nebula

listen to the pronunciation of nebula
Englisch - Türkisch
{i} bulutsu uzak yıldız topluluğu
bulutsu

Bir bulutsu; toz, hidrojen, helyum ve diğer iyonize gazlardan oluşmuş bir yıldızlararası buluttur. - A nebula is an interstellar cloud of dust, hydrogen, helium and other ionized gases.

nebula
gözbebeğine arız olan duman
pek uzak olduğundan bulut gibi görünen yıldızlar yığını
{ç} --s (neb'yılız)/--e (neb'yıli) i., (Gökbilim) bulutsu, nebülöz
spiral nebula sarmal yapılı yıldız takımı
bulutsu/nebula
(Tıp) (nebulae). Göz bebeğine arız olan duman, nebula
(Askeri) bulutlu

Relevante Übersetzungen

nebulae
(Askeri) BULUTSULAR, SAMANYOLU BULUT SULARI: Mevcudiyetlerini ya parlak bir yıldızın aydınlatması veya göğün belirli bir bölgesindeki yıldızların ışığını aşikar şekilde zayıflatmalarıyla belli eden yıldızlararası madde bulutları; oluşmamış yıldızlardır
dark nebula
(Astronomi) kara bulutsu
dark nebula
kara nebula
dust nebula
toz nebulası
gaseous nebula
gaz nebula, gaz bulutsu
nebulae
bulutsular
planetary nebula
gezegensi bulut
solar nebula
(Astronomi) Güneş bulutumsusu
solar nebula
(Astronomi) Güneş sisteminde uzak olduğundan bulut gibi görünen yıldızlar yığını
the crab nebula
Yengeç Bulutsusu
dust nebula
(Astronomi) toz nebula
dust nebula
(Astronomi) toz bulutsu
nebular
{s} nebulaya ait
nebular
bulut gibi görünen yıldız kümesinenebular hypothesis güneş sisteminin aslında bulut şeklinde bir madde yığınından ileri gelmiş olduğu varsayımı
nebular
bulutsuya ait
nebular
(sıfat) nebulaya ait
solar nebula
güneş nebulası
Türkisch - Türkisch
Bulutsu
Roma mimarlığında,dalgaları andıran sürekli bezeme
Uzayda bulunan gaz bulutsularına verilen isim
Uzayda ekseni çevresinde yavaşça dönen, gaz ve tozlardan oluşmuş gök varlığı
Englisch - Englisch
A cloud in outer space consisting of gas or dust (e.g. a cloud formed after a star explodes)
a gaseous body of unorganized stellar substance
–A cloud of interstellar gas and dust, often illuminated by stars
A cloud of dense gas and/or dust in interstellar space or surrounding a star They appear indistinct or fuzzy and the term encompasses a wide variety of phenomena For example, star forming regions, shells of gas ejected from evolved stars (``planetary nebulae) and the remants of exploded stars (``supernovae'') can all be called ``nebulae'' Before their nature and distances were determined galaxies were termed spiral nebulae
A cloudy appearance in the urine
cloudiness of the urine
Cloud of gas and dust usually left by a dead star Such clouds are where most stars form They are primarily located by reflecting light from stars, emitting light from young stars which lie within, or by blocking the view of background stars behind them See also: open cluster
A cloud of gas or dust among the stars A nebula may be luminous (like a neon sign) if excited by a nearby star, or, if it is dusty it may blot out the background of starlight In the past, this term was also used for galaxies because they appeared nebulous
A diffuse mass of interstellar dust and gas
A glowing cloud of gas or dust reflecting the light of nearby stars Here is an example of the ring nebula taken here with the Ultima 2000 telescope and a CCD camera
A term used by optical astronomers to denote any object that resembles a cloud, either bright or dark, and is not stellar in appearance
(plural=nebulae) A mass of gas and dust in space This image is the Crab nebula
{i} cloud of cosmic gas or dust in outer space (Astronomy); clouded spot or faint corneal opacity on the cornea (Medicine); cloudiness or cloudy appearance in the urine (Medicine); oily preparation used in a nebulizer
Bright or dark cloud of gas and dust, which may contain stars
a diffuse mass of interstellar dust and gas A reflection nebula shines by light reflected from nearby stars An emission nebula shines by emitting light as electrons recombine with protons to form hydrogen The electrons were made free by the ultraviolet light of a nearby star shining on a cloud of hydrogen gas A planetary nebula results from the explosion of a solar-like type star
n a scattered mass of interstellar dust and/or gas, visible as light patches or dark areas, depending on the way the mass reflects or absorbs light
a medicinal liquid preparation intended for use in an atomizer
Originally a fixed, extended and somewhat fuzzy white haze observed in the sky with a telescope Many of these objects can now be resolved into clouds of individual stars and have been identified as galaxies The gaseous nebulae, however, cannot be resolved into individual stars and consist, for the most part, or interstellar dust and gas In some of these gaseous nebulae the gas atoms have been ionised by ultraviolet radiation from nearby stars and light is emitted as these ions interact with the free electrons in the gas These are called emission nebulae In the dark nebulae, there are no nearby stars and these objects are consequently dark; they can only be detected by what they obscure
a gas or dust cloud in space NIGHT the dark hours between sunset and sunrise NORTH to the left of a person standing east where the sun rises
A white spot or a slight opacity of the cornea
a cloud of interstellar gas and dust made up mostly of hydrogen and helium Nebulas come in different forms; planetary nebulas, supernova remnants, and diffuse nebulas When stars form, they form as a result of a nebula condensing
A faint, cloudlike, self- luminous mass of matter situated beyond the solar system among the stars
A nebula is a cloud of dust and gas in space. New stars are produced from nebulae. Any of various tenuous clouds of gas and dust in interstellar space. Nebulae constitute only a small percentage of a galaxy's mass. Dark nebulae (e.g., the Coalsack) are very dense, cold molecular clouds that appear as large, obscure, irregularly shaped areas in the sky. Bright nebulae (e.g., the Crab Nebula, planetary nebula) appear as faintly luminous, glowing surfaces; they emit their own light or reflect that of stars near them. The term nebula also formerly referred to galaxies outside the Milky Way Galaxy. Crab Nebula Gum Nebula Orion Nebula planetary nebula solar nebula
a collection of gas and/or dust
A cloud of dust and gas in space, usually illuminated by one or more stars Nebulae represent the raw material the stars are made of
A large, tenuous cloud of interstellar dust and gas in space created of the remnants of an exploded star or a galaxy in the making The dust and gas can pose a hazard to the ship when traveling at high impulse speeds
(pathology) a faint cloudy spot on the cornea
(plural: nebulae) A cloud of gas and dust, usually found in the spiral arms of a galaxy
A huge cloud of dust and gases found in space It usually signifies the beginning or ending of a star
A cloud of gas and/or dust in interstellar space (The word nebula in Latin means "cloud"; its plural is "nebulae '') Nebulae can make themselves apparent by glowing (as "emission nebulae''), by scattering light from stars within them (as "reflection nebulae''), or by blocking light from things behind them (as "obscuration nebulae'')
True nebulæ are gaseous; but very distant star clusters often appear like them in the telescope
An interstellar cloud of gas and dust
A term used to describe celestial objects which have a fuzzy, or nebulous, appearance (from the Latin for cloud ), such as gas, or dust, clouds Galaxies were once described thus
Cloud of dust or gas in space which is sometimes made visible by the reflected light from nearby stars Nebulae are the birthplace of stars
(pathology) a faint cloudy spot on the cornea an immense cloud of gas (mainly hydrogen) and dust in interstellar space cloudiness of the urine a medicinal liquid preparation intended for use in an atomizer
an immense cloud of gas (mainly hydrogen) and dust in interstellar space
A diffuse mass of interstellar dust and gas Neutrino A fundamental particle supposedly produced in massive numbers by the nuclear reactions in stars; they are very hard to detect because the vast majority of them pass completely through the Earth without interacting Nuclear Fusion A nuclear process whereby several small nuclei are combined to make a larger one whose mass is slightly smaller than the sum of the small ones The difference in mass is converted to energy by Einstein's famous equivalence E=mc2 This is the source of the Sun's energy and, ultimately, of (almost) all energy on Earth
Cloud of glowing gas in space, lit up by hot young stars within it

Relevante Übersetzungen

Great Nebula in Andromeda
a great nebula, white nebula, and spiral nebula in the constellation of Andromeda, now known to be the Andromeda Galaxy, a spiral galaxy
Orion Nebula
A diffuse nebula visible in the night sky below Orion's Belt; it is approximately 40 light years across. It is one of the brightest nebulae visible to the naked eye and is the closest region of stellar formation to Earth
dark nebula
A type of nebula that unlike other types of nebulae does not emit or reflect light and therefore appears as a starless region in the sky

Horsehead Nebula is a typical dark nebula, and is famous for resembling the head of a horse.

nebular
Of or pertaining to a nebula
planetary nebula
A nebulosity surrounding a dying star, consisting of material expelled by the star
preplanetary nebula
A stage in stellar evolution when a star starts to shed its outer layers before coming a true planetary nebula
protoplanetary nebula
A stage in stellar evolution when a star starts to shed its outer layers before coming a true planetary nebula
radio nebula
Any nebula that emits radio waves
reflection nebula
A nebula that consist of dust which reflects starlight and appears blue in photographs

The Pleiades are surrounded by a reflection nebula.

solar nebula
A disc-shaped cloud of gas and dust left over from the formation of the Sun
spiral nebula
a spiral-shaped white nebula; these were generally determined to be spiral galaxies in the 20th century
spiral nebula
a spiral-shaped nebula
white nebula
a nebula that appears white in colouration through a high-powered telescope (nebulae often appear to have some hint of colour through a powerful telescope, but white when not using a powerful instrument); these nebulae were generally to be determined to be galaxies in the 20th century
solar nebula
(Astronomi) The rotating flattened cloud of gas and dust from which the sun and the rest of the bodies in the solar system
spiral nebula
A galaxy exhibiting a central nucleus or barred structure from which extend curved arms of higher luminosity ― called also spiral galaxy
A nebula
nebulosity
A nebula
nubecula
Crab Nebula
Bright nebula in the constellation Taurus, about 5,000 light-years from Earth. Roughly 12 light-years in diameter, it is the remnant of a supernova, first observed by Chinese and other astronomers in 1054, that was visible in daylight for 23 days and at night for almost two years. Identified as a nebula 1731, it was named (for its form) in the mid-19th century. In 1921 it was discovered to be still expanding; the present rate is about 700 mi/second (1,100 km/second). The Crab is one of the few astronomical objects from which electromagnetic radiation has been detected over the entire measurable spectrum. In the late 1960s a pulsar, thought to be the collapsed remnant star of the supernova, was found near its centre
Gum Nebula
Largest known emission nebula in terms of how much of the sky it occupies as seen from Earth, extending over about 35° in the southern constellations Puppis and Vela. A complex of diffuse, glowing gas too faint to see with the unaided eye, it was discovered in the 1950s. It lies roughly 1,000 light-years from Earth and may be the remnant of an ancient supernova
Orion Nebula
Bright nebula, faintly visible to the unaided eye in the sword of the hunter's figure in the constellation Orion. About 1,500 light-years from Earth, it contains hundreds of very hot young stars clustered about a group of four massive stars known as the Trapezium. Radiation primarily from these four stars excites the nebula to glow. Discovered in the early 17th century, it was the first nebula to be photographed (1880)
Ring Nebula
A planetary nebula in the constellation Lyra
crab nebula
a remnant of a supernova detected first in 1054 AD
diffuse nebula
a cluster of stars within an intricate cloud of gas and dust
emission nebula
A nebula that absorbs ultraviolet radiation from stars and reemits it as visible light
nebulae
From the Latin work meaning 'fuzzy' A cloud like aggregation of gas and/or dust associated with star forming regions and in the case of planetary nebula, the death of stars Nebulae are typically classified as
nebulae
Before the `Great Debate', this term referred to any resolved nebulosity observed in the sky It had also been noticed that a there were different types of nebulae (singular: nebula), one of which had spiral structure and so were referred to as "spiral nebulae " Today "spiral nebulae" are referred to as "spiral galaxies" and "nebulae" refer to large gas and dust clouds that populate a galaxy
nebulae
A diffuse of interstellar dust or gas Nebulae come from the Latin word for mist or cloud Nebula comes in several different forms to include emission nebula, reflection nebula, and dark nebulae just to name a few The gas in nebulae is mostly H (Hydrogen) gas
nebulae
definition
nebulae
plural of nebula
nebular
of or relating to or resembling a nebula; "the nebular hypothesis of the origin of the solar system"
nebular
Of or pertaining to nebulæ; of the nature of, or resembling, a nebula
nebular
Or or pertaining to a nebula
nebular
of or relating to or resembling a nebula; "the nebular hypothesis of the origin of the solar system
nebular
resembling a cloud
nebular
{s} pertaining to a cloud of cosmic gas and dust in outer space (Astronomy)
nebulas
plural of nebula
planetary nebula
a nebula that was once thought to be a star with its planets but is now thought to be a very hot star surrounded by an expanding envelope of ionized gases that emit a fluorescent glow because of intense radiation from the star
planetary nebula
A nebula, such as the Ring Nebula, consisting of a hot, blue-white, central star surrounded by an envelope of expanding gas. Any of a class of bright nebulae that may somewhat resemble planets when viewed through a small telescope but are, in fact, expanding shells of luminous gas around dying stars. A planetary nebula is the outer envelope shed by a red giant star not massive enough to become a supernova. Instead, the star's intensely hot core becomes exposed (see white dwarf star) and ionizes the surrounding shell of gas, which is expanding at tens of miles per second
solar nebula
Gaseous cloud from which, in the nebular hypothesis of the origin of the solar system, the Sun and planets formed by condensation. In 1755 Immanuel Kant suggested that a nebula gradually pulled together by its own gravity developed into the Sun and planets. Pierre-Simon Laplace in 1796 proposed a similar model, in which a rotating and contracting cloud of gas the young Sun shed concentric rings of matter that condensed into the planets. James Clerk Maxwell showed that if all the matter in the known planets had once been distributed this way, shearing forces would have prevented such condensation. Another objection was that the Sun has less angular momentum than the theory seems to require. In the early 20th century most astronomers preferred the collision theory: that the planets formed as a result of a close approach to the Sun by another star. Eventually, however, stronger objections were mounted to the collision theory than to the nebular hypothesis, and a modified version of the latter, in which a rotating matter disk gave rise to the planets through successively larger aglommerations from dust grains through planetesimals and protoplanets, became the prevailing theory of the solar system's origin
Türkisch - Englisch
nebula

Relevante Übersetzungen

kara nebula
dark nebula
spiral nebula
spiral nebula
nebula

    Silbentrennung

    ne·bu·la

    Türkische aussprache

    nebyılı

    Aussprache

    /ˈnebyələ/ /ˈnɛbjələ/

    Etymologie

    [ 'ne-by&-l& ] (noun.) circa 1738. From Latin nebula (“little cloud", "mist”). Akin to Greek νεφέλη, "cloud", German Nebel, "mist", "nebula", Old Norse nifl.
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