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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. Venus (retrograde)
Summer Solstice
slowest rotation
Roundest orbit
Lagrangian Razor
2. The distance between a lens and its focal plane
Spectral Lines
Hubble law
Focal Length
molecular clouds
3. The distance a moon can be from a planet before shattering from tidal forces
Inverse Square Law
roche limit
most eccentric orbit
CNO Cycle
4. Venus (retrograde)
Light Curve
synchronous rotation
Total Eclipse
slowest rotation
5. Mercury - Venus - Earth - Mars
MOONS: roundest shape
Planck time
Terrestrial Planets
CNO Cycle
6. The lens in a telescope used to determine the magnification
Eyepiece Lens
2 Reasons Why there are Supermassive Black holes at the center of every Galaxy
Terrestrial Planets
Stephen-Boltzman Law
7. A streak of light in the atmosphere
accretion disk
meteor
self-propagating star formation
quasar
8. VENUS
Light-Year
Clouds of sufuric acid (very inhospitable and brightest object in the sky) - process called greenhouse affect traps radiation making it 900 degrees at times - spins with retrograde rotation (sun rises in west) and takes 58.4 days for it to set. Thick
meteoriod
accretion
9. A point in the sky where meteors appear to come from during a shower
Red Giant Branch Star
Dark matter is located at center of clusters - pulling the cluster members into faster orbits--dark matter gravity keeps objects in galxies bound.
radiant
Oort Cloud
10. The telescope configuration that has the focus placed at the back of the primary mirror
Sidereal Day
quarks
Cassegrain Focus
Dwarf planets
11. An important quality of telescopes that increases as the square of the primary mirror or objective lens
Light Gathering Power
Extrasolar Planet
tectonics of Mars
Terrestrial Planets
12. Milky way galaxy is a member - a small poor cluster-about 30 galaxies
Black Hole
2 Reasons Why there are Supermassive Black holes at the center of every Galaxy
Blackbody
The Local Group
13. The amount an image is enlarged by a telescope
Rich Cluster
Magnification
Emission Spectrum
meteoriod
14. A collection of galaxies like the one the Milky Way belongs to
Hydrostatic Equilibrium
Poor Cluster
Doppler Shift
synchronous rotation
15. Long - meandering cliff formed when a planet surface cools and shrinks
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.
superclusters
scarp
Synodic Day
16. Radiation given off by electrons accelerating in a magnetic field
Objective Lens
solar nebula
Jupiters red spot
Synchrotron Rotation
17. A particle of light.
Quasar
Steady State Theory (Leads to Olber's Paradox)
Photon
MOONS: larger than mercury
18. When the Moon entirely blocks the Sun.
chondrite
greehouse effects
Total Eclipse
2 Reasons Why there are Supermassive Black holes at the center of every Galaxy
19. The point in its orbit where a planet is nearest the sun
radio galaxy
synchrotron radiation
Chromosphere
Perihelion
20. The rotation period of the Earth measured relative to the Sun.
Synodic Day
Spectroscopic Parallax
Hubble constant
Cepheid Variable
21. A phenomenon seen when the Earth passes through the orbit of a burned out comet
Interstellar Extinction
widmanstatten pattern
Heliocentric
meteor shower
22. A collection of comets in the plane of the solar system - located beyond the orbit of Pluto
Flat - Remain Parallel - Exactly 1
dark matter
Kuiper belt
Sunspot cycle
23. The shadow behind the Earth or Moon where the Sun is partially obscured.
Penumbra
H2 Regions
radio galaxy
CMB
24. The dark - relativley smooth areas on the moon; Latin for sea
Steady State Theory (Leads to Olber's Paradox)
Maria
Hydrostatic Equilibrium
Cassini division
25. A large and bright but cool star.
Red Giant
Focal Plane
H-are Diagram
accretion disk
26. A star that blows itself apart
Particle Horizon
Instability strip
Supernova (You can be my supernova girl)
cosmological principle
27. When massive objects bend space and time enough to create multiple images of an object located behind them
Olber's paradox
Ecliptic
Gravitational Lens
Flocculent spirals
28. A measure of how an object resists accelerating when acted upon by a force. It is proportional the amount of matter in an object
Ganymede (Jupiter)
fastest rotation
mass
cosmological red shift
29. The number of protons in an atom.
Atomic Number
Magnification
Spectroscopic parallax
solar nebula
30. Old - pock marked - icy surface - interior is not differentiated - geologically dead - NOT ACTIVE SURFACE
Callisto (Jupiter)
MOONS: thickest atmosphere
synchronous rotation
Hipparchus
31. The nuclei of very distant galaxies. Likely a manifestation of supermassive black holes
Color Index
Quasar
White Dwarf
partile horizon
32. An entity that is likely in the nucleus of most - if not all - galaxies.
supermassive black hole
Spectral Lines
fewest moons
direct motion
33. The fusion process that turns three helium nuclei into a carbon nucleus
Dark Nebula
MOONS: larger than mercury
Triple Alpha rocess
OB Associations
34. The name for the only seriously considered theory of the universe.
terrestrial planet
Apparent Magnitude
Titus-Bode Law
Big Bang
35. When material is heated and moves taking the heat energy with it
Thickest atmosphere
Convection
Rich Cluster
Hipparchus
36. Plate tectonics due to thickness of crust and maintain their general form when they collide-where most volcanoes are.
tectonics of Earth
High Velocity Stars
Sunspots
Thermal Equilibrium
37. A spinning neutron star
Ammonia - methane - and water
density
Radiative Diffusion
Pulsar
38. Places in the asteroid belt - caused by resonance with Jupiter - where there are no asteroids
Kirkwood gaps
Summer Solstice
Emission Spectrum
Most dense
39. A bridge of material held in position above the solar surface. They can remain for hours even days
Planck time
nucleus
Kuiper belt
Prominence
40. Why does the earth have few craters while the moon has many?
Earth resurfaces itself due to erosion and plate tectonics - while the moon has neither.
smallest diameter
Open - flat - and closed.
Molecular Clouds
41. Venus
Thermal Equilibrium
Thickest atmosphere
Heliocentric
Open Cluster
42. The amount of density needed to stop the universe from expanding and to begin the big crunch represented by Pc
critical density
Sidereal Day
Spectroscopic parallax
Big Bang
43. The relation that tells how light dims with distance.
Zenith
H2 Regions
We don't know. It might be but does not have to be.
Inverse Square Law
44. What do we think the actual fate of the universe will be and why do we think this?
Make up of the terrestrial planets
Electromagnetic Radiation
Observations of distant type Ia supernovae indicate that the expansion of the universe is speeding up with time - not slowing down! So there must be a force causing this.
Instability strip
45. 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
cosmic singularity
Globular Cluster
Autumnal Equinox
Spectroscopic parallax
46. 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.
Focal Length
radiation dominated universe
2 Reasons Why there are Supermassive Black holes at the center of every Galaxy
Degeneracy
47. 1-orbit aroudn the sun 2- are in hydrostatic equilibrium and 'mostly round' 3- have not cleared debris around its orbit 4- are not satellites
Electron
Dwarf planets
coma
Inverse Square Law
48. A nearby galaxy with a quasar-like nucleus. closer but less bright than quasars-weaker
widmanstatten pattern
Seyfert galaxy
Continuous Spectrum
Radio Galaxy
49. The location in the Milky Way where stars orbit like a solid wheel
Bulge
Interstellar Extinction
Eclipses of the Moons of Jupiter
tectonics of Venus
50. After stars form they pump light energy into surrounding gas causing it to heat up and glow (H2=ionized hydrogen - H1= neutral hydrogen in molcular couds)
nova
Callisto (Jupiter)
meteor
H2 Regions