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1,000+ results for "Jupiter"

Do 'planemos' have progeny?

Researchers have discovered six 'planemos,' planetary mass objects with masses similar to extra-solar planets, surrounded by dusty discs that may evolve into miniature planetary systems. These findings suggest similar infancies for our Sun and smaller objects, blurring the definition of a planet.

SourceESO·DateJun 5, 2006

Ice volcanoes on Saturn's moon Enceladus

Scientists have found evidence of volcanic activity on Enceladus, a key player in shaping the E ring. The discovery sheds light on the dynamics of ice particles in Saturn's system and challenges existing assumptions about how the moon contributes to the ring's mass distribution.

SourceMax-Planck-Gesellschaft·JournalScience·DateMar 14, 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

Closer to home

The discovery of OGLE-2005-BLG-390Lb provides strong evidence that low-mass planets, potentially supporting life, are more common than Jupiter-like gas giants. Researchers hope the gravitational microlensing technique will reveal more habitable worlds in the Milky Way galaxy.

AGU journal highlights - 4 January 2006

Research on Martian aurorae reveals localized ultraviolet emissions near magnetic field lines. Air pollution reduction could exacerbate global warming due to increased solar radiation scattering. A new study detects potential oilfield brine leaks in Nueces Bay, Texas, using sediment resistivity and radium isotope analysis.

SourceAmerican Geophysical Union·JournalGeophysical Research Letters·DateJan 4, 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

Even 'failed stars' form planets

A team of astronomers investigated six young brown dwarfs and found that dust particles in their circumstellar discs stuck together, forming larger clumps of olivine. This material is also found in comets and normal stars, suggesting a similar growth process in planet formation

SourceMax-Planck-Gesellschaft·JournalScience·DateOct 25, 2005

Rubble-pile minor planet Sylvia and her twins

Astronomers have discovered a triple asteroid system, with minor planet 87 Sylvia and its twin moons Romulus and Remus. The asteroids were found using the NACO instrument at ESO's Very Large Telescope Array in Chile, revealing details about their orbits and composition.

SourceESO·JournalNature·DateAug 10, 2005

AGU journal highlights - 9 March 2005

Researchers improved hurricane prediction using high-resolution general circulation models, predicting the course of four storms with increased accuracy. A new study found that solar emissions likely control Jupiter's X-ray emissions, providing a potential proxy for monitoring flares invisible to space weather satellites.

SourceAmerican Geophysical Union·JournalGeophysical Research Letters·DateMar 9, 2005

Jupiter: A cloudy mirror for the Sun?

Astronomers using the European Space Agency's XMM-Newton telescope discovered that Jupiter's x-ray glow is due to x-rays from the Sun being reflected back off the planet's atmosphere. The discovery synchronises Jupiter's day-to-day disk x-rays with the Sun's emissions, providing new insights into solar activity.

SourceScience and Technology Facilities Council·JournalGeophysical Research Letters·DateMar 7, 2005

Surf's up in the solar nebula

Scientists have long puzzled over the origin of chondrules, glassy particles found in meteorites that formed in the solar nebula. New calculations suggest that spiral arms in the disk surrounding Jupiter may have generated shock waves that melted dust clumps to form these particles.

SourceIndiana University·JournalThe Astrophysical Journal Letters·DateMar 3, 2005

Weighing the smallest stars

An international team of astronomers using the VLT's NACO SDI camera discovered a faint companion to AB Dor A, a young star, which is 93 times more massive than Jupiter and twice as heavy as predicted. The object's mass was determined by observing its precise location and orbit around its host star.

SourceESO·JournalNature·DateJan 19, 2005

Astronomers tackle 400-year-old heavenly mystery

Using the Spitzer Space Telescope, Hubble Space Telescope, and Chandra X-ray Observatory, researchers observed the Kepler's supernova remnant, uncovering a bubble-shaped shroud of gas and dust expanding at 4 million miles per hour. The observations revealed distinct features, including heated interstellar dust and regions of hot gas.