A Closer Look at Planetary Formation

Astronomers have used the European Southern Observatory to map a vast disc of gas and dust surrounding a newly born massive star. The star is called HD 97048, and it’s located in the Chameleon I dark cloud, a stellar nursery 600 light-years away. The central star has 40 times the mass of our Sun, and the surrounding disc stretches 12 times further than the orbit of Neptune in our own Solar System.
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Two Hot New Planets Discovered

An international team of astronomers have turned up two new Jupiter-sized planets orbiting distant stars. These planets are incredibly close to their parent stars; just a fraction of the distance from Mercury to the Sun. Astronomers believe these planets are being eroded by the intense radiation of their stars. The discovery was made using the new SuperWASP program, which looks for stars that dim and brighten on a regular schedule as a planet passes in front of them.
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Brown Dwarf Discovered in Planetary System

NASA’s Spitzer Space Telescope has directly imaged a small brown dwarf star orbiting a larger star – the first time this has ever been seen. The brown dwarf, HD 3651, is classified as a “T dwarf”, has about 50 times the mass of Jupiter, and orbits about 10 times the distance from the Sun to Pluto. Astronomers theorized that the system contained a brown dwarf, because a Saturn-sized planet had a strangely elliptical orbit; something was tugging on it.
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Huge, Lightweight Planet Discovered

A new, lightweight planet has been discovered orbiting a star 450 light-years away in the constellation Lacerta. This unusual planet is larger than Jupiter, but it has only half its mass; astronomers estimate it has the same density as cork. The planet, named HAT-P-1, orbits its host star every 4.5 days. A network of automated telescopes detected how the planet dims its parent star by 1.5% when it passes in between the star and the Earth. Why this planet is so swollen is still a mystery to astronomers.
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Identifying Planets with Life

Telescope technology is advancing quickly, as larger and larger instruments are getting built. Eventually, an observatory will be built capable of resolving Earth-sized worlds orbiting other stars. If there’s life there, will we recognize it? Researchers from Harvard-Smithsonian Center for Astrophysics and NASA have developed a list of epochs in Earth’s atmosphere’s history that could be visible through this instrument; from the earliest times that life emerged to our current, oxygen/nitrogen-abundant atmosphere.
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Network of Small Telescopes Find a Big Planet

A network of amateur astronomers has discovered an extrasolar planet located 500 light years away. This incredible discovery was made using a technique that measures the brightness of thousands of stars, watching for a periodic dimming. In this case, the Jupiter-sized planet, TrES-2, orbits its host star every 2.5 days, dimming it by 1.5%. Although the planet was discovered by a 10cm telescope, followup observations were made using the 10 metre W.M. Keck Observatory on Mauna Kea in Hawaii.
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Earth-Sized Planets are Probably Common

Of the many extrasolar planetary systems discovered so far, more than a third could contain Earth-like planets. This is according to a new study by scientists associated with NASA’s Center for Astrobiology. It was originally thought that Jupiter-sized planets should clear out their star systems as they form, but some new calculations show that they actually promote the formation of rocky planets – and even help pull in icy objects that deliver water to the inner planets.
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Giant Planet or Failed Star?

The Hubble Space Telescope has helped astronomers uncover an object right at the dividing line between stars and planets. The object, known as CHXR 73 B, weighs in at about 12 times the mass of Jupiter, and orbits a larger red dwarf star. The two objects are separated by 200 times the distance of the Earth to the Sun, so astronomers don’t think they both formed out of the same disk of gas and dust.
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Astrophoto: Stellar Nursery NGC 7129 by Bob Allevo

Prior to 1957, virtually all photographs of the sky were produced as monochrome, black and white images. In that year, Ansco, once the world’s largest supplier of professional films, papers, and photo chemicals, introduced Super Anscochrome and over the next twenty-four months, full color images of the heavens were being released by the larger observatories. Over the years technology has improved and the colors captured in astronomical imagery have become more vivid and meaningful. For example, the hues seen in the accompanying picture represent not only this scene’s true-to-nature pallet, but it also reveals what you are looking at, too.
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