NASA’s Swift satellite makes best-ever ultraviolet portrait of Andromeda galaxy

Washington, September 17 (ANI): NASA’s Swift satellite has acquired the highest-resolution view of a neighboring spiral galaxy ever attained in the ultraviolet.

The galaxy, known as M31 in the constellation Andromeda, is the largest and closest spiral galaxy to our own.

“Swift reveals about 20,000 ultraviolet sources in M31, especially hot, young stars and dense star clusters,” said Stefan Immler, a research scientist on the Swift team at NASA’s Goddard Space Flight Center in Greenbelt, Maryland.

“Of particular importance is that we have covered the galaxy in three ultraviolet filters. That will let us study M31′s star-formation processes in much greater detail than previously possible,” he added.

M31, also known as the Andromeda Galaxy, is more than 220,000 light-years across and lies 2.5 million light-years away.

On a clear, dark night, the galaxy is faintly visible as a misty patch to the naked eye.

Between May 25 and July 26, 2008, Swift’s Ultraviolet/Optical Telescope (UVOT) acquired 330 images of M31 at wavelengths of 192.8, 224.6, and 260 nanometers.

The images represent a total exposure time of 24 hours.

The task of assembling the resulting 85 gigabytes of images fell to Erin Grand, an undergraduate student at the University of Maryland at College Park who worked with Immler as an intern this summer.

“After ten weeks of processing that immense amount of data, I’m extremely proud of this new view of M31,” she said.

Several features are immediately apparent in the new mosaic.

The first is the striking difference between the galaxy’s central bulge and its spiral arms.

“The bulge is smoother and redder because it’s full of older and cooler stars,” Immler explained. “Very few new stars form here because most of the materials needed to make them have been depleted,” he added.

Dense clusters of hot, young, blue stars sparkle beyond the central bulge.

M31′s disk and spiral arms contain most of the gas and dust needed to produce new generations of stars.

Star clusters are especially plentiful in an enormous ring about 150,000 light-years across.

“Swift is surveying nearby galaxies like M31 so astronomers can better understand star- formation conditions and relate them to conditions in the distant galaxies where we see gamma-ray bursts occurring,” said Neil Gehrels, the mission’s principal investigator at NASA Goddard. (ANI)

Galileoscope to make wonders of the night sky more accessible to everyone

Berlin, March 5 (ANI): A team of leading astronomers, optical engineers and science educators has designed the Galileoscope – a high quality, easy-to-assemble and easy-to-use telescope, which would make the wonders of the night sky more accessible to everyone.

The Galileoscope was developed as a Cornerstone project of the International Year of Astronomy 2009 (IYA2009).

By encouraging the experience of personally seeing celestial objects, the Galileoscope project aims to facilitate a main goal of IYA2009: promoting widespread access to new knowledge and observing opportunities.

Observing through a telescope for the first time is an experience that shapes our view of the sky and the Universe.

It prompts people to think about the importance of astronomy, and for many, it’s a life-changing experience.

Galileoscopes will open up a whole new world for their users and are an excellent means of pursuing an interest in astronomy during IYA2009 and beyond.

The Galileoscope is named after the Italian astronomer Galileo Galilei, who first observed the heavens through a telescope 400 years ago.

The Galileoscope is optimized to provide views of the very same objects that inspired Galileo all those years ago – including craters and mountains on the Moon, the rings of Saturn, the phases of Venus, a variety of star clusters, and moons orbiting the planet Jupiter.

Galileoscopes are also educational tools, tying in with topics such as mathematics, physics, history and philosophy.

As practical instruments they can be used to demonstrate basic optical theory in a real-world scenario, a technique often praised by educators and pupils themselves.

“Users will learn many aspects of optics and even have a chance to construct two types of telescopes – a modern one and a more primitive one similar to Galileo’s,” said Stephen Pompea, US IYA2009 Project Director and member of the IYA2009 Cornerstone project.

“Building and using a Galileoscope gives kids the feeling that science is fun,” he added.

Galileoscopes are available at a low price of 15 dollars (US) per kit.

Discounts are available for group purchases of 100 or more, bringing the price down even lower, to 12.50 dollars each, reducing costs for schools, colleges, astronomical societies, or even parties of interested individuals.

To further this aim, the Galileoscope Cornerstone project has also initiated the “Give a Galileoscope” program.

Donated Galileoscopes will go to less advantaged schools and other organizations worldwide, especially in developing countries.

This will help bring a modern education to students in poor schools and empower them to pursue science and technology knowledge. (ANI)

Milky Way is 50 percent heftier than thought

London, Jan 21 (ANI): A new measurement of the Milky Way’s mass has suggested that the galaxy is 50 percent heftier than thought and about as heavy as our nearest large neighbour, Andromeda.

Astronomers have attempted to measure the mass of the Milky Way since the 1920s.

But, the measurement turns out to be exceedingly tricky, not least because some 90 percent of the galaxy’s mass is thought to be made of dark matter – a mysterious, invisible substance that only reveals its presence by its gravitational tugs on stars and gas clouds.

For a number of other galaxies, astronomers can circumvent the dark-matter problem by observing how a galaxy bends the light of more distant galaxies.

The larger the distortion, the stronger the gravitational tug of the intervening galaxy’s ordinary and dark matter.

But, because of Earth’s position within the Milky Way, astronomers are limited to directly measuring objects they can see: the galaxy’s gas and stars, as well as distant satellite galaxies and star clusters.

In principle, the motion of these objects can be used to estimate the galaxy’s mass.

The faster they move, the more mass must lie within their orbits to keep them from escaping into intergalactic space.

Now, according to a report in New Scientist, Mark Reid of the Harvard-Smithsonian Center for Astrophysics in Cambridge, Massachusetts, examined masers – dense star-forming regions that naturally emit microwaves, to find out the Milky Way’s mass.

By observing the same regions at different times of year, Reid and colleagues were able to discern slight changes in the masers’ position, which revealed their distance from Earth.

The team found that the masers seem to be orbiting the galactic centre faster than expected at those distances, meaning more mass is needed to keep them in orbit.

The revised speed suggests the Milky Way weighs some 3 trillion times the mass of the Sun.

Masers can only be used to weigh the Milky Way out to the edge of its visible disc, which ends some 60,000 light years from the galactic centre.

However, most of the Milky Way’s mass is thought to lie further away, out to a distance of some 650,000 light years.

Though measuring the mass of the Milky Way out to the very edge may be impossible, the motion of distant satellite galaxies and globular clusters – dense clumps of ancient stars – could offer some clue. (ANI)