within the observable universe contains about 10104 units of entropy (joules per Kelvin), a factor of 10 to 1000 times higher than previous estimates that did not include some of the biggest known black holes (www.arxiv.org/abs/0909.3983, submitted to The Astrophysical Journal).

If entropy were ever to reach a maximum level, that would mean the heat death of the universe. In this scenario no energy can flow, because everything is the same temperature and so life and other processes become impossible. "Our results suggest we're a little further along that road than previously thought," Egan says.

But although black holes do boost the universe's total entropy, it is not clear whether they will hasten its heat death. Supermassive black holes don't contribute much to the flows of heat that even out temperature throughout the universe, says physicist Stephen Hsu at the University of Oregon in Eugene.

It's true that these black holes will slowly evaporate by releasing Hawking radiation, particles created near the boundary of the black hole. And this radiation could move the universe towards heat death.

Black holes may evaporate via Hawking radiation, tipping the universe towards its heat death

However, it will take some 10102 years for a supermassive black hole to evaporate. "The entropy inside those black holes is effectively locked up in there forever," Hsu says. So we may have reached a state approaching heat death long before, as stars burn out and their matter decays.


(Image: NASA/CXC/CfA/R.Kraft et al/NSF/VLA/Univ.Hertfor dshire/M.Hardcastle/ESO/VLT/ISAAC/M.Rejk uba et al.)