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Auroras Found to Occur Beyond Our Solar System --Could Provide Clues to Alien Planets

 

 

             Jokusarlon1_2000

 

University of Leicester planetary scientists have found new evidence suggesting auroras – similar to Earth's Aurora Borealis - occur on bodies outside our solar system. Auroras occur on several planets within our solar system, and the brightest - on Jupiter – are 100 times brighter than those on Earth. However, no auroras have yet been observed beyond Neptune. Auroras occur when charged particles in an object's magnetosphere collide with atoms in its upper atmosphere, causing them to glow. However, before hitting the atmosphere, these particles also emit radio waves into space, which could provide us with key information about the length of the planet's day, the strength of its magnetic field, how the planet interacts with its parent star and even whether it has any moons.

A new study led by Dr Nichols, a Lecturer and Research Fellow in the University of Leicester's Department of Physics and Astronomy,  has shown that processes strikingly similar to those which power Jupiter's auroras could be responsible for radio emissions detected from a number of objects outside our solar system. In addition, the radio emissions are powerful enough to be detectable across interstellar distances – meaning that auroras could provide an effective way of observing new objects outside our solar system.

The study, Origin of Electron Cyclotron Maser Induced Radio Emissions at Ultracool Dwarfs: Magnetosphere-Ionosphere Coupling Currents, which recently appeared in the Astrophysical Journal, shows that this phenomenon is not limited to our solar system. It shows that the radio emissions from a number of ultracool dwarfs may be caused in a very similar, but significantly more powerful, way to Jupiter's auroras.

 "We have recently shown that beefed-up versions of the auroral processes on Jupiter are able to account for the radio emissions observed from certain "ultracool dwarfs" - bodies which comprise the very lowest mass stars - and "brown dwarfs" - 'failed stars' which lie in between planets and stars in terms of mass," Nichols said. "These results strongly suggest that auroras do occur on bodies outside our solar system, and the auroral radio emissions are powerful enough - one hundred thousand times brighter than Jupiter's - to be detectable across interstellar distances."

The paper, which also involved researchers at the Center for Space Physics, Boston University, USA, could have major implications for the detection of planets and objects outside our solar system which could not be discovered with other methods.

"I am part of a group who have recently been awarded time on the Low Frequency Array (LOFAR) - centred in the Netherlands but with stations across a number of countries in northern Europe including the UK - to try to observe auroras on exoplanets, so hopefully there will be some interesting results soon," Dr Nichols added.

 

           ISS006-E-21591_540

The Daily Galaxy via University of Leicester

Image credit: NASA/APOD

Comments

TARGET NUMBER ONE: Fomalhaut b! Not only would it prove the planet's existance beyond a shadow of a doubt, BUT; if evidence for exomoons also turns up in the data, it would strongly suggest that all the icy dust around the planet COULD hae come from a head-on collision between two of them!

This seems so basic...suprised me that it took till YR 2013 to figure it out!! Amazing!

the radio emissions are powerful enough to be detectable across interstellar distances – meaning that auroras could provide an effective way of observing new objects outside our solar system.

However, before hitting the atmosphere, these particles also emit radio waves into space, which could provide us with key information about the length of the planet's day, the strength of its magnetic field, how the planet interacts with its parent star and even whether it has any moons.

For the complete information about the all planets of the
solar system and about the moon must go on below url.
Click Here: About the moon

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