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Will Gamma-Ray Detector Find Asteroid Treasure

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“With our proposed system it should be possible to measure sub-surface elemental abundances accurately, and to do it much more cheaply because our sensors weigh less and require less power to operate,” says Keivan Stassun. “That is good news for commercial ventures where cost, power and launch weight are all at a premium.”

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Will Gamma-Ray Detector Find Asteroid Treasure ?

Two recent events—one legal and the other technological—have brought asteroid mining a step closer to reality.

First, the US Senate Commerce, Science and Transportation Committee passed a bill titled H.R. 2262—SPACE Act of 2015, which has a number of measures designed to facilitate commercial space development, including a provision that gives individuals or companies ownership of any material that they mine in outer space. According to one estimate, asteroid mining could ultimately develop into a trillion-dollar market.

Second, researchers have devised a new generation of gamma-ray spectroscope that appears perfectly suited for detecting veins of gold, platinum, rare earths, and other valuable material hidden within the asteroids, moons, and other airless objects floating around the solar system.

It’s just the type of “sensor” that asteroid miners will need to sniff out these valuable materials.

The first commercial missions to nearby asteroids could launch as early as 2020, but it will be decades before asteroid mining begins in earnest. In the meantime, the new spectroscopic technology promises to provide planetary scientists with new details about the chemical composition of the asteroids, comets, moons, and minor planets in the solar system—information that is certain to improve our understanding of how the solar system formed.

In addition, it could become an important tool in the planetary defense arsenal because it can determine whether objects crossing Earth’s orbit are made from rock or ice.

Gamma Rays
Planetary gamma-ray spectroscopy takes advantage of the fact that cosmic rays continually bombard all of the objects in the solar system. These high-energy particles from deep space strike the exposed surfaces at relativistic velocities, smashing apart atoms in the top layers and producing a secondary shower of particles, including neutrons.

The neutrons then collide repeatedly with the atoms in the material, producing gamma rays as they go. Gamma rays are a form of electromagnetic radiation like light, but they are considerably more powerful and penetrating. The decay of long-lived radioactive elements is a secondary source of gamma rays.

A gamma-ray spectroscope records the intensity and wavelengths of the gamma rays coming from a surface. This spectrum can be analyzed to determine the concentration of a number of important, rock-forming elements, including oxygen, magnesium, silicon, and iron—in addition to precious metals like gold and valuable crystals like diamonds.

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“Space missions to the Moon, Mars, Mercury, and the asteroid Vesta among others have included low-resolution spectrometers, but it has taken months of observation time and great expense to map their elemental surface compositions from orbit,” says coauthor Keivan Stassun, professor of astronomy at Vanderbilt University.

“With our proposed system it should be possible to measure sub-surface elemental abundances accurately, and to do it much more cheaply because our sensors weigh less and require less power to operate. That is good news for commercial ventures where cost, power, and launch weight are all at a premium.”

The Key Crystal

The key to the new instrument is a recently discovered material, europium-doped strontium iodide (SrI2). This is a transparent crystal that can act as an extremely efficient gamma-ray detector. It registers the passage of gamma rays by giving off flashes of light that can be detected and recorded.

“The gold standard for gamma-ray spectroscopy is the high purity germanium (HPGe) detector,” says Arnold Burger, a physics professor at Fisk University who developed the SrI2 detector. “However, it requires cryogenic cooling so it is very bulky. It also needs vacuum-tube technology so it consumes too much energy to run on batteries.

“SrI2 isn’t quite as good HPGe, but it is more than adequate to do the job and it is compact enough and its power requirements low enough so that it can be used in spacecraft and even placed on robotic landers.”

Coauthors from NASA’s Jet Propulsion Laboratory and the Planetary Science Institute also contributed to the report, which appears in the SPIE Newsroom.

Source: Vanderbilt University


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