Blizzard of Snowflake Particles Around a Young Star

Debris disk around AU Microscopii. Image credit: HubbleThe Hubble Space Telescope has imaged a ring of dust around a nearby star that will probably become a system of planets. The star is AU Microscopii, and it’s located about 32 light-years away in the southern constellation of Microscopium (the Microscope). The particles are probably as fluffy as snowflakes, and about 10 times larger than typical interstellar dust grains.
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New Planet Hunter Prepares for Launch

A powerful new instrument for finding extrasolar planets is about to launch: COROT (Convection Rotation and planetary Transits). Developed by the European Space Agency, COROT will search for planets using the transit method; it will be able to detect the slight drop in brightness as a planet moves in front of its parent star. If the observatory performs as expected, it should be able to detect rocky worlds just a few times larger than the Earth. COROT is scheduled to launch in December, 2006.
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Brown Dwarf Companion Seen Directly

Astronomers have directly imaged a brown dwarf companion to the star HD 3651. This star is already known to host an extrasolar planet – less massive than Saturn, but sitting within the orbit of Mercury. HD 3651 is slightly less massive than the Sun, and is located 36 light-years away in the constellation Pisces. The brown dwarf, or HD 3651B, is probably between 20 and 60 Jovian masses, and has a temperature between 500 and 600 degrees Celsius.
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Day and Night on an Extrasolar Planet

NASA’s Spitzer Space Telescope has measured the day and night time temperatures of an extrasolar planet. This planet is located 40 light-years away, circling the star Upsilon Andromedae. It’s classified as a “hot Jupiter”, and orbits its parent star once every 4.6 days. The temperature difference between the day and night sides is enormous – differing about about 1,400 degrees Celsius (2,550 degrees Fahrenheit). Although the planet itself is tidally locked to the star, and always presents one face, its atmosphere probably does swirl around, and distributes the heat somewhat.
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Super Earths Emerge From Snowy Conditions

Many extrasolar planets have been discovered circling other stars, a few of which are 5-15 times the mass of the Earth, and thought to be solid like our planet. Astronomers were surprised to find these planets orbiting small, cooler red dwarf stars. Researchers believe these “super Earths” form in the chilly halo of snow, ice and frozen gasses that collect around red stars as they cool. There probably isn’t enough solid material to form rocky planets much larger than Mercury in the star’s habitable zone.
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Hubble Examines the Closest Known Extrasolar Planet

The Hubble Space Telescope turned its gaze towards a relatively nearby Jupiter-sized world recently. The planet orbits the Sun-like star Epsilon Eridani, which is located only 10.5 light-years away. This makes the planet so close that it could be directly observable by Hubble, and large ground-based observatories. The best opportunity will come in 2007, when the planet makes its closest approach to its parent star, and the reflected light should make it observable with our best instruments.
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Hubble Finds Distant Extrasolar Planets

The Hubble Space Telescope has identified 16 stars that could have extrasolar planets. The discoveries were made as part of a new Hubble survey, called the Sagittarius Window Eclipsing Extrasolar Planet Search (SWEEPS). This survey looked at 180,000 stars in the central bulge of the Milky Way – 26,000 light years away. The discovery was made using the transit method, where planets dim their parent stars slightly as they pass in front. Further observations will be needed to actually calculate the mass of the transiting planets.
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Are There Oceans on Neptune?

Are There Oceans on Neptune
Neptune
Smaller and cooler than the gas giants, Neptune and Uranus are classified as ice giants. It’s a good name, since they do have large quantities of water ice mixed in with a largely hydrogen and helium atmosphere. There’s very little water at the cloud tops, but the percentage of water increases as you descend towards the heavier core. Could there be a layer on Neptune with enough pressure and temperature for liquid water to form into vast oceans? And if not Neptune, what about a Neptune-like planet orbiting another star?
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