Astronomers used the Keck Observatory in Hawaii to listen to the "music" of the nearby star HD 219134, discovering it is slightly smaller than previously thought and providing insights into stars' rotation and planets' characteristics.
By studying the subtle vibrations or oscillations emitted by stars, astronomers can determine their mass, size, and age, as well as measure the sizes and densities of planets orbiting them.
The technique of listening to stars' sound waves, known as asteroseismology, allows scientists to gain valuable information about stars' interiors and evolutionary processes.
The Keck Planet Finder instrument at the W. M. Keck Observatory was crucial in detecting the stellar vibrations of the cooler orange star HD 219134, aiding in precise measurements and discoveries.
Studying the oscillations within stars like HD 219134 helps determine their ages, rotational speeds, and how they evolve over billions of years, contributing to a better understanding of stellar lifetimes.
The new study on HD 219134 revealed it to be more than twice the age of our sun, emphasizing the importance of asteroseismic data in calibrating stellar models and accurately estimating star ages.
Surprisingly, HD 219134 was found to be about 4% smaller than previously believed, challenging existing stellar models and raising questions about the causes of this size difference.
With at least five confirmed planets, including super-Earths, orbiting HD 219134, the refined measurements of the star's size will aid in better understanding the planets' properties and potential for extraterrestrial life.
Further research using instruments like the Keck Planet Finder can help in the quest to identify planets with potential for hosting life and determine the ages of stars and their associated planetary systems more accurately.
Studying the music of nearby stars through asteroseismology offers valuable insights into stellar evolution, planetary characteristics, and the potential for discovering life beyond Earth.