Which kind of light travels fastest in a vacuum?
X-Rays.
Gamma Rays.
Radio waves.
Infrared.
They all travel at the same speed.
What kind of light has wavelengths between those of ultraviolet light and those of gamma waves?
Microwaves.
X-rays.
Visible light.
How long does it take light from the Sun to reach us?
63,2000 years.
4.3 years.
8.3 minutes.
8.3 seconds.
4.3 seconds.
The mass of a positron is the same as that of:
a neutron.
an electron.
a proton.
a neutrino.
a photon.
In the second step of the proton-proton chain sequence of nuclear reactions occuring in the core of the Sun, a 2H nucleus and a 1H nucleus react. What is produced?
A 3^H nucleus.
A 3^He nucleus.
Three 1^H nuclei.
A 3^Li nucleus.
Only energy; they annilihate each other.
Which of the following processes in an atom is called 'excitation'?
when an atom loses an electron.
when an atom fuses with another atom.
when the nucleus of an atom splits into two or more parts.
when an atom gains a neutron.
when an electron in an atom gains energy and jumps to a higher energy level.
32 degrees Fahrenheit is equal to:
0 degrees Kelvin.
-273 degrees Kelvin.
-273 degrees Celsius.
273 degrees Celsius.
273 degrees Kelvin.
In equation form, the inverse square law of light states:
luminosity is proportional to T^4.
brightness is proportional to 1/D^2.
lambda(max) is proportional to 1/T.
parallax is proportional to 1/D.
luminosity is proportional to radius^2.
Which portion of the Sun covers the largest total volume, in kilometers^3?
the corona.
the convective zone.
the radiative zone.
the chromosphere.
the photosphere.
As the frequency of light increases:
the wavelength increases and the energy decreases.
the wavelength decreases and the energy decreases.
the wavelength increases and the energy increases.
the wavelength decreases and the energy increases.
the wavelength increases and the energy remains the same.
When viewed carefully in visible light through a solar telescope, the Sun appears `speckled', with small (about 1000 km wide) variations in brightness covering the whole photosphere. These 'speckles' are the tops of convective cells. These features are called:
Granules.
Cosmological spots.
Isotopes.
Wien's spots.
Sunspots.
The peak of the spectrum of the photosphere of Betelgeuse lies in the:
ultraviolet.
infrared.
visible.
X-ray.
radio.
What is a watt?
A unit of distance.
A unit of energy.
A unit of energy/time.
A unit of angle.
A sub-atomic particle.
How are the distances to the nearest stars determined?
From their Doppler shift.
From their parallax.
From Wien's Law.
By detecting neutrinos from them.
Using Convection.
A hot solid (like a burner on a stove) produces:
a continuous spectrum.
an emission line spectrum.
an absorption line spectrum.
light at a single wavelength.
light at only a few specific wavelengths.
Deuterium is:
Anti-matter.
Hydrogen.
Helium.
Positrons.
Particles of light.
A parsec is:
1/3600 of a degree.
3.26 light years.
8.3 light minutes.
The distance from the Earth to the Sun.
The distance from the Earth to the Moon.
The strong force is:
the force that keeps electrons bound to their atoms.
another name for the gravitational force.
the force that is involved whenever an atom is ionized.
the force that keeps the nuclei of atoms together.
the force that keeps the Earth in orbit around the Sun.
Kinetic energy is:
energy carried by light.
energy produced when an electron and a positron collide.
energy of motion.
energy stored for future use.
all of the above.
Why does it take so long for the energy produced in the core of the Sun to make its way out of the Sun?
The convective cells in the convective layer move very slowly, transporting the energy very slowly.
The speed of light is very low in the interior of the Sun because of the strong gravity.
Photons do not travel very far without being absorbed, and when they are re-emitted, it is in a random direction.
Millions of small black holes throughout the Sun trap the energy.
The nuclear reactions in the core produce mostly radio waves, which travel very slowly.
A tenth magnitude star is:
2.5 times fainter than an eleventh magnitude star.
2.5 times brighter than an eleventh magnitude star.
ten times fainter than an eleventh magnitude star.
ten times brighter than an eleventh magnitude star.
100 times brighter than an eleventh magnitude star.
Luminosity Class III stars are classified as:
Supergiant stars.
White dwarf stars.
Main sequence stars.
Giant stars.
Either giant or supergiant, depending upon the spectral class.
Which of the following spectral types of stars has the hottest photospheric temperature?
A.
B.
F.
K.
O.
Which of the following spectral types of stars has the strongest lines from ionized helium?
G.
M.
What is Henry Norris Russell known for?
Pioneering the use of plots of luminosity vs. temperature for stars.
Re-organizing the spectral sequence ABCDEF... to the sequence used today.
Determining that the acceleration of an object is inversely proportional to its mass.
Determining that the gravitational force between two objects is inversely proportional to the square of the distance apart.
Determining that stars are made up of mostly hydrogen and helium.
Spectral type A stars:
have very strong spectral lines of Titanium Oxide (TiO).
have very low B-V values (-0.3), compared to most stars.
have stronger hydrogen lines than all other types of stars.
have stronger lines of ionized helium than all other types of stars.
have surface temperatures of about 30,000K.
Which of the following is NOT a main sequence star?
A M2V star.
A M5I star.
A B2V star.
The Sun.
A star fusing hydrogen to helium in its core.
If a star is too far away to get its distance via stellar parallax, what is another method that can sometimes be used?
Measure its proper motion.
Measure its Doppler shift.
Spectroscopic parallax.
Use Wien's Law.
Search for sunspots on the star.
Solar maximum occurs approximately every:
5 minutes.
25 hours.
11 years.
250 years.
25,000 years.
The magnetic polarity of the Sun switches approximately every:
5-10 minutes.
1 - 100 days.
6 months.
26,000 years.
Newton's Second Law, in mathematical form, states:
F = MA.
the angular size is inversely proportional to the distance.
Fv1 = Fv2.
p is proportional to 1/D
When the Moon moves directly in front of the Sun, but the Moon's angular size is too small to completely block the photosphere of the Sun, the eclipse that is produced is called:
A lunar eclipse.
A coronal eclipse.
A spicular eclipse.
A magnetodynamical eclipse.
An annular eclipse.
The Earth is 81 times more massive than the Moon. How does the gravitational force on the Earth due to the Moon compare with the gravitational force on the Moon due to the Earth?
the gravitational force on the Earth due to the Moon is 81 times smaller.
the gravitational force on the Earth due to the Moon is 812 = 6561 times smaller.
the gravitational force on the Earth due to the Moon is square root of 81 = 9 times smaller.
the gravitational force on the Earth due to the Moon is 81 times larger.
the two forces are the same.
An astronaut on the International Space Station orbiting Earth:
has a mass of 0 kg.
has a constant velocity.
is not accelerating.
is constantly accelerating.
has a mass equal to 1/6th of his/her mass on Earth.
Newton's Law of Universal Gravitation can be written mathematically as:
F = GMv1Mv2/R^2
F = GMv1/Mv2R^2
F = GMv1Mv2/R
F = GMv1Mv2R^2
F = Mv1Mv2/GR^2
Gas in which component of the Sun has a typical temperature of about a million degrees Kelvin?
The core.
The photosphere.
The chromosphere.
The corona.
How long does an individual sunspot last?
5 - 10 minutes.
22 years.
more than four hundred years. We still see the same sunspots that Galileo saw.
Which of the following stars has the highest B - V?
A main sequence O star.
A white dwarf.
An A2V star.
Betelgeuse.
Which type of star has temperatures between M stars and G stars?
Which type of star has the largest radius?
G2V.
M2I.
M2III.
M2V.
K2V.
A white dwarf is:
the burnt-out core of a star like the Sun, after the outer layers of the star have blown off and dispersed into interstellar space.
a main sequence M star.
an object with a mass between 0.08 and 0.013 solar masses, that never became a star.
an extrasolar planet.
another name for a brown dwarf.
The Pleiades open cluster contains many B stars. Blue glowing nebulae surround the stars in this cluster. These are called:
HII Regions.
Reflection Nebulae.
Supernova Remnants.
Planetary Nebulae.
Protostars.
The Pisgah Radio Telescope detects a strong 21 cm emission line from interstellar gas clouds. What produces this line?
Atomic hydrogen gas.
Molecular hydrogen.
Carbon monoxide.
interstellar dust.
Ionized helium.
Planetary nebulae are a type of interstellar cloud. What type?
Molecular clouds.
Ionized clouds.
Atomic hydrogen clouds.
The remnants of the explosions of supernovae.
Dark clouds.
The light curve of a star is a plot of what property of the star vs. time?
proper motion vs. time.
position vs. time.
velocity vs. time.
brightness vs. time.
angular size vs. time.
The thermal spectrum (blackbody spectrum) of an interstellar dust grain peaks:
in the ultraviolet.
in the far-infrared.
in the middle of the visible range.
in the X-ray.
at 21 cm.
The strong red emission line from hydrogen called the H-alpha line is strongest from what kind of interstellar clouds?
molecular clouds.
HI clouds.
HII regions.
dark clouds.
reflection nebulae.
When two stars in a binary system are both clearly seen from Earth as individual stars, and their orbital motion can be measured to confirm that they are gravitationally bound together, the pair is called a/an:
Astrometric binary.
Visual binary.
Spectroscopic binary.
Optical double.
Eclipsing binary.
What happens to the observed color of a star when it is behind an interstellar cloud?
It appears bluer than it really is.
It appears redder than it really is.
Its color does not change; it gets dimmer the same amount at all wavelengths.
The optical color doesn't change, but all of the IR light from the star is absorbed by the cloud.
The red and blue light gets dimmed similar amounts, while the yellow light is not affected by the cloud.
Which of the following kinds of interstellar clouds are the hottest?
Atomic clouds.
Reflection nebulae.
Which type of main sequence star has the lowest mass?
A stars.
B stars.
F stars.
G stars.
M stars.
In class, we did a demonstration in which a person sat on a stool and spun around. When he pulled in his arms, he spun faster. The reason this happens is because of:
mass conservation.
energy conservation.
linear momentum conservation.
angular momentum conservation.
the center of mass relation.
What is the best type of telescope to use if you want to discover previously-unknown protostars?
Ultraviolet.
Gamma ray.
The star Algol in Perseus (`The Ghoul' or `The Demon Star') was well-known to ancient astronomers, because of its peculiar nature. What unusual observational effect did ancient astronomers notice about this star?
its large proper motion.
its large parallax.
a regular back-and-forth motion on the sky, indicating a companion.
every few days, it gets much brighter for a short period.
every few days, it gets much dimmer for a short period.
What is the difference between a planet like Jupiter and a brown dwarf?
there is no difference: Jupiter is an example of a brown dwarf.
a brown dwarf is the burned-out core of a star that has run out of nuclear fuel.
a brown dwarf is a low luminosity main sequence star.
a brown dwarf may have 1H fusion going on in its core; Jupiter does not.
a brown dwarf may have 2H fusion going on in its core; Jupiter does not.
The dark cloud shaped like a horse's head, that is known as the Horsehead Nebula, is:
A reflection nebula.
An HI cloud.
A molecular cloud.
An HII region.
An ionized gas cloud.
Compared to an unobscured GV star, a GV star that lies behind an interstellar cloud will appear:
more redshifted.
bluer.
redder.
hotter.
more luminous.
What luminosity class stars approximately obey the mass-luminosity relation described by the formula luminosity is proportional to mass to the fourth power?
I.
II.
III.
IV.
V.
Millimeter (microwave) telescopes detect the 2.6 millimeter emission lines from dense interstellar gas clouds. What produces this line?
When an interstellar cloud gravitationally collapses to form a protostar, what happens to the temperature of the gas in the core of the cloud?
it remains constant until nuclear fusion starts, then it increases.
the temperature of the gas in the core decreases as the cloud collapses until nuclear fusion starts, then it increases.
the temperature of the gas in the core increases as the cloud collapses, even before nuclear fusion starts, then it increases further.
the temperature of the gas in the core decreases as the cloud collapses until nuclear fusion starts, then it decreases further as fusion cools the core down.
no protostars have ever been found, so scientists have no idea what happens.
In high mass main sequence stars, hydrogen is fusing to helium in the core. What is name of the main set of reactions by which this process occurs?
The proton-proton chain.
The CNO cycle.
The triple alpha process.
The brown dwarf process.
The asymptotic giant branch process.
If a white dwarf in a mass transfer binary system exceeds the Chandrasekhar limit, it becomes:
A nova.
A Type I supernova (a carbon-detonation supernova).
A Type II supernova (a core-collapse supernova).
A planetary nebula.
A black hole.
Who discovered the first pulsar?
Annie Jump Cannon.
Henry Norris Russell.
Jocelyn Bell.
Cecilia Payne-Gaposchkin.
Ejnar Hertzsprung.
Three solar masses is:
The upper mass limit to the mass of a neutron star.
The upper mass limit to the mass of a white dwarf.
The upper mass limit to the mass of a brown dwarf.
The approximate mass of a main sequence M star.
The approximate mass of a main sequence O star.
Which of the following objects is closest in diameter to the Earth?
A main sequence M star.
A neutron star.
The very regular `pulses' of radio light we see from some neutron stars are due to:
the star pulsating in size.
a companion dumping gas onto the neutron star, causing flare-ups of nuclear reactions.
a companion periodically eclipsing the neutron star.
as the pulsar spins, a beam of light from the magnetic poles of the neutron star sweeps across the Earth.
an extragalactic civilization.
When a 1 solar mass star leaves the main sequence and moves up the red giant branch of the H-R diagram for the first time, what is occuring in the interior of the star?
no nuclear reactions are occuring anywhere in its interior.
hydrogen fusion in the core.
helium fusion in the core.
carbon fusion in the core.
no reactions in the core; hydrogen fusion in a shell surrounding the core.
Why doesn't a white dwarf contract under the force of its own gravity?
Because carbon fusion is occuring in its core.
Because the CNO process is occuring in its core.
Because the triple alpha process is occuring in its core.
it is held up against gravity by electron degeneracy pressure.
it is held up against gravity by neutron degeneracy pressure.
Which of the following statements is true about the lifetimes of main sequence stars?
Lower luminosity main sequence stars live longer than higher luminosity main sequence stars.
Main sequence A stars live longer than main sequence K stars.
Hot main sequence stars live longer than cool main sequence stars.
The greater the mass of a star, the longer its main sequence lifetime.
All main sequence A stars ever formed are still main sequence A stars.
Approximately how many years from now will the Sun runs out of hydrogen in its core?
1 million years.
5 million years.
5 billion years.
5 trillion years.
five hundred trillion years.
A particular star cluster is observed to have a full main sequence, extending from MV stars to OV stars. Approximately how old is this cluster?
Less than a few million years old.
100 million years old.
1 billion years old.
10 billion years old.
1 trillion years old.
Iron is produced:
In the core of main sequence stars.
In the cores of red giant stars.
In white dwarf stars.
In the last stages of life of a 1 solar mass star.
In the cores of massive stars, just before a supernova.
What is the heaviest chemical element that will ever be created in large amounts in the core of the Sun?
Iron.
Uranium.
Silicon.
Titanium.
Carbon.
From lowest mass to highest mass, what is the correct order of the following objects or types of objects?
Neutron stars, brown dwarfs, MV stars, the Sun.
Brown dwarfs, MV stars, the Sun, Neutron stars.
Brown dwarfs, neutron stars, MV stars, the Sun.
The Sun, brown dwarfs, neutron stars, MV stars.
Brown dwarfs, the Sun, neutron stars, MV stars.
The triple alpha process is:
Another name for the proton-proton chain.
The process that produces uranium and other high mass elements.
When three helium-4 nuclei fuse to form carbon.
The formation of neutrons out of protons and electrons.
When three stars combine to form a more massive star.
Synchrotron radiation is produced by:
a hot sold object, like the filament in a light bulb.
electrons in atoms jumping from lower energy levels to higher energy levels.
electrons in atoms jumping from higher energy levels to lower energy levels.
only supernova.
accelerated charged particles.
Which of the following chemical elements is only produced during a supernova explosion?
Plutonium.
Magnesium.
Oxygen.
Which of the following stars will likely eventually explode as a supernova?
The MV star Proxima Cen.
A 0.5 solar mass AGB star.
All of the above.
Over the course of its lifetime, the Sun will go through all of the following stages except one. Which is the exception?
white dwarf.
AGB star.
neutron star.
horizontal branch star.
red giant.
Approximately how frequently does a supernova occur in the Milky Way Galaxy?
once every million years.
once every 200 years.
once per year.
about 100 supernova occur in the Milky Way per year.
about a million supernova occur in the Milky Way per year.
On the Hubble Tuning Fork diagram, galaxies that sit between the ellipticals and the spiral galaxies are called:
Irregular galaxies.
S0 galaxies.
Sc galaxies.
Sb galaxies.
SBd galaxies.
Most of the following types of objects are mainly found in the disk of the Milky Way. Which of the following is the exception, also being seen regularly in the bulge and halo?
open clusters.
SN Type II.
O and B main sequence stars.
planetary nebulae.
What is the mass of a photon of light?
1/2000th the mass of a proton.
1/2000th the mass of an electron.
It depends upon the wavelength: the longer the wavelength, the larger the mass.
It depends upon the wavelength: the longer the wavelength, the smaller the mass.
Zero.
The Schwarzchild Radius is defined as:
The radius of the stellar disk of the Milky Way.
The point between two stars in a binary star system such that the gravitational force from the two stars is equal.
The maximum possible radius of a white dwarf.
The maximum possible radius of a neutron star.
The radius of the event horizon of a black hole.
What is the main difference between E0 and E7 galaxies?
E0 galaxies are much larger, in physical diameter.
E7 galaxies are flatter in appearance, while E0 galaxies are round.
E7 galaxies have spiral arms; E0 galaxies do not.
E0 galaxies have bars in the center; E7 galaxies do not.
E0 galaxies have tightly wrapped spiral arms; E7 galaxies have loosely wrapped spiral arms.
An SBc galaxy:
has a large bulge and tightly wrapped spiral arms.
has a large bulge and loosely wrapped spiral arms.
has a large bulge and a bar.
has a small bulge and a bar.
is a spheroidal ball of stars which is approximately round in appearance on the sky.
Who was the first person to classify spiral and elliptical galaxies into sub-types according to their appearance?
Edwin Hubble.
Henrietta Leavitt.
Harlow Shapley.
William Herschel.
Robert Trumpler.
Who was the first person to conclude that the Sun is NOT in the center of the Milky Way?
Henrietta Leavitt discovered:
Diffuse interstellar dust in the Milky Way.
Sagittarius A*.
The Cepheid Period-Luminosity Relation.
Cepheid Variables in the Andromeda Galaxy.
The first pulsar.
On the H-R Diagram, Cepheid Variables sit:
On the bottom of the Main Sequence.
On the top of the Main Sequence.
Below and to the left of the Main Sequence.
On the far right: they are M stars.
Near the middle of the diagram, above the Main Sequence.
In the Milky Way, most of the interstellar gas is:
In the spiral arms.
In the bulge.
In the halo.
In the disk.
Evenly spread between the bulge, the disk, and the halo.
What object lies in the center of the Milky Way galaxy?
Cygnus X-1.
delta Cephei.
Sirius.
The first conclusive evidence that light is affected by gravity was obtained:
About three years ago, at the CERN laboratory in Switzerland.
In 1919, during a total solar eclipse.
In the 1960's, with a radio telescope.
About 10 years ago, with the Hubble Telescope.
No evidence has been found yet; it has just been theorized.
In the Milky Way, open clusters are found:
Mainly in the disk.
Mainly in the bulge.
Mainly in the halo.
Evenly spread in the disk, bulge, and halo.
In both the bulge and halo, but usually not the disk.
William Herschel:
Discovered Cepheid variables in the Andromeda Galaxy.
Discovered the Period-Luminosity relation for Cepheid variable stars.
Made the first 3-dimensional map of the Milky Way.
Classified galaxies according to the bulge/disk ratio and the tightness of wrapping of the spiral arms.
Was the first person to conclude that the Sun is not in the center of the Milky Way.
By tradition, plots of the circular orbital velocities of stars and gas in the disks of spiral galaxies vs. the distance from the center are called:
Spin diagrams.
Hubble diagrams.
Rotation curves.
Light curves.
Tidal diagrams.
RR Lyrae stars are:
Brown dwarfs.
White dwarfs.
Variable stars.
Eclipsing binary stars.
What did Friedrich Bessel detect for the first time in 1838?
Cepheid variables in the Andromeda Galaxy.
An eclipsing binary star.
A pulsar.
Stellar parallax.
Cygnus X-1 is most likely:
A Cepheid variable star.
An RR Lyrae star.
A black hole with the same mass as Jupiter has an event horizon with a radius of about 3 meters. The Sun has a mass about 1000 times that of Jupiter. Therefore, the radius of the event horizon of a 1 solar mass black hole is:
3 kilometers.
3 centimeters.
3^3 = 27 meters.
3 million meters = 3000 kilometers.
1/3 meter.
What is the second-to-top step on the Cosmological Distance Ladder?
Hubble's Law.
Supernovae Type I.
Cepheid Variables.
Spectroscopic Parallax.
Stellar Parallax.
The Local Group is in the center of:
The Coma Cluster.
The Great Wall.
The Virgo Cluster.
The Local Supercluster.
None of the above.
The Magellanic Clouds are in the:
Virgo Cluster.
The Local Group.
The Milky Way.
Double-Lobed Radio Galaxies are mostly:
Giant Elliptical galaxies.
Spiral galaxies.
Barred spiral galaxies.
Both barred and unbarred spiral galaxies.
Quasars are:
Only found in the Milky Way.
Only found in the Local Group.
Only found in the Local Supercluster.
Similar in luminosity to Sagittarius A*.
Less frequent in the present than in the past.
The Sun was first detected in the radio by:
Karl Jansky.
Allan Sandage.
Radar operators in World War II.
Hubble's constant is approximately 75 (km/s)/Mpc. If a galaxy is moving away from us at a speed of 7500 km/s, what is its approximate distance?
7500 X 75 = 562,500 Mpc.
75/7500 = 0.01 Mpc.
7500 / 75 = 100 Mpc.
7500 X 75 X 75 = 42,188,000 Mpc
7500 / 752 = 1.33 Mpc.
Hubble's Law is a useful way to determine astronomical distances, but only for some objects. For which of these objects would it work to get an approximate distance?
A globular cluster in the halo of the Milky Way.
The stars in the belt of Orion.
The Andromeda Galaxy.
The emission lines seen in the optical spectra of quasars were initially unidentified. Who first identified these lines, and showed that they are just lines of ordinary elements, but very redshifted?
Maarten Schmidt.
The Cartwheel galaxy is:
a giant elliptical galaxy in the center of the Coma cluster.
a spiral galaxy very similar to the Milky Way.
a dwarf irregular galaxy in orbit around the Milky Way.
a ring galaxy.
a dwarf elliptical galaxy in the Local Group.
A Universe that will collapse back upon itself in a `Big Crunch' is called a/an:
Flat Universe.
Closed Universe.
Open Universe.
Infinite Universe.
Universe with a density equal to the the critical density.
The Cosmological Constant was initially introduced into the equations governing the evolution of the Universe by:
Albert Einstein.
Which of the following objects is the most luminous?
A quasar.
The nucleus of a Seyfert galaxy.
The Zone of Avoidance is:
A large spherical 'void' containing very few galaxies, as seen in 'slice of the Universe' plots.
The large volume of nearby space which does not contain any quasars.
The plane of the Milky Way, whose dust blocks light from distant galaxies.
All parts of the Universe outside of the Local Supercluster.
Parts of the Universe too far away for us to see, since light has not had time yet to reach us.
Observations of Supernovae Type I in very distant galaxies provided the first evidence for:
Dark Energy.
Dark Matter.
A closed Universe.
The theory that the Universe will end in a `Big Crunch'.
16. The diagram to the right is a plot of time (on the x axis) vs. the distance between any two galaxies in the Universe (on the y axis) for three different Universes: Universe A, Universe B, and Universe C. Which of the three Universes in the above diagram has the highest density of matter?
Universe A.
Universe B.
Universe C.
Universe A and B are the same.
All three Universes are the same.
What is the top step on the Cosmological Distance Ladder?
The difference between a double-lobed radio galaxy and a core-halo radio galaxy is:
Double-lobed radio galaxies are ellipticals; core-halo radio galaxies are spirals.
Double-lobed radio galaxies are spirals; core-halo radio galaxies are ellipticals.
Double-lobed radio galaxies are much more luminous than core-halo radio galaxies.
Double-lobed radio galaxies are much less luminous than core-halo radio galaxies.
The difference is just due to our viewing location; physically, they are the same kind of objects.
The Great Wall is:
Another name for the Local Supercluster.
A large 'wall' of galaxies centered on the Local Group.
A large `wall' of galaxies about 100 Mpc away, containing the Coma cluster.
The part of the Universe hidden in visible light by the dust in the plane of the Milky Way.
The group of galaxies we live in.
What kind of galaxies are NOT found in the Local Group, but ARE seen in the Virgo Cluster?
dwarf ellipticals.
giant ellipticals.
spiral galaxies.
irregular galaxies.
all of the above are seen in both the Local Group and the Virgo Cluster.
Please wait - loading…