Detecting wandering worlds that host life

May 12, 2011 By Charles Q. Choi
Hubble Space Telescope’s close-up view of an electric-blue aurora on the giant planet Jupiter, eerily glowing one half billion miles away. Image credit: NASA and the Hubble Heritage Team (STScI/AURA) Credit: NASA/ESA, John Clarke (University of Michigan)

Some planets that roam the galaxy without a star to call home still may be able to host life. Finding such rogue planets is difficult, but new research suggests these wandering worlds could be detected by their atmospheric auroras.

Interstellar planets — those without stars to orbit — could serve as havens for . They are often thought to be nearly invisible, since they are much dimmer than stars and do not have any suns nearby to illuminate them. Now, however, research suggests these worlds might be detected by their auroras.

Interstellar planets might either be rogue planets that were originally born around a star and were later cast out by gravitational tugs of war, or sub-brown dwarfs that formed alone in interstellar space. Scientists have suggested that interstellar planets could support life under or even on their surfaces.

"It has been speculated that Earth-like rogue planets could have very thick atmosphere that keeps them relatively warm, or moons of giant rogue planets could experience tidal heating and have oceans beneath their icy surface," said planetary scientist Heikki Vanhamaki at the Finnish Meteorological Institute in Helsinki.

Planets reflect light from their host star, making them visible in the blackness of space. A new study says that planets can be detected from their auroras even if a planet has no reflected starlight, does not have a gravitational influence on a star, and does not pass in front of a star from our point of view. Credit: ESO

Planet hunters have used a variety of methods to detect the indirect effects extrasolar planets have on their host stars, because the planets themselves are too small and dim to be seen by our telescopes. For example, the slight gravitational wobble an orbiting planet induces in its parent star -- called the radial velocity method -- is one way to detect a far-off world. Another way to find a planet is when it passes directly in front of its star from our point of view, causing a momentary dimming of starlight.

Scientists recently suggested that alien worlds around distant stars could be detected by looking for radio waves given off by their auroras. Now Vanhamaki calculates the same technique might work for interstellar planets.

Auroras occur when charged particles interact with magnetic fields. There are two ways that detectable auroral radiation might emerge from interstellar planets — either from the worlds passing through interstellar plasma, or from moons of interstellar planets as they zip through fields of plasma trapped in that planet's magnetic field, as is the case with Jupiter and its moon Io, Vanhamaki said.

Vanhamaki found that auroral emissions linked with moons were roughly 100 times stronger than that from interstellar planets colliding with interstellar plasma.

"Motion of the moon through the planet's magnetic field creates an electric potential across the moon," Vanhamaki explained. The electrically charged moon then accelerates electrons in the plasma around the interstellar planet, which give off radiation when they move in the planet's .

Detecting an interstellar planet the size of Jupiter using radio telescopes that either exist now or in the near future "may be theoretically possible, but extremely unlikely — perhaps practically impossible — in the foreseeable future," Vanhamaki told Astrobiology Magazine.

Voyager 1 took photos of Jupiter and two of its satellites (Io, left, and Europa). The new study says that moons orbiting a gas giant planet greater than 8 Jupiter masses could help astronomers detect a rogue planet. Credit: NASA/JPL

Still, in very favorable conditions, he noted that an interstellar planet more strongly magnetized than Jupiter — for instance, far more massive and faster spinning — with a large nearby moon could be detected up to 185 light years away with the Square Kilometer Array radio telescope planned for either Australia or South Africa. There may be about 2,800 interstellar planets within that distance, he added.

"My results show that there is a real, although small, chance of detecting moon-induced emissions from giant rogue planets that weigh more than eight Jupiter masses," Vanhamaki said.

Vanhamaki detailed his findings online April 17 in the journal Planetary and Space Science.

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not rated yet May 13, 2011
It may also be possible to use microlensing to discover these. We may have to put up thousands of telescopes across the solar system, then we could track a lensing of a remote star due to a planet passing in front.

The shadow of a planet passing in front of a star may also be possible to detect, but it would be basicly a one off, without a repeat that you would get from an orbitting planet.

A third opportunity is to detect disturbance in the intergalactic wind caused by these objects. The wind could blow off nitrogen or other atoms from the planet and be detected like smoke in an exhaust plume from a smokestack.
5 / 5 (1) May 13, 2011
that is the technique we currently use now -- we have telescopes in space that look for stars getting dimmer and birghter then asserts if those intervals are regular and then checks for a planets at the cooresponding time.

the issue with that technique is that only fairly large plantes can be found in that fashion. That is why we have found so very many Jupiter type planets -- they are very large and tend to have these short orbits that are on the order of months because anything that has an orbit of a few years has yet to be found because we haven't been observing for that long with these newest telescopes.

When we come up with a way of tracking planets that are near to Earth, Venus and Mars in size then we will have something awesome -- because those planets will mostly likely be rocky balls like the Earth. From there it is all about detecting it's atmosphere.
5 / 5 (1) May 13, 2011
that is the technique we currently use now...for a planets at the cooresponding time.


the issue with that technique is that only fairly large plantes can be found in that fashion. That is why we have found so very many Jupiter type planets...found because we haven't been observing for that long with these newest telescopes.

This is not correct, we can find planets that are on the same order of magnitude in size as the Earth. The largest problem with looking for transiting planets is you only see the planets that are on a similar plane as the telescope. The "dip" in light that can be detected by Kepler is extremely sensitive.

When we come up with a way of tracking planets that are near to Earth...From there it is all about detecting it's atmosphere.

This is just going to be a matter of time, it is easily done with current technology. There are over 1,000 new extrasolar planet candidates. Some of them will probably be ~2-5 Earth masses.
not rated yet May 13, 2011
Also, I could be incorrect (it has been so long since I've read about what technologies Kepler uses), but I think that as well as Kepler's primary detection method (transiting planets) Kepler is equipped with instruments to detect spectroscopic radial velocity, "wobble", of stars. This would take out the problem of not detecting planets that do not transit their host star on the same plane as Kepler (other telescopes around the world use these two methods as well).
not rated yet May 13, 2011
"....we can find planets that are on the same order of magnitude in size as the Earth"

Indeed, COROT-7b appears to have a diameter ~1.6 times that of Earth:]http://en.wikiped...COROT-7b[/url]

At this time several ground based searches for transiting exoplanets are under way and more are planned.

Of note:

TrES: http://en.wikiped...t_Survey

SuperWASP: http://en.wikiped...uperWASP

HATNet: http://en.wikiped..._Project

XO: http://en.wikiped...elescope

And, of course, the space-based surveys of-



Kepler: http://en.wikiped..._Mission
not rated yet May 13, 2011
Ooops. Correct link for COROT-7b: http://en.wikiped...COROT-7b
not rated yet May 13, 2011
I suggest we start looking in the Omarion Nebula...

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