BepiColombo BepiColombo Fr.: BepiColombo A → European Space Agency (ESA) mission aimed at studying → Mercury, the least explored planet in the inner → Solar System. It was launched on 20 October 2018. Among several goals, BepiColombo will make a complete map of Mercury at different wavelengths. It will chart the planet's → mineralogy and elemental → composition, determine whether the interior of the planet is molten or not, and investigate the extent and origin of Mercury's → magnetic field, the properties of its → magnetosphere, and history of the planet. The trajectory will also be modified by eight planetary flybys: of Earth in April 2020, Venus in 2020 and 2021, and then six times of Mercury itself between 2021 and 2025. BepiColombo will enter Mercury orbit in December 2025. BepiColombo is a joint mission between ESA and the Japanese Aerospace Exploration Agency (JAXA), executed under ESA leadership. Named after Giuseppe (Bepi) Colombo (1920-1984), a scientist who studied Mercury's orbital motion in detail as well as orbits and interplanetary travel in general. |
Ecliptic Plane Input Catalogue (EPIC) kâtâlog-e darundâd-e hâmon-e hurpehi Fr.: catalogue d'entrée du plan de l'écliptique A catalog of fields along the → ecliptic observed by the → K2 mission. The catalog is hosted at the → Mikulski Archive for Space Telescopes (MAST). |
epi- api- Fr.: épi- Prefix meaning "upon, at, close upon (in space or time), on the occasion of, in addition." Gk. epi- "upon, at, close upon (in space or time), on the occasion of, in addition," cognate with O.Pers./Av. apiy-, aipi- "upon, toward, along; also; however;" Skt. api "also, besides." Prefix api-, from O.Pers./Av. apiy-, aipi-, as above. |
epicycle 1) falak-e tadvir (#); 2) apicarxé Fr.: épicycle 1) In → Ptolemaic system, a circular
→ orbit of a body around a point that itself
orbits circularly another point. Such a system was formulated to explain some
→ planetary
orbits in terms of → circular
motions in a → geocentric
cosmology. 1) Falak-e tadvir, from Ar. falak al-tadwir, from falak
"sphere" + tadwir "causing to turn in a circle." |
epicyclic apicarxe-yi Fr.: épicyclique Of or pertaining to an → epicycle. |
epicyclic frequency basâmad-e apicarxe-yi Fr.: fréquence épicyclique In the → epicyclic theory of Galactic rotation, the frequency at which a star in the → Galactic disk describes an ellipse around its mean circular orbit. The epicyclic frequency relates to the → Oort's constants. In the solar neighborhood the epicyclic frequency is about 32 km s-1 kpc-1. |
epicyclic oscillation naveš-e apicarxe-yi Fr.: oscillation épicyclique In a → disk galaxy, the motion of a star about the orbital → guiding center when it is displaced radially. See also → epicyclic frequency, → epicyclic theory. → epicyclic; → oscillation. |
epicyclic theory negare-ye apicarxe-yi Fr.: théorie épicyclique The theory that describes the Galactic dynamics, that is the orbits of stars and gas clouds in the → Galactic disk, as well as the spiral → density wave. Formulated by Bertil Lindblad (1895-1965), the epicyclic theory assumes that orbits are circular with small deviations. Star orbits are described by the superposition of two motions: i) a rotation of the star (epicenter) around the Galactic center at the circular angular velocity, Ω, and ii) a retrograde elliptical motion at → epicyclic frequency, κ. The epicyclic motion in the Galactic plane occurs in a retrograde sense to conserve → angular momentum. In general Ω and κ are different and, therefore, orbits do not close. However, seen by an observer who rotates with the epicenter, orbits are closed ellipses. |
epicycloid apicarxzâd Fr.: épicycloïde A curve traced by a point of a circle that rolls on the outside of a fixed circle. This curve was described by the Gk. mathematicians and astronomer Hipparchus, who made use of it to account for the apparent movement of many of the heavenly bodies. |
Epimetheus Epimeteus Fr.: Épiméthée The fifth of → Saturn's known satellites. It has a mean radius of 55 x 69 km and orbits its planet at a mean distance of 151,422 km. It shares the same → horseshoe orbit with → Janus. Epimetheus was discovered by Richard L. Walker in 1966. Also known as Saturn XI. In Gk. mythology, brother of → Prometheus and → Atlas, and husband of → Pandora. His task was to populate the Earth with animals. |
epimorphism api-rixtmandi Fr.: épimorphisme A → morphism f : Y → X if, for any two morphisms u,v : X → Z, u f = v f implies u = v. |
episode apyâ Fr.: épisode 1) An incident in the course of a series of events. From Fr. épisode from Gk. epeisodion "addition," noun use of neuter of epeisodios "coming in besides," from → epi- "in addition" + eisodos "a coming in, entrance" (from eis"into" + hodos "way," → period). Apyâ, literally "coming in besides," from api-, → epi-, + â- present stem of âmadan "to come," → rise. |
episodic apyâyi Fr.: épisodique 1) Pertaining to or of the nature of an episode. |
epistemology šenaxtšenâsi (#) Fr.: épistémologie A branch of philosophy that investigates the possibility, origins, nature, methods, and limits of human knowledge. From Gk. episteme "knowledge," from Ionic Gk. epistasthai "to understand," literally "overstand," from → epi- "over, near" + histasthai "to stand;" cognate with Pers. istâdan "to stand," → standard; PIE base *sta- "to stand." |
eyepiece cašmi (#) Fr.: oculaire A → lens system, also known as an → ocular, used to → magnify the → image formed by the → objective of a → telescope. Cašmi "ocular," adj. of cašm→ eye + -i adj. suffix. |
Greisen-Zatsepin-Kuzmin limit (GZK) hadd-e Greisen-Zatsepin-Kuzmin Fr.: limite de Greisen-Zatsepin-Kuzmin A theoretical limit of approximately 6 × 1019 → electron-volts for the energy of → cosmic rays above which they would lose energy in their interaction with the → cosmic microwave radiation background photons. Cosmic ray protons with these energies produce → pions on blackbody photons via the Δ resonance according to: γCMB + p → p + π0, or γCMB + p → n + π+, thereby losing a large fraction of their energy. These interactions would reduce the energy of the cosmic rays to below the GZK limit. Due to this phenomenon, → Ultra-high-energy cosmic rays are absorbed within about 50 Mpc. Named after Kenneth Greisen (1966), Physical Review Letters 16, 748 and Georgiy Zatsepin & Vadim Kuzmin (1966), Journal of Experimental and Theoretical Physics Letters 4, 78; → limit. |
Kellner eyepiece cešmi-ye Kellner (#) Fr.: oculaire de Kellner The first achromatic eyepiece consisting of a convex lens and a plano-convex lens. The convex surfaces are turned toward one another. Named after the inventor Carl Kellner (1826-1855), a German engineer and optician; → eyepiece |
orthoscopic eyepiece cešmi-ye ardâbini Fr.: oculaire orthoscopique A telescopic eyepiece that produces a wide field of view (between 40° and 50°). The eyepiece consists of a single element lens that is normally plano-convex, and a cemented triplet that is usually symmetrical. → orthoscopic; → eyepiece. |
parallelepiped parâsuruyé, lowzivâr Fr.: parallélépipède A solid figure whose six bases are → parallelograms, opposite pairs being identical and parallel. From Gk. parallelepipedon, from parallelos, → parallel + epipedon "plane surface," from neuter of epipedos "flat," from → epi- + pedon "ground," cognate with L. ped-, pes, → foot. Parâsuruyé, from parâsu, → parallel, + ruyé, → surface. Lowzivâr, from lowzi, → rhombus + -vâr, → -oid. |
Ramsden eyepiece cešmi-ye Ramsden (#) Fr.: oculaire de Ramsden An eyepiece consisting of two planoconvex lenses of the same focal length, placed with the convex sides facing each other and with a separation between the lenses of about two-thirds of the focal length of each. Named after Jesse Ramsden (1735-1800), English maker of astronomical instruments; → eyepiece. |