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RAS PN06/05: RAVE-ing Success As Generations of Astronomers Survey the Stars

Last Updated on Sunday, 01 December 2013 20:40
Published on Friday, 10 February 2006 00:00
A Cambridge PhD student is following in his great-great-grandfather's footsteps by helping to measure the speeds of up to one million stars passing near the Sun. The first data release is being announced today (10 February).

"The speeds of stars reveal where they were born," said George Seabroke, a graduate student at the Institute of Astronomy in Cambridge. "We're trying to find out whether stars in our own Milky Way galaxy were actually made here or whether some of them existed in other galaxies, before becoming part of our Galaxy. Such a large survey wasn't possible in my great-great-grandfather's era."

Current galaxy formation theories predict that some of these other galaxies were cannibalised by the Milky Way a long time ago as it was growing, leaving their very old stars where we see them today. Uncovering these fossil remains will reveal the history of our Galaxy – a practice known as Galactic Archaeology.

In order to undertake a survey of this scope, astronomers are participating in the RAdial Velocity Experiment (RAVE). This ambitious spectroscopic survey is intended to measure, over the next few years, radial velocities and stellar atmosphere parameters (temperature, metallicity, surface gravity) of up to one million stars passing near the Sun.

For the last three years, RAVE has been using the unique capabilities of the ‘six degree field' (6dF) multi-object spectrograph on the 1.2-m UK Schmidt Telescope of the Anglo-Australian Observatory, sited at Siding Spring Observatory in New South Wales, Australia.

This instrument is capable of obtaining spectroscopic information for as many as 150 stars at once, over a full six degree diameter, equivalent to 12 full Moons lined up in row. This is more than one hundred times larger than typical spectrographs. The combination of area and number of simultaneous spectra allows this unprecedented survey to be feasible.

Today (10 February), the leader of RAVE, Professor Matthias Steinmetz of the Astrophysical Institute Potsdam (AIP) in Germany, announced the first data release from the experiment to the astronomical community at the Local Group Cosmology meeting in Aspen, Colorado, USA. The data release includes 25,000 stars from the first year of RAVE (over 80,000 stars have been observed to date).

"RAVE will run for several more years, and the full RAVE survey will provide a vast resource of stellar motions and chemical abundances, allowing us to answer fundamental questions of the formation and evolution of our Galaxy," said Professor Steinmetz.

George Michael Seabroke is part of the international team of astronomers working on RAVE. His great-great-grandfather, George Mitchell Seabroke, was an early pioneer in measuring the speeds of stars at the Temple Observatory, Rugby School, Warwickshire, in the 1880s.  His competitor at the time was Carl Hermann Vogel, who was the first to measure a star speed from a photograph in 1888. Vogel was the director of the institute that later on became the AIP in Germany. Now, Professor Matthias Steinmetz, the leader of RAVE, is the AIP director. The current Seabroke generation is now collaborating with the AIP via RAVE.

George Senior could only look at the light spectrum of one star at a time through the telescope eyepiece. RAVE's telescope looks at an area of sky more than 100 times greater than the full Moon. It has 100 optical fibres, each acting like an eyepiece that can be automatically pointed towards a star. This enables RAVE to simultaneously receive light from lots of stars so that it can survey the Southern Sky at a rate many times faster than the extremely patient Mr. Seabroke Senior!

NOTES FOR EDITORS

Radial velocity is the motion of a star along the line-of-sight between the telescope and the star. Starlight is split into its different colours making a rainbow-like spectrum.

RAVE looks for features at specific colours produced by calcium atoms in the star's atmosphere. Because scientists know where these colours should be, they can tell if they have moved or ‘shifted’ in the spectrum. Light is influenced by the Doppler effect in a similar way to sound. This Doppler shift in frequency (colour) tells us whether the star is moving towards or away from us and at what speed.

CONTACT:

George Seabroke
University of Cambridge
Mobile: +44 (0) 7941611053
E-mail: This email address is being protected from spambots. You need JavaScript enabled to view it.
FURTHER INFORMATION:

Official RAVE web site:
http://rave-survey.org

George Seabroke's web page:
http://www.ast.cam.ac.uk/~gs310

IMAGES:

http://www.ast.cam.ac.uk/~gs310/pressreleases.html

OR by contacting George Seabroke directly (see above).

UK INVOLVEMENT AND FUNDING:

George Seabroke's PhD is funded by the Particle Physics and Astronomy Research Council (PPARC), which partially funds RAVE. He is supervised by Gerry Gilmore and Wyn Evans. Vasily Belokurov, Genevieve Parmentier and Simon Vidrih make up the rest of the RAVE team in Cambridge. Other RAVErs at UK universities include James Binney (Oxford), Walter Dehnen (Leicester), Brad Gibson (University of Central Lancashire) and Mike Read (Edinburgh). Funding for RAVE is also provided by the national research councils of other team members' countries, as well as by private sources. Other RAVE-ing nations include the US, Australia (including expatriates Quentin Parker and Fred Watson), Canada, the Netherlands, Italy, France, Switzerland and Slovenia.