Exoplanets and Future Astronomy

radius of the event horizon for a simple non-rotating black hole.

a feature of classical black-hole solutions where the theory ceases to provide a complete physical description.

extreme stretching caused by strong tidal forces near a compact object.

study of how matter interacts with different wavelengths of electromagnetic radiation.

a black hole formed primarily through massive stellar evolution.

a black hole containing millions or billions of solar masses.