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Milky Way Inhaltsstoffe

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Weitere Proteinriegel Weider Yippie! Recipe Rating Recipe Rating. The Milky Way is one of the largest galaxies in the group, second to the Andromeda Galaxy.

Therefore, present estimates of the total number are uncertain. This can be compared to the one trillion 10 12 stars of the neighbouring Andromeda Galaxy.

The stellar disc of the Milky Way does not have a sharp edge, a radius beyond which there are no stars. Rather, the number of stars drops smoothly with distance from the centre of the Galaxy.

Beyond a radius of about 40, light years, the number of stars drops much faster, for reasons that are not understood. Extending beyond the stellar disk is a much thicker disk of gas.

Recent observations indicate that the gaseous disk of the Milky Way has a thickness of around light years—twice the previously accepted value.

The Galactic halo extends outward, but is limited in size by the orbits of two Milky Way satellites, the Large and the Small Magellanic Clouds , whose closest approach is at about , light years.

The galactic disc, which bulges outward at the galactic center, has a diameter of 70—, light years. The exact distance from the Sun to the galactic center is debated.

The latest estimates give distances to the Galactic center of 25—28, light years. Movement of material around the galactic center shows that it has a compact object of very large mass.

The nature of the galaxy's bar is also actively debated, with estimates for its half-length and orientation spanning from 3,—16, light years short or a long bar and 10—50 degrees.

Individual galaxies, including the Milky Way, have peculiar velocities relative to the average flow. Thus, to compare the Milky Way to the Hubble flow, one must consider a volume large enough so that the expansion of the Universe dominates over local, random motions.

A large enough volume means that the mean motion of galaxies within this volume is equal to the Hubble flow. Another reference frame is provided by the cosmic microwave background CMB.

In western culture, the name "Milky Way" is derived from its appearance as a dim un-resolved "milky" glowing band arching across the night sky.

In Greek mythology , the Milky Way was formed after the trickster god Hermes suckled the infant Heracles at the breast of Hera , the queen of the gods, while she was asleep.

The Milky Way, or "milk circle", was just one of 11 "circles" the Greeks identified in the sky, others being the zodiac , the meridian , the horizon , the equator , the tropics of Cancer and Capricorn , Arctic and Antarctic circles , and two colure circles passing through both poles.

In his view, the Milky Way is celestial. This idea would be influential later in the Islamic world.

Because of this, it was likened to milk in color. Proof of the Milky Way consisting of many stars came in when Galileo Galilei used a telescope to study the Milky Way and discovered that it is composed of a huge number of faint stars.

Wright and Kant also conjectured that some of the nebulae visible in the night sky might be separate "galaxies" themselves, similar to our own.

Kant referred to both the Milky Way and the "extragalactic nebulae" as "island universes", a term still current up to the s. The first attempt to describe the shape of the Milky Way and the position of the Sun within it was carried out by William Herschel in by carefully counting the number of stars in different regions of the visible sky.

He produced a diagram of the shape of the Milky Way with the Solar System close to the center. In , Lord Rosse constructed a new telescope and was able to distinguish between elliptical and spiral-shaped nebulae.

He also managed to make out individual point sources in some of these nebulae, lending credence to Kant's earlier conjecture. In , studying the proper motions of stars, Jacobus Kapteyn reported that these were not random, as it was believed in that time; stars could be divided into two streams, moving in nearly opposite directions.

Searching the photographic record, he found 11 more novae. Curtis noticed that these novae were, on average, 10 magnitudes fainter than those that occurred within the Milky Way.

As a result, he was able to come up with a distance estimate of , parsecs. He became a proponent of the "island universes" hypothesis, which held that the spiral nebulae were independent galaxies.

To support his claim that the Great Andromeda Nebula is an external galaxy, Curtis noted the appearance of dark lanes resembling the dust clouds in the Milky Way, as well as the significant Doppler shift.

The controversy was conclusively settled by Edwin Hubble in the early s using the Mount Wilson observatory 2.

With the light-gathering power of this new telescope, he was able to produce astronomical photographs that resolved the outer parts of some spiral nebulae as collections of individual stars.

He was also able to identify some Cepheid variables that he could use as a benchmark to estimate the distance to the nebulae.

He found that the Andromeda Nebula is , parsecs from the Sun, far too distant to be part of the Milky Way. The ESA spacecraft Gaia provides distance estimates by determining the parallax of a billion stars and is mapping the Milky Way with four planned releases of maps in , , and From Wikipedia, the free encyclopedia.

This article is about the galaxy. For other uses, see Milky Way disambiguation. Spiral galaxy containing our Solar System.

Play media. New view of the Milky Way with four clearly defined and symmetric spiral arms [88]. Artist's conception of the spiral structure of the Milky Way with two major stellar arms and a bar [89].

Main article: Galactic quadrant. Main article: Galactic Center. Further information: Spiral galaxy. Diagram of the Sun's location in the Milky Way, the angles represent longitudes in the galactic coordinate system.

Main article: Galaxy formation and evolution. Diagram of the galaxies in the Local Group relative to the Milky Way. The position of the Local Group within the Laniakea Supercluster.

Main article: Local Group. Astronomy portal. Pasachoff in his textbook Astronomy: From the Earth to the Universe states the term Milky Way should refer exclusively to the band of light that the galaxy forms in the night sky , while the galaxy should receive the full name Milky Way Galaxy ; however, this does not reflect a firm consensus in the astronomical community.

See: Pasachoff, Jay M. Astronomy: From the Earth to the Universe. Harcourt School. Combined with a color index of 0.

Note that determining the absolute magnitude of the Milky Way is very difficult, because Earth is inside it. Chandra X-ray Observatory. Harvard-Smithsonian Center for Astrophysics.

January 6, Archived from the original on March 17, Retrieved May 20, October 3, The Astrophysical Journal. Bibcode : ApJ Archived PDF from the original on December 2, Retrieved July 31, Space Science Reviews.

Bibcode : SSRv.. Archived from the original on May 31, Retrieved May 30, July Monthly Notices of the Royal Astronomical Society. February 11, Archived from the original on March 24, Retrieved March 27, Universe Today.

Archived from the original on September 24, Retrieved November 28, The Astronomy and Astrophysics Review. Izdatel'stvo Nauka.

Archived from the original on March 4, Retrieved April 5, Galaxies in the Universe: An Introduction. December 10, Online Etymology Dictionary.

Archived from the original on May 27, Pioneers of Light and Sound. Compass Point Books. Archived from the original on November 20, Archived from the original on March 21, Retrieved April 8, Bulletin of the National Research Council.

Bibcode : BuNRC March 23, ScienceNews Journal. Archived from the original on August 13, Retrieved August 13, Martialay March 11, Rensselaer Polytechnic Institute.

Archived from the original on March 13, Archived from the original on June 7, Retrieved June 9, Archived from the original on March 2, NASA Blueshift.

Archived from the original on January 25, January 11, Bibcode : Natur. Archived from the original on January 3, Retrieved January 3, Archived from the original on March 8, Retrieved March 8, February 2, In some it was possible to view massive star clusters still in the process of formation.

Thick clouds of dust in the Milky Way can be studied by still another means. Many such objects contain detectable amounts of molecules that emit radio radiation at wavelengths that allow them to be identified and analyzed.

More than 50 different molecules, including carbon monoxide and formaldehyde , and radicals have been detected in dust clouds. The stars in the Galaxy, especially along the Milky Way, reveal the presence of a general, all-pervasive interstellar medium by the way in which they gradually fade with distance.

This occurs primarily because of interstellar dust , which obscures and reddens starlight. On the average, stars near the Sun are dimmed by a factor of two for every 3, light-years.

Thus, a star that is 6, light-years away in the plane of the Galaxy will appear four times fainter than it would otherwise were it not for the interstellar dust.

Another way in which the effects of interstellar dust become apparent is through the polarization of background starlight.

Dust is aligned in space to some extent, and this results in selective absorption such that there is a preferred plane of vibration for the light waves.

The electric vectors tend to lie preferentially along the galactic plane, though there are areas where the distribution is more complicated.

It is likely that the polarization arises because the dust grains are partially aligned by the galactic magnetic field. If the dust grains are paramagnetic so that they act somewhat like a magnet, then the general magnetic field, though very weak, can in time line up the grains with their short axes in the direction of the field.

As a consequence, the directions of polarization for stars in different parts of the sky make it possible to plot the direction of the magnetic field in the Milky Way.

The dust is accompanied by gas , which is thinly dispersed among the stars, filling the space between them. This interstellar gas consists mostly of hydrogen in its neutral form.

Radio telescopes can detect neutral hydrogen because it emits radiation at a wavelength of 21 cm. Such radio wavelength is long enough to penetrate interstellar dust and so can be detected from all parts of the Galaxy.

Most of what astronomers have learned about the large-scale structure and motions of the Galaxy has been derived from the radio waves of interstellar neutral hydrogen.

The distance to the gas detected is not easily determined. Statistical arguments must be used in many cases, but the velocities of the gas, when compared with the velocities found for stars and those anticipated on the basis of the dynamics of the Galaxy, provide useful clues as to the location of the different sources of hydrogen radio emission.

Even before they first detected the emission from neutral hydrogen in , astronomers were aware of interstellar gas. Minor components of the gas, such as sodium and calcium , absorb light at specific wavelengths, and they thus cause the appearance of absorption lines in the spectra of the stars that lie beyond the gas.

Since the lines originating from stars are usually different, it is possible to distinguish the lines of the interstellar gas and to measure both the density and velocity of the gas.

Frequently it is even possible to observe the effects of several concentrations of interstellar gas between Earth and the background stars and thereby determine the kinematics of the gas in different parts of the Galaxy.

The Magellanic Clouds were recognized early in the 20th century as companion objects to the Galaxy. When American astronomer Edwin Hubble established the extragalactic nature of what we now call galaxies, it became plain that the Clouds had to be separate systems, both of the irregular class and more than , light-years distant.

The current best values for their distances are , and , light-years for the Large and Small Clouds, respectively.

Additional close companions have been found, all of them small and inconspicuous objects of the dwarf elliptical class. The core of this galaxy is about 90, light-years distant.

Distances for them range from approximately , to , light-years. The grouping of these galaxies around the Milky Way Galaxy is mimicked in the case of the Andromeda Galaxy , which is also accompanied by several dwarf companions.

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