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)

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)

Jupiter made comet its temporary moon for 12 years in mid-20th century

Washington, September 14 (ANI): An international team of astronomers has discovered that Jupiter had captured the comet 147P/Kushida-Muramatsu as its temporary moon in the mid-20th century, in an irregular orbit for about twelve years.

There are only a handful of known comets where this phenomenon of temporary satellite capture has occurred and the capture duration in the case of Kushida-Muramatsu, which orbited Jupiter between 1949 and 1961, is the third longest.

The phenomenon was detected by an international team led by Dr. Katsuhito Ohtsuka that modeled the trajectories of 18 “quasi-Hilda comets”, objects with the potential to go through a temporary satellite capture by Jupiter that results in them either leaving or joining the “Hilda” group of objects in the asteroid belt.

Most of the cases of temporary capture were flybys, where the comets did not complete a full orbit.

However, Dr. Ohtsuka’s team used recent observations tracking Kushida-Muramatsu over nine years to calculate hundreds of possible orbital paths for the comet over the previous century.

In all scenarios, Kushida-Muramatsu completed two full revolutions of Jupiter, making it only the fifth captured orbiter to be identified.

According to Dr. David Asher, “Our results demonstrate some of the routes taken by cometary bodies through interplanetary space that can allow them either to enter or to escape situations where they are in orbit around the planet Jupiter.”

Asteroids and comets can sometimes be distorted or fragmented by tidal effects induced by the gravitational field of a capturing planet, or may even impact with the planet.

The most famous victim of both these effects was comet D/1993 F2 (Shoemaker-Levy 9), which was torn apart on passing close to Jupiter and whose fragments then collided with that planet in 1994.

Previous computational studies have shown that Shoemaker-Levy 9 may well have been a quasi-Hilda comet before its capture by Jupiter.

“Fortunately for us Jupiter, as the most massive planet with the greatest gravity, sucks objects towards it more readily than other planets and we expect to observe large impacts there more often than on Earth,” said Dr. Asher.

“Comet Kushida-Muramatsu has escaped from the giant planet and will avoid the fate of Shoemaker-Levy 9 for the foreseeable future”, he added. (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)

Minerals on ancient Martian rock formed in a habitable environment

London, August 29 (ANI): A new analysis has suggested that a rock found on Mars in 1996, which was claimed by scientists to host life, has minerals which could have only been formed in a habitable environment.

Researchers led by David McKay of NASA’s Johnson Space Center in Houston, Texas, caused a sensation 13 years ago when they proposed that a chunk of Mars rock found in Antarctica, called ALH 84001, contained possible signs of past life on the Red Planet, including complex carbon-based molecules and some microscopic objects shaped like bacteria.

But, the claim was never widely accepted.

Other scientists countered that the shapes were ambiguous and that the complex carbon-based molecules could have been produced without life, since they are also found in chunks of asteroids that fall to Earth as meteorites, for example.

Some argued that the carbon in the meteorite could have been deposited in very harsh conditions, involving water at more than 150 degrees Celsius.

Even the hardiest known terrestrial microbes die above about 120 degrees C.

But, according to a report in New Scientist, a new analysis suggests that the water involved was cool enough to allow for life, which at least keeps open the possibility of fossilized life in the meteorite.

The study was led by Paul Niles of NASA Johnson. Neither he nor any of the other team members were part of the 1996 life claim.

To explain deposits of minerals containing calcium, magnesium, and iron, in the rock, Niles and his colleagues suggest the rock was sitting at or near the surface of Mars, with water rich in carbon dioxide bubbling up to the surface in the area from deep underground, perhaps as part of a hot spring.

The relative amounts of the three metals deposited from solution depend on the temperature of the water they were dissolved in.

The team used previous measurements of these amounts to calculate a water temperature of less than 100 degrees C.

This was not a certainty beforehand, since water can remain liquid above that temperature at the higher pressures underground.

“These minerals were formed in what is very likely to have been a habitable environment,” Niles said.

The study shows there is still more to learn from what is “probably the single most examined rock in all of human history,” said Marc Fries of NASA’s Jet Propulsion Laboratory in Pasadena, California. (ANI)

Scientists find ‘stopwatch for the solar system’

London, August 26 (ANI): In a new study, a team of scientists has described how aluminium radioisotopes can now offer precise timing of events 4.5 billion years ago, and thus have been dubbed as the ‘stopwatch for the solar system’.

According to a report by BBC News, the study shows that the rate of decay of isotopes can now be relied upon to give accurate measures of time for that period.

It is hoped that this will give new insights into how the Solar System formed in its first five million years.

The scientists showed how aluminium radioisotopes were uniformly distributed in the region where the Solar System was formed.

As the isotopes decayed steadily across the early Solar System, this allows their use as a type of clock for that period.

“We can now use the isotopes to measure the age of different chondrules, parts of meteorites, and understand far more about the early part of our Solar System,” one of the scientists, Johan Villeneuve, told BBC News.

The findings could also shed light on the origins of the planets.

Philip Bland, from Imperial College London, described the research as “a really nice study”.

“With their high precision measurements, they are able to date formation times for chondrules very precisely,” he said.

“And what is interesting is that they’ve shown that these building blocks for asteroids, and possibly for planets as well, formed over an extended period of two to three million years,” he added. (ANI)

Asteroids may have flocked together to build planets

London, August 18 (ANI): New computer simulations have suggested that dense swarms of asteroids collapsed under their own gravity to make the building blocks of the planets in our solar system.

The planets are thought to have formed from a disc of dust and gas around the infant sun.

The initial process is well known: dust grains clumped together, forming objects in the millimetre-to-metre range.

However, it is not known how the growth process continued.

The gas in the disc should have put a drag on the new boulders, causing them to spiral into the sun before they could grow further.

According to a report in New Scientist, evidence is now mounting that the next step was a sudden leap forward, skipping intermediate sizes to make asteroids hundreds of kilometers across – massive enough to resist gas drag.

Asteroids hundreds of kilometers across appeared – too massive to be dragged into the sun

This basic idea is decades old, but it attracted renewed attention in 2007 and 2008 following simulations by a team led by Anders Johansen of the Max Planck Institute for Astronomy in Heidelberg, Germany, and by another team led by Jeffrey Cuzzi of NASA’s Ames Research Center in Moffett Field, California.

These showed that turbulence in the nebula could have concentrated objects less than a meter across in dense enough swarms to collapse under their mutual gravity and form large asteroids tens to hundreds of kilometers across.

“If either one of these models turns out to be right, this will be a big step forward,” said John Chambers of the Carnegie Institution in Washington DC.

Now, a new study has found evidence that such a process did occur in our solar system. It is based on the size of objects in the asteroid belt.

Estimates from telescopic surveys suggest there are millions of the smallest asteroids, which are less than a kilometer across, with the numbers of larger ones dropping off sharply.

Yet this size distribution and number would once have been different: asteroids can grow by sweeping up smaller objects, and shatter if they collide with an object of similar size.

Alessandro Morbidelli of the Cote D’Azur Observatory in Nice, France, led a team that simulated the evolution of the asteroid belt, modelling a variety of starting populations.

They did find a good fit when they started with a mixture of sizes between 100 and 1000 kilometers across, suggesting that large asteroids did form spontaneously during the solar system’s development. (ANI)

U.S. study shows asteroids may have accelerated life on

WASHINGTON, May 20 (Xinhua) — A NASA-funded study indicates that an intense asteroid bombardment nearly 4 billion years ago may not have sterilized the early Earth as completely as previously thought, while the asteroids possibly even provided a boost for early life.

The study focused on a particularly cataclysmic occurrence known as the Late Heavy Bombardment, or LHB. This event occurred approximately 3.9 billion years ago and lasted 20 to 200 million years. In a letter to be published Thursday in Nature, Oleg Abramov and Stephen J. Mojzsis, astrobiologists at the University of Colorado’s Department of Geological Sciences, report on the results of a computer modeling project designed to study the heating of Earth by the bombardment.

Results from their project show that while the Late Heavy Bombardment might have generated enough heat to sterilize Earth’s surface, microbial life in subsurface and underwater environments almost certainly would have survived.

“Exactly when life originated on Earth is a hotly debated topic,” said Michael H. New, the astrobiology discipline scientist and manager of the Exobiology and Evolutionary Biology Program at NASA Headquarters in Washington.

“These findings are significant because they indicate that if life had begun before the LHB or some time prior to 4 billion years ago, it could have survived in limited refuges and then expanded to fill our world,” New said.

“Our new results point to the possibility life could have emerged about the same time that evidence for our planet’s oceans first appears,” said Mojzsis, principal investigator of the project.

A growing scientific consensus is that during our solar system’s formation, planetary bodies were pummeled by debris throughout the Late Heavy Bombardment. A visual record of the event is preserved in the form of the scarred face of our moon. On Earth, all traces of the bombardment appear to have been erased by rock recycling forces like weathering, volcanoes or other conditions that cause the crust to move or change.

Surface habitats for microbial life on early Earth would have been destroyed repeatedly by the bombardment. However, at the same time, impacts could have created subsurface habitats for life, such as extensive networks of cracks or even hydrothermal vents. Any existing microbial life on Earth could have found refuge in these habitats. If life had not yet emerged on Earth by the time of the bombardment, these new subsurface environments could have been the place where terrestrial life emerged.

“Even under the most extreme conditions we imposed on our model, the bombardment could not have sterilized Earth completely,” said Abramov, lead author of the paper. “Our results are in line with the scientific consensus that hyperthermophilic, or ‘heat-loving,’ microbes could have been the earliest life forms on Earth, or survivors from an even more ancient biosphere. The results also support the potential for the persistence of microbial biospheres on other planetary bodies whose surfaces were reworked by the bombardment, including Mars.”

Study turns back clock on origins of life on Earth

Study turns back clock on origins of life on EarthA heavy bombardment by asteroids the size of Ireland was not enough to wipe out life on Earth 3.9 billion years ago, researchers said on Wednesday in a finding that turns back the clock of life by 500 million years.

Many scientists had thought the violent pelting by massive asteroids during the period known as the Late Heavy Bombardment would have melted the Earth’s crust and vaporized any life on the planet.

But new three-dimensional computer models developed by a team at the University of Colorado at Boulder shows much of Earth’s crust, and the microbes living on it, could have survived and may even have thrived.

“These new results push back the possible beginnings of life on Earth to well before the bombardment period 3.9 billion years ago,” said Oleg Abramov, a researcher at the university whose study appears in the journal Nature.

“It opens up the possibility that life emerged as far back as 4.4 billion years ago, about the time the first oceans are thought to have formed,” Abramov said in a statement.

To study this period, Abramov and colleague Stephen Mojzsis used data from moon rocks, meteorite samples and the dented surfaces of neighboring planets to develop a three-dimensional model of this period of bombardment.

“What we did was recreate the Late Heavy Bombardment on a computer,” Abramov said, adding that the simulation randomly “smacked the Earth” with giant asteroids.

The team then looked at the impact that would have had on the Earth’s temperature in the so-called geophysical habitable zone — a zone representing the top 2.5 miles (4 km) of the Earth’s crust.

Based on these models, Abramov said this sustained period of impacts would have killed any life on the Earth’s surface, but not all life on Earth, as many had assumed.

“We find it is essentially impossible to sterilize the entire habitable zone of the Earth by this kind of bombardment,” Abramov said in a telephone interview.

“Certainly, the surface of the Earth was sterilized repeatedly,” he said.

But he said hydrothermal vents below the surface of the Earth may have offered sanctuaries for certain heat-loving microbes, and may have even provided a kind of incubator for life.

He said many scientists had thought that a cataclysmic bombardment event would have sterilized the planet and life would have had to start anew.

“The important thing about these results is they push back the possible beginnings of life as we know it,” he said.

“Exactly when life originated on Earth is a hotly debated topic,” said Michael New, an astrobiologist at the National Aeronautics and Space Administration, which sponsored the research.

“These findings are significant because they indicated life could have begun well before the Late Heavy Bombardment, during the so-called Hadean Eon of Earth’s history 3.8 billion to 4.5 billion years ago,” New said in a statement.

Asteroids may have boosted life on Earth 3.9 billion years ago

Washington, May 21 (ANI): A new study has indicated that the bombardment of Earth by asteroids 3.9 billion years ago may have enhanced early life rather then wipe it out.

The study, by University of Colorado at Boulder researchers, determined that the bombardment of Earth nearly 4 billion years ago by asteroids as large as the US state of Kansas would not have had the firepower to extinguish potential early life on the planet and may even have given it a boost.

Impact evidence from lunar samples, meteorites and the pockmarked surfaces of the inner planets paints a picture of a violent environment in the solar system during the Hadean Eon 4.5 to 3.8 billion years ago, particularly through a cataclysmic event known as the Late Heavy Bombardment about 3.9 million years ago.

Although many believe the bombardment would have sterilized Earth, the new study shows it would have melted only a fraction of Earth’s crust, and that microbes could well have survived in subsurface habitats, insulated from the destruction.

“These new results push back the possible beginnings of life on Earth to well before the bombardment period 3.9 billion years ago,” said CU-Boulder Research Associate Oleg Abramov.

“It opens up the possibility that life emerged as far back as 4.4 billion years ago, about the time the first oceans are thought to have formed,” he added.

The researchers used data from Apollo moon rocks, impact records from the moon, Mars and Mercury, and previous theoretical studies to build three-dimensional computer models that replicate the bombardment.

Abramov and CU-Boulder geological sciences Professor Stephen Mojzsis plugged in asteroid size, frequency and distribution estimates into their simulations to chart the damage to the Earth during the Late Heavy Bombardment, which is thought to have lasted for 20 million to 200 million years.

The 3-D models allowed Abramov and Mojzsis to monitor temperatures beneath individual craters to assess heating and cooling of the crust following large impacts in order to evaluate habitability.

The study indicated that less than 25 percent of Earth’s crust would have melted during such a bombardment.

“Even under the most extreme conditions we imposed, Earth would not have been completely sterilized by the bombardment,” said Abramov.

Instead, hydrothermal vents may have provided sanctuaries for extreme, heat-loving microbes known as “hyperthermophilic bacteria” following bombardments, said Mojzsis.

Even if life had not emerged by 3.9 billion years ago, such underground havens could still have provided a “crucible” for life’s origin on Earth, Mojzsis added. (ANI)

‘Chevrons’ are not evidence of megatsunamis, say scientists

Washington, April 30 (ANI): A new research has refuted the hypothesis that ‘chevrons’, large U- or V-shaped formations found in some of the world’s coastal areas, are evidence of megatsunamis caused by asteroids or comets slamming into the ocean.

The research was done by University of Washington (UW) geologist and tsunami expert Jody Bourgeois.

The term “chevron” was introduced to describe large dunes shaped something like the stripes one might see on a soldier’s uniform that are hundreds of meters to a kilometer in size and were originally found in Egypt and the Bahamas.

But, the discovery of similar forms in Australia and Madagascar led some scientists to theorize that they were, in fact, deposits left by huge tsunami waves, perhaps 10 times larger than the devastating Indian Ocean tsunami of December 2005.

Such huge waves, they suggest, would result from the giant splash of an asteroid or comet hitting the ocean.

They also suggest one such impact occurred 4,800 to 5,000 years ago, and that chevrons in Australia and Madagascar point to its location in the Indian Ocean.

But, Bourgeois said the theory just doesn’t hold water.

For example, she said, there are numerous chevrons on Madagascar, but many are parallel to the coastline.

Models created by Bourgeois’ colleague Robert Weiss show that if they were created by tsunamis, they should point in the direction the waves were travelling, mostly perpendicular to the shore.

“And if it really was from an impact, you should find evidence on the coast of Africa too, since it is so near,” said Bourgeois, a UW professor of Earth and space sciences who has studied earthquakes and tsunamis in various parts of the world.

The scientists used an online program called Google Earth, made up of satellite images of the Earth’s surface, to get close-up looks at chevrons in different locations.

Chevrons often are found in coastal areas, but they also are common in semiarid areas inland.

For the research, Weiss created a computer model that generated actual conditions that would occur during a tsunami.

The scientists then used the model to examine what would happen if an asteroid or comet hit in the area theorized by the megatsunami proponents.

The model showed the wave approach would be at a 90-degree orientation to the chevron deposits. But, if the megatsunami interpretation is correct, the chevrons should be parallel to wave approach.

“That’s just not the case here. The model shows such a tsunami could not have created these chevrons, unless you have some unimaginable process at work,” Bourgeois said. (ANI)

‘Chevrons’ are not evidence of megatsunamis, say scientists

Washington, April 30 (ANI): A new research has refuted the hypothesis that ‘chevrons’, large U- or V-shaped formations found in some of the world’s coastal areas, are evidence of megatsunamis caused by asteroids or comets slamming into the ocean.

The research was done by University of Washington (UW) geologist and tsunami expert Jody Bourgeois.

The term “chevron” was introduced to describe large dunes shaped something like the stripes one might see on a soldier’s uniform that are hundreds of meters to a kilometer in size and were originally found in Egypt and the Bahamas.

But, the discovery of similar forms in Australia and Madagascar led some scientists to theorize that they were, in fact, deposits left by huge tsunami waves, perhaps 10 times larger than the devastating Indian Ocean tsunami of December 2005.

Such huge waves, they suggest, would result from the giant splash of an asteroid or comet hitting the ocean.

They also suggest one such impact occurred 4,800 to 5,000 years ago, and that chevrons in Australia and Madagascar point to its location in the Indian Ocean.

But, Bourgeois said the theory just doesn’t hold water.

For example, she said, there are numerous chevrons on Madagascar, but many are parallel to the coastline.

Models created by Bourgeois’ colleague Robert Weiss show that if they were created by tsunamis, they should point in the direction the waves were travelling, mostly perpendicular to the shore.

“And if it really was from an impact, you should find evidence on the coast of Africa too, since it is so near,” said Bourgeois, a UW professor of Earth and space sciences who has studied earthquakes and tsunamis in various parts of the world.

The scientists used an online program called Google Earth, made up of satellite images of the Earth’s surface, to get close-up looks at chevrons in different locations.
Chevrons often are found in coastal areas, but they also are common in semiarid areas inland.

For the research, Weiss created a computer model that generated actual conditions that would occur during a tsunami.

The scientists then used the model to examine what would happen if an asteroid or comet hit in the area theorized by the megatsunami proponents.

The model showed the wave approach would be at a 90-degree orientation to the chevron deposits. But, if the megatsunami interpretation is correct, the chevrons should be parallel to wave approach.

“That’s just not the case here. The model shows such a tsunami could not have created these chevrons, unless you have some unimaginable process at work,” Bourgeois said. (ANI)

Asteroids age quickly because of a ‘sun tan’

Munich, April 23 (ANI): A new study has revealed that asteroid surfaces age and redden much faster than previously thought – in less than a million years, all thanks to solar winds.

“Asteroids seem to get a ‘sun tan’ very quickly,” said lead author Pierre Vernazza. “But not, as for people, from an overdose of the Sun’s ultraviolet radiation, but from the effects of its powerful wind,” he added.

It has long been known that asteroid surfaces alter in appearance with time.

The observed asteroids are much redder than the interior of meteorites found on Earth, but the actual processes of this “space weathering” and the timescales involved were controversial.

Thanks to observations of different families of asteroids using ESO’s New Technology Telescope at La Silla and the Very Large Telescope at Paranal, as well as telescopes in Spain and Hawaii, Vernazza’s team have now solved the puzzle.

When two asteroids collide, they create a family of fragments with “fresh” surfaces.

The astronomers found that these newly exposed surfaces are quickly altered and change color in less than a million years – a very short time compared to the age of the Solar System.

“The charged, fast moving particles in the solar wind damage the asteroid’s surface at an amazing rate,” said Vernazza.

Unlike human skin, which is damaged and aged by repeated overexposure to sunlight, it is, perhaps rather surprisingly, the first moments of exposure (on the timescale considered) – the first million years – that causes most of the aging in asteroids.

By studying different families of asteroids, the team has also shown that an asteroid’s surface composition is an important factor in how red its surface can become.

After the first million years, the surface “tans” much more slowly. At that stage, the color depends more on composition than on age.

Moreover, the observations reveal that collisions cannot be the main mechanism behind the high proportion of “fresh” surfaces seen among near-Earth asteroids.

Instead, these “fresh-looking” surfaces may be the results of planetary encounters, where the tug of a planet has “shaken” the asteroid, exposing unaltered material.

Thanks to these results, astronomers will now be able to understand better how the surface of an asteroid, which often is the only thing we can observe, reflects its history. (ANI)

Scientists glimpse ‘end of the world’ by analyzing dying stars

London, April 20 (ANI): A research into dying stars that once blazed as brightly as the Sun has revealed a glimpse of the ‘end of the world’, which awaits the Earth billions of years from now.

According to a report in The Times, a team led by Jay Farihi, of the University of Leicester, UK, did the research.

The astronomers discovered that at least one in 100 white dwarfs the burnt-out remnants of Sun-like stars – once had solar systems, with planets that were destroyed or deep-frozen by the death throes of their stars.

The research suggests millions of other solar systems have endured the destiny predicted for the Earth when the Sun dies.

When stars like the Sun die, they swell into red giants.

When the process begins for the Sun in approximately 4 billion years, it will fill much of the inner solar system; most calculations suggest the Earth will be engulfed.

Once red giants burn themselves out, they collapse into much smaller bodies, known as white dwarfs.

These dying stars no longer sustain themselves with nuclear fusion, and glow only because of their residual heat as they cool over billions of years.

Using NASA’s Spitzer Space Telescope, the team analyzed the gassy atmospheres around existing white dwarfs, some of which contain particles of dust.

They found that the dust is made from the same basic materials as asteroids and rocky planets.

It suggests that the debris could be the remains of Earth-like planets, which were engulfed by a swelling red giant before it turned into a white dwarf.

“What we have seen is a possible fate for our own solar system,” said Dr Farihi. “Many of the systems we are studying will have been similar to our own. It’s a possibility that some of them ould once have held life,” he added. (ANI)

“Noise” from space may help reveal mass of near-Earth asteroids

Washington, April 4 (ANI): Planetary scientists are all set to turn “noise” from the data obtained by NASA/ESA LISA satellites’ mission into useful information about the mass of near-Earth asteroids.

LISA is on a mission to detect gravitational waves – a warping of the space/time continuum that scientists hope to see directly for the first time.

Slated for launch no earlier than 2018, LISA will include three satellites connected by laser beams. The distance between the satellites should change as a gravitational wave passes.

Einstein’s General Theory of Relativity predicts that gravitational waves from exploding stars or colliding black holes ripple across the universe, causing other bodies to wobble like driftwood in a motorboat’s wake.

In 2006, planetary scientists realized that Near Earth Asteroids (NEAs) also would make the spacecraft wobble as they passed nearby, creating a distinct signature in the data being collected.

Pasquale Tricarico, a scientist at the Tucson-based Planetary Science Institute, expanded on that work to predict the number of asteroid encounters LISA can expect and how those encounters can be used to determine the mass of passing asteroids.

According to Tricarico, LISA can expect to see one or two known near-Earth asteroids a year, and a total of around ten during the expected mission lifetime.

When an encounter with a known asteroid shows up in the data, scientists will already know its trajectory.

“So from the signal, we can indirectly measure the asteroid’s mass because that’s the only uncertainty in the equation,” Tricarico said.

“These mass measurements are important because we only know the mass of asteroids that have been visited by spacecraft or the mass of a few binary asteroids observed from Earth,” he added.

“We always wonder about the porosity, the density, and this will give us measurements from additional asteroids,” he explained.

If a known asteroid passes one of the satellites and doesn’t leave a signature, “that allows us to put an upper limit on the mass of that asteroid,” Tricarico added.

Tricarico also has predicted the number of potential encounters with smaller, unknown NEAs.

If LISA starts detecting five asteroids a year instead of two or three, this could modify theories concerning the distribution of sizes in the NEA population. (ANI)

Giant salt lakes could have triggered off largest mass extinction in history

Berlin, March 31 (ANI): An international team of scientists has suggested that the largest known mass extinction in the history of the earth could have been triggered off by giant salt lakes, whose emissions of halogenated gases changed the atmospheric composition so dramatically that vegetation was irretrievably damaged.

At the Permian/Triassic boundary, 250 million years, ago about 90 percent of the animal and plant species ashore became extinct.

Previously, it was thought that volcanic eruptions, the impacts of asteroids, or methane hydrate were instigating causes.

The new theory is based on a comparison with today’s biochemical and atmospheric chemical processes.

“Our calculations show that airborne pollutants from giant salt lakes like the Zechstein Sea must have had catastrophic effects at that time,” said co-author Dr. Ludwig Weibflog from the Helmholtz-Center for Environmental Research (UFZ).

The team of researchers from Russia, Austria, South Africa and Germany investigated whether a process that has been taking place since primordial times on earth could have led to global mass extinctions, particularly at the end of the Permian.

The starting point for this theory was their discovery in the south of Russia and South Africa that microbial processes in present-day salt lakes naturally produce and emit highly volatile halocarbons such as chloroform, trichloroethene, and tetrachloroethene.

They transcribed these findings to the Zechstein Sea, which about 250 million years ago in the Permian Age, was situated about where present day Central Europe is.

Based on comparable calculations from halogenated gas emissions in the atmosphere from present-day salt seas in the south of Russia, the scientists calculated that from the Zechstein Sea alone an annual VHC emissions rate of at least 1.3 million tonnes of trichloroethene, 1.3 million tonnes of tetrachloroethene, 1.1 million tonnes of chloroform as well as 0.050 million tonnes of methyl chloroform can be assumed.

“Using steppe plant species we were able to prove that halogenated gases contribute to speeding up desertification: The combination of stress induced by dryness and the simultaneous chemical stressor ‘halogenated hydrocarbons’ disproportionately damages and destabilize the plants and speeds up the process of erosion,” Dr. Karsten Kotte from the University of Heidelberg explained.

Based on both of these findings the researchers were able to form their new hypothesis.

At the end of the Permian Age, the emissions of halogenated gases from the Zechstein Sea and other salt seas were responsible in a complex chain of events for the world’s largest mass extinction in the history of the earth, in which about 90 percent of the animal and plant species of that time became extinct. (ANI)

How to save Earth from an asteroid impact

London, March 27 (ANI): Scientists have used a virtual model to investigate options to save the Earth from an asteroid impact.

According to a report in New Scientist, the model was developed by a team led by David Dearborn of the Lawrence Livermore National Laboratory in California, which modelled the impact of a nuclear explosion on an asteroid’s trajectory.

It is based on the option of gently nudging the asteroid away from Earth without breaking it apart, either by exploding a nuclear device at a distance or zapping it with high-powered lasers.

The team’s virtual asteroid was 1 kilometer in diameter and made of rocky rubble loosely bound together by gravity, which is considered by many planetary scientists to be the most likely composition for small asteroids.

Thirty years before the asteroid was set to collide with Earth, a nuclear blast, equivalent to 100 kilotonnes of TNT, was set off 250 meters behind it.

The nudge from the explosion increased its velocity by 6.5 millimeters per second, a slight change but enough for it to miss us.

The technique also reduced the risk of a break-up.

Just 1 per cent of the asteroid’s material was dislodged by the blast, and of that only about 1 part in a million remained on a collision course with Earth.

Dearborn adds that the technology for this method is already established, unlike for the use of a heavy object to shove the asteroid onto a different path – the “kinetic impactor” strategy.

“Should an emergency arise, we should know that the technology is available, and we should have some idea of how to properly use it,” he said.

He has now begun simulating the effect of nudging an asteroid with a smaller nuclear explosion – less than 1 kilotonne – 1 meter below its surface.

This would reduce the device’s weight, making it easier and quicker to launch. (ANI)

Studying asteroid before impact may lead to advance warning system for Earth

London, March 26 (ANI): Astronomers, for the first time, have observed a rare asteroid as it was hurtling towards our planet and have captured the only spectrum of it before it exploded in our atmosphere, which may lead to an advanced warning system for Earth.

The observation was made by UK astronomers, using the Science and Technology Facilities Council’s (STFC) William Herschel Telescope on La Palma.

The asteroid in question – 2008 TC3 – an 80 ton, 4 meter asteroid with a rare composition, was first sighted by US telescopes on 6th October 2008.

Subsequent observations by an international army of professional and amateur astronomers led to the discovery that it was racing towards our planet and was due to enter the atmosphere the following morning.

“This was the first ever predicted impact of an asteroid with the Earth and the very first time an asteroid of any size has been studied before impact,” said Professor Alan Fitzsimmons, from the Queen’s University Belfast.

“The faint observed brightness implied a small size, which in turn meant there was little advance warning,” he added.

According to Fitzsimmons, “It was important to try and figure out what type of asteroid it was before impact, which would give us a better idea of its size and where it came from.”

“This event shows we can successfully predict the impact of asteroids even with a short warning time, and obtain the astronomical observations necessary to estimate what will happen when the asteroid reaches us,” he said.

The spectrum gathered by the UK astronomers allowed them to obtain information on the size and composition of the asteroid and to establish the first direct link between an asteroid and the individual meteorites produced as it breaks up in our atmosphere.

Not only does this help to validate the whole process of remotely surveying asteroids, but comparing the asteroid and meteorite data tells us that 2008 TC3 may have only spent a few million years existing in the Inner Solar system before it hit our planet.

“This asteroid was made of a particularly fragile material that caused it to explode at a high 37 km altitude, before it was significantly slowed down, so that the few surviving fragments scattered over a large area,” explained Dr. Peter Jenniskens of the SETI institute in California.

“The recovered meteorites were unlike anything in our meteorite collections up to that point,” he added. (ANI)

Watery asteroids may explain why life is ‘left-handed’

London, March 17 (ANI): A new study has suggested that watery asteroids hurtling through the solar system gave a boost to left-handed proteins on Earth, which explains why life on our planet is ‘left-handed’.

Curiously, almost every living organism on Earth uses left-handed amino acids instead of their right-handed counterparts.

According to a report in New Scientist, the new research suggests that water on asteroids amplified left-handed amino acid molecules, making them dominate over their right-handed mirror images.

In the 1990s, scientists found that meteorites contain up to 15 percent more of the left version too.

That suggests space rocks bombarding the early Earth biased its chemistry so that life used left-handed amino acids instead of right.

“Meteorites would have seeded the Earth with some of the prebiotic compounds like amino acids that are needed to get life started, and also biased the origin of life to the left-handed amino acid form,” said Daniel Glavin at NASA’s Goddard Space Flight Center in Greenbelt, Maryland.

Some have suggested that polarized starlight preferentially destroyed right-handed amino acids on asteroids.

But, this alone couldn’t explain why the meteorite bias is so strong.

Now, Glavin and colleague Jason Dworkin have shown that water amplified the asymmetry.

They studied an amino acid called isovaline in six meteorites that showed evidence of ancient exposure to liquid water for about 1000 to 10,000 years.

The longer water persisted in the rock, the stronger its left-handed isovaline bias, the team found. (ANI)

Asteroid dust in and around dead stars hints at Earth-like planets

London, Jan 7 (ANI): Scientists have observed asteroid dust in and around a handful of dead stars, that is made up of similar materials as the Earth, which suggests Earth-like planets may be common in the Universe.

According to a report in New Scientist, six white dwarfs, the burned-out embers of Sun-like stars, showed heavy elements, or metals, in their atmospheres.

That is unusual because white dwarfs contain about as much mass as the Sun squeezed into bodies the size of the Earth, giving them surface gravities 10,000 times stronger than the Sun’s.

That should cause heavy elements to sink towards their centres – and out of sight.

In addition, the six stars also shine more brightly than expected in infrared light, which suggests the stars are surrounded by dust, which glows at infrared wavelengths.

The dusty debris is thought to be the remains of asteroids that once orbited the white dwarfs, but were gravitationally torn apart when they wandered too close to the stars.

Michael Jura of the University of California, Los Angeles, and colleagues measured the infrared light from these stars using NASA’s Spitzer Space Telescope.

The team found the dust contains a glassy silicate material similar to olivine, which is common on Earth and has also been seen on the Moon and Mars.

The dust also seems to have no carbon, consistent with Earth’s composition, which has little carbon compared to the Sun.

Two previously studied white dwarfs have dust of a similar composition, bringing the tally of such stellar gluttons up to eight.

“What was once kind of a freak is now a systematic pattern,” Jura said.

Since asteroids form in the same way as planets, by bulking up through collisions between smaller rocky objects, they have a similar composition to their larger brethren.

That suggests terrestrial planets might have once existed in these systems. “This strengthens suspicions that Earth-like planets are common,” Jura said. (ANI)