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Welcome to Everything Science
Disks encircling hypergiant stars may spawn planets in inhospitable environment PDF Print
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Everything Space
Written by Everything Science   
Feb 08, 2006 at 12:00 AM
The discovery of dusty disks--the building blocks of planets--around two of the most massive stars known suggests that planets might form and survive in surprisingly hostile environments.

Dust Ring
This illustration compares the size of a gargantuan star and its surrounding dusty disk (top) to that of our solar system.

The discovery was made through NASA's Spitzer Space Telescope observations of two hypergiant stars in the Large Magellanic Cloud--the Milky Way's nearest neighboring galaxy--by a team led by Joel Kastner, a professor at Rochester Institute of Technology's Chester F. Carlson Center for Imaging Science. His team's findings will appear in the Feb. 10 issue of Astrophysical Journal Letters.

So far, searches for planets outside the solar system have been restricted to sun-like stars. All of these stars are older, dimmer and cooler objects than hypergiants, which are extraordinarily large and luminous but shorter-lived by billions of years.

Kastner and his team used infrared spectra obtained by Spitzer to study a population of dying stars. They added a new direction to their project when Spitzer's infrared spectrograph revealed unexpected information. Spitzer's sensitive spectrometer, which breaks down infrared radiation into component wavelengths as a prism splits visible light into a rainbow, indicated that a third of the stars in the population thought to be in decline--including two massive and exceedingly luminous hypergiants--were actually younger stars in varying stages of development.

The curious spectra of these two hypergiants (R126 and R66)--with one star being 70 times bigger than the sun--led Kastner to reexamine the stars' classifications as dying. The shape of the spectra, or the amount of light from different wavelengths, is characteristic of flattened disks of dust orbiting the stars.

The two stars' similar spectra differ in detail, with one encircled by dust in crystalline form, the other by more shapeless, amorphous dust grains. This expands the range of known conditions under which complex dust grains and molecules can form and persist around stars, Kastner says.

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Counting Cells That Ensure Gene Balance PDF Print
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Everything Biology
Written by Everything Science   
Feb 05, 2006 at 12:00 AM
Two are one too many – this is the motto used by cells of a female organism: These contain two X chromosomes, one of which always becomes inactivated. How does the cell recognize that it contains two of these sex chromosomes and how does it choose which one to turn off? Scientists of the German Cancer Research Center (Deutsches Krebsforschungszentrum, DKFZ), working together with French colleagues, have now been able to elucidate an early step in this complex process.

ncb3
Female embryonic stem cells differentiated for 2 days. Red: X-chromosomes, green: X-inactivation centers (Xics)

Forty-five years ago, British scientist Mary Lyon already described this chromosome inactivation typical of female cells. Lyon proposed a hypothesis: With two copies of the X chromosome, all X-linked genes are present in two copies. However, in a male organism, which is equipped with a set of one X and one Y chromosome, the X genes are present in only one copy in each cell. To restore genetic balance, a female cell inactivates one of its two X chromosomes.

During development of a female embryo, inactivation of either of the X chromosomes, the one inherited from the father or the one inherited from the mother, occurs at random. To coordinate inactivation, the cell first needs to determine whether it contains more than one X chromosome and then make a choice which of the two to switch off. Since the mid-1980s it has been known that a specific region of the X chromosome termed X inactivation center (Xic) is crucial for a correct inactivation process.

Professor Dr. Roland Eils, who leads the bioinformatics departments at the German Cancer Research Center and at the Institute of Pharmacy and Molecular Biotechnology of Heidelberg University, suspected that the spatial arrangement of the Xics within the nucleus is key to inactivation. Working together with colleagues of the Curie Institute, Paris, he searched different cells for distinctive features in the distribution of Xic regions. The scientists compared developing female embryonic stem cells of mice just before X inactivation, with mouse cells in which X inactivation had already taken place. Using a 3-dimensional visualization of fluorescent labels of the Xic regions, they observed that the Xics of both X chromosomes in the developing stem cells were located very close to each other in up to 15 percent of cells. In the comparative cell line, this was found in only about three percent of cells, which constitutes a random result. The formation of pairs (co-localization) was particularly noticeable in the stem cells after about one and a half days of development, i.e. shortly before X inactivation.

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Plasma vessel for Wendelstein 7-X ready PDF Print
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Everything Physical Science
Written by Everything Science   
Jan 22, 2006 at 12:00 AM
The first large production order for the Wendelstein 7-X fusion experiment, construction of the plasma chamber, has been successfully completed: The 20 sectors of the bizarrely shaped 35-ton vessel were assembled from several hundred individual components – an engineering masterpiece. Installation of the whole complex device, which started in spring 2005 at the Greifswald branch of Max Planck Institute of Plasma Physics (IPP), will take about six years.

w7x_gefaess_klein
Part of the plasma chamber of Wendelstein 7-X: Twenty of these elements are joined to form a ring shaped in keeping with the twisting contours of the plasma. The ports in the vessel grant access for heating and measuring facilities. (Photo: IPP, W. Filser)

The aim of fusion research is to derive energy from fusion of atomic nuclei like the sun. To ignite the fusion fire the fuel in a future power plant, a hydrogen plasma, has to be confined in magnetic fields and heated to temperatures of over 100 million degrees. Wendelstein 7-X, which on completion will be the biggest fusion device of the stellarator type in the world, is aimed at investigating the suitability of this concept for application in power plants.

The plasma vessel was produced in 20 sections by MAN DWE GmbH at Deggendorf, Germany, four of which are already in use at IPP for installing the experiment. The assembled ring-shaped plasma chamber with a diameter of about 12 metres will later confine the plasma heated to 100 million degrees. The shape of the vessel is matched to the twisting plasma ring. This peculiar shape in conjunction with the high precision required constitutes a major challenge for production: tolerances of less than 3 millimetres being called for in some cases.

In order to fashion the bizarre shape from steel, the 35-ton vessel was assembled from 200 individual rings. Each ring, in turn, is composed of several finger-thick steel strips 18 centimetres wide which are multiply bent in keeping with the twisting contours. The more than 800 individual components of the vessel are joined vacuum-proof by more than 1,600 metres of brazing. For this purpose the components to be connected were placed in exactly defined positions two millimetres apart, the gaps being closed by hand with several adjacent and superposed brazed layers of wire – a total of several kilometres of brazing wire being used in the process.

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Dinosaurs: Slower Growth in Hard Times PDF Print
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Everything Archaeology
Written by Everything Science   
Dec 15, 2005 at 12:00 AM
Palaeontologists from the University of Bonn report on an intriguing diagnosis in the 16 December issue of the journal Science. A dinosaur which they have examined was apparently able to vary the speed of its growth according the conditions obtaining in its environment. Although tortoises and crocodiles also do this, plateosaurus engelhardti seems to be unique among dinosaurs, leading experts to puzzle over whether the family history of the dinosaurs will need to be rewritten.

Martin Sander
Martin Sander taking samples of a fossil dinosaur bone for further examinations.
‘Basically dinosaurs grew like we do,’ the Bonn palaeontologist Dr. Martin Sander explains: ‘Each age corresponded to a particular body size.’ There was not much leeway involved. Reptiles do things differently: when food is scarce they grow more slowly than when there is food galore. Thus, a tortoise can be 30, 40 or even 60 centimetres long at the same age. ‘Warm-blooded animals, by contrast, cannot so easily turn down their metabolism,’ the lecturer says: ‘If the food supply is inadequate, there’s only one thing they can do – die.’

Dinosaurs lie somewhere in between: although they are descended from the reptiles, many of them had become warm-blooded, most researchers today agree. And they all grew like modern mammals: in accordance with a genetically programmed blueprint and in addition relatively fast. ‘At least that’s what was thought until recently,’ Dr. Sander says. ‘However, our findings have thrown this conception into disarray, at least for one dinosaur.’

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