Earth-Like Planets Should Be Easy Spot While They’re Forming

Researchers at the Washington University in St. Louis have developed a “field guide” for planet hunters searching for other Earths. They modeled the chemistry of silicate vapour and steam rich environments, similar to the early stages when an Earthlike planet is forming. During this stage, the planet is covered with a magma ocean which vapourises. This is a very distinct moment in the lifetime of a planet, and should be detectable because silicon monoxide gas is easy to see in infrared and radio wavelengths.

Canada’s Humble Space Telescope

One of the more productive telescopes in space is the tiny Canadian MOST satellite (Microvariability and Oscillations of Stars). Developed and maintained on a shoestring – $7 million USD – MOST is only the size of a suitcase, but it has a very sensitive instrument which can detect the variations in star brightness. MOST has been used to analyze recently discovered extrasolar planets as they pass in front of their parent stars, and even get some information about their atmospheres.

Capturing the Fastest Events in the Universe

A new high-speed camera has been mounted to the European Southern Observatory’s Very Large Telescope in Chile. This ultra fast camera is called ULTRACAM, and it’s capable of recording some of the most rapid astronomical events. It’s capable of taking 500 pictures a second, so it will be used to watch any object that can change quite rapidly, like black holes, gamma ray bursts, white dwarfs or cataclysmic variables.

Planet Forces its Star’s Rotation

Canadian astronomers using the MOST (Microvariability & Oscillations of STars) Space Telescope have detected that a giant extrasolar planet has forced its parent star into a lock-step orbit. This interaction is between the star tau Bootis and its “hot Jupiter” planet discovered in 1997. MOST was able to detect subtle variations in the star’s brightness that correspond with the planet’s orbit. It’s likely that the planet has forced the outer layer of tau Bootis’ atmosphere so that it rotates to keep the same side facing.

Probing the Atmosphere of an Extrasolar Planet

Astronomers working with the Canadian Microvariability & Oscillations of STars (MOST) space telescope have been able to indirectly probe the atmosphere of a planet orbiting another star. The planet, HD209458b, was imaged earlier this year by NASA’s Spitzer space telescope; it’s a “hot jupiter”, orbiting very close to its parent star. MOST will watch how its parent star changes in brightness as the planet passes in front and behind, and should be able to provide details about its temperature, pressure, and even cloud cover.

Is This the First Photo of an Exoplanet?

Astronomers have discovered more than 150 planets orbiting distant stars, but only indirectly. Now an international team of researchers think they might have the first direct photograph of a planet orbiting another star. The image is of GQ Lupi, a young star located 400-500 light-years away. A dimmer object, potentially a planet, is located to the right of the star separated by 100 astronomical units (2.5 times the distance of the Sun to Pluto). Unfortunately, the astronomers haven’t been able to determine the mass of the object, so they can’t rule out that it might be a brown dwarf.

How Many Habitable Planets Could Be Out There?

The chances of finding life somewhere else in the Universe depends on how many planets are capable of supporting life. Well, according to new calculations by astronomers at Open University, as many as half of all star systems could contain habitable planets. The team created mathematical models of known exoplanetary systems, and then added Earth-sized planets into the mix. They found that in half of all planetary systems they simulated, the gravity of the gas giants won’t catastrophically affect the orbits of these smaller planets, giving life a chance to evolve.

Jupiter-Sized Star Found

Astronomers have found a core burning star, like our own Sun, that’s only 16% larger than Jupiter; although, it has 96 times as much mass. The observations were made using the European Southern Observatory’s 8.2m VLT Kueyen telescope in Chile. Astronomers watched tracked 60 stars which were known to have a regular dip in brightness, when a dimmer object was passing in front. This survey found 7 of these low mass stars which eclipsed their brighter companion.

It Gave Until it Couldn’t Give Any More

Astronomers using the Gemini observatories have got themselves a bit of a mystery. They’ve found a binary system at EF Eridanus, located 300 light-years away from Earth, where one of the objects defies classification. It’s about the size of Jupiter but it’s way too massive to be a planet. It’s the temperature of a brown dwarf, but its light doesn’t match a brown dwarf’s characteristics. The researchers believe that the object was once a regular star, but then it had most of its material stripped away by the gravity of the larger star over the course of 5 billions years. Eventually it just couldn’t give any more.

First Direct Image of An Exoplanet?

A team of European and US astronomers think they’ve taken the first direct image of a planet orbiting another star about 230 light-years away. Until now, planets have been discovered because of the effect they have on their parent star – they haven’t been “seen” directly. Using the European Southern Observatory’s 8.2-m telescope in Chile, the team found a faint, red object nearby a brown dwarf star called 2M1207. By analyzing the object with various instruments, they believe the object is approximately 5 times the mass of Jupiter. There’s still some uncertainty, though, so the team will make regular observations over the next 2 years to see how its position and composition changes.