Images from Planck space observatory reveal star formation processes

Washington, April 27 (ANI): Star formation takes place hidden behind veils of gas and dust, but ESA’s Planck space observatory – with its microwave eyes – can peer beneath that shroud to provide new insights into star-forming process.

The latest images released by the Planck team bring to light two different star forming regions in the Milky Way, and in stunning detail, reveal the different physical processes at work.

The Orion region is a cradle of star formation, some 1,500 light-years away. It is famous for the Orion Nebula, which can be seen by the naked eye as a faint smudge.

The first image covers much of the constellation of Orion. The nebula is the bright spot to the lower center. The bright spot to the right of center is around the Horsehead Nebula, so called because at high magnifications a pillar of dust resembles a horse’s head.

The giant red arc of Barnard’s Loop is thought to be the blast wave from a star that blew up inside the region about two million years ago. The bubble it created is now about 300 light-years across.

In contrast to Orion, the Perseus region is a less vigorous star-forming area but, as Planck shows in the other image, there is still plenty going on.

The images both show three physical processes taking place in the dust and gas of the interstellar medium. Planck can show us each process

separately.

At the lowest frequencies, Planck maps emission caused by high-speed electrons interacting with the Galaxy’s magnetic fields. An additional diffuse component comes from spinning dust particles emitting at these frequencies.

At intermediate wavelengths of a few millimeters, the emission is from

gas heated by newly formed hot stars.

At still higher frequencies, Planck maps the meager heat given out by extremely cold dust. This can reveal the coldest cores in the clouds, which are approaching the final stages of collapse, before they are reborn as fully-fledged stars. The stars then disperse the surrounding clouds.

The delicate balance between cloud collapse and dispersion regulates the number of stars that the Galaxy makes. (ANI)

Planck spacecraft obtains first peek of big bang’s ‘afterglow’

London, September 18 (ANI): European Space Agency’s (ESA’s) Planck spacecraft has obtained its first peek at the afterglow of the big bang, revealing it in unprecedented detail.

The ESA spacecraft was launched into space on May 14 this year. It is observing the glow of hot gas from just 380,000 years after the big bang, called the cosmic microwave background (CMB).

According to a report in New Scientist, the detailed properties of this background may contain hints of hidden extra dimensions or multiple universes, as well as providing clues to what caused a brief, early period of incredibly rapid cosmic expansion.

Planck began surveying the microwave background on August 13, a few weeks after reaching its planned perch 1.5 million kilometres from Earth at a point called L2 and cooling its detectors to within 0.1 degrees Celsius above absolute zero.

Now, the Planck team has released the probe’s first image, an observational strip covering about 5 per cent of the sky.

Slight variations in temperature from place to place in the early universe give the image its mottled appearance.

“With a few per cent of the data in, you can see it’s working well and delivering good stuff,” said team member George Efstathiou of the University of Cambridge.

Planck is expected to provide the most detailed all-sky map of the cosmic microwave background yet, improving on the best current map, obtained by NASA’s Wilkinson Microwave Anisotropy Probe (WMAP), which launched in 2001.

Planck’s detectors have more than 10 times the sensitivity of WMAP’s, and about 2.5 times the angular resolution.

“Every strip that Planck scans, we’re getting data that is many, many times more sensitive than WMAP,” Efstathiou told New Scientist.

Although Planck was only designed to observe the sky for 15 months, the team believes it could last for more than 30 months, based on new estimates of how long its coolant will last.

The extra time will allow Planck to measure the radiation with even greater precision, since it will scan the entire sky four times – two more than originally planned. (ANI)

Scientists capture first image of memory formation

Washington, June 19 : Scientists have for the first time captured an image of a mechanism that underlies long-term memory formation.

It shows that when a new memory is formed, new proteins are made locally at the synapse – the connection between nerve cells – increasing the strength of the synaptic connection and reinforcing the memory.

The study, conducted by researchers at the Montreal Neurological Institute and Hospital (The Neuro), McGill University and University of California, Los Angeles, is important for understanding how memory traces are created and the ability to monitor it in real time will allow a detailed understanding of how memories are formed.

When considering what might be going on in the brain at a molecular level two essential properties of memory need to be taken into account.

First, because a lot of information needs to be maintained over a long time there has to be some degree of stability. Second, to allow for learning and adaptation the system also needs to be highly flexible.

For this reason, research has focused on synapses, which are the main site of exchange and storage in the brain.

They form a vast but also constantly fluctuating network of connections whose ability to change and adapt, called synaptic plasticity, may be the fundamental basis of learning and memory.

“But, if this network is constantly changing, the question is how do memories stay put, how are they formed? It has been known for some time that an important step in long-term memory formation is “translation”, or the production, of new proteins locally at the synapse, strengthening the synaptic connection in the reinforcement of a memory, which until now has never been imaged,” says Dr. Wayne Sossin, neuroscientist at The Neuro and co-investigator in the study.

“Using a translational reporter, a fluorescent protein that can be easily detected and tracked, we directly visualized the increased local translation, or protein synthesis, during memory formation. Importantly, this translation was synapse-specific and it required activation of the post-synaptic cell, showing that this step required cooperation between the pre and post-synaptic compartments, the parts of the two neurons that meet at the synapse. Thus highly regulated local translation occurs at synapses during long-term plasticity and requires trans-synaptic signals,” Sossin added.

Long-term memory and synaptic plasticity require changes in gene expression and yet can occur in a synapse-specific manner.

This study provides evidence that a mechanism that mediates this gene expression during neuronal plasticity involves regulated translation of localized mRNA at stimulated synapses.

According to researchers, these findings are instrumental in establishing the molecular processes involved in long-term memory formation and provide insight into diseases involving memory impairment.

The study has been published in Science journal.

World’s largest solar telescope offers better understanding of Sun’s magnetic field

Washington, May 29 (ANI): The world’s largest solar telescope, which can capture the Sun’s magnetic field better than other telescopes, is now operational.

The new 1.6-meter clear aperture solar telescope, the largest of its kind in the world, is housed at the New Jersey Institute of Technology in Newark, New Jersey, US.

“We are already seeing images offering a better understanding of the Sun,” said NJIT Distinguished Professor of Physics Philip R. Goode.

“With this instrument, we should be able to have a better understanding of dynamic storms and space weather, which can have dramatic effects on Earth,” he added.

Earlier this month, researchers achieved what is called first scientific light.

This means the telescope is operational. To achieve its full powers, at least three more years of work will be needed to bring on-line ever-more sophisticated hardware for observing the Sun.evertheless, Goode and the BBSO (Big Bear Solar Observatory) research team were able to extract a few unique images and one is shown.

The photos clearly illustrate the before-and-after capabilities of the old versus new telescope. Our prized first image shows the Sun’s ever-present, turbulent granular field with its largest granules being about the size of Alaska,” Goode said.

“The small, bright points in the dark lanes are less than 50 miles across and are the smallest-scale magnetic structures on the Sun,” he added.

According to Goode, if one looks closely at the “after” photo, you will see a string of pearls. Each pearl is a cross-section of an intense, single fiber of the Sun’s magnetic field – the basic building block of the solar magnetism,” he said.

Goode added that the Sun is now in a state of prolonged magnetic inactivity, perhaps the longest such time in a century.

“The new telescope is ideal for studying the Sun as it rises from this strange state of quietude,” he said.

The new instrument has three times the aperture of the old telescope.

It represents a significant advance in high-resolution observations of the Sun, since it has the largest aperture of any solar telescope in existence, said Goode.

The new telescope will be used in joint observation campaigns with NASA satellites to optimize the scientific output of all observations of the Sun. (ANI)