heic0113 — Science Release
Gravitational lens helps Hubble and Keck discover galaxy building block
5 October 2001
A very small, faint galaxy - possibly one of the long sought `building blocks' of present-day galaxies - has been discovered by a collaboration between the Hubble Space Telescope and the Keck Telescopes at a tremendous distance of 13.4 billion light-years (based on the estimate of 14 billion years as the age of the Universe). The discovery was made possible by examining small areas of sky viewed through massive intervening clusters of galaxies. These act as a powerful gravitational lens, magnifying distant objects and allowing scientists to probe how galaxies assemble at very early times. This has profound implications for our understanding of how and when the first stars and galaxies formed in the Universe.
A unique systematic search for very distant objects - among the most distant known - using the NASA/ESA Hubble Space Telescope and the 10 metre Keck Telescopes has produced a remarkable result. Benefiting from the magnifying power of a foreground giant cluster of galaxies, a team of European and American scientists has discovered one of the smallest and most distant galaxies known to date by pushing both telescopes to their limits.
Abell 2218 is a rich galaxy cluster composed of thousands of galaxies and a mass equivalent to ten thousand galaxies interspersed throughout the cluster. The cluster is located relatively nearby - at a distance of 2 billion light-years (redshift 0.18). Redshift is the stretching of light waves as they travel across expanding space. The longer they travel, the more they are stretched, and the higher the measured redshift.
The gravitational field from this huge concentration of matter distorts and magnifies the light from distant galaxies according to Einstein's General Theory of Relativity. Gravitational lenses acting as `natural telescopes' give researchers a unique tool with which to learn more about the detailed physics of the first galaxies in the Universe.
The recently discovered `baby-galaxy' has a redshift of 5.58, corresponding to a distance of about 13.4 billion light-years. The galaxy's light has been magnified more than 30 times by Abell 2218 and split into two `images' by the uneven distribution of matter in the cluster.
The team, led by Richard Ellis from the California Institute of Technology (Caltech), USA, determined the amount of matter in the object to be astoundingly low for a galaxy - only a few million times the mass of our Sun, or about one hundred thousand times less than the amount of matter in our own Milky Way galaxy. The object is only around 500 light-years across, as compared to the 100 000 light-year diameter of the Milky Way.
Many galaxy clusters were investigated before such a clear-cut candidate for a very distant galaxy building block was found. Images taken from the Hubble archive and spectroscopy carried out by one of the ground-based Keck Telescopes revealed that this galaxy is one of the most distant found so far.
Ellis explains, 'Without the benefit of the powerful cosmic lens, the source would not even have been detected in the Hubble Deep Fields, historic deep exposures taken in 1995 and 1998.'
Jean-Paul Kneib from the Observatoire Midi-Pyrenees, France, an expert in gravitational lensing, describes the excitement of the team: 'It took two observing runs with the Keck Telescope before we had gathered enough light from this feeble object to determine its distance and thus confirm the discovery. When we realised what we had found, we literally jumped up and down.'
Research team member Konrad Kuijken from the Kapteyn Institute, the Netherlands, continues: 'We are very excited. We are looking at something very small and very young. A two million year old, one million solar mass, galaxy-like object consisting of young hot stars is the best fit to the observations. We believe it is one of the galaxy building blocks that join together and make up larger galaxies later in the history of the Universe. With this discovery, we may finally be witnessing the circumstances in which this first generation of stars was born.'
The first galaxies in the Universe hold invaluable clues that shed light on the period known as the cosmic `Dark Ages', a period that lasted possibly up to one billion years after the Big Bang and ended when the first generation of stars appeared.
ESA is planning two different observatories to probe these distant regions of space and time: the Herschel Space Observatory and the Next Generation Space Telescope (NGST - in collaboration with NASA and CSA, the Canadian Space Agency). ESA's project scientist for NGST, Peter Jakobsen (ESA-ESTEC, the Netherlands) states: 'The gravitational lensing provided by the foreground galaxy cluster is clearly extremely powerful - but a bit hard to point in other directions! This young, faint galaxy is precisely the kind of object we hope to study in more detail with NGST - all over the sky.' NGST is planned for launch around 2009.
The team's research paper will appear in the Astrophysical Journal Letters.
The W.M. Keck Observatory is operated as a scientific partnership among the California Institute of Technology, the University of California and NASA.
Members of the team of scientists include: Jean-Paul Kneib (Observatoire Midi-Pyrenees, France), Richard Ellis and Mike Santos (Caltech, USA) and Konrad Kuijken (Kapteyn Institute, the Netherlands).
This news release is issued jointly by ESA (Hubble European Space Agency Information Centre), NASA (STScI/Office of Public Outreach), Caltech/the W.M. Keck Observatory and NOVA (the Netherlands Research School for Astronomy).
Acknowledgements: The original images of Abell 2218 were obtained by A. Fruchter and the ERO team (STScI, ST-ECF) as part of the Hubble Servicing Mission 3A Early Release Observations.
LinksMore about gravitational lensing
Abell 2218 news release (2000)
Lars Lindberg Christensen
Hubble European Space Agency Information Centre, Garching, Germany
Phone: +49-89-3200-6306 (089 in Germany)
Cellular (24 hr): +49-173-38-72-621 (0173 in Germany)
Space Telescope Science Institute, Baltimore, USA
California Institute of Technology (Caltech), Pasadena, USA
W.M. Keck Observatory, Hawaii, USA
Contact details for the scientists:
Observatoire Midi-Pyrenees, Toulouse, France
Phone: +33-5-61-33-28-24 and +33-5-61-33-29-29 (05 in France)
Kapteyn Institute, Groningen, the Netherlands