New Model Helps Predict Earth-Sized Planets

look over yonder writes "A new computer model created by astronomers from the Smithsonian Center and Astrophysics and the University of Utah predicts that systems which harbour Earth-sized planets will have a fingerprint of a ring of dust orbiting the star. This model will make it much easier for astronomers to locate stars and predict the size of planets orbiting it by simply measuring how bright the star system is at infrared (IR) wavelengths of light. Stars with dusty disks are brighter in the IR than stars without disks. The more dust a star system holds, the brighter it is in the IR."

Comments

Finding life?

[Via_Patrino]

"predicts (...) systems which harbour Earth-sized planets"

I don't think that's not the only way of finding life or an enviroment friendly to humans. Earth-sized moons of big planets can have a more friendly enviroment than earth-sized planets.

Re:Absorption/re-emission?

[Tau Zero]

I'm curious as to how they distinguish between a "normal" dust cloud and one that's due to an Earth sized planet.

The article states "The size of the largest objects in the disk determines the dust production rate. The amount of dust peaks when 600-mile protoplanets have formed." The dust forms in roughly the same orbit as the planet, so presumably you could detect a protoplanet forming at an Earth-like distance by watching for dust at a temperature of ~250 K; if there was the amount of dust you'd expect from an 8000-mile planet (well down from the peak at the 600-mile planetoid size), you might well have something like the prototypical Earth in that orbit.

I'm not sure how useful this is going to be in locating habitable planets; getting to them long before the intense bombardment phase has stopped isn't going to make for good colonization prospects. On the other hand, as a way of calculating the prevalence of Earth-like planets this is a huge breakthrough.