Tag Archives: star

Planets From Stardust

Stunning images captured by Atacama Millimetre-submillimetre Array (ALMA) radio telescope in Chile show the early stages of a planet forming from stardust around a star located 450 light-years from Earth. This is the first time that astronomers have snapped such a clear picture of the process, confirming long-held theories of planetary formation.

[div class=attrib]From Independent:[end-div]

The world’s highest radio telescope, built on a Chilean plateau in the Andes 5,000 metres above sea level, has captured the first image of a new planet being formed as it gobbles up the cosmic dust and gas surrounding a distant star.

Astronomers have long predicted that giant “gas” planets similar to Jupiter would form by collecting the dust and debris that forms around a young star. Now they have the first visual evidence to support the phenomenon, scientists said.

The image taken by the Atacama Millimetre-submillimetre Array (ALMA) in Chile shows two streams of gas connecting the inner and outer disks of cosmic material surrounding the star HD 142527, which is about 450 light-years from Earth.

Astronomers believe the gas streamers are the result of two giant planets – too small to be visible in this image – exerting a gravitational pull on the cloud of surrounding dust and gas, causing the material to flow from the outer to inner stellar disks, said Simon Casassus of the University of Chile in Santiago.

“The most natural interpretation for the flows seen by ALMA is that the putative proto-planets are pulling streams of gas inward towards them that are channelled by their gravity. Much of the gas then overshoots the planets and continues inward to the portion of the disk close to the star, where it can eventually fall onto the star itself,” Dr Casassus said.

“Astronomers have been predicting that these streams exist, but this is the first time we’ve been able to see them directly. Thanks to the new ALMA telescope, we’ve been able to get direct observations to illuminate current theories of how planets are formed,” he said.

[div class=attrib]Read the entire article following the jump.[end-div]

[div class=attrib]Image: Observations (left) made with the ALMA telescope of the young star HD 142527. The dust in the outer disc is shown in red. Dense gas in the streams flowing across the gap, as well as in the outer disc, is shown in green. Diffuse gas in the central gap is shown in blue. The gas filaments can be seen at the three o’clock and ten o’clock positions, flowing from the outer disc towards the centre. And (right) an artist’s impression. Courtesy of Independent.[end-div]

A Star is Born, and its Solar System

A diminutive stellar blob some 450 million light years away seems to be a young star giving birth to a planetary system much like our very own Solar System. The developing protostar and its surrounding gas cloud is being tracked astronomers at the National Radio Astronomy Observatory in Charlottesville, Virginia. Stellar and planetary evolution in action.

[div class=attrib]From New Scientist:[end-div]

Swaddled in a cloud of dust and gas, the baby star shows a lot of potential. It is quietly sucking in matter from the cloud, which holds enough cosmic nourishment for the infant to grow as big and bright as our sun. What’s more, the star is surrounded by enough raw material to build at least seven planetary playmates.

Dubbed L1527, the star is still in the earliest stages of development, so it offers one of the best peeks yet at what our solar system may have looked like as it was taking shape.

The young star is currently one-fifth of the mass of the sun, but it is growing. If it has been bulking up at the same rate all its life, the star should be just 300,000 years old – a mere tyke compared to our 4.6-billion-year-old sun. But the newfound star may be even younger, because some theories say stars initially grow at a faster rate.

Diminutive sun

The cloud feeding the protostar contains at least as much material as our sun, says John Tobin of the National Radio Astronomy Observatory in Charlottesville, Virginia.

“The key factor in determining a star’s characteristics is the mass, so L1527 could potentially grow to become similar to the sun,” says Tobin.

Material from the cloud is being funnelled to the star through a swirling disc that contains roughly 0.5 per cent the mass of the sun. That might not sound like a lot, but that’s enough mass to make up at least seven Jupiter-sized planets.

Previous observations of L1527 had hinted that a disk encircled the star, but it was not clear that the disk was rotating, which is an essential ingredient for planet formation. So Tobin and his colleagues took a closer look.

Good rotations

The team used radio observations to detect the presence of carbon monoxide around the star and watched how the material swirled around in the disc to trace its overall motion. They found that matter nearest to the star is rotating faster than material near the edge of the disc – a pattern that mirrors the way planets orbit a star.

“The dust and gas are orbiting the protostar much like how planets orbit the sun,” says Tobin. “Unfortunately there is no telling how many planets might form or how large they will be.”

[div class=attrib]Read the entire article following the jump.[end-div]

[div class=attrib]Protostar L1527. Courtesy of NASA / JPL, via tumblr.[end-div]