c, speed of lightThe speed that light travels in a vacuum. It is about 3 x 108 m/s (186,000 miles/s).
Chromosphere2,500 km thick (1,600 mi) layer of plasma above the Sun’s photosphere. Temperatures range from ~4500 K to 60,000 K (110,000 to 8,000°F).
Closed UniverseA universe where the geometry of space closes upon itself like the surface of a sphere.
clusterClusters are fixed length blocks of bytes that store data for Microsoft operating systems.
Constant of ProportionalityWhen scientists or theoreticians find a mathematical relationship between two quantities, they design an equation, so that, for example, if one quantity…
ConvectionThe movement of matter due to changes in temperature and density. Warm material rises because it is less dense (lighter) and cool material sinks because…
Convective ZoneThe Sun is made up of different layers. From its center outward, the Sun’s layers include the core, the convective zone, the radiative zone, the…
Core(Kor) the central part of anything, such as the central mass of necrotic matter in a boil.
CoronaThe outermost layer of the Sun’s outer atmosphere. This halo of ions extends millions of miles into space and consists of a gas that is much thinner…
CoronagraphAn instrument designed to study the Sun’s corona by covering the bright disk of the Sun.
Coronal HoleAn area of the corona that appears dark when viewed in ultraviolet light. They are usually located around the poles of the Sun, but can occur at other…
Coronal Mass Ejection (CME)A catastrophic expansion of a part of the coronal magnetic field that causes a huge bubble of plasma and magnetic field to erupt from the Sun.
Cosmic Microwave Backgroun (CMB)Radiation filling the universe, remaining from the early, hot phase. (It is sometimes called the "primal glow.") Today this radiation has cooled to 2.
Cosmic RayHigh energy charged particles traveling through interstellar space at nearly the velocity of light. Most are produced in supernova explosions.
Cosmological Constant, ΛThe energy density of the smooth vacuum. Eisntein introduced it as a component of the universe but later withdrew it.
Cosmological PrincipleA principle invoked in cosmology that severely restricts the large variety of possible cosmological theories: On large scales, the Universe is homogeneous…
CosmologyThe study of the universe as a whole, of the contents, structure, and evolution of the universe from the beginning of time to the future.
Coupled to RadiationMatter, such as charged particles, that is strongly affected by radiation.
Critical DensityThe density of matter/energy that would just halt the expansion of the universe. The dividing line between a collapsing and an ever-expandinguniverse.
Curvature of SpacetimeAccording to Einstein's General Theory of Relativity, mass curves space and time.