The Milky Way is a spiral galaxy that contains over 200 billion stars. It is 100,000 light years in diameter and located in the Local Group of galaxies. The Sun is located about 26,000 light years from the center of the Milky Way in one of the galaxy's spiral arms. The Milky Way consists of a bar-shaped core surrounded by a disk containing stars, gas and dust, as well as four major spiral arms.

1. Milky Way
.

2. The Milky Way, sometimes
called simply the Galaxy, is
the galaxy in which our Solar
System is located. It is a spiral
galaxy that is part of the Local
Group of galaxies. It is one of
billions of galaxies in the
observable universe.
Milky Way Galaxy
Infrared image of the core of the Milky Way galaxy
Observation data
Type
SBbc (barred spiral galaxy)
Diameter 100,000 light years
Thickness 1,000 light years (stars)
Number of stars 200 to 400 billion
Oldest known star 13.2 billion years[1]
Mass 5.8 × 1011
M☉
Sun's distance to galactic
center
26,000 ± 1,400 light-years
Sun's galactic rotation
period
220 million years (negative
rotation)
Spiral pattern rotation
period
50 million years[2]
Bar pattern rotation period 15 to 18 million years[2]
Speed relative to CMB rest
frame
552 km/s[3]

3. Its name is a translation of the Latin Via Lactea, in turn translated from the Greek
Γαλαξίας (Galaxias), referring to the pale band of light formed by the galactic plane as
seen from Earth (see etymology of galaxy). Some sources hold that, strictly speaking, 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, or
alternatively the Galaxy. However, it is unclear how widespread this convention is, and
the term Milky Way is routinely used in either context.
Appearance from Earth
The Milky Way galaxy, as viewed from Earth, itself situated on a spur off one of the
spiral arms of the galaxy (see Sun's location and neighborhood), appears as a hazy and in
some areas dark band of white light in the night sky arching across the entire celestial
sphere and originating from stars and other material that lie within the galactic plane. The
plane of the Milky Way is inclined by about 60° to the ecliptic (the plane of the Earth's
orbit), with the North Galactic Pole situated at right ascension 12h 49m, declination
+27.4° (B1950) near beta Comae Berenices. The South Galactic Pole is near alpha
Sculptoris.
The center of the galaxy is in the direction of Sagittarius, and the Milky Way then
"passes" (going westward) through Scorpius, Ara, Norma, Triangulum Australe,
Circinus, Centaurus, Musca, Crux, Carina, Vela, Puppis, Canis Major, Monoceros, Orion
& Gemini, Taurus, Auriga, Perseus, Andromeda, Cassiopeia, Cepheus & Lacerta,
Cygnus, Vulpecula, Sagitta, Aquila, Ophiuchus, Scutum, and back to Sagittarius.
The Milky Way looks 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.
360-degree photographic panorama of the
galaxy. The Milky Way as seen from Death Valley,
2007. This is a panoramic picture.

4. Size
The stellar disk of the Milky Way galaxy is approximately 100,000 light-years
(9.5×1017
km) in diameter, and is believed to be, on average, about 1,000 ly
(9.5×1015
km) thick.[7]
It is estimated to contain at least 200 billion stars[8]
and possibly up
to 400 billion stars,[9]
the exact figure depending on the number of very low-mass stars,
which is highly uncertain. 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 12,000 ly (1.1×1017
km)—twice the previously accepted value.[10]
As a guide to
the relative physical scale of the Milky Way, if it were reduced to 100 m in diameter, the
Solar System, including the Oort Cloud, would be no more than 1 mm in width.
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 perigalacticon is at
~180,000 ly (1.7×1018
km).[11]
At this distance or beyond, the orbits of most halo objects
would be disrupted by the Magellanic Clouds, and the objects would likely be ejected
from the vicinity of the Milky Way.
Recent measurements by the Very Long Baseline Array (VLBA) have revealed that the
Milky Way is much larger than previously thought. The size of our home galaxy is now
considered to be roughly similar to that of our largest local neighbour, the Andromeda
galaxy. By using the VLBA to measure the apparent shift of far-flung star-forming
regions when the Earth is on opposite sides of the Sun, the researchers were able to
measure the distance to those regions using fewer assumptions than prior efforts. The
newer and more accurate estimate of the galaxy's rotational speed (and in turn the amount
of dark matter contained by the galaxy) puts the figure at about 254 km/s, significantly
higher than the widely accepted value of 220 km/s.[12]
This in turn implies that the Milky
Way has a total mass equivalent to around 3 trillion Suns, about 50% more massive than
previously thought.[13]
Age
A green and red Perseid meteor streaks across the sky just below the Milky Way in
August 2007.
Main articles: Galaxy formation and evolution and nucleocosmochronology

5. It is extremely difficult to define the age at which the Milky Way formed, but the age of
the oldest star in the Galaxy yet discovered, HE 1523-0901, is estimated to be about 13.2
billion years, nearly as old as the Universe itself.[1]
This estimate is based on research by a team of astronomers in 2004 using 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.[14][citation needed]
From this
research, 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 was deduced to be 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. Based upon this emerging science, the Galactic thin disk is estimated to
have been formed between 6.5 and 10.1 billion years ago. The Milky Way is believed to
be approximently 5.6 million years old.
Composition and structure
The Milky Way is thought to be a barred spiral galaxy. Messier 109 is one possible
analog.[15]
The Galaxy consists of a bar-shaped core region surrounded by a disk of gas, dust and
stars forming four distinct arm structures spiralling outward in a logarithmic spiral shape
(see Spiral arms). The mass distribution within the Galaxy closely resembles the Sbc
Hubble classification, which is a spiral galaxy with relatively loosely-wound arms.[16]
Astronomers first began to suspect that the Milky Way is a barred spiral galaxy in the
1990s[17]
rather than an ordinary spiral galaxy. Their suspicions were confirmed by the
Spitzer Space Telescope observations in 2005[18]
which showed the Galaxy's central bar
to be larger than previously suspected. The Milky Way's mass is thought to be about
5.8 × 1011
solar masses (M☉)[19][20][21]
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 M☉ which is spread out relatively uniformly.[21]

6. The galactic center in the direction of Sagittarius. The primary stars of Sagittarius are
indicated in red.
Galactic center
Main article: Galactic Center
The galactic disc, which bulges outward at the galactic center, has a diameter of between
70,000 and 100,000 light-years.[22]
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 as determined by the
motion of material around the center.[23]
The intense radio source named Sagittarius A*,
thought to mark the center of the Milky Way, is newly confirmed to be a supermassive
black hole. For a photo see Chandra X-ray Observatory; Jan. 6, 2003 Most galaxies are
believed to have a supermassive black hole at their center.[24]
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.[25]
Spiral arms
Observed and extrapolated structure of the 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 near the Galaxy's center. These are named as follows, according to the image at
right:
color arm(s)

7. cyan 3-kpc and Perseus Arm
purple Norma and Cygnus Arm (Along with a newly discovered extension)
green Scutum-Crux Arm
pink Carina and Sagittarius Arm
There are at least two smaller arms or spurs, including:
orang
e
Orion Arm (which contains our own Solar System and 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.[26]
Hence the orbital period of the typical star is directly
proportional only to the length of the path traveled. This is unlike the situation within the
Solar System, where two-body gravitational dynamics dominate and different orbits are
expected to have significantly different velocities associated with them. This difference 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.

8. Artist's conception of the spiral structure of the Milky Way with two major stellar arms
and a bar.
Observations presented in 2008 by Robert Benjamin of the University of Wisconsin-
Whitewater suggest that the Milky Way possesses only two major stellar arms: the
Perseus arm and the Scutum-Centaurus arm. The rest of the arms are minor or adjunct
arms.
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,[28]
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 which obscure 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,[29]
the possibility of the disk of our own Galaxy extending
further is apparent, and this is supported by evidence of the newly discovered Outer Arm
extension of the Cygnus Arm.[30]
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 Jurić 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

9. tentatively named the Virgo Stellar Stream and is found in the direction of Virgo about
30,000 light-years away.
Sun's location and neighborhood
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 inside the Local Bubble, and in the Gould
Belt, at a distance of 7.62±0.32 kpc (~25,000±1,000 ly) from the Galactic Center.[31][32][33]
[34]
The distance between the local arm and the next arm out, the Perseus Arm, is about
6,500 light-years.[35]
The Sun, and thus the Solar System, is found in the galactic
habitable zone.
There are about 208 stars brighter than absolute magnitude 8.5 within 15 parsecs of the
Sun, giving a density of 0.0147 such stars per cubic parsec, or 0.000424 per cubic light-
year (from List of nearest bright stars). On the other hand, there are 64 known stars (of
any magnitude, not counting 4 brown dwarfs) within 5 parsecs of the Sun, giving a
density of 0.122 stars per cubic parsec, or 0.00352 per cubic light-year (from List of
nearest stars), illustrating the fact that most stars are less bright than absolute magnitude
8.5.
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 (damping) term. These oscillations often
coincide with mass extinction periods on Earth; presumably the higher density of stars
close to the galactic plane leads to more impact events.[36]
It takes the Solar System about 225–250 million years to complete one orbit of the galaxy
(a galactic year),[37]
so it is thought to have completed 20–25 orbits during the lifetime of
the Sun and 1/1250 of a revolution since the origin of humans. The orbital speed of the
Solar System about the center of the Galaxy is approximately 220 km/s. At this speed, it
takes around 1,400 years for the Solar System to travel a distance of 1 light-year, or 8
days to travel 1 AU (astronomical unit).[38]

10. Environment
Broad infrared view of our Milky Way Galaxy from the Spitzer Space Telescope created
from more than 800,000 frames. This is the most detailed infrared picture of our galaxy
to date.
Main articles: Local group and Andromeda-Milky Way collision
The Milky Way and the Andromeda Galaxy are a binary system of giant spiral galaxies
belonging to a group of 50 closely bound galaxies known as the Local Group, itself being
part of the Virgo Supercluster.
Two smaller galaxies and a number of dwarf galaxies in the Local Group orbit the Milky
Way. 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, as well as some that have already been cannibalized by the
Milky Way, such as Omega Centauri. 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.[39]
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 twenty-fold 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

11. 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, individual stars within the galaxies would not collide, but instead
the two galaxies will merge to form a single elliptical galaxy over the course of about a
billion years.[40]
Galaxy rotation curve for the Milky Way. Vertical axis is speed of rotation about the
galactic center. Horizontal axis is distance from the galactic center in kpcs. The sun is
marked with a yellow ball. The observed curve of speed of rotation is blue. The predicted
curve based upon stellar mass and gas in the Milky Way is red. Scatter in observations
roughly indicated by gray bars. The difference is due to dark matter or perhaps a
modification of the law of gravity.[41][42][43]
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.)
Astronomers believe the Milky Way is moving at approximately 630 km per second
relative to the local co-moving frame of reference that moves with the Hubble flow.[44]
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 Milky Way
is thought to be moving in the direction of the Great Attractor. The Local Group (a
cluster of gravitationally bound galaxies containing, among others, the Milky Way and
the Andromeda galaxy) is part of a supercluster called the Local Supercluster, centered
near the Virgo Cluster: although they are moving away from each other at 967 km/s as
part of the Hubble flow, the velocity is less than would be expected given the

12. 16.8 million pc distance due to the gravitational attraction between the Local Group and
the Virgo Cluster.[45]
Another reference frame is provided by the cosmic microwave background (CMB). The
Milky Way is moving at around 552 km/s[3]
with respect to the photons of the CMB,
toward 10.5 right ascension, -24° declination (J2000 epoch, near the center of Hydra).
This motion is observed by satellites such as the Cosmic Background Explorer (COBE)
and the Wilkinson Microwave Anisotropy Probe (WMAP) as a dipole contribution to the
CMB, as photons in equilibrium in the CMB frame get blue-shifted in the direction of the
motion and red-shifted in the opposite direction.[citation needed]
The galaxy rotates about its center according to its galaxy rotation curve as shown in the
figure. The discrepancy between the observed curve (relatively flat) and the curve based
upon the known mass of the stars and gas in the Milk Way (decaying cure) is attributed to
dark matter.[46]
History
Etymology and beliefs
Main articles: List of names for the Milky Way and Milky Way (mythology)
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 Γαλαξίας,
Galaxias, which is derived from the word for milk (γάλα, gala). This is also the origin of
the word galaxy. Indians call it the Akashganga or a celestial form of the holy river,
Ganga.[citation needed]
In Greek myth, the Milky Way was caused by milk spilt by Hera when
suckling 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.[48]
In several Uralic, Turkic languages, Fenno-Ugric languages
and in the Baltic languages the Milky Way is called the "Birds' Path" (Linnunrata in
Finnish), since the route of the migratory birds appear to follow the Milky Way. The
Chinese name "Silver River" (銀河) is used throughout East Asia, including Korea and
Japan. An alternative name for the Milky Way in ancient China, especially in poems, is
"Heavenly Han River"(天汉). In Japanese, "Silver River" (銀河 ginga) means galaxies in

13. general and the Milky Way is called the "Silver River System" (銀河系 gingakei) or the
"River of Heaven" (天の川 Amanokawa or Amanogawa). In Swedish, it is called
Vintergatan, or "Winter Street", because the stars in the belt were used to predict time of
the approaching winter.[citation needed]
In some of the Iberian languages, the name refers to
"Road of Saint James"
Discovery
The shape of the Milky Way as deduced from star counts by William Herschel in 1785;
the Solar System was assumed near center.
As Aristotle (384-322 BC) informs us in Meteorologica (DK 59 A80), the Greek
philosophers Anaxagoras (ca. 500–428 BC) and Democritus (450–370 BC) proposed that
the Milky Way might consist of distant stars. However, Aristotle himself believed the
Milky Way to be caused by "the ignition of the fiery exhalation of some stars which were
large, numerous and close together" and that the "ignition takes place in the upper part of
the atmosphere, in the region of the world which is continuous with the heavenly
motions."[49]
The Arabian astronomer, Alhazen (965-1037 AD), refuted this by making
the first attempt at observing and measuring the Milky Way's parallax,[50]
and he thus
"determined that because the Milky Way had no parallax, it was very remote from the
earth and did not belong to the atmosphere."[51]
The Persian astronomer, Abū Rayhān al-Bīrūnī (973-1048), proposed the Milky Way
galaxy to be a collection of countless nebulous stars.[52]
Avempace (d. 1138) proposed the
Milky Way to be made up of many stars but appears to be a continuous image due to the
effect of refraction in the Earth's atmosphere.[49]
Ibn Qayyim Al-Jawziyya (1292-1350)
proposed the Milky Way galaxy to be "a myriad of tiny stars packed together in the
sphere of the fixed stars" and that that these stars are larger than planets.[53]
Actual proof of the Milky Way consisting of many stars 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.[54]
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.[55]
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 visible sky. He produced a diagram of the shape of the
Galaxy with the Solar System close to the center.

14. Photograph of the "Great Andromeda Nebula" from 1899, later identified as the
Andromeda Galaxy
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.[56]
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.[57]
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.[58]
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.[59]
In 1936
Hubble produced a classification system for galaxies that is used to this day, the Hubble
sequence.[60]