Articles tagged with Stellar Oscillations
Astronomers have discovered a planetary system with an enormous planet sandwiched between a Sun-like star and a dwarf star. The planet's massive eccentric orbit indicates gravitational influence from the dwarf star, leading to Kozai oscillations that cause it to 'dance' between the two stars.
Researchers used asteroseismology to probe magnetic fields in the cores of red giants, finding them strongly magnetized. The strong fields disrupt gravity waves, causing energy loss and affecting star evolution.
Researchers use asteroseismology to track waves through stars and determine internal properties, finding nearly a million times stronger magnetic fields than typical refrigerator magnets. This technique allows probing of previously hidden regions of stars.
Researchers have developed a new method to probe the internal magnetic fields of red giant stars using asteroseismology. This technique involves analyzing variations in light emitted from a star as due to sound waves from its interior, revealing strong internal magnetic fields in these stars.
A new study has precisely measured the ages of 33 Kepler stars with solar-like oscillations, revealing that even stars older than 11 billion years have Earth-like planets. The research uses asteroseismology to analyze tiny variations in starlight and provides a large sample for studying galactic archeology.
A team of astronomers found that 74 Earth-sized exoplanets orbit their stars in circular patterns, contrary to expectations. This discovery suggests that small planets may maintain stable climates year-round, making them more hospitable to life.
An international team of astronomers has discovered a Sun-like star with orbiting Earth-sized planets dating back to the dawn of the Galaxy. The discovery, Kepler-444, hosts five small planets smaller than Mercury and Venus.
Researchers have found that stars that oscillate at the same frequency as gravitational waves can absorb energy from those waves and brighten temporarily. This effect could provide scientists with another method to indirectly detect gravitational waves.
A team of 20 scientists monitored the 'heartbeats' of young stars using data from two space telescopes. They found that emerging stars pulsate slowly at first, then faster as they near ignition, revealing insights into their internal structures and ages.
Researchers used data from NASA's Kepler space telescope to observe a distant planetary system with multiple planets at severe tilt to their host star. The discovery suggests that tilted planetary orbits are possible even in systems without a hot Jupiter, providing new insights into the architecture of alien solar systems.
Astronomers have developed a new technique to measure the surface gravity of distant stars, which is crucial for calculating their physical properties and evolutionary state. The technique has been shown to be more accurate than existing methods and can significantly improve estimates of exoplanet sizes.
A team of researchers has developed a new method to measure the internal properties of stars, enabling more accurate assessments of their orbiting planets. By using asteroseismology, they were able to determine the mass and rotation rate of a pulsating star, confirming the existence of an exoplanet in its orbit.
Astronomers used Kepler spacecraft data to discover a planet smaller than Mercury, about the size of Earth's moon, in the Cygnus-Lyra region of the Milky Way. The planet, Kepler-37b, is likely a rocky world with no atmosphere or water.
Researchers have identified a QPO signal in a distant galaxy's black hole, revealing insights into the nature of compact objects. The detection extends the reach of relativity testing to smaller black holes, about 3.5 minutes apart.
Researchers at Caltech found a correlation between the neutrino signal and the gravitational-wave signal that occurs when the proto-neutron star reaches high rotational velocities. This discovery provides new insights into understanding the explosion process in massive stars.
The newly discovered two-planet system of Kepler-36 features a rocky planet Kepler-36b and a gas giant Kepler-36c that experience close encounters every 97 days. Researchers are struggling to understand how these worlds ended up in such tight orbits, but the discovery has significant implications for the search for exoplanets.
Astronomers have found two planets with diverse densities and compositions locked in close orbits, defying the planetary pattern of our solar system. The discovery, made possible by NASA's Kepler Mission, reveals a 'puzzling pair' that challenges theories on planet migration and orbital rearrangement.
Researchers have discovered two planets that survived being engulfed by their parent star, shedding new light on stellar and planetary systems. The discovery may also offer insights into the possible future of our own solar system.
Researchers have discovered two planets of sizes comparable to Earth orbiting an old star that has just passed the red giant stage. The planets, named KOI 55.01 and KOI 55.02, are thought to be the dense cores of ancient giant planets whose gaseous envelopes were vaporized during the immersion phase.
Researchers have detected stellar oscillations in a hotter star, revealing insights into its internal structure and composition. The discovery was made possible by the Kepler space telescope and provides new information on the processes that govern stellar behavior.
Astronomers have updated the census of sun-like stars with data from NASA's Kepler Mission, detecting changes in brightness in 500 stars. This provides a much better understanding of the stars' properties and their evolution, allowing for detailed measurements of star basics such as mass and age.
The Kepler spacecraft provides clear views of changes in star brightness, allowing astronomers to probe a star's core and determine its density and chemistry. The mission helps understand the life cycle of red giant stars, including whether they burn hydrogen or helium in the core.
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.
Researchers analyzed data from the CoRoT space telescope mission, finding that three nearby stars have larger vibrations and finer surface texture than our Sun. The study provides valuable information about the physical properties of nearby stars and sheds new light on the Sun's interior.
Astronomers using the Global Oscillation at Low Frequency (GOLF) instrument on SOHO have detected possible long-sought oscillations on the Sun's surface. This finding provides insight into the Sun's core and its role in the formation of our solar system.
The Corot space mission is scheduled to launch on December 27, 2006, and will detect planets orbiting around other stars. The mission will also probe the secrets of stellar interiors, potentially discovering rocky worlds similar to Earth.
Researchers have discovered a remarkably stable indentation in the fabric of space and time, created by the spin of a black hole. The finding is based on identical patterns observed in X-ray light emitted near the black hole nine years apart, using NASA's Rossi X-ray Timing Explorer.
A team of astrophysicists discovered X-ray oscillations in a neutron star that provide critical information about its internal structure. The oscillations, generated by massive quakes, contain frequency vibrations that can help scientists understand the nature of neutron stars.
The MOST team discovered that star Procyon shows no pulsations, overturning 20 years of previous research and forcing future space missions to revise their strategies. The tiny satellite measured brightness variations more precisely than any other instrument, revealing a new perspective on the stars in our Galactic backyard.
A rapidly spinning neutron star can naturally produce a Gamma-ray burst by oscillating and radiating its rotation energy. The spin-down process is triggered by the gravitational wave instability, which grows explosively in hours or minutes, strengthening the magnetic field and eventually radiating away all remaining rotation energy.
Astrophysicists have discovered rapid oscillations in neutron star brightness, which may confirm a unique effect of curved space-time predicted by Einstein's theory. The data was obtained using NASA's Rossi X-Ray Timing Explorer satellite.