ASTR Review for Final #1 (All 5 Quizzes)

Questão 1 de 120

1

Which kind of light travels fastest in a vacuum?

Selecione uma das seguintes:

X-Rays.
Gamma Rays.
Radio waves.
Infrared.
They all travel at the same speed.

Explicação

Questão 2 de 120

1

What kind of light has wavelengths between those of ultraviolet light and those of gamma waves?

Selecione uma das seguintes:

Infrared.
Microwaves.
Radio waves.
X-rays.
Visible light.

Explicação

Questão 3 de 120

1

How long does it take light from the Sun to reach us?

Selecione uma das seguintes:

63,2000 years.
4.3 years.
8.3 minutes.
8.3 seconds.
4.3 seconds.

Explicação

Questão 4 de 120

1

The mass of a positron is the same as that of:

Selecione uma das seguintes:

a neutron.
an electron.
a proton.
a neutrino.
a photon.

Explicação

Questão 5 de 120

1

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?

Selecione uma das seguintes:

A 3^H nucleus.
A 3^He nucleus.
Three 1^H nuclei.
A 3^Li nucleus.
Only energy; they annilihate each other.

Explicação

Questão 6 de 120

1

Which of the following processes in an atom is called 'excitation'?

Selecione uma das seguintes:

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.

Explicação

Questão 7 de 120

1

32 degrees Fahrenheit is equal to:

Selecione uma das seguintes:

0 degrees Kelvin.
-273 degrees Kelvin.
-273 degrees Celsius.
273 degrees Celsius.
273 degrees Kelvin.

Explicação

Questão 8 de 120

1

In equation form, the inverse square law of light states:

Selecione uma das seguintes:

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.

Explicação

Questão 9 de 120

1

Which portion of the Sun covers the largest total volume, in kilometers^3?

Selecione uma das seguintes:

the corona.
the convective zone.
the radiative zone.
the chromosphere.
the photosphere.

Explicação

Questão 10 de 120

1

As the frequency of light increases:

Selecione uma das seguintes:

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.

Explicação

Questão 11 de 120

1

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:

Selecione uma das seguintes:

Granules.
Cosmological spots.
Isotopes.
Wien's spots.
Sunspots.

Explicação

Questão 12 de 120

1

The peak of the spectrum of the photosphere of Betelgeuse lies in the:

Selecione uma das seguintes:

ultraviolet.
infrared.
visible.
X-ray.
radio.

Explicação

Questão 13 de 120

1

What is a watt?

Selecione uma das seguintes:

A unit of distance.
A unit of energy.
A unit of energy/time.
A unit of angle.
A sub-atomic particle.

Explicação

Questão 14 de 120

1

How are the distances to the nearest stars determined?

Selecione uma das seguintes:

From their Doppler shift.
From their parallax.
From Wien's Law.
By detecting neutrinos from them.
Using Convection.

Explicação

Questão 15 de 120

1

A hot solid (like a burner on a stove) produces:

Selecione uma das seguintes:

a continuous spectrum.
an emission line spectrum.
an absorption line spectrum.
light at a single wavelength.
light at only a few specific wavelengths.

Explicação

Questão 16 de 120

1

Deuterium is:

Selecione uma das seguintes:

Anti-matter.
Hydrogen.
Helium.
Positrons.
Particles of light.

Explicação

Questão 17 de 120

1

A parsec is:

Selecione uma das seguintes:

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.

Explicação

Questão 18 de 120

1

The strong force is:

Selecione uma das seguintes:

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.

Explicação

Questão 19 de 120

1

Kinetic energy is:

Selecione uma das seguintes:

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.

Explicação

Questão 20 de 120

1

Why does it take so long for the energy produced in the core of the Sun to make its way out of the Sun?

Selecione uma das seguintes:

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.

Explicação

Questão 21 de 120

1

A tenth magnitude star is:

Selecione uma das seguintes:

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.

Explicação

Questão 22 de 120

1

Luminosity Class III stars are classified as:

Selecione uma das seguintes:

Supergiant stars.
White dwarf stars.
Main sequence stars.
Giant stars.
Either giant or supergiant, depending upon the spectral class.

Explicação

Questão 23 de 120

1

Which of the following spectral types of stars has the hottest photospheric temperature?

Selecione uma das seguintes:

A.
B.
F.
K.
O.

Explicação

Questão 24 de 120

1

Which of the following spectral types of stars has the strongest lines from ionized helium?

Selecione uma das seguintes:

A.
K.
G.
M.
O.

Explicação

Questão 25 de 120

1

What is Henry Norris Russell known for?

Selecione uma das seguintes:

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.

Explicação

Questão 26 de 120

1

Spectral type A stars:

Selecione uma das seguintes:

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.

Explicação

Questão 27 de 120

1

Which of the following is NOT a main sequence star?

Selecione uma das seguintes:

A M2V star.
A M5I star.
A B2V star.
The Sun.
A star fusing hydrogen to helium in its core.

Explicação

Questão 28 de 120

1

If a star is too far away to get its distance via stellar parallax, what is another method that can sometimes be used?

Selecione uma das seguintes:

Measure its proper motion.
Measure its Doppler shift.
Spectroscopic parallax.
Use Wien's Law.
Search for sunspots on the star.

Explicação

Questão 29 de 120

1

Solar maximum occurs approximately every:

Selecione uma das seguintes:

5 minutes.
25 hours.
11 years.
250 years.
25,000 years.

Explicação

Questão 30 de 120

1

The magnetic polarity of the Sun switches approximately every:

Selecione uma das seguintes:

5-10 minutes.
1 - 100 days.
6 months.
11 years.
26,000 years.

Explicação

Questão 31 de 120

1

Newton's Second Law, in mathematical form, states:

Selecione uma das seguintes:

F = MA.
lambda(max) is proportional to 1/T.
the angular size is inversely proportional to the distance.
Fv1 = Fv2.
p is proportional to 1/D

Explicação

Questão 32 de 120

1

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:

Selecione uma das seguintes:

A lunar eclipse.
A coronal eclipse.
A spicular eclipse.
A magnetodynamical eclipse.
An annular eclipse.

Explicação

Questão 33 de 120

1

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?

Selecione uma das seguintes:

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.

Explicação

Questão 34 de 120

1

An astronaut on the International Space Station orbiting Earth:

Selecione uma das seguintes:

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.

Explicação

Questão 35 de 120

1

Newton's Law of Universal Gravitation can be written mathematically as:

Selecione uma das seguintes:

F = GMv1Mv2/R^2
F = GMv1/Mv2R^2
F = GMv1Mv2/R
F = GMv1Mv2R^2
F = Mv1Mv2/GR^2

Explicação

Questão 36 de 120

1

Gas in which component of the Sun has a typical temperature of about a million degrees Kelvin?

Selecione uma das seguintes:

The core.
The photosphere.
Sunspots.
The chromosphere.
The corona.

Explicação

Questão 37 de 120

1

How long does an individual sunspot last?

Selecione uma das seguintes:

5 - 10 minutes.
1 - 100 days.
11 years.
22 years.
more than four hundred years. We still see the same sunspots that Galileo saw.

Explicação

Questão 38 de 120

1

Which of the following stars has the highest B - V?

Selecione uma das seguintes:

A main sequence O star.
A white dwarf.
The Sun.
An A2V star.
Betelgeuse.

Explicação

Questão 39 de 120

1

Which type of star has temperatures between M stars and G stars?

Selecione uma das seguintes:

F.
A.
B.
O.
K.

Explicação

Questão 40 de 120

1

Which type of star has the largest radius?

Selecione uma das seguintes:

G2V.
M2I.
M2III.
M2V.
K2V.

Explicação

Questão 41 de 120

1

A white dwarf is:

Selecione uma das seguintes:

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.

Explicação

Questão 42 de 120

1

The Pleiades open cluster contains many B stars. Blue glowing nebulae surround the stars in this cluster. These are called:

Selecione uma das seguintes:

HII Regions.
Reflection Nebulae.
Supernova Remnants.
Planetary Nebulae.
Protostars.

Explicação

Questão 43 de 120

1

The Pisgah Radio Telescope detects a strong 21 cm emission line from interstellar gas clouds. What produces this line?

Selecione uma das seguintes:

Atomic hydrogen gas.
Molecular hydrogen.
Carbon monoxide.
interstellar dust.
Ionized helium.

Explicação

Questão 44 de 120

1

Planetary nebulae are a type of interstellar cloud. What type?

Selecione uma das seguintes:

Molecular clouds.
Ionized clouds.
Atomic hydrogen clouds.
The remnants of the explosions of supernovae.
Dark clouds.

Explicação

Questão 45 de 120

1

The light curve of a star is a plot of what property of the star vs. time?

Selecione uma das seguintes:

proper motion vs. time.
position vs. time.
velocity vs. time.
brightness vs. time.
angular size vs. time.

Explicação

Questão 46 de 120

1

The thermal spectrum (blackbody spectrum) of an interstellar dust grain peaks:

Selecione uma das seguintes:

in the ultraviolet.
in the far-infrared.
in the middle of the visible range.
in the X-ray.
at 21 cm.

Explicação

Questão 47 de 120

1

The strong red emission line from hydrogen called the H-alpha line is strongest from what kind of interstellar clouds?

Selecione uma das seguintes:

molecular clouds.
HI clouds.
HII regions.
dark clouds.
reflection nebulae.

Explicação

Questão 48 de 120

1

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:

Selecione uma das seguintes:

Astrometric binary.
Visual binary.
Spectroscopic binary.
Optical double.
Eclipsing binary.

Explicação

Questão 49 de 120

1

What happens to the observed color of a star when it is behind an interstellar cloud?

Selecione uma das seguintes:

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.

Explicação

Questão 50 de 120

1

Which of the following kinds of interstellar clouds are the hottest?

Selecione uma das seguintes:

HII regions.
Molecular clouds.
Atomic clouds.
Reflection nebulae.
Dark clouds.

Explicação

Questão 51 de 120

1

Which type of main sequence star has the lowest mass?

Selecione uma das seguintes:

A stars.
B stars.
F stars.
G stars.
M stars.

Explicação

Questão 52 de 120

1

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:

Selecione uma das seguintes:

mass conservation.
energy conservation.
linear momentum conservation.
angular momentum conservation.
the center of mass relation.

Explicação

Questão 53 de 120

1

What is the best type of telescope to use if you want to discover previously-unknown protostars?

Selecione uma das seguintes:

X-ray.
Ultraviolet.
Visible light.
Infrared.
Gamma ray.

Explicação

Questão 54 de 120

1

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?

Selecione uma das seguintes:

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.

Explicação

Questão 55 de 120

1

What is the difference between a planet like Jupiter and a brown dwarf?

Selecione uma das seguintes:

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.

Explicação

Questão 56 de 120

1

The dark cloud shaped like a horse's head, that is known as the Horsehead Nebula, is:

Selecione uma das seguintes:

A reflection nebula.
An HI cloud.
A molecular cloud.
An HII region.
An ionized gas cloud.

Explicação

Questão 57 de 120

1

Compared to an unobscured GV star, a GV star that lies behind an interstellar cloud will appear:

Selecione uma das seguintes:

more redshifted.
bluer.
redder.
hotter.
more luminous.

Explicação

Questão 58 de 120

1

What luminosity class stars approximately obey the mass-luminosity relation described by the formula luminosity is proportional to mass to the fourth power?

Selecione uma das seguintes:

I.
II.
III.
IV.
V.

Explicação

Questão 59 de 120

1

Millimeter (microwave) telescopes detect the 2.6 millimeter emission lines from dense interstellar gas clouds. What produces this line?

Selecione uma das seguintes:

Atomic hydrogen gas.
Molecular hydrogen.
Carbon monoxide.
interstellar dust.
Ionized helium.

Explicação

Questão 60 de 120

1

When an interstellar cloud gravitationally collapses to form a protostar, what happens to the temperature of the gas in the core of the cloud?

Selecione uma das seguintes:

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.

Explicação

Questão 61 de 120

1

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?

Selecione uma das seguintes:

The proton-proton chain.
The CNO cycle.
The triple alpha process.
The brown dwarf process.
The asymptotic giant branch process.

Explicação

Questão 62 de 120

1

If a white dwarf in a mass transfer binary system exceeds the Chandrasekhar limit, it becomes:

Selecione uma das seguintes:

A nova.
A Type I supernova (a carbon-detonation supernova).
A Type II supernova (a core-collapse supernova).
A planetary nebula.
A black hole.

Explicação

Questão 63 de 120

1

Who discovered the first pulsar?

Selecione uma das seguintes:

Annie Jump Cannon.
Henry Norris Russell.
Jocelyn Bell.
Cecilia Payne-Gaposchkin.
Ejnar Hertzsprung.

Explicação

Questão 64 de 120

1

Three solar masses is:

Selecione uma das seguintes:

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.

Explicação

Questão 65 de 120

1

Which of the following objects is closest in diameter to the Earth?

Selecione uma das seguintes:

A main sequence M star.
A main sequence O star.
A neutron star.
A white dwarf.
Betelgeuse.

Explicação

Questão 66 de 120

1

The very regular `pulses' of radio light we see from some neutron stars are due to:

Selecione uma das seguintes:

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.

Explicação

Questão 67 de 120

1

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?

Selecione uma das seguintes:

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.

Explicação

Questão 68 de 120

1

Why doesn't a white dwarf contract under the force of its own gravity?

Selecione uma das seguintes:

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.

Explicação

Questão 69 de 120

1

Which of the following statements is true about the lifetimes of main sequence stars?

Selecione uma das seguintes:

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.

Explicação

Questão 70 de 120

1

Approximately how many years from now will the Sun runs out of hydrogen in its core?

Selecione uma das seguintes:

1 million years.
5 million years.
5 billion years.
5 trillion years.
five hundred trillion years.

Explicação

Questão 71 de 120

1

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?

Selecione uma das seguintes:

Less than a few million years old.
100 million years old.
1 billion years old.
10 billion years old.
1 trillion years old.

Explicação

Questão 72 de 120

1

Iron is produced:

Selecione uma das seguintes:

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.

Explicação

Questão 73 de 120

1

What is the heaviest chemical element that will ever be created in large amounts in the core of the Sun?

Selecione uma das seguintes:

Iron.
Uranium.
Silicon.
Titanium.
Carbon.

Explicação

Questão 74 de 120

1

From lowest mass to highest mass, what is the correct order of the following objects or types of objects?

Selecione uma das seguintes:

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.

Explicação

Questão 75 de 120

1

The triple alpha process is:

Selecione uma das seguintes:

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.

Explicação

Questão 76 de 120

1

Synchrotron radiation is produced by:

Selecione uma das seguintes:

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.

Explicação

Questão 77 de 120

1

Which of the following chemical elements is only produced during a supernova explosion?

Selecione uma das seguintes:

Plutonium.
Silicon.
Iron.
Magnesium.
Oxygen.

Explicação

Questão 78 de 120

1

Which of the following stars will likely eventually explode as a supernova?

Selecione uma das seguintes:

The Sun.
The MV star Proxima Cen.
Betelgeuse.
A 0.5 solar mass AGB star.
All of the above.

Explicação

Questão 79 de 120

1

Over the course of its lifetime, the Sun will go through all of the following stages except one. Which is the exception?

Selecione uma das seguintes:

white dwarf.
AGB star.
neutron star.
horizontal branch star.
red giant.

Explicação

Questão 80 de 120

1

Approximately how frequently does a supernova occur in the Milky Way Galaxy?

Selecione uma das seguintes:

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.

Explicação

Questão 81 de 120

1

On the Hubble Tuning Fork diagram, galaxies that sit between the ellipticals and the spiral galaxies are called:

Selecione uma das seguintes:

Irregular galaxies.
S0 galaxies.
Sc galaxies.
Sb galaxies.
SBd galaxies.

Explicação

Questão 82 de 120

1

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?

Selecione uma das seguintes:

open clusters.
HII regions.
SN Type II.
O and B main sequence stars.
planetary nebulae.

Explicação

Questão 83 de 120

1

What is the mass of a photon of light?

Selecione uma das seguintes:

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.

Explicação

Questão 84 de 120

1

The Schwarzchild Radius is defined as:

Selecione uma das seguintes:

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.

Explicação

Questão 85 de 120

1

What is the main difference between E0 and E7 galaxies?

Selecione uma das seguintes:

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.

Explicação

Questão 86 de 120

1

An SBc galaxy:

Selecione uma das seguintes:

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.

Explicação

Questão 87 de 120

1

Who was the first person to classify spiral and elliptical galaxies into sub-types according to their appearance?

Selecione uma das seguintes:

Edwin Hubble.
Henrietta Leavitt.
Harlow Shapley.
William Herschel.
Robert Trumpler.

Explicação

Questão 88 de 120

1

Who was the first person to conclude that the Sun is NOT in the center of the Milky Way?

Selecione uma das seguintes:

Henrietta Leavitt.
Harlow Shapley.
Edwin Hubble.
William Herschel.
Robert Trumpler.

Explicação

Questão 89 de 120

1

Henrietta Leavitt discovered:

Selecione uma das seguintes:

Diffuse interstellar dust in the Milky Way.
Sagittarius A*.
The Cepheid Period-Luminosity Relation.
Cepheid Variables in the Andromeda Galaxy.
The first pulsar.

Explicação

Questão 90 de 120

1

On the H-R Diagram, Cepheid Variables sit:

Selecione uma das seguintes:

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.

Explicação

Questão 91 de 120

1

In the Milky Way, most of the interstellar gas is:

Selecione uma das seguintes:

In the spiral arms.
In the bulge.
In the halo.
In the disk.
Evenly spread between the bulge, the disk, and the halo.

Explicação

Questão 92 de 120

1

What object lies in the center of the Milky Way galaxy?

Selecione uma das seguintes:

Cygnus X-1.
delta Cephei.
The Sun.
Sirius.
Sagittarius A*.

Explicação

Questão 93 de 120

1

The first conclusive evidence that light is affected by gravity was obtained:

Selecione uma das seguintes:

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.

Explicação

Questão 94 de 120

1

In the Milky Way, open clusters are found:

Selecione uma das seguintes:

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.

Explicação

Questão 95 de 120

1

William Herschel:

Selecione uma das seguintes:

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.

Explicação

Questão 96 de 120

1

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:

Selecione uma das seguintes:

Spin diagrams.
Hubble diagrams.
Rotation curves.
Light curves.
Tidal diagrams.

Explicação

Questão 97 de 120

1

RR Lyrae stars are:

Selecione uma das seguintes:

Brown dwarfs.
White dwarfs.
Variable stars.
Eclipsing binary stars.
Protostars.

Explicação

Questão 98 de 120

1

What did Friedrich Bessel detect for the first time in 1838?

Selecione uma das seguintes:

Brown dwarfs.
Cepheid variables in the Andromeda Galaxy.
An eclipsing binary star.
A pulsar.
Stellar parallax.

Explicação

Questão 99 de 120

1

Cygnus X-1 is most likely:

Selecione uma das seguintes:

An eclipsing binary star.
A Cepheid variable star.
A neutron star.
A black hole.
An RR Lyrae star.

Explicação

Questão 100 de 120

1

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:

Selecione uma das seguintes:

3 kilometers.
3 centimeters.
3^3 = 27 meters.
3 million meters = 3000 kilometers.
1/3 meter.

Explicação

Questão 101 de 120

1

What is the second-to-top step on the Cosmological Distance Ladder?

Selecione uma das seguintes:

Hubble's Law.
Supernovae Type I.
Cepheid Variables.
Spectroscopic Parallax.
Stellar Parallax.

Explicação

Questão 102 de 120

1

The Local Group is in the center of:

Selecione uma das seguintes:

The Coma Cluster.
The Great Wall.
The Virgo Cluster.
The Local Supercluster.
None of the above.

Explicação

Questão 103 de 120

1

The Magellanic Clouds are in the:

Selecione uma das seguintes:

Virgo Cluster.
The Great Wall.
The Coma Cluster.
The Local Group.
The Milky Way.

Explicação

Questão 104 de 120

1

Double-Lobed Radio Galaxies are mostly:

Selecione uma das seguintes:

Giant Elliptical galaxies.
Spiral galaxies.
Barred spiral galaxies.
Both barred and unbarred spiral galaxies.
Irregular galaxies.

Explicação

Questão 105 de 120

1

Quasars are:

Selecione uma das seguintes:

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.

Explicação

Questão 106 de 120

1

The Sun was first detected in the radio by:

Selecione uma das seguintes:

Karl Jansky.
Edwin Hubble.
Jocelyn Bell.
Allan Sandage.
Radar operators in World War II.

Explicação

Questão 107 de 120

1

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?

Selecione uma das seguintes:

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.

Explicação

Questão 108 de 120

1

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?

Selecione uma das seguintes:

A globular cluster in the halo of the Milky Way.
The stars in the belt of Orion.
Sagittarius A*.
The Andromeda Galaxy.
The Great Wall.

Explicação

Questão 109 de 120

1

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?

Selecione uma das seguintes:

Edwin Hubble.
Jocelyn Bell.
Maarten Schmidt.
Harlow Shapley.
Allan Sandage.

Explicação

Questão 110 de 120

1

The Cartwheel galaxy is:

Selecione uma das seguintes:

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.

Explicação

Questão 111 de 120

1

A Universe that will collapse back upon itself in a `Big Crunch' is called a/an:

Selecione uma das seguintes:

Flat Universe.
Closed Universe.
Open Universe.
Infinite Universe.
Universe with a density equal to the the critical density.

Explicação

Questão 112 de 120

1

The Cosmological Constant was initially introduced into the equations governing the evolution of the Universe by:

Selecione uma das seguintes:

Edwin Hubble.
Henrietta Leavitt.
Harlow Shapley.
Albert Einstein.
Allan Sandage.

Explicação

Questão 113 de 120

1

Which of the following objects is the most luminous?

Selecione uma das seguintes:

A quasar.
A Cepheid variable star.
Sagittarius A*.
The nucleus of a Seyfert galaxy.
A pulsar.

Explicação

Questão 114 de 120

1

The Zone of Avoidance is:

Selecione uma das seguintes:

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.

Explicação

Questão 115 de 120

1

Observations of Supernovae Type I in very distant galaxies provided the first evidence for:

Selecione uma das seguintes:

Dark Energy.
Dark Matter.
A closed Universe.
The theory that the Universe will end in a `Big Crunch'.
The Great Wall.

Explicação

Questão 116 de 120

1

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?

Selecione uma das seguintes:

Universe A.
Universe B.
Universe C.
Universe A and B are the same.
All three Universes are the same.

Explicação

Questão 117 de 120

1

What is the top step on the Cosmological Distance Ladder?

Selecione uma das seguintes:

Hubble's Law.
Supernovae Type I.
Cepheid Variables.
Spectroscopic Parallax.
Stellar Parallax.

Explicação

Questão 118 de 120

1

The difference between a double-lobed radio galaxy and a core-halo radio galaxy is:

Selecione uma das seguintes:

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.

Explicação

Questão 119 de 120

1

The Great Wall is:

Selecione uma das seguintes:

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.

Explicação

Questão 120 de 120

1

What kind of galaxies are NOT found in the Local Group, but ARE seen in the Virgo Cluster?

Selecione uma das seguintes:

dwarf ellipticals.
giant ellipticals.
spiral galaxies.
irregular galaxies.
all of the above are seen in both the Local Group and the Virgo Cluster.

	Criado por Taylor Campbell mais de 11 anos atrás

Quiz sobre ASTR Review for Final #1 (All 5 Quizzes), criado por Taylor Campbell em 24-04-2015.

ASTR Review for Final #1 (All 5 Quizzes)

Questão 1 de 120

Which kind of light travels fastest in a vacuum?

Selecione uma das seguintes:

Explicação

Questão 2 de 120

What kind of light has wavelengths between those of ultraviolet light and those of gamma waves?

Selecione uma das seguintes:

Explicação

Questão 3 de 120

How long does it take light from the Sun to reach us?

Selecione uma das seguintes:

Explicação

Questão 4 de 120

The mass of a positron is the same as that of:

Selecione uma das seguintes:

Explicação

Questão 5 de 120

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?

Selecione uma das seguintes:

Explicação

Questão 6 de 120

Which of the following processes in an atom is called 'excitation'?

Selecione uma das seguintes:

Explicação

Questão 7 de 120

32 degrees Fahrenheit is equal to:

Selecione uma das seguintes:

Explicação

Questão 8 de 120

In equation form, the inverse square law of light states:

Selecione uma das seguintes:

Explicação

Questão 9 de 120

Which portion of the Sun covers the largest total volume, in kilometers^3?

Selecione uma das seguintes:

Explicação

Questão 10 de 120

As the frequency of light increases:

Selecione uma das seguintes:

Explicação

Questão 11 de 120

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:

Selecione uma das seguintes:

Explicação

Questão 12 de 120

The peak of the spectrum of the photosphere of Betelgeuse lies in the:

Selecione uma das seguintes:

Explicação

Questão 13 de 120

What is a watt?

Selecione uma das seguintes:

Explicação

Questão 14 de 120

How are the distances to the nearest stars determined?

Selecione uma das seguintes:

Explicação

Questão 15 de 120

A hot solid (like a burner on a stove) produces:

Selecione uma das seguintes:

Explicação

Questão 16 de 120

Deuterium is:

Selecione uma das seguintes:

Explicação

Questão 17 de 120

A parsec is:

Selecione uma das seguintes:

Explicação

Questão 18 de 120

The strong force is:

Selecione uma das seguintes:

Explicação

Questão 19 de 120

Kinetic energy is:

Selecione uma das seguintes:

Explicação

Questão 20 de 120

Why does it take so long for the energy produced in the core of the Sun to make its way out of the Sun?