Earth-like planets orbiting other stars in the Milky Way are three times more likely to have the same type of minerals as Earth than astronomers had previously thought. In fact, conditions for making the building blocks of Earth-like rocks are ubiquitous throughout the Milky Way. The results of a new study of the chemical evolution of our galaxy are being presented today by Prof Brad Gibson, of the University of Hull, at the National Astronomy Meeting in Llandudno.
"The ratio of elements on Earth has led to the chemical conditions 'just right' for life. Too much magnesium or too little silicon and your planet ends up having the wrong balance between minerals to form the type of rocks that make up the Earth's crust," said Gibson. "Too much carbon and your rocky planet might turn out to be more like the graphite in your pencil than the surface of a planet like the Earth."
Gibson and team from the E.A. Milne Centre for Astrophysics at the University of Hull have constructed a sophisticated simulation of the chemical evolution of the Milky Way, which results in an accurate recreation of the Milky Way as we see it today. This has allowed them to zoom in and examine the chemistry of processes, such as planetary formation, in detail. Their findings came as something of a surprise.
The cloud out of which the solar system formed has approximately twice as many atoms of oxygen as carbon, and roughly five atoms of silicon for every six of magnesium. Observers trying to ascertain the chemical make-up of planetary systems have tended to look at large planets orbiting very bright stars, which can lead to uncertainties of 10 or 20 per cent. In addition, historically the spectra of oxygen and nickel have been hard to differentiate. Improvements in spectroscopy techniques have cleaned up the oxygen spectra, providing data that matches the Hull team's estimates.
"Even with the right chemical building blocks, not every planet will be just like Earth, and conditions allowing for liquid water to exist on the surface are needed for habitability," said Gibson. "We only need to look to Mars and Venus to see how differently terrestrial planets can evolve. However, if the building blocks are there, then it's more likely that you will get Earth-like planets -- and three times more likely than we'd previously thought."
Source: Royal Astronomical Society [July 08, 2015]
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