<< < -ci cal Cal can Cap car cas cat cau cel cen cen cha cha cha che Chi chr cir cir civ Cla clo clu CNO coa coe coh col col col com com com com com com com com Com con con con con con con con con con con con con Coo cor cor cor cos cos cos cou cov cra cri cro cry cum cur cyc > >>
cascade shower ragbâr-e peyšâri, ~ âbšâri Fr.: gerbe Multiple generations of secondary cosmic rays when the primary particles produce a succession of secondaries which have the same effects as the primary. |
cascade transition gozareš-e peyšâri Fr.: transition en cascade A photon generation mechanism in an atom in which a transition initiates a series of secondary transitions from lower electronic levels. → cascade; → transition. |
case kâté Fr.: cas 1) An instance of the occurrence, or existence of something. M.E. cas, from O.Fr. cas "an event, happening, situation," from L. casus "a chance, occasion, opportunity; accident," literally "a falling," from cadere "to fall, sink, settle down" (Sp. caer, caida); Sp. caso; It. caso; Port. caso; PIE root *kad- "to fall;" cf. Skt. śad- "to fall down;" Pers. kat, as below. Kâté, from Iranian dialects/languages kat- "to fall" (with extension of the first vowel), as Laki: katen "to fall," kat "he/she fell," beko "fall!" (an insult); katyâ "fallen;" Lori: kat "event, error;" Kurd. (Soriani): kawtin "to fall, befall," kett "fallen;" Kurd. (Kurmanji): da.ketin "to fall down;" Lârestâni: kata "to fall;" Garkuyeyi: darkat, varkat "he/she fell (sudden death);" Gilaki (Langarud, Tâleš): katan "to fall," bakatam "I fell," dakatan "to fall (in a marsh, in a pit)," vakatan "to fall from tiredness, be exhausted," fakatan "to fall from (i.e., lose) reputation;" Tabari: dakətə "fallen," dakətən "to crash down," dakət.gu "stray cow;" Proto-Iranian *kat- "to fall;" cf. L. cadere, as above. Alternatively, from Proto-Ir. *kap-, *kaf- "to (be)fall, strike (down);" cf. Baluci kapag, kafag "to fall," kapt "(past tense) fell;" Bampuri kapte "fallen;" Kurd. (Sanandaj) kaften "to fall;" Gilaki jekaftan "to fall;" Nâyini derkaftan "to fall down." |
Casimir effect oskar-e Casimir Fr.: effet Casimir A small attractive force that appears between two close parallel uncharged plates in a vacuum. It is due to quantum vacuum fluctuations of the electromagnetic field. According to the quantum theory, the vacuum contains → virtual particles which are in a continuous state of fluctuation. Because the distance between the plates is very small, not every possible wavelength can exist in the space between the two plates, quite in contrast to the surrounding vacuum. The energy density decreases as the plates are moved closer, creating a negative pressure which pulls the plates together. The first successfully measurement of the effect was by Steve Lamoreaux in 1997. A more recent experiment in 2002 used a polystyrene sphere 200 μm in diameter coated in gold or aluminium. This was brought to within 0.1 μm of a flat disk coated with the same metals. The resulting attraction between them was monitored by the deviation of a laser beam. The Casimir force was measured to within 1% of the expected theoretical value. After the Dutch physicist Hendrik Casimir (1909-2000), who predicted the phenomenon in 1948; → effect. |
Cassegrain focus kânun-e Cassegrain (#) Fr.: foyer Cassegrain The main focus in → Cassegrain telescope. → Cassegrain telescope; → focus. |
Cassegrain telescope durbin Cassegrain, teleskop-e ~ (#) Fr.: Télecope Cassegrain A reflecting telescope whose primary mirror has a hole bored through the center to allow the reflected light from the convex secondary mirror be focused beyond the back end of the tube. Cassegrain, named after the French priest and school teacher Laurent Cassegrain (1629-1693), who invented this system in 1672; → telescope. |
Cassini division šekâf-e Cassini (#) Fr.: division de Cassini The main dark gap, 4,700 km wide, which divides Saturn's outermost A and B rings. Named after Jean-Dominique Cassini (1625-1712), French astronomer of Italian origin, who discovered the division in 1675; → division. |
Cassini state estât-e Cassini Fr.: état de Cassini A state characterizing a system which obeys → Cassini's laws. → Cassini's law; → state. |
Cassini's law qânun-e Cassini Fr.: loi de Cassini Any of the three empirical laws governing the rotational dynamics of the
→ Moon: Named after Jean-Dominique Cassini (1625-1712), French astronomer of Italian origin, who established these laws in 1693 (Traité de l'origine et du progrès de l'astronomie), ; → law. |
Cassini-Huygens Cassini-Huygens Fr.: Cassini-Huygens A joint endeavor of → NASA, → ESA, and the Italian space agency that sent a spacecraft to study the planet → Saturn and its system, including → Saturn's rings and its natural satellites. The spacecraft was 6.70 m × 4 m × 4 m and weighed about 6 tons. Cassini drew its electric power from the heat generated by the decay of 33 kg of → plutonium-238. The spacecraft carried 12 sophisticated observation and measuring instruments. Cassini-Huygens was launched on 15 October 1997. It used several → gravity assist manoeuvres to boost itself toward Saturn. It flew past Venus two times (April 1998 and June 1999), made → flybys of Earth (August 1999), and f Jupiter (December 2000). After 6 years and 8 months, covering about 8 billion km it entered Saturn orbit on July 1, 2004. It stayed there for 13 years and made detailed observations of the planet, its rings, and its moons. A scientific probe called Huygens was released on December 25, 2004 from the main spacecraft to parachute through the atmosphere to the surface of Saturn's largest and most interesting moon, → Titan. The data that Huygens transmitted during its final descent and for 72 minutes from the surface included 350 pictures that showed a shoreline with erosion features and a river delta. Cassini continued to orbit Saturn and complete many flybys of Saturn's moons. A particularly exciting discovery during its mission was that of → geysers of water ice and organic molecules at the south pole of → Enceladus, which erupt from an underground global ocean that could be a possible environment for life. Cassini's radar mapped much of Titan's surface and found large lakes of liquid → methane. Cassini also discovered six new moons and two new rings of Saturn. The mission was ended on September 15, 2017 when the spacecraft was crashed into Saturn's body and destroyed. This was the best way to avoid contaminating Saturn's moons with possible Earth microbes, because the moons may have the potential to support life. Named after two famous scientists. The Saturn orbiter is named after the Italian/french astronomer Jean-Domenique Cassini, who discovered the Saturnian satellites → Iapetus in 1671, → Rhea in 1672, and both → Tethys and → Dione in 1684. In 1675 he discovered what is known today as the → Cassini division, the narrow gap separating Saturn's rings into two parts. The Titan probe was named Huygens in honor of the Dutch scientist, Christiaan Huygens, who discovered Titan in 1655. |
Cassiopeia Kâsiopé (#) Fr.: Cassiopée A prominent circumpolar → constellation in the northern sky. Its brightest stars form a distinctive, turning W shape. Abbreviation Cas, genitive form Cassiopeiae. L. Cassiopea, from Gk. Kassiepeia, Andromeda's mother and king Cepheus of Ethiopia's wife, who boasted about her beauty to the degree that she considered herself more beautiful than the sea-nymphs. The consequences were awful for her daughter → Andromeda. |
Castor (α Geminorum) Kâstor Fr.: Castor The second brightest star in the → constellation → Gemini. This star has the identifier "alpha," but it is fainter than β Geminorum (→ Pollux). Castor was known as a main sequence, blue star of magnitude 1.98 and → spectral type A1. However, it is actually a → gravitationally bound family of six stars. The two brightest of the six, Castor A and Castor B, revolve around one another over a period of about 445 years. Castor A, the brighter of the two, is magnitude 1.9, while its companion is 3.0. Castor A is of spectral type A1 V and Castor B is Am. They are hotter than the Sun and about three times more massive, and lie 51 → light-years from Earth. Castor A and B are orbited by a third star called Castor C. It's a 9th magnitude → red dwarf (dMe1) and lies about one arc minute to the south. Castor C is about 1,000 → astronomical units from the bright pair and takes 14,000 years to orbit around them. Each of the three is a → spectroscopic binary making Castor a → sextuplet. Castor C is a → binary star of red dwarf stars a little more than half the size of the Sun. They revolve around one another evry 19 hours. The companions of Castor A and B are also smaller dwarf stars. In Gk. mythology, Castor and → Pollux were twin heroes called the Dioscuri. Castor was the son of Leda and Tyndareus, Pollux the son of Leda and Zeus. They were great warriors and were noted for their devotion to each other. After Castor was killed by Lynceus, Pollux implored Zeus to allow his brother to share his immortality with him. Zeus created the constellation Gemini in their honor. |
cata- katâ-, kâtâ-, kât-, kat- Fr.: cata- A prefix meaning "down," also "against; back; by, about; with, along," occurring originally in loanwords from Greek; variants cat- and cath-, as in catalog, cataclysm, cataract, cathode, catastrophe, etc. From Gk. kata-, before vowels kat-, from kata "down from, down to." Katâ-, kâtâ-, kât-, kat-, loan from Gk., as above. |
cataclysm gatlur Fr.: cataclysme 1) A devastating flood; deluge. From Fr. cataclysme, from L. cataclysmos "deluge," from Gk. kataklysmos, from kataklyzein "to inundate," from kata "down" + klyzein "to wash." Gatlur "great flood," from gat "great, large, big" [Mo'in, Dehxodâ] + lur "flood" [Mo'in, Dehxodâ], cf. Gk. louein "to wash," L. luere "to wash," Bret. laouer "trough," PIE *lou- "to wash." Variants of lur in Pers. dialects are: Lori, Kordi laf, lafow, lafaw, Tabari lé, all meaning "flood." |
cataclysmic gatluri Fr.: cataclysmique 1) Of, pertaining to, or resulting from a → cataclysm. |
cataclysmic variable vartande-ye gatluri Fr.: variable cataclysmique A → variable star that shows a sudden and dramatic change in brightness, including → flare stars, → novae, and some types of → symbiotic stars. They are believed to be very → close binary systems consisting of an → accreting → white dwarf → primary and an evolved → late-type secondary star that has filled its → Roche lobe. For systems with an → accretion disk, it is believed that a thermal instability is the cause of repetitive outbursts observed in cataclysmic variables called → dwarf novae. → cataclysmic; → variable. |
catalog kâtâlog (#) Fr.: catalogue A list or record of items systematically arranged with descriptive details. → Index Catalogue; → Messier catalog; → New General Catalogue. M.E. cathaloge, cateloge, from M.Fr. catalogue, from L.L. catalogus, from Gk. katalogos "a list, register," from kata "down, completely" + legein "to say, count," → -logy. Kâtâlog, loan from Fr., as above. |
catalog place jâ-ye kâtâlogi Fr.: position catalogue Same as catalog position and → mean catalog place. |
catalog position neheš-e kâtâlogi Fr.: position catalogue Same as catalog place and → mean catalog place. |
catastrophe negunzâr Fr.: catastrophe A great, often sudden calamity; a complete failure; a sudden violent change in the earth's surface. → cataclysm. From Gk. katastrophe "an overturning, ruin," from katastrephein "to overturn, ruin" from kata "down" + strephein "to turn." Negunzâr, from negun "overturned, inverted" + -zâr suffix denoting profusion, abundance, as in kârzâr "a field of battle; combat" šurezâr "unfertile, salty ground; nitrous earth," xoškzâr "arid land," and so forth. |
<< < -ci cal Cal can Cap car cas cat cau cel cen cen cha cha cha che Chi chr cir cir civ Cla clo clu CNO coa coe coh col col col com com com com com com com com Com con con con con con con con con con con con con Coo cor cor cor cos cos cos cou cov cra cri cro cry cum cur cyc > >>