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Search results for “Star Cluster”

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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

Recipe for water: Just add starlight

Astronomers discovered a cloud of hot water vapor around the old star IRC+10216 and suspected comets or dwarf planets were evaporating to produce it. However, Herschel's instruments revealed that ultraviolet light from surrounding stars is the actual source of the water, which forms closer to the star than comets can stably exist.

SourceEuropean Space Agency·JournalNature·DateSep 2, 2010

Stars just got bigger

Scientists have discovered a star with a mass of 265 solar masses in the Large Magellanic Cloud, exceeding previous records. This finding raises questions about the formation process of such massive stars and their role in shaping the universe.

SourceESO·JournalMonthly Notices of the Royal Astronomical Society·DateJul 21, 2010

Exoplanet caught on the move

The discovery of exoplanet Beta Pictoris b, located 60 light-years from Earth, confirms that giant planets can form in time-spans as short as a few million years. The planet has a massive nine-Jupiter-mass orbit, challenging previous theories on planetary formation.

SourceESO·JournalScience·DateJun 10, 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

The big blow-up

Researchers discover supernova that fits predictions for a star hundreds of times the sun's mass, revealing new insights into star formation and heavy metal creation. The study also suggests hyper-giant stars may exist beyond 150 suns, challenging our understanding of celestial physics.

SourceWeizmann Institute of Science·JournalNature·DateDec 3, 2009

Invading black holes explain cosmic flashes

Mathematicians at the University of Leeds propose that black holes are directly responsible for producing gamma ray bursts, contradicting the orthodox model. The theory suggests that rotating black holes can devour nearby stars, creating long-lasting jets of plasma that produce the high-energy radiation.

SourceUniversity of Leeds·JournalMonthly Notices of the Royal Astronomical Society·DateSep 18, 2009

Scientists discover magnetic superatoms

Researchers at Virginia Commonwealth University discovered a stable cluster of atoms that can mimic different elements of the periodic table, exhibiting strong magnetic properties. The discovery has potential applications in creating faster computers, larger memory storage, and molecular electronic devices.

SourceVirginia Commonwealth University·JournalNature Chemistry·DateJun 15, 2009

World's observatories watching 'cool' star

Scientists are synchronizing lenses of the Whole Earth Telescope network to monitor a white dwarf, shedding light on its composition and applying knowledge to Earth's weather. The star, WDJ1524-0030, is losing brightness as it cools, with astronomers studying its pulses to understand internal movements.

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

After the collapse

Scientists have directly observed a gigantic star blowing up, supporting the idea that massive stars end as black holes. The explosion revealed most of the star's mass collapsed into a dense core, creating an invisible black hole.

Even stars get fat

A team of scientists discovered that blue stragglers, massive rogue stars found in globular clusters, are formed through a process known as stellar cannibalism. This theory is supported by observations of over 50 globular clusters and suggests that binary star systems play a key role in the formation of these stars.

SourceMcMaster University·JournalNature·DateJan 14, 2009