The Milky Way

..
Myspace Layout Generator by TheMyspaceLayout.com

Generate your own contact table!

Myspace Extended Network Banners
Myspace Codes

Milky Way

The Milky Way (a translation of the Latin Via Lactea, in turn derived from the Greek ,,,,λ,,ξί,,ς (Galaxias) sometimes referred to simply as "the Galaxy"), is a barred spiral galaxy that is part of the Local Group of galaxies. Although the Milky Way is one of billions of galaxies in the observable universe, the Galaxy has special significance to humanity as it is the home galaxy of the planet Earth. The Milky Way galaxy is visible from Earth as a band of light in the night sky, and it is the appearance of this band of light which has inspired the name for our galaxy.
Some sources hold that, strictly speaking, the term Milky Way should refer exclusively to the band of light, while the full name Milky Way Galaxy, or alternatively the Galaxy should be used to describe our galaxy as a whole. It is unclear how widespread the usage of this convention is, however, and the term "Milky Way" is routinely used in either context.

Infrared image of the core of the Milky Way galaxy

The Milky Way as seen from Death Valley, 2007. This is a panoramic picture.

View from Earth

Visible from Earth as a hazy band of white light that is seen in the night sky, arching across the entire celestial sphere, the visual phenomenon of the Milky Way (as seen in the night sky) originates from stars and other material which lies within the galactic plane.
The Milky Way appears brightest in the direction of the constellation of Sagittarius, toward the galactic center. Relative to the celestial equator, it passes as far north as the constellation of Cassiopeia and as far south as the constellation of Crux, indicating the high inclination of Earth's equatorial plane and the plane of the ecliptic relative to the galactic plane. The fact that the Milky Way divides the night sky into two roughly equal hemispheres indicates that our Solar System lies close to the galactic plane. The Milky Way has a relatively low surface brightness, making it difficult to see from any urban or suburban location suffering from light pollution.

The Milky Way as it appears in a night sky time exposure from a dark location.

Size

The Milky Way is estimated to contain 200 billion, and up to 400 billion, stars (if small-mass stars predominate). As a guide to the relative physical scale of the Milky Way, if it were reduced to 130 km (80 mi) in diameter, the Solar System would be a mere 2 mm (0.08 inches) in width. The Galactic Halo extends outward, but is limited in size by the orbits of the two Milky Way satellites, the Large and the Small Magellanic Clouds, whose perigalacticon is at ~180,000 light-years.New discoveries indicate that the disk extends much farther than previously thought.
Age

It is extremely difficult to define the age at which the Milky Way formed, but the age of the oldest stars in the Galaxy is now estimated to be about 13.6 billion years, nearly as old as the Universe itself.
This estimate is based on research done in 2004 by astronomers Luca Pasquini, Piercarlo Bonifacio, Sofia Randich, Daniele Galli, and Raffaele G. Gratton. The team used the UV-Visual Echelle Spectrograph of the Very Large Telescope to measure, for the first time, the beryllium content of two stars in globular cluster NGC 6397. This allowed them to deduce the elapsed time between the rise of the first generation of stars in the entire Galaxy and the first generation of stars in the cluster, at 200 million to 300 million years. By including the estimated age of the stars in the globular cluster (13.4 ± 0.8 billion years), they estimated the age of the oldest stars in the Milky Way at 13.6 ± 0.8 billion years. (See also nucleocosmochronology.) Based upon this emerging science, the Galactic thin disk is estimated to have been formed between 8.3 ± 1.8 billion years ago

A green and red Perseid meteor is striking the sky just below the Milky Way in August 2007.

Composition and structure

In 2005, observations by the Spitzer Space Telescope backed up previously collected evidence that suggested the Milky Way is a barred spiral galaxy. It consists of a bar-shaped core region surrounded by a disk of gas, dust and stars. Within the disk region are several arm structures that spiral outward in a logarithmic spiral shape. The mass distribution within the Galaxy closely resembles the Sbc Hubble classification, which is a spiral-galaxy with relatively loosely-wound arms. It was only in the 1980s that astronomers began to suspect that the Milky Way is a barred spiral rather than an ordinary spiral, which observations in 2005 with the Spitzer Space Telescope have since confirmed, showing that the Galaxy's central bar is larger than previously suspected.This argues for a classification of type SBbc (loosely wound barred spiral). In 1970 Gérard de Vaucouleurs predicted that the Milky Way was of type SAB(rs)bc, where the "rs" indicates a broken ring structure around the core region.
As of 2006, the Milky Way's mass is thought to be about 5.8×1011 M☉comprising 200 to 400 billion stars. Its integrated absolute visual magnitude has been estimated to be −20.9. Most of the mass of the Galaxy is thought to be dark matter, forming a dark matter halo of an estimated 600–3000 billion solar masses (M☉) which is spread out relatively evenly.

NGC 7331 is often referred to as "the Milky Way's twin." This is what an observer from another galaxy might see when looking at our own.

Galactic center

The galactic disk, which bulges outward at the galactic center, has a diameter of between 70,000 and 100,000 light-years.The distance from the Sun to the galactic center is now estimated at 26,000 ± 1400 light-years, while older estimates could put the Sun as far as 35,000 light-years from the central bulge.
The galactic center harbors a compact object of very large mass (named Sagittarius A*), strongly suspected to be a supermassive black hole. Most galaxies are believed to have a supermassive black hole at their center.
The Galaxy's bar is thought to be about 27,000 light-years long, running through its center at a 44 ± 10 degree angle to the line between the Sun and the center of the Galaxy. It is composed primarily of red stars, believed to be ancient (see red dwarf, red giant). The bar is surrounded by a ring called the "5-kpc ring" that contains a large fraction of the molecular hydrogen present in the Galaxy, as well as most of the Milky Way's star formation activity. Viewed from the Andromeda Galaxy, it would be the brightest feature of our own galaxy.

The galactic center in the direction of Sagittarius. The primary stars of Sagittarius are indicated in red.

Spiral arms

Each spiral arm describes a logarithmic spiral (as do the arms of all spiral galaxies) with a pitch of approximately 12 degrees. There are believed to be four major spiral arms which all start at the Galaxy's center. These are named as follows, according to the image.

Observed and extrapolated structure of the spiral arms

color arm(s)

cyan 3-kpc and Perseus Arm
sky-blue Norma and Cygnus Arm (Along with a newly discovered extension)
chlorine-green Crux and Scutum Arm
pink Carina and Sagittarius Arm
orange Orion Arm (which contains the solar system and the Sun)

Outside of the major spiral arms is the Outer Ring or Monoceros Ring, a ring of stars around the Milky Way proposed by astronomers Brian Yanny and Heidi Jo Newberg, which consists of gas and stars torn from other galaxies billions of years ago.
As is typical for many galaxies, the distribution of mass in the Milky Way Galaxy is such that the orbital speed of most stars in the Galaxy does not depend strongly on its distance from the center. Away from the central bulge or outer rim, the typical stellar velocity is between 210 and 240 km/s. Hence the orbital period of the typical star is directly proportional only to the length of the path traveled. This is unlike in the Solar System where different orbits are also expected to have significantly different velocities associated with them, and is one of the major pieces of evidence for the existence of dark matter. Another interesting aspect is the so-called "wind-up problem" of the spiral arms. If one believes that the inner parts of the arms rotate faster than the outer part, then the Galaxy will wind up so much that the spiral structure will be thinned out. But this is not what is observed in spiral galaxies; instead, astronomers propose that the spiral arms form as a result of a matter-density wave emanating from the galactic center. This can be likened to a moving traffic jam on a highway—the cars are all moving, but there is always a region of slow-moving cars. Thus this results in several spiral arms where there are a lot of stars and gas. This model also agrees with enhanced star formation in or near spiral arms; the compressional waves increase the density of molecular Hydrogen and protostars form as a result.
Halo

The galactic disk is surrounded by a spheroid halo of old stars and globular clusters, of which 90% lie within 100,000 light-years,suggesting a stellar halo diameter of 200,000 light-years. However, a few globular clusters have been found farther, such as PAL 4 and AM1 at more than 200,000 light-years away from the galactic center. While the disk contains gas and dust obscuring the view in some wavelengths, the spheroid component does not. Active star formation takes place in the disk (especially in the spiral arms, which represent areas of high density), but not in the halo. Open clusters also occur primarily in the disk.
Recent discoveries have added dimension to the knowledge of the Milky Way's structure. With the discovery that the disc of the Andromeda Galaxy (M31) extends much further than previously thought, the possibility of the disk of the Galaxy extending further is apparent, and this is supported by evidence of the newly discovered Outer Arm extension of the Cygnus Arm. With the discovery of the Sagittarius Dwarf Elliptical Galaxy came the discovery of a ribbon of galactic debris as the polar orbit of Sagittarius and its interaction with the Milky Way tears it apart. Similarly, with the discovery of the Canis Major Dwarf Galaxy, it was found that a ring of galactic debris from its interaction with the Milky Way encircles the galactic disk.
On January 9, 2006, Mario Juric and others of Princeton University announced that the Sloan Digital Sky Survey of the northern sky found a huge and diffuse structure (spread out across an area around 5,000 times the size of a full moon) within the Milky Way that does not seem to fit within current models. The collection of stars rises close to perpendicular to the plane of the spiral arms of the Galaxy. The proposed likely interpretation is that a dwarf galaxy is merging with the Milky Way. This galaxy is tentatively named the Virgo Stellar Stream and is found in the direction of Virgo about 30,000 light-years away.
Sun's location

The Sun (and therefore the Earth and Solar System) may be found close to the inner rim of the Galaxy's Orion Arm, in the Local Fluff, at a hypothesized distance of 7.62±0.32 kpc from the Galactic Center.The distance between the local arm and the next arm out, the Perseus Arm, is about 6,500 light-years.The Sun, and thus the Solar System, is found in what scientists call the galactic habitable zone.
The Apex of the Sun's Way, or the solar apex, is the direction that the Sun travels through space in the Milky Way. The general direction of the Sun's galactic motion is towards the star Vega near the constellation of Hercules, at an angle of roughly 60 sky degrees to the direction of the Galactic Center. The Sun's orbit around the Galaxy is expected to be roughly elliptical with the addition of perturbations due to the galactic spiral arms and non-uniform mass distributions. In addition the Sun oscillates up and down relative to the galactic plane approximately 2.7 times per orbit. This is very similar to how a simple harmonic oscillator works with no drag force (dampening) term.
It takes the Solar System about 225–250 million years to complete one orbit (a galactic year),and so it is thought to have completed about 20–25 orbits during its lifetime or 0.0008 orbit since the origin of humans. The orbital speed of the solar system is 220 km/s, i.e., 1 light-year in ca. 1400 years, and 1 AU in 8 days

360-degree photographic panorama of the entire galaxy, from the viewpoint of the solar system

Environment

The Milky Way and the Andromeda Galaxy are a binary system of giant spiral galaxies. Together with their companion galaxies they form the Local Group, a group of some 50 closely bound galaxies. The Local Group is part of the Virgo Supercluster.
The Milky Way is orbited by two smaller galaxies and a number of dwarf galaxies in the Local Group. The largest of these is the Large Magellanic Cloud with a diameter of 20,000 light-years. It has a close companion, the Small Magellanic Cloud. The Magellanic Stream is a peculiar streamer of neutral hydrogen gas connecting these two small galaxies. The stream is thought to have been dragged from the Magellanic Clouds in tidal interactions with the Galaxy. Some of the dwarf galaxies orbiting the Milky Way are Canis Major Dwarf (the closest), Sagittarius Dwarf Elliptical Galaxy, Ursa Minor Dwarf, Sculptor Dwarf, Sextans Dwarf, Fornax Dwarf, and Leo I Dwarf. The smallest Milky Way dwarf galaxies are only 500 light-years in diameter. These include Carina Dwarf, Draco Dwarf, and Leo II Dwarf. There may still be undetected dwarf galaxies, which are dynamically bound to the Milky Way. Observations through the zone of avoidance are frequently detecting new distant and nearby galaxies. Some galaxies consisting mostly of gas and dust may also have evaded detection so far.
In January 2006, researchers reported that the heretofore unexplained warp in the disk of the Milky Way has now been mapped and found to be a ripple or vibration set up by the Large and Small Magellanic Clouds as they circle the Galaxy, causing vibrations at certain frequencies when they pass through its edges.Previously, these two galaxies, at around 2% of the mass of the Milky Way, were considered too small to influence the Milky Way. However, by taking into account dark matter, the movement of these two galaxies creates a wake that influences the larger Milky Way. Taking dark matter into account results in an approximately twentyfold increase in mass for the Galaxy. This calculation is according to a computer model made by Martin Weinberg of the University of Massachusetts, Amherst. In this model, the dark matter is spreading out from the galactic disc with the known gas layer. As a result, the model predicts that the gravitational effect of the Magellanic Clouds is amplified as they pass through the Galaxy.
Current measurements suggest the Andromeda Galaxy is approaching us at 100 to 140 kilometers per second. The Milky Way may collide with it in 3 to 4 billion years, depending on the importance of unknown lateral components to the galaxies' relative motion. If they collide, it is thought that the Sun and the other stars in the Milky Way will probably not collide with the stars of the Andromeda Galaxy, but that the two galaxies will merge to form a single elliptical galaxy over the course of about a billion years.
Velocity

In the general sense, the absolute velocity of any object through space is not a meaningful question according to Einstein's Special Theory of Relativity, which declares that there is no "preferred" inertial frame of reference in space with which to compare the Galaxy's motion. (Motion must always be specified with respect to another object.)
Many astronomers believe the Milky Way is moving at approximately 600 km per second relative to the observed locations of other nearby galaxies. Most recent estimates range from 130 km/s to 1,000 km/s. If the Galaxy is moving at 600 km/s, Earth travels 51.84 million km per day, or more than 18.9 billion km per year, about 4.5 times its closest distance from Pluto. The Galaxy is thought to be moving towards the constellation Hydra, and may someday become a close-knit member of the Virgo cluster of galaxies.
Another reference frame is provided by the Cosmic microwave background (CMB). The Milky Way is moving at around 552 km/s with respect to the photons of the CMB. This can be observed by satellites such as COBE and WMAP as a dipole contribution to the CMB, as photons in equilibrium at the CMB frame get blue-shifted in the direction of the motion and red-shifted in the opposite direction.
History

Etymology and beliefs

There are many creation myths around the world which explain the origin of the Milky Way and give it its name. The English phrase is a translation from Greek ,,,,λ,,ξί,,ς, Galaxias, which is derived from the word for milk (,,άλ,,, gala). This is also the origin of the word galaxy. In Greek myth, the Milky Way was caused by milk spilt by Hera when suckled by Heracles.
The term Milky Way first appeared in English literature in a poem by Chaucer.
"See yonder, lo, the Galaxyë
Which men clepeth the Milky Wey,
For hit is whyt."
—Geoffrey Chaucer, Geoffrey Chaucer The House of Fame, c. 1380.
In a large area from Central Asia to Africa, the name for the Milky Way is related to the word for straw. It has been claimed that this was spread by Arabs who in turn borrowed the word from Armenian.[35] In several Uralic and Turkic languages and in the Baltic languages the Milky Way is called the "Birds' Path". The Chinese name "Silver River" (銀河) is used throughout East Asia, including Korea. In Japanese, "Silver River" (銀河) means galaxies in general and the Milky Way is called the "Silver River System" (銀河系) or the "River of Heaven" (天の川). In Swedish, it is called Vintergatan, or "Winter Street", because the stars in the belt were used to predict time of the approaching winter.
Discovery

The Greek philosopher Democritus (450–370 BC) was the first known person to propose that the Milky Way might consist of distant stars. Actual proof of this came in 1610 when Galileo Galilei used a telescope to study the Milky Way and discovered that it was composed of a huge number of faint stars. In a treatise in 1755, Immanuel Kant, drawing on earlier work by Thomas Wright, speculated (correctly) that the Milky Way might be a rotating body of a huge number of stars, held together by gravitational forces akin to the Solar System but on much larger scales. The resulting disk of stars would be seen as a band on the sky from our perspective inside the disk. Kant also conjectured that some of the nebulae visible in the night sky might be separate "galaxies" themselves, similar to our own.
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 1785 by carefully counting the number of stars in different regions of the sky. He produced a diagram of the shape of the Galaxy with the solar system close to the center.
In 1845, 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.

The shape of the Milky Way as deduced from star counts by William Herschel in 1785; the solar system was assumed near center.

In 1917, Heber Curtis had observed the nova S Andromedae within the "Great Andromeda Nebula" (Messier object M31). 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 our galaxy. As a result he was able to come up with a distance estimate of 150,000 parsecs. He became a proponent of the "island universes" hypothesis, which held that the spiral nebulae were actually independent galaxies. In 1920 the Great Debate took place between Harlow Shapley and Heber Curtis, concerning the nature of the Milky Way, spiral nebulae, and the dimensions of the universe. To support his claim that the Great Andromeda Nebula was 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 matter was conclusively settled by Edwin Hubble in the early 1920s using a new telescope. He was able to resolve the outer parts of some spiral nebulae as collections of individual stars and identified some Cepheid variables, thus allowing him to estimate the distance to the nebulae: they were far too distant to be part of the Milky Way. In 1936 Hubble produced a classification system for galaxies that is used to this day, the Hubble sequence.

Photograph of the "Great Andromeda Nebula" from 1899, later identified as the Andromeda Galaxy

The Milky Way Galaxy

The Milky Way Galaxy is a spiral galaxy; our sun and solar system are a small part of it. Most of the stars that we can see are in the Milky Way Galaxy. The main plane of the Milky Way looks like a faint band of white in the night sky. The Milky Way is about 100,000 light-years in diameter and 1,000 light-years thick. There are about 2 x 10 11 stars in the Milky Way. This spiral galaxy formed about 14 billion years ago. It takes the sun roughly 250 million years to orbit once around the Milky Way. The Earth is about 26,000 light-years from the center of the Milky Way Galaxy. The major arms of the Milky Way galaxy are the Perseus Arm, Sagittarius Arm, Centaurus Arm, and Cygnus Arm; our Solar System is in a minor arm called the Orion Spur.

This panoramic view of the entire sky has been assembled from 51 wide-angle photographcs. The individual images were transformed to a cartesian frame based on galactic coordinates prior to assembly, thus eliminating the distortions introduced by the wide-angle lens.
The Milky Way galaxy is the spiral galaxy we call home, as do roughly 100 billion other stars. It looks very much like other spiral galaxies when viewed from above. There are spiral arms and a bright central part. The Sun is far from the center of the Galaxy, halfway to the edge of the Galaxy along the Orion spiral arm. The Sun is revolving around the center of the Galaxy at a speed of half a million miles per hour, yet it will still take 200 million years for it to go around once. Do you feel like you are moving at that speed through space? If you did, you would certainly need a seat belt! When we run, we feel the wind on our bodies because there are molecules which make up the air that push against our bodies. But there are very few molecules in the space between the stars. So there is nothing to push against our planet so that we "feel" like we are rushing around at half a million miles per hour.
Like other spiral galaxies, the Milky Way has a bulge, a disk, and a halo. Although all are parts of the same galaxy, each contains different objects. The halo and central bulge contain old stars and the disk is filled with gas, dust, and young stars. Our Sun is itself a fairly young star at only 5 billion years old. The Milky Way galaxy is at least 5 billion years older than that.Our Solar System is part of a huge "community" of stars, the Milky Way Galaxy. This chapter discusses the discovery of the nature of the Milky Way and its place in the larger cosmos.

THE DISCOVERY OF THE MILKY WAY GALAXY

The question of just how big our Universe is has been around since prehistory, but it wasn't until the development of the telescope and modern astronomy in the 17th century that astronomers decided to actually try to get a measured value for the size of the Universe.

Before that time, early astronomers such as Hipparchus had of course made catalogues of the visible stars, with the count going up to a few thousand. However, the telescope made far more many stars visible, and the number kept multiplying every time a new, more powerful telescope was put into service.
There was a still a reason, a very logical one, for believing that there was a finite number of stars in the Universe. In 1826, a German astronomer named Heinrich Wilhelm Matthaeus Olbers (1758:1840) pointed out that if there were an infinite number of stars in the sky, no matter where we looked, we would see a star, and the sky would be uniformly bright. This became known as "Olbers' paradox". There was a fallacy in it, one which Olbers could be easily forgiven for not seeing, but an explanation will have to be put off to a later chapter.
If the number of stars in the Universe was finite, then the other question was to ask how these stars were arranged. The night sky gave a big hint, in the form of a lovely pale band of light that cut across the heavens like a river. The Greeks called it the "Galaxias Kyklos (Milky Circle)", and the Romans called it the "Via Lactea (Milky Way)". The Greek term survived as the modern name "Galaxy". Even before the invention of the telescope some thinkers had wondered if it were made up of countless stars. This was basically confirmed by the telescope.
In 1784, the energetic William Herschel decided to characterize the distribution of stars in the Milky Way. Counting them all would take more than his lifetime, so he mapped out a set of 684 sampling regions over the sky, counted the stars in each one, and obtained the statistics on the samples. Herschel concluded that the density of stars was a maximum along the central plane of the Milky Way through the sky, and that it fell off gradually with the separation of stars from the plane, reaching a minimum at a right angle to that plane. However, the average density of stars along that plane, and any plane parallel to it, seemed constant.
Herschel concluded from these facts that the stars in the sky were arranged in a disk, with our Sun inside that disk, in fact fairly near the center of it. Based on the knowledge of stellar distances known at the time he even put together an estimate of the size of this disk, judging it to be about 8,000 light-years across, 1,500 light-years from top to bottom, and containing 300,000,000 stars.
Herschel was right about the disk, wrong about the Sun being near its center, and way too small in his estimate of its size. The size estimate was gradually increased into the early 20th century. In 1920, following exhaustive photographic sky surveys, the Dutch astronomer Jacobus Cornelius Kapteyn (1851:1922) estimated the Galaxy to be 55,000 light-years across and about 11,000 light-years from top to bottom. The notion that the Sun was at the center of the disk remained intact, but that notion was just about ready to fall over.
As discussed in an earlier chapter, Charles Messier had published his list of Messier objects in 1781, and William Herschel studied them carefully. Among the Messier objects were spherical puffballs of light, the brightest of them being "M13", located in the constellation Hercules. There were similar but less spectacular spherical nebulas in the Messier list. Nobody was sure if they were just luminous clouds of gas or collections of stars.
Herschel, using the excellent telescopes he had built himself, was able to get a better look at M13 and realized that it was in fact a dense collection of stars. Such objects became known as "globular clusters", as opposed to the more irregular clusters such as the Pleiades, which were eventually referred to as "open clusters". M13 became known as the "Great Hercules Cluster".
As telescopes and observations improved, more globular clusters were discovered. William Herschel's son, John Herschel (1792:1871), inspected the map of globular clusters known at the time and found something puzzling: the globular clusters were heavily concentrated in the sky in the direction of the constellation Sagittarius, and were absent in the opposite direction. There had to be some significance to this distribution, but he did not know what it might be.
It wasn't until the 1920s, with the discovery of the period-luminosity relationship of Cepheid variables, that the reason for this distribution of globular clusters was understood. The American astronomer Harlow Shapley (1885:1972) used the relationship to obtain distances to the globular clusters, and his analysis showed they were arranged in a sphere whose center was in the direction of the Sagittarius.
A simple understanding of the law of gravity suggested that the globular clusters were orbiting around the center of mass of the Milky Way. This meant that the Earth wasn't at the center of the Galaxy after all. Shapley's analysis showed that this center of mass was about 50,000 light-years away. As mentioned, the Cepheid yardstick had to be adjusted to compensate for reddening by the interstellar medium later, but that still gave a distance of about 27,000 light-years to the Galactic center. The Milky Way appeared to be about 100,000 light-years in diameter, and was presently estimated to contain about 100,000 million stars.
Astronomers were puzzled because star counts of the Milky Way gave about the same density at any place along its central plane. The answer to the puzzle came from the dark molecular clouds such as the Coal Sack. Their nature was not clearly understood at the time and they were simply known as "dark regions".
In 1919, the American astronomer Edward Emerson Barnard (1857:1923) published a list of 182 such dark regions. Barnard and the German astronomer Max Wolf (1863:1932) correctly suspected that these regions were not empty of stars, they were actually cold dark clouds that blocked out the light of stars behind them. Given that realization it didn't take too much imagination to realize that the presence of such "dark nebulas" in the plane of the Milky Way would create a curtain to hide the center of the Galaxy from view, at least in the visible region of the electromagnetic spectrum.