Testing the Titius-Bode law on exoplanets
From examining extrasolar planetary systems, we can test if the Titius-Bode “law” is actually a law.
From examining extrasolar planetary systems, we can test if the Titius-Bode “law” is actually a law.
Exoplanets with moons could mimic alien life-signs.
How do pulsating stars give away their secret identities as binary dance partners? In this paper, the authors demonstrate a new way to not only detect binaries we may have missed in the Kepler data, but also to measure their velocities without spectra.
Kepler finds the signature of a transiting white dwarf. Instead blocking the light of its companion star, the white dwarf magnifies it, creating a light curve that periodically brightens.
The orbits of some recently discovered exoplanets seem to be synchronised with the rotation of their host stars. Can this mystery be explained?
We have repeatedly seen how Kepler goes above and beyond its original mission of finding exoplanets. Today’s paper is no exception.