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Avatar Moon Could be Real

Posted by Science Oxford on January 14, 2010 | comments

Have you seen the blockbuster film Avatar? Well some astronomers have and they say habitable moons may soon become science fact!
Read on to find out more and go and watch the movie!

In the new block­bust­er film Av­a­tar, hu­mans vis­it the hab­it­a­ble—and in­hab­it­ed—al­ien moon Pan­do­ra. Life-bearing moons like Pan­do­ra or the Star Wars for­est moon of En­dor are a sta­ple of sci­ence fic­tion.

But hab­it­a­ble moons may soon be­come sci­ence fact, and could per­haps even ex­ist around the same star that il­lu­mi­nates the fic­tional Pan­do­ra, as­tro­no­mers say.

“If Pan­do­ra ex­isted, we po­ten­tially could de­tect it and study its at­mos­phere in the next decade,” said Li­sa Kal­te­neg­ger of the Har­vard-Smith­son­ian Cen­ter for As­t­ro­phys­ics in Cam­bridge, Mass.

A new pa­per by Kal­te­neg­ger ar­gues that NASA’s new James Webb Space Tel­e­scope, to be launched in 2014, will be able to study their at­mos­pheres and de­tect key gas­es like car­bon di­ox­ide, ox­y­gen, and wa­ter va­por.

So far, plan­et searches have spot­ted hun­dreds of Ju­pi­ter-sized ob­jects in a range of or­bits. Such gi­ant gas plan­ets, while eas­i­er to de­tect, could not serve as homes for life as we know it. How­ev­er, sci­en­tists have spec­u­lat­ed wheth­er a rocky moon or­bit­ing a gas gi­ant could be life-friendly, if that plan­et or­bited with­in the star’s hab­it­a­ble zone, the re­gion warm enough for liq­uid wa­ter to ex­ist.

“All of the gas gi­ant plan­ets in our so­lar sys­tem have rocky and icy moons,” said Kal­te­neg­ger. “That raises the pos­si­bil­ity that al­ien Ju­pi­ters will al­so have moons. Some of those may be Earth-sized and able to hold on­to an at­mos­phere.”

NASA’s space-based Kep­ler tel­e­scope looks for plan­ets that cross in front of their host stars, which cre­ates a mini-eclipse and dims the star by a small but de­tecta­ble amount. Such a trans­it lasts only hours and re­quires ex­act align­ment of star and plan­et along our line of sight.

Once they have found an al­ien Ju­pi­ter, as­tro­no­mers can look for or­bit­ing moons. A moon’s gra­vity would tug on the plan­et and ei­ther speed or slow its trans­it, de­pend­ing on wheth­er the moon leads or trails the plan­et. The re­sult­ing trans­it dura­t­ion varia­t­ions would in­di­cate the moon’s ex­istence.

Once a moon is found, the next ob­vi­ous ques­tion would be: Does it have an at­mos­phere? If it does, those gas­es will ab­sorb a frac­tion of the star’s light dur­ing the trans­it, leav­ing a ti­ny, tell­tale fin­ger­print to the at­mos­phere’s com­po­si­tion.

The sig­nal is strongest for large worlds with hot, puffy at­mos­pheres, but an Earth-sized moon could be stud­ied if con­di­tions are just right. For ex­am­ple, the separa­t­ion of moon and plan­et needs to be large enough that we could catch just the moon in trans­it, while its plan­et is off to one side of the star.

Kal­te­neg­ger cal­cu­lat­ed what con­di­tions are best for ex­am­in­ing the at­mos­pheres of al­ien moons. She found that Al­pha Cen­tau­ri A, the sys­tem fea­tured in Av­a­tar, would be an ex­cel­lent tar­get.

“Al­pha Cen­tau­ri A is a bright, near­by star very si­m­i­lar to our Sun, so it gives us a strong sig­nal,” Kalteneg­ger ex­plained. “You would only need a hand­ful of trans­its to find wa­ter, ox­y­gen, car­bon di­ox­ide, and meth­ane on an Earth-like moon such as Pan­do­ra.”

While Al­pha Cen­tau­ri A of­fers tan­ta­liz­ing pos­si­bil­i­ties, small, dim, red dwarf stars are bet­ter tar­gets in the hunt for hab­it­a­ble plan­ets or moons, she added. The hab­it­a­ble zone for a red dwarf is clos­er to the star, which in­creases the prob­a­bil­ity of a trans­it.

As­tro­no­mers have de­bat­ed wheth­er tid­al lock­ing could be a prob­lem for red dwarfs. A plan­et close enough to be in the hab­it­a­ble zone would al­so be close enough for the star’s gra­vity to slow it un­til one side al­ways faces the star. (The same pro­cess keeps one side of the Moon al­ways fac­ing Earth.) One side of the plan­et then would be baked in con­stant sun­light, while the oth­er side would freeze in con­stant dark­ness.

An moon in the hab­it­a­ble zone would­n’t face this di­lem­ma. The moon would be tid­ally locked to its plan­et, not to the star, and there­fore would have reg­u­lar day-night cy­cles just like Earth. Its at­mos­phere would mod­er­ate tem­per­a­tures, and plant life would have a source of en­er­gy moon-wide.

“Alien moons or­bit­ing gas gi­ant plan­ets may be more likely to be hab­it­a­ble than tid­ally locked Earth-sized plan­ets or super-Earths,” said Kal­te­neg­ger. “We should cer­tainly keep them in mind as we work to­ward the ul­ti­mate goal of find­ing al­ien life.”

Scott Fleming of the University of Florida has also argued that a single habitable-zone gas giant could serve as a “signpost” for perhaps several habitable moons.

Kalteneg­ger’s pa­per is posted on­line at the arXiv database of Cor­nell Un­ivers­ity in New York.

Image Credit: Da­vid A. Aguilar, CfA

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