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Monoceros Takšâx (#) Fr.: Licorne The Unicorn. An extensive but faint constellation across the celestial equator , at 7h right ascension, 4° south declination. Abbreviation: Mon; genitive: Monocerotis. Monoceros "the unicorn," from O.Fr., from L., from Gk. monokeros, from → mono- "single" + keras "horn," kara "head," karena "head, top;" cf. Pers. soru "horn," sar "head;" L. cornu "horn," cerebrum "brain;" Skt. śiras- "head, chief;" O.E. horn "horn of an animal," also "wind instrument" (originally made from animal horns), from P.Gmc. *khurnaz (Ger. Horn, Du. horen), from PIE *ker- "head, horn, top, summit." Takšâx, from tak "single" → mono- + šâx "horn, branch" (Mid.Pers šâk; cf. Skt. sakha- "a branch, a limb;" Arm. cax; Lith. šaka; O.S. soxa; PIE *kakhâ "branch"). |
Monoceros Loop gerdâl-e takšâx Fr.: Boucle de la Licorne A faint filamentary loop of nebulosity about 1 kpc distant, the remnant of a supernova that occurred about 300,000 years ago. It contains the Rosette Nebula as well as the Cone Nebula. |
monochromatic takfâm (#) Fr.: monochromatique Characterized by light of one color or by radiation of a single wavelength or narrow range of wavelengths. |
monochromatic opacity kederi-ye takfâm Fr.: opacité monochromatique The sum of → absorption coefficient (κν) and → scattering coefficient (σν) at a given frequency: kν = κν + σν. See also the → Rosseland mean opacity. → monochromatic; → opacity. |
monomial taknâmin Fr.: 1) monôme; 2) monomial 1) A single algebraic term, such as 2xy, 125, 2x2.
The → degree of the monomial is the sum of the exponents of
all included variables. Constants have the monomial degree of 0. |
monomorphism tak-rixtmandi Fr.: monomorphisme A → morphismf : Y → X if, for any two morphisms u,v : Z → Y, f u = f v implies that u =v. |
monosemy takcemi Fr.: monosémie The fact of having only a single meaning. Same as → univocity. Compare with → polysemy. From → mono- "single," + sem, from sema "sign," → semantic, + -y. Takcemi, from tak-, → mono-, + cem, → meaning, + noun suffix -i. |
monotheism yektâ-yazdân-bâvari, yektâ-parasti (#) Fr.: monothéisme The belief or doctrine that there is only one → God. |
monotonic yeknavâxt (#) Fr.: monotone Of a mathematical function, either continuously increasing or decreasing. From Fr. monotone, from Gk. monotonos "monotonous, of one tone," from monos, → mono- "single, alone" + tonos "tone" + → -ic. Yeknavâxt "monotonous," from yek "one, single," + navâxt"rhythm," from navâxtan, navâzidan "to play an instrument; to gratify," navâ "music, song, melody;" Mid.Pers. nw'c "to treat kindly, honour," niwag "music, melody;" Proto-Iranian *ni-uac-, from *ni- (→ ni-) + *uac- "to speak, treat kindly," → word. |
monsoon bâdhâ-ye mowsemi (#) Fr.: mousson A seasonal change in wind direction bringing dry air or heavy rain in India and nearby lands. Monsoon, from Du. monssoen, from Port. monçao, from Ar. mausim "season." It was first applied to the winds over the Arabian Sea, which blow for six months from northeast and for six months from southwest, but it has been extended to similar winds in other parts of the world. Bâd, → "wind;" mowsem, related to mowsem, from Ar. mausim, as above. |
Monte Carlo Method raveš-e Monte Carlo Fr.: méthode de Monte Carlo A computer-intensive technique that relies on repeated random sampling of a statistical population to compute its results. Monte Carlo simulation is often used for approximate numerical computations when application of strict methods requires too much calculation, or when it is infeasible or impossible to compute an exact result with a deterministic algorithm. The term Monte Carlo was coined in the 1940s by physicists (Stanislaw Ulam, Enrico Fermi, John von Neumann, and Nicholas Metropolis) working on nuclear weapon projects in the Los Alamos National Laboratory. The name is a reference to a famous casino in Monaco which, it is said that, Ulam's uncle would borrow money to gamble at. → method. |
month mâh (#) Fr.: mois A period of time based on the revolution of the Moon around the Earth. Several types of months are defined: → anomalistic month; → draconic month; → sidereal month; → synodic month; → tropical month. O.E. monað, from P.Gmc. *mænoth- (O.N. manaðr, M.Du. manet, Du. maand, O.H.G. manod, Ger. Monat, Goth. menoþs "month"), related to *mænon-, → moon. Mâh and mâng in Pers. are variants of the same term, the dominant form being
mâh, while mâng (Av. from, see below) is used in classical literature
as well as in some dialects: Tabari, Kurd. mâng, Laki, Tâti, Taeši
mong, Šahmirzâdi,
Sangesari mung; Mid.Pers. mâh "moon, month;" O.Pers. māha-
"moon, month;" Av. māh- "month, moon," also māwngh-; cf.
Skt. mās- "moon, month;" Gk.
mene "moon," men "month;" L. mensis "month;"
O.C.S. meseci, Lith. menesis "moon, month;" O.Ir. mi,
Welsh mis, Bret. miz "month;"
O.E. mona; E. moon, month; Ger. Mond, Monat;
Du. maan; PIE base *me(n)ses- "moon, month." |
moon mâh (#), mâng (#) Fr.: Lune 1) Natural satellite of the Earth. Mass 7.35 x 1025 g = 1/81 or
0.0123 Earth's. Mean radius 1740 km = ~ 1/4 the Earth's; this relatively small
size ratio makes the Earth-Moon
system unique in the → solar system.
Mean density 3.34 g cm-3.
Mean distance from Earth 384,400 km.
→ Escape velocity 2.38 km s-1.
→ Surface gravity 162.2 cm s-2 = 0.165 Earth's.
→ Sidereal period 27d 7h 43m 11s. → Eccentricity
0.0549. → Inclination of → orbital plane
to → ecliptic 5° 8' 43''.
→ Obliquity 6° 41'.
→ Synodic period 29d 12h 44m 2s.9.
→ Orbital velocity 1.02 km s-1.
The Moon's average visual → Albedo is 0.12, a factor of
three smaller than that of Earth.
The Moon's → center of mass is displaced about 2 km in the
direction of Earth.
The average temperature on the surface of the Moon during the day is
107 °C. During the night, the average temperature drops to -153 °C.
Studies of lunar rock have shown that melting and separation must have begun
at least 4.5 x 109 years ago, so the → crust
of the Moon was beginning to form
a very short time after the → solar system itself.
Thickness of crust ~ 60 km; of mantle ~ 1000 km. Temperature of core ~ 1500 K.
It would have taken only 107 years to slow the Moon's rotation into
its present lock with its → orbital period.
Because of this → synchronous rotation,
the Moon revolves once on its axis
each time it orbits the Earth, thus always presenting the same face,
the nearside, toward Earth.
The Moon may have formed during a collision between the early
Earth and a Mars-sized rocky planet about 4.6 billion years ago;
→ Theia. O.E. mona, from P.Gmc. *mænon- (cf. O.S., O.H.G. mano, O.Fris. mona, O.N. mani, Du. maan, Ger. Mond, Goth. mena "moon"), cognate with Pers. mâh, as below, from PIE *me(n)ses- "moon, month." Mâh and mâng in Pers. are variants of the same term, the dominant form being
mâh, while mâng (Av. from, see below) is used in classical literature
as well as in some dialects: Tabari, Kurd. mâng, Laki, Tâti, Taelši
mong, Šahmirzâdi,
Sangesari mung; Mid.Pers. mâh "moon, month;" O.Pers. māha-
"moon, month;" Av. māh- "month, moon," also māwngh-; cf.
Skt. mās- "moon, month;" Gk.
mene "moon," men "month;" L. mensis "month;"
O.C.S. meseci, Lith. menesis "moon, month;" O.Ir. mi,
Welsh mis, Bret. miz "month;"
O.E. mona; E. moon, month; Ger. Mond, Monat;
Du. maan; PIE base *me(n)ses- "moon, month." |
Moon formation diseš-e Mâng Fr.: formation de la Lune Any of several theories about how the → Moon originated, among which: → fission theory, → capture theory, → co-formation theory, and → giant impact hypothesis. The model that is best supported by all the available data is the giant impact hypothesis. See also → canonical model. |
Moon halo hâle-ye mâh (#) Fr.: halo de la lune Same as → lunar halo. |
Moon's age 1) kohan-ruzi-ye mâh; 2) senn-e mâh Fr.: âge de la lune 1) The number of days that have elapsed since the last → conjunction
of the Sun and Moon. It is 7 days at
→ first quarter, 15 days at → full moon,
and 22 days at → third quarter. 1) Kohan-ruzi literally "age in days," from kohan-ruz "old in days,"
from kohan "old, ancient," kohné "worn;"
Mid.Pers. kahwan "old, aged, worn;"
pir; Mid.Pers. pir "old, aged, ancient;" Av. parô (adv.) "before,
before (of time)," in front (of space); cf. Skt. puáh, combining form
of puras "before (of time and place), in front, in advance;" mâh,
→ Moon. |
Moon's apsidal precession pišâyân-e habâki-ye mâng Fr.: précession absidiale de la Lune The → rotation of the Moon's → orbit within the → orbital plane, whereby the axes of the ellipse change direction. The Moon's → major axis makes one complete revolution every 8.85 Earth years, or 3,232.6054 days, as it rotates slowly in the same direction as the Moon itself (direct, or → prograde motion). The Moon's apsidal precession is a → relativistic effect, and should not be confused with its → axial procession. → Moon; → apsidal; → precession. |
Moon's prime meridian nimruzân-e naxosti-ye Mâng Fr.: méridien origine de la lune The line connecting the Moon's north pole with its south pole, and passing through the center of the lunar disk. The longitude of the Moon's prime meridian is zero degrees. → Moon; → prime meridian. |
moonbow mâhkamân Fr.: arc en ciel lunaire A rainbow that arises from the refraction and reflection of moonlight on rain drops or mist. |
moonlet mângcé Fr.: satellite mineur, lune mineure A very small natural or artificial satellite orbiting a planet. Saturn has dozens of moonlets often associated with its → planetary rings. |
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