راه ِ شیری
Râh-e Širi (#)
Fr.: Voie lactée
The diffuse glowing band of light seen on dark nights spanning the sky as a
great circle. It is produced by light from stars and nebulae in the
→ Galactic plane. The apparent form of the Milky Way in the
sky results from a geometrical effect created by our location in the outlying regions
of a huge, flattened disk of stars. → Milky Way galaxy.
From L.L. galaxias "Milky Way," from Gk. galaxis kyklos
"emilky circle," from gala (gen. galaktos) "milk."
In Gk. mythology, Jupiter, hoping to immortalize his infant son Hercules
(who was born to a mortal woman), placed the baby on Juno's breast. Her milk
spilled up, forming the Milky Way.
Milky, from milk; M.E.; O.E. meol(o)c, (Anglian)
milc; cf. Gr. Milch, Goth. miluks; akin to L.
mulgere, Gk amelgein "to milk;" PIE base *melg- "wiping, stroking;"
Râh, → way; širi,
adj. of šir "milk;" Mid.Pers. šir;
cf. Skt. ksira- "milk."
کهکشان ِ راه ِ شیری
kahkešân-e râh-e širi (#)
Fr.: Voie lactée
A → spiral galaxy, of which the
→ solar system is a small part.
It is the second largest in our → Local Group of galaxies.
The Milky Way is a disk-shaped system,
with a diameter of between 80,000 and 100,000 → light-years
and a thickness of about 2,000 light-years, containing more than
1011 stars. The stars are divided into two main categories,
→ Population II stars and
→ Population I stars.
The core, or nucleus, of the Galaxy is
surrounded by an ellipsoidal central → bulge
that measures some 15,000 light-years in
diameter and about 6,000 light-years in the direction perpendicular to
the plane of the disk. Surrounding the bulge and extending in a near
spherical distribution above and below the → Galactic plane
is the → Galactic halo. The halo contains about 200
→ globular clusters and an extremely thinly scattered
population of individual stars.
The Sun is located just over half way out from the center to the edge
of the disk at a distance of about 25,000 light-years.
In common with other stars, the Sun
revolves around the → Galactic Center.
Its → orbital velocity is
about 220 km s-1 and its → orbital period
is about 225 million
years. Overall, the Galaxy exhibits → differential rotation,
that is stars and
gas clouds closer to the center have shorter orbital periods than
those that are located further out.
The → spiral arms of the Milky Way lie
within its disk, where bright → young stars,
→ H II regions, and → molecular clouds
of gas and dust are concentrated into curved "arms" that appear to
radiate from the central bulge in a spiral pattern. The Galaxy's
spiral pattern consists of several major arms and a number of shorter
segments, one of which, the → Orion arm,
contains the Sun and the Orion star-forming region.
have shown that the stars in the central bulge are arranged in an
elongated → galactic bar,
about twice as long as it is wide, that is seen nearly
end on from the present location of the solar system. The exact
center, or nucleus, of the Galaxy coincides with a strong source of
radio emission, called → Sagittarius A,
that is less than 15
astronomical units in diameter. Observations of the speeds at which clouds of
ionized gas are revolving round the → Galactic center
imply that several
million solar masses of material are concentrated within a region of
about one light-year in radius. Since only about half of this mass can
be accounted for by stars, it seems likely that the balance (about 2.5
million solar masses) is contained in a central black hole and that
accretion onto this black hole is the underlying source of the energy
radiated by Sagittarius A.
The Milky Way also has a → dark matter component.
The Galactic → rotation curve
there is a large amount of invisible → non-baryonic
surrounding the whole Galaxy.
→ Milky Way; → galaxy.
راژمان ِ راه ِ شیری
râžmân-e râh-e širi
Fr.: Voie lactée
The huge star system of which the Sun is a member. Same as the Galaxy or
the Milky Way galaxy.
→ Milky Way; → system.
ستارهی ِ گریزان
Fr.: étoile en fuite
A massive, young, and hot star that is moving quickly
through space. Runaways are probably propelled through space
from a binary star when its companion has exploded as a supernova, or ejected from
a stellar cluster by the dynamical interactions in the system.
→ run; away, from O.E. aweg, earlier on weg
"on from this (that) place;" → star.
Setâré, → star; gorizân present participle of
"to escape; to flee, run away;" Mid.Pers. virextan;
Proto-Iranian *vi-raik, from vi- "apart, asunder"
+ *raik; Av. raek- "to leave, set free, let off;"
Mid./Mod.Pers. reg/rig (in mordé-rig "inheritance");
Skt. ric- "to leave," rinakti "gives up, evacuates;"
Gk. leipein "to leave;" L. linquere "to leave;" from PIE *linkw-, from
*leikw- "to leave behind" (cf. Goth. leihvan; O.E. lænan
"to lend;" O.H.G. lihan "to borrow;" O.N. lan "loan").
واژیرش ِ گرماهستهای ِ لگام گسیخته
vâžireš-e garmâhaste-yi-e legâm gosixté
Fr.: emballement thermonucléaire
1) The uncontrolled → fusion of hydrogen into helium.
2) A → thermonuclear reaction process occurring at electron
→ degenerate conditions in stellar material, such as
in → Type Ia supernovae.
→ thermonuclear; → runaway.
Vâžireš, → reaction;
garmâhaste-yi, → thermonuclear;
legâm gosixté literally "rampant, unrestrained," from
legâm "bridle, rein" + gosixté "broken off, torn away,"
p.p. of gosixtan "to tear away, to break off."
Fr.: voie, chemin
A road, track, or path.
M.E. wei(gh)e, wai, from
O.E. weg "road, path;" cf. Du. weg,
O.H.G. weg, Ger. Weg, Goth. wigs "way;" PIE base
*wegh- "to move."
Râh "way, path"
(from Mid.Pers. râh, râs "way, street," also rah, ras "chariot;"
from Proto-Iranian *rāθa-; cf.
Av. raθa- "chariot;" Skt. rátha- "car, chariot,"
rathyā- "road;" L. rota "wheel," rotare "to revolve, roll;"
Lith. ratas "wheel;" O.H.G. rad; Ger. Rad; Du. rad;
O.Ir. roth; PIE *roto- "to run, to turn, to roll");