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Increasing the odds of the sweep

Astronomers confirm two exoplanets using ESO's Very Large Telescope and Hubble Space Telescope data. The discoveries provide strong evidence for at least 6 billion Jupiter-sized planets in the Milky Way, including five new ultra-short-period planet types.

SourceESO·JournalNature·DateOct 4, 2006

IAU names dwarf planet Eris

The International Astronomical Union has named the newly discovered dwarf planet Eris and its moon Dysnomia. The name Eris was proposed by Michael Brown and accepted unanimously by the Working Group for Planetary System Nomenclature and the Committee for Small Body Nomenclature.

Trio of Neptunes and their belt

Three tiny companions orbiting HD 69830 have been discovered by astronomers using the ESO's HARPS instrument. The newly found planets have minimum masses between 10 and 18 times the mass of Earth, with one located in the habitable zone.

SourceESO·JournalNature·DateMay 17, 2006

Scientists reveal fate of Earth's oceans

Researchers at the University of Manchester have identified seawater in volcanic gas samples from the Earth's mantle, supporting the theory that seawater is subducted deep into the Earth. The study reveals that up to 10% of the Earth's oceans have been absorbed into the planet since its formation.

SourceUniversity of Manchester·JournalNature·DateMay 10, 2006

It's far, it's small, it's cool: It's an icy exoplanet!

Astronomers have discovered the first and only icy exoplanet that matches theoretical predictions for Solar System formation. OGLE-2005-BLG-390Lb orbits a small red star at an extremely close distance, with a surface temperature of -220°C, and is likely to resemble Pluto more than rocky planets like Earth.

SourceESO·JournalNature·DateJan 25, 2006

The land of three rising suns

A team of astronomers has discovered a hot Jupiter planet in a triple star system, challenging conventional theories of planetary formation. The discovery suggests that it is possible for planets to form around the host star and then be captured by a binary system, explaining the unusual configuration of the HD 188753 system.

SourceNew Scientist·JournalThe New Scientist·DateNov 16, 2005

Organised wind chaos on Jupiter

Jupiter's atmosphere is driven by heat from within the planet, creating organized wind chaos. The computer models explain why there are two classes of jet winds: strong and narrow near the equator, but weak and wide at higher latitudes due to the planet's curvature and rotation.

SourceMax-Planck-Gesellschaft·JournalNature·DateNov 9, 2005

Early Mars: Warm enough to melt water?

Early Mars research suggests that the planet may have been too cold to melt water, contradicting Dr. James F. Kasting's theory of a greenhouse effect. However, Kasting proposes that methane-producing bacteria could have warmed the planet, allowing for the formation of features like Nanedi Vallis.