Astrophysics & Cosmological Lexicon
Search foundational concepts, mathematical formulations, and observational terms across modern astronomy, astrophysics, and general relativity.
Accretion Disk
AstrophysicsA rotating flattened structure of gas, plasma, and dust in orbit around a massive central body such as a protostar, white dwarf, neutron star, or black hole, heated by gravitational shear friction.
Albedo
Planetary ScienceThe fraction of incident solar electromagnetic radiation reflected by a planetary body's surface or atmosphere, measured on a dimensionless scale from 0 (perfect absorber) to 1 (perfect reflector).
Astronomical Unit (AU)
Orbital MechanicsA standardized unit of length defined as exactly 149,597,870,700 meters (~149.6 million km), representing the mean distance from the center of Earth to the center of the Sun.
Baryon Acoustic Oscillations (BAO)
CosmologyPeriodic fluctuations in the density of visible baryonic matter caused by acoustic sound waves traveling through the hot relativistic plasma of the early universe prior to recombination at z ≈ 1100.
Chandrasekhar Limit
AstrophysicsThe maximum mass possible for a stable, electron-degenerate white dwarf star before gravitational collapse overcomes electron degeneracy pressure, triggering a Type Ia supernova or collapse into a neutron star.
Coronagraph
InstrumentationA specialized optical device integrated inside astronomical telescopes designed to occult (block) blinding direct light from a host star so that faint orbiting exoplanets or circumstellar debris disks can be resolved.
Event Horizon
AstrophysicsThe boundary surface in spacetime enclosing a black hole singularity beyond which the escape velocity exceeds the speed of light, making inward causal trajectories irreversible.
Gravitational Lensing
CosmologyThe deflection of electromagnetic radiation around massive foreground galaxies, galaxy clusters, or dark matter halos in accordance with general relativity, producing magnified arcs, multiple images, and Einstein rings.
Heliopause
Orbital MechanicsThe theoretical outer boundary of the heliosphere where the outward dynamic pressure of the solar wind balances the inward pressure of the local interstellar medium (LISM).
Lagrange Points
Orbital MechanicsFive equilibrium positions in an orbital configuration where the gravitational forces of two large bodies (e.g., Earth and Sun) combine with the centrifugal force to create a stable or quasi-stable parking location for a smaller mass.
Redshift (z)
CosmologyThe fractional displacement of spectral absorption or emission lines toward longer wavelengths caused by cosmological metric expansion, relativistic Doppler velocity, or intense gravitational potential wells.
Transit Photometry
AstrophysicsAn observational method that detects exoplanets by measuring periodic, minute dips in the total luminous flux received from a star as an orbiting planet eclipses a portion of the stellar disk.