Finding Terrestrial Worlds in the Dust

by Paul Gilster on October 13, 2008

Computer simulations are showing us how to detect the signature of Earth-like planets — indeed, planets nearly as small as Mars — around other stars. That interesting news comes out of NASA’s Goddard Space Flight Center, where a supercomputer named Thunderbird has been put to work studying dusty disks around stars similar to the Sun.

Varying the size of the dust particles along with the mass and orbital distance of the planet, the team led by Christopher Stark (University of Maryland) ran 120 different simulations.

“It isn’t widely appreciated that planetary systems — including our own — contain lots of dust,” Stark says. “We’re going to put that dust to work for us.”

Indeed. Useful and observable things happen as dust responds to the forces acting upon it. For one thing, starlight can exert a drag that causes dust particles to move closer to the parent star. More to the point, particles spiraling inward can become involved in orbital resonances with planets in the system. A resonance like this is what happens when periodic gravitational influences go to work on orbiting objects. Particles that make three orbits around their star as a planet makes one, for example, will over time settle into identifiable structures, a complex dance that is played out with vast numbers of such particles.

Image: A planet twice Earth’s mass forms a ringed dust structure in this simulation. Enhanced dust density leads and trails the planet and causes periodic brightenings. Credit: NASA/Christopher Stark, GSFC.

Stark believes that this work will be useful as we study dust structures around exoplanets, particularly via future space platforms like the James Webb Space Telescope. Certainly the idea appears promising, as it means using dust that might otherwise complicate direct imaging attempts as a solution rather than a problem, capable of detecting planets down to a few times the mass of Mars. The paper is Stark and Kuchner, “The Detectability of Exo-Earths and Super-Earths Via Resonant Signatures in Exozodiacal Clouds,” Astrophysical Journal 686 (October 10, 2008), pp. 637–648 (abstract). Stark’s Exozodi Simulation Catalog is available online.

{ 1 comment }

ljk November 25, 2008 at 14:06

Super Earth Explorer: A Coronagraphic Off-Axis Space Telescope

Authors: J. Schneider, A. Boccaletti, D. Mawet, P. Baudoz, J. L. Beuzit, R. Doyon, M. Marley, D. Stam, G. Tinetti, W. Traub, J. Trauger, A. Aylward, J. Y. K. Cho, C. U. Keller, S. Udry, for the SEE-COAST Team

(Submitted on 24 Nov 2008 (v1), last revised 25 Nov 2008 (this version, v2))

Abstract: The Super-Earth Explorer is an Off-Axis Space Telescope (SEE-COAST) designed for high contrast imaging. Its scientific objective is to make the physico-chemical characterization of exoplanets possibly down to 2 Earth radii >. For that purpose it will analyze the spectral and polarimetric properties of the parent starlight reflected by the planets, in the wavelength range 400-1250 nm

Comments: Accepted in Experimental Astronomy

Subjects: Astrophysics (astro-ph)

Cite as: arXiv:0811.3908v2 [astro-ph]

Submission history

From: Schneider [view email]

[v1] Mon, 24 Nov 2008 16:17:19 GMT (719kb)

[v2] Tue, 25 Nov 2008 14:32:01 GMT (719kb)

http://arxiv.org/abs/0811.3908

Comments on this entry are closed.

{ 1 trackback }