oskar-e Kaiser Fr.: effet de Kaiser The observed peculiar velocities of galaxies in the → redshift space
of → galaxy clusters when the galaxies
undergo → infall toward a central mass. See also: Kaiser, N., 1987, MNRAS 227, 1; → effect. |
oskar-e Kaiser Fr.: effet de Kaiser The observed peculiar velocities of galaxies in the → redshift space
of → galaxy clusters when the galaxies
undergo → infall toward a central mass. See also: Kaiser, N., 1987, MNRAS 227, 1; → effect. |
engâre-ye Kant-Laplace Fr.: hypothèse de Kant-Laplace The hypothesis of the origin of the solar system proposed first by Kant (1755) and later by Laplace (1796). According to this hypothesis, the solar system began as a nebula of tenuous gas. Particles collided and gradually, under the influence of gravitation, the condensing gas took the form of a disk. Larger bodies formed, moving in circular orbits around the central condensation (the Sun). See also: Named after the German prominent philosopher Immanuel Kant (1724-1804) and the French great mathematician, physicist, and astronomer Pierre-Simon Marquis de Laplace (1749-1827); → hypothesis. |
engâre-ye Kant-Laplace Fr.: hypothèse de Kant-Laplace The hypothesis of the origin of the solar system proposed first by Kant (1755) and later by Laplace (1796). According to this hypothesis, the solar system began as a nebula of tenuous gas. Particles collided and gradually, under the influence of gravitation, the condensing gas took the form of a disk. Larger bodies formed, moving in circular orbits around the central condensation (the Sun). See also: Named after the German prominent philosopher Immanuel Kant (1724-1804) and the French great mathematician, physicist, and astronomer Pierre-Simon Marquis de Laplace (1749-1827); → hypothesis. |
kâon Fr.: kaon Any of a group of four short-lived → mesons distinguished by a → quantum number called → strangeness. Also called K meson and denoted K. They are positive, negative, or neutral and have a mass of about 495 MeV/c (about 970 times that of an → electron). See also: Kaon, from ka (for the letter K) + (mes)on, → meson. |
kâon Fr.: kaon Any of a group of four short-lived → mesons distinguished by a → quantum number called → strangeness. Also called K meson and denoted K. They are positive, negative, or neutral and have a mass of about 495 MeV/c (about 970 times that of an → electron). See also: Kaon, from ka (for the letter K) + (mes)on, → meson. |
sâzokâr-e κ Fr.: mécanisme κ A process based on the effects of → opacity (κ) that drives the
→ pulsations
of many types of variable stars. Consider a layer of material within a
star and suppose that it undergoes inward contraction. This inward
motion tends to compress the layer and increase the density. Therefore
the layer becomes more opaque (See also → partial ionization zone).
If a certain amount of flux comes from
the deeper layers it gets stuck in the high κ region. The energy
accumulates and heat builds up beneath it. The pressure rises below
the layer, pushing it outward. The layer expands as it moves
outward, cools and becomes more transparent to radiation. Energy can
now escape from below the layer, and pressure beneath the layer
diminishes. The layer falls inward and the cycle repeats. The
κ mechanism is believed to account for the pulsations of several
star families, including → Delta Scuti stars,
→ Beta Cephei variables, → Cepheids,
and → RR Lyrae stars See also: κ, the Gk. letter which denotes opacity; → mechanism. |
sâzokâr-e κ Fr.: mécanisme κ A process based on the effects of → opacity (κ) that drives the
→ pulsations
of many types of variable stars. Consider a layer of material within a
star and suppose that it undergoes inward contraction. This inward
motion tends to compress the layer and increase the density. Therefore
the layer becomes more opaque (See also → partial ionization zone).
If a certain amount of flux comes from
the deeper layers it gets stuck in the high κ region. The energy
accumulates and heat builds up beneath it. The pressure rises below
the layer, pushing it outward. The layer expands as it moves
outward, cools and becomes more transparent to radiation. Energy can
now escape from below the layer, and pressure beneath the layer
diminishes. The layer falls inward and the cycle repeats. The
κ mechanism is believed to account for the pulsations of several
star families, including → Delta Scuti stars,
→ Beta Cephei variables, → Cepheids,
and → RR Lyrae stars See also: κ, the Gk. letter which denotes opacity; → mechanism. |
marpel-e Kardashev Fr.: échelle de Kardashev A way of measuring a civilization’s technological advancement based upon how much usable energy it has at its disposal. The scale was originally designed in 1964 by the Russian astrophysicist Nikolai Kardashev (who was looking for signs of extraterrestrial life within cosmic signals). It has three base classes, each with an energy disposal level: Type I, Type II, and Type III. Type I designates a civilization that is capable of controlling the total energy of its home planet (1016 watts). Type II is an interstellar civilization, capable of harnessing the total energy output of a star (1026 W). And Type III represents a galactic civilization, capable of inhabiting and harnessing the energy of an entire galaxy (1036 W). The scale has since been expanded by another four. See also: The scale was originally designed in 1964 by the Russian astrophysicist Nikolai Kardashev (1932-); → scale. |
marpel-e Kardashev Fr.: échelle de Kardashev A way of measuring a civilization’s technological advancement based upon how much usable energy it has at its disposal. The scale was originally designed in 1964 by the Russian astrophysicist Nikolai Kardashev (who was looking for signs of extraterrestrial life within cosmic signals). It has three base classes, each with an energy disposal level: Type I, Type II, and Type III. Type I designates a civilization that is capable of controlling the total energy of its home planet (1016 watts). Type II is an interstellar civilization, capable of harnessing the total energy output of a star (1026 W). And Type III represents a galactic civilization, capable of inhabiting and harnessing the energy of an entire galaxy (1036 W). The scale has since been expanded by another four. See also: The scale was originally designed in 1964 by the Russian astrophysicist Nikolai Kardashev (1932-); → scale. |