Diamond Planets.

Cover Image: January 2013 Scientific American Magazine See Inside

Carbon Planets Turn Earth’s Chemistry on Its Head

Scientists have discovered exoplanets where carbon, relatively rare on Earth, might be as common as dirt

rendering of  55 Cancrie, exoplanets, earth's chemistry Image: Ron Miller
The study of exoplanets—worlds orbiting distant stars—is still in its early days. Yet already researchers have found hundreds of worlds with no nearby analogue: giants that could steamroll Jupiter; tiny pebbles broiling under stellar furnaces; puffy oddballs with the density of peat moss. Still other exoplanets might look familiar in broad-brush, only to reveal a topsy-turvy realm where rare substances are ordinary, and vice versa.
Take carbon, for instance: the key constituent of organic matter accounts for some of humankind's most precious materials, from diamonds to oil. Despite its outsize importance, carbon is uncommon—it makes up less than 0.1 percent of Earth's bulk.
On other worlds, though, carbon might be as common as dirt. In fact, carbon and dirt might be one and the same. An exoplanet 40 light-years away was recently identified as a promising candidate for just such a place—where carbon dominates and where the pressures in the planet's interior crushes vast amounts of the element into diamond.
The planet, known as 55 Cancri e, might have a crust of graphite several hundred kilometers thick. “As you go beneath that, you see a thick layer of diamond,” says astrophysicist Nikku Madhusudhan, a postdoctoral fellow at Yale University. The crystalline diamond could account for a third of the planet's thickness.
Carbon-based worlds would owe their distinct makeup to a planet-formation process very different from our own. If the composition of the sun is any indication, the cloud of dust and gas that coalesced into the planets of our solar system ought to have contained about twice as much oxygen as carbon. Indeed, Earth's rocks are mostly based on oxygen-rich minerals called silicates. Astronomers have determined that 55 Cancri e's host star, however, contains slightly more carbon than oxygen, which may reflect a very different planet-forming environment. And Madhusudhan and his colleagues calculated that the planet's bulk properties—denser than a water world but less dense than a world made of Earth-like minerals—match those predicted for a carbon planet. The researchers published their findings in the November 10, 2012, Astrophysical Journal Letters.
Life-forms on a carbon planet—if they exist—would little resemble the oxygen-dependent organisms of Earth. Precious oxygen would prove valuable as a fuel in much the same way that humans covet hydrocarbon fuels on Earth, says Marc Kuchner of the NASA Goddard Space Flight Center. Even courtship customs would be worlds apart from ours. “You would not be impressed if someone gave you a diamond ring,” Kuchner muses. “If your suitor showed up with a glass of water, that would be really exciting.”
  • 'Scientists discover potential cure for AIDS'

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STAFF WRITER 12:55 HRS IST
From Natasha Chaku

Melbourne, Jan 16 (PTI)
In a breakthrough, Australian researchers claim to have discovered how to modify a protein in HIV which could lead to a potential cure for AIDS.

According to researcher David Harrich from Queensland Institute of Medical Research, the protein can be modified so that, instead of replicating, it protects against the deadly infection.

"I consider that this is fighting fire with fire.

star most ancient just 186 light years away from Earth[THOUGHT ANCIENT STARS ARE ON THE FRINGES OF UNIVERSE!]


13.2bn-year-old star most ancient in the universe


LONDON: Scientists have identified a star, at least 13.2 billion-years-old, as the oldest yet seen in the universe and it is just 186 light years away from Earth.
The Big Bang is calculated by scientists to have taken place about 13.77 billion years ago and the star, known as HD 140283, was among the earliest stars to form, the 'Daily Mail' reported.
"We believe this star is the oldest known in the Universe with a well determined age," Howard Bond, an astronomer at Pennsylvania State University, told the American Astronomical Society.
Since it contains some heavy elements it is thought to have been one of the second generation of stars to be created following the Big Bang. The first generation of stars contained hardly any elements heavier than helium but when they exploded in a succession of supernovas within a few hundred million years after forming they were replaced by stars like HD 140283.
Observations from the Hubble Telescope helped experts fix the distance of the star from the Earth with unprecedented accuracy which allowed them to make more accurate measurements of how brightly it shines. Once its brightness was established they were able to work out how rapidly its hydrogen is being exhausted and so determine its age.