Lensing cluster Abell 383
Annotated view of Abell 383
Gravitational lensing in action
Wide field view of Abell 383
Gravitational lensing in action
Pan across Abell 383
Richard’s team spotted the galaxy in recent observations from the NASA/ESA Hubble Space Telescope, verified it with observations from the NASA Spitzer Space Telescope and measured its distance using W. M. Keck Observatory in Hawaii.
The distant galaxy is visible through a cluster of galaxies called Abell 383, whose powerful gravity bends the rays of light almost like a magnifying glass . The chance alignment of the galaxy, the cluster and the Earth amplifies the light reaching us from this distant galaxy, allowing the astronomers to make detailed observations. Without this gravitational lens, the galaxy would have been too faint to be observed even with today’s largest telescopes.
After spotting the galaxy in Hubble and Spitzer images, the team carried out spectroscopic observations with the Keck-II telescope in Hawaii. Spectroscopy is the technique of breaking up light into its component colours. By analysing these spectra, the team was able to make detailed measurements of its redshift  and infer information about the properties of its component stars.
The galaxy’s redshift is 6.027, which means we see it as it was when the Universe was around 950 million years old . This does not make it the most remote galaxy ever detected — several have been confirmed at redshifts of more than 8, and one has an estimated redshift of around 10 (heic1103), placing it 400 million years earlier. However the newly discovered galaxy has dramatically different features from other distant galaxies that have been observed, which generally shine brightly with only young stars.
“When we looked at the spectra, two things were clear,” explains co-author Eiichi Egami. “The redshift placed it very early in cosmic history, as we expected. But the Spitzer infrared detection also indicated that the galaxy was made up of surprisingly old and relatively faint stars. This told us that the galaxy was made up of stars already nearly 750 million years old — pushing back the epoch of its formation to about 200 million years after the Big Bang, much further than we had expected.”
The discovery has implications beyond the question of when galaxies first formed, and may help explain how the Universe became transparent to ultraviolet light in the first billion years after the Big Bang. In the early years of the cosmos, a diffuse fog of neutral hydrogen gas blocked ultraviolet light in the Universe. Some source of radiation must therefore have progressively ionised the diffuse gas, clearing the fog to make it transparent to ultraviolet rays as it is today — a process known as reionisation.
Astronomers believe that the radiation that powered this reionisation must have come from galaxies. But so far, nowhere near enough of them have been found to provide the necessary radiation. This discovery may help solve this enigma.
“It seems probable that there are in fact far more galaxies out there in the early Universe than we previously estimated — it’s just that many galaxies are older and fainter, like the one we have just discovered,” says co-author Jean-Paul Kneib. “If this unseen army of faint, elderly galaxies is indeed out there, they could provide the missing radiation that made the Universe transparent to ultraviolet light.”
As of today, we can only discover these galaxies by observing through massive clusters that act as cosmic telescopes. In coming years, the NASA/ESA/CSA James Webb Space Telescope, scheduled for launch later this decade, will specialise in high resolution observations of distant, highly redshifted objects. It will therefore be in an ideal position to solve this mystery once and for all.
 The research will appear in a paper entitled “Discovery of a possibly old galaxy at z=6.027, multiply imaged by the massive cluster Abell 383”, to be published in the Monthly Notices of the Royal Astronomical Society. The international team of astronomers in this study consists of Johan Richard (CRAL, Observatoire de Lyon, Université Lyon 1, France and Dark Cosmology Centre, Niels Bohr Institute, University of Copenhagen, Denmark), Jean-Paul Kneib (Laboratoire d’Astrophysique de Marseille, France), Harald Ebeling (University of Hawaii, USA), Daniel P Stark (University of Cambridge, UK), Eiichi Egami (University of Arizona, USA) and Andrew K Fiedler (University of Arizona, USA). Lead author Johan Richard is a former Marie Curie fellow. The European Union's Marie Curie research fund provides grants at post-graduate and post-doctoral level to encourage mobility among Europe's best researchers. The EU will allocate more than €4.5 billion through the scheme in 2007-2013.
 Gravity distorts space-time, the fabric of the cosmos. This means that for extremely massive objects with very strong gravitational fields, light is visibly bent as it travels through and around them. Massive galaxy clusters like Abell 383 therefore act like an enormous lens, concentrating the light from distant objects behind them, in a process known as gravitational lensing. While the galaxies seen through gravitational lenses are typically distorted and multiply imaged (this newly discovered galaxy is actually visible twice in the Hubble observations), using these gravitational lenses multiplies a telescope’s power and lets it see galaxies that would otherwise be too faint to be visible. Abell 383, the gravitational lens used in this study, was imaged as part of the CLASH survey (Cluster Lensing And Supernova survey with Hubble), a Multi Cycle Treasury project to observe a sample of 25 galaxy clusters using Hubble (PI: Marc Postman). Abell 383 is also one of the 50 clusters imaged with the Spitzer Warm mission large project led by Eiichi Egami.
 Because the Universe is expanding, the light from distant objects is stretched and reddened as it moves towards us, a phenomenon known as redshift. The further an object is away, the more heavily redshifted it is. For very remote objects, redshift can be used to quantify their distance.
 Because light travels at a finite speed, the further away an object is, the further back in time we see it. For an object at a redshift of 6, the light has taken around 12.8 billion years to travel to Earth. Since we know that the Universe is about 13.75 billion years old, this means we are seeing the object in the state it was in less than a billion years after the Big Bang. Redshift is therefore a measure of time elapsed since the Big Bang as well as of an object’s distance.
Image credit: NASA, ESA, J. Richard (CRAL) and J.-P. Kneib (LAM). Acknowledgement: Marc Postman (STScI)
Images of Hubble
Research paper link
NASA Hubble release
Centre de Recherche Astrophysique de Lyon, Université Lyon 1, Observatoire de Lyon
Tel: +33 478 868 381
Laboratoire d’Astrophysique de Marseille — CNRS, Université de Provence
Tel: +33 685 988 265
Space Telescope Science Institute
W. M. Keck Observatory
Mauna Kea, Hawaii, USA
NASA’s Jet Propulsion Laboratory