apparent sidereal day ruz-e axtari-ye padidâr Fr.: jour sidéral apparent The time interval between two successive → upper transits of the → true equinox of date. |
apparent sidereal time zamân-e axtari-ye padidâr Fr.: temps sidéral apparent The → mean sidereal time corrected for the → nutation and shift in the obliquity of the ecliptic that occurs as a result of the Moon's gravitational effect. Apparent sidereal time differs from mean sidereal time in that the → true vernal equinox point is used. |
apsides, line of xatt-e habâkhâ Fr.: ligne des apsides The line connecting the two apsides, i.e. the major axis of an elliptical orbit. → apsis. |
apsis (pl. apsides) habâk Fr.: apside The point of greatest or least distance of the orbit of a celestial body from a center of attraction. The closest point is the → periapsis, the further point the → apoapsis. L. apsis "arch, vault," from Gk. hapsis "loop, arch," from haptein "fasten together". Mod.Pers. habâk "top of the head; the summit of a mountain". |
consider âgâridan Fr.: considérer To think carefully about, especially in order to make a decision; contemplate; reflect on (dictionary.com). M.E. consideren, from O.Fr. considerer "reflect on, study," from L. considerare "to examine, look at closely," literally "to observe the stars," from → com- "with" + sider (stem of sidus) "star, group of stars," → sideral. Âgâridan, from intensive prefix â- + gâr-, variants gar-, gâl- "to consider, observe," as in engâridan "to suppose," negaristan "to observe, look, notice," segâl "thought," segâlidan "to think, meditate," ultimately from Proto-Iranian *kar- "to observe, to consider;" cf. Av. kar- "to remember; to impress on memory;" Skt. kal- "to observe, consider," kalayati "considers, observes." |
considerable âgâridani Fr.: considérable 1) Rather large or great in size, distance, extent, etc. |
consideration âgâreš Fr.: considération The act or an instance of considering. |
countryside rustâ (#) Fr.: campagne A rural area; he inhabitants of a countryside. Rustâ, from Mid.Pers. rôstâk, rôtastâk "village, district, river-bed;" loaned into Armenian rotstak, ərotastak "district." |
Greenwich Apparent Sidereal Time (GAST) zamân-e axtari-ye padidâr-e Greenwich Fr.: temps sidéral apparent de Greenwich The → Greenwich Mean Sidereal Time corrected for → nutation. Therefore, it is measured with respect to the → true vernal equinox. GAST and GMST differ by the → equation of the equinoxes. → Greenwich Meridian; → apparent; → sidereal; → time. |
Greenwich Mean Sidereal Time (GMST) zamân-e axtari-ye miyângin-e Greenwich Fr.: temps sidéral moyen de Greenwich The → sidereal time related to the angle between the → prime meridian and the → mean vernal equinox, measured in the plane of the equator. → mean; → Greenwich Meridian; → sidereal; → time. |
Greenwich sidereal date ruz-e axtari-ye Greenwich Fr.: jour sidéeal de Greenwich The number and fraction of → mean sidereal days elapsed on the → Greenwich meridian since 12h January 1, 4773 BC (mean sidereal). → Greenwich meridian; → sidereal; → date. |
Greenwich sidereal day number šomâre-ye ruz-e axtari-ye Greenwich Fr.: nombre du jour sidéral de Greenwich The integral part of the → Greenwich sidereal date. |
Heaviside layer lâye-ye Heaviside (#) Fr.: couche de Heaviside English physicist Oliver Heaviside (1850-1925). |
highly siderophile element (HSE) bonpâr-e besyâr âhandust Fr.: élément hautement sidérophile A → chemical element that is → geochemically characterized as having a strong → affinity to partition into → metals relative to → silicates. The highly siderophile elements, → ruthenium (Ru), → rhodium (Rh), → palladium (Pd), → rhenium (Re), → osmium (Os), → iridium (Ir), → platinum (Pt), and → gold (Au), are of interest to planetary scientists because they give insights into the early history of → accretion and → differentiation. HSEs prefer to reside in the metal of planetary cores. Therefore, the HSEs found in planetary → mantles are considered to be overabundant relative to their known preferences for metal over silicate. Therefore, it has been inferred that processes other than → equilibrium partitioning have been responsible for establishing the abundances of → mantle siderophiles. A detailed understanding of the absolute → concentrations and relative abundances of the HSEs may therefore give important insights into the earliest history of a planet (Jones et al., 2003, Chemical Geology 196, 21). From Gk. sidero-, from sideros "iron" + → -phile. |
Kennelly-Heaviside layer lâye-ye Kennelly-Heaviside (#) Fr.: couche de Kennelly-Heaviside One of several layers in the Earth's ionosphere occurring at 90-150 km above the ground. It reflects medium-frequency radio waves whereby radio waves can be propagated beyond the horizon. Named after the American electrical engineer Arthur Edwin Kennelly (1861-1939) and the English physicist Oliver Heaviside (1850-1925), who independently predicted the existence of the reflecting layer in 1902; → layer. |
line of apsides xatt-e habâkhâ Fr.: ligne des apsides Of an elliptical orbit, the straight line drawn from the → perigee to the → apogee. |
local sidereal time zamân-e axtari-ye mahali Fr.: temps sidéral local Local time measured by the apparent motion of the stars. It is the most useful form of sidereal time since it gives the right ascension of a transiting celestial object at a given location. |
lunar far side ruy-e dur-e mâng Fr.: face cachée de la Lune The Moon's hemisphere which is not visible from the Earth. The Moon always shows the same face to the Earth, because Earth and Moon are → tidally locked. This means that the period of → lunar rotation on it axis is the same as its sidereal revolution period around the Earth (→ sidereal month). In other words, the Moon is in → synchronous rotation with the Earth. As a result, the same side always faces the Earth. To be more precise, taking the lunar → libration into account, the Moon presents about 59% of its surface to Earth. → libration in longitude, → libration in latitude, → physical libration, → geometrical libration. |
lunar sidereal orbital period dowre-ye madâri-ye axtari-ye mâng Fr.: période orbitale sidérale de la Lune Same as → sidereal month. |
mean sidereal day ruz-e axtari-ye miyângin Fr.: jour sidéral moyen The average time interval between two successive → upper transits of the → mean equinox. |