Tag Archives: redshift

A galaxy far, far away… (take two)

Last November I wrote about the most distant galaxy ever seen. Since then, one even further away has been found. This post is (slightly) adapted from an article I wrote for Felix about this new galaxy.

The newly discovered galaxy is circled in the top left hand corner. Credit: NASA/ESA

There haven’t always been stars and galaxies in the universe, and the time when they began to form — known as the reionisation epoch — is the subject of much interest in astrophysics. A paper published in Nature details a discovery that could tell us more about this mysterious time.

In the paper, Rychard Bouwens and colleagues say they have detected the most distant galaxy ever seen; the light from the galaxy was emitted only 500 million years after the Big Bang. This age puts it well within the epoch of reionisation.

The galaxy has the highest redshift ever observed; it was from this that the team were able to calculate the galaxy’s age.

Cosmological redshift is a measure of how fast an object is moving away from the Earth and is a consequence of the expanding Universe. Objects with higher redshift are moving away from the Earth faster than those with lower redshifts, which means they are further away from Earth and also further back in time. To put it simply, the higher the redshift the older the galaxy.

Bouwens and colleagues used something known as the Lyman-break technique to identify the galaxy. This technique relies on a sharp drop in the spectrum of a galaxy that is due to the absorption of energetic photons by neutral gas that surrounds galaxy forming regions. The discovery can then be confirmed by looking at optical images.

For a long time the observations required to study the reionisation epoch were out of reach, but recent images from Hubble are making the detection and study of far away galaxies possible for the first time. The new galaxy was discovered in images taken by Hubble’s Wide Field Camera 3.

Bouwens and colleagues also looked into the rate of star formation at the time just after the newly discovered galaxy. They discovered that in just 200 million years the rate of star formation increased tenfold. This confirms that the newly discovered galaxy is right in the heart of the reionisation epoch, and sheds new light on how the stars and galaxies we see today formed.

It seems that galaxies around at the same time as this new discovery may not have been able to fully reionise the universe. This leaves the means by which the universe went from being a neutral gas to an ionised one, with electrons and protons stripped away from each other, a mystery. However, the existence of galaxies at this time does point to the first stars forming 100 million years beforehand, or around 400 million years after the Big Bang.

“We’re seeing huge changes in the rate of star birth that tell us that if we go a little further back in time we’re going to see even more dramatic changes,” said Garth Illingworth, a co-author of the paper from the University of California at Santa Cruz. “We’re moving into a regime where there are big changes afoot. Another couple of hundred million years back towards the Big Bang, and that will be the time when the first galaxies really are starting to build up.”

References
Bouwens, R., Illingworth, G., Labbe, I., Oesch, P., Trenti, M., Carollo, C., van Dokkum, P., Franx, M., Stiavelli, M., González, V., Magee, D., & Bradley, L. (2011). A candidate redshift z ≈ 10 galaxy and rapid changes in that population at an age of 500 Myr Nature, 469 (7331), 504-507 DOI: 10.1038/nature09717

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A galaxy far, far away…

This post was chosen as an Editor's Selection for ResearchBlogging.org

When we look up into the sky at night, we see stars (even in London I can usually spot a few!). But there haven’t always been stars and galaxies in the universe. In a period known as the dark ages – not to be confused with the other dark ages – there was no light at all. After the the ionised gas that filled the universe in its very early life cleared, there was a very long period of, well, nothing. The universe was transparent, but contained no stars or galaxies for just less than 400 million years. The process that allowed stars and galaxies to eventually form is known as reionisation, and new research published in Nature last month details a discovery that may open a new window on to this time.

Galaxy UDFy-38135539 shown in the Hubble Ultra Deep Field. Image: NASA

In the paper, Lehnert and colleagues reported detecting the most distant object physicists have ever seen: a galaxy, the light from which was emitted less than 600 million years after the Big Bang. It’s the first galaxy known to have lived fully within the epoch of reionisation.

The galaxy, which goes by the catchy name UDFy-38135539, has a redshift* of z = 8.6 – the highest ever observed – and it was from this that the team were able to calculate the galaxy’s age. UDFy-38135539 was first spotted by Hubble’s Wide Field Camera 3, but Lehnert and colleagues made ground based observations using an instrument called SINFONI on the Very Large Telescope in Chile to look at the galaxy in more detail.

The instrument helped by splitting up the light from the galaxy in a process known as spectroscopy, allowing the team to look for a feature called the Lyman-α line. Each photon making up the Lyman-α line would have been emitted when an electron in a hydrogen ion dropped down from a higher energy level to a lower one. The photons that Lehnert and colleagues observed were ultraviolet when they were emitted from the galaxy, but when they reached Earth had wavelengths in the infrared region, giving the high redshift mentioned above. This stretching of the wavelength occurs because of the length of time the photons took to travel here – they were created just 600 million years after the big bang. This may sound like a long time, but if you consider that the age of the Universe is 13.7 billion years, you’ll appreciate that 600 million years is actually very early on in the grand scheme of things, and certainly very, very long ago. Physicists know that reionisation started within 600 million years of the Big Bang, so Lehnert and colleagues came to the conclusion that galaxy UDFy-38135539 must have lived within the epoch of reionisation.

Diagram showing the universe from the Big Bang, to now. Image: Wikipedia

At the beginning, the Universe was very hot and dense, with conditions similar to that in a particle accelerator. After three minutes, the Universe had expanded and cooled enough to have formed all of the elementary particles, as well as protons and neutrons (also in these first three minutes was the matter-antimatter annihilation that destroyed most of the antimatter in the universe). For 400,000 years after this the universe was full of ionised gas, and was opaque. Then, in a period known as recombination, the electrons and protons in the gas got together and formed atoms; this made everything a lot clearer. For around 400 million years after that, the universe remained transparent and rather empty, with no stars or galaxies. It was only when astronomical objects, possibly quasars or small galaxies, began to form due to gravitational collapse that things began to get a bit more interesting.

These objects poured radiation out into the universe, causing reionisation. During reionisation, electrons were stripped back off the hydrogen atoms that were formed when they first joined up with the protons, and the universe began to turn into an ionised gas once again. Fortunately, due to the expansion that had taken place in the time between recombination and reionisation, the universe was able to remain transparent despite these bubbles of plasma that had begun to form all over the place. This process led to the formation of the stars and galaxies we see today, but physicists are not yet sure exactly how this all happened.

Because the galaxy UDFy-38135539 lived within the epoch of reionisation, it may be able to help us explain how reionisation started, and how these objects that formed in the cosmological dark ages were able to transform the universe from a mostly neutral one, to one filled with ionised gas.

There are already a few other faraway candidates lined up for study too, and Lehnert and colleagues have shown that such study is possible with current instruments, but astronomers will have to wait for the new wave of telescopes to really study reionisation in detail. The James Webb Space Telescope (JWST), which is the successor to Hubble, and the Extremely Large Telescope (ELT), which is the successor of the VLT, are two that will allow for this more detailed investigation. Both are due to be up and running later on this decade.

* Cosmological redshift is a measure of how fast an object is moving away from the Earth and is a consequence of the expanding Universe. Objects with higher redshift are moving away from the Earth faster than those with lower redshifts, and are further away too. See an earlier post of mine for an image showing redshift in action.

Reference

M. D. Lehnert, N. P. H. Nesvadba, J. -G. Cuby, A. M. Swinbank, S. Morris, B. Clement, C. J. Evans, M. N. Bremer, & S. Basa (2010). Spectroscopic confirmation of a galaxy at redshift z=8.6 Nature, 467 arXiv: 1010.4312v1

Further reading

BBC article, including short phone interview with Malcolm Bremer who was one of the physicists on the team.

Blog post at Cosmic log, which includes a Q&A with lead researcher Matt Lehnert.

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New limit on neutrino mass… from cosmology, not particle physics

Physicists at University College London have found a new upper limit on the mass of a neutrino – one of the tightest constraints yet from either particle physics or cosmology.

Neutrinos are elementary particles that travel close to the speed of light, but are very difficult to detect because they are not electrically charged. In fact, in the time it takes you to read this sentence, thousands of billions of neutrinos will have passed through your body – and you won’t have felt a thing.

According to the Standard Model of particle physics, neutrinos should be massless – just like the photons that make up light – but in reality they do have a very small mass. What the Standard Model failed to take into account is the fact that neutrinos undergo something known as oscillations, or mixing.

Neutrinos come in three “flavours”: electron neutrinos, mu neutrinos and tau neutrinos (as well as a corresponding antiparticle for each). When a neutrino is created, for example in the Sun during nuclear fusion, it has a specific flavour. Over time the neutrino can change flavour, but only if its mass is non-zero. All of the neutrinos created in the Sun are electron neutrinos. However, by the time they reach the Earth, we detect equal amounts of each flavour of neutrino; this is how we know that neutrinos must have mass.

Sudbury Neutrino Observatory: underground detector of solar neutrinos. Image: NASA

Shaun Thomas and colleagues at UCL have now found an upper limit on that mass. It’s the tightest constraint ever placed on the neutrino mass, and comes from cosmology rather than particle physics. Thomas et al took redshift data from over 700,000 galaxies using the Sloan Digital Sky Survey and combined this with results from Wilkinson Microwave Anisotropy Probe, which measured the radiation left over from the Big Bang. They were then able to compare density distributions from the early and more recent Universe.

A Universe where neutrinos are massless would look a bit different to our own. Having massive neutrinos means that the total mass in the Universe is higher than it otherwise would be, and the evolution of the Universe is affected. Larger neutrinos suppress the growth of galaxies more than smaller ones; the more mass neutrinos have, the fewer galaxies will be able to form.

From this relationship, Thomas et al were able to provide the first limit on neutrino mass to come from a galaxy redshift survey, and the tightest constraint yet. The new limit found will complement future neutrino experiments such as KATRIN, and provides hope that the next generation of galaxy surveys may be able to put even tighter constraints on the mass.

Reference:
Thomas, S., Abdalla, F., & Lahav, O. (2010). Upper Bound of 0.28 eV on Neutrino Masses from the Largest Photometric Redshift Survey Physical Review Letters, 105 (3) DOI: 10.1103/PhysRevLett.105.031301

PDF available here.

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Mapping the cosmos: Can a new technique help us learn more about dark energy?

In a paper published in Nature today, physicists detail a new method of looking at faraway galaxies that may help shed light on dark energy.

In order to learn more about dark energy – the mysterious force that is believed to be responsible for the ever increasing rate of expansion of the Universe – astronomers need to be able to peer further back in time. Luckily, due to the finite speed of light, all we need to do to see further back in time is to look at objects further away. For example, if we look at a galaxy that is ten light years away, we see it as it was ten years ago. Simple.

What is not so simple is working out how we can observe far away objects in enough detail to make the observations useful. When observing galaxies, astronomers look at their emission spectra, which are made up of spectral lines that each correspond to a certain wavelength of light that has been emitted by a particular element. From these lines astronomers can determine which elements are present, but spectral lines can have other uses too.

The emission line with a wavelength of 21cm is caused by neutral hydrogen, and is potentially very useful when it comes to probing dark energy. So far, astronomers have been able to detect the 21cm line in galaxies with a redshift up to 0.24. Cosmological redshift is a measure of how fast an object is moving away from the Earth and is a consequence of the expanding Universe. Objects with higher redshift are moving away from the Earth faster than those with lower redshifts, and are further away too. Galaxies more distant than those with a redshift of 0.24 are too faint for the 21cm line to be detected using traditional methods. It is believed that observations of the 21cm line from galaxies with redshifts between 0.5 and 2.5 would allow us to gain a better understanding of dark energy, so physicists have been trying to find a way to make these observations.

Emission spectrum for the Sun (left) compared to the spectrum from a supercluster of distant galaxies (right). Spectral lines are shifted towards the red end of the spectrum as shown by arrows, because the cluster of galaxies is moving away from us at an ever increasing speed. Image: Wikipedia

Chang et al have come up with a new technique called intensity mapping that may help to solve this problem. Rather than trying to look at the 21cm emission line from individual galaxies that are too far away, they have measured the total emission from a “cosmic web” containing thousands of galaxies. Combining this with data from the DEEP2 optical galaxy redshift survey they have produced a 3D intensity map for redshifts between z=0.53 and z=1.12, giving an insight into the 21cm emission line in the region needed to probe dark energy. In doing this they have avoided having to look at every individual galaxy and instead jumped straight to determining the large scale structure of the Universe.

The large scale structure, which describes the distribution of galaxies in the Universe on scales of millions of light years, can give us an insight into the effects of dark energy on the Universe. In developing a new method that allows us to look at the 21cm emission line for even further away galaxies, and therefore find the large scale structure at times closer to the big bang, Chang et al have given us a first taste of what we may be able to do with further study of the large scale structure of our Universe.

Reference:
Chang, T., Pen, U., Bandura, K., & Peterson, J. (2010). An intensity map of hydrogen 21-cm emission at redshift z ≈ 0.8 Nature, 466 (7305), 463-465 DOI: 10.1038/nature09187

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