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Clocking Neptune's spin

A University of Arizona planetary scientist has determined Neptune's rotation with high accuracy by tracking atmospheric features in its atmosphere. The discovery improves upon previous measurements and provides a better understanding of the planet's fundamental properties.

SourceUniversity of Arizona·JournalIcarus·DateJun 29, 2011

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

Planet from another galaxy discovered

Astronomers have discovered a planet from another galaxy orbiting a star that has entered our Milky Way, providing the first confirmed detection of an extragalactic exoplanet. The planet, HIP 13044 b, was detected using high-resolution spectrograph FEROS attached to the MPG/ESO telescope at ESO's La Silla Observatory.

SourceESO·JournalScience·DateNov 18, 2010

How to weigh a star using a moon

New work by astrophysicist David Kipping reveals that astronomers can calculate a star's mass using its orbiting planet and moon. By measuring the size of the planet and moon relative to the star and their orbital periods, scientists can use Kepler's Laws of Motion to determine the density of the star.

SourceCenter for Astrophysics | Harvard & Smithsonian·JournalMonthly Notices of the Royal Astronomical Society·DateOct 15, 2010

Planet hunters no longer blinded by the light

Using new optics technology developed at the University of Arizona's Steward Observatory, astronomers have obtained images of a planet on a closer orbit around its parent star than any other extrasolar planet previously found. The discovery enables scientists to search for planets closer to the star than has been previously possible.

SourceUniversity of Arizona·JournalThe Astrophysical Journal Letters·DateOct 14, 2010

Discovery of Saturn's auroral heartbeat

A team of researchers has discovered that Saturn's aurora pulses in tandem with its radio emissions, providing a long-suspected link between the two phenomena. The discovery offers new insights into Saturn's irregular heartbeat and has significant implications for understanding the planet's rotation period.

SourceUniversity of Leicester·JournalGeophysical Research Letters·DateAug 4, 2010

Venus is alive -- geologically speaking

Scientists from NASA and the European Space Agency found evidence of relatively young lava flows on Venus, suggesting the planet remains capable of volcanic eruptions. These findings indicate that volcanic activity on Venus is likely gradual rather than cataclysmic.

SourceEuropean Space Agency·JournalScience·DateApr 8, 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

First temperate exoplanet sized up

Astronomers have discovered a temperate exoplanet, Corot-9b, with a mass about 80% that of Jupiter and an orbit similar to Mercury's. The planet is thought to have a temperature range of -20°C to 160°C, making it a significant finding in the study of exoplanets.

SourceESO·JournalNature·DateMar 17, 2010

The first portrait of a cool planet

Astronomers have directly imaged a faint celestial body orbiting the star GJ 758, estimated to be between 10 and 40 Jupiter masses. The discovered planet, GJ 758 B, has a temperature of around 330 degrees Celsius, making it the coldest companion of a Sun-like star ever imaged.

SourceMax-Planck-Gesellschaft·JournalThe Astrophysical Journal Letters·DateDec 7, 2009

Team using Subaru Telescope makes major discovery

An international team of scientists has made the first direct observation of a planet-like object orbiting a star similar to the sun. The object, GJ 758 B, is estimated to be 10-40 times as massive as Jupiter and orbits its star at a distance of approximately 300 trillion miles.

SourcePrinceton University·JournalThe Astrophysical Journal Letters·DateDec 3, 2009

Exoplanets clue to sun's curious chemistry

Astronomers have discovered that Sun-like stars with planetary systems tend to have lower levels of lithium than those without planets. The study, which analyzed 500 stars, found that planet-bearing stars had less than 1% of the lithium present in other similar stars.

SourceESO·JournalNature·DateNov 11, 2009

The search for ET just got easier

Astronomers at the Science and Technology Facilities Council's William Herschel Telescope have confirmed an effective way to search the atmospheres of planets for signs of life. This method uses transmission spectra, which can reveal vital information about a planet's atmosphere, providing clues about potential biological processes.

Creating the astro-comb to locate Earth-like planets

Researchers at Harvard-Smithsonian Center for Astrophysics have created an 'astro-comb' to help detect lighter planets around distant stars. The technique sharpens spectroscopy, enabling more accurate pinpointing of planet locations and opening possibilities for detecting more Earth-like planets.

SourceOptica·DateMay 7, 2009