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Test your basic knowledge |
Cosmology
Start Test
Study First
Subject
:
science
Instructions:
Answer 50 questions in 15 minutes.
If you are not ready to take this test, you can
study here
.
Match each statement with the correct term.
Don't refresh. All questions and answers are randomly picked and ordered every time you load a test.
This is a study tool. The 3 wrong answers for each question are randomly chosen from answers to other questions. So, you might find at times the answers obvious, but you will see it re-enforces your understanding as you take the test each time.
1. A collection of comets in the plane of the solar system - located beyond the orbit of Pluto
Kuiper belt
Flat - Flat
Gravitational Lens
superclusters
2. The instant of time after the Big Bang when space and time obtained their characteristics. (t=10^-43 sec when gravity freezes out-instant when gravity started existing as a separate force)
tectonics of Venus
Planck time
great dark spots
How is winding dilemma solved?
3. Where is the center of the expansion
Sb spiral galaxy
Eclipses of the Moons of Jupiter
Nowhere visible to us. If there are higher dimension then the center would be visible to someone who lives in one. If there are no higher dimensions then the center does not exist.
Objective Lens
4. Ganymede and Titan
radio galaxy
MOONS: larger than mercury
Horizontal Branch Star
Spectral Lines
5. The shadow area behind the Earth or Moon where the Sun is completely obscured.
great dark spots
HII Region
Meridian
Umbra
6. The process that powers the sun and hydrogen bombs
Electromagnetic Radiation: Ultraviolet Light
Thermonuclear Fusion
Open Cluster
Negative - Diverge - Less than 1
7. 100 nm 10 nm
slowest rotation
Yes - frozen at the poles- remains protected from the suns rays
Electromagnetic Radiation: Ultraviolet Light
rotation curve = dark matter?
8. The mass of an object divided by its volume
Kuiper belt
Lagrangian Razor
density
Plank's Law
9. A collection of galaxies like the one the Milky Way belongs to
inferior planets
rotation curve=winding dilemma?
Poor Cluster
Neutron Star
10. Sa - Sb galaxies where two magnificent arms wind their way from nucleus out in a symmetrical manner.
evidence of water on mars
Grand design spirals
Spectroscopy
semimajor axis
11. A very distant - star-like object with huge - broad emission lines. Probably the nucleus of a distant active galaxy.
protostar
quasar
Inverse Square Law
Synodic Day
12. A word used in astronomy to describe all elements besides hydrogen and helium
Metals
Kuiper belt
Total Eclipse
interstellar dust
13. A huge sphere of tenuous gas surrounding the nucleus of a comet
great dark spots
Pixel
coma
Winter Solstice
14. A phenomenon seen when the Earth passes through the orbit of a burned out comet
Light Curve
Void
High and low pressure which stretch into bands due to the rapid differential rotation. deeper - darker colors are in the belts and zones are lighter
meteor shower
15. Atmosphere blocks high energy wavelengths - atmosphere blurs optical radiation - atmosphere absorbs some radiation at all wavelengths even when it gets through.
Earth resurfaces itself due to erosion and plate tectonics - while the moon has neither.
Population 1 vs Population 2 stars
3 reasons we orbit satellites to observe universe
Chandrasekhar Limit
16. A crystalline patter found in iron meteorites
widmanstatten pattern
Dark matter candidates
Ole Roemer
Quasar
17. Small moons that maintain the shape of rings around Saturn and Uranus
Shepherd satellite
mare basalt
accretion disk
White Dwarf
18. A galaxy emitting large amounts of energy at long wavelengths.
Cassegrain Focus
SETI
MOONS: larger than mercury
radio galaxy
19. Finding a star's absolute magnitude from it's placement on an HR diagram. After finding the absolute magnitude - we measure the apparent magnitude - for a distance modulus and use this to find the distance. This method is good for finding distances t
retrograde motion
zone
meteor shower
Spectroscopic parallax
20. A volume of space where few - if any - galaxies are located
nova
Asymptotic giant Branch Star
Void
Ground State
21. The force of attraction between any two objects having mass
The Local Group
Oort cloud
Sa spiral galaxy
gravity
22. The light produced when particles from the sun collide with atmospheric molecules
The Big Bang Theory resolves Olber's Paradox
Trojan asteroids
Pixel
aurora
23. All wavelengths of light emitted by a blackbody.
Blackbody Curve
Emission Spectrum
most eccentric orbit
Negative - Diverge - Less than 1
24. The measure of a variable star's apparent magnitude as it brightens and dims with time
Main Sequence
interstellar dust
Light Curve
Radiative Diffusion
25. Radiation (possibly left over from the big bang) that fills the universe. Perfect black body spectrum and tells us a bit aout how galaxies are formed.
Thickest atmosphere
Hubble constant
Occam's razor
Cosmic Microwave Background (CMB)
26. The Big Bang says that the universe has not existed forever. It had a distinct beginning about 14 billion years ago called the 'Big Bang'. Therefore light from any object more than 14 billion light years away has not had time to reach us. The other p
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27. Earth
terrestrial planet
Most dense
Jupiters red spot
widmanstatten pattern
28. Arcs of increased mass concentration that slow stars and gas down as they orbit through which cause the formation of stars.
density waves
semimajor axis
Celestial Equator
Black Hole
29. The lens in a telescope used to determine the magnification
Cosmic Microwave Background
Emission Spectrum
Eyepiece Lens
Black Hole
30. Highlands: rocks are made of lighter anorthosite (similar to old earth rocks) Maria: rocks made of heavy mare basalt (volcanic rock) everywhere else is loose regolith created by meteoric impact.
The Big Bang Theory
radio galaxy
difference between maria and highlands of the moon.
comet
31. The apparent path of the Sun through the stars on the celestial sphere.
Blackbody
Neutron Star
CMB
Ecliptic
32. Sc galaxies
Flocculent spirals
Seeing
meteor shower
Seyfert galaxy
33. 1. We see rapid movements or high energy radiation coming at some level from the nuclei of nearly every galaxy we have looked at. 2. We suspect that the creation of these supermassive black holes is part of the galaxy formation process.
Light Gathering Power
2 Reasons Why there are Supermassive Black holes at the center of every Galaxy
CCD
nova
34. The oldest part of the Milky Way
Halo
SETI
Active Optics
smallest diameter
35. A term referring to Jupiter-like planets
evidence of water on mars
Planetary Nebula
Parsec
jovian
36. When the Moon entirely blocks the Sun.
High Velocity Stars
Total Eclipse
Thermal Equilibrium
neutrino
37. A star fusing hydrogen to helium in it's core
Black Hole
Differential Rotation
cosmological red shift
Main Sequence Stars
38. Material that shoots rapidly out into space. Flares cause Auroras
Nowhere visible to us. If there are higher dimension then the center would be visible to someone who lives in one. If there are no higher dimensions then the center does not exist.
MOONS: larger than mercury
Flare
Objective Lens
39. First accurately measured the speed of light in a vacuum
Jovian Planets
tectonics of Earth
fewest moons
Ole Roemer
40. Places in the asteroid belt - caused by resonance with Jupiter - where there are no asteroids
Make up of the terrestrial planets
Thermonuclear Fusion
Kirkwood gaps
nova
41. When material is heated and moves taking the heat energy with it
supernova
Convection
Void
The Big Bang Theory
42. Matter so dense that even light cannot escape its gravity
MOONS: largest size
Black Hole
blazar
Light Curve
43. The powdered stone fragments that make up the lunar 'soil'
Spectral Lines
interstellar dust
Dark Matter
regolith
44. Electromagnetic Radiation
quarks
Nucleus
A family of radiant energy- includes light
Neutron Star
45. The projection of the Earth's equator onto the celestial sphere.
SETI
Autumnal Equinox
Celestial Equator
Open - flat - and closed.
46. The Greek philosopher responsible for making the stellar magnitude scale.
Rich vs poor clusters
Hipparchus
Continuous Spectrum
Cosmic Microwave Background (CMB)
47. Radiation emitted when charged particles spiral rapidly in a magnetic field. come off of jets from black holes.
molecular clouds
synchrotron radiation
Steady State Theory (Leads to Olber's Paradox)
contrast northern lowlands and the southern highlands of mars...
48. A logarithmically scaled value for the measured brightness of a star.
Apparent Magnitude
radio lobe
coma
Umbra
49. The average distance between the Earth and the Sun (=1.5 x10^8km)
Astronomical Unit
Refractor
Chandrasekhar Limit
Spectroscopic parallax
50. How is the Hubble Law consistent with an expanding universe?
Pulsar
acceleration
Bulge
In an expanding universe all galaxies see all other galaxies that are not gravitationally bound to them receding away. This is what we see in the Hubble Law. We infer that the Hubble law also holds true for all other galaxies.