Scientists observe budding solar systems

Washington, June 11 (ANI): Scientists have observed, for the first time ever, the processes that give rise to stars and planets in nascent solar systems.

The discoveries, appearing in the Astrophysical Journal, provide a better understanding of the way hydrogen gas from the protoplanetary disk is incorporated into the star.

By coupling both Keck telescopes on Mauna Kea in Hawaii with a specifically engineered instrument named ASTRA (ASTrometric and phase-Referenced Astronomy), University of Arizona astronomer Joshua Eisner and his colleagues were able to peer deeply into protoplanetary disks -swirling clouds of gas and dust that feed the growing star in its centre and eventually coalesce into planets and asteroids to form a solar system.

Combining the Keck interferometer with the spectro-astrometry technique, Eisner and his collaborators were able to distinguish between the distributions of gas, mostly made up of hydrogen, and dust, thereby resolving the disk””s features.

“We were able to get really, really close to the star and look right at the interface between the gas-rich protoplanetary disk and the star,” said Eisner, who serves as project scientist on the ASTRA team.

He added: “We want to understand how material accretes onto the star.

“This process has never been measured directly.” (ANI)

Astronomers see supernova from different angle

Washington, April 1 (ANI): A group of astronomers has observed an exploding star or supernova, which left behind what we know today as Cassiopeia A, from another angle as well as in a 3-D perspective.

Armin Rest of Harvard University and his colleagues have used a technique that has allowed them to observe Cassiopeia A from a perspective other than that from the Solar System.

“The same event looks different from different places in the Milky Way. For the first time, we can see a supernova from an alien perspective,” said lead author Armin Rest of Harvard University.

The technique that the astronomers used is based on the familiar echo concept, but instead of sound it is applied to light.

When dust clouds in space reflect the light from the supernova it bounces off them; by catching those reflections, the astronomers were able to capture the images on them.

Thus, by collecting reflections from various dust clouds in different areas of space, they composed images of Cassiopeia A that depicted different angles of the supernova.

Additionally, by grouping all the images from multiple angles together with X-ray data on the supernova remnants and the movement of the left over neutron star, the astronomers were able to get a 3-D perspective as well.

The team observed that the supernova looks very different when viewed from all the different angles, especially from one particular direction.

They found this to possibly be due to the supernova explosion sending gas out one way and the star the other. (ANI)

Runaway star may have spawned our solar system

London, March 31 (ANI): A team of scientists has theorized that a runaway star may have spawned our solar system.

Meteorites that contain bits of rock called calcium-aluminium-rich inclusions suggest that the solar system may have formed very quickly from the ashes of other stars.

That’s because the inclusions formed with the radioactive isotope aluminium-26, which is forged inside stars tens of times as massive as the sun and decays with a half-life of only 720,000 years.

Such massive stars tend to form in clusters, and they shed material in roiling winds that can cool down and seed planetary systems.

But, according to a report in New Scientist, Vincent Tatischeff of the National Center for Scientific Research in Orsay, France, and colleagues suspect a massive star cluster would have been have been so hot that most of the Al-26 would have decayed before planets could congeal.

Instead, they suggest the solar system sprang from a solitary star’s ashes, which could have cooled more quickly.

To account for the amount of Al-26 observed in meteorites, the star would still have had to be massive, meaning it probably formed in a clutch of other stars.

At some point, it may have been flung out of its birth cluster by gravitational tussles with its siblings or the explosion of a companion.

“The scenario may look complicated, but we think it is the most likely origin of the aluminium-26 in the solar system,” Tatischeff said.

As it zipped through interstellar space, the star would have released Al-26 in winds, forming a shell of material around it.

When the star later exploded, its remains would have slammed into this shell, creating a turbulent region with areas dense enough for the sun to form.

According to Tatischeff, most of the galaxy’s planetary systems may not have formed as quickly as ours, since many probably arose from clusters.

This makes them likely to have lower levels of Al-26, which generates heat as it decays.

The cooler temperatures may have led rocky planets to take a different evolutionary path to Earth, perhaps becoming ocean worlds. (ANI)

Newly discovered exoplanet may have water

Washington, March 19 (ANI): Scientists have suggested that the newly discovered planet Corot-9b is temperate enough to allow the presence of liquid water.

Corot-9b was found on 16 May 2008 and orbits its star every 95.274 days, a little longer than Mercury takes to go round the Sun.

It is the first transiting planet to have both a longer period and a near-circular orbit.

A transit is a kind of eclipse and occurs when a celestial body passes in front of its host star and blocks some but not all of the star’s light.

Corot-9b’s orbit is slightly elliptical but at closest approach to its parent star it reaches a distance of 54 million kilometers.

Although that is only about the distance of Mercury in our Solar System, it is by far the largest orbit of any transiting planet found so far.

Because it orbits a star cooler than our Sun, calculations estimate that Corot-9b’s temperature could lie somewhere between -23 degrees C and 157 degrees C.

Corot-9b has a radius around 1.05 times that of Jupiter but only 84 percent of the mass. This leads to a density of 0.90 g/cc, or 68 percent that of Jupiter.

“Corot-9b is the first exoplanet that is definitely similar to a planet in our Solar System,” said Hans Deeg, a researcher at the Instituto de Astrofisica de Canarias.

The similarity is caused by the fact that Corot-9b is sufficiently far from its star to prevent tidal forces from heating its interior.

Tidal forces are created by the strength of gravity weakening from the front to back of the celestial body.

When the difference between the near side and the far side is great, the tidal force can prevent the planet from spinning quickly, forcing it to only show one face to the star.

It can also provide heat to the interior of the planet, changing its physical condition.

Based on calculations, neither of these is possible in this case.

“Although we don’t know, because we can’t see the planet directly, there is reason to believe that this planet has a normal day-night cycle,” said Malcolm Fridlund, ESA Project Scientist for Corot.

It means that lacking a tidal heat source, Corot-9b’s interior is likely to have remained similar to the gas giants in our Solar System. (ANI)

Scientists make interior weather map of Jupiter’s giant storm system

Munich, March 17 (ANI): Using new ground-breaking thermal images obtained with ESO’s (European Southern Observatory’s) Very Large Telescope and other powerful ground-based telescopes, scientists have made the first detailed interior weather map of Jupiter’s giant storm system linking its temperature, winds, pressure and composition with its colour.

The images show swirls of warmer air and cooler regions never seen before within Jupiter’s Great Red Spot.

“This is our first detailed look inside the biggest storm of the Solar System,” said Glenn Orton, who led the team of astronomers that made the study.

“We once thought the Great Red Spot was a plain old oval without much structure, but these new results show that it is, in fact, extremely complicated,” he added.

The observations reveal that the reddest colour of the Great Red Spot corresponds to a warm core within the otherwise cold storm system, and images show dark lanes at the edge of the storm where gases are descending into the deeper regions of the planet.

The observations, detailed in a paper appearing in the journal Icarus, give scientists a sense of the circulation patterns within the solar system’s best-known storm system.

Sky gazers have been observing the Great Red Spot in one form or another for hundreds of years, with continuous observations of its current shape dating back to the 19th century.

The spot, which is a cold region averaging about -160 degrees Celsius, is so wide that about three Earths could fit inside its boundaries.

The thermal images were mostly obtained with the VISIR instrument attached to ESO’s Very Large Telescope in Chile, with additional data coming from the Gemini South telescope in Chile and the National Astronomical Observatory of Japan’s Subaru Telescope in Hawaii.

“One of the most intriguing findings shows the most intense orange-red central part of the spot is about 3 to 4 degrees warmer than the environment around it,” said lead author Leigh Fletcher.

This temperature difference might not seem like a lot, but it is enough to allow the storm circulation, usually counter-clockwise, to shift to a weak clockwise circulation in the very middle of the storm.

Not only that, but on other parts of Jupiter, the temperature change is enough to alter wind velocities and affect cloud patterns in the belts and zones.

“This is the first time we can say that there’s an intimate link between environmental conditions – temperature, winds, pressure and composition – and the actual colour of the Great Red Spot,” said Fletcher. (ANI)

New evidence points towards water on Moon

London, September 19 (ANI): Two separate lunar missions have found evidence which indicates that the polar regions of the moon are chock full of water-altered minerals.

According to a report in Nature News, early results from NASA’s Lunar Reconnaissance Orbiter (LRO), launched on June 18, are offering a wide array of watery signals.

The Moon, in fact, has water in all sorts of places: not just locked up in minerals, but scattered throughout the broken-up surface, and, potentially, in blocks or sheets of ice at depth.

“We are on the verge of a renaissance in our thinking about the poles of the Moon, including how water ice gets there,” said Anthony Colaprete, principal investigator for the Lunar Crater Observation and Sensing Satellite (LCROSS), which on October 9, will slam into a polar crater with the intention of ploughing up a plume of water ice for many telescopic eyes to see.

The initial LRO results confirm what was long suspected as a way for ice to stay trapped on the Moon for billions of years.

A thermal mapping instrument showed that permanently shadowed regions within deep polar craters are as cold as 35o Kelvin (-238o Celsius).

Project scientist Richard Vondrak said that they are the coldest spots in the Solar System – even colder than the surface of Pluto.

Variations in the flux of neutrons suggests variability in water content among craters.

But, the surprise comes from a different instrument on LRO, which counts slow-moving neutrons as a way of measuring hydrogen abundance in the top metre or so of the surface.

This hydrogen is often interpreted as a proxy for water ice, although it could also be molecular hydrogen or hydrogen trapped in other molecules.

The LRO instrument has already found a significant excess of hydrogen at the poles.

But, with added resolution, it is seeing surprising variability within the polar regions. Some of the craters appear enriched in hydrogen. Others are not.

Stranger still, some areas outside the crater walls, which were thought to get too hot for water to linger, show an excess of hydrogen.

Vondrak said this shows that the water could have arrived more recently, or that it can persist if buried as impacts till the lunar soil.

If the LCROSS impact spews up ice, it will eliminate the last vestiges of doubt about water on the Moon.

It could also start a new hunt: to find a record of impact events, such as water-rich comet strikes, that put the ice there in the first place. (ANI)

New evidence points towards water on Moon

London, September 19 (ANI): Two separate lunar missions have found evidence which indicates that the polar regions of the moon are chock full of water-altered minerals.

According to a report in Nature News, early results from NASA’s Lunar Reconnaissance Orbiter (LRO), launched on June 18, are offering a wide array of watery signals.

The Moon, in fact, has water in all sorts of places: not just locked up in minerals, but scattered throughout the broken-up surface, and, potentially, in blocks or sheets of ice at depth.

“We are on the verge of a renaissance in our thinking about the poles of the Moon, including how water ice gets there,” said Anthony Colaprete, principal investigator for the Lunar Crater Observation and Sensing Satellite (LCROSS), which on October 9, will slam into a polar crater with the intention of ploughing up a plume of water ice for many telescopic eyes to see.

The initial LRO results confirm what was long suspected as a way for ice to stay trapped on the Moon for billions of years.

A thermal mapping instrument showed that permanently shadowed regions within deep polar craters are as cold as 35o Kelvin (-238o Celsius).

Project scientist Richard Vondrak said that they are the coldest spots in the Solar System – even colder than the surface of Pluto.

Variations in the flux of neutrons suggests variability in water content among craters.

But, the surprise comes from a different instrument on LRO, which counts slow-moving neutrons as a way of measuring hydrogen abundance in the top metre or so of the surface.

This hydrogen is often interpreted as a proxy for water ice, although it could also be molecular hydrogen or hydrogen trapped in other molecules.

The LRO instrument has already found a significant excess of hydrogen at the poles.

But, with added resolution, it is seeing surprising variability within the polar regions. Some of the craters appear enriched in hydrogen. Others are not.

Stranger still, some areas outside the crater walls, which were thought to get too hot for water to linger, show an excess of hydrogen.

Vondrak said this shows that the water could have arrived more recently, or that it can persist if buried as impacts till the lunar soil.

If the LCROSS impact spews up ice, it will eliminate the last vestiges of doubt about water on the Moon.

It could also start a new hunt: to find a record of impact events, such as water-rich comet strikes, that put the ice there in the first place. (ANI)

Scientists find meteorite that came from innermost asteroid belt between Mars and Jupiter

Washington, September 18 (ANI): In a very rare finding, scientists have discovered an unusual kind of meteorite in the Western Australian desert and have uncovered that it came from the innermost main asteroid belt between Mars and Jupiter.

Meteorites are the only surviving physical record of the formation of our Solar System.

However, information about where individual meteorites originated, and how they were moving around the Solar System prior to falling to Earth, is available for only a dozen of around 1100 documented meteorite falls over the past two hundred years.

According to Dr Phil Bland from the Department of Earth Science and Engineering at Imperial College London, the lead author of the study, “We are incredibly excited about our new finding. Meteorites are the most analysed rocks on Earth, but it’s really rare for us to be able to tell where they came from.”

The new meteorite, which is about the size of cricket ball, is the first to be retrieved since researchers from Imperial College London, Ondrejov Observatory in the Czech Republic, and the Western Australian Museum, set up a trial network of cameras in the Nullarbor Desert in Western Australia in 2006.

The researchers aim to use these cameras to find new meteorites, and work out where in the Solar System they came from, by tracking the fireballs that they form in the sky.

The new meteorite was found on the first day of searching using the new network, by the first search expedition, within 100m of the predicted site of the fall.

The meteorite appears to have been following an unusual orbit, or path around the Sun, prior to falling to Earth in July 2007, according to the researchers’ calculations.

The team believes that it started out as part of an asteroid in the innermost main asteroid belt between Mars and Jupiter.

It then gradually evolved into an orbit around the Sun that was very similar to Earth’s.

The new meteorite is also unusual because it is composed of a rare type of basaltic igneous rock.

According to the researchers, its composition, together with the data about where the meteorite comes from, fits with a recent theory about how the building blocks for the terrestrial planets were formed.

This theory suggests that the igneous parent asteroids for meteorites like today’s formed deep in the inner Solar System, before being scattered out into the main asteroid belt.

Asteroids are widely believed to be the building blocks for planets like the Earth, so the new finding provides another clue about the origins of the Solar System. (ANI)

Scientists design “gravity tractor” to save earth from asteroids

London, Aug 30 (ANI): British space scientists have designed a special spacecraft that can save the earth from a catastrophic asteroid collision.

The 10 tonne spacecraft named “gravity tractor” would be deployed to intercept an asteroid en route to the earth and has the ability to fly 160 ft alongside it.

Once near an asteroid the craft will use gravitational force to pull the rock towards itself.

Gradually the gravity tractor will be able to change the asteroids path and thus make sure it misses the earth.

According to rough estimates of the American space agency NASA, there are more than 100,000 asteroids orbiting near the Earth and have the capacity to destroy cities.

The engineers of space company EADS Astrium, which designs crafts for NASA and the European Space Agency, have made the gravity tractor.

The team believes the craft could successfully divert the course of asteroids up to 430 yards across, which can release 100,000 times more than the Hiroshima bomb.

The Telegraph quoted Dr Ralph Cordey, science and exploration business development manager at Astrium as saying: “Anything bigger than 30m (32 yards) across is a real threat to the Earth.

“Unfortunately it is a matter of when rather than if one of them hits us.

“The gravity tractor exploits the principals of very basic physics – every object with a mass has its own gravity that affects objects around it. It can move fairly large objects 300 metres (984ft) to 400 metres (1,312ft) across.

“These asteroids are hurtling around our solar system at 10km per second, so when you scale that up, you just need a tiny nudge to send it off course.” (ANI)

Most successful and longest mission in spaceflight history to end

Washington, June 27 (ANI): The joint ESA/NASA solar orbiter Ulysses is slated to shut down operations on June 30, which would mark the end of one of the most successful and longest missions in spaceflight history.

After 18.6 years in space and defying several earlier expectations of its demise, Ulysses will achieve ‘end of mission’ on June 30. T

The final communication pass with a ground station will start at 17:35 CEST and run until 22:20 CEST on the above mentioned date or until the final command is issued to switch the satellite’s radio communications into ‘monitor only’ mode.

No further contact with Ulysses is planned.

Ulysses is the first spacecraft to survey the environment in space above and below the poles of the Sun in the four dimensions of space and time.

Among many other ground-breaking results, the hugely successful mission showed that the Sun’s magnetic field is carried into the Solar System in a more complicated manner than previously believed.

Particles expelled by the Sun from low latitudes can climb up to high latitudes and vice versa, even unexpectedly finding their way down to planets.

This is very important as regions of the Sun not previously considered as possible sources of hazardous particles for astronauts and satellites must now be taken into account and carefully monitored.

“Ulysses has taught us far more than we ever expected about the Sun and the way it interacts with the space surrounding it,” said Richard Marsden, ESA’s Ulysses Project Scientist and Mission Manager.

The shut-down of the satellite is a joint decision of the two agencies and comes a year after the mission was expected to end.

A year ago, the satellite’s power supply had weakened to the point that it was thought the low temperatures would cause the fuel lines to freeze up, rendering Ulysses uncontrollable.

It was decided to maintain the spacecraft in operation using NASA’s 70 m-diameter ground station network allocated on a ‘spare-capacity’ basis.

But as Ulysses has moved further from Earth, the communications bit-rate has gone down while other demands for the 70 m-diameter Deep Space Network stations have gone up.

Most importantly, the overall return of scientific data has decreased to a level where it is hard to justify the cost of keeping Ulysses in operation.

According to Paolo Ferri, Head of the Spacecraft Operations Solar and Planetary Missions Division. “Although it is always hard to take the decision to terminate a mission, we have to accept that the satellite is running out of resources and a controlled switch-off is the best ending.” (ANI)

Aliens do exist but US govt hides the truth, says ex-astronaut

London, April 22 (ANI): There is extraterrestrial life and it is being concealed by the United States government, claims ex-NASA astronaut Edgar Mitchell.itchell made the claims at the fifth annual X-Conference – a meeting of those who believe in UFOs and other life forms.

Mitchell, who was part of the 1971 Apollo 14 moon mission, said that alien life does exist but the truth is being covered up by the U.S. govt.

The 78-year-old also said that he had tried investigating the 1947 ‘Roswell Incident’, which some believe was the crash-landing of a UFO, but had been thwarted by military authorities.We’re not alone. Our destiny, in my opinion, and we might as well get started with it, is [to] become a part of the planetary community. … We should be ready to reach out beyond our planet and beyond our solar system to find out what is really going on out there,” the Telegraph quoted Mitchell as saying.

“I urge those who are doubtful: Read the books, read the lore, start to understand what has really been going on. Because there really is no doubt we are being visited. The universe that we live in is much more wondrous, exciting, complex and far-reaching than we were ever able to know up to this point in time,” Mitchell added.

A rep for NASA told CNN: “NASA does not track UFOs. NASA is not involved in any sort of cover-up about alien life on this planet or anywhere else – period.” (ANI)

‘Cannibalistic’ Jupiter gobbled up its early moons

London, March 9 (ANI): A computer simulation has indicated that the gas giant Jupiter was once a cannibal, in the sense that it ate many of its moons early in its history.

The four giant “Galilean” moons orbiting Jupiter are the last survivors of at least five generations of moons that once circled the planet.

“All the other moons – and there could have been 20 or more – were devoured by the planet in the early days of the solar system,” Robin Canup of the Southwest Research Institute in Boulder, Colorado, told New Scientist.

The four Galilean moons have played a key role in the history of science. Their discovery by Galileo 400 years ago provided irrefutable evidence that not all bodies orbited the Earth.

But until recently, nobody had suspected that Jupiter had once had many more moons.

“Astronomers have long been aware of a mystery thrown up by simulations of the way Jupiter and its moons formed,” said Canup.

These models indicate that the mass of the debris disc around Jupiter, from which the moons formed, was several tens of a per cent of the mass of giant planet; And yet only 2 per cent is enough to make the moons we see today.

Now, Canup and her colleague William Ward believe they know why. The extra mass can be explained if other moons formed while the debris disc was still present.

“A key process is therefore the interaction between the growing moons and the disc material still flowing in from the solar system,” said Canup.

This interaction would have caused the early moons to spiral in towards Jupiter and eventually be “eaten”.

According to Canup, this would explain the discrepancy in the earlier simulations, as one set of moons was swallowed, a new set immediately began to form.

“There could have been five generations of moons,” she said. “The current Galilean moons formed just as the inflow of material into the disc from the solar system choked off, so they escaped the fate of their unfortunate predecessors,” she added.

According to Canup and Ward, in each generation, the total mass of the moons was the same, but the number of moons could have varied.

“We think something similar happened around Saturn, where the last generation contained one giant moon – Titan,” said Canup.

This could have implications for the solar system as a whole. Rocky planets may take as long as 10 million years to aggregate, chunk by chunk. (ANI)

Cannibalistic Jupiter ate its early moons

THE four giant “Galilean” moons orbiting Jupiter are the last survivors of at least five generations of moons that once circled the gas giant.

“All the other moons – and there could have been 20 or more – were devoured by the planet in the early days of the solar system,” says Robin Canup of the Southwest Research Institute in Boulder, Colorado.

The four Galilean moons have played a key role in the history of science – their discovery by Galileo 400 years ago provided irrefutable evidence that not all bodies orbited the Earth. But until recently, nobody had suspected that Jupiter had once had many more moons.

Astronomers have long been aware of a mystery thrown up by simulations of the way Jupiter and its moons formed, says Canup. These models indicate that the mass of the debris disc around Jupiter, from which the moons formed, was several tens of a per cent of the mass of giant planet. And yet only 2 per cent is enough to make the moons we see today.

Now Canup and her colleague William Ward believe they know why. The extra mass can be explained if other moons formed while the debris disc was still present (www.arxiv.org/abs/0812.4995). “A key process is therefore the interaction between the growing moons and the disc material still flowing in from the solar system,” says Canup. This interaction would have caused the early moons to spiral in towards Jupiter and eventually be “eaten”.

This would explain the discrepancy in the earlier simulations, says Canup: as one set of moons was swallowed, a new set immediately began to form. “There could have been five generations of moons,” she says. “The current Galilean moons formed just as the inflow of material into the disc from the solar system choked off, so they escaped the fate of their unfortunate predecessors.”

According to Canup and Ward, in each generation the total mass of the moons was the same, but the number of moons could have varied. “We think something similar happened around Saturn, where the last generation contained one giant moon – Titan,” says Canup.

This could have implications for the solar system as a whole. Rocky planets may take as long as 10 million years to aggregate, chunk by chunk. The process continues long after the debris disc around the sun has blown away, so these planets would not have been at risk of spiralling inwards.

In contrast, the gaseous cores of gas giants like Saturn and Jupiter condense out of the solar debris disc very quickly via gas shrinkage. This means they would have had time to interact with the debris disc. John Papaloizou of the University of Cambridge says it is entirely conceivable that the sun may have swallowed numerous gas cores before the current stable configuration of the solar system emerged.

Iran backs nuclear energy for peaceful means

New Delhi, Feb 10 (ANI): Iran has said it retains the right to use nuclear energy for peaceful power generation.

Talking to reporters here on Monday, Iran’s Ambassador to India, Seyed Mehdi Nabizadeh, said any country had the right to develop energy sources.
“We have been trying our best for the development and progressive of the knowledge and technology. It has come from figure at time that we have been able to show Nano technology, bio technology as well esteem stem cell and technology of the neo energy wind as well as solar system and nuclear energy that we have been just going ahead,” Nabizadeh said.
Western powers said on Saturday that Iran risked isolation and more sanctions if it did not comply with demands to rein in its nuclear programme.

The U.N. Security Council has imposed three rounds of sanctions on Iran for refusing to suspend uranium enrichment. Western powers suspect the work is aimed at building an atomic bomb. Tehran says it is for peaceful power generation only.

Referring to attacks in Mumbai late last year in which nearly 200 people were killed, Nabizadeh said countries nurturing terrorist had a responsibility to rein them. (ANI)

Mineral kingdom has co-evolved with life on Earth

Washington : Scientists at the Carnegie Institution in the US have found that the mineral kingdom co-evolved with life, and that up to two thirds of the more than
4,000 known types of minerals on Earth can be directly or indirectly linked to biological activity.

Robert Hazen and Dominic Papineau of the Carnegie Institution”s Geophysical Laboratory, along with six colleagues, made the finding.

The team reviewed the physical, chemical, and biological processes that gradually transformed about a dozen different primordial minerals in ancient interstellar dust grains to the thousands of mineral species on the present-day Earth.

“We found both the variety and relative abundances of minerals have changed dramatically over more than 4.5 billion years of Earth”s history,” said Hazen.

All the chemical elements were present from the start in the solar system”s primordial dust, but they formed comparatively few minerals.

Only after large bodies such as the Sun and planets congealed did there exist the extremes of temperature and pressure required to forge a large diversity of mineral species.

Many elements were also too dispersed in the original dust clouds to be able to solidify into mineral crystals.

As the solar system took shape through “gravitational clumping” of small, undifferentiated bodies-fragments of which are found today in the form of meteorites-about 60 different minerals made their appearance.

Only on Earth did mineral evolution progress to the next stages.

A key factor was the churning of the planet”s interior by plate tectonics, the process that drives the slow shifting continents and ocean basins over geological time.

Unique to Earth, plate tectonics created new kinds of physical and chemical environments where minerals could form, and thereby boosted mineral diversity to more than a thousand types.

What ultimately had the biggest impact on mineral evolution, however, was the origin of life, approximately 4 billion years ago.

“Of the approximately 4,300 known mineral species on Earth, perhaps two thirds of them are biologically mediated,” said Hazen. “This is principally a consequence of our oxygen-rich atmosphere, which is a product of photosynthesis by microscopic algae,” he added.

Many important minerals are oxidized weathering products, including ores of iron, copper and many other metals.

Microorganisms and plants also accelerated the production of diverse clay minerals.

In the oceans, the evolution of organisms with shells and mineralized skeletons generated thick-layered deposits of minerals such as calcite, which would be rare on a lifeless planet.

“For at least 2.5 billion years, and possibly since the emergence of life, Earth”s mineralogy has evolved in parallel with biology,” said Hazen. “One implication of this finding is that remote observations of the mineralogy of other moons and planets may provide crucial evidence for biological influences beyond Earth,” he added. (ANI)

Hubble captures first image of planet circling another star

Hubble captures first image of planet circling another starWashington – The US space agency said Thursday its Hubble Space Telescope has captured the first image, taken in visible light, of a planet circling a star in another solar system.

The planet, Fomalhaut b, is estimated to have about three times the mass of Jupiter, the largest planet in our solar system. The image was taken as Fomalhaut b orbited the star Fomalhaut, which is located 25 light years from Earth in the constellation Piscis Australis or the Southern Fish.

It’s challenging to take such pictures as a star’s glare makes it almost impossible in visible light to see any orbiting planets. This forces astronomers to look for planets indirectly by measuring the gravitational influence on the star being orbited.

In the image released by the National Aeronautics and Space Administration (NASA), the planet appears as a tiny dot in the middle of a giant red dust ring of proto-planetary debris.

This large debris disk is similar to the Kuiper Belt, which circles the solar system and contains numerous icy bodies – dust grains and even objects the size of dwarf planets, such as Pluto in Earth’s own solar system.

“Our Hubble observations were incredibly demanding. Fomalhaut b is 1 billion times fainter than the star. We began this programme in 2001, and our persistence finally paid off,” Hubble astronomer Paul Kalas of the University of California at Berkeley said in a statement.

NASA said that Fomalhaut has been a candidate for planet hunting ever since the agency’s Infrared Astronomy Satellite discovered excessive dust around the star in the early 1980s.

In 2004, Kalas and his team discovered the debris disk that scatters Fomalhaut’s starlight. They later concluded that the ring of debris was being gravitationally modified by a planet lying between the star and the ring’s inner edge.

NASA confirmed that the planet is more than 17.2 billion kilometres from the star, or about 10 times the distance of Saturn from our sun. The alien planet is also brighter than expected for an object its size, probably because it has a Saturn-like ring of ice and dust that reflects starlight. (dpa)

NASA spacecraft all set explore the dynamic interactions in outer solar system

NASA spacecraft all set explore the dynamic interactions in outer solar systemWashington, Oct 7: The first NASA spacecraft to image and map the dynamic interactions taking place where the hot solar wind slams into the cold expanse of space in the outer solar system, is ready for launch on October 19.

The two-year mission will begin from the Kwajalein Atoll, a part of the Marshall Islands in the Pacific Ocean.

Called the Interstellar Boundary Explorer or IBEX, the spacecraft will conduct extremely high-altitude orbits above Earth to investigate and capture images of processes taking place at the farthest reaches of the solar system.

Known as the interstellar boundary, this region marks where the solar system meets interstellar space.

“The interstellar boundary regions are critical because they shield us from the vast majority of dangerous galactic cosmic rays, which otherwise would penetrate into Earth’s orbit and make human spaceflight much more dangerous,” said David J. McComas, IBEX principal investigator and senior executive director of the Space Science and Engineering Division at the Southwest Research Institute in San Antonio.

The story of the outer solar system began to unfold when the Voyager 1 and Voyager 2 spacecrafts left the inner solar system and headed out toward the boundary between our solar system and interstellar space.

“The Voyager spacecraft are making fascinating observations of the local conditions at two points beyond the termination shock that show totally unexpected results and challenge many of our notions about this important region,” said McComas.

Other spacecraft have continued the exploration of the interstellar boundary region.

Recently, a pair of NASA sun-focused satellites, the Solar Terrestrial Relations Observatory mission, detected a higher-energy version of the particles IBEX will observe in the heliosphere.

The heliosphere is an area that contains the solar wind. It stretches from the sun to a distance several times the orbit of Pluto.

IBEX is poised to thoroughly map this interstellar boundary region of the solar system.

The images will allow scientists to understand the global interaction between our sun and the galaxy for the very first time.

IBEX will be launched aboard a Pegasus rocket dropped from under the wing of an L-1011 aircraft flying over the Pacific Ocean. The Pegasus will carry the spacecraft approximately 130 miles above Earth and place it in orbit. (ANI)