Forum for Science, Industry and Business

Sponsored by:     3M 
Search our Site:


Astronomers see era of rapid galaxy formation


New findings pose a challenge for cold dark matter theory

"The universe is always more complicated than our cosmological theories would have it," says Nigel Sharp, program officer for extra-galactic astronomy and cosmology at the National Science Foundation (NSF). Witness a collection of new and recently announced discoveries that, taken together, suggest a considerably more active and fastmoving epoch of galaxy formation in the early universe than prevailing theories had called for.

The findings, each of which was obtained at facilities supported in whole or in part by the NSF, include the following:

  • Evidence from the Sloan Digital Sky Survey (SDSS) that at least a few ultra-massive black holes had come into existence less than a billion years after the universe began in the Big Bang, some 13.7 billion years ago. Each of these black holes is several billion times more massive than stars like our own Sun, and is sitting in the middle of an otherwise normal galaxy, swallowing up the surrounding gas and dust; the thermonuclear energy released in that process is visible to the SDSS astronomers as a brilliant, but very distant, point of light known as a quasar. The puzzle is that the SDSS black holes are as large as any ever seen, including those observed in nearby quasars that are much older. So how did they manage to form and grow to such a size before the universe was a tenth its present age? "The formation should have taken time," says Michael A. Strauss of Princeton University, who is the scientific spokesperson for the SDSS project and a co-principal investigator on this study. A formal report will be published in the Astronomical Journal in March 2004. A press release is available online at

  • Evidence from the Gemini Observatory that at least some galaxies had formed, grown, and "matured" by the time the universe was only 20 to 40 percent of its present age. This observation, which comes from a systematic scan of early galaxies known as the Gemini Deep Deep Survey (GDDS), gives us a snapshot of the cosmos at a considerably later time than the Sloan observations: several billion years after the Big Bang, versus 1 billion years. But it is surprising nonetheless. A "mature" galaxy is one that, like our own Milky Way, has already lived through its tumultuous youth-a period that typically includes the violent accretion of smaller galaxies and multiple bursts of star formation-and has finally settled down into a quieter, more stable middle age. Finding such individuals in the Gemini survey is like walking into a junior-high classroom and finding it full of adults. How did these galaxies manage to grow up so fast? The GDDS finding was presented on January 5, 2004, at the Atlanta meeting of the American Astronomical Society. A press release, along with artwork and illustrations, is available online at

  • Evidence from a U.S.-Australian team, working in part at the NSF’s Cerro Tololo Inter-American Observatory in Chile, that galaxies in this same era of the early universe had already begun to collect into well-defined clusters. Again, the question is how clustering could have progressed so rapidly. This discovery was reported at the astronomical society meeting on January 7, 2004. A press release, along with images and background material, is available at The team’s formal paper will be published by the Astrophysical Journal in February 2004.

In sum, says Princeton’s Strauss, these results give us "a variety of different types of hints that at least some types of galaxies settled down very early in the universe." Yet that fact, if true, is hard to understand in the prevailing theory of galaxy formation. According to the "Cold Dark Matter" model, as it’s known, galaxies and clusters grew in a bottom-up fashion-that is, with small structures forming first, and the bigger structures accumulating only much later. But does that mean that the Cold Dark Matter model is wrong? Or does it just mean that we’ve still got a lot to learn about how ordinary matter formed that first generation of stars?
Whatever the answer, says NSF’s Sharp, "there may be more happening early in the universe than we previously thought. It will be interesting to see how this plays out in the more extensive surveys that are now being planned."

Background: Cold Dark Matter and Galaxy Formation

Each of these studies, in various ways, addresses one of the most fundamental questions of cosmology: How did the Big Bang give rise to us? In the beginning, the matter that emerged from the primeval fireball was remarkably smooth and uniform. And yet now, some 13.7 billion years later, the matter in the universe is anything but uniform. Atoms have long since been swept up into planets, stars, and interstellar gas clouds. These objects, in turn, are organized into galaxies, which are grouped into clusters of galaxies, which are grouped into superclusters, and so on. How did that happen? What caused the universe to clump up in this way?

The short answer is "gravity": the universal force of attraction. As astronomers have known for generations, gravity had the power to destabilize even the smoothest distribution of matter. Say that by chance, a given region of the primeval fireball just happened to have a few more particles than average. That would have made the mutual gravitational attraction among those particles a little bit stronger than average. But then the resulting imbalance of forces would have pulled the particles closer together and increased their mutual attraction still further. That would have accelerated their motion, decreased their separation, increased their attraction-on and on, faster and faster and faster. Conversely, a region that happened to have a few less particles than average would have tended to hollow out over time, as gravity pulled as more and more matter into the denser regions. Either way, the result would have been a distribution of matter that was very lumpy indeed-lumps that presumably gave rise to the stars, galaxies, and clusters of galaxies.

A longer and more complete answer is "gravity"-but gravity acting on a universe that has, literally, much more than meets the eye. Over the past three decades or so, astronomers have come to realize that the stars, galaxies, and clusters they can see through their telescopes don’t contain nearly enough mass to clump up on their own. Instead, it’s now apparent that these visible objects are more like bright flecks of foam on a dark, swelling ocean. The "ocean waves," in this case, consist of Cold Dark Matter: an utterly invisible essence that is thought to be a haze of weakly interacting elementary particles left over from the Big Bang. (The dark matter is "cold" because the particles are presumed to be moving fairly slowly, at much less than the speed of light.) But whatever it is, the dark matter permeates the cosmos, is immensely massive, and controls the evolution of everything we can see. It is the dark matter that undergoes gravitational collapse and makes the universe lumpy; all the ordinary matter, the stuff that makes up stars, galaxies, and us, simply gets carried along.

The process of gravitational collapse in a Cold Dark Matter dominated universe has been studied through many, many computer simulations. Some vivid examples have been posted on the Universe in a Box page prepared by the University of Chicago’s Center for Cosmological Physics, an NSF-funded Physics Frontier Center. Many more examples can be found on the Cosmos In a Computer page posted by the University of Illinois’ National Center for Supercomputer Applications, one of the NSF-supported supercomputer centers.

Both of these sites also offer introductory tutorials on modern cosmology in general. Two sites that offer more extensive (and technical) tutorials are:, and

Meanwhile, there are a number of experiments underway around the world to detect the dark matter particles. One major effort is the Cryogenic Dark Matter Search, which is being funded jointly by NSF and the Department of Energy. The NSF award abstract is available here.

NSF is an independent federal agency that supports fundamental research and education across all fields of science and engineering, with an annual budget of nearly $5.3 billion. NSF funds reach all 50 states through grants to nearly 2,000 universities and institutions. Each year, NSF receives about 30,000 competitive requests for funding, and makes about 10,000 new funding awards. NSF also awards over $200 million in professional and service contracts yearly. Receive official NSF news electronically through the e-mail delivery system, NSFnews. To subscribe, send an e-mail message to In the body of the message, type "subscribe nsfnews" and then type your name. (Ex.: "subscribe nsfnews John Smith")

M. Mitchell Waldrop | NSF
Further information:

More articles from Physics and Astronomy:

nachricht New Method of Characterizing Graphene
30.05.2017 | Universität Basel

nachricht NASA's SDO sees partial eclipse in space
29.05.2017 | NASA/Goddard Space Flight Center

All articles from Physics and Astronomy >>>

The most recent press releases about innovation >>>

Die letzten 5 Focus-News des innovations-reports im Überblick:

Im Focus: Strathclyde-led research develops world's highest gain high-power laser amplifier

The world's highest gain high power laser amplifier - by many orders of magnitude - has been developed in research led at the University of Strathclyde.

The researchers demonstrated the feasibility of using plasma to amplify short laser pulses of picojoule-level energy up to 100 millijoules, which is a 'gain'...

Im Focus: Can the immune system be boosted against Staphylococcus aureus by delivery of messenger RNA?

Staphylococcus aureus is a feared pathogen (MRSA, multi-resistant S. aureus) due to frequent resistances against many antibiotics, especially in hospital infections. Researchers at the Paul-Ehrlich-Institut have identified immunological processes that prevent a successful immune response directed against the pathogenic agent. The delivery of bacterial proteins with RNA adjuvant or messenger RNA (mRNA) into immune cells allows the re-direction of the immune response towards an active defense against S. aureus. This could be of significant importance for the development of an effective vaccine. PLOS Pathogens has published these research results online on 25 May 2017.

Staphylococcus aureus (S. aureus) is a bacterium that colonizes by far more than half of the skin and the mucosa of adults, usually without causing infections....

Im Focus: A quantum walk of photons

Physicists from the University of Würzburg are capable of generating identical looking single light particles at the push of a button. Two new studies now demonstrate the potential this method holds.

The quantum computer has fuelled the imagination of scientists for decades: It is based on fundamentally different phenomena than a conventional computer....

Im Focus: Turmoil in sluggish electrons’ existence

An international team of physicists has monitored the scattering behaviour of electrons in a non-conducting material in real-time. Their insights could be beneficial for radiotherapy.

We can refer to electrons in non-conducting materials as ‘sluggish’. Typically, they remain fixed in a location, deep inside an atomic composite. It is hence...

Im Focus: Wafer-thin Magnetic Materials Developed for Future Quantum Technologies

Two-dimensional magnetic structures are regarded as a promising material for new types of data storage, since the magnetic properties of individual molecular building blocks can be investigated and modified. For the first time, researchers have now produced a wafer-thin ferrimagnet, in which molecules with different magnetic centers arrange themselves on a gold surface to form a checkerboard pattern. Scientists at the Swiss Nanoscience Institute at the University of Basel and the Paul Scherrer Institute published their findings in the journal Nature Communications.

Ferrimagnets are composed of two centers which are magnetized at different strengths and point in opposing directions. Two-dimensional, quasi-flat ferrimagnets...

All Focus news of the innovation-report >>>



Event News

Marine Conservation: IASS Contributes to UN Ocean Conference in New York on 5-9 June

24.05.2017 | Event News

AWK Aachen Machine Tool Colloquium 2017: Internet of Production for Agile Enterprises

23.05.2017 | Event News

Dortmund MST Conference presents Individualized Healthcare Solutions with micro and nanotechnology

22.05.2017 | Event News

Latest News

Reptile vocalization is surprisingly flexible

30.05.2017 | Life Sciences

EU research project DEMETER strives for innovation in enzyme production technology

30.05.2017 | Power and Electrical Engineering

New insights into the ancestors of all complex life

29.05.2017 | Earth Sciences

More VideoLinks >>>