Initial Stage of Earth-Like Planet Formation Observed for First Time

 

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For more information contact:

William Herbst, Wesleyan University

860-685-3672(o)

wherbst@wesleyan.edu

 

(Middletown, Conn.) For the first time, astronomers have observed the initial phase in the formation of an earth-like planet.

 

The discovery, highlighted in the March 13th issue of Nature, was documented by a team of astronomers led by William Herbst, an astronomy professor at Wesleyan University in Middletown, Conn., and Catrina Hamilton, professor of physics and astronomy at Dickinson College.

 

What Herbst and other astronomers on his team observed was that a protoplanetary disk, or ring, around the binary star known as KH 15D, is composed of solid particles larger than what is usually observed in space.

 

ÒFor hundreds of years, scientists have been theorizing that Earth-like planets form when gas and dust around a star get compressed into these disks and the material begins to coalesce into planets. But until now we never had the ability to study this process in detail,Ó Herbst said. ÒThe unique geometry presented by KH 15D and the way the light was being reflected off the disk allowed us to get a good look at the structure of the disk. We were amazed at what we saw.Ó

 

The disk orbiting KH 15D is at least the size of JupiterÕs orbit and composed of sand-sized grains that have grown from microscopic-sized particles to form the larger grains. These grains are now approximately 1 mm in diameter, much larger than the tiny particles typically seen in space. This is also the characteristic size of "chondrules,Ó small glassy spherules that are found in the most primitive solar system, the so-called carbonaceous chondrite meteorites.

 

A Flash animation of what the team observed can be seen here:

http://www.wesleyan.edu/newsrel/kh15d_animation.html  

 

The observations of the disk were made over several years using some of the largest telescopes in the world, including the 10-meter telescope of the W.M. Keck Observatory in Hawaii. More modest telescopes, including the one at Wesleyan UniversityÕs Van Vleck observatory and the Maidanak Observatory in Uzbekistan, were also used in the study.

 

Located approximately 2400 light years from earth and also known within the astronomical community as the Òwinking star,Ó KH 15D was first documented in 1995 by Herbst and his then-graduate student Kristin Kearns. An ensuing Ph.D. thesis by Herbst student Catrina Hamilton, now on the faculty of Dickenson College, further solidified the importance of this star and brought it to the attention of the astronomical community. In 2004, two groups of astronomers on opposite coasts showed that KH 15DÕs winking was a result binary star with an orbiting period of 48.36 days within a large disk. The winking effect was generated as one of the stars alternately rose above and set below the disk.

 

What Herbst, Hamilton and the rest of the team observed recently is that the disk is slowly hiding the stars from view and putting them in a permanent state of faintness, though still visible by the reflection off the disk.

 

ÒBecause of how the light is being reflected there are opportunities to make observations about the chemical composition of these sand-like particles,Ó Herbst said. ÒThatÕs very exciting because it opens up so many doors for new type of research on this disk.Ó

 

Herbst is the Chair and Van Vleck Professor of Astronomy at Wesleyan University. The members of HerbstÕs team documenting the observations include Catrina Hamilton, who received her Ph.D. degree in Physics from Wesleyan University in 2003 with Herbst as her advisor and is now on the faculty of Dickinson College; Katherine LeDuc, who received her M.A. degree in astronomy at Wesleyan in May, 2007; Joshua N. Winn of M.I.T.; Christopher M. Johns-Krull of Rice University; Reinhard Mundt of the Max-Planck-Institute for Astronomy in Heidelberg, Germany; and Mansur Ibrahimov of the Ulugh Bek Astronomical Institute in Tashkent, Uzbekistan. Support for the work has come over the years from NASA's Origins of Solar Systems program and from the W. M. Keck Observatory Principal Investigator's Fund.

 

 

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