Add BrightSurf on Google Email

Common Jupiters?

A recent study using data collected between 2006 and 2007 found evidence for 10 free-floating planets roughly the mass of Jupiter, suggesting they are common. The discovery supports the 'ejection' scenario where planets are kicked out from their solar systems due to close gravitational encounters with other planets or stars.

Flipping hot Jupiters

Astronomers at Northwestern University have developed a computer simulation that explains how hot Jupiters form with flipped orbits around their stars. The study, published in Nature, suggests that gravitational perturbations from other planets in the system can cause the inner planet to lose energy and orbit closer to its star.

SourceNorthwestern University·JournalNature·DateMay 11, 2011

Turning planetary theory upside down

Astronomers discover six exoplanets orbiting their stars in the opposite direction to the star's rotation, contradicting conventional wisdom. This finding sparks alternative migration theories, suggesting that hot Jupiters may form far from their stars and migrate inward due to gravitational interactions with distant companions.

SourceESO·DateApr 13, 2010

Helium rain on Jupiter

Researchers discovered a layer where helium condenses into droplets, allowing neon to dissolve and fall towards the planet's interior. This phenomenon explains the observed lack of neon in Jupiter's upper atmosphere.

SourceAmerican Physical Society·JournalPhysical Review Letters·DateMar 22, 2010

Helium rains inside jovian planets

Scientists at Lawrence Livermore National Laboratory and the University of Illinois have determined the temperature at which helium becomes insoluble in dense metallic hydrogen. This finding has significant implications for models of the interior structure and evolution of Jovian planets, including Saturn and Jupiter.

SourceDOE/Lawrence Livermore National Laboratory·JournalProceedings of the National Academy of Sciences·DateJan 26, 2009

Jupiter and Saturn full of liquid metal helium

Researchers at UC Berkeley and University College London discovered that metallic helium is produced under extreme conditions found at the centers of Jupiter and Saturn, mixing with metal hydrogen to form a liquid metal alloy. This finding challenges previous theories about the energy source powering these planets.

SourceUniversity of California - Berkeley·JournalProceedings of the National Academy of Sciences·DateAug 6, 2008

Storn winds blow in Jupiter's Little Red Spot

A team of scientists from Johns Hopkins University used data from NASA's New Horizons spacecraft and multiple telescopes to observe the high winds in Jupiter's Little Red Spot. The winds have increased substantially over previous storms, with maximum speeds reaching 384 miles per hour, surpassing Category 5 storm thresholds.

Novel spots found on Jupiter

Researchers have found unexpected luminous spots on Jupiter's atmosphere caused by the moon Io's volcanic eruptions. The discovery challenges previous models of the Io footprint and reveals a new interpretation where beams of electrons travel from one hemisphere to another.

SourceAmerican Geophysical Union·JournalGeophysical Research Letters·DateMar 17, 2008

Extreme winds rule exoplanet's weather

Researchers have mapped weather on a gas giant planet called HD 189733b, discovering supersonic winds that can move at speeds of up to 22,000 mph. The winds are so fast they redistribute heat across the planet's surface, with dayside and nightside temperatures differing by only 500 degrees Fahrenheit.

SourceUniversity of Arizona·JournalNature·DateMay 9, 2007

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

The 'planemo' twins

Astronomers have discovered a double planetary mass object in the Ophiuchus star-forming region, approximately 400 light years away. The objects, which are similar to extra-solar giant planets, are not orbiting around a star but instead appear to be circling each other.

SourceESO·JournalScience·DateAug 3, 2006

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

AGU journal highlights - 10 April 2006

Research papers in Geophysical Research Letters and Paleoceanography reveal the connection between terrestrial gamma-ray flashes and intracloud lightning, as well as the potential of dinoflagellate microfossils to document past climate changes. The findings suggest that these marine organisms can provide valuable information on ocean c...

SourceAmerican Geophysical Union·JournalGeophysical Research Letters·DateApr 10, 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