Research news on Extrinsic variable stars

Extrinsic variable stars constitute a research area focused on stellar brightness variations arising from external geometric or environmental factors rather than intrinsic changes in stellar structure or energy generation. This field primarily investigates eclipsing binaries, rotating spotted stars, and systems with circumstellar or circumbinary material that modulate observed luminosity through occultation, reflection, or beaming effects. Research emphasizes precise photometric and spectroscopic monitoring, light-curve modeling, and orbital parameter determination to infer stellar radii, masses, inclination angles, and surface inhomogeneities, thereby constraining stellar evolution models, binary interaction physics, and population statistics of variable systems in different Galactic environments.

Astronomers collect rare evidence of two planets colliding

Anastasios (Andy) Tzanidakis was combing through old telescope data from 2020 when he found an otherwise boring star acting very strangely. The star, named Gaia20ehk, was about 11,000 light-years from Earth near the constellation ...

Ring around Tabby's star

This illustration shows a hypothetical uneven ring of dust orbiting KIC 8462852, also known as Boyajian's Star or Tabby's Star. The star has experienced unusual dips in brightness over a matter of days, as well as much subtler ...