18 August 2014
A University of Central Lancashire (UCLan) professor is among an international team of astronomers who have produced new maps of the material between the stars in the Milky Way that should move scientists closer to cracking a stardust puzzle that has vexed them for nearly a century.
Professor Brad Gibson, from UCLan’s Jeremiah Horrocks Institute, and his fellow researchers say their work demonstrates a new way of uncovering the location and eventually the composition of the interstellar medium, which refers to the material found in the vast expanse between star systems within a galaxy.
This material, including dust and gas composed of atoms and molecules are left behind when a star dies. They also become the building blocks of new stars and planets. How and why stars form where they do, with the sizes and mass that they possess remains something of a mystery though.
“This work provides surprising clues about the interstellar medium out of which stars form.”
“This work provides surprising clues about the interstellar medium out of which stars form,” said Professor Gibson, one of the Builders of the experiment used in the new study.
Analysing rainbow-coloured bands of starlight that have passed through space gives astronomers important information about the makeup of the space materials that the light has encountered. As early as 1922 though, photographs yielded peculiar dark lines indicating ‘missing’ starlight and that something in the interstellar medium between Earth and the star was absorbing the light. These features were called diffuse interstellar bands (DIBs).
Since then, scientists have identified more than 400 of these DIBs, but the material that is causing these bands to appear and their precise location in the Milky Way have remained a mystery.
Researchers have speculated that the absorption of starlight that creates these dark bands points to the presence of unusually large complex molecules, but the proof has remained elusive. The nature of this puzzling material is important to astronomers because of the clues it could give about the physical conditions and chemistry of these regions between stars, critical components in theories of how stars and galaxies are formed.
The new study published in Science is the culmination of 10 years of data collection by 23 scientists from 10 countries, as part of the Radial Velocity Experiment (RAVE). Three dimensional maps of the distribution of the DIBs in the Milky Way were constructed using 500,000 stars pointed in many different directions and analysing the dark mysterious bands seen in each of these directions.
“To figure out what something is, you first have to figure out where it is and that’s what this paper does. Larger surveys will provide more details in the future. This paper has demonstrated how to do that.”
The resulting maps have shown the intriguing results that the complex molecules thought to be responsible for the DIBs are distributed differently to another known component of the interstellar medium, the solid particles known as dust, also traced by the RAVE survey.
Future studies can use the techniques outlined in the new paper to assemble other maps that should further solve the mysteries surrounding where DIBs are located, what exact materials cause them, and why they appear to be distributed differently to the Milky Way’s dust.
Co-author Rosemary Wyse said: “To figure out what something is, you first have to figure out where it is and that’s what this paper does. Larger surveys will provide more details in the future. This paper has demonstrated how to do that.”
The maps and an accompanying journal article appear in the 15 August issue of the journal Science.